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.

Wavelet component manifestation o fSolar Windparameter disturbances Fig. 2. Example of registering skeletons marked with arrows before the storm. The abscissa is time in minutes, vertical axis - the value of large-scale wavelet coefficients corresponding to the frequency range of 2-8 mHz. A fragment of the data corresponds to the undisturbed interval before the storm 02.09.2002 1100 -1400 UT, Dst = -10 nT. 12 l O О In f Й*>1 Inf t-'OJ £3i). In f [эзЬ _____.... 1 40 U P $ Inf [3 3 1 Fig. 3. Example of registering skeletons marked with arrows in the initial phase of the storm. The abscissa is time in minutes, vertical axis - the value of large-scale wavelet coefficients corresponding to the frequency range of 2-8 mHz. A fragment of the data corresponds to the initial phase of the storm 15.07.2000 1400 -1300 UT, Dst = 10 nT 1 4 12 Ю I» f* 4 1 4 12 Ю Ь G 4 Fig. 4. Example of registering skeletons marked with arrows on the main phase of the storm. The abscissa is time in minutes, vertical axis - the value of large-scale wavelet coefficients corresponding to the frequency range of 2-8 mHz. A fragment of the data corresponds to the main phase of the storm 24.11.2001 1500 -1800 UT, Dst = -240 nT. 39