Areas of enhanced ionization in the deep nightside ionosphere of Mars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F11%3A00482045" target="_blank" >RIV/68378289:_____/11:00482045 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1029/2011JE003804" target="_blank" >http://dx.doi.org/10.1029/2011JE003804</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1029/2011JE003804" target="_blank" >10.1029/2011JE003804</a>
Alternative languages
Result language
angličtina
Original language name
Areas of enhanced ionization in the deep nightside ionosphere of Mars
Original language description
We present observations of areas of enhanced ionization located in the deep nightside ionosphere of Mars as observed by Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on board the Mars Express spacecraft. Oblique ionospheric echoes coming from the same region observed during several consecutive MARSIS measurements enable us to constrain the geographic location of the reflection area that is the source of the echoes. We have identified 90 such events in all available data. None of the reflection areas are located in regions typically having a closed magnetic field line configuration. The locations of the reflection areas of enhanced plasma density are consistent with the ionization due to precipitating electrons on field lines connected to the collisional atmosphere. Reflection areas observed in regions of stronger magnetic field are found to have larger plasma number density. We use a model of Martian crustal magnetic field lines to demonstrate that the magnetic field has a focusing effect on incident particles. Electron impact ionization is thus expected to take place only in well-defined areas, in agreement with our observations. Our observations show that the deep nightside ionosphere of Mars is very irregular, controlled primarily by the configuration of crustal magnetic fields. Copyright © 2011 by the American Geophysical Union.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2011
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
ISSN
0148-0227
e-ISSN
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Volume of the periodical
116
Issue of the periodical within the volume
6
Country of publishing house
US - UNITED STATES
Number of pages
9
Pages from-to
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UT code for WoS article
000292383300002
EID of the result in the Scopus database
2-s2.0-79960167430