{"id":10619,"date":"2025-12-20T06:18:26","date_gmt":"2025-12-20T06:18:26","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=10619"},"modified":"2025-12-20T07:19:42","modified_gmt":"2025-12-20T07:19:42","slug":"solnechno-zemnaya-fizika-tom-11-%e2%84%964-2025","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-11-%e2%84%964-2025\/","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, \u21164, 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>
\u041a\u0438\u0447\u0430\u0442\u0438\u043d\u043e\u0432 \u041b.\u041b<\/em>. <\/strong>\u041c\u043e\u0434\u0435\u043b\u044c \u043a\u0440\u0443\u043f\u043d\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u0445 \u0442\u0435\u0447\u0435\u043d\u0438\u0439 \u0432 \u043a\u043e\u043d\u0432\u0435\u043a\u0442\u0438\u0432\u043d\u044b\u0445 \u0437\u043e\u043d\u0430\u0445 \u0421\u043e\u043b\u043d\u0446\u0430 \u0438 \u0437\u0432\u0435\u0437\u0434 (Kitchatinov L.L<\/em>. <\/strong>Large-scale flow model for solar and stellar convection zones)<\/td>5\u201316<\/td>PDF<\/a><\/strong><\/td>3\u201313<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u0417\u043e\u043b\u043e\u0442\u0443\u0445\u0438\u043d\u0430 \u041d.\u0410., \u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u0411\u0435\u043b\u0438\u043d\u0441\u043a\u0430\u044f \u0410.\u042e., \u0413\u0440\u043e\u0437\u043e\u0432 \u0412.\u041f., \u041e\u0439\u043d\u0430\u0446 \u0410.\u0412., \u041f\u043e\u0434\u0434\u0435\u043b\u044c\u0441\u043a\u0438\u0439 \u0410.\u0418., \u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0410.\u0412., \u0426\u0435\u0434\u0440\u0438\u043a<\/em><\/strong> \u041c.\u0412<\/strong><\/em>. <\/strong>\u042d\u0444\u0444\u0435\u043a\u0442\u044b \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 10\u201313 \u043c\u0430\u044f 2024 \u0433. \u0432 \u0410\u0437\u0438\u0430\u0442\u0441\u043a\u043e\u043c \u0440\u0435\u0433\u0438\u043e\u043d\u0435 \u0420\u043e\u0441\u0441\u0438\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \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., Zolotukhina N.A., Kurkin V.I., Belinskaya A.Yu., Grozov V.P., Oinats A.V., Poddelsky A.I., Podlesnyi A.V., Cedrik M.V<\/em>.<\/strong> Effects of the May 10\u201313, 2024 magnetic storm in the Asian region of Russia from ionospheric sounding with a continuous chirp signal)<\/td>17\u201332<\/td>PDF<\/a><\/strong><\/td>14\u201328<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u0415\u0434\u0435\u043c\u0441\u043a\u0438\u0439 \u0418.\u041a., \u0428\u0435\u043b\u043a\u043e\u0432 \u0410.\u0414., \u0410\u0440\u0442\u0430\u043c\u043e\u043d\u043e\u0432 \u041c.\u0424., \u0410\u043b\u0441\u0430\u0442\u043a\u0438\u043d \u0421.\u0421., \u0415\u0432\u0441\u0435\u0435\u0432 \u0423.\u041d., \u041b\u0435\u0431\u0435\u0434\u0435\u0432 \u0412.\u041f., \u0422\u0430\u0448\u043b\u044b\u043a\u043e\u0432 \u0412.\u041f., \u0422\u0430\u0449\u0438\u043b\u0438\u043d \u0410.\u0412., \u0422\u0438\u043c\u0447\u0435\u043d\u043a\u043e \u0410.\u0412<\/em>. <\/strong>\u0410\u043d\u0430\u043b\u0438\u0437 \u043f\u043e\u0432\u0435\u0434\u0435\u043d\u0438\u044f \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u0438 \u0441\u0432\u0435\u0447\u0435\u043d\u0438\u044f I<\/em>630<\/sub> \u0441\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0439 \u0432\u0435\u0440\u0445\u043d\u0435\u0439 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0441 \u0438\u0441\u043f\u043e\u043b\u044c\u0437\u043e\u0432\u0430\u043d\u0438\u0435\u043c \u0434\u0430\u043d\u043d\u044b\u0445 \u0440\u0430\u0434\u0430\u0440\u0430 \u041d\u0420 \u0438 \u0438\u043d\u0442\u0435\u0440\u0444\u0435\u0440\u043e\u043c\u0435\u0442\u0440\u0430 \u0424\u0430\u0431\u0440\u0438\u2014\u041f\u0435\u0440\u043e (Vasiliev R.V., Edemskiy I.K., Shelkov A.D., Artamonov M.F., Alsatkin S.S., Evseev U.N., Lebedev V.P., Tashlykov V.P., Tashchilin A.V., Timchenko A.V<\/em>. <\/strong>Analyzing the behavior of mid-latitude upper atmosphere ionospheric plasma and airglow I<\/em>630<\/sub> from IS radar and Fabry\u2014Perot interferometer data)<\/td>33\u201343<\/td>PDF<\/a><\/strong><\/td>29\u201338<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0424\u0435\u0434\u043e\u0440\u043e\u0432 \u0415.\u041d., \u041c\u0430\u0437\u0443\u0440 \u041d.\u0413., \u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u0415.\u041d., \u0420\u044f\u0431\u043e\u0432 \u0410.\u0412., \u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421., \u041c\u0430\u0440\u0447\u0443\u043a \u0420.\u0410., \u041a\u043e\u043b\u043e\u0431\u043e\u0432 \u0412.\u0412., \u0410\u043d\u0438\u0441\u0438\u043c\u043e\u0432 \u0421.\u0412., \u041f\u043e\u0437\u0434\u043d\u044f\u043a\u043e\u0432\u0430 \u0414.\u0414<\/em>. <\/strong>\u0412\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u0435 \u0438\u0441\u043a\u0443\u0441\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0445 \u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432 \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0430 \u0420\u04411 \u0432 \u044d\u043a\u0441\u043f\u0435\u0440\u0438\u043c\u0435\u043d\u0442\u0435 FENICS-2024: 2. \u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 (Pilipenko V.A., Fedorov E.N., Mazur N.G., Ermakova E.N., Ryabov A.V., Potapov A.S., Marchuk R.A., Kolobov V.V., Anisimov S.V., Pozdnyakova D.D<\/em>. <\/strong>Excitation of global artificial Pc1 signals during FENICS-2024 experiment: 2. Modeling)<\/td>44\u201354<\/td>PDF<\/a><\/strong><\/td>39\u201348<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0431\u044f\u043a\u043e\u0432\u0430 \u0421.\u0415., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u0410.\u042e., \u041a\u0430\u0440\u0438\u043c\u043e\u0432 \u0420.\u0420., \u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432<\/em><\/strong> \u0410.\u0415<\/strong><\/em>.<\/strong> \u0422\u0440\u0435\u043d\u0434\u044b \u043a\u0440\u0438\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u0447\u0430\u0441\u0442\u043e\u0442\u044b \u0441\u043b\u043e\u044f F2 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u0441\u0442\u0430\u043d\u0446\u0438\u0438 \u00ab\u042f\u043a\u0443\u0442\u0441\u043a\u00bb \u0437\u0430 \u043f\u0435\u0440\u0438\u043e\u0434 \u0441 1956 \u043f\u043e 2017 \u0433. (Kobyakova S.E., Gololobov A.Yu., Karimov R.R., Stepanov A.E<\/em>. <\/strong>Trends in the F2-layer critical frequency from data obtained at the ionospheric station Yakutsk during the period from 1956 to 2017)<\/td>55\u201363<\/td>PDF<\/a><\/strong><\/td>49\u201356<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0415., \u0425\u0430\u043b\u0438\u043f\u043e\u0432 \u0412.\u041b<\/em>.<\/strong> \u041f\u043e\u043b\u043e\u0436\u0435\u043d\u0438\u0435 \u043f\u043e\u043b\u044f\u0440\u043d\u043e\u0439 \u0441\u0442\u0435\u043d\u043a\u0438 \u0433\u043b\u0430\u0432\u043d\u043e\u0433\u043e \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043f\u0440\u043e\u0432\u0430\u043b\u0430 \u0432 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u043f\u043e\u043a\u043e\u0439\u043d\u044b\u0445 \u0443\u0441\u043b\u043e\u0432\u0438\u044f\u0445 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u0441\u0442\u0430\u043d\u0446\u0438\u0438 \u00ab\u0422\u0438\u043a\u0441\u0438\u00bb \u0438 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432 DMSP (Stepanov A.E., Khalipov V.L<\/em>.<\/strong> Position of the main ionospheric trough polar wall in magnetically quiet conditions according to data from the ionospheric Tixie Bay station and DMSP satellites)<\/td>64\u201370<\/td>PDF<\/a><\/strong><\/td>57\u201363<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0430\u0440\u043f\u043e\u0432 \u0418.\u0412., \u0411\u0435\u0441\u0441\u0430\u0440\u0430\u0431 \u0424.\u0421., \u0411\u043e\u0440\u0447\u0435\u0432\u043a\u0438\u043d\u0430 \u041e.\u041f<\/em>.<\/strong> \u0427\u0438\u0441\u043b\u0435\u043d\u043d\u043e\u0435 \u043c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0445 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043e\u0442 \u043b\u043e\u043a\u0430\u043b\u044c\u043d\u044b\u0445 \u0442\u0440\u043e\u043f\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u043e\u0432 (Karpov I.V., Bessarab F.S., Borchevkina O.P<\/em>. <\/strong>Numerical modeling of spatial perturbations of the ionosphere from local tropospheric sources)<\/td>71\u201378<\/td>PDF<\/a><\/strong><\/td>64\u201371<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0414\u0435\u043d\u0438\u0441\u0435\u043d\u043a\u043e \u0412.\u0412., \u0420\u043e\u0437\u0430\u043d\u043e\u0432 \u0415.\u0412<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043e\u0431\u043b\u0430\u0447\u043d\u043e\u0441\u0442\u0438  \u043d\u0430 \u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u043e\u0435 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u043f\u0440\u043e\u0432\u043e\u0434\u0438\u043c\u043e\u0441\u0442\u0438 \u0432 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0435 (Denisenko V.V., Rozanov E.V<\/em>. <\/strong>Influence of clouds on spatial distribution of conductivity in the atmosphere)<\/td>79\u201391<\/td>PDF<\/a><\/strong><\/td>72\u201382<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0432\u043e\u0437\u0434\u0430\u0440\u0435\u0432 \u0410.\u042e., \u0423\u0447\u0430\u0439\u043a\u0438\u043d \u0415.\u041e<\/em>.<\/strong> \u041e\u043f\u044b\u0442 \u043c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433\u0430 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e-\u0438\u043d\u0434\u0443\u0446\u0438\u0440\u043e\u0432\u0430\u043d\u043d\u044b\u0445 \u0442\u043e\u043a\u043e\u0432 \u0432 \u044d\u043d\u0435\u0440\u0433\u043e\u0441\u0435\u0442\u0438 \u0420\u0435\u0441\u043f\u0443\u0431\u043b\u0438\u043a\u0438 \u0410\u043b\u0442\u0430\u0439 ()Gvozdarev A.Yu., Uchaikin E.O<\/em>. <\/strong>Experience in monitoring geomagnetically induced currents in the Altai Republic power grid<\/td>92\u2013105<\/td>PDF<\/a><\/strong><\/td>83\u201396<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u043b\u044f\u043a\u043e\u0432 \u0410.\u0420., \u0426\u044d\u0433\u043c\u044d\u0434 \u0411.<\/em> <\/strong>\u0414\u0435\u0442\u0435\u043a\u0442\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0433\u0440\u0443\u043f\u043f \u0441\u043e\u0431\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0445 \u0447\u0430\u0441\u0442\u043e\u0442 \u0432\u0435\u0440\u0442\u0438\u043a\u0430\u043b\u044c\u043d\u044b\u0445 \u0441\u0442\u043e\u044f\u0447\u0438\u0445 \u0432\u043e\u043b\u043d \u0432 \u0441\u043b\u043e\u0438\u0441\u0442\u043e\u0439 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0435 \u0437\u0435\u043c\u043d\u043e\u0439 \u043a\u043e\u0440\u044b (Polyakov A.R., Tsegmed B<\/em>. <\/strong>Detecting groups of eigenfrequencies of vertical standing waves in the layered structure of the Earth\u2019s crust)<\/td>106\u2013113<\/td>PDF<\/a><\/strong><\/td>97\u2013103<\/td>PDF<\/a><\/strong><\/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>
\u041f\u0430\u0432\u043b\u043e\u0432 \u0414.\u0410., \u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411., \u041a\u0430\u043b\u0438\u043d\u0438\u043d \u041c.\u0421., \u041a\u043e\u0434\u0443\u043a\u043e\u0432 \u0410.\u0412., \u0421\u0438 \u041b\u043e, \u0424\u0430\u043d \u0428\u044d\u043d\u044c, \u042e\u0439\u0446\u0437\u0438 \u0427\u0436\u0443.<\/em> <\/strong>\u041c\u0413\u0414-\u043c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u043a\u043e\u0440\u043e\u0442\u0438\u0440\u0443\u044e\u0449\u0438\u0445 \u043e\u0431\u043b\u0430\u0441\u0442\u0435\u0439 \u0432\u0437\u0430\u0438\u043c\u043e\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u044f \u0432 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u0435 \u0441 \u0440\u0430\u0437\u043d\u044b\u043c\u0438 \u0433\u0440\u0430\u043d\u0438\u0447\u043d\u044b\u043c\u0438 \u0443\u0441\u043b\u043e\u0432\u0438\u044f\u043c\u0438 \u0438 \u0440\u0430\u0437\u043d\u044b\u043c\u0438 \u043f\u0440\u043e\u0433\u0440\u0430\u043c\u043c\u043d\u044b\u043c\u0438 \u043f\u0430\u043a\u0435\u0442\u0430\u043c\u0438 (Pavlov D.A., Krainev M.B., Kalinin M.S., Kodukov A.V., Xi Luo, Fang Shen, Yuji Zhu<\/em>. <\/strong>MHD-simulation of corotating interaction regions in the heliosphere using different boundary conditions and codes)<\/td>114\u2013126<\/td>PDF<\/a><\/strong><\/td>104\u2013115<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u0432\u0435\u0440\u0435\u0432 \u0410.\u0421., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u0413., \u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e<\/em>. <\/strong>\u041f\u0440\u043e\u0433\u043d\u043e\u0437 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c \u0432 \u0430\u043f\u0440\u0435\u043b\u0435\u2013\u043d\u043e\u044f\u0431\u0440\u0435 2024 \u0433. \u043f\u043e \u0440\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u0430\u043c \u043c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433\u0430 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Zverev A.S., Grigoryev V.G., Starodubtsev S.A., Gololobov P.Yu<\/em>. <\/strong>Forecast of geomagnetic storms in April\u2013November 2024 based on cosmic ray monitoring results)<\/td>127\u2013131<\/td>PDF<\/a><\/strong><\/td>116\u2013119<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0443\u043a\u043e\u0432 \u0414.\u0410., \u042f\u0433\u043e\u0432\u0430 \u041d.\u0412<\/em>. <\/sup><\/strong>\u0432\u0440\u0435\u043c\u0435\u043d\u043d\u044b\u0435 \u043c\u0430\u0441\u0448\u0442\u0430\u0431\u044b \u043a\u043e\u0433\u0435\u0440\u0435\u043d\u0442\u043d\u043e\u0441\u0442\u0438 \u0434\u043b\u0438\u043d\u043d\u043e\u043f\u0435\u0440\u0438\u043e\u0434\u043d\u044b\u0445 \u0423\u041d\u0427-\u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0439 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0432 \u043e\u043a\u0440\u0435\u0441\u0442\u043d\u043e\u0441\u0442\u0438 \u043d\u043e\u0447\u043d\u043e\u0439 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u043f\u0430\u0443\u0437\u044b (Stukov D.A., Yagova N.V<\/em>.  <\/sup><\/strong>coherence time scales of long-period ULF variations of magnetic field in vicinity of the night-side magnetopause)<\/td>132\u2013142<\/td>PDF<\/a><\/strong><\/td>120\u2013129<\/td>PDF<\/a><\/strong><\/td><\/tr><\/tbody><\/table><\/figure>","protected":false},"excerpt":{"rendered":"

\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. Pp. \u041a\u0438\u0447\u0430\u0442\u0438\u043d\u043e\u0432 \u041b.\u041b. \u041c\u043e\u0434\u0435\u043b\u044c \u043a\u0440\u0443\u043f\u043d\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u0445 \u0442\u0435\u0447\u0435\u043d\u0438\u0439 \u0432 \u043a\u043e\u043d\u0432\u0435\u043a\u0442\u0438\u0432\u043d\u044b\u0445 \u0437\u043e\u043d\u0430\u0445 \u0421\u043e\u043b\u043d\u0446\u0430 \u0438 \u0437\u0432\u0435\u0437\u0434 (Kitchatinov L.L. Large-scale flow model for solar and stellar convection zones) 5\u201316 PDF 3\u201313 PDF \u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u0417\u043e\u043b\u043e\u0442\u0443\u0445\u0438\u043d\u0430 \u041d.\u0410., \u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u0411\u0435\u043b\u0438\u043d\u0441\u043a\u0430\u044f \u0410.\u042e., \u0413\u0440\u043e\u0437\u043e\u0432 \u0412.\u041f., \u041e\u0439\u043d\u0430\u0446 \u0410.\u0412., \u041f\u043e\u0434\u0434\u0435\u043b\u044c\u0441\u043a\u0438\u0439 \u0410.\u0418., \u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0410.\u0412., \u0426\u0435\u0434\u0440\u0438\u043a \u041c.\u0412. \u042d\u0444\u0444\u0435\u043a\u0442\u044b \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 10\u201313 \u043c\u0430\u044f 2024 \u0433. \u0432 […]<\/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-10619","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/10619","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=10619"}],"version-history":[{"count":12,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/10619\/revisions"}],"predecessor-version":[{"id":10659,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/10619\/revisions\/10659"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=10619"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=10619"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=10619"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}