Physics of auroral phenomena : proceedings of the 35th Annual seminar, Apatity, 28 Februaru – 02 March, 2012 / [ed. board: A. G. Yahnin, A. A. Mochalov]. - Апатиты : Издательство Кольского научного центра РАН, 2012. - 187 с. : ил., табл.

Various magnetospheric inputs to the GSM TIP model Model results and comparison with observation Feshchenko and Maltsev (2003) Boyle et al. (1997) Vorobjov and Yagodkina (2005, 2007) Zhang and Paxton (2008) Vorobjov and Yagodkina (2005, 2007) Zhang and Paxton (2008) Irkutsk (cp 52.2°N, X = 104.ГЕ) 7 -3 ' 1 11rГР1111 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 8 12 18 0 8 12 18 24 02.05 03.05 UT (h) 0 8 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 11 10 N 9 X 8 2 7 6 * 5 4 3 2 Palmas (<p= 10.2°S, I = 48.2°W) UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 = 23.2°S, A, = 45.9°W) UT (h) 0 6 12 18 0 8 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 Kaliningrad (cp 54.6°N, A. = 20.2°E) в -3 UT (h) o 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 8 12 18 24 02.05 03.05 Norilsk (ф - 69.2°N, UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 ■1111111p m UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05_____________________ 02.05 03.05 UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 UT (h) 0 8 16 0 6 12 18 24 02.05 03.05 UT (h) 0 8 12 18 0 6 12 18 24 02.05 03.05 Sao Jose dos Campos (cp UT (h) 0 6 12 18 0 6 12 18 24 02.05 03.05 Fig. 2. foF2 behavior during 2-3 May, 2010 geomagnetic storm above Irkutsk (Russia), Kaliningrad (Russia), Norilsk (Russia), Palmas (Brazil) and Sao Jose dos Campos (Brazil). The observational data are shown by light circles - quiet day 1 May, 2010 and dark circles - disturbed days. The simulated data obtained with different model input parameters are shown by dotted lines - quiet day 1May, 2010 and solid lines - disturbed days. 113