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...
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...
We investigate the effects of solar energetic particle (SEP) events on the Martian ionosphere using ...
We have used radio occultation data obtained from Mars Global Surveyor (MGS) at high latitudes (65.3...
We have used Mars Global Surveyor (MGS) observations for the period 12 to 18 May 2005 to address the...
Responses of solar X-ray flares were observed in a layer of the Martian ionosphere at altitudes of ~...
From an analysis of electron density profiles recorded aboard Mars Global Surveyor, we report observ...
Solar extreme ultraviolet and X-ray photons are the main sources of ionization in the Martian ionosp...
The relationship of the solar flare and the Coronal Mass Ejection (CME) with the ionosphere is a key...
International audienceSolar extreme ultraviolet and X-ray photons are the main sources of ionization...
173-182The photoelectron flux, ion production rates and electron densities are calculated in the en...
We report the first global, time-dependent simulation of the Mars upper atmospheric responses to a r...
We report the first global, time-dependent simulation of the Mars upper atmospheric responses to a r...
The photoelectron flux, ion production rates and electron densities are calculated in the energy ran...
[1] We use a simple photochemical model of Mars ’ ionosphere to investigate the changes in calculate...
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...
We investigate the effects of solar energetic particle (SEP) events on the Martian ionosphere using ...
We have used radio occultation data obtained from Mars Global Surveyor (MGS) at high latitudes (65.3...
We have used Mars Global Surveyor (MGS) observations for the period 12 to 18 May 2005 to address the...
Responses of solar X-ray flares were observed in a layer of the Martian ionosphere at altitudes of ~...
From an analysis of electron density profiles recorded aboard Mars Global Surveyor, we report observ...
Solar extreme ultraviolet and X-ray photons are the main sources of ionization in the Martian ionosp...
The relationship of the solar flare and the Coronal Mass Ejection (CME) with the ionosphere is a key...
International audienceSolar extreme ultraviolet and X-ray photons are the main sources of ionization...
173-182The photoelectron flux, ion production rates and electron densities are calculated in the en...
We report the first global, time-dependent simulation of the Mars upper atmospheric responses to a r...
We report the first global, time-dependent simulation of the Mars upper atmospheric responses to a r...
The photoelectron flux, ion production rates and electron densities are calculated in the energy ran...
[1] We use a simple photochemical model of Mars ’ ionosphere to investigate the changes in calculate...
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...
We investigate the effects of solar energetic particle (SEP) events on the Martian ionosphere using ...