Display device

Abstract: In a superimposing display device that superimposes indicators upon the image seen in the viewfinder are provided a display means that displays multiple displays in fields superimposed upon said image of said viewfinder, a detection means that detects the brightness intensity of said fields, and a control means that controls the brightness of said displays, said control means controlliong the brightness intensity information concerning a field obtained by the detection means. The superimpose indicators are displayed at several locations and by application of both a phased constant drive and brightness modulation, thereby enabling to display superimposed indicators with a wide dynamic range capable of keeping track of an object possessing a brightness pattern.

Description: BACKGROUND OF THE INVENTION Field of the Invention The present invention generally relates to a display device which is overlaid on a picture in the viewfinder of a camera. Related Background Art In past conventional models, since all information such as the exposure and lens opening was indicated outside a picture frame in a viewfinder, a rough parallelism between the brightness of the information and that of the object to be photographed was enough to ensure basic visual comfort. One example of this is U.S. Patent No. 4,692,014 in which the brightness level of an indication outside the frame is controlled in accordance with average photometric data obtained within the frame. Another way to control the brightness level of the indication outside the frame which is disclosed in Japanese Patent Application No. 62-6344 (No Patent Application made in the United States) is based on photometric information obtained by measuring the brightness of the frame's periphery and by measuring the brightness level of the frame after dividing it into several blocks. Document EP-A-0 224 336 discloses a camera capable of visually displaying photographic information within the viewfinder by superimposing the respective information onto the observed image or scene, and of adjusting the brightness of the information display in response to scene brightness. In detail, an alphanumeric display comprised of a plurality of light emitting diodes mounted on a circuit board is arranged such that the light emitted by the light emitting diodes, which represents the information to be displayed, is optically transmitted by a prism into a lens group, thereby rendering the information visible in the eye-piece. Further, the camera provides a brightness detect mode for detecting ambient scene brightness prior to exposure, being capable of discriminating between a high and a low ambient scene brightness by using a brightness threshold value. According to the ambient scene brightness being high or low, the light emitting diodes are adjusted to appear bright or dim, respectively. SUMMARY OF THE INVENTION When an indication is "superimposed" on an object in a frame it is sometimes vague because of the object's brightness. On the other hand, when the indication is too bright against the object, then it becomes uncomfortable to look at it. One aspect of the present invention is the possibility to choose whether or not to have a superimposed indication within the frame and if the indication is chosen, the brightness in compliance with the numeric information will track the brightness of the object to ensure utmost visual comfort. Another aspect of this invention is the automatic variation of the brightness of the information in response to that of the object. Since this is made possible through a phased combination of a constant-current drive and a brightness modulation drive, photometric error under low brightness due to delayed response of the photometric sensor is prevented. According to the invention the aforementioned object is accomplished by a superimposing display device for displaying and superimposing indicators upon an image seen in a viewfinder, said device comprising: display means for selectively displaying a plurality of indicators and superimposing the image of each of said plurality of indicators in a corresponding one of a plurality of fields defined upon the image observed in the viewfinder; detection means for detecting brightness intensity information of the image scene observed in the viewfinder; and control means for controlling the brightness of said plurality of indicators in accordance with the brightness intensity information obtained by said detection means; characterized in that said detection means is arranged to detect the brightness intensity information of the image scene within each of said fields; and said control means individually controls the brightness of each of said indicators in the corresponding field in accordance with the brightness intensity information of said corresponding field obtained by said detection means. Furthermore, the object is accomplished by a camera comprising a viewfinder and the aforementioned superimposing display device. Further advantages, features and objects of the present invention will become apparent from the following description of a preferred embodiment taken in conjunction with the accompanying drawings, of which: BRIEF DESCRIPTION OF THE DRAWINGS Figures 1A and 1B show explanatory drawings of a camera according to an embodiment of the present invention. Figure 2 shows an example of indication in the viewfinder. Figure 3 shows a schematic circuit diagram of the camera according to the present embodiment. Figure 4 shows a photometric circuit and drive according to the present embodiment. Figure 5 shows a drive current and drive time for indication. Figure 6 shows a time sharing relationship between indication and photometry. Figure 7 shows a relationship between current and drive time pertaining to the indication. Figure 8 shows a flow chart. DETAILED DESCRIPTION OF PREFERRED EMBODIMENT The explanatory Figure 1A shows a camera seen from the side. The reference numeral 1 denotes a mount, 2a a main mirror, 2b a sub-mirror, 3 a film surface, 4 a LED flood light prism, 5 a focusing frame, 6 a device for displaying information outside the frame reticle in the viewfinder, 7 a pentaprism, 8 a photometric lens for the SPC photometric sensor, and 9 an eyepiece of the viewfinder, and 10 a sensor for autofocusing. The light passing through the objective (not shown in the figure) is deflected 90° by the main mirror 2a and reflected by the pentaprism 7 and reaches the eye after passing through the eyepiece 9. The light reflected by the sub-mirror 2b is directed to the autofocusing sensor 10. The light reaching the matter field of the focusing frame 5 is projected onto the SPC photometric sensor via the photometric lens 8. The LED light passes through the LED flood light prism 4 and is reflected by the main-mirror 2a. The light is deflected vertically by the microprism array 5a on the indicator portion of the focusing frame 5 and travels through the pentaprism 7 to reach the eye via the eyepiece 9. By selectively distributing this microprism array 5a of the focusing frame 5 it is possible to use the LED light source to obtain bright LED indications like the so-called superimpose indicators d1, d2 and d3 shown in Figure 2. The superimpose indicators d1 to d3 are superimposed on the object inside the frame reticle of the viewfinder 9. Accordingly, an appropriate brightness should be found since they must be indicated with a brightness that is not outshone by the brightness of the subject. Conversely, if they are too bright, they may hamper observation of the object. Hitherto, indications, like the information generated by the display device 6, have been shown outside the frame reticle device and could not get lost in the viewfinder image. Selecting a reasonable brightness once for all was enough. However, to track the brightness of the object when superimposing, it is necessary to change the brightness of the superimpose indicators d1 to d3 to follow the camera's 20-step dynamic photometric range. The three fields Z1 to Z3, shown in Figure 2, indicate the photometric fields of the SPC photometric sensor. These fields, including the superimpose indicators d1 through d3, can be distributed as necessary. Figure 3 shows the circuit that actualizes the present embodiment. The photometric sensors SPC1 to SPC3 correspond to the fields Z1 to Z3. Each sensor is connected with photometric amplifiers AMP1 to AMP3 and condenser diodes DI1 to DI3 to thereby transform the light into electric impulses and the logarithmical compressed voltage is transmitted to the inputs IN1 to IN3 of the MPX multiplexers. One of the inputs IN1 to IN3, selected as the SELECT terminal signal, is sent via OUT to the A/D converter and read-out by the CPU central processing unit (hereinafter referred to only as CPU). The following elements are connected in the internal BUS of the microcomputer; ROM where the programs are stored in; RAM contains the random access memory concerning the work area for arithmetic functions; EEPROM is a non-volatile storage for storing non-volatile memory like data concerning adjustments, PIO is general-use input and output port; TIMER, which is a timer/counter. The CPU executes according to the ROM program and has access to the ROM, RAM, EEPROM, PIO, TIMER and A/D converter. The LEDs corresponding to the superimpose indicators d1 to d3 (Figure 2) are called LED1 to LED3 and each has three constant current sources I i1 to I i3 (I corresponds to LED1 to LED3). These constant current sources are constructed in a way so that when the register REG's output Bij is HIGH they are in 'enable' state. When LOW, they are in 'disable' state. The photometric circuit will be described with reference to Figure 4. The condenser diode DI1 contains a condenser C1. As explained above, the brightness of the superimpose indicators d1 to d3 must be adjusted to track the brightness of the subject in the viewfinder 9 in order to obtain an image easily observed with the eye. The brightness of the object processed by the camera is divided into a maximum of 20 different levels. When brightness modulation is used to maintain such a wide dynamic range, problems like that indicated in (a) may appear. In modulation, a large current should be used to allow observation under high brightness conditions. During low brightness conditions, the LED should light for a short time and duty should be shortened to thereby suppress the brightness observed by the human eye. The output of the SPC1 photometric sensor in the form of the photo-electric current ISPC1 is greatly increased when the LED lights. Accordingly, the electric charge is sufficient to charge the capacitor C1 and the current is quickly returned to a balanced state. However, particularly in the case of subjects with low brightness, even when the LED is put out, the photo-electric current ISPC1, depending upon the brightness of the subject, used to discharge the charged capacitor C1 has not yet reached a balanced state at the time 't'. (b) shows the drive when a low electric current and long lighting time is applied and (a), that will appear to be the same as (b) when observed by the human eye, shows the drive when a high electric current and short lighting time is applied. In the case of (b), the photo-electric current ISPC1 does not increase so much according to the lighting of the LED and the charge of the capacitor C1 also requires time. Since the potential difference of the voltage V1 between a lighted state and un-lighted state is small, it is possible for the current to reach a balanced state at the 't' time instant. Accordingly, during low brightness condition, it is practical to control the LED drive current in order to maintain a LED brightness that keeps track of the brightness of the object. However, it is difficult to maintain a wide dynamic range only by utilizing electric current. On the other hand it is also difficult to obtain a 20-step brightness modulation by brightness modulation alone. When superimposing, the SPC photometric sensor measures the object. Since the superimpose indicators d1 to d3 appear within the sensitivity distribution, the light intensity is increased by the presence of the superimpose indicators d1 to d3. Accordingly, if photometry is carried out while the superimpose indicators d1 to d3 are displayed, the measured output will consist of wrong data. A time sharing process is therefore indispensable. Figure 6 shows a relationship between photometry and a time sharing of superimpose indication, where t = 0 - T a represents the maximum display time in the indicator section, and t = T b - T C denotes a photometry section. Since the photometry is based upon man-made flickering, it is desirable for the photometry to be carried out within a range of approximately 8.3 ms - 10.0 ms in view of power frequency of 50Hz or 60Hz. However, to prevent the superimpose indicators d1 to d3 from flickering the cycle T c should be at a frequency where the human eye cannot perceive the flicker, that is below 20 ms and above 50Hz. Accordingly, TLEDON-MAX = T a should be within 10 ms(= 20 ms - 10 ms). Since the mechanism in which a tracked wide dynamic-range brightness control is applied, as stated before, to the object brightness, involving the Figure 4(b) driving, T wait is necessitated, with maximum value of T wait added to TLEDON-MAX resulting in 10 ms (20 ms - 10 ms). In other words, as shown in Figure 6, while the superimpose is suspended, the photometry is performed for a T measure span during which man-made light source flickering is inhibited. And then, the display is lit for a T x period at a brightness that corresponds to the photometric output for the object to be displayed. And before the next measurement, there will be a T wait span of waiting time that allows the voltage at the photometric circuit to settle down to a level that corresponds to the voltage for the brightness of the object. An ample wait-time may be secured in addition to a T wait span by having this display luminance modulation successive to the previous sequence, eliminating any intervening gap. Figure 5 is a graphic presentation of the relationships among the superimpose display corresponding to the object brightness, the drive current and the drive time, with the horizontal bar showing by logarithm the object brightnesses on the PINT plate 5, and the vertical bar showing the LED-lit time T x , and the drive current of the superimpose display at a phase shown at Figure 6. With reference to Figure 5, a strong drive current is applied when the object is very bright like line one, and the drive current should be decreased as the object brightness goes down. With regard to the luminance modulation, as the brightness darkens below T x = T a , the drive time must be exponentially shortened. Figure 7 shows the currents and the drive-time lengths, T x , corresponding respectively to point a through point f, with the vertical line length representing the current and the horizontal "on" span T x . Figure 7 seems to show that the superimpose display time should be halved as the object brightness halves or darkens one-step. It should be noted, however, that T x does not correspond to T a /2 at x = 20, while Figure 5 shows T x = T a at x = 20. This is caused by the nature of human eye wanting the drive time to be. For example, even if the ratio of line one to line two may be one to eight, the drive time ratio of line one to line two at which the human eye perceives the object to be at the same brightness, the drive time ratio still does not agree to one eights, resulting from the unlinear relationship between the current and the beam quantity. With γ j (j = 1-3) as modulation factor for the current line 1 - line 3. Therefore, T x = T a × 1 2 γJ(Lj-x) This equation represents assured proper operation of the superimpose for the following reasons: Here, γ j is recommendably 0.4 - 0.8, depending on LED. With regard to L j (j=1-3) and points a, c and e, as the object brightness goes down below point a, it changes as shown by points b and g along the line 1 and at point c, it trips over to the line 2. Points g and c refer to where the human eye perceives as the same brightness. In this manner, simple application of modulation factors like L₁, L₂, L₃ and γ₁, γ₂, γ₃ to the equation shown above allows superimpose operation that is free of undesirable influences from such as the human eye characteristics, LED characteristics, constant current fluctuations, dispersion in LED beam projection, etc. Furthermore, combined use of duty-drive and gradual-constant-current drive provides for superimpose coverage over a wide and dynamic range. Figure 8 represents the following: ST01: The photometry, computation and display are performed as the main routine operation. In addition, timered insertion is also available when it carries timewise compatibility as well as simultaneous operation of another program. This main routine operation is based on an arrangement LED (i) i=1-3 with the input coming in via port PIO; and also on a setting in which, with regard to LED 1-3, 1 for on and 0 for off as per the input from another program (auto-focus as explained later on); and also on the modulation factors (γ j , L j , j=1-3) are written in EEPROM at the factory. ST02: Calling of the photometric routine. N represents the input factor, that is, the number of the photometric sampling; and AD(i),1-3 stands for the object brightness within the sensitivities of the three sensors. In the photometric routine, the measured value AD(i) of each sensor is taken from the mean value of several sampling within the T measure time span. At this time, superimpose indicator is putout. ST03: A brightness decision routine is called. As stated above, a superimpose display should be neither too bright nor too dark since it will be overlaid on the object to be photographed in the frame of the view finder, Therefore, the display and photometric area should be placed proportionately as shown in Figure 2. When only LED1 flashes on, the brightness of it must necessarily be determined by the photometric output power of area Z1. It will be the same for LED2 and for LED3. However, when more than two LEDs are lit up simultaneously, it will be difficult to access control because of the differences in contrast between indicators resulting from the brightness of each corresponding object. At the same time, when one sees into the viewfinder, he or she may feel uncomfortable, because of the difference in brightness of the LEDs. When only one of the superimpose LEDs is operating, the brightness of the indicator to be lit up as against that of the object to be photographed will be the same to everyone and no one will be able to tell the difference at this level. However, it would be easy to see the difference between two levels of brightness when there are more than two LEDs in operation. In this case, it may be unpleasant to notice every level of difference in brightness. This problem will be solved, in the Light DEFINE Routine mode, as shown in step 3, by taking the average photometric output power of each corresponding zones, and by driving both displays with the same brightness or substantially the same brightness. The input variables of this Routine are LED (i) = 1 to 3 which are the flashing LEDs, and AD (i) i = 1 to 3 which is the photometric value of the three photometric sensors. The output variables, 'x' determine the brightness of the flashing LEDs on the focus panel 5. ST04: The brightness information 'x' on the focus panel 5 is the input power, and the electrical current plus the duty drive time T x are the output power. The method shown in Figure 5 is algorithmic in principle. ST05: A Display Driven Routine is called. The input power information is regulated by the combination of the following factors; constant electrical current, duty driven time 'T x ', and LED (i) i = 1 to 3 which represent the LED to be lit up. ST06: Wait for 'T wait ' is necessary for safe photometry. Then, it will go back to the photometric routine - call mode. Now the explanation about each sub-routine will be made. ST11: Photometric routine. ST12: In order to measure the flicker of an artificial light source, some sampling of photometry is needed. The number of flickers should be counted, and the value 'T LOOP ' which is the photometric sensitivity, will be taken from that number. The three sensors are monitored to determine the photometric average as described in the following formula; T LOOP = T measure 3 × N When the number of sensors become 'm' pieces, the 3 of the above formula will be changed into 'm' and 'fori = 1 to 3' in step 17 will be 'for i = 1 to m'. ST13 to 15: To get the average value of 'N' times of three sensors, the value of SUM (i) 1 to 3 should be temporary cleared. ST18: To do the photometry of the 'i' th number of sensor IN i should be selected by transmitting the output power to a port of multiplexer. ST19: Do a A/D conversion through the A/D converter and make that value "D". ST20: Repeat the calculation of SUM (i) = SUM (i) + D. ST21: Wait for 'T LOOP ' which have been obtained from ST 12. ST16 to ST23: Repeat the processes of ST18 through ST21 'N' times and do the sampling of TOTAL 3 x 'N' times. It means that 'AD' value of the corresponding sensor has been already added 'N' times to SUM (i) i = 1 to 3. ST24 to ST26: AD (i) = SUM (i) N i = 1 to 3 tells that the average photometry value 'N' times, of each corresponding sensor, will be inputted to each 'AD (i)'. Namely, it means that the brightness of the object on focus panel 5, when the LED is off, which has been inputted into AD (i), was correspondingly determined by each sensor. ST27: Return to Main Routine. ST31: Light-Define Routine ST32: Temporarily make the variables SUM = bit = 0. ST33 to ST37: LED which is expected to light as described in "LED (i) = 1" and others which should be off as described in "LED (i) = 0". The number of LEDs which should be lighted with the variables 'bit' is counted, and the photometric value AD (i) of the sensors which corresponds to each LED is calculated to obtain 'SUM'. ST38: When the number of LEDs to be lighted is 0, bit = 0, and therefore the process goes to ST40 in order to avoid the error of the mathematical division by zero. ST39: Calculate the average photometric value of the sensors, which corresponds to the flashing LEDs by x = SUM bit ST40: Return to Main Routine ST51: Calculation Routine ST52: Retrieve the adjustment data of γ₁ - γ₃, and L₁ - L₃ which have been inputted in EEPROM. ST53 to ST60: Formulate 'j' and 'T x ' as follows to clarify the relation of 'x' and L₁, L₂, L₃ in Figure 5. The above calculation has been obtained from ST53 to ST60. Current = 1 to 3 corresponds to the constant electrical currents of lines 1 to 3, in Figure 5, respectively. ST61: Return to Main Routine. ST71: LED Driven Routine ST72 to ST76: Set the output of B ij of register REG while watching the (i) value of the expected lighting LEDs. For example, when LED 1 is driven by the constant electrical current source 2 (line 2), the constant electrical current I₁₂ will be turned on by setting B₁₂ high, and LED 1 will be driven by the electrical current corresponding to line 2. ST77: Wait for lighting time T x . ST78 to ST82: Turn off all LEDs by making B = 0, including those lighted during ST72 through ST76. ST83: Wait for 'T a - T x ' time. ST84: Return to Main Routine. Ideally, delay time due to execution of program should be taken into consideration when setting the wait time. However, in order to be practical, we have excluded the factor for simplicity sake, and because the value of it is small enough to discard. ST90: Auto-focus Routine This auto-focus routine is the program which has been drawn from the Main routine mode. It has three measuring areas which have been set up almost in the same way as the superimpose area of d1 - d3 shown in Figure 1. This will be achieved by setting up the position of sensor 10 for focus and for photometry. ST91: Select the mode for auto-focus. Auto-focus will be possible by three area measurements. There is a manual-mode in which the photographer can select a certain measuring area, and auto-focus mode where 3 sets of sensors measure an adequate amount of area automatically. ST92: It judges, when the auto-focus mode is selected, where the main subject is located within the three measuring areas. For example, it judges that the nearest object is the main subject and achieves automatic focusing by the output of the particular sensor for that area. ST93: When the manual mode is selected, activate the superimpose display (one of d1, d2 or d3) which corresponds to an area selected among the three measuring areas. And, give the command when the auto-mode is selected, to flash the superimposition of d1 to d3 which corresponds to the measuring areas on the focus lens. In this case, the number of indicated superimposition d1 to d3 is not necessarily one. ST94: Return In the present embodiment, the photometric fields of the SPC photometry sensor corresponding to the superimpose indicators d1 to d3 are slightly larger than the indicators, but one indicator corresponds to one sensor. However, sometimes one indicator area may stretch over the photometric fields of several SPC photometry sensors. In this case, the average of the outputs of the involved sensors is output and used to control the brightness to obtain an optimum display. The operation is based on the average value of the logarithmical compressed photometric values in the case of this embodiment, but by giving priority to bright sensor outputs and then basing the operation on the average output, an even more appropriate brightness of the superimpose indicators d1 to d3 is obtainable. In the embodiment mentioned above, it was decided to calculate the ON duration of the brightness modulation of the superimpose indicators d1 to d3 as T x = T a x 2 -γ(L-X) However, in some cases the program area necessary to operate 2 -γ(L-X) becomes too large. In these cases, in advance the previously mentioned T x method should be followed to store in memory several (x, T x ) computation tables. By referring to these tables it is possible to calculate according to the T x method in most cases. By employing the above described method to drive the display, it is possible to offer a display brightness that is visually more appropriate also in the case of the kind of display indications that appear in normal viewfinders. As described above, the superimpose indicators d1 to d3 are displayed at several locations, when selecting one indicator among several to be displayed, this indicator will have a brightness corresponding to the brightness of the corresponding field of the object. If more than 2 indicators are selected to be displayed, the brightness of the display will be determined by the average output determined by the brightness intensity of the fields corresponding to the indicators. In this way it is possible to obtain an optimum display of the indications superimposed on the object inside the frame reticle of the viewfinder 9. The superimpose indicators d1 to d3 will neither be too light nor too dark, but will keep track with the brightness of the object. At the same time it is possible to obtain a camera display device that is also capable of maintaining balance of brightness between several superimpose indicators. In the embodiment, by application of both a phased constant drive and brightness modulation it is possible to display superimposed indicators d1 to d3 with a wide dynamic range capable of keeping track of an object possessing a brightness pattern also characterized by a wide dynamic range. By activating the light state, wait state and display state in a cyclic order it is possible to control the brightness of the display so the brightness in near real-time follows the brightness of the object. In addition, it is possible to prevent bad influences upon the photometry. By parallel application of the phased constant-current drive and brightness modulation, the amount of stray light is kept to a minimum especially in the case of low brightness conditions. Accordingly, the slowness of the response speed of the SPC photometer sensor in the case of low brightness conditions is effective in preventing erroneous light measuring. Furthermore, since the duration of both the display state and wait state in the embodiment is kept below 10 ms, a display with a frequency above 50 Hz that is not seen to flicker by the human eye becomes obtainable even when the photometric period of about 10 ms, that is necessary to prevent flicker, is added in the embodiment. Since the brightness of the superimpose indicators d1 to d3 is maintained by a simple brightness modulation method, it is possible to offer a visually comfortable display that is always easily discernible. Since individual eyesights vary greatly, the control of the display is systematized, opeing up for simplified process adjustment The improved capacity of the memory, where the data concerning adjustments is stored, also contributes to minimizing the adjustment variables.

Claims: A superimposing display device for displaying and superimposing indicators upon an image seen in a viewfinder (9), said device comprising: display means (LED, 4, 5a) for selectively displaying a plurality of indicators (d1, d2, d3) and superimposing the image of each of said plurality of indicators (d1, d2, d3) in a corresponding one of a plurality of fields (Z1, Z2, Z3) defined upon the image observed in the viewfinder; detection means (SPC1, SPC2, SPC3) for detecting brightness intensity information of the image scene observed in the viewfinder; and control means (CPU) for controlling the brightness of said plurality of indicators in accordance with the brightness intensity information obtained by said detection means; characterized in that said detection means (SPC1, SPC2, SPC3) is arranged to detect the brightness intensity information of the image scene within each of said fields (Z1, Z2, Z3); and said control means (CPU) individually controls the brightness of each of said indicators (d1, d2, d3) in the corresponding field (Z1, Z2, Z3) in accordance with the brightness intensity information of said corresponding field (Z1, Z2, Z3) obtained by said detection means (SPC1, SPC2, SPC3). A device according to claim 1, characterized in that said indicators (d1, d2, d3) are provided as light radiation elements superimposed within a viewfinder. A device according to claim 1, characterized in that the display time (T x ) of said display means and the detection time (T c ) of said detection means (SPC1 to SPC3) are staggered. A device according to claim 1, characterized in that said control means (CPU), in case that one indicator (d1, d2, d3) is selected to be displayed, controls the brightness of said display based upon the brightness intensity information of the field (Z1, Z2, Z3) corresponding to the selected indicator, while in case that two or more indicators are displayed simultaneously, the control of the display brightness of the indicators is based upon an average brightness intensity of all corresponding fields. A device according to claim 1, characterized in that said control means (CPU) utilizes both phased constant-current drive andindicatorsbrightness modulation to control the brightness of said indicators (d1, d2, d3). A device according to claim 2, characterized in that the control of the brightness of said light radiating elements by said control means (CPU) is obtained both by phased constant-current drive and duty restricted brightness modulation. A device according to claim 3, characterized in that a wait state (T wait ) is provided between said display time (T x ) caused by the display means and said detection time (T c ) caused by said detection means (SPC1 to SPC3), and said display time (T x ), said wait state (T wait ), and said detection time (T c ) are repeated in a cyclic order. A device according to claim 7, characterized in that the total duration of both said display time (T x ) and said wait state (T wait ) is below 10 ms. A device according to one of the preceding claims 3, 7, or 8, characterized in that said display time T x of a lighted one of said indicators (d1, d2, d3) is determined according to the formula T x = T a · 2 -γ(L-x) where T a represents the maximum display time; x is the brightness of the image; L is the brightness of the image when the display time T x corresponds to the maximum display time T a ; and γ represents a linearity constant. A device according to claim 2, characterized in that LED's (LED1 to LED3) are used as said light radiating elements. A device according to claim 9, characterized in that said control means (CPU) determines the duration of the display time (T x ) of said indicators (d1, d2, d3) corresponding to said fields (Z1, Z2, Z3). A camera comprising a viewfinder and the superimposing display device defined in any of claims 1 to 11. A camera according to claim 12, characterized by further comprising a second detection means (ST90) for detecting a focusing condition of an object located within the fields (Z1, Z2, Z3) substantially corresponding to said plurality of indicators (d1, d2, d3). A camera according to claim 13, characterized in that said display means selectively displays the indicators (d1, d2, d3) based upon the information obtained by said second detection means (ST90). A camera according to claim 14, characterized in that said second detection means (ST90) outputs information that is used in order to display the field indicators (d1, d2, d3) in the infocus state. A camera according to claim 12, characterized by further comprising a focusing means that allows selective detection of a focusing condition of an object located within the fields (Z1, Z2, Z3) substantially corresponding to said multiple indicators (d1, d2, d3). A camera according to claim 16, characterized in that said display means selectively displays the indicators (d1, d2, d3) based upon the information obtained by said second detection means (ST90).

Inventors: HARADA YOSHIHITO C O CANON KAB, HARADA, YOSHIHITO, C/O CANON KABUSHIKI KAISHA
Applicants: CANON KK, CANON KABUSHIKI KAISHA
Application year: 1990
Main classification: G03B17
IPC codes: G03B17