For the purpose of clarifying the occurrence character of the ionization ledge and its relation to the diurnal variation of the eastward electric field, plasma density profiles in the equatorial ionosphere of the American longitude sector obtained from topside sounder on-board the Ohzora (EXOS-C) and the ISIS-2 satellites were analyzed. The ionization ledge appeared in a limited dip latitude region from - 13.5 degrees to 19.3 degrees, near the dip equator. The structure of the ionization ledge tends to align along the geomagnetic field line, and to appear within local time sectors from morning (09LT) to slightly after midnight (02LT). Comparing with the eastward electric field deduced by analyzing the variations of the geomagnetic field on the ground, the ionization ledge tends to occur with the enhancement of the eastward electric field. The occurrence probability shows a seasonal variation giving maxima in equinox seasons and minima in solstice seasons. Comparing with the seasonal dependence of the upward drift velocity based on the variation of the electric field, the seasonal variation of the occurrence probability is well interpreted as the character of the ionospheric electric field. (c) 2006 Elsevier Ltd. All rights reserved.
机构:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
University of Chinese Academy of SciencesKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Jiang-Tao Su
Jie Chen
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Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
State Key Laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of SciencesKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Jie Chen
Yuan-Yong Deng
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Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of SciencesKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Yuan-Yong Deng
Debi Prasad Choudhury
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California State UniversityKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
机构:
Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Univ Chinese Acad Sci, Beijing 100049, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Priya, Thambaje Gopalan
Su, Jiang-Tao
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Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Univ Chinese Acad Sci, Beijing 100049, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Su, Jiang-Tao
Chen, Jie
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Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, Beijing 100190, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Chen, Jie
Deng, Yuan-Yong
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Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R ChinaChinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China
Deng, Yuan-Yong
Choudhury, Debi Prasad
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Calif State Univ Northridge, Northridge, CA 91330 USAChinese Acad Sci, Natl Astron Observ, Key Lab Solar Act, Beijing 100012, Peoples R China