{"id":9071,"date":"2025-09-24T14:57:17","date_gmt":"2025-09-24T14:57:17","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=9071"},"modified":"2025-09-30T00:47:32","modified_gmt":"2025-09-30T00:47:32","slug":"solnechno-zemnaya-fizika-tom-11-%e2%84%963-2025-2","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-11-%e2%84%963-2025-2\/","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 11, \u21163, 2025"},"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>
\u0414\u0432\u0430\u0434\u0446\u0430\u0442\u0430\u044f \u0435\u0436\u0435\u0433\u043e\u0434\u043d\u0430\u044f \u043a\u043e\u043d\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u044f \u00ab\u0424\u0438\u0437\u0438\u043a\u0430 \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0441\u0438\u0441\u0442\u0435\u043c\u0435\u00bb,<\/strong>
10\u201314 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 2025 \u0433., \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0439 \u0420\u0410\u041d<\/strong><\/td>		<\/td><\/td><\/td><\/td><\/tr>
\u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0410\u043d\u0444\u0438\u043d\u043e\u0433\u0435\u043d\u0442\u043e\u0432 \u0421.\u0410., \u0416\u0434\u0430\u043d\u043e\u0432 \u0414.\u0410., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418.,<\/em> \u0418\u0432\u0430\u043d\u043e\u0432 \u0415.\u0424., \u0427\u044d\u043d\u043c\u0438\u043d \u0422\u0430\u043d\u044c, \u0427\u0436\u0430\u043e \u0423<\/em>. <\/strong>\u041f\u0440\u043e\u0446\u0435\u0441\u0441\u044b \u0443\u0441\u043a\u043e\u0440\u0435\u043d\u0438\u044f \u0438 \u043f\u0435\u0440\u0435\u043d\u043e\u0441\u0430 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u0432 \u0438\u043c\u043f\u0443\u043b\u044c\u0441\u043d\u043e\u0439 \u043a\u0440\u0443\u0433\u043e\u0432\u043e\u0439 \u043b\u0435\u043d\u0442\u043e\u0447\u043d\u043e\u0439 \u0432\u0441\u043f\u044b\u0448\u043a\u0435 (Altyntsev A.T., Meshalkina N.S., Anfinogentov S.A., Zhdanov D.A., Myshyakov I.I., Ivanov E.F., Chengming Tan, Zhao Wu<\/em>. <\/strong>Processes of acceleration and transfer of electrons in a pulse circular ribbon flare)<\/td>5\u201315<\/td>PDF<\/a><\/strong><\/td>3\u201312<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0420\u0430\u0445\u043c\u0430\u043d\u043e\u0432\u0430 \u041b.\u0421., \u0420\u044f\u0437\u0430\u043d\u0446\u0435\u0432\u0430 \u041c.\u041e., \u0425\u043e\u0445\u043b\u0430\u0447\u0435\u0432 \u0410.\u0410., \u0415\u0440\u043c\u043e\u043b\u0430\u0435\u0432 \u042e.\u0418., \u0417\u0430\u0441\u0442\u0435\u043d\u043a\u0435\u0440<\/em><\/strong> \u0413.\u041d<\/strong><\/em>. <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0442\u0443\u0440\u0431\u0443\u043b\u0435\u043d\u0442\u043d\u043e\u0433\u043e \u043a\u0430\u0441\u043a\u0430\u0434\u0430 \u0432 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u043b\u043e\u0435 \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b ICME (Rakhmanova L.S., Riazantseva M.O., Khokhlachev A.A., Yermolaev Yu.I., Zastenker G.N<\/em>. <\/strong>Features of turbulent cascade development in the magnetosheath during ICME)<\/td>16\u201325<\/td>PDF<\/a><\/strong><\/td>13\u201321<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0442\u043e\u0432\u0430 \u0413.\u0410., \u0427\u0443\u0433\u0443\u043d\u0438\u043d \u0414.\u0412., \u0411\u0435\u0437\u0440\u0443\u043a\u0438\u0445 \u0412.\u0412<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u043d\u0430 \u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u0443 \u0438 \u043f\u043b\u043e\u0442\u043d\u043e\u0441\u0442\u044c \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u043f\u043b\u0430\u0437\u043c\u043e\u0441\u0444\u0435\u0440\u0435 \u0417\u0435\u043c\u043b\u0438 (Kotova G.A., Chugunin D.V., Bezrukikh V.V<\/em>. <\/strong>Effect of solar activity and solar wind parameters on plasma temperature and density in Earth\u2019s plasmasphere)<\/td>26\u201335<\/td>PDF<\/a><\/strong><\/td>22\u201330<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u043a\u0430\u0440\u043e\u0432 \u0413.\u0410<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u044b\u0445 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043d\u0430 \u043f\u043e\u043a\u0430\u0437\u0430\u0442\u0435\u043b\u044c \u0441\u0442\u0435\u043f\u0435\u043d\u0438 \u0441\u0438\u043c\u043c\u0435\u0442\u0440\u0438\u0438 \u043a\u043e\u043b\u044c\u0446\u0435\u0432\u043e\u0433\u043e \u0442\u043e\u043a\u0430 (Makarov G.A<\/em>. <\/strong>Influence of interplanetary parameters on the degree of symmetry of the ring current)<\/td>36\u201341<\/td>PDF<\/a><\/strong><\/td>31\u201336<\/td>PDF<\/a><\/strong><\/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>\u0413\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0435 \u043e\u0431\u0440\u0435\u0437\u0430\u043d\u0438\u0435 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 23\u201324 \u043c\u0430\u0440\u0442\u0430 2023 \u0433.: \u0441\u0432\u044f\u0437\u044c \u0441 \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 \u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u044c\u044e \u0441 \u0443\u0447\u0435\u0442\u043e\u043c \u0448\u0438\u0440\u043e\u0442\u043d\u044b\u0445 \u044d\u0444\u0444\u0435\u043a\u0442\u043e\u0432 (Danilova O.A., Ptitsyna N.G., Sdobnov V.E<\/em>. <\/strong>Geomagnetic cutoff of cosmic rays during the March 23\u201324, 2023 magnetic storm: Relationship with solar wind parameters and geomagnetic activity taking into account latitudinal <\/strong>effects)<\/td>42\u201349<\/td>PDF<\/a><\/strong><\/td>37\u201343<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u0413., \u0413\u0435\u0440\u0430\u0441\u0438\u043c\u043e\u0432\u0430 <\/a>\u0421.\u041a<\/em>. <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u0434\u0438\u043d\u0430\u043c\u0438\u043a\u0438 \u044d\u043d\u0435\u0440\u0433\u0435\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u0441\u043f\u0435\u043a\u0442\u0440\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0441\u0443\u0442\u043e\u0447\u043d\u044b\u0445 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0439 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432 20\u201325 \u0446\u0438\u043a\u043b\u0430\u0445 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0441\u043a\u0440\u0435\u0449\u0435\u043d\u043d\u044b\u0445 \u043c\u044e\u043e\u043d\u043d\u044b\u0445 \u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f\u043e\u0432 (Gololobov P.Yu., Grigoryev V.G., Gerasimova S.K<\/em>. <\/strong>Studying dynamics of energy spectrum of solar diurnal variations in cosmic rays during solar activity cycles 20\u201325, using method of crossed muon telescopes)<\/td>50\u201355<\/td>PDF<\/a><\/strong><\/td>44\u201349<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410<\/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\u043e\u0439 \u0443\u0434\u0430\u0440\u043d\u043e\u0439 \u0432\u043e\u043b\u043d\u044b 10 \u043c\u0430\u044f 2024 \u0433. (Starodubtsev S.A<\/em>. <\/strong>MHD waves in the pre-front region of the interplanetary shock on May 10, 2024)<\/td>56\u201364<\/td>PDF<\/a><\/strong><\/td>50\u201358<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u043e\u0438\u0441\u0435\u0435\u0432 \u0410.\u0412., \u041f\u043e\u043f\u043e\u0432 \u0412.\u0418., \u041c\u0438\u0448\u0438\u043d \u0412.\u0412., \u041f\u0435\u043d\u0441\u043a\u0438\u0445 \u042e.\u0412<\/em>. <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u044f \u0432 \u0441\u0438\u0441\u0442\u0435\u043c\u0435 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u0430\u2014\u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0430  \u043a\u043e\u043c\u043f\u0440\u0435\u0441\u0441\u0438\u043e\u043d\u043d\u044b\u0445 \u0434\u043b\u0438\u043d\u043d\u043e\u043f\u0435\u0440\u0438\u043e\u0434\u043d\u044b\u0445 \u043a\u043e\u043b\u0435\u0431\u0430\u043d\u0438\u0439, \u043f\u0440\u043e\u043d\u0438\u043a\u0430\u044e\u0449\u0438\u0445 \u0438\u0437 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u0441\u0440\u0435\u0434\u044b (Moiseev A.V., Popov V.I., Mishin V.V., Penskikh Yu.V<\/em>. <\/strong>Features of propagation of compressional long-period oscillations penetrating from the interplanetary medium in the magnetosphere\u2014ionosphere system)<\/td>65\u201376<\/td>PDF<\/a><\/strong><\/td>59\u201369<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0435\u043b\u043e\u0432\u0430 \u0410.\u041e., \u041c\u044f\u0433\u043a\u043e\u0432\u0430 \u0418.\u041d.<\/em> <\/strong>\u041f\u0440\u043e\u0433\u043d\u043e\u0437\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u043f\u043e\u0442\u043e\u043a\u043e\u0432 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u043d\u0430 \u043a\u0440\u0443\u0433\u043e\u0432\u043e\u0439 \u043f\u043e\u043b\u044f\u0440\u043d\u043e\u0439 \u043e\u0440\u0431\u0438\u0442\u0435: \u043e\u0442\u0431\u043e\u0440 \u043f\u0440\u0435\u0434\u0438\u043a\u0442\u043e\u0440\u043e\u0432 (Belova A.O., Myagkova I.N.<\/em> <\/strong>Prediction of electron fluxes in a circular polar orbit: Selection of predictors)<\/td>77\u201387<\/td>PDF<\/a><\/strong><\/td>70\u201379<\/td>PDF<\/a><\/strong><\/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\u0442\u043a\u043b\u0438\u043a \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430 \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435 \u043d\u0430 \u043d\u0435\u0435 \u043d\u0435\u043e\u0431\u044b\u043a\u043d\u043e\u0432\u0435\u043d\u043d\u043e\u0439 \u0440\u0430\u0434\u0438\u043e\u0432\u043e\u043b\u043d\u043e\u0439 \u043f\u0440\u0438 \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0438 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u043d\u0430 \u0447\u0430\u0441\u0442\u043e\u0442\u0435, \u0431\u043b\u0438\u0437\u043a\u043e\u0439 \u043a \u043d\u0430\u0433\u0440\u0435\u0432\u043d\u043e\u0439 (Bakhmetieva N.V., Grigoriev G.I., Zhemyakov I.N., Kalinina E.E., Lisov A.A<\/em>. <\/strong>Ionosphere response to the impact of an extraordinary radio wave when located at a frequency close to the heating frequency)<\/td>88\u201399<\/td>PDF<\/a><\/strong><\/td>80\u201390<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0430\u0440\u0430\u0445\u0430\u043d\u044f\u043d \u0410.\u0410., \u041c\u043e\u043b\u043e\u0434\u044b\u0445 \u0421.\u0418.<\/em> <\/strong>\u041c\u0435\u0442\u0435\u043e\u0440\u043e\u043b\u043e\u0433\u0438\u0447\u0435\u0441\u043a\u0438\u0439 \u043e\u0442\u043a\u043b\u0438\u043a \u043d\u0430 \u0438\u0437\u043c\u0435\u043d\u0435\u043d\u0438\u0435 \u044d\u043b\u0435\u043a\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043f\u043e\u0442\u0435\u043d\u0446\u0438\u0430\u043b\u0430 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b, \u043e\u0431\u0443\u0441\u043b\u043e\u0432\u043b\u0435\u043d\u043d\u043e\u0433\u043e \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u044b\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u043c \u0432\u0435\u0442\u0440\u043e\u043c (Karakhanyan A.A., Molodykh S.I.<\/em> <\/strong>Meteorological response to changes in ionospheric electric potential caused by disturbed solar wind)<\/td>100\u2013107<\/td>PDF<\/a><\/strong><\/td>91\u201397<\/td>PDF<\/a><\/strong><\/td><\/tr>
15-\u044f \u0420\u043e\u0441\u0441\u0438\u0439\u0441\u043a\u043e-\u041a\u0438\u0442\u0430\u0439\u0441\u043a\u0430\u044f \u043a\u043e\u043d\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u044f \u043f\u043e \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043f\u043e\u0433\u043e\u0434\u0435,<\/strong>
9\u201313 \u0441\u0435\u043d\u0442\u044f\u0431\u0440\u044f 2024 \u0433., \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u043e\u0439 \u0444\u0438\u0437\u0438\u043a\u0438 \u0421\u041e \u0420\u0410\u041d<\/strong><\/td>		<\/td><\/td><\/td><\/td><\/tr>
Medvedev A.V., Zherebtsov G.A., Perevalova N.P<\/em>. <\/strong>Chinese-Russian Joint Research Center on Space Weather: Results and prospects<\/td>108\u2013124<\/td>PDF<\/a><\/strong><\/td>98\u2013113<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0412., \u0417\u0430\u0439\u0446\u0435\u0432 \u0412.\u0412<\/em>. <\/strong>\u041d\u0435\u0443\u0441\u0442\u043e\u0439\u0447\u0438\u0432\u043e\u0441\u0442\u044c \u0420\u044d\u043b\u0435\u044f\u2014\u0422\u0435\u0439\u043b\u043e\u0440\u0430 \u043a\u0430\u043a \u0442\u0440\u0438\u0433\u0433\u0435\u0440 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u0435\u043a (Stepanov A.V., Zaitsev V.V.<\/em> <\/strong>The Rayleigh\u2014Taylor instability as a trigger of solar flares)<\/td>125\u2013131<\/td>PDF<\/a><\/strong><\/td>114\u2013119<\/td>PDF<\/a><\/strong><\/td><\/tr>
Demidov M.L., Wang X.F., Sun Y.Z., Deng Y.Y<\/em>. <\/strong>Observations of large-scale solar magnetic fields with a new Chinese telescope constructed for the International Meridian Circle Program (IMCP)<\/td>132\u2013136<\/td>PDF<\/a><\/strong><\/td>120\u2013124<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0433\u043e\u043c\u043e\u043b\u043e\u0432 \u0410.\u0412., \u0411\u043e\u0433\u043e\u043c\u043e\u043b\u043e\u0432 \u0412.\u0412., \u0418\u044e\u0434\u0438\u043d \u0410.\u0424., \u041a\u0430\u043b\u0435\u0433\u0430\u0435\u0432 \u0412.\u0412., \u041c\u044f\u0433\u043a\u043e\u0432\u0430 \u0418.\u041d., \u041e\u0441\u0435\u0434\u043b\u043e \u0412.\u0418., \u0421\u0432\u0435\u0440\u0442\u0438\u043b\u043e\u0432 \u0421.\u0418., \u042f\u0448\u0438\u043d \u0418.\u0412<\/em>. <\/strong>\u041c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433 \u044f\u0432\u043b\u0435\u043d\u0438\u0439 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043f\u043e\u0433\u043e\u0434\u044b \u0441 \u0438\u0441\u043f\u043e\u043b\u044c\u0437\u043e\u0432\u0430\u043d\u0438\u0435\u043c \u0433\u0440\u0443\u043f\u043f\u0438\u0440\u043e\u0432\u043a\u0438 \u043d\u0430\u043d\u043e\u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432 \u00ab\u0421\u043e\u0437\u0432\u0435\u0437\u0434\u0438\u0435-270\u00bb \u041c\u043e\u0441\u043a\u043e\u0432\u0441\u043a\u043e\u0433\u043e \u0443\u043d\u0438\u0432\u0435\u0440\u0441\u0438\u0442\u0435\u0442\u0430 (Bogomolov \u0410.V., Bogomolov V.V., Iyudin \u0410.F., \u041a\u0430legaev V.V., Myagkova I.N., \u041esedlo V.I., Svertilov S.I., Yashin I.V<\/em>. <\/strong>Monitoring of space weather effects with Sozvezdie-270 nanosatellite constellation of Moscow University)<\/td>137\u2013148<\/td>PDF<\/a><\/strong><\/td>125\u2013134<\/td>PDF<\/a><\/strong><\/td><\/tr>
Moiseev A.V., Gololobov A.Yu., Ievenko I.B., Korsakov A.A., Petukhov I.S., Starodubtsev S.A.<\/em><\/strong> Space weather research in Yakutia<\/td>149\u2013159<\/td>PDF<\/a><\/strong><\/td>135\u2013145<\/td>PDF<\/a><\/strong><\/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. \u0414\u0432\u0430\u0434\u0446\u0430\u0442\u0430\u044f \u0435\u0436\u0435\u0433\u043e\u0434\u043d\u0430\u044f \u043a\u043e\u043d\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u044f \u00ab\u0424\u0438\u0437\u0438\u043a\u0430 \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0441\u0438\u0441\u0442\u0435\u043c\u0435\u00bb,10\u201314 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 2025 \u0433., \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0439 \u0420\u0410\u041d \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0410\u043d\u0444\u0438\u043d\u043e\u0433\u0435\u043d\u0442\u043e\u0432 \u0421.\u0410., \u0416\u0434\u0430\u043d\u043e\u0432 \u0414.\u0410., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418., \u0418\u0432\u0430\u043d\u043e\u0432 \u0415.\u0424., \u0427\u044d\u043d\u043c\u0438\u043d \u0422\u0430\u043d\u044c, \u0427\u0436\u0430\u043e \u0423. \u041f\u0440\u043e\u0446\u0435\u0441\u0441\u044b \u0443\u0441\u043a\u043e\u0440\u0435\u043d\u0438\u044f \u0438 \u043f\u0435\u0440\u0435\u043d\u043e\u0441\u0430 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u0432 \u0438\u043c\u043f\u0443\u043b\u044c\u0441\u043d\u043e\u0439 \u043a\u0440\u0443\u0433\u043e\u0432\u043e\u0439 \u043b\u0435\u043d\u0442\u043e\u0447\u043d\u043e\u0439 \u0432\u0441\u043f\u044b\u0448\u043a\u0435 (Altyntsev A.T., Meshalkina N.S., Anfinogentov S.A., Zhdanov D.A., Myshyakov I.I., Ivanov […]<\/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-9071","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/9071","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=9071"}],"version-history":[{"count":15,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/9071\/revisions"}],"predecessor-version":[{"id":9376,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/9071\/revisions\/9376"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=9071"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=9071"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=9071"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}