Corresponding Dataset for "Electron Density in Io's Alfvén Wing Observed via Radio Occultation with Juno"
<div> Corresponding Dataset for "Electron Density in Io’s Alfvén Wing </div> <div> Observed via Radio Occultation with Juno"</div> <div> README FILE</div> <div> Dustin Buccino</div> <div> July 15, 2024</div> <div> Jet Propulsion Laboratory</div> <div> California Institute of Technology</div> <div> </div> <div>=============================================================================</div> <div>INTRODUCTION</div> <div>=============================================================================</div> <div> </div> <div> This dataset contains processed radio science data and results of the</div> <div>Juno Ganymede radio occultation. This dataset is provided in order to </div> <div>supplement the submitted article to the "Geophysical Research Letters"</div> <div>journal:</div> <div> </div> <div> Buccino, D.R., et al (2024), Electron Density in Io’s Alfvén Wing </div> <div> Observed via Radio Occultation with Juno, Geophysical Research </div> <div> Letters, submitted July 2024.</div> <div> </div> <div> </div> <div> Please note the raw data used in this analysis are not provided in this</div> <div>supplementary dataset. The raw Juno Gravity Science Data may be found at </div> <div>the Planetary Data System:</div> <div> </div> <div> Buccino, D. R. (2016). Juno jupiter gravity science raw data set </div> <div> V1.0, JUNO-J-RSS-1 JUGR-V1.0, NASA planetary data system (PDS). </div> <div> Retrieved from https://atmos.nmsu.edu/PDS/data/jnogrv_1001/</div> <div> </div> <div> </div> <div>=============================================================================</div> <div>ARCHIVE INFORMATION</div> <div>=============================================================================</div> <div> </div> <div> This archive contains ten files within the root directory.</div> <div> </div> <div> </div> <div> I57 Data</div> <div> </div> <div> i57_observed.txt</div> <div> Raw frequency observables. Reported as X-band minus Ka-band,</div> <div>see paper for details (X_freq - 880.0/3360.0*Ka_freq)</div> <div> </div> <div> i57_tec.csv</div> <div>Total electron content information from the flyby</div> <div>(uncalibrated, model, calibrated data)</div> <div> </div> <div> i57_density_inbound_raytracing.txt</div> <div>Estimated electron density inbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i57_density_outbound_raytracing.txt</div> <div>Estimated electron density outbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i57_density_tubes.csv</div> <div>Estimated electron density during the flyby using</div> <div>the horizontal tubes method (see paper)</div> <div> </div> <div> I58 Data</div> <div> </div> <div> i58_observed.txt</div> <div> Raw frequency observables. Reported as X-band minus Ka-band,</div> <div>see paper for details (X_freq - 880.0/3360.0*Ka_freq)</div> <div> </div> <div> i58_tec.csv</div> <div>Total electron content information from the flyby</div> <div>(uncalibrated, model, calibrated data)</div> <div> </div> <div> i58_density_inbound_raytracing.txt</div> <div>Estimated electron density inbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i58_density_outbound_raytracing.txt</div> <div>Estimated electron density outbound during the flyby </div> <div>estimated with the ray tracing method (see paper)</div> <div> </div> <div> i58_density_tubes.csv</div> <div>Estimated electron density during the flyby using</div> <div>the horizontal tubes method (see paper)</div> <div> </div> <div>=============================================================================</div> <div>FILE FORMAT</div> <div>=============================================================================</div> <div> </div> <div> This dataset contains only ASCII formatted files. There are two formats,</div> <div> a plain-text file with the extension *.txt and a comma-separated file</div> <div> with the extension *.csv.</div> <div> </div> <div> </div> <div> PLAIN-TEXT FILES</div> <div> -------------------------------------------------------------------------</div> <div> </div> <div> The plain ASCII text files (TXT) files are fixed-width columns. Values in</div> <div> each data file are separated with spaces. Each column is defined </div> <div> by a header row which provides a description of each column.</div> <div> </div> <div> CSV FILES</div> <div> -------------------------------------------------------------------------</div> <div> </div> <div> The Comma-Separated Value (CSV) files are plain-text files. Values in</div> <div> each data file are separated using a comma ",". Each column is defined </div> <div> by a header row which provides a description of each column.</div> <div> </div> <div> </div> <div>=============================================================================</div> <div>ACKNOWLEDGMENTS</div> <div>=============================================================================</div> <div> </div> <div>The work of DB, MP, RP, and SL was carried out at the Jet Propulsion </div> <div>Laboratory, California Institute of Technology, under a contract with the </div> <div>National Aeronautics and Space Administration. Government sponsorship </div> <div>acknowledged.</div> <div> </div> <div>AC, LGC, MZ, EG, and PT are grateful to the Italian Space Agency (ASI) for </div> <div>financial support through Agreement No. 2023-6-HH.0 in the context of ESA’s </div> <div>JUICE mission, and Agreement No. 2022-16-HH.0, for ESA’s BepiColombo and </div> <div>NASA’s Juno radio science experiments.</div> <div> </div> <div>PW and DC acknowledge support from NASA award 80NSSC23K0020.</div> <div> </div> <div>PS was supported by NASA Contract NNM06AA75C from the Marshall Space </div> <div>Flight Center under subcontract 699054X from Southwest Research Institute.</div> <div> </div> <div>(c) 2024 California Institute of Technology. Government sponsorship </div> <div>acknowledged.</div> <div> </div> <div>=============================================================================</div> <div>PRIMARY POINT OF CONTACT</div> <div>=============================================================================</div> <div> </div> <div>Dustin Buccino</div> <div>Jet Propulsion Laboratory</div> <div>Planetary Radar and Radio Sciences</div> <div>(818) 393 - 1072</div> <div>Dustin.R.Buccino@jpl.nasa.gov</div> <div> </div> <div>=============================================================================</div> <div>ACRONYMS AND ABBREVIATIONS</div> <div>=============================================================================</div> <div> </div> <div> ASCII American Standard Code for Information Interchange</div> <div> DOY Day of year</div> <div> DSN Deep Space Network</div> <div> JPL Jet Propulsion Laboratory</div> <div> NAIF Navigation Ancillary Information Facility</div> <div> NASA National Aeronautics and Space Administration</div> <div> PDS Planetary Data System</div> <div> RS Radio Science</div> <div> RSS Radio Science Subsystem</div> <div> SIS Software Interface Specification</div> <div> TXT Text file</div> <div> UTC Universal Time, Coordinated</div>
ShareScore
28/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 0
- Engagement
- 0
Dataset details
- Repository
- zenodo
- Published
- July 17, 2024
- License
- cc-by-4.0
- DOI
- 10.5281/zenodo.12746259
Scored with release 0.9.0
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