Daytime geomagnetic disturbances at high latitudes during a strong magnetic storm of June 21–23, 2015: The storm initial phase

• Published in: Geomagnetism and Aeronomy Vol. 56; no. 3; pp. 281 - 292
• Main Authors: Gromova, L. I., Kleimenova, N. G., Levitin, A. E., Gromov, S. V., Dremukhina, L. A., Zelinskii, N. R.
• Format: Journal Article
• Language: English
• Published: Moscow Pleiades Publishing 01.05.2016; Springer Nature B.V
• Subjects: Atmospheric sciences; Boundaries; Daytime; Dynamics; Earth; Earth and Environmental Science; Earth Sciences; Geomagnetism; Geophysics; Geophysics/Geodesy; Latitude; Magnetic fields; Magnetic storms; Polar substorms; Solar activity; Storms; Wind speed
• ISSN: 0016-7932; 1555-645X; 0016-7940
• DOI: 10.1134/S0016793216030051

The high-latitude geomagnetic effects of an unusually long initial phase of the largest magnetic storm ( SymH ~–220 nT) in cycle 24 of the solar activity are considered. Three interplanetary shocks characterized by considerable solar wind density jumps (up to 50–60 cm –3 ) at a low solar wind velocity (350–400 km/s) approached the Earth’s magnetosphere during the storm initial phase. The first two dynamic impacts did not result in the development of a magnetic storm, since the IMF Bz remained positive for a long time after these shocks, but they caused daytime polar substorms (magnetic bays) near the boundary between the closed and open magnetosphere. The magnetic field vector diagrams at high latitudes and the behaviour of high-latitude long-period geomagnetic pulsations ( ipcl and vlp ) made it possible to specify the dynamics of this boundary position. The spatiotemporal features of daytime polar substorms (the dayside polar electrojet, PE ) caused by sudden changes in the solar wind dynamic pressure are discussed in detail, and the singularities of ionospheric convection in the polar cap are considered. It has been shown that the main phase of this two-stage storm started rapidly developing only when the third most intense shock approached the Earth against a background of large negative IMF Bz values (to–39 nT). It was concluded that the dynamics of convective vortices and the related restructing of the field-aligned currents can result in spatiotemporal fluctuations in the closing ionospheric currents that are registered on the Earth’s surface as bay-like magnetic disturbances.