Review script for paper "2022Icar..37214724C" made with predictor "DataLinkerOptimizedRefine"

Created by Paper Data Linking Bot

Please review the download script and instrument details for the paper.

bibcode: 2022Icar..37214724C predictor: DataLinkerOptimizedRefine annotated pdf: view here (requires login)

Checklist

Download Script

[ ] Correct time ranges specified
[ ] Correct VSO instruments specified
[ ] Query returns good results or contains warning with reasoning if not
[ ] Physical observables omitted or correct
[ ] Wavelengths omitted or correct
[ ] Cadences omitted or correct

Instrument Details

[ ] Consistent with download_script.py

README

[ ] Contains the bibcode for the relevant paper
[ ] Contains the title for the relevant paper
[ ] Contains the authors for the relevant paper
[ ] VSO sources consistent with download_script.py
[ ] VSO instruments consistent with download_script.py

For more details, refer to the Contributing Guide.

Several instruments got binned together, and this -- I believe --led to a lack of specificity about the time for SUMER which should be April 20 1997. Perhaps being more sure that the instruments details split out by instrument instead of binning would be helpful. Structured responses may help with this, or just a prompt alteration.

### TIMED/SEE, SOHO/SUMER, and WHI Campaign
- **General Comments**:
   - These instruments provided solar flux data at various spectral resolutions used in the energy deposition model.
- **Supporting Quote**: "These neutral profiles are fed into an energy deposition model employing soft X-ray and Extreme UltraViolet (EUV) solar fluxes at a range of spectral resolutions (∆λ = 4×10−3 nm to 1 nm) assembled from TIMED/SEE, from SOHO/SUMER, and from the Whole Heliosphere Interval (WHI) quiet Sun campaign."

#### Data Collection Period 1: Solar Flux Measurements
- **Time Range**: Various dates in 1997 and 2008
   - **Supporting Quote**: "The WHI dataset is composed of measurements from the XPS instrument on TIMED/SEE between 0.1 – 6.0 nm, a rocket measurement between 6.0 – 105 nm, the EGS instrument on TIMED/SEE between 105 – 116 nm, and a SORCE/SOLSTICE spectrum beyond 116 nm. The rocket was launched on 14 April 2008, and the TIMED/SEE and SORCE/SOLSTICE spectra that compose the WHI spectrum are averages over 10 – 16 April 2008."
- **Wavelength(s)**: 0.1 to 152 nm
   - **Supporting Quote**: "The SUMER spectrum extends from 67 to 152 nm at a resolution of 4 × 10−3 nm."
- **Physical Observable**: Solar flux
   - **Supporting Quote**: "Our energy deposition model calculates ion production rate profiles through photo-ionisation and electron-impact ionisation processes."
- **Additional Comments**: The solar flux data was critical for modeling the ionization processes in Saturn's atmosphere.

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