{"id":8074,"date":"2025-04-23T04:13:56","date_gmt":"2025-04-23T04:13:56","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8074"},"modified":"2025-10-24T17:01:51","modified_gmt":"2025-10-24T17:01:51","slug":"solnechno-zemnaya-fizika-tom-10-%e2%84%963-2024","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-10-%e2%84%963-2024\/","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 10, \u21163, 2024"},"content":{"rendered":"
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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/td>\u0421\u0442\u0440.<\/td><\/td>Pp.<\/td><\/td><\/tr>
\u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0421\u044b\u0447 \u0420.\u0410<\/em>. <\/strong>\u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u044b\u0445 \u0434\u044b\u0440 \u043d\u0430 \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u043e\u043c \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u0435 (Altyntsev A.T., Globa M.V., Meshalkina N.S., Sych R.A<\/em>. <\/strong>Observations of coronal holes with the Siberian Radioheliograph)<\/td>5\u201312<\/td>PDF<\/strong><\/a><\/td>3\u201310<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422<\/em>. <\/strong>\u041f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u044f \u043d\u0430\u0433\u0440\u0435\u0432\u0430 \u0432 \u043d\u0430\u0447\u0430\u043b\u0435 \u0432\u0441\u043f\u044b\u0448\u043a\u0438 29 \u0438\u044e\u043d\u044f 2012 \u0433. (Meshalkina N.S., Altyntsev A.T<\/em>. <\/strong>Heating manifestations at the onset of the 29 June 2012 flare)<\/td>13\u201320<\/td>PDF<\/strong><\/a><\/td>11\u201317<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041e\u0432\u0447\u0438\u043d\u043d\u0438\u043a\u043e\u0432\u0430 \u041d.\u0415., \u0411\u043e\u0433\u043e\u0434 \u0412.\u041c., \u041b\u0435\u0431\u0435\u0434\u0435\u0432 <\/sup>\u041c.\u041a<\/em>. <\/strong>\u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0435 \u0432 \u0440\u0430\u0434\u0438\u043e\u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0435 \u043b\u0438\u043d\u0438\u0438 \u043f\u043e\u0433\u043b\u043e\u0449\u0435\u043d\u0438\u044f \u0433\u0438\u0434\u0440\u043e\u043a\u0441\u0438\u043b\u0430 (\u041e\u041d) \u0432 \u0432\u043e\u043b\u043e\u043a\u043d\u0430\u0445 \u0438 \u043f\u0440\u043e\u0442\u0443\u0431\u0435\u0440\u0430\u043d\u0446\u0430\u0445 \u043d\u0430\u0434 \u0430\u043a\u0442\u0438\u0432\u043d\u044b\u043c\u0438 \u043e\u0431\u043b\u0430\u0441\u0442\u044f\u043c\u0438 \u0421\u043e\u043b\u043d\u0446\u0430 (Ovchinnikova N.E., Bogod V.M., Lebedev M.K<\/em>. <\/strong>Observation at radio frequencies of the hydroxyl (OH) absorption line in filaments and prominences above active regions of the Sun)<\/td>21\u201326<\/td>PDF<\/strong><\/a><\/td>18\u201324<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u043c\u0438\u0440\u043d\u043e\u0432 \u0414.\u0410., \u041c\u0435\u043b\u044c\u043d\u0438\u043a\u043e\u0432 \u0412.\u0424<\/em>. <\/strong>\u041c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u0430\u044f \u0434\u0438\u0430\u0433\u043d\u043e\u0441\u0442\u0438\u043a\u0430 \u0432\u0441\u043f\u044b\u0448\u0435\u0447\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0444\u0438\u0442\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c C\u0438\u0431\u0438\u0440\u0441\u043a\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u0430 (Smirnov D.A., Melnikov V.F<\/em>. <\/strong>Microwave diagnostics of flare plasma by the direct fitting method based on data from the Siberian Radioheliograph)<\/td>27\u201339<\/td>PDF<\/strong><\/a><\/td>25\u201336<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411., \u041a\u0430\u043b\u0438\u043d\u0438\u043d \u041c.\u0421<\/em>. <\/strong>\u041f\u044f\u0442\u044c\u0434\u0435\u0441\u044f\u0442 \u043b\u0435\u0442 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043f\u043e\u0432\u0435\u0434\u0435\u043d\u0438\u044f \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0413\u041a\u041b \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0438\u043d\u0432\u0435\u0440\u0441\u0438\u0438 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f. II. \u0418\u043d\u0432\u0435\u0440\u0441\u0438\u044f \u0413\u041c\u041f \u043d\u0430 \u0432\u043d\u0443\u0442\u0440\u0435\u043d\u043d\u0435\u0439 \u0433\u0440\u0430\u043d\u0438\u0446\u0435 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u044b (Krainev M.B., Kalinin M.S<\/em>. <\/strong>Fifty years of studying the GCR intensity during inversion of the heliospheric magnetic fields. II. HMF inversion on the inner heliospheric boundary)<\/td>40\u201352<\/td>PDF<\/strong><\/a><\/td>37\u201349<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410., \u0428\u0430\u0434\u0440\u0438\u043d\u0430<\/em><\/strong> <\/em>\u041b.\u041f<\/em>. <\/strong>\u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u044b \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u043f\u0440\u0435\u0434\u0444\u0440\u043e\u043d\u0442\u0430 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u044b\u0445 \u0443\u0434\u0430\u0440\u043d\u044b\u0445 \u0432\u043e\u043b\u043d 6 \u0438 7 \u0441\u0435\u043d\u0442\u044f\u0431\u0440\u044f 2017 \u0433. (Starodubtsev S.A., Shadrina L.P<\/em>. <\/strong>MHD waves at the pre-front of interplanetary shocks on September 6 and 7, 2017)<\/td>53\u201361<\/td>PDF<\/strong><\/a><\/td>50\u201357<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0430\u043f\u0443\u043d\u043e\u0432\u0430 \u041e.\u0412., \u0411\u043e\u0440\u043e\u0434\u043a\u043e\u0432\u0430 \u041d.\u041b., \u0417\u0430\u0441\u0442\u0435\u043d\u043a\u0435\u0440<\/em><\/strong> \u0413.\u041d<\/strong><\/em>. <\/strong>\u0410\u043d\u0430\u043b\u0438\u0437 \u0441\u043f\u0435\u043a\u0442\u0440\u043e\u0432 \u0444\u043b\u0443\u043a\u0442\u0443\u0430\u0446\u0438\u0439 \u0432\u0435\u043b\u0438\u0447\u0438\u043d\u044b \u043f\u043e\u0442\u043e\u043a\u0430 \u043f\u043b\u0430\u0437\u043c\u044b \u0438 \u043c\u043e\u0434\u0443\u043b\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u043d\u0430 \u043e\u0431\u0440\u0430\u0442\u043d\u044b\u0445 \u0443\u0434\u0430\u0440\u043d\u044b\u0445 \u0432\u043e\u043b\u043d\u0430\u0445 (Sapunova O.V., Borodkova N.L., Zastenker G.N<\/em>. <\/strong>Spectral properties of solar wind plasma stream and magnetic field fluctuations across the fast reverse interplanetary shock)<\/td>62\u201369<\/td>PDF<\/strong><\/a><\/td>58\u201365<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0414\u0430\u043d\u0438\u043b\u043e\u0432\u0430 \u041e.\u0410., \u041f\u0442\u0438\u0446\u044b\u043d\u0430 \u041d.\u0413., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.E<\/em>. <\/strong>\u042f\u0432\u043b\u0435\u043d\u0438\u044f \u0433\u0438\u0441\u0442\u0435\u0440\u0435\u0437\u0438\u0441\u0430 \u0432 \u043e\u0442\u043a\u043b\u0438\u043a\u0435 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u043d\u0430 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u0441\u0440\u0435\u0434\u044b \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 (Danilova O.A., Ptitsyna N.G., Sdobnov V.E<\/em>. <\/strong>Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm)  <\/td>70\u201378<\/td>PDF<\/strong><\/a><\/td>66\u201374<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0443\u0432\u043e\u0440\u043e\u0432\u0430 \u0410.\u0412., \u0414\u043c\u0438\u0442\u0440\u0438\u0435\u0432 \u0410.\u0412<\/em>. <\/strong>\u0423\u0441\u043b\u043e\u0432\u0438\u044f \u043f\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u044f \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u044b\u0445 \u043f\u043e\u0442\u043e\u043a\u043e\u0432 \u044d\u043d\u0435\u0440\u0433\u0438\u0447\u043d\u044b\u0445 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u043d\u0430 L<\/em><1.2, \u0441\u0432\u044f\u0437\u0430\u043d\u043d\u044b\u0435 \u0441 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u044c\u044e \u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430\u043c\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 (Suvorova A.V., Dmitriev A.V<\/em>. <\/strong>Conditions for the occurrence of intense fluxes of energetic electrons at L<\/em><1.2 associated with solar activity and solar wind parameters)<\/td>79\u201387<\/td>PDF<\/strong><\/a><\/td>75\u201382<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0411\u0435\u0441\u043f\u0430\u043b\u043e\u0432 \u041f.\u0410., \u0421\u0430\u0432\u0438\u043d\u0430 \u041e.\u041d., \u0416\u0430\u0440\u0430\u0432\u0438\u043d\u0430 \u041f.\u0414<\/em>. <\/strong>\u0421\u0443\u0449\u0435\u0441\u0442\u0432\u0435\u043d\u043d\u043e\u0441\u0442\u044c \u0432\u0435\u043b\u0438\u0447\u0438\u043d\u044b \u043f\u043b\u0430\u0437\u043c\u0435\u043d\u043d\u043e\u0433\u043e \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u0434\u043b\u044f \u0432\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u044f \u0445\u043e\u0440\u043e\u0432 \u0438 \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u043d\u0435\u0440\u0435\u0433\u0443\u043b\u044f\u0440\u043d\u043e\u0441\u0442\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u0438\u0445 \u0432\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u044f (Bespalov P.A., Savina O.N., Zharavina P.D<\/em>. <\/strong>Importance of the electron plasma parameter for excitation of chorus and formation  of magnetic field irregularity in the region of their excitation)<\/td>88\u201396<\/td>PDF<\/strong><\/a><\/td>83\u201390<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u0430\u043a\u0430\u0440\u043e\u0432 \u0413.\u0410<\/em>. <\/strong>\u041a\u0440\u0443\u043f\u043d\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u0435 \u0441\u0432\u044f\u0437\u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0438\u043d\u0434\u0435\u043a\u0441\u043e\u0432 SYM-H<\/em> and ASY-H<\/em> \u0441 \u0441\u0435\u0432\u0435\u0440\u043e-\u044e\u0436\u043d\u043e\u0439 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442\u043e\u0439 \u041c\u041c\u041f \u0438 \u0431\u0435\u0442\u0430-\u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 (Makarov G.A<\/em>. <\/strong>Large-scale relationships of the geomagnetic indices SYM-H<\/em> and ASY-H<\/em> with the north-south IMF component and the solar wind beta parameter)<\/td>97\u2013103<\/td>PDF<\/strong><\/a><\/td>91\u201396<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u043e\u0438\u0441\u0435\u0435\u0432 \u0410.\u0412., \u041f\u043e\u043f\u043e\u0432 \u0412.\u0418., \u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410<\/em>. <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u043e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0435\u0439 \u0430\u0437\u0438\u043c\u0443\u0442\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u044f \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 P\u04415-\u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0439 \u0438 \u0438\u0445 \u044d\u043a\u0432\u0438\u0432\u0430\u043b\u0435\u043d\u0442\u043d\u044b\u0445 \u0442\u043e\u043a\u043e\u0432\u044b\u0445 \u0432\u0438\u0445\u0440\u0435\u0439 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043d\u0430\u0437\u0435\u043c\u043d\u044b\u0445 \u0438 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432\u044b\u0445 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0439 (Moiseev A.V., Popov V.I., Starodubtsev S.A<\/em>. <\/strong>Investigating azimuthal propagation of Pc5 geomagnetic pulsations and their equivalent current vortices from ground-based and satellite data)<\/td>104\u2013115<\/td>PDF<\/strong><\/a><\/td>97\u2013107<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0414\u043c\u0438\u0442\u0440\u0438\u0435\u0432 \u0410.\u0412., \u0414\u043e\u043b\u0433\u0430\u0447\u0435\u0432\u0430 \u0421.\u0410., \u0422\u0440\u043e\u0448\u0438\u0447\u0435\u0432 \u041e.\u0410., \u041f\u0443\u043b\u0438\u043d\u0435\u0446 \u041c.\u0421<\/em>. <\/strong>\u0421\u0440\u0430\u0432\u043d\u0435\u043d\u0438\u0435 \u043c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u044d\u0444\u0444\u0435\u043a\u0442\u0430 \u043f\u043e\u0433\u043b\u043e\u0449\u0435\u043d\u0438\u044f \u0432 \u043f\u043e\u043b\u044f\u0440\u043d\u043e\u0439 \u0448\u0430\u043f\u043a\u0435 \u0441 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f\u043c\u0438 \u043d\u0430 \u0441\u0435\u0442\u0438 \u0441\u0442\u0430\u043d\u0446\u0438\u0439 \u0410\u0410\u041d\u0418\u0418 (Dmitriev A.V., Dolgacheva S.A., Troshichev O.A., Pulinets M.S<\/em>. <\/strong>Comparison of modeling of the polar cap absorption effect with observations at the AARI ground-based network)<\/td>116\u2013128<\/td>PDF<\/strong><\/a><\/td>108\u2013120<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0411\u0430\u0445\u043c\u0435\u0442\u044c\u0435\u0432\u0430 \u041d.\u0412., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0413.\u0418., \u0416\u0435\u043c\u044f\u043a\u043e\u0432 \u0418.\u041d., \u041a\u0430\u043b\u0438\u043d\u0438\u043d\u0430 \u0415.\u0415., \u041b\u0438\u0441\u043e\u0432 \u0410.\u0410<\/em>. <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u043d\u0438\u0436\u043d\u0435\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0417\u0435\u043c\u043b\u0438 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0437\u0430\u0442\u043c\u0435\u043d\u0438\u0439 \u0421\u043e\u043b\u043d\u0446\u0430 \u0438 \u0432 \u0437\u0430\u0445\u043e\u0434\u043d\u043e-\u0432\u043e\u0441\u0445\u043e\u0434\u043d\u044b\u0435 \u0447\u0430\u0441\u044b \u043f\u043e \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u044f\u043c \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0418\u041f\u041d \u0432\u0431\u043b\u0438\u0437\u0438 \u041d\u0438\u0436\u043d\u0435\u0433\u043e \u041d\u043e\u0432\u0433\u043e\u0440\u043e\u0434\u0430 (Bakhmetieva N.V., Grigoriev G.I., Zhemyakov I.N., Kalinina E.E., Lisov A.A<\/em>. <\/strong>Features of Earth\u2019s lower ionosphere during solar eclipse and sunset and sunrise hours according to measurements by the API method near Nizhny Novgorod)<\/td>129\u2013145<\/td>PDF<\/strong><\/a><\/td>121\u2013136<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u042f\u0433\u043e\u0432\u0430 \u041d.\u0412., \u0421\u0430\u0445\u0430\u0440\u043e\u0432 \u042f.\u0410., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0421\u0435\u043b\u0438\u0432\u0430\u043d\u043e\u0432 \u0412.\u041d<\/em>. <\/strong>\u0414\u043b\u0438\u043d\u043d\u043e\u043f\u0435\u0440\u0438\u043e\u0434\u043d\u044b\u0435 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0438 \u043a\u0430\u043a \u044d\u043b\u0435\u043c\u0435\u043d\u0442 \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043f\u043e\u0433\u043e\u0434\u044b \u043d\u0430 \u0442\u0435\u0445\u043d\u043e\u043b\u043e\u0433\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u0441\u0438\u0441\u0442\u0435\u043c\u044b (Yagova N.V., Sakharov Ya.A., Pilipenko V.A., Selivanov V.N.<\/em><\/strong><\/strong><\/strong> Long-period geomagnetic pulsations as an element of the space weather influence on technologocal systems)<\/td>146\u2013156<\/td>PDF<\/strong><\/a><\/td>137\u2013146<\/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. \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0421\u044b\u0447 \u0420.\u0410. \u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u044b\u0445 \u0434\u044b\u0440 \u043d\u0430 \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u043e\u043c \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u0435 (Altyntsev A.T., Globa M.V., Meshalkina N.S., Sych R.A. Observations of coronal holes with the Siberian Radioheliograph) 5\u201312 PDF 3\u201310 PDF \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422. \u041f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u044f \u043d\u0430\u0433\u0440\u0435\u0432\u0430 \u0432 \u043d\u0430\u0447\u0430\u043b\u0435 \u0432\u0441\u043f\u044b\u0448\u043a\u0438 29 \u0438\u044e\u043d\u044f 2012 \u0433. (Meshalkina N.S., Altyntsev A.T. Heating […]<\/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-8074","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8074","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=8074"}],"version-history":[{"count":15,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8074\/revisions"}],"predecessor-version":[{"id":9702,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8074\/revisions\/9702"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8074"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8074"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8074"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}