Magnetic local time and latitude dependence of amplitude of the main impulse (MI) of geomagnetic sudden commencements and its seasonal variation
Atsuki Shinbori1, Yuji Tsuji2, Takashi Kikuchi2, Tohru Araki3, Akihiro Ikeda4, Teiji Uozumi4, Dmitry Baishev5, Boris M. Shevtsovv6, Tsutomu Nagatsuma7, Kiyohumi Yumoto4
- Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japan
- Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan
- SOA Key Laboratory for Polar Science, Polar Research Institute of China, Shanghai, China
- International Center for Space Weather Science and Education, Kyushu University, Fukuoka, Japan
- IKFIA, Yakutsk, Russia
- Institute of Cosmophysical Researches and Radio Wave Propagation, FEB RAS, Paratunka, Russia
- National Institute of Information and Communications Technology, Tokyo, Japan
The magnetic local time and latitude dependence of amplitude of the main impulse (MI) of geomagnetic sudden commencements (SCs) and its seasonal variation have been investigated using high time resolution (1–3 sec) geomagnetic data in the latitudinal range 27–70 degrees for the period 1996–2010. The daytime distribution of the SC-MI amplitude in the sub-auroral and middle latitudes (35–60 degrees) is similar to the DP-2 type geomagnetic variation which shows negative and positive changes in the morning and afternoon, respectively. The magnetic field variation is reversed around the magnetic latitude of 63–65 degrees. This suggests that a pair of field-aligned currents (FACs), resembling the region-1 (R-1) FACs, is located near the magnetic latitude of 63–65 degrees. The nighttime SC amplitude is enhanced significantly in the low and middle latitudes (27–60 degrees). The enhancement is due to the magnetic effect produced by the SC-MI FACs. In the nighttime auroral latitude (63–65 degrees), the SC amplitude decreases steeply due to the enhanced westward auroral electrojet associated with the compression of the magnetosphere. The size of the diurnal variation tends to increase significantly during the summer, compared with that during the winter. This seasonal variation suggests that the DP-2 type ionospheric currents (ICs) and FACs generated during the SC-MI phase are intensified by increased ionospheric conductivities during the summer. It can be concluded that the large-scale MI current system in the ionosphere and magnetosphere is voltage generator.
Shinbori A., Tsuji Y., Kikuchi T., Araki T., Ikeda A., Uozumi T., Baishev D., Shevtsov B.M., Nagatsuma T., Yumoto K. Magnetic local time and latitude dependence of amplitude of the main impulse (MI) of geomagnetic sudden commencements and its seasonal variation // J. Geophys. Res. V.117. A08322 DOI:10.1029/2012JA018006 Published: AUG 21 2012.
