Solar cycle variations in the ionosphere of Mars

被引：2

作者：

Sanchez-Cano, Beatriz ^{[1
]}

Lester, Mark ^{[1
]}

Witasse, Olivier ^{[2
]}

Blelly, Pierre-Louis ^{[3
]}

Cartacci, Marco ^{[4
]}

Radicella, Sandro M. ^{[5
]}

Herraiz, Miguel ^{[6
,7
]}

机构：

[1] Univ Leicester, Dept Phys & Astron, Radio & Space Plasma Phys Grp, Leicester, Leics, England

[2] European Space Agcy, ESTEC Sci Support Off, Noordwijk, Netherlands

[3] Inst Rech Astrophys & Planetol, Toulouse, France

[4] Ist Nazl Astrofis INAF, IAPS, Rome, Italy

[5] Abdus Salam Int Ctr Theoret Phys ICTP, Telecommun ICT Dev Lab, Str Costiera 11, I-34151 Trieste, Italy

[6] Univ Complutense Madrid, Dept Fis Tierra Astron & Astrofis 1, E-28040 Madrid, Spain

[7] UCM, CSIC, Inst Geociencias, Madrid, Spain

来源：

FISICA DE LA TIERRA | 2016年 / 28卷

基金：

英国科学技术设施理事会;

关键词：

solar cycle; ionosphere of Mars; TEC;

D O I：

10.5209/rev_FITE.2016.v28.53899

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

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.

引用

页码：97 / 110

页数：14

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