scholarly journals Oblique reflections in the Mars Express MARSIS data set: Stable density structures in the Martian ionosphere

2014 ◽  
Vol 119 (5) ◽  
pp. 3944-3960 ◽  
Author(s):  
D. J. Andrews ◽  
M. André ◽  
H. J Opgenoorth ◽  
N. J. T. Edberg ◽  
C. Diéval ◽  
...  
Author(s):  
B. Sánchez-Cano ◽  
O. Witasse ◽  
M. Herraiz ◽  
S. M. Radicella ◽  
J. Bauer ◽  
...  

Abstract. Since 2005 the Mars Advanced Radar and Ionospheric Sounding experiment (MARSIS) aboard Mars Express has acquired a unique data set on the ionosphere of Mars made up of ionospheric soundings taken by the instrument working in its Active Ionospheric Sounding (AIS) mode. These soundings play a role similar to those of modern Terrestrial digisondes in the analysis of our planet ionosphere and have allowed us to dramatically improve our knowledge about the Martian ionosphere. This paper describes this kind of data, which are available from the public Planetary Science Archive, and introduces the MAISDAT tool developed by the European Space Agency to analyze and derive the vertical profile of electron density. Comparisons with radio-occultation profiles obtained from Mars Express Radio Science instrument are performed to validate the procedure used in this study.


Science ◽  
2005 ◽  
Vol 310 (5749) ◽  
pp. 837-839 ◽  
Author(s):  
M. Pätzold ◽  
S. Tellmann ◽  
B. Häusler ◽  
D. Hinson ◽  
R. Schaa ◽  
...  

The daytime martian ionosphere has been observed as a two-layer structure with electron densities that peak at altitudes between about 110 and 130 kilometers. The Mars Express Orbiter Radio Science Experiment on the European Mars Express spacecraft observed, in 10 out of 120 electron density profiles, a third ionospheric layer at altitude ranges of 65 to 110 kilometers, where electron densities, on average, peaked at 0.8 × 1010 per cubic meter. Such a layer has been predicted to be permanent and continuous. Its origin has been attributed to ablation of meteors and charge exchange of magnesium and iron. Our observations imply that this layer is present sporadically and locally.


2012 ◽  
Vol 29 (4) ◽  
pp. 337-342 ◽  
Author(s):  
Eojin Kim ◽  
Haingja Seo ◽  
Joo Hyeon Kim ◽  
Joo Hee Lee ◽  
Yong Ha Kim ◽  
...  

2009 ◽  
Vol 27 (12) ◽  
pp. 4533-4545 ◽  
Author(s):  
N. J. T. Edberg ◽  
U. Auster ◽  
S. Barabash ◽  
A. Bößwetter ◽  
D. A. Brain ◽  
...  

Abstract. We report on new simultaneous in-situ observations at Mars from Rosetta and Mars Express (MEX) on how the Martian plasma environment is affected by high pressure solar wind. A significant sharp increase in solar wind density, magnetic field strength and turbulence followed by a gradual increase in solar wind velocity is observed during ~24 h in the combined data set from both spacecraft after Rosetta's closest approach to Mars on 25 February 2007. The bow shock and magnetic pileup boundary are coincidently observed by MEX to become asymmetric in their shapes. The fortunate orbit of MEX at this time allows a study of the inbound boundary crossings on one side of the planet and the outbound crossings on almost the opposite side, both very close to the terminator plane. The solar wind and interplanetary magnetic field (IMF) downstream of Mars are monitored through simultaneous measurements provided by Rosetta. Possible explanations for the asymmetries are discussed, such as crustal magnetic fields and IMF direction. In the same interval, during the high solar wind pressure pulse, MEX observations show an increased amount of escaping planetary ions from the polar region of Mars. We link the high pressure solar wind with the observed simultaneous ion outflow and discuss how the pressure pulse could also be associated with the observed boundary shape asymmetry.


2013 ◽  
Vol 118 (8) ◽  
pp. 5348-5357 ◽  
Author(s):  
Takuya Hara ◽  
Kanako Seki ◽  
Yoshifumi Futaana ◽  
Masatoshi Yamauchi ◽  
Stas Barabash ◽  
...  

Icarus ◽  
2010 ◽  
Vol 206 (1) ◽  
pp. 83-94 ◽  
Author(s):  
D.A. Gurnett ◽  
D.D. Morgan ◽  
F. Duru ◽  
F. Akalin ◽  
J.D. Winningham ◽  
...  

2017 ◽  
Vol 145 ◽  
pp. 1-8 ◽  
Author(s):  
E. Dubinin ◽  
M. Fraenz ◽  
M. Pätzold ◽  
D. Andrews ◽  
O. Vaisberg ◽  
...  

2014 ◽  
Vol 119 (7) ◽  
pp. 5891-5908 ◽  
Author(s):  
D. D. Morgan ◽  
C. Diéval ◽  
D. A. Gurnett ◽  
F. Duru ◽  
E. M. Dubinin ◽  
...  

2008 ◽  
Vol 41 (9) ◽  
pp. 1335-1346 ◽  
Author(s):  
D.A. Gurnett ◽  
R.L. Huff ◽  
D.D. Morgan ◽  
A.M. Persoon ◽  
T.F. Averkamp ◽  
...  

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