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EISCAT Observations of Main Ionization Troughs in the High-Latitude Ionosphere 被引量:1
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作者 LIU Peng 1 ,MA Shu ying 1,2 ,K. Schlegel 3 1. College of Electronic Information, Wuhan University, Wuhan 430072, China 2. Ionospheric Observatory, Wuhan Institute of Physics,the Chinese Academy of Sciences, Wuhan 430071, China 3. Max P 《Wuhan University Journal of Natural Sciences》 EI CAS 2000年第2期187-193,共7页
F-region electron density depletions associated with main ionization troughs in the high-latitude ionosphere are studied using EISCAT CP3 data of meridian scanning experiments. The troughs in our observations are foun... F-region electron density depletions associated with main ionization troughs in the high-latitude ionosphere are studied using EISCAT CP3 data of meridian scanning experiments. The troughs in our observations are found to appear mainly in dusk sector, extending from late afternoon to pre-midnight, with higher occurrence rate during equinox and winter. Simultaneous ion drift velocity inF-region shows that the main trough minimum is mostly located at the equator ward edge of the plasma convection flow, rather than in the region where the largest ion flow are observed. 展开更多
关键词 high latitude ionosphere main ionization trough plasma convection flow incoherent scatter radar observation
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Mean ionospheric properties in winter at Zhongshan Station,Antarctica
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作者 刘顺林 贺龙松 刘瑞源 《Chinese Journal of Polar Science》 1997年第2期57-62,共6页
Ionograms taken from a Digisonde Portable Sounder (DPS 4) at Zhongshan Station of Antarctica in 1995 are used to analyse the mean ionospheric properties in winter. The F region is rather unstable in winter and has la... Ionograms taken from a Digisonde Portable Sounder (DPS 4) at Zhongshan Station of Antarctica in 1995 are used to analyse the mean ionospheric properties in winter. The F region is rather unstable in winter and has large diurnal variation. The monthly medium value of f oF 2 has a main peak around 0900UT when maximum value occurs and a sub peak between 1300 1500UT. It may be affected synthetically by the low energy electron precipitation in cusp region, the high latitude plasma convection and the solar radiation, resulted in so called F region magnetic noon phenomena. Low values of f oF 2 occur in post midnight (2000 0100UT) when Zhongshan Station crosses the ionospheric polar hole. Sporadic E layer which caused mostly by auroral particle precipitation can be observed almost every day with the highest value of f oE s around 1700UT. The diurnal variation of E layer is relatively smooth. 展开更多
关键词 high latitude ionosphere magnetic noon phenomena plasma convection polar hole Zhongshan Station.
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