Solar-Terrestrial Physics | |
Modeling the influence of magnetospheric heat fluxes on the electron temperature in the subauroral ionosphere | |
Gololobov Artem1  | |
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 | |
学科分类:天文学(综合) | |
来源: INFRA-M | |
【 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】
CC BY-NC-ND
【 预 览 】
Files | Size | Format | View |
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RO201904026069640ZK.pdf | 694KB | download |