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Description A time series of SEP electron fluxes at energies 25 (a), 50 (b), 75 (c), and 100 keV (d) as observed by SEP instrument onboard MAVEN during 15–23 December 2014.
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description Total electron impact ionization cross section of CO2+ obtained from theory (Jackman et al., ; Yogesh et al., ) and observations (Hudson et al., ; Rieke & Prepejchal, ).
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description Schematic diagram of IMF field lines around Mars (Schneider et al., ). The SEP electrons can enter into the atmosphere of Mars along these IMF field lines.
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description The limb intensities of CO2+ UVD due to impact of H+‐H at SZA 105° and 127° and SEP electron impact at energies 25, 50, 75, and 100 keV in the nighttime ionosphere of Mars. The estimated results...
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description The ion densities of CO2+, O2+, and NO+ due to impact of SEP electrons of 100 keV and H+‐H impact at SZA 105° and 127° in the nighttime ionosphere of Mars. The electron density (Ne) due to impact...
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description The ion production rates of CO2+, N2+, and O+ due to impact of SEP electrons of 100 keV and H+‐H impact at SZA = 105° and 127° in the nighttime ionosphere of Mars.
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description The ion production rates of CO2+ due to precipitation of SEP electrons at energies 25, 50, 75, and 100 keV in the nighttime ionosphere of Mars.
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics -
Description The orbit average solar wind plasma parameters between 15 and 23 December 2014. First top panel, (a) IMF field directions, theta and phi in degrees; second panel, (b) solar wind velocity in km/s;...
Article Title: Modeling of Diffuse Aurora due to Precipitation of H+‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation
Publication Title: Journal of Geophysical Research: Space Physics