Solar cycle variations in the ionosphere of Mars

1. Beatriz Sánchez-Cano
2. Mark Lester
3. Olivier Witasse
4. Pierre-Louis Blelly
5. Marco Cartacci
6. Sandro M. Radicella
7. Miguel Herráiz

Export

Export

×

MLA

modern-language-association

APA

apa

Chicago

chicago-fullnote-bibliography

Harvard

harvard-cite-them-right

Vancouver

vancouver-author-date

---

RIS BibTex

Export

×

This document cannot be exported because it belongs to another portal.

Full text

lock_openFull text externo

DOI: 10.5209/REV_FITE.2016.V28.53899 DIALNET GOOGLE SCHOLAR lock_openOpen access editor

More publications in: Física de la tierra

Abstract

Solar cycle variations in solar radiation create notable changes in the Martian ionosphere, which have been analysed with Mars Express plasma datasets in this paper. In general, lower densities and temperatures of the ionosphere are found during the low solar activity phase, while higher densities and temperatures are found during the high solar activity phase. In this paper, we assess the degree of influence of the long term solar flux variations in the ionosphere of Mars.

Data source: Dialnet