Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95423/1/jgra20373.pd
Solar extreme ultraviolet and X‐ray photons are the main sources of ionization in the Martian ionosp...
An edited version of this paper was published by AGU. Copyright 2019 American Geophysical Union.The ...
International audienceModel studies of the ionosphere of Mars under daytime conditions reveal that f...
We have calculated photoelectron flux, ion production rates, and electron densities in the Martian i...
173-182The photoelectron flux, ion production rates and electron densities are calculated in the en...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95006/1/jgra21110.pd
Many aspects of the Martian upper atmosphere are known to vary with solar zenith angle (SZA). One wo...
The photoelectron flux, ion production rates and electron densities are calculated in the energy ran...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95296/1/jgre1782.pd
Photoelectrons are important for heating, ionization, and airglow production in planetary atmosphere...
This paper presents a study of the energetics of the dayside ionosphere of Mars using models and dat...
Photoelectron peaks in the 20â 30Â eV energy range are commonly observed in the planetary atmospher...
a b s t r a c t Using an electron transport model, we calculate the electron density of the electron...
Understanding the evolution of the Martian atmosphere requires knowledge of processes transforming s...
This is an open access article under the CC BY-NC-ND license.This work uses a subset of “q...
Solar extreme ultraviolet and X‐ray photons are the main sources of ionization in the Martian ionosp...
An edited version of this paper was published by AGU. Copyright 2019 American Geophysical Union.The ...
International audienceModel studies of the ionosphere of Mars under daytime conditions reveal that f...
We have calculated photoelectron flux, ion production rates, and electron densities in the Martian i...
173-182The photoelectron flux, ion production rates and electron densities are calculated in the en...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95006/1/jgra21110.pd
Many aspects of the Martian upper atmosphere are known to vary with solar zenith angle (SZA). One wo...
The photoelectron flux, ion production rates and electron densities are calculated in the energy ran...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95296/1/jgre1782.pd
Photoelectrons are important for heating, ionization, and airglow production in planetary atmosphere...
This paper presents a study of the energetics of the dayside ionosphere of Mars using models and dat...
Photoelectron peaks in the 20â 30Â eV energy range are commonly observed in the planetary atmospher...
a b s t r a c t Using an electron transport model, we calculate the electron density of the electron...
Understanding the evolution of the Martian atmosphere requires knowledge of processes transforming s...
This is an open access article under the CC BY-NC-ND license.This work uses a subset of “q...
Solar extreme ultraviolet and X‐ray photons are the main sources of ionization in the Martian ionosp...
An edited version of this paper was published by AGU. Copyright 2019 American Geophysical Union.The ...
International audienceModel studies of the ionosphere of Mars under daytime conditions reveal that f...
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