The seasonal and solar cycle variations of electron density gradient scale length during magnetically disturbed days: implications for Spread F

被引:3
|
作者
Manju, G. [1 ]
Devasia, C. V. [1 ]
Ravindran, Sudha [1 ]
机构
[1] Vikram Sarabhai Space Ctr, Space Phys Lab, Trivandrum 695022, Kerala, India
来源
EARTH PLANETS AND SPACE | 2009年 / 61卷 / 07期
关键词
Equatorial ionosphere; ionospheric irregularities; plasma instability; Equatorial Spread F; EQUATORIAL IONOSPHERE; PEDERSEN CONDUCTIVITY; RADAR OBSERVATIONS; WINDS; FIELD; DRIFT; IRREGULARITIES; SCINTILLATIONS; THERMOSPHERE; EVOLUTION;
D O I
10.1186/BF03353202
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The behaviour of electron density gradient scale length, L, around post-sunset hours during the magnetically disturbed days of the summer, winter and equinox seasons of solar maximum (2002) and minimum years (1995) has been studied, using ionosonde data of Trivandrum (8.5 degrees N, 76.5 degrees E, dip = 0.5 degrees N) in the Indian longitude sector. The results indicate a clear seasonal and solar cycle variation in L. Seasonal variations of the maximum vertical drift of the F layer were also examined on these days. In particular, the seasonal variation of the Equatorial Spread F (ESF) during this period is examined in terms of the relative roles of L and the vertical drift of the F layer in the triggering of the collisional Rayleigh-Taylor instability. Our results on the clear-cut seasonal and solar cycle variation in L for disturbed days and its control of ESF occurrence are presented and discussed.
引用
收藏
页码:913 / 917
页数:5
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