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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • 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

  • 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

  • UT code for WoS article

    000292383300002

  • EID of the result in the Scopus database

    2-s2.0-79960167430