Исследование стационарной магнитосферной конвекции / В. А. Сергеев [и др.] ; Акад. наук СССР, Кол. фил. им. С. М. Кирова, Поляр. геофиз. ин-т. – Препр. ПГИ 86-05-47. - Апатиты : Кольский филиал АН СССР, 1986.

Figure captions Fig.1. Main features of the magnetic activity during February 19-20, 1978. From top to bottom: magnetosheath magnetic field at X ~ - 26 Rg according to IMP-8 measurements (in GSE coordinate system); AU-AL and AE indices; time in tervals contained the substorm related signatures, in cluding AEJW expansions to high latitudes (HLB), mid- latitude magnetic bays (MLB) and Pi2 activity. Fig.2. The same as in Fig.1, but for Nov.24, 1981; GSM compo nents of IMF measured by ISEE-3 are given here without time correction due to the propagation of IMF to the near-Earth region. Fig.3. XT projection of ISEE-1 and GEOS-1 trajectories during time intervals, contained SMC episodes. Fig.4. Time variations of 15 min averaged parameters measured by ISEE-1 in the plasma sheet during Feb.19-20, 1978. From top to bottom: GSE components of proton bulk flow; proton thermal pressure (Px = 2/3n-E) and local magnetic field pressure (Pg); number density of thermal protons (n); average thermal energy of protons (E) - according to the Lockheed experiment. At the top: the periods of substorm expansions (from Fig.1) are given, whereas the bottom panel shows both Z coordinate of the space craft and its distance against the position of the planar neutral sheet, having 7 Rg hinging distance (DZH). Fig.5. Time variations of differential fluxes of energetic electrons and protone (from MEPI experiment) together with the GSM magnetic field at ISEE-1 location during Feb.19, 1978. Fig.6. Equivalent currents at 108°CGLong meridian (top block) and isointensity contour lines of the energy flux of precipitated auroral electrons (in ergs/cm‘'sec estimated from the auroral emission 3914 £ distribution along the 115°CGLong meridian) for the SMC episode on Feb.19, 1978. 23