Solar dependence of equatorial F-region irregularities observed by COSMIC radio occultations
Solar dependence of equatorial F-region irregularities observed by COSMIC radio occultations
复制标题
COSMIC 射电掩星观测到的赤道 F 区不规则性的太阳依赖性
DOI:
10.1029/2018ja025936
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发表时间:
2018
期刊:
影响因子:
--
通讯作者:
Tian Mao
中科院分区:
文献类型:
--
作者:
Tao Yu;Yasunobu Miyoshi;Chunliang Xia;Xiaomin Zuo;Xiangxiang Yan;Na Yang;Yangyi Sun;Xinan Yue;Tian Mao
With an improved method for retrieving the equatorialFregion irregularities (EFIs) from radio occultation measurements, a huge amount of S4 index profiles from Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites is employed to study the solar cycle variation of global EFIs during the period of 2007 to 2017. This full solar cycle data show that impacts of the solar activity on the occurrence rates and heights of EFIs are notable and complex. The occurrence rates of EFIs at higher altitude (greater than 500 km) increase with increasing the solar activity. The mean heights ( ) and heights standard deviation (σh) of EFIs at higher altitudes do not show clearly the solar activity dependence. On the other hand, the occurrence rates of EFIs at entire altitudes (from 150 to 800 km) do not have clear relation with the solar activity. The and σhof EFIs at entire altitudes increase with increasing the solar activity. Moreover, the dependence of the occurrence rates of EFIs on the solar activity are the strongest in the equinoxes, weaker in winter and weakest in summer. The electric fields and corresponding seasonal variation can account for the EFIs occurrence and height variation versus solar activities, and the EFIs at low altitudes seem to be related to theseedassociated with atmospheric gravity wave.