MARSIS observations of the Martian nightside ionosphere dependence on solar wind conditions
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10288988" target="_blank" >RIV/00216208:11320/14:10288988 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1002/2014JA019788" target="_blank" >http://dx.doi.org/10.1002/2014JA019788</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1002/2014JA019788" target="_blank" >10.1002/2014JA019788</a>
Alternative languages
Result language
angličtina
Original language name
MARSIS observations of the Martian nightside ionosphere dependence on solar wind conditions
Original language description
Despite the absence of solar radiation on the Martian nightside, a weak, irregular, and variable ionosphere is produced there. The nightside ionosphere is thought to be maintained by two main sources: dayside-nightside plasma transport and electron precipitation. Observations by Mars Express (MEX) and Mars Global Surveyor (MGS) have shown that these plasma sources are either hindered or favored by the presence of strong crustal magnetic fields and that these effects are modulated by external parameters,such as the solar wind dynamic pressure and the orientation of the interplanetary magnetic field (IMF). These external drivers are expected to influence the supply of plasma to the nightside and thus the formation of the irregular nightside ionosphere.We here present a statistical study of the Martian ionosphere at solar zenith angle greater than 107 degrees from November 2005 to May 2006, using remote measurements of ionospheric echoes with the Mars Advanced Radar for Subsurface and I
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BL - Plasma physics and discharge through gases
OECD FORD branch
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Result continuities
Project
<a href="/en/project/LH13031" target="_blank" >LH13031: Ionosphere of Mars: Radar soundings by the Mars Express spacecraft</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Journal of Geophysical Research - Space Physics
ISSN
2169-9380
e-ISSN
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Volume of the periodical
119
Issue of the periodical within the volume
5
Country of publishing house
US - UNITED STATES
Number of pages
17
Pages from-to
4077-4093
UT code for WoS article
000337622100060
EID of the result in the Scopus database
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