# Patent

## Title
Method for detection and automatic identification of damage to rolling bearings

## Abstract

The subject of the invention is a method for detection and automatic identification of defects in rolling bearings applicable in diagnosing rolling bearings and detecting damage in a very early stage of its occurrence.
The inventive method in which the vibrations of a bearing in operation are measured, the measured analogue signals are converted to digital data which are filtered and next shock pulses are detected, whereupon defects present in the tested bearing or bearings are identified, characterized in that the detection of shock pulses is done using shock pulse likelihood ratio (Ms).

## Background
The subject of the invention is a method for detection and automatic identification of damage to rolling bearings applicable in diagnosing rolling bearings and detecting damage in a very early stage of their occurrence.
BACKGROUND
In present-day methods of diagnosing technical equipment, the detection of existing faults and damage occurring in the early phase of the use of equipment or its individual parts and their accurate location are of paramount importance, and the sooner it can be done the greater the importance of the method. The diagnosing of the condition of equipment and especially the detection and automatic identification of defects in rotating electric machines and their parts makes use of methods based on measuring electric or mechanical signals, their processing as well as the analysis and interpretation of the results of the measurements.
The nowadays applied methods of monitoring bearings during operation consist in comparing the measured and digitally processed results with data obtained for bearings which operate in proper conditions and which are not in danger of any failure. In most cases such comparison is done by an expert trained for this purpose.
The most frequently used method for early determination of defects in bearings consists in the examination of shock pulses combined with the examination of vibrations in the tested parts of the bearing. Then, such shapes of the pulses are selected from the measured data for further analysis which suggest the possibility of the presence of a defect. Computerised methods of data analysis allow to detect faults early and to determine the place of their occurrence, their types and the degree of damage.
A method and a device for checking the condition of a rolling bearing is known from the patent description U.S. Pat. No. 5,477,730. The method consists in detecting the primary signals of vibrations emitted by the bearing, demodulation of these signals to output signals after demodulation, converting the output signals from analogue signals to digital output signals, filtering noise out of these signals by means of a digital filtration technology selected from many known technologies, and outputting the digital signals to an output device. In another variant of the invention, instead of the demodulation of primary signals, band-pass filtration within a range from 2000 to 15,000 Hertz is used, and the signals after this filtration are subjected to transformations as described earlier. In still another variant of the invention the primary vibration signals emitted by the bearing are converted from analogue to digital, whereupon noise is filtered off the signals using a digital filtration technology selected from many known technologies, which includes the action of separation of noise signals from the digital output signals, and then digital signals are introduced to the output device.
A method for evaluating the condition of the elements of a bearing is known from patent application WO 00/04361. This method employs the measurements of bearing element vibrations by generating an analogue acceleration signal, converting this signal into digital data, sampling the digital signal to locate its components coming from the bearing defect. The method is characterized in that the influence of any unwanted, deterministic signal components is removed from the digital acceleration signal by means of filtering so as to obtain a signal consisting essentially of white noise proportional to overall smoothness of the microstructure of the bearing surface and shock pulse. The following signal characteristic parameters that are sensitive to the bearing defects are selected: sharp vibration pulses or shock pulses, peak-to-peak amplitude a mean value proportional to the mean amplitude without shock pulses a peak content of the signal. Detection of narrow-band shock pulses in regular intervals is done using a known method, so called autocorrelation of the envelope signal estimation.
SUMMARY OF THE INVENTION
The essence of the method for detection and automatic identification of damage to rolling bearings, in which vibrations of a bearing in operation, measured as an analogue timewave signal is converted into digital data and prefiltered in a known way, is that the detection of the shock pulses is performed with use of the binary vector p that is determined in the following actions:
in the prefiltered timewave of the processed signal two first, adjacent vector intervals are selected: a reference interval and a test interval and the signal present in the test and reference intervals are subjected to multiple filtering whereupon after each filtering, the shock pulse likelihood ratios are calculated defined as a ratio of mean square values of filtered signal present in the test interval to the mean square values of filtered signal present in the reference interval,
calculated likelihood ratios are compared with the preset threshold value and the probability of shock pulse occurrence in the first test interval is estimated,
information about shock pulse occurrence in examined test interval is recorded as initial elements of binary vector p, and next
all remaining elements of the binary vector p are determined for all successive test and reference intervals that are selected iteratively with an offset in a specific direction and those elements of binary vector p take on the values 1 in the area of shock pulse occurrence and 0 in the area where the shock pulse does not occur.
Preferably mean square value of the signal in the examined test interval subjected to Lth filtering τt[L] is determined on the basis of the following relation:




  
    
      
        τ
        t
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          K
          t
        
      
      ⁢
      
        
          ∑
          
            
              k
              t
            
            =
            1
          
          
            K
            t
          
        
        ⁢
        
          
        
        ⁢
        
          
            
              z
              t
              L
            
            ⁡
            
              [
              
                k
                t
              
              ]
            
          
          2
        
      
    
  
  ,




whereas the mean square value of the signal in the examined reference interval subjected to Lth filtering τr[L] is determined on the basis of this relation:





  
    
      
        τ
        r
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          K
          r
        
      
      ⁢
      
        
          ∑
          
            
              k
              r
            
            =
            1
          
          
            K
            r
          
        
        ⁢
        
          
        
        ⁢
        
          
            
              z
              r
              L
            
            ⁡
            
              [
              
                k
                r
              
              ]
            
          
          2
        
      
    
  
  ,




where:

    
    
        L—is a natural number from the range 1 . . . NS and denotes the number of filters,
        kt, kr denotes successive natural numbers 1 to Kt or to Kr,
        ztL, denotes a vector representing the examined test interval of the signal subjected to Lth filtering,
        zrL denotes a vector representing the examined reference interval of the signal subjected to Lth filtering.

Preferably the mean square value of a signal in the examined reference interval τr[L] is determined using Lth filtering, that is an adaptive filtering, with use of Singular Value Decomposition (SVD) of autocovariance matrix Cr according to the following relation:

Cr=VΣrUT,

where matrix Σr is a diagonal matrix whose diagonal elements are nonzero and nonnegative and denote mean square values τr[L]:

    
    






  
    
      Σ
      r
    
    =
    
      [
      
        
          
            
              
                τ
                r
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            0
          
          
            ⋯
          
          
            0
          
        
        
          
            0
          
          
            
              
                τ
                r
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ⋯
          
          
            0
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            0
          
          
            0
          
          
            ⋯
          
          
            
              
                τ
                r
              
              ⁡
              
                [
                L
                ]
              
            
          
        
      
      ]
    
  
  ,




and matrices V and U are orthogonal matrices and at the same time the autocovariance matrix Cr has the following form:





  
    
      C
      r
    
    =
    
      [
      
        
          
            
              r
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                2
                ]
              
            
          
          
            ⋯
          
          
            
              r
              ⁡
              
                [
                L
                ]
              
            
          
        
        
          
            
              r
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                0
                ]
              
            
          
          
            ⋯
          
          
            
              r
              ⁡
              
                [
                
                  L
                  -
                  1
                
                ]
              
            
          
        
        
          
            ⋯
          
          
            ⋯
          
          
            ⋯
          
          
            ⋯
          
        
        
          
            
              r
              ⁡
              
                [
                L
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                
                  L
                  -
                  1
                
                ]
              
            
          
          
            ⋯
          
          
            
              r
              ⁡
              
                [
                1
                ]
              
            
          
        
      
      ]
    
  
  ,




for which:





  
    r
    ⁡
    
      [
      
        i
        r
      
      ]
    
  
  =
  
    
      1
      
        K
        r
      
    
    ⁢
    
      
        ∑
        
          
            k
            r
          
          =
          1
        
        
          K
          r
        
      
      ⁢
      
        
          
            x
            r
          
          ⁡
          
            [
            
              k
              r
            
            ]
          
        
        ⁢
        
          
            x
            r
          
          ⁡
          
            [
            
              
                k
                r
              
              +
              
                i
                r
              
            
            ]
          
        
      
    
  




where:

xr[kr] are the elements of the reference interval,

kr denotes successive natural numbers from 1 to Kr,

ir denotes successive natural numbers from 1 to L,

Kr denotes the length of the reference interval,

L denotes the number of adaptive filters.

Preferably the mean square value of a signal in the examined test interval τt[L] is determined using Lth filtering, that is an adaptive filtering, on the basis of the following relation:





  
    
      
        τ
        t
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          N
          t
        
      
      ⁢
      
        
          ∑
          
            
              k
              t
            
            =
            1
          
          
            N
            t
          
        
        ⁢
        
          
            
              z
              t
              L
            
            ⁡
            
              [
              
                k
                t
              
              ]
            
          
          2
        
      
    
  
  ,




where ztL are the elements of the matrix Zt presented in the following form:





  
    
      Z
      t
    
    =
    
      [
      
        
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                
                  N
                  t
                
                ]
              
            
          
        
        
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                3
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                
                  
                    N
                    t
                  
                  +
                  1
                
                ]
              
            
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  L
                  t
                
                ]
              
            
          
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  
                    L
                    t
                  
                  +
                  1
                
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  K
                  t
                
                ]
              
            
          
        
      
      ]
    
  
  ,




and calculated according to the following relation:

Zt=XtU, 

where matrix Xt is defined as:





  
    
      X
      t
    
    =
    
      [
      
        
          
            
              
                x
                t
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  N
                  t
                
                ]
              
            
          
        
        
          
            
              
                x
                t
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                3
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  
                    N
                    t
                  
                  +
                  1
                
                ]
              
            
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  L
                  t
                
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  
                    L
                    t
                  
                  +
                  1
                
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  K
                  t
                
                ]
              
            
          
        
      
      ]
    
  
  ,




and matrix U is an orthogonal matrix whose elements are the adaptive filter coefficients, while:

    
    
        Kt denotes the length of the examined test interval;
        xt[kt], are the elements of the test interval;
        kt denotes the successive natural numbers from 1 to Kt,
        Nt=Kt−L,
        L denotes the number of adaptive filters.
    
    


Preferably the multiple filtering of signals in the test and reference intervals is performed with use of band pass filter
Preferably the length of the test interval is 15% of the length of the reference interval
Preferably the identification of the defect in the bearing or bearings is done automatically for the binary vector p determined for all examined test and reference intervals of the timewave X of the processed signal and the set of known defect frequencies of examined bearing or bearings Ff=[ff1, ff1, . . . , ffK], by means of the following actions:
for each successive, known defect frequency ffK from the set Ft of the examined bearing, the test frequency νfKε└(1−Pg)ffK,(1+Pg)ffK┘ that belongs to the neighbourhood Pg of the frequency ffK is determined, where Pg is a configuration parameter denoting the searching frequency range related to known defect frequency and next, using known maximum likelihood mathematical principles, for each test frequency νfK the maximum likelihood function J in time domain is determined using the binary vector p,
next, it is checked for which test frequency νfK the maximum likelihood function J reaches the maximum value JA,
the ratio FA of the maximum value JA to the noise level nA is calculated and the result is compared with the preset threshold parameter SA:
if the ratio FA is greater than the preset threshold parameter SA, information about examined bearing defect with specific frequency that belongs to set Ft and corresponds to test frequency νfK generated automatically,
if the ratio FA is less than or equal to the preset threshold parameter SA, it is assumed that none of the shock pulses present in the binary vector p corresponds to any of known defect frequencies ffK of examined bearings and information that no specific defect occurred in the examined bearing or bearings is generated automatically.
Preferably the test frequency νfK, for which the maximum likelihood function calculated for the binary vector p in time domain reaches the maximum value JA, is determined by maximising the sum of squares of harmonic amplitudes Ak according to the following relation:




  
    
      J
      A
    
    =
    
      
        ∑
        
          k
          =
          1
        
        
          N
          h
        
      
      ⁢
      
        
          [
          
            A
            k
          
          ]
        
        2
      
    
  
  ,




where: Nh is a preset number of the examined harmonics.

Preferably values of the amplitudes of harmonics Ak are determined in time domain using the binary vector p, presented in the form of the sinusoidal model.

The binary vector p is presented as a sum of sinusoidal model and the noise vector:





  
    
      p
      ⁡
      
        [
        n
        ]
      
    
    =
    
      
        
          ∑
          
            k
            =
            1
          
          
            N
            h
          
        
        ⁢
        
          [
          
            
              
                A
                k
              
              ⁢
              
                cos
                ⁡
                
                  (
                  
                    n
                    ⁢
                    
                      
                    
                    ⁢
                    
                      ω
                      k
                    
                  
                  )
                
              
              ⁢
              
                cos
                ⁡
                
                  (
                  
                    φ
                    k
                  
                  )
                
              
            
            -
            
              
                A
                k
              
              ⁢
              
                sin
                ⁡
                
                  (
                  
                    n
                    ⁢
                    
                      
                    
                    ⁢
                    
                      ω
                      k
                    
                  
                  )
                
              
              ⁢
              
                sin
                ⁡
                
                  (
                  
                    φ
                    k
                  
                  )
                
              
            
          
          ]
        
      
      +
      
        ɛ
        ⁡
        
          [
          n
          ]
        
      
    
  
  ,




which can be also presented in the following matrix form:

p=Bθ+e 

where:

    
    
        φk is a phase,
        ωk=2πνk/fs, k=1, 2 . . . Nh is an angular velocity corresponding to a test frequency (νfK), and k=1, 2 . . . Nh,
        fs is a sampling frequency for analogue to digital processing of measured analogue signal,
        e=[ε[n]]T—denotes the noise vector,
        n—denotes a natural number from 1 to N−1,
        N—denotes number of elements in the binary vector (p),
        B is the matrix of known constant parameters, presented in the following form:
    
    






  B
  =
  
    

  
  ⁢
  
    [
    
      
    
    ⁢
    
      
        
          1
        
        
          0
        
        
          1
        
        
          0
        
        
          ...
        
        
          1
        
        
          0
        
      
      
        
          
            cos
            ⁡
            
              (
              
                ω
                1
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  1
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                ω
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  2
                
                )
              
            
          
        
        
          ...
        
        
          
            cos
            ⁡
            
              (
              
                ω
                
                  N
                  h
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  
                    N
                    h
                  
                
                )
              
            
          
        
      
      
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  1
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    1
                  
                  ⁢
                  2
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  2
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    2
                  
                  ⁢
                  2
                
                )
              
            
          
        
        
          ...
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  
                    N
                    h
                  
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    
                      N
                      h
                    
                  
                  ⁢
                  2
                
                )
              
            
          
        
      
      
        
          ⋮
        
        
          ⋮
        
        
          ⋮
        
        
          ⋮
        
        
          
            
          
        
        
          ⋮
        
        
          ⋮
        
      
      
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  1
                
                ⁡
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    1
                  
                  ⁡
                  
                    (
                    
                      N
                      -
                      1
                    
                    )
                  
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  2
                
                ⁡
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    2
                  
                  ⁢
                  
                    (
                    
                      N
                      -
                      1
                    
                    )
                  
                
                )
              
            
          
        
        
          ...
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  
                    N
                    h
                  
                
                ⁢
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            
              -
              
                sin
                ⁡
                
                  (
                  
                    
                      ω
                      
                        N
                        h
                      
                    
                    ⁢
                    
                      (
                      
                        N
                        -
                        1
                      
                      )
                    
                  
                  )
                
              
            
            ⁢
            
              
            
          
        
      
    
    ]
  




and θ is the vector of unknown parameters presented in the following form:

θ=└A1 cos(φ1), A1 sin(φ1), A2 cos(φ2), A2 sin(φ2), . . . , ANh cos(φNh), ANh sin(φNh)┘,

which is the Least Square Estimator for the relation:

θ=(BTB)−1BTp 

where p is a binary vector in the following form:

p=[p[0], p[1], . . . , p[N−1]]T.

Preferably the noise level nA is calculated by taking a median value of maximum function values J found in the neighbourhood of the examined defect frequency ffK from the set Ff.
Alternatively the noise level nA is calculated by taking a mean value of maximum function values J found in the neighbourhood of the examined defect frequency ffK from the set Ff.
Compared with the known methods of the detection and automatic identification of defects in rolling bearings, the inventive solution allows the detection of defects in a very early phase of their emergence. Measured signal is processed so that non-shock pulse related signal components are removed from it on the basis of adaptive filtering combined with shock pulse likelihood ratio calculation in a specific test and reference intervals. Moreover, detection of each potential shock pulse is performed in the time domain, individually, one at the time in contrary to other techniques where the shock pulse detection is based on the analysis of demodulated signal in the frequency domain. In consequence the sensitivity of inventive solution is increased. As a result of shock pulse detection algorithm, the binary vector p is created that contains only shock pulse related signal components. For the bearing fault identification, the binary vector p is processed in the time domain with high resolution maximum likelihood method. There is no Fourier transform used in the fault identification process at all.



BRIEF DESCRIPTION OF THE DRAWING FIGURES
FIG. 1 shows a block diagram of the device used for detecting and automatically identifying defects in rolling bearings,
FIG. 2 shows a timewave of a processed signal X with indicated test and reference intervals,
FIG. 3 shows the graph of the course of occurrence of shock pulses in the binary form against the background of a time pass of the processed signal X,
FIG. 4 shows a fragment of the frequency spectrum in which the defect frequency ffault has been indicated,
FIG. 5 shows a diagram of operations performed when detecting shock pulses according to the presented method and
FIG. 6 shows a diagram of operations performed when identifying defects in bearings according to the presented method.



DETAILED DESCRIPTION OF THE INVENTION
Placed on a rotating shaft 1, a rolling bearing 2 comprises measuring points, marked on its housing, where a vibration sensor 3 is placed for measuring the bearing vibrations and the shaft 1 speed sensor 4. The sensors are connected to a measuring device 5 used to measure the analogue signal of voltage proportional to the vibrations of the operating bearing 2 and to measure the rotational speed of the shaft. The output of the measuring device 5 is connected to the input of a processor 6 in whose memory 7, a processing module 8 and a function module 9 can be distinguished. The processing module 8 incorporates a processing system 10 in which the measured signal is converted to a digital signal which is then sent as input data to a high pass filtering system 11 also incorporated in the module 8, wherein the signal components unwanted in further analysis are filtered off. Output data received from the system 11 are fed to a shock pulse detector 12 which makes one of the systems of the function module 9 of the processor 6. Configuration data 13 related mathematical calculations performed in the function module 9 and input data 14 which are the known frequencies of the defects of the tested rolling bearings 2 are also fed to the function module 9. Output data from the system of the shock pulse detector 12 are transmitted to a fault identifier 15 which belongs to the function module 9 and in which the identification of the defects of rolling bearings is performed. The output of the processor 6 is connected with a device for visualising and/or recording the obtained results 16, which can be a computer display, a printer or any carrier for data recording.
The inventive method is implemented according to the following actions shown in FIG. 6.
Vibration and rotation speed measurement. By means of the vibration sensor 3 and the measuring device 5 the vibrations of the operating rolling bearing 2 are measured in the indicated measuring points 3, and by means of the speed sensor 4 and the measuring device 5 the rotational speed of the bearing-supported shaft 1 is measured 1—(activity 101).
Analogue to digital conversion. The results of the measurements are converted from the analogue form to digital data in the processing unit 10, or in the measuring device 5, and then these results are stored in the digital form in the memory 7 of the processor 6 of the computer device as the signal timewave—(activity 102).
Digital data filtering. The stored data are prefiltered in the high pass filtering system 11 producing a timewave X, where X=x[k, k+1, k+2, k+K], where k denotes successive time samples of a processed signal from the range of 1 to K. As the high pass filtering system, a FIR (Finite Impulse Response) filter can be used, for example. The characteristic feature of the FIR filter is that its response to a given sequence of input samples has a finite length. The purpose of data filtration is to remove signals of a frequency lower than a preset limit constituting one of the configuration parameters—(activity 103).
Adaptive filtering and the determination of shock pulse likelihood ratios MS. Data obtained as a result of prefiltering are transmitted to the shock pulse detector 12 in which the signal timewave undergo adaptive filtering and the shock pulse likelihood ratios MS are determined. In the shock pulse detector 12, in the prefiltered timewave X, adjacent reference interval of a length of Kr and a test interval of a length of Kt are selected, the length Kr of the reference interval being less than the time distance between two successive shock pulses generated by the same type of bearing defect, and the length of the test interval Kt being less than or equal to at least half of the length of the reference interval. Preferably it is assumed that the length of the test interval makes 15% of the length of the reference interval. Next, a definite number of filters NS is assumed, preferably NS=5 and for each Lth filtering, where L is a natural number from the range of 1 to NS, the adaptive filtering of a signal from the test and reference intervals is performed, after which for each Lth filtering the shock pulse likelihood ratio MS is calculated according to the following relation—(activity 104):




  
    
      
        
          
            M
            S
          
          =
          
            
              
                τ
                t
              
              ⁡
              
                [
                L
                ]
              
            
            
              
                τ
                r
              
              ⁡
              
                [
                L
                ]
              
            
          
        
        ,
      
    
    
      
        (
        1
        )
      
    
  




    
    
        where τt[L] is the mean square value of the signal in the examined test interval subjected to Lth adaptive filtering, defined in the following form:
    
    






  
    
      
        
          
            
              τ
              t
            
            ⁡
            
              [
              L
              ]
            
          
          =
          
            
              1
              
                K
                t
              
            
            ⁢
            
              
                ∑
                
                  
                    k
                    t
                  
                  =
                  1
                
                
                  K
                  t
                
              
              ⁢
              
                
                  
                    z
                    t
                    L
                  
                  ⁡
                  
                    [
                    
                      k
                      t
                    
                    ]
                  
                
                2
              
            
          
        
        ,
      
    
    
      
        (
        2
        )
      
    
  




    
    
        and τr[L] is mean square value of the signal in the examined reference interval subjected to Lth adaptive filtering, defined in the following form:
    
    






  
    
      
        
          
            
              τ
              r
            
            ⁡
            
              [
              L
              ]
            
          
          =
          
            
              1
              
                K
                r
              
            
            ⁢
            
              
                ∑
                
                  
                    k
                    r
                  
                  =
                  1
                
                
                  K
                  r
                
              
              ⁢
              
                
                  
                    z
                    r
                    L
                  
                  ⁡
                  
                    [
                    
                      k
                      r
                    
                    ]
                  
                
                2
              
            
          
        
        ,
      
    
    
      
        (
        3
        )
      
    
  




    
    
        where:
        L—is a natural number from the interval 1 . . . NS and denotes the number of adaptive filters,
        K—is the total length of the examined timewave of processed signal,
        Kt, Kr are the lengths of the test and reference intervals, respectively,
        kt, kr are the successive natural numbers from 1 to Kt or to Kr,
        ztL, denotes a vector representing the examined test interval of the signal subjected to Lth adaptive filtering,
        zrL denotes a vector representing the examined reference interval of the signal subjected to Lth adaptive filtering.
    
    


Verification of the occurrence of the shock pulse in the test interval. For each Lth adaptive filtering the value of shock pulse likelihood ratio MS is compared with a preset threshold value SL, previously supplied to the computer device memory, and if the likelihood ratio MS is bigger than SL in at least S1 filters, this means that an shock pulse occurred in the examined test interval, whereas if likelihood ratio MS is bigger than SL in less than S1 filters, this means that an shock pulse did not occur in the examined test interval, the occurrence of the shock pulse in the test interval being recorded in a binary form as a vector pn, by filling the initial elements of the vector pn with the numbers “1” or the numbers “0” for non-occurrence of an shock pulse—(action 105).
Determination of remaining elements of the binary vector pn. In the timewave X of the processed signal, successive adjacent test and reference intervals offset in relation to those previously determined by a preset step are iteratively determined and activities connected with adaptive filtering, determination of shock pulse likelihood ratios MS for all successive test intervals, for a preset filtering number NS, and verification of the occurrence of an shock pulse for all intervals of the whole timewave X of the processed signal are repeated and thus the remaining elements of the binary vector pn are obtained. The binary vector pn is stored in the memory 7 of the processor 6 as a binary timewave which takes on the values 1 in the area of shock pulses occurrence and 0 in the area where shock pulses do not occur—(activity 106).
Determination of the vector pr, A reversion of the order of the time samples in the stored, prefiltered timewave X of the processed signal of the test and reference intervals is performed and for such a reversed signal timewave all previous activities from 104 to 106 are performed as before and the information on shock pulses presence is stored as a binary vector pr, where the value 1 denoting the presence of an shock pulse for the given time sample, and the value 0 denoting its absence (activity 107).
Determination of the vector p. The order of the elements in the binary vector pr is reversed and summed up logically with the vector pn in order to obtain the binary vector p. The binary vector p is stored in the memory 7 of the processor 6 (activity 109) as a binary time wave which takes on the values 1 in the area of shock pulse occurrence and 0 in the area where shock pulses do not occur (activity 108).
Saving the vector p in the processor memory. The obtained results are stored in special equipment 18—(activity 109).
Then the elements of the vector p are used as preliminary data for the automatic identification of bearing defects—(activity 110).
In order to determine the mean square value of the signal in the reference interval τr[L], subjected to the Lth adaptive filtering, which is necessary to determine the shock pulse likelihood ratio MS, mathematical relations are used in which the autocovariance matrix Cr is defined as the relation between orthogonal matrices V and UT and of the matrix Σr. The diagonal elements of the matrix Σr are nonzero, nonnegative and they denote mean square values τr[L]. This relation is shown in the following formula:

Cr=VΣrUT  (4),

where the matrix Σr is defined by the following relation:





  
    
      
        
          ∑
          r
        
        ⁢
        
          =
          
            
              [
              
                
                  
                    
                      
                        τ
                        r
                      
                      ⁡
                      
                        [
                        1
                        ]
                      
                    
                  
                  
                    0
                  
                  
                    ...
                  
                  
                    0
                  
                
                
                  
                    0
                  
                  
                    
                      
                        τ
                        r
                      
                      ⁡
                      
                        [
                        2
                        ]
                      
                    
                  
                  
                    ...
                  
                  
                    0
                  
                
                
                  
                    ⋮
                  
                  
                    ⋮
                  
                  
                    ⋱
                  
                  
                    ⋮
                  
                
                
                  
                    0
                  
                  
                    0
                  
                  
                    ...
                  
                  
                    
                      
                        τ
                        r
                      
                      ⁡
                      
                        [
                        L
                        ]
                      
                    
                  
                
              
              ]
            
            .
          
        
      
    
    
      
        (
        5
        )
      
    
  




At the same time the autocovariance matrix Cr is defined as follows:





  
    
      
        
          
            C
            r
          
          =
          
            [
            
              
                
                  
                    r
                    ⁡
                    
                      [
                      1
                      ]
                    
                  
                
                
                  
                    r
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    r
                    ⁡
                    
                      [
                      L
                      ]
                    
                  
                
              
              
                
                  
                    r
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  
                    r
                    ⁡
                    
                      [
                      0
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    r
                    ⁡
                    
                      [
                      
                        L
                        -
                        1
                      
                      ]
                    
                  
                
              
              
                
                  ...
                
                
                  ...
                
                
                  ...
                
                
                  ...
                
              
              
                
                  
                    r
                    ⁡
                    
                      [
                      L
                      ]
                    
                  
                
                
                  
                    r
                    ⁡
                    
                      [
                      
                        L
                        -
                        1
                      
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    r
                    ⁡
                    
                      [
                      1
                      ]
                    
                  
                
              
            
            ]
          
        
        ,
      
    
    
      
        (
        6
        )
      
    
  




for which:





  
    r
    ⁡
    
      [
      
        i
        r
      
      ]
    
  
  =
  
    
      1
      
        K
        r
      
    
    ⁢
    
      
        ∑
        
          
            k
            r
          
          =
          1
        
        
          K
          r
        
      
      ⁢
      
        
          
            x
            r
          
          ⁡
          
            [
            
              k
              r
            
            ]
          
        
        ⁢
        
          
            x
            r
          
          ⁡
          
            [
            
              
                k
                r
              
              +
              
                i
                r
              
            
            ]
          
        
      
    
  




where:

xr[kr] are the elements of the reference interval,

kr denotes successive natural numbers from 1 to Kr,

ir denotes successive natural numbers from 1 to L,

Kr denotes the length of the reference signal.

As a result of the comparison of the relations 4 and 6, using the singular value decomposition of the autocovariance matrix Singular Value Decomposition (SVD), the mean square value of the signal in the reference interval τr[L] is obtained.

Next, in order to determine the mean square value of a signal in the test interval τr[L], subjected to the Lth adaptive filtering, which value is necessary to determine the shock pulse likelihood MS, the following mathematical relations are used:





  
    
      
        
          
            
              τ
              t
            
            ⁡
            
              [
              L
              ]
            
          
          =
          
            
              1
              
                N
                t
              
            
            ⁢
            
              
                ∑
                
                  
                    k
                    t
                  
                  =
                  1
                
                
                  N
                  t
                
              
              ⁢
              
                
                  
                    z
                    t
                    L
                  
                  ⁡
                  
                    [
                    
                      k
                      t
                    
                    ]
                  
                
                2
              
            
          
        
        ,
      
    
    
      
        (
        7
        )
      
    
  




where ztL are the elements of the matrix Zt presented in this form:





  
    
      
        
          
            Z
            t
          
          =
          
            [
            
              
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      1
                      ]
                    
                  
                
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      
                        N
                        t
                      
                      ]
                    
                  
                
              
              
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      3
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      z
                      t
                      1
                    
                    ⁡
                    
                      [
                      
                        
                          N
                          t
                        
                        +
                        1
                      
                      ]
                    
                  
                
              
              
                
                  ⋮
                
                
                  ⋮
                
                
                  ⋱
                
                
                  ⋮
                
              
              
                
                  
                    
                      z
                      t
                      L
                    
                    ⁡
                    
                      [
                      
                        L
                        t
                      
                      ]
                    
                  
                
                
                  
                    
                      z
                      t
                      L
                    
                    ⁡
                    
                      [
                      
                        
                          L
                          t
                        
                        +
                        1
                      
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      z
                      t
                      L
                    
                    ⁡
                    
                      [
                      
                        K
                        t
                      
                      ]
                    
                  
                
              
            
            ]
          
        
        ,
      
    
    
      
        (
        8
        )
      
    
  




and calculated according to this relation:

Zt=XtU  (9),

where the matrix Xt is defined as:





  
    
      
        
          
            X
            t
          
          =
          
            [
            
              
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      1
                      ]
                    
                  
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      
                        N
                        t
                      
                      ]
                    
                  
                
              
              
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      2
                      ]
                    
                  
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      3
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      
                        
                          N
                          t
                        
                        +
                        1
                      
                      ]
                    
                  
                
              
              
                
                  ⋮
                
                
                  ⋮
                
                
                  ⋱
                
                
                  ⋮
                
              
              
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      
                        L
                        t
                      
                      ]
                    
                  
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      
                        
                          L
                          t
                        
                        +
                        1
                      
                      ]
                    
                  
                
                
                  ...
                
                
                  
                    
                      x
                      t
                    
                    ⁡
                    
                      [
                      
                        K
                        t
                      
                      ]
                    
                  
                
              
            
            ]
          
        
        ,
      
    
    
      
        (
        10
        )
      
    
  




and the matrix U is an orthogonal matrix whose elements are the coefficients of adaptive filtering, whereas:

    
    
        Kt denotes the length of the examined test interval;
        xt[kt] are the elements of the test interval;
        kt denotes successive natural numbers from 1 to Kt,
        Nt=Kt−L.

Then, the identification of the defect in a bearing or bearings is done automatically in the defect identifier 15 for a binary vector p determined by means of the inventive method and for the base of input data which are known fault frequencies of examined bearing or bearings Ff=(ff1, ff2, . . . ffK), making use of the following activities depicted in FIG. 6.

    
    


A binary decimation vector pd is determined by subjecting the binary vector p to decimation with a preset decimation coefficient, in order to obtain the binary decimation vector pd— (activity 111).
Maximum likelihood functions J are determined for successive frequencies ffK of the defects in the tested bearing. For each successive defect frequency ffK from the set Ff, of the tested bearing, the test frequency νfKε└(1−Pg)ffK,(1+Pg)ffK┘ is determined roughly and then precisely from the neighbourhood Pg of the frequency ffK, where Pg is a configuration parameter denoting the range of search in relation to the given defect frequency. Next, using known mathematical methods, the maximum likelihood function J is determined for each such test frequency νfK using the binary decimation vector pd—(activity 112).
Searching for the shock pulse with the biggest amplitude. The maximum value JA of the maximum likelihood function J is determined by checking for which test frequency νfK the likelihood function J reaches the maximum value JA (activity 113).
Generation of information about the occurrence or lack of defects in the examined bearing. The ratio FA of the maximum value JA to the noise level nA is calculated and its result is compared with the preset threshold parameter SA. If the ratio is bigger than the preset threshold parameter SA, then information that a specific defect has occurred in the examined bearing, for example ff1, corresponding to the test frequency νfK, is automatically generated.
When the ratio FA is less than or equal to the preset threshold parameter SA, it means that none of the found shock pulses presented in the form of a binary vector corresponds to the examined frequency which would be similar to the test frequency of the defects of the tested bearings, and then information that no specific defect occurred in the tested bearing or bearings is automatically generated—(activity 114).

In order to determine the maximum value JA of the maximum likelihood function J the following mathematical relations are used:





  
    
      
        
          
            J
            A
          
          =
          
            
              ∑
              
                k
                =
                1
              
              
                N
                h
              
            
            ⁢
            
              
            
            ⁢
            
              
                [
                
                  A
                  k
                
                ]
              
              2
            
          
        
        ,
      
    
    
      
        (
        11
        )
      
    
  




where: Nh is the preset number of the examined harmonics,

and Ak is a harmonic amplitude determined in the time domain using the binary vector p, presented in the form of sinusoidal model.

The binary vector p is presented as a sum of sinusoidal model and the noise vector:





  
    
      
        
          
            p
            ⁡
            
              [
              n
              ]
            
          
          =
          
            
              
                ∑
                
                  k
                  =
                  1
                
                
                  N
                  h
                
              
              ⁢
              
                [
                
                  
                    
                      A
                      k
                    
                    ⁢
                    
                      cos
                      ⁡
                      
                        (
                        
                          n
                          ⁢
                          
                            
                          
                          ⁢
                          
                            ω
                            k
                          
                        
                        )
                      
                    
                    ⁢
                    
                      cos
                      ⁡
                      
                        (
                        
                          φ
                          k
                        
                        )
                      
                    
                  
                  -
                  
                    
                      A
                      k
                    
                    ⁢
                    
                      sin
                      ⁡
                      
                        (
                        
                          n
                          ⁢
                          
                            
                          
                          ⁢
                          
                            ω
                            k
                          
                        
                        )
                      
                    
                    ⁢
                    
                      sin
                      ⁡
                      
                        (
                        
                          φ
                          k
                        
                        )
                      
                    
                  
                
                ]
              
            
            +
            
              ɛ
              ⁡
              
                [
                n
                ]
              
            
          
        
        ,
      
    
    
      
        (
        12
        )
      
    
  




which can be also presented in the following matrix form:

p=Bθ+e  (13),

where:

    
    
        φk is a phase,
        ωk=2πνk/fs, k=1, 2 . . . Nh is angular velocity corresponding to a specific frequency (ν), a k=1, 2 . . . Nh,
        fs is the sampling frequency of the measured analogue signal when analogue-digital conversion is performed,
        e=[ε[n]]T—denotes the noise vector,
        n—denotes a natural number from 1 to N−1,
        N—denotes the number of elements in the binary vector p,
        B is the matrix of known constant parameters, presented in the following form:
    
    






  
    
      
        
          B
          =
          
            [
            
              
                
                  1
                
                
                  0
                
                
                  1
                
                
                  0
                
                
                  ...
                
                
                  1
                
                
                  0
                
              
              
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        ω
                        1
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          ω
                          1
                        
                        )
                      
                    
                  
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        ω
                        2
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          ω
                          2
                        
                        )
                      
                    
                  
                
                
                  ...
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        ω
                        
                          N
                          h
                        
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          ω
                          
                            N
                            h
                          
                        
                        )
                      
                    
                  
                
              
              
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          1
                        
                        ⁢
                        2
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            1
                          
                          ⁢
                          2
                        
                        )
                      
                    
                  
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          2
                        
                        ⁢
                        2
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            2
                          
                          ⁢
                          2
                        
                        )
                      
                    
                  
                
                
                  ...
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          
                            N
                            h
                          
                        
                        ⁢
                        2
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            
                              N
                              h
                            
                          
                          ⁢
                          2
                        
                        )
                      
                    
                  
                
              
              
                
                  ⋮
                
                
                  ⋮
                
                
                  ⋮
                
                
                  ⋮
                
                
                  
                    
                  
                
                
                  ⋮
                
                
                  ⋮
                
              
              
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          1
                        
                        ⁡
                        
                          (
                          
                            N
                            -
                            1
                          
                          )
                        
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            1
                          
                          ⁡
                          
                            (
                            
                              N
                              -
                              1
                            
                            )
                          
                        
                        )
                      
                    
                  
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          2
                        
                        ⁡
                        
                          (
                          
                            N
                            -
                            1
                          
                          )
                        
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            2
                          
                          ⁡
                          
                            (
                            
                              N
                              -
                              1
                            
                            )
                          
                        
                        )
                      
                    
                  
                
                
                  ...
                
                
                  
                    cos
                    ⁡
                    
                      (
                      
                        
                          ω
                          
                            N
                            h
                          
                        
                        ⁡
                        
                          (
                          
                            N
                            -
                            1
                          
                          )
                        
                      
                      )
                    
                  
                
                
                  
                    -
                    
                      sin
                      ⁡
                      
                        (
                        
                          
                            ω
                            
                              N
                              h
                            
                          
                          ⁡
                          
                            (
                            
                              N
                              -
                              1
                            
                            )
                          
                        
                        )
                      
                    
                  
                
              
            
            ]
          
        
        ,
      
    
    
      
        (
        14
        )
      
    
  




and θ is the vector of unknown parameters, presented in the following form: θ=└A1 cos(φ1), A1 sin(φ1), A2 cos(φ2), A2 sin(φ2), . . . , ANh cos(φNh), ANh sin(φNh)┘,

which is Least Square Estimator for this relation:

θ=(BTB)−1BTp  (15),

where p is a binary vector in this form:

p=[p[0], p[1], . . . , p[N−1]]T.

The comparison of the relations 12 and 13 allows to obtain values of harmonic amplitudes Ak, necessary to calculate the ratio JA which is then used to determine the place of defect occurrence, i.e. which bearing may be defective, and the type of the occurring defect.

The noise level nA is calculated using the median or mean values of the maximum function J found in the neighbourhood of the examined defect frequency ffK.

The final result of the performed activities is the automatic generation of information about the presence or absence of defects in the examined bearing or bearings. The occurrence of a defects causes an automatic generation of information which of the examined bearings has been damaged and what is the type of the defect.

## Claims

1. An method for detection and automatic identification of damage to rolling bearings, in which vibrations of a bearing in operation, measured as an analogue timewave signal, are converted into digital data and prefiltered, wherein the detection of shock pulses are performed with use of a binary vector (p) that is determined in the following actions: selecting a first and second adjacent vector intervals in the prefiltered digital timewave data, said first adjacent vector intervals being a reference interval and said second adjacent vector interval being a test interval, filtering the signal in said test interval and said reference interval multiple times whereupon after each filtering a shock pulse likelihood ratio is calculated as a ratio of mean square values of filtered signal present in said test interval to the mean square values of filtered signal present in said reference interval, comparing said likelihood ratios with a preset threshold value and the probability of shock pulse occurrence in the first test interval is estimated, recording information about shock pulse occurrence in said test interval as initial elements of binary vector (p), wherein if said likelihood ratio is greater than said preset threshold value, the elements of the binary vector (p) take the value 1 and if said likelihood ratio is less than said preset threshold value, the elements of the binary vector (p) take the value 0, and thereafter determining all remaining elements of the binary vector (p) for all successive test and reference intervals that are selected iteratively with an offset in a specific direction, wherein the identification of the defect in the bearing or bearings is done automatically for the binary vector (p) determined for all examined said test intervals and said reference intervals of timewave (X) of the processed signal and the set of known defect frequencies of examined bearing or bearings ((Ff)=[ff1, ff1, . . . ffK]), by means of the following actions:
for each successive, known defect frequency (ffK) from a set (Ft) of the examined bearing, a test frequency (νfKε└(1−Pg)ffK,(1+Pg)ffK┘) that belongs to a neighbourhood (Pg) of the frequency (ffK) is determined, where (Pg) is a configuration parameter denoting the searching frequency range related to known defect frequency and next, using maximum likelihood mathematical principles, for each test frequency (νfK) the maximum likelihood function (J) in time domain is determined using the binary vector (p), checking which test frequency (νfK) correlates to a maximum likelihood function value (JA), calculating a ratio (FA) of the maximum value (JA) to a noise level (nA) and comparing said ratio (FA) with a reset threshold parameter (SA): generating information about examined bearing defect with specific frequency that belongs to set (Ft) and corresponds to test (νfK) if the ratio (FA) is greater than the preset threshold parameter (SA), generating information that no specific defect occurred in the examined bearing or bearings if the ratio (FA) is less than or equal to the preset threshold (SA).

2. A method according to claim 1 wherein the mean square value of the signal in the test interval subjected to Lth filtering (τt[L]) is determined on the basis of the following relation:




  
    
      
        τ
        t
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          K
          t
        
      
      ⁢
      
        
          ∑
          
            
              k
              t
            
            =
            1
          
          
            K
            t
          
        
        ⁢
        
          
        
        ⁢
        
          
            
              z
              t
              L
            
            ⁡
            
              [
              
                k
                t
              
              ]
            
          
          2
        
      
    
  
  ,



whereas the mean square value of the signal in the reference interval subjected to Lth filtering (τr[L]) is determined on the basis of this relation:





  
    
      
        τ
        r
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          K
          r
        
      
      ⁢
      
        
          ∑
          
            
              k
              r
            
            =
            1
          
          
            K
            r
          
        
        ⁢
        
          
        
        ⁢
        
          
            
              z
              r
              L
            
            ⁡
            
              [
              
                k
                r
              
              ]
            
          
          2
        
      
    
  
  ,



where:
L—is a natural number from the interval 1 . . . NS and denotes the number of filters,
kt, kr denotes successive natural numbers 1 to Kt or to Kr,
ztL, denotes a vector representing the examined test interval of the signal subjected to Lth filtering,
zrL denotes a vector representing the examined reference interval of the signal subjected to Lth filtering.

3. A method according to claim 2, wherein the mean square value of a signal in the reference interval (τr[L]) is determined using Lth filtering, that is an adaptive filtering, with use of Singular Value Decomposition (SVD) of autocovariance matrix (Cr) according to the following relation:


Cr=VΣrUT,

where matrix (Σr) is a diagonal matrix whose diagonal elements are nonzero and nonnegative and denote mean square values (τr[L]):





  
    
      Σ
      r
    
    =
    
      [
      
        
          
            
              
                τ
                r
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            0
          
          
            ...
          
          
            0
          
        
        
          
            0
          
          
            
              
                τ
                r
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            0
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            0
          
          
            0
          
          
            ...
          
          
            
              
                τ
                r
              
              ⁡
              
                [
                L
                ]
              
            
          
        
      
      ]
    
  
  ,



and matrices (V) and (U) are orthogonal matrices and at the same time the autocovariance matrix (Cr) has the following form:





  
    
      C
      r
    
    =
    
      [
      
        
          
            
              r
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            
              r
              ⁡
              
                [
                L
                ]
              
            
          
        
        
          
            
              r
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                0
                ]
              
            
          
          
            ...
          
          
            
              r
              ⁡
              
                [
                
                  L
                  -
                  1
                
                ]
              
            
          
        
        
          
            ...
          
          
            ...
          
          
            ...
          
          
            ...
          
        
        
          
            
              r
              ⁡
              
                [
                L
                ]
              
            
          
          
            
              r
              ⁡
              
                [
                
                  L
                  -
                  1
                
                ]
              
            
          
          
            ...
          
          
            
              r
              ⁡
              
                [
                1
                ]
              
            
          
        
      
      ]
    
  
  ,



for which:





  
    r
    ⁡
    
      [
      
        i
        r
      
      ]
    
  
  =
  
    
      1
      
        K
        r
      
    
    ⁢
    
      
        ∑
        
          
            k
            r
          
          =
          1
        
        
          K
          r
        
      
      ⁢
      
        
      
      ⁢
      
        
          
            x
            r
          
          ⁡
          
            [
            
              k
              r
            
            ]
          
        
        ⁢
        
          
            x
            r
          
          ⁡
          
            [
            
              
                k
                r
              
              +
              
                i
                r
              
            
            ]
          
        
      
    
  



where:
xr[kr] are the elements of the reference interval,
kr denotes successive natural numbers from 1 to Kr,
it denotes successive natural numbers from 1 to L,
Kr denotes the length of the reference interval,
L denotes the number of adaptive filters.

4. A method according to claim 2, wherein the mean square value of a signal in the test interval (τt[L]) is determined using Lth filtering, that is an adaptive filtering, on the basis of the following relation:




  
    
      
        τ
        t
      
      ⁡
      
        [
        L
        ]
      
    
    =
    
      
        1
        
          N
          t
        
      
      ⁢
      
        
          ∑
          
            
              k
              t
            
            =
            1
          
          
            N
            t
          
        
        ⁢
        
          
        
        ⁢
        
          
            
              z
              t
              L
            
            ⁡
            
              [
              
                k
                t
              
              ]
            
          
          2
        
      
    
  
  ,



where ztL, are the elements of the matrix Zt presented in the following form:





  
    
      Z
      t
    
    =
    
      [
      
        
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                
                  N
                  t
                
                ]
              
            
          
        
        
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                3
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                1
              
              ⁡
              
                [
                
                  
                    N
                    t
                  
                  +
                  1
                
                ]
              
            
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  L
                  t
                
                ]
              
            
          
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  
                    L
                    t
                  
                  +
                  1
                
                ]
              
            
          
          
            ...
          
          
            
              
                z
                t
                L
              
              ⁡
              
                [
                
                  K
                  t
                
                ]
              
            
          
        
      
      ]
    
  
  ,



and calculated according to the following relation:


Zt=XtU, 


where matrix (Xt) is defined as:





  
    
      X
      t
    
    =
    
      [
      
        
          
            
              
                x
                t
              
              ⁡
              
                [
                1
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  N
                  t
                
                ]
              
            
          
        
        
          
            
              
                x
                t
              
              ⁡
              
                [
                2
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                3
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  
                    N
                    t
                  
                  +
                  1
                
                ]
              
            
          
        
        
          
            ⋮
          
          
            ⋮
          
          
            ⋱
          
          
            ⋮
          
        
        
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  L
                  t
                
                ]
              
            
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  
                    L
                    t
                  
                  +
                  1
                
                ]
              
            
          
          
            ...
          
          
            
              
                x
                t
              
              ⁡
              
                [
                
                  K
                  t
                
                ]
              
            
          
        
      
      ]
    
  
  ,



and matrix (U) is an orthogonal matrix whose elements are the adaptive filter coefficients, while:
Kt denotes the length of the examined test interval;
xt[kt], are the elements of the test interval;
kt denotes the successive natural numbers from 1 to Kt,
Nt=Kt−L,
L denotes the number of adaptive filters.

5. A method according to claim 1, wherein the multiple filtering of signals in said test interval and said reference interval is performed with use of band pass filter.

6. A method according to claim 1, wherein the length of said test interval (Kt)) is 15% of the length of said reference interval (Kr).

7. A method according to claim 1, wherein the test frequency (νfK), for which the maximum likelihood function calculated for the binary vector (p) in time domain reaches the maximum value (JA), is determined by maximising the sum of squares of harmonic amplitudes (Ak)) according to this relation:




  
    
      J
      A
    
    =
    
      
        ∑
        
          k
          =
          1
        
        
          N
          h
        
      
      ⁢
      
        
      
      ⁢
      
        
          [
          
            A
            k
          
          ]
        
        2
      
    
  
  ,



where: Nh is a preset number of the examined harmonics.

8. A method according to claim 7, wherein the values of the amplitudes of harmonics (Ak) are determined in the time domain using the binary vector (p), presented in the form of the sinusoidal model in which the binary vector (p) is presented as a sum of sinusoidal model and the noise vector:




  
    
      p
      ⁡
      
        [
        n
        ]
      
    
    =
    
      
        
          ∑
          
            k
            =
            1
          
          
            N
            h
          
        
        ⁢
        
          [
          
            
              
                A
                k
              
              ⁢
              
                cos
                ⁡
                
                  (
                  
                    n
                    ⁢
                    
                      
                    
                    ⁢
                    
                      ω
                      k
                    
                  
                  )
                
              
              ⁢
              
                cos
                ⁡
                
                  (
                  
                    φ
                    k
                  
                  )
                
              
            
            -
            
              
                A
                k
              
              ⁢
              
                sin
                ⁡
                
                  (
                  
                    n
                    ⁢
                    
                      
                    
                    ⁢
                    
                      ω
                      k
                    
                  
                  )
                
              
              ⁢
              
                sin
                ⁡
                
                  (
                  
                    φ
                    k
                  
                  )
                
              
            
          
          ]
        
      
      +
      
        ɛ
        ⁡
        
          [
          n
          ]
        
      
    
  
  ,



which can be also presented in the following matrix form:


p=Bθ+e, 


where:
φk is a phase,
ωk=2πνk/fs, k=1, 2 . . . Nh is an angular velocity corresponding to a test frequency (νfK), and k=1, 2 . . . Nh,
fs is a sampling frequency for analogue to digital processing of measured analogue signal,
e=[ε[n]]T denotes the noise vector,
n—denotes a natural number from 1 to N−1,
N—denotes number of elements in the binary vector (p),
B is the matrix of known constant parameters, presented in the following form:






  B
  =
  
    [
    
      
        
          1
        
        
          0
        
        
          1
        
        
          0
        
        
          ⋯
        
        
          1
        
        
          0
        
      
      
        
          
            cos
            ⁡
            
              (
              
                ω
                1
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  1
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                ω
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  2
                
                )
              
            
          
        
        
          ⋯
        
        
          
            cos
            ⁡
            
              (
              
                ω
                
                  N
                  h
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  ω
                  
                    N
                    h
                  
                
                )
              
            
          
        
      
      
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  1
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    1
                  
                  ⁢
                  2
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  2
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    2
                  
                  ⁢
                  2
                
                )
              
            
          
        
        
          ⋯
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  
                    N
                    h
                  
                
                ⁢
                2
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    
                      N
                      h
                    
                  
                  ⁢
                  2
                
                )
              
            
          
        
      
      
        
          ⋮
        
        
          ⋮
        
        
          ⋮
        
        
          ⋮
        
        
          
            
          
        
        
          ⋮
        
        
          ⋮
        
      
      
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  1
                
                ⁡
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    1
                  
                  ⁡
                  
                    (
                    
                      N
                      -
                      1
                    
                    )
                  
                
                )
              
            
          
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  2
                
                ⁡
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    2
                  
                  ⁡
                  
                    (
                    
                      N
                      -
                      1
                    
                    )
                  
                
                )
              
            
          
        
        
          ⋯
        
        
          
            cos
            ⁡
            
              (
              
                
                  ω
                  
                    N
                    h
                  
                
                ⁡
                
                  (
                  
                    N
                    -
                    1
                  
                  )
                
              
              )
            
          
        
        
          
            -
            
              sin
              ⁡
              
                (
                
                  
                    ω
                    
                      N
                      h
                    
                  
                  ⁡
                  
                    (
                    
                      N
                      -
                      1
                    
                    )
                  
                
                )
              
            
          
        
      
    
    ]
  



and θ is the vector of unknown parameters presented in the following form:
0=└A1 cos(φ1), A1 sin(φ1), A2 cos(φ2), A2 sin(φ2), . . . , ANk cos(φNh), ANh sin(φNh)┘,
which is the Least Square Estimator for the relation:


θ=(BTB)−1BTp 


where (p) is a binary vector in this form:
p=[p[0],p[1], . . . ,p[N−1]]T.

9. A method according to claim 1, wherein the noise level (nA) is calculated by taking a median value of maximum function values (J) found in the neighbourhood of the examined defect frequency (ffK) from the set (Ff).

10. A method according to claim 1, wherein the noise level (nA) is calculated by taking a mean value of maximum function values (J) found in the neighbourhood of the examined defect frequency (ffK) from the set (Ff).