Precipitating Electron Energy Flux and Characteristic Energies in Jupiter's Main Auroral Region as Measured by Juno/JEDI
- Submitting institution
-
The University of Leicester
- Unit of assessment
- 9 - Physics
- Output identifier
- 1933
- Type
- D - Journal article
- DOI
-
10.1029/2018JA025639
- Title of journal
- Journal of Geophysical Research: Space Physics
- Article number
- -
- First page
- 7554
- Volume
- 123
- Issue
- 9
- ISSN
- 2169-9402
- Open access status
- Compliant
- Month of publication
- August
- Year of publication
- 2018
- URL
-
-
- Supplementary information
-
https://doi.org/10.1029/2018JA025639
- Request cross-referral to
- -
- Output has been delayed by COVID-19
- No
- COVID-19 affected output statement
- -
- Forensic science
- No
- Criminology
- No
- Interdisciplinary
- No
- Number of additional authors
-
24
- Research group(s)
-
B - Planetary Science
- Citation count
- 16
- Proposed double-weighted
- No
- Reserve for an output with double weighting
- No
- Additional information
- -
- Author contribution statement
- The paper presents a comparison of plasma data with theory for electron acceleration above Jupiter's auroras. Nichols was centrally involved in this study from its inception in Juno Science Team meetings. Specifically, he contributed the computer code, expertise and text regarding the theoretical model used in Section 3 "Data/theory comparison". The lines plotted on Figure 4b are from the computer code contributed by Nichols. He contributed significantly to the interpretation of the comparison with data described in Section 5, which is a central component of the paper and its conclusions.
- Non-English
- No
- English abstract
- -
