Dynamics of field-aligned currents in two hemispheres during a magnetospheric storm from magnetogram inversion technique data
Journal Title: Solar-Terrestrial Physics - Year 2021, Vol 7, Issue 1
Abstract
We continue to study the physical processes occurring during the August 17, 2001 magnetospheric storm by analyzing the dynamics of the intensity of field-aligned currents (FACs) in Iijima—Potemra Region 1 in the polar ionospheres of the two hemispheres, using the modernized magnetogram inversion technique. The results obtained on the dynamics of two types of FAC asymmetry (dawn-dusk and interhemispheric), as well as the previously obtained regularities in the behavior of Hall currents and the polar cap boundaries depending on the large azimuthal component of the interplanetary magnetic field (IMF), observed during the storm, and the seasonal behavior of the conductivity are consistent with the open magnetosphere model and with satellite observations of auroras in two hemispheres. We have shown that the weakening of the asymmetry of two types in the FAC distribution during substorms in the storm under study occurs almost completely in the winter hemisphere and is much weaker in the summer one. We associate this phenomenon with the predominance of the effect of long-term exposure to the azimuthal IMF component in the sunlit polar ionosphere of the summer hemisphere over the substorm symmetrization effect of the night magnetosphere. A symmetrization effect of the polar cap and FACs, created by the solar wind pressure pulse at the end of the storm, is observed. We propose a qualitative explanation of this effect.
Authors and Affiliations
Mishin V. V. , Karavaev Yu. A. , Silina A. S. , Penskikh Yu. V. , Kapustin V. E.
ACCELERATION OF PARTICLES IN A CONSTANT MAGNETIC FIELD AND AN ELECTRIC FIELD PERPENDICULAR TO IT, INCREASING WITH TIME
The paper addresses the problem of acceleration of particles in a constant, uniform magnetic field of magnitude B and a uniform electric field perpendicular to it, which slowly increases with time. Assuming that the elec...
ON THE GROUP VELOCITY OF WHISTLING ATMOSPHERICS
The dynamic spectrum of a whistling atmospheric is a signal of falling tone, and the group delay time of the signal as a function of frequency is formed as a result of propagation of a broadband pulse in a medium (magnet...
IONOSPHERIC RESPONSE TO THE PASSAGE OF TYPHOONS OBSERVED BY SUBIONOSPHERIC VLF RADIO SIGNALS
The response of the lower ionosphere to the passage of several dozen typhoons has been studied using a regional network of VLF stations in the Russian Far East. The experimental data presented in all cases clearly demons...
STATISTICAL RELATION OF TRAVELING IONOSPHERIC DISTURBANCES WITH NEUTRAL WIND AND DISTURBANCES IN THE STRATOSPHERE
Using the representative statistics on traveling ionospheric disturbances (TIDs) obtained by Yekaterinburg and Magadan radars, we have shown that distributions of TIDs and average TID velocities by azimuths and local tim...
CONNECTION OF TOTAL ELECTRON CONTENT DISTURBANCES WITH AE INDEX OF GEOMAGNETIC ACTIVITY DURING GEOMAGNETIC STORM IN MARCH 2015
Ionospheric response to the March 17, 2015 geomagnetic storm has been investigated using simulations of the Global Self-consistent Model of the Thermosphere, Ionosphere, Protonosphere (GSM TIP) [Dmitriev et al., 2017; Kl...