About: Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events     Goto   Sponge   NotDistinct   Permalink

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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 of ionograms 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 list-type=%22bulleted%22> <list-item id=%22grl51372-li-0001%22>List of SEP events compiled using the Mars Express data <list-item id=%22grl51372-li-0002%22>Nightside ionosphere during these periods is extremely enhanced <list-item id=%22grl51372-li-0003%22>Ionization below 80 km, evidence for magnetic shadow effect
  • 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 of ionograms 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 list-type=%22bulleted%22> <list-item id=%22grl51372-li-0001%22>List of SEP events compiled using the Mars Express data <list-item id=%22grl51372-li-0002%22>Nightside ionosphere during these periods is extremely enhanced <list-item id=%22grl51372-li-0003%22>Ionization below 80 km, evidence for magnetic shadow effect (en)
Title
  • Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events
  • Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events (en)
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  • Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events
  • Enhanced ionization of the Martian nightside ionosphere during solar energetic particle events (en)
skos:notation
  • RIV/00216208:11320/14:10288940!RIV15-MSM-11320___
http://linked.open...avai/riv/aktivita
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  • I, P(LH13031)
http://linked.open...iv/cisloPeriodika
  • 3
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  • 14672
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  • RIV/00216208:11320/14:10288940
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  • nightside ionosphere; Mars Express; MARSIS (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [F0D2A8641435]
http://linked.open...i/riv/nazevZdroje
  • Geophysical Research Letters
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
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  • 41
http://linked.open...iv/tvurceVysledku
  • Gurnett, D. A.
  • Morgan, D. D.
  • Němec, František
  • Dieval, C.
  • Futaana, Y.
http://linked.open...ain/vavai/riv/wos
  • 000332990500007
issn
  • 0094-8276
number of pages
http://bibframe.org/vocab/doi
  • 10.1002/2013GL058895
http://localhost/t...ganizacniJednotka
  • 11320
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