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Intensity of nightside MARSIS AIS surface reflections and implications for low-altitude ionospheric densities

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10319443" target="_blank" >RIV/00216208:11320/15:10319443 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1002/2014JA020888" target="_blank" >http://dx.doi.org/10.1002/2014JA020888</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1002/2014JA020888" target="_blank" >10.1002/2014JA020888</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Intensity of nightside MARSIS AIS surface reflections and implications for low-altitude ionospheric densities

  • Original language description

    Spacecraft radar sounding signals at frequencies higher than the ionospheric peak plasma frequency are not reflected by the ionosphere. Instead, they make it to the ground where they are reflected by the planetary surface. We analyze the intensity of thesurface reflections measured by the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) ionospheric radar sounder on board the Mars Express spacecraft. Apart from the surface reflectivity and the spacecraft altitude, the detected intensity of surface reflections is controlled primarily by the signal attenuation during the ionospheric propagation. We focus on the nightside region, where the ionospheric densities in the main layer are too low to cause a significant attenuation and allow sampling of the surface reflections at frequencies down to 3MHz. The attenuation occurs mainly at altitudes below 100km, where the electron-neutral collision frequency is a maximum. The intensity of surface reflections can thus serve as a

  • Czech name

  • Czech description

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

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

    2015

  • 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

  • Volume of the periodical

    120

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    14

  • Pages from-to

    3226-3239

  • UT code for WoS article

    000354894800062

  • EID of the result in the Scopus database

    2-s2.0-84929619798