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磁暴期内夜间h’F的突增现象
引用本文:沈长寿,资民筠.磁暴期内夜间h’F的突增现象[J].地球物理学报,1998,41(2):156-161.
作者姓名:沈长寿  资民筠
作者单位:1. 北京大学地球物理系,北京 100871; 2. 中国艺术研究院,北京 100009; 3. 电子工业部电波传播研究所,河南新乡 453003; 4. 国家地震局地球物理研究所,北京 100081
基金项目:国家自然科学基金,49674245
摘    要:用3个经度链上电离层垂测站资料分析磁暴时夜间h'F的同时突增现象提出了电动耦合在夜间出现东向电场从而使F层抬升的物理机制同时也解释了突增现象在午夜后更多,且增幅更强的事实.

关 键 词:磁暴  电离层F层扰动  h'F变化  
收稿时间:1997-04-30

ON THE NIGHTTIME SUDDEN ENHANCEMENT OF h' F DURING MAGNETIC STORMS
SHEN CHANG-SHOU,ZI MIN-JUN,WU--JIAN,SUO YU-CHENG,GAO YU-FEN.ON THE NIGHTTIME SUDDEN ENHANCEMENT OF h' F DURING MAGNETIC STORMS[J].Chinese Journal of Geophysics,1998,41(2):156-161.
Authors:SHEN CHANG-SHOU  ZI MIN-JUN  WU--JIAN  SUO YU-CHENG  GAO YU-FEN
Institution:1. Geophysical Department, Peking University, Beijing 100871, China; 2. The Academy of Arts of China, Beijing 100009,China; 3. China Rsearch Institute of Radiowave Propagation, Xinxiang 453003,China; 4. Institute of Geophysics,State Seismological Bureau,Beijing 100081,China
Abstract:The simultaneously sudden enhancements of h' F at nighttime during magneticstorms are analyzed by using ionosonde data from stations distributed nearby 3meridian chains. The related physical mechanism is proposed. Generally, the effects ofthe magnetospheric convection and the driving potential across the polar cap (or theregion 1 field-aligned current) during a magnetic storm will lead to a westwardelectric field, but not an eastward one. On the other hand, the shielding effect of theregion 2 field-aligned current may confine the disturbed field within the auroral oveland weaken its influence in lower latitude area. Since the region 1 field--alignedcurrent is usually stronger than the region 2 current the westward electric field cannot be reversed eastward. The turning of the interplanetary magnetic field (IMF) fromsouthward to northward is equivalent to shutting off the driving potential across thepolar cap. If the region 2 field--aligned current strengthens during an IMF turning, theappearance of an eastward field at nighttime is possible, and the drift E×B effectwill lift the F--region obviously. With this mechanism, it is also easy to be understoodwhy the enhancement occurs more frequently and is more intensive in themidnight--dawn sector.
Keywords:Magnetic storm  Disturbance of the ionospheric F-regions  Variation of h' F
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