The repository contains 3 major folders corresponding to the three orbits of Cassini:
  - Enceladus Plume_279
  - Enceladus Plume_286
  - Enceladus Plume_290
  Each of these folders contain a subfolder with the calibrated files for their respective orbits:
      - calibrated_S100_279
      - calibrated_S101_286
      - calibrated_S101_290
  The calibrated .erpj files contain the I/F data we use in our analysis.
  
The repo contains wavelength_vims.txt file that containts the wavelengths used in this analysis.

The jupyter notebooks in the repo:
   - Enceladus plume background removal.ipynb creates and saved the following files for each orbit. 
     The below file names are just example for orbit no 279
       - outlier_cube_indices_279.txt saves the index of outliers cubes/images in orbit no 279
       - images_binned_indices_279.txt saves the index of images/cubes that have been averaged/binned together in multiple of 10 each. 
         For example first 10 cubes that are binned together have indices [4, 5, 6, ...] of size 10
       - inten_before_alt_279.txt plume spectra intensity across altitude before background removal in the 
         shape of 240 spectral channels, 29 orbital phases, 30 altitudes. 
         Values are stored with their respective standard deviation.
       - inten_after_alt_279.txt plume spectra intensity across altitude after background removal in the 
         shape of 240 spectral channels, 29 orbital phases, 30 altitudes. 
         Values are stored with their respective standard deviation.
         
   - Mie Code_100.ipynb generates mie spectra at the scattering angles of all 3 orbits and uses the folliwing:
        - 100.txt contains the refractive index at 100K for all the relevant wavelength channels.
        - encplume_filelist_geom_S100_279_062420 contains the parameters for the corresponding orbit. (SImilary for the other 2 orbits)
        And creates the following files:
        - File wavelength_index.txt stores the index at which the wavelength for which refractive indices 
          (used to generate mie spectra) are defined coincides with the wavelength corresponding to plume observations.
        - File mie_wavelength.txt contains the wavelength for mie spectra
        - File plume_wavelength.txt contains the wavelength for plume spectra
        - File max_radius.txt saves the maximum radius for each of the 676 combinations of size parameters
        - File power_index.txt saves the power law index for each of the 676 combinations of size parameters
        - Folder Enceladus Plume_279 (similarly for orbit 286 and 290)
              - File binned_orbital_phase_279.txt that stores binned orbital phase values for orbit no. 279
              - File binned_scattering_angle_279.txt that stores binned scattering angle values for orbit no. 279
        - File mie_spectra_100.txt stores the spectra generated using mie scattering theory. 
        - File mie_scatt_angle.txt save the 32 scattering angles for which mie spectra is generated.

   - Plume and Mie binning_100_50 real.ipynb creates the following important files (these are replicated for the other 2 orbits):
        - plume_spectra_279_100_50 
        - scatt_index_279: these files save the index of the scattering angles
        - mie_spectra_279_100_50: contacins mie spectra with augmentations
        - plume_spectra_279_100_50_err
        - plume_spectra_279_orb_100_50
        
   - ML model_100_50 calculates the fianl results : 
        - plume_spectra_results_279_100_50 and similarly for the other 2 orbits
        - EW_mie_augmented
        - EW_plume_augmented
        - mie_spectra_rad
        - mie_spectra_pow
        - max_rad_50_aug_man
        - pow_50_aug_man
        - size_orb_50_aug_man