{"id":11334,"date":"2026-03-29T13:05:24","date_gmt":"2026-03-29T05:05:24","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=11334"},"modified":"2026-04-05T22:01:19","modified_gmt":"2026-04-05T14:01:19","slug":"solnechno-zemnaya-fizika-tom-12-%e2%84%961-2026","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-12-%e2%84%961-2026\/","title":{"rendered":"\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u0430\u044f \u0444\u0438\u0437\u0438\u043a\u0430. \u0422\u043e\u043c 12, \u21161, 2026"},"content":{"rendered":"
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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/td>
\u0421\u0442\u0440.<\/strong>
<\/td>		<\/td>Pp.<\/strong><\/td><\/td><\/tr>
\u041c\u0430\u0448\u043d\u0438\u0447 \u0413.\u041f., \u0422\u043e\u043c\u0438\u043d \u0412.\u0415., \u041f\u0443\u043b\u044f\u0435\u0432<\/em><\/strong> \u0412.\u0410<\/strong><\/em>.<\/strong> \u0421\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0434\u0432\u0438\u0436\u0435\u043d\u0438\u0439 \u0432 \u0432\u043e\u043b\u043e\u043a\u043d\u0435 \u0438 \u0435\u0433\u043e \u043e\u043a\u0440\u0435\u0441\u0442\u043d\u043e\u0441\u0442\u044f\u0445: \u043f\u043e\u043f\u0435\u0440\u0435\u0447\u043d\u044b\u0435 \u043a\u043e\u043b\u0435\u0431\u0430\u043d\u0438\u044f (Mashnich G.P., Tomin V.E., Pulyaev V.A<\/em>. <\/strong>Spectral observations of the motions in and around filament: Transverse oscillations)<\/td>5\u201313<\/td>PDF<\/strong><\/a><\/td>3\u201310<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0422\u0443\u043b\u044c\u043d\u0438\u043a\u043e\u0432 \u0415.\u0414., \u041c\u0430\u0445\u043c\u0443\u0442\u043e\u0432 \u0412.\u0421., \u0424\u0438\u043b\u0438\u043f\u043f\u043e\u0432 \u041c.\u0412<\/em>. <\/strong>\u041f\u0440\u0438\u043c\u0435\u043d\u0435\u043d\u0438\u0435 \u043c\u0435\u0442\u043e\u0434\u043e\u0432 \u043c\u0430\u0448\u0438\u043d\u043d\u043e\u0433\u043e \u043e\u0431\u0443\u0447\u0435\u043d\u0438\u044f \u0434\u043b\u044f \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0432 \u044d\u043a\u0441\u043f\u0435\u0440\u0438\u043c\u0435\u043d\u0442\u0435 \u00ab\u0421\u043e\u043b\u043d\u0446\u0435-\u0422\u0435\u0440\u0430\u0433\u0435\u0440\u0446\u00bb (Tulnikov E.D., Makhmutov V.S., Philippov M.V<\/em>.<\/strong> Application of machine learning methods to determine spectral characteristics of radiation in the \u201cSolntse-Terahertz\u201d experiment)<\/td>14\u201320<\/td>PDF<\/strong><\/a><\/td>11\u201317<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0412\u0435\u043d\u0438\u0430\u043c\u0438\u043d\u043e\u0432 \u0421.\u0421<\/em>., \u041a\u043e\u0437\u043b\u043e\u0432 \u0421.\u0418., \u041a\u0443\u0437\u044c\u043c\u0438\u0447\u0435\u0432\u0430 \u041c.\u042e.<\/em> <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043c\u0443\u0441\u043e\u0440\u0430 \u043d\u0430 \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f (Veniaminov S.S., Kozlov S.I., Kuzmicheva M.Yu<\/em>. <\/strong>Space debris effect on solar radiation propagation)<\/td>21\u201324<\/td>PDF<\/strong><\/a><\/td>18\u201321<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0438\u0434\u043e\u0440\u0435\u043d\u043a\u043e \u041a.\u0410., \u0412\u0430\u0441\u0435\u043d\u0438\u043d\u0430 \u0410.\u0410<\/em>. <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u0432\u043b\u0438\u044f\u043d\u0438\u044f \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c \u043d\u0430 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u044b \u0441\u043b\u043e\u044f F2 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u0442\u0435\u0447\u0435\u043d\u0438\u0435 24-\u0433\u043e \u0446\u0438\u043a\u043b\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Sidorenko K.A., Vasenina<\/em><\/strong> <\/em>A.A<\/em>. <\/strong>Studying the influence of geomagnetic storms on parameters of the ionospheric F2 layer during solar activity cycle 24)<\/td>25\u201332<\/td>PDF<\/strong><\/a><\/td>22\u201328<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0424\u0435\u0434\u043e\u0440\u043e\u0432 \u0415.\u041d., \u0417\u0438\u043d\u043a\u0438\u043d<\/em><\/strong> \u0414.\u0412<\/strong><\/em>. <\/strong>\u041c\u0430\u0433\u043d\u0438\u0442\u043e\u0442\u0435\u043b\u043b\u0443\u0440\u0438\u0447\u0435\u0441\u043a\u043e\u0435 \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0438 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u0430\u044f \u0434\u0438\u0430\u0433\u043d\u043e\u0441\u0442\u0438\u043a\u0430 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b \u0438 \u043b\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b: \u0432\u043e\u0437\u043c\u043e\u0436\u043d\u043e\u0441\u0442\u0438 \u0432\u0437\u0430\u0438\u043c\u043e\u0434\u043e\u043f\u043e\u043b\u043d\u0435\u043d\u0438\u044f (Pilipenko V.A., Fedorov E.N., Zinkin D.V<\/em>. <\/strong>Magnetotelluric sounding and electromagnetic diagnostics of the magnetosphere and lithosphere: possibilities of complementarity)<\/kbd><\/td>33\u201344<\/td>PDF<\/strong><\/a><\/td>29\u201339<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439 \u041a.\u0413., \u041c\u0435\u0434\u0432\u0435\u0434\u0435\u0432\u0430<\/em><\/strong> \u0418.\u0412<\/strong><\/em>. <\/strong>\u0421\u0440\u0430\u0432\u043d\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u043e\u0442\u043a\u043b\u0438\u043a\u043e\u0432 \u043c\u0438\u043d\u0438\u043c\u0430\u043b\u044c\u043d\u043e\u0439 \u0447\u0430\u0441\u0442\u043e\u0442\u044b \u043e\u0442\u0440\u0430\u0436\u0435\u043d\u0438\u0439 \u043d\u0430 \u0438\u043e\u043d\u043e\u0433\u0440\u0430\u043c\u043c\u0430\u0445 \u0438 \u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u044b \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u043c\u0435\u0437\u043e\u0441\u0444\u0435\u0440\u044b \u0438 \u043d\u0438\u0436\u043d\u0435\u0439 \u0442\u0435\u0440\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430 \u0437\u0438\u043c\u043d\u0438\u0435 \u0432\u043d\u0435\u0437\u0430\u043f\u043d\u044b\u0435 \u0441\u0442\u0440\u0430\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0435 \u043f\u043e\u0442\u0435\u043f\u043b\u0435\u043d\u0438\u044f (Ratovsky K.G., Medvedeva<\/em><\/strong> I.V<\/strong><\/em>. <\/strong>Comparative analysis of responses of minimum frequency of ionogram reflections and mesosphere-lower thermosphere temperature to winter sudden stratospheric warmings)<\/td>45 \u201354<\/td>PDF<\/strong><\/a><\/td>40\u201349<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u0413\u0440\u043e\u0437\u043e\u0432<\/em><\/strong> \u0412.\u041f<\/strong><\/em>. <\/strong>\u041c\u0435\u0442\u043e\u0434\u0438\u043a\u0430 \u0430\u0432\u0442\u043e\u043c\u0430\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0432\u0435\u0440\u0442\u0438\u043a\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u043d\u0435\u043f\u0440\u0435\u0440\u044b\u0432\u043d\u044b\u043c \u041b\u0427\u041c-\u0441\u0438\u0433\u043d\u0430\u043b\u043e\u043c (Ponomarchuk S.N., Grozov V.P<\/em>. <\/strong>Technique of ionospheric parameter automatic determination using data from vertical sounding with a continuous chirp signal)<\/td>55\u201363<\/td>PDF<\/strong><\/a><\/td>50\u201358<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041d\u0438\u043a\u0438\u0442\u0435\u043d\u043a\u043e \u0410.\u0421., \u041b\u0435\u0431\u0435\u0434\u044c \u041e.\u041c., \u041b\u0430\u0440\u0447\u0435\u043d\u043a\u043e \u0410.\u0412., \u0424\u0435\u0434\u043e\u0440\u0435\u043d\u043a\u043e \u042e.\u0412<\/em>. <\/strong>\u0410\u043d\u0430\u043b\u0438\u0437 \u0441\u043e\u0431\u044b\u0442\u0438\u0439 \u043e\u0434\u043d\u043e\u0432\u0440\u0435\u043c\u0435\u043d\u043d\u043e\u0439 \u043d\u0430\u0437\u0435\u043c\u043d\u043e\u0439 \u0440\u0435\u0433\u0438\u0441\u0442\u0440\u0430\u0446\u0438\u0438 \u0432\u0441\u043f\u043b\u0435\u0441\u043a\u043e\u0432 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0448\u0438\u043f\u0435\u043d\u0438\u0439 \u0438 \u0432\u043e\u0437\u0440\u0430\u0441\u0442\u0430\u043d\u0438\u044f \u0440\u0438\u043e\u043c\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043f\u043e\u0433\u043b\u043e\u0449\u0435\u043d\u0438\u044f (Nikitenko A.S., Lebed O.M., Larchenko A.V., Fedorenko Yu.V<\/em>. <\/strong>Analyzing events of simultaneous ground-based registration of auroral hiss bursts and riometric absorption increase)<\/td>64\u201373<\/td>PDF<\/strong><\/a><\/td>59\u201367<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0427\u0435\u0440\u043d\u0438\u0433\u043e\u0432\u0441\u043a\u0430\u044f \u041c.\u0410., \u0425\u0430\u0431\u0438\u0442\u0443\u0435\u0432 \u0414.\u0421., \u0421\u0435\u0442\u043e\u0432 \u0410.\u0413., \u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439 \u041a.\u0413., \u041a\u0430\u043b\u0438\u0448\u0438\u043d \u0410.\u0421., \u0414\u043e\u043b\u0433\u0430\u0447\u0435\u0432\u0430 \u0421.\u0410., \u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0415., \u0411\u0435\u043b\u0438\u043d\u0441\u043a\u0430\u044f \u0410.\u042e., \u0411\u044b\u0447\u043a\u043e\u0432 \u0412.\u0412., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432\u0430 \u0421.\u0410., \u041f\u0430\u043d\u0447\u0435\u043d\u043a\u043e \u0412.\u0410., \u0422\u0438\u043c\u0447\u0435\u043d\u043a\u043e<\/em><\/strong> \u0410.\u0412<\/strong><\/em>. <\/strong>\u0422\u0435\u0440\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0435 \u044d\u0444\u0444\u0435\u043a\u0442\u044b \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0441\u0443\u043f\u0435\u0440\u0431\u0443\u0440\u044c \u0432 \u043c\u0430\u0435 2024 \u0433. \u0438 \u043e\u043a\u0442\u044f\u0431\u0440\u0435\u2013\u043d\u043e\u044f\u0431\u0440\u0435 2003 \u0433.  \u0432 \u0421\u0435\u0432\u0435\u0440\u043d\u043e\u043c \u043f\u043e\u043b\u0443\u0448\u0430\u0440\u0438\u0438  \u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0439 \u043e\u0442\u043a\u043b\u0438\u043a \u043d\u0430 \u043d\u0438\u0445 (Chernigovskaya M.A., Khabituev D.S., Setov A.G., Ratovsky K.G., Kalishin A.S., Dolgacheva S.A., Stepanov A.E., Belinskaya A.Yu., Bychkov V.V., Grigorieva S.A., Panchenko V.A., Timchenko A.V<\/em>. <\/strong>Thermospheric effects during the magnetic superstorms in May 2024 and October\u2013November 2003 in the Northern Hemisphere and the ionospheric response to them)<\/td>74\u201394<\/td>PDF<\/strong><\/a><\/td>68\u201386<\/td>PDF<\/a><\/td><\/tr>
\u041b\u0435\u0431\u0435\u0434\u044c \u041e.\u041c., \u041f\u0438\u043b\u044c\u0433\u0430\u0435\u0432 \u0421.\u0412., \u041b\u0430\u0440\u0447\u0435\u043d\u043a\u043e \u0410.\u0412., \u0411\u043b\u0430\u0433\u043e\u0432\u0435\u0449\u0435\u043d\u0441\u043a\u0430\u044f \u041d.\u0424., \u041a\u0430\u043b\u0438\u0448\u0438\u043d \u0410.\u0421., \u0411\u043e\u0440\u0438\u0441\u043e\u0432\u0430 \u0422.\u0414., \u0421\u0442\u0440\u0438\u0431\u043d\u044b\u0439 \u041e.\u042e., \u0424\u0438\u043b\u0430\u0442\u043e\u0432 \u041c.\u0412., \u041a\u0443\u0437\u043d\u0435\u0446\u043e\u0432\u0430 \u041c.\u0412., \u041d\u0438\u043a\u0438\u0442\u0435\u043d\u043a\u043e \u0410.\u0421., \u0411\u0435\u043a\u0435\u0442\u043e\u0432\u0430 \u0415.\u0411., \u0424\u0435\u0434\u043e\u0440\u0435\u043d\u043a\u043e \u042e.\u0412<\/em>. <\/strong>\u041f\u0435\u0440\u0432\u044b\u0435 \u0440\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u044b \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0439 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0448\u0438\u043f\u0435\u043d\u0438\u0439 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u044d\u043a\u0441\u043f\u0435\u0434\u0438\u0446\u0438\u0438 \u00ab\u0421\u0435\u0432\u0435\u0440\u043d\u044b\u0439 \u043f\u043e\u043b\u044e\u0441\u201341\u00bb (Lebed O.M., Pilgaev S.V., Larchenko A.V., Blagoveshchenskaya N.F., Kalishin A.S., Borisova T.D., Stribny O.Yu<\/em>., Filatov M.V., Kuznetsova M.V., Nikitenko A.S., Beketova E.B., Fedorenko Yu.V<\/em>.<\/strong> The first results of observations of auroral hiss during the \u00abNorth Pole\u201341\u00bb expedition)<\/td>95\u2013106<\/td>PDF<\/strong><\/a><\/td>87\u201397<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u043e\u0437\u043b\u043e\u0432 \u0421.\u0418., \u041b\u044f\u0445\u043e\u0432 \u0410.\u041d., \u041d\u0438\u043a\u043e\u043b\u0430\u0439\u0448\u0432\u0438\u043b\u0438 \u0421.\u0428., \u042f\u043a\u0438\u043c \u0412.\u0412<\/em>. <\/strong>\u041f\u043e\u043b\u0443\u044d\u043c\u043f\u0438\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0439 \u043f\u0440\u0438\u0431\u043b\u0438\u0436\u0435\u043d\u043d\u044b\u0439 \u043c\u0435\u0442\u043e\u0434 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043d\u0435\u043a\u043e\u0442\u043e\u0440\u044b\u0445 \u0432\u043e\u043f\u0440\u043e\u0441\u043e\u0432 \u0430\u044d\u0440\u043e\u043d\u043e\u043c\u0438\u0438 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 D \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b. III. \u0414\u0435\u0442\u0430\u043b\u044c\u043d\u044b\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u0444\u043e\u0442\u043e\u0445\u0438\u043c\u0438\u0438 \u0441\u0440\u0435\u0434\u044b \u0432 \u0443\u0441\u043b\u043e\u0432\u0438\u044f\u0445 \u043f\u043e\u0432\u044b\u0448\u0435\u043d\u043d\u043e\u0433\u043e \u0443\u0440\u043e\u0432\u043d\u044f \u0438\u043e\u043d\u0438\u0437\u0430\u0446\u0438\u0438 (Kozlov S.I., Lyakhov A.N., Nikolaishvili S.Sh., Yakim V.V<\/em>.<\/strong> A semi-empirical approximate method for studying some issues of aeronomy of the ionospheric D-region. III. Detailed analysis of the photochemistry of the environment under conditions of increased ionization)<\/td>107\u2013114<\/td>PDF<\/strong><\/a><\/td>98\u2013104<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0413\u0430\u0432\u0440\u0438\u043b\u043e\u0432 \u041d.\u041c., \u041a\u0448\u0435\u0432\u0435\u0446\u043a\u0438\u0439 \u0421.\u041f., \u041a\u043e\u0432\u0430\u043b\u044c \u0410.\u0412., \u041a\u0443\u0440\u0434\u044f\u0435\u0432\u0430 \u042e.\u0410<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043a\u0440\u0438\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0443\u0440\u043e\u0432\u043d\u0435\u0439 \u043d\u0430 \u0441\u043f\u0435\u043a\u0442\u0440\u044b \u0432\u0442\u043e\u0440\u0438\u0447\u043d\u044b\u0445 \u0433\u0440\u0430\u0432\u0438\u0442\u0430\u0446\u0438\u043e\u043d\u043d\u044b\u0445 \u0432\u043e\u043b\u043d \u0432 \u0441\u0440\u0435\u0434\u043d\u0435\u0439 \u0438 \u0432\u0435\u0440\u0445\u043d\u0435\u0439 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0435 (Gavrilov N.M., Kshevetski S.P., Koval A.V., Kurdyaeva<\/em><\/strong> Yu.A<\/strong><\/em>. <\/strong>Critical level influence on spectra of secondary gravity waves in the middle and upper atmosphere)<\/td>115\u2013124<\/td>PDF<\/strong><\/a><\/td>105\u2013113<\/td>PDF<\/a><\/td><\/tr>
\u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432 \u0410.\u0412., \u0421\u043e\u043b\u043e\u0432\u044c\u0435\u0432 \u0410.\u0410., \u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432\u0430 \u0413.\u0420., \u041b\u0430\u043f\u0438\u043d <\/sup>\u0410.\u041d<\/em>.<\/strong> \u0412\u0435\u0440\u043e\u044f\u0442\u043d\u043e\u0441\u0442\u043d\u0430\u044f \u043e\u0446\u0435\u043d\u043a\u0430 \u0443\u0440\u043e\u0432\u043d\u044f \u0433\u0435\u043e\u0438\u043d\u0434\u0443\u0446\u0438\u0440\u043e\u0432\u0430\u043d\u043d\u044b\u0445 \u0442\u043e\u043a\u043e\u0432 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043e \u043b\u043e\u043a\u0430\u043b\u0438\u0437\u0430\u0446\u0438\u0438 \u0438 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0435 \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u0439 (Vorobev A.V., Soloviev A.A., Vorobeva G.R., Lapin <\/sup>A.N.<\/em><\/strong> Probabilistic assessment of geomagnetically induced current level based on auroral localization and structure data)<\/td>125\u2013
133<\/td>		PDF<\/strong><\/a><\/td>114\u2013122<\/td>PDF<\/strong><\/a><\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

<\/p>","protected":false},"excerpt":{"rendered":"

\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. Pp. \u041c\u0430\u0448\u043d\u0438\u0447 \u0413.\u041f., \u0422\u043e\u043c\u0438\u043d \u0412.\u0415., \u041f\u0443\u043b\u044f\u0435\u0432 \u0412.\u0410. \u0421\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0434\u0432\u0438\u0436\u0435\u043d\u0438\u0439 \u0432 \u0432\u043e\u043b\u043e\u043a\u043d\u0435 \u0438 \u0435\u0433\u043e \u043e\u043a\u0440\u0435\u0441\u0442\u043d\u043e\u0441\u0442\u044f\u0445: \u043f\u043e\u043f\u0435\u0440\u0435\u0447\u043d\u044b\u0435 \u043a\u043e\u043b\u0435\u0431\u0430\u043d\u0438\u044f (Mashnich G.P., Tomin V.E., Pulyaev V.A. Spectral observations of the motions in and around filament: Transverse oscillations) 5\u201313 PDF 3\u201310 PDF \u0422\u0443\u043b\u044c\u043d\u0438\u043a\u043e\u0432 \u0415.\u0414., \u041c\u0430\u0445\u043c\u0443\u0442\u043e\u0432 \u0412.\u0421., \u0424\u0438\u043b\u0438\u043f\u043f\u043e\u0432 \u041c.\u0412. \u041f\u0440\u0438\u043c\u0435\u043d\u0435\u043d\u0438\u0435 \u043c\u0435\u0442\u043e\u0434\u043e\u0432 \u043c\u0430\u0448\u0438\u043d\u043d\u043e\u0433\u043e \u043e\u0431\u0443\u0447\u0435\u043d\u0438\u044f \u0434\u043b\u044f \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f […]<\/p>","protected":false},"author":54,"featured_media":0,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[],"tags":[],"class_list":["post-11334","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11334","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/users\/54"}],"replies":[{"embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/comments?post=11334"}],"version-history":[{"count":7,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11334\/revisions"}],"predecessor-version":[{"id":11394,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11334\/revisions\/11394"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=11334"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=11334"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=11334"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}