Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/35944
Title: Evidence of scale height variations in the Martian ionosphere over the solar cycle
Authors: Sanchez-Cano, Beatriz
Lester, M.
Witasse, O.
Milan, S. E.
Hall, B. E. S.
Blelly, P. L.
Radicella, S. M.
Morgan, D. D.
First Published: 24-Nov-2015
Citation: Journal of Geophysical Research: Space Physics, 2015, DOI: 10.1002/2015JA021949
Abstract: Solar cycle variations in solar radiation create density changes in any planetary ionosphere, which are well established in the Earth's case. At Mars, however, the ionospheric response to such changes is not well understood. We show the solar cycle impact on the topside ionosphere of Mars, using data from the Mars Advance Radar for Subsurface and Ionospheric Sounding (MARSIS) on board Mars Express. Topside ionospheric variability during the solar cycle is analyzed through neutral scale height behavior. For moderate and high solar activity phases, the topside electron density profile is reproduced with an altitude-variable scale height. However, for the period of extremely low solar activity in 2008 and 2009, the topside was smaller in density than in the other phases of the solar cycle, and there is evidence that it could be reproduced with either a constant scale height or a height-variable scale height with lower electron density. Moreover, the ionosphere during this time did not show any apparent dependence on the EUV flux. This singular behavior during low solar activity may respond to the presence of an induced magnetic field which can penetrate to lower ionospheric altitudes than in other phases of the solar cycle due to the reduced thermal pressure. Numerical simulations of possible scenarios for two different solar cycle phases indicate that this hypothesis is consistent with the observations.
DOI Link: 10.1002/2015JA021949
ISSN: 2169-9402
Links: http://onlinelibrary.wiley.com/wol1/doi/10.1002/2015JA021949/abstract
http://hdl.handle.net/2381/35944
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2015, The Authors. This is an open-access article distributed under the terms of the Creative Commons Attribution License ( http://creativecommons.org/licenses/by/4.0/ ), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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