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Flare X‐ray photochemistry of the E region ionosphere of Mars
Based on electron density profiles obtained from the Mars Global Surveyor (MGS) we report X‐ray flare responses in the E region ionosphere of Mars during six events that occurred on 28 March and 6 April 2001, 17 and 18 March and 21 April 2003, and 19 February 2005. We have developed a time‐dependent...
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Published in: | Journal of geophysical research. Space physics 2016-07, Vol.121 (7), p.6870-6888 |
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Main Authors: | , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Based on electron density profiles obtained from the Mars Global Surveyor (MGS) we report X‐ray flare responses in the E region ionosphere of Mars during six events that occurred on 28 March and 6 April 2001, 17 and 18 March and 21 April 2003, and 19 February 2005. We have developed a time‐dependent Analytical Yield Spectrum model to calculate a time series of photoionization rate, photoelectron impact ionization rate, photoelectron flux, ion density, electron density, and ionospheric electron content (IEC) of the E region for each flare day. The estimated production rate, flux, and densities increase by 1–2 orders of magnitude due to effect of these flares in the E region ionosphere of Mars. The estimated IEC are compared with the measured IEC. It is found that the normalized IEC of the simulated E layer increased by a factor of 5–10 at the flare time compared to a factor of 2 enhancements in the normalized IEC of the corresponding MGS profiles.
Key Points
Production and densities in Martian ionosphere
Six new flare responses in the Martian ionosphere
Modeling of X‐ray aeronomy of Mars |
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ISSN: | 2169-9380 2169-9402 |
DOI: | 10.1002/2016JA022435 |