Morning Overshoot of Te Enhanced by Downward Plasma Drift in the Equatorial Topside Ionosphere.
-
- Oyama K.-I.
- Institute of Space & Astronautical Science
-
- Balan N.
- Institute of Space & Astronautical Science
-
- Watanabe S.
- Department of Astronomy and Geophysics, Tohoku University
-
- Takahashi T.
- Department of Astronomy and Geophysics, Tohoku University
-
- Isoda F.
- Faculty of Education, Yokohama National University
-
- Bailey G. J.
- Applied Mathematics Section, School of Mathematics, University of Shefeld
-
- Oya H.
- Department of Astronomy and Geophysics, Tohoku University
Bibliographic Information
- Other Title
-
- Morning Overshoot of Te Enhanced by Dow
Search this article
Abstract
The morning overshoot in electron temperature, Te, which occurs in the sunlit atmosphere of low electron density during early morning hours, is a well known phenomenon. Studies of the phenomenon carried out using the Hinotori satellite observations reveal that the overshoot enhances in the topside equatorial F-region for a short period of time in the morning. The enhancement in the overshoot is found to depend on season and solar activity; it is strong during the northern summer months and grows with the increase in solar activity. Theoretical model calculations show that the enhancement in Te is caused by a reduction in electron density in the topside ionosphere due to a downward drift of plasma.
Journal
-
- Journal of geomagnetism and geoelectricity
-
Journal of geomagnetism and geoelectricity 48 (7), 959-966, 1996
Society of Geomagnetism and Earth, Planetary and Space Sciences
- Tweet
Details 詳細情報について
-
- CRID
- 1390282681487818880
-
- NII Article ID
- 130003423135
- 10002201944
-
- NII Book ID
- AA00698879
-
- ISSN
- 21855765
- 00221392
-
- NDL BIB ID
- 4060386
-
- Text Lang
- en
-
- Data Source
-
- JaLC
- NDL
- Crossref
- CiNii Articles
-
- Abstract License Flag
- Disallowed