Corresponding Dataset for "Measurements of Europa's Ionosphere from Juno's close flyby"
<p> Corresponding Dataset for "Radio Occultation Measurements of Europa's </p><p> Ionosphere from Juno's close flyby"<br> Marzia Parisi<br> September 29, 2023<br> Jet Propulsion Laboratory<br> California Institute of Technology</p><p>=============================================================================<br>INTRODUCTION<br>=============================================================================</p><p> This dataset contains processed radio science data and results of the<br>Juno Europa radio occultation. This dataset is provided in order to <br>supplement the submitted article to the "Geophysical Research Letters"<br>journal:</p><p> Parisi, M. et al. (2023 or 2024), Measurements of Europa's Ionosphere from Juno's close flyby, Geophysical Research <br> Letters, submitted September 2023.</p><p>Please note the raw data used in this analysis are not provided in this<br>supplementary dataset. The raw Juno Gravity Science Data may be found at <br>the Planetary Data System:</p><p> </p><p> Buccino, D. R. (2016). Juno jupiter gravity science raw data set <br> V1.0, JUNO-J-RSS-1 JUGR-V1.0, NASA planetary data system (PDS). <br> Retrieved from https://atmos.nmsu.edu/PDS/data/jnogrv_1001/<br> </p><p>=============================================================================<br>ARCHIVE INFORMATION<br>=============================================================================</p><p> This archive contains two files within the root directory.<br> <br> - JunoE45OccData_Ingress_v1.csv</p><p> This data file contains the INGRESS data relevant to the radio<br> occultation. The data is a timeseries of impact parameter, </p><p> the uncalibrated frequency residuals, the calibrated frequency residuals, </p><p> Total Electron Content, Electron density, 1-sigma electron density uncertainty (thermal only) </p><p> and 1-sigma electron density uncertainty (thermal+trajectory).</p><p> </p><p> - JunoE45OccData_Egress_v1.csv</p><p> This data file contains the EGRESS data relevant to the radio<br> occultation. The data is a timeseries of impact parameter, </p><p> the uncalibrated frequency residuals, the calibrated frequency residuals, </p><p> Total Electron Content, Electron density, 1-sigma electron density uncertainty (thermal only) </p><p> and 1-sigma electron density uncertainty (thermal+trajectory).</p><p> </p><p>=============================================================================<br>FILE FORMAT<br>=============================================================================</p><p> This dataset contains only a comma-separated text files which are<br>given with the "*.csv" extension.</p><p><br> CSV FILES<br> -------------------------------------------------------------------------</p><p> The Comma-Separated Value (CSV) files are plain-text files. Values in<br> each data file are separated using a comma ",". Each column is defined <br> by a header row which provides a description of each column.<br> </p><p>=============================================================================<br>ACKNOWLEDGMENTS<br>=============================================================================</p><p>This work was carried out at the Jet Propulsion Laboratory, <br>California Institute of Technology, under contract with the National <br>Aeronautics and Space Administration. Government sponsorship acknowledged.</p><p>AC, EG, LGC, PT and MZ are grateful to the Italian Space Agency for financial support through</p><p>Agreement No. 2018-25-HH.0 in the context of ESA's JUICE mission, and Agreement</p><p>No. 2017-40-H.1-2020, and its extension 2017-40-H.02020-13-HH.0, for ESA's BepiColombo</p><p>and NASA's Juno radio science experiments. EG is grateful to "Fondazione Cassa dei</p><p>Risparmi di Forl`ı" for financial support of his PhD fellowship. PS was supported by NASA</p><p>Contract NNM06AA75C from the Marshall Space Flight Center under subcontract 699054X</p><p>from Southwest Research Institute. </p><p><br>=============================================================================<br>PRIMARY POINT OF CONTACT<br>=============================================================================</p><p>Marzia Parisi </p><p>Jet Propulsion Laboratory<br>Planetary Radar and Radio Sciences<br>(818) 354 - 0463 </p><p>marzia.parisi@jpl.nasa.gov</p><p>=============================================================================<br>ACRONYMS AND ABBREVIATIONS<br>=============================================================================</p><p> ASCII American Standard Code for Information Interchange<br> DOY Day of year<br> DSN Deep Space Network<br> JPL Jet Propulsion Laboratory<br> NAIF Navigation Ancillary Information Facility<br> NASA National Aeronautics and Space Administration<br> PDS Planetary Data System<br> RS Radio Science<br> RSS Radio Science Subsystem<br> SIS Software Interface Specification<br> TXT Text file<br> UTC Universal Time, Coordinated</p>
ShareScore
36/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 8
- Harmonization
- 4
- Access
- 12
- Reuse readiness
- 8
- Engagement
- 4