binchensun
commented
4 months ago - Use beamforming calibration tables to determine beamforming flux correction factors.
- Determine time-dependent correction factors by considering 1) the exact factor csv file to be used and 2) solar altitude
- Apply the correction factors to the beamforming data and generate new hdf5/fits files. These would be our level 1 data products.
- Determine background from daily drift scan data and subtract it from the data, export hdf5/fits files. These would be our level 1.5 data products.