Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10288940" target="_blank" >RIV/00216208:11320/14:10288940 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1002/2013GL058895" target="_blank" >http://dx.doi.org/10.1002/2013GL058895</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1002/2013GL058895" target="_blank" >10.1002/2013GL058895</a>
Alternative languages
Result language
angličtina
Original language name
Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events
Original language description
Electron densities in the Martian nightside ionosphere are more than 90% of time too low to be detected by the Mars Advanced Radar for Subsurface and Ionosphere Sounding radar sounder on board the Mars Express spacecraft. However, the relative number ofionograms with peak electron density high enough to be detected represents a good statistical proxy of the ionospheric density. We focus on solar energetic particle (SEP) events, and we analyze their effects on ionospheric formation. SEP time intervals were identified in situ using the background counts recorded by the ion sensor of the ASPERA-3 instrument on board Mars Express. We show that peak electron densities during the SEP events are large enough to be detected in more than 30% of measurements, and, moreover, the reflections of the sounding signal from the ground almost entirely disappear. Nightside electron densities during SEP events are thus substantially increased as compared to normal nightside conditions. Key Points <list l
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
Geophysical Research Letters
ISSN
0094-8276
e-ISSN
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Volume of the periodical
41
Issue of the periodical within the volume
3
Country of publishing house
US - UNITED STATES
Number of pages
6
Pages from-to
793-798
UT code for WoS article
000332990500007
EID of the result in the Scopus database
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