Modeling the influence of magnetospheric heat fluxes on the electron temperature in the subauroral ionosphere

Solar-Terrestrial Physics

卷:3

Gololobov A.Yu.¹  Varlamov I.I.¹  Golikov I.A.² 

[1] M.K. Ammosov North-Eastern Federal University, Yakutsk, Russia;

[2] Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy, Yakutsk, Russia;

关键词: subauroral ionosphere;    electron temperature;    heat flux;    three-dimensional model;    ring current;    F2 region;    elevated electron temperature regions;    longitudinal features;   

DOI  :  10.12737/stp-3220178

来源: DOAJ

【 摘 要 】

We present results of modeling of the electron temperature distribution in the F region of the subauroral ionosphere for different helio-geomagnetic conditions with consideration for magnetospheric heat fluxes. It is shown that under quiet geomagnetic condi-tions during a winter period in the dawn and dusk sec-tors “hot” zones with a higher electron temperature are formed, and under disturbed geomagnetic conditions an annular “hot” region is formed in a time interval 04–06 UT as a result of heat inflow from Earth’s magnetosphere along magnetic field lines. The analysis of the DE-2 satellite data demonstrates that such zones can be formed during geomagnetic disturbances.

【 授权许可】

Unknown