Physics of auroral phenomena : proceedings of the 36th Annual seminar, Apatity, 26 February – 01 March, 2013 / [ed. board: A. G. Yahnin, A. A. Mochalov]. - Апатиты : Издательство Кольского научного центра РАН, 2013. - 215 с. : ил., табл.

В. Мишин и др. 1. Как влияет на мощность и энергию суббури переход от режима MR1/E01 к режиму MR2/E02? 2. Когда и где (в какой области хвоста) отмечены признаки Е01?. 3. Как связаны наблюдаемые expansion onsets с явлением КЗ в возмущённой М-И системе? 4. Каковы последовательности во времени и пространстве двух главных expansion onsets? 5. Где начинается и продолжается процесс MR2/E02 ? Мы продолжаем аналогичное исследование по данным возмущений различного типа. Авторы благодарят Сапронову JI. А. за расчеты и подготовку рисунков. Работа выполнена при частичной поддержке РФФИ (гранты №12-05-91159-ГФЕН и №13-05-92219-М(ЖГ). Список литературы Baker, D. N., et al. (2002), Timing of magnetic reconnection initiation during a global magnetospheric substorm onset, Geophys. Res. Lett., 29(24), 2190. Bim, J., and M. Hesse (2013), The substorm current wedge in MHD simulations, J. Geophys. Res., 118(6), 3364-3376. Blake, J. B., R. Mueller-Mellin, J. A. Davies, X. Li, and D. N. 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