首页 | 本学科首页   官方微博 | 高级检索  
     检索      

太阳活动低年南极中山站电离层F层的平均特性
引用本文:贺龙松,刘瑞源,刘顺林,刘勇华.太阳活动低年南极中山站电离层F层的平均特性[J].地球物理学报,2000,43(3):289-295.
作者姓名:贺龙松  刘瑞源  刘顺林  刘勇华
作者单位:中国极地研究所,上海200129
基金项目:国家自然科学基金!49634160,国家海洋局青年海洋基金!98605
摘    要:根据1995-1997年3年中山站数字式电离层测高仪的数据,分析了中山站不同季 节F层的临频变化特点.中山站夏季主要受太阳光光化电离的影响,F层临频随地方时的变 化与中纬台站相似;两分季,极隙区软电子沉降的作用显著,F层临频随磁地方时而变化,有 较明显的磁中午现象.冬季,太阳全天处于地平线以下,中山站F层临频的变化主要受极隙 区软电子沉降和极区等离子体漂移的影响,其峰值变化处于碰中午和地方时中午之间.中山 站夏季全天都能观测到F层的存在;两分季F层在地方时子夜附近的出现率较少;冬季月份 在磁地方时午后和子夜F层出现率明显减少,这可能与南半球冬季的高纬槽和极洞有关.对 F层不均匀区的分析认为,中山站在t_(LT)为16:00左右处于极光带赤道侧,20:00左右进入极盖 区。

关 键 词:F层临频磁  中午现象  F层不均匀区极光带  中山站  
文章编号:0001-5733(2000)03-0289-07
收稿时间:1999-04-20

OVERALL PROPERTIES OF F REGION AROUND SOLAR MINIMUM AT ZHONGSHAN STATION,ANTARCTICA
HE LONG-SONG,LIU RUI-YUAN,LIU SHUN-LIU,YONG-HUA.OVERALL PROPERTIES OF F REGION AROUND SOLAR MINIMUM AT ZHONGSHAN STATION,ANTARCTICA[J].Chinese Journal of Geophysics,2000,43(3):289-295.
Authors:HE LONG-SONG  LIU RUI-YUAN  LIU SHUN-LIU  YONG-HUA
Institution:Polar Research Institute of China, Shanghai 200129, China
Abstract:Based on the monthly data of DPS--4 in 1995-- 1997, we analyze the seasonal properties of F region at Zhongshan Station. In summer, F region ionization is dominated by the solar ultraviolet radiation. Similar to the phenomenon of midlatitude, the f_0 F_2 varies with local time; In equinox seasons, soft electron precipitation from the cusp / cleft region seems apparent. f_0 F_2 chages with MLT, and shows the magnetic noon phenomenon. In winter, solar radiation is less effective to F region ionization. Instead, F region is affected by particle precipitation from cusp / cleft region as well as ionospheric plasma convection, and so the diurnal variation of critical frequency lies between LT and MLT; F region in summer and equinox are more stable. However, in winter the occurrences of F region near afternoon cusp and midnight are much less. We think this phenomenon is caused by the high-latitude ionospheric trough and polar hole; After further analysis of F region spread, we find that the duration of aurora oval passing over the Zhongshan Station t_(TL) is from 16:00 to 20:00h.
Keywords:f_0 F_2  Magnetic noon phenomenon  FLIZ  Aurora oval  Zhongshan Station  
本文献已被 CNKI 维普 万方数据 等数据库收录!
点击此处可从《地球物理学报》浏览原始摘要信息
点击此处可从《地球物理学报》下载免费的PDF全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号