Wenas Wenas is the old version of code which takes a number of inputs and finds either the spectra , interferometry data and other things and writes the output to either an hdf file or ascii format. This code also creates an information file to tell the programs that use the hdf files where the specific time and ranges of the data are stored. The data is stored in a different directory called spec, so you must have a directory called spec off the current directory for this code to work. Pull is the code which can take the hdf files and either print out the information in a readable format or take the data and put it into smaller hdf files.
Work is in progress to create image files using pull.
The inputs for pull are listed below. It takes the raw radar data does some operations on it and creates hdf files containing the information. The inputs are listed below. Watermann uses the spectral data to estimate the moments of the autocorrelation function. Currently this code is being updated to also find a best fit exponential and Gaussian approximation, and with this information find a good estimate of the signal to noise ratio.