Proton Aurora on Mars: A Dayside Phenomenon Pervasive in Southern Summer
Open Access
- 12 December 2019
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Space Physics
- Vol. 124 (12), 10533-10548
- https://doi.org/10.1029/2019ja027140
Abstract
No abstract availableKeywords
Funding Information
- National Aeronautics and Space Administration
This publication has 40 references indexed in Scilit:
- Mars H Escape Rates Derived From MAVEN/IUVS Lyman Alpha Brightness Measurements and Their Dependence on Model AssumptionsJournal of Geophysical Research: Planets, 2018
- Elevated atmospheric escape of atomic hydrogen from Mars induced by high-altitude waterNature Geoscience, 2017
- The structure and variability of Mars dayside thermosphere from MAVEN NGIMS and IUVS measurements: Seasonal and solar activity trends in scale heights and temperaturesJournal of Geophysical Research: Space Physics, 2017
- Analysis and modeling of remote observations of the martian hydrogen exosphereIcarus, 2017
- A strong seasonal dependence in the Martian hydrogen exosphereGeophysical Research Letters, 2015
- Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphereJournal of Geophysical Research: Planets, 2014
- Unexpected variability of Martian hydrogen escapeGeophysical Research Letters, 2014
- Dayside induced magnetic field in the ionosphere of MarsIcarus, 2010
- Discovery of an aurora on MarsNature, 2005
- Martian magnetic morphology: Contributions from the solar wind and crustJournal of Geophysical Research, 2003