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  • Using 8 years of CHAMP satellite observations of the equatorial electron temperature, T(e), we investigate its behavior during the morning overshoot and at ionospheric altitudes below 450 km including its variation with solar activity. The morning T(e) has a maximum at the dip equator and decreases gradually with increasing latitude, which is due to the increasing importance of heat conduction as the dip angle becomes larger. The amplitude of the equatorial morning overshoot T(e) decreases with increasing solar flux by about -10 degrees K/solar flux unit depending on season and longitude. Trends of similar magnitude are predicted by the FLIP model. The model calculations confirm that the electron cooling due to enhanced electron-ion collisions increases faster than the heating of thermal electrons through collision with photoelectrons for increasing solar EUV. Both data and model showed that elevated electron temperatures persist to later local times during low solar activity.
  • Using 8 years of CHAMP satellite observations of the equatorial electron temperature, T(e), we investigate its behavior during the morning overshoot and at ionospheric altitudes below 450 km including its variation with solar activity. The morning T(e) has a maximum at the dip equator and decreases gradually with increasing latitude, which is due to the increasing importance of heat conduction as the dip angle becomes larger. The amplitude of the equatorial morning overshoot T(e) decreases with increasing solar flux by about -10 degrees K/solar flux unit depending on season and longitude. Trends of similar magnitude are predicted by the FLIP model. The model calculations confirm that the electron cooling due to enhanced electron-ion collisions increases faster than the heating of thermal electrons through collision with photoelectrons for increasing solar EUV. Both data and model showed that elevated electron temperatures persist to later local times during low solar activity. (en)
Title
  • Solar flux variation of the electron temperature morning overshoot in the equatorial F region
  • Solar flux variation of the electron temperature morning overshoot in the equatorial F region (en)
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  • Solar flux variation of the electron temperature morning overshoot in the equatorial F region
  • Solar flux variation of the electron temperature morning overshoot in the equatorial F region (en)
skos:notation
  • RIV/68378289:_____/11:00366447!RIV12-AV0-68378289
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(GAP209/10/2086), Z(AV0Z30420517)
http://linked.open...iv/cisloPeriodika
  • -
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  • 230476
http://linked.open...ai/riv/idVysledku
  • RIV/68378289:_____/11:00366447
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • IONOSPHERIC PHOTOELECTRON FLUX; MODEL; DENSITY; ATMOSPHERE; ION (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [A892146D7C54]
http://linked.open...i/riv/nazevZdroje
  • Journal of Geophysical Research
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http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 116
http://linked.open...iv/tvurceVysledku
  • Liu, H.
  • Truhlík, Vladimír
  • Lühr, H.
  • Richards, G.
  • Stolle, C.
http://linked.open...ain/vavai/riv/wos
  • 000289644900005
http://linked.open...n/vavai/riv/zamer
issn
  • 0148-0227
number of pages
http://bibframe.org/vocab/doi
  • 10.1029/2010JA016235
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