Solar flux variation of the electron temperature morning overshoot in the equatorial F region
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378289%3A_____%2F11%3A00366447" target="_blank" >RIV/68378289:_____/11:00366447 - isvavai.cz</a>
Result on the web
<a href="http://www.agu.org/pubs/crossref/2011/2010JA016235.shtml" target="_blank" >http://www.agu.org/pubs/crossref/2011/2010JA016235.shtml</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1029/2010JA016235" target="_blank" >10.1029/2010JA016235</a>
Alternative languages
Result language
angličtina
Original language name
Solar flux variation of the electron temperature morning overshoot in the equatorial F region
Original language description
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.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
DG - Atmospheric sciences, meteorology
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GAP209%2F10%2F2086" target="_blank" >GAP209/10/2086: Modeling of variability of the thermal plasma parameters in the Earth's upper ionosphere and inner magnetosphere</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
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
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Country of publishing house
US - UNITED STATES
Number of pages
13
Pages from-to
"A04308/1"-"A04308/13"
UT code for WoS article
000289644900005
EID of the result in the Scopus database
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