You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
This is handled by pyrate.vcm.cvd. Currently the calculation of autocovariance follows the method used in the Matlab code. This method truncates the covariance data used to fit the exponential model by the dimension of the minimum image axis. Is this sensible? Should we not include data at any distance from the zero-lag pixel? The consequence may well be that the exponential model may not be a good fit when the full data is included
Other models could also be introduced, like the zero-th order Bessel function, and a method to determine the best fitting 'type' of model for a particular data set by calculating weighted RMS on the model-observation residuals.
Below is a Matlab example of the method currently used to decimate autocovariance data. Values are plotted against distance (radius) in km from zero lag pixel. In Figure 1 the values have been truncated at ~1.8 km - the width of the image x-axis. In Figure 2, the values have been binned. In Figure 3, the mean of each bin has been calculated. This is the data that is input into the function fitting algorithm (fmin).
The text was updated successfully, but these errors were encountered:
This is handled by pyrate.vcm.cvd. Currently the calculation of autocovariance follows the method used in the Matlab code. This method truncates the covariance data used to fit the exponential model by the dimension of the minimum image axis. Is this sensible? Should we not include data at any distance from the zero-lag pixel? The consequence may well be that the exponential model may not be a good fit when the full data is included
Other models could also be introduced, like the zero-th order Bessel function, and a method to determine the best fitting 'type' of model for a particular data set by calculating weighted RMS on the model-observation residuals.
Below is a Matlab example of the method currently used to decimate autocovariance data. Values are plotted against distance (radius) in km from zero lag pixel. In Figure 1 the values have been truncated at ~1.8 km - the width of the image x-axis. In Figure 2, the values have been binned. In Figure 3, the mean of each bin has been calculated. This is the data that is input into the function fitting algorithm (fmin).
The text was updated successfully, but these errors were encountered: