Эксперимент «Авроральный брейкап» (результаты МИМ) : [сборник статей] / Акад. наук СССР, Кол. фил. им С. М. Кирова, Поляр. геофиз. ин-т ; [редкол.: О. М. Распопов (отв. ред.) и др.]. - Апатиты : Кольский филиал АН СССР, 1979. - 127 с. : ил.

YDK 550.388.8 Spectra of aurora at February - March 1978 during Auroral Breakup Campaign - 1. Totunovu G.J?., Fedorova N.I. - Experi­ ment "Auroral breakup" (resulta of IMS). Ed. Kola Branch Acad. Sci. USSR, Apatity, 1979, p.70-78. It is described the time variations of the main auroral spe­ ctral components by C-180-S spectrograph data. The observation carried out also during the cloud weather. By the different emis­ sion radio there obtained the values of the energy of precipita­ tions. It is shown the magnetic activity increase usually accom­ panies by the increase of the auroral electron energy. At March 8-9 there observed the red aurora accompanied the middle magnetic disturbance. Fig. - 4, ref. - 4. YDK. 550*388.8 The distribution of the auroral luminosity of the scaning photometer data. Vlaskov V.A., Bogolyubov A.A. - Experiment "Auroral breakup" (results of IMS}. Ed. Kola Branch Acad. Sci. USSR, Apatity, 1979, p.78-82. During Auroral breakup campaign the intensity of auroral lu­ minosity was measured by the two scaning photometers with field of view 1.4^. The altitude of auroral forms was measured at March 16, 1978, during the eubstonn. The electron concentration in the maximum of luminosity was valued. Pig. - 4, ref. - 2. YDK 550.388.2 The measurements of the ionospheric small-scale irregulari­ ties in the auroral zone. Bogolubov A.A., Kosolapenko V.I.-, Kryarhev V.A., Mizun Yu.G., Ogloblina O.F.,Cheremnyiy V.A. Experiment "Auroral breakup" (results of IMS). Ed. Kola Branch Acad. Sci. USSR, Apatity, 1979, p.82-93* During Auroral breakup campaign the method of the space re­ ception used for the study of the VHP satellite scintillations. The authors suggested the satellite scintillations as well as so­ me phenomenon are space homogenous and stationary. It was found the power spectra of fading may describe by power from -2.7 to -4.7. During the disturbances the middle altitude of the irregu­ larity layer decreases from 300-400 km in morning and noon to 150-300 km in evening. During substorm the region of the irregu­ larities is widened in the west-east directions and their anyzo- tropy is increased. Pig. - 10, ref. - 6. I26

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