{"id":8066,"date":"2025-04-23T04:06:34","date_gmt":"2025-04-23T04:06:34","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8066"},"modified":"2025-10-24T17:11:11","modified_gmt":"2025-10-24T17:11:11","slug":"solnechno-zemnaya-fizika-tom-9-%e2%84%962-2023","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-9-%e2%84%962-2023\/","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 9, \u21162, 2023"},"content":{"rendered":"
\"\"<\/figure>\n\n\n\n
\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/strong><\/td>\u0421\u0442\u0440.<\/strong><\/td><\/td>Pp.<\/strong><\/td><\/td><\/tr>
\u041a\u0438\u0440\u0438\u0447\u0435\u043d\u043a\u043e \u0410.\u0421., \u041b\u043e\u0431\u043e\u0434\u0430 \u0418.\u041f., \u0420\u0435\u0432\u0430 \u0410.\u0410., \u0423\u043b\u044c\u044f\u043d\u043e\u0432 \u0410.\u0421., \u0411\u043e\u0433\u0430\u0447\u0435\u0432<\/em><\/strong> \u0421.\u0410<\/strong><\/em>. <\/strong>\u0428\u0438\u0440\u043e\u0442\u043d\u044b\u0435 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u043c\u0438\u043a\u0440\u043e\u0432\u0441\u043f\u044b\u0448\u0435\u043a \u0438 \u0432\u044b\u0441\u043e\u043a\u043e\u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u043c\u0438\u043d\u0438\u043c\u0443\u043c\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Kirichenko A.S., Loboda I.P., Reva A.A., Ulyanov A.S., Bogachev S.A<\/em>. <\/strong>Latitude distribution of solar microflares and high-temperature plasma at solar minimum)<\/td>5\u201311<\/td>PDF<\/a><\/strong><\/td>3\u20138<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0422\u0443\u0440\u043e\u0432\u0430 \u0418.\u041f., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432\u0430 \u0421.\u0410., \u041e\u0436\u043e\u0433\u0438\u043d\u0430 \u041e.\u0410.<\/em> <\/strong>\u041b\u0438\u043d\u0438\u0438 CaII \u0432 \u0441\u043f\u043e\u043a\u043e\u0439\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u043d\u0430 \u0421\u043e\u043b\u043d\u0446\u0435.   I. \u0414\u0438\u043d\u0430\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043f\u0440\u043e\u0446\u0435\u0441\u0441\u044b \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0435 (Turova I.P., Grigoryeva S.A., Ozhogina O.A<\/em>. <\/strong>CAII lines in a quiet region on the Sun. I. Dynamic processes in the solar atmosphere)<\/td>12\u201325<\/td>PDF<\/a><\/strong><\/td>9\u201321<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432 \u0410.\u0412., \u0421\u043e\u043b\u043e\u0432\u044c\u0435\u0432 \u0410.\u0410., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432\u0430 \u0413.\u0420., \u0413\u0430\u0439\u043d\u0435\u0442\u0434\u0438\u043d\u043e\u0432\u0430 \u0410.\u0410., \u041b\u0430\u043f\u0438\u043d \u0410.\u041d., \u0411\u0435\u043b\u0430\u0445\u043e\u0432\u0441\u043a\u0438\u0439 \u0412.\u0411., \u0420\u043e\u043b\u0434\u0443\u0433\u0438\u043d \u0410.\u0412<\/em>. <\/strong>\u041b\u043e\u043a\u0430\u043b\u044c\u043d\u0430\u044f \u0434\u0438\u0430\u0433\u043d\u043e\u0441\u0442\u0438\u043a\u0430 \u043d\u0430\u043b\u0438\u0447\u0438\u044f \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u0439 \u043d\u0430 \u043e\u0441\u043d\u043e\u0432\u0435 \u0438\u043d\u0442\u0435\u043b\u043b\u0435\u043a\u0442\u0443\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0430\u043d\u0430\u043b\u0438\u0437\u0430 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0434\u0430\u043d\u043d\u044b\u0445 (Vorobev \u0410.V., Soloviev \u0410.\u0410., Pilipenko V.\u0410., Vorobeva G.R., Gainetdinova A.A., Lapin A.N., Belakhovsky V.B., Roldugin<\/em><\/strong> A.V<\/strong><\/em>. <\/strong>Local diagnostics of aurora presence based on intelligent analysis of geomagnetic <\/strong>dat\u0430)<\/td>26\u201334<\/td>PDF<\/a><\/strong><\/td>22\u201330<\/td>PDF<\/a><\/strong><\/td><\/tr>
Namuun B., Tsegmed B., Li L.Y., Leghari<\/em><\/strong> G.M<\/strong><\/em>. <\/strong>Differences in the response to CME and CIR drivers of geomagnetic disturbances<\/td>35\u201340<\/td>PDF<\/a><\/strong><\/td>31\u201336<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0430\u043b\u0430\u0431\u0438\u043d \u042e.\u0412., \u0413\u0435\u0440\u043c\u0430\u043d\u0435\u043d\u043a\u043e \u0410.\u0412., \u0413\u0432\u043e\u0437\u0434\u0435\u0432\u0441\u043a\u0438\u0439 \u0411.\u0411., \u041c\u0430\u0443\u0440\u0447\u0435\u0432 \u0415.\u0410., \u041c\u0438\u0445\u0430\u043b\u043a\u043e<\/em><\/strong> \u0415.\u0410<\/strong><\/em>. <\/strong>\u0421\u0432\u044f\u0437\u0430\u043d\u043d\u044b\u0435 \u0441 \u043e\u0441\u0430\u0434\u043a\u0430\u043c\u0438 \u0441\u043e\u0431\u044b\u0442\u0438\u044f \u0432\u043e\u0437\u0440\u0430\u0441\u0442\u0430\u043d\u0438\u044f \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442\u044b \u0432\u0442\u043e\u0440\u0438\u0447\u043d\u044b\u0445 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439: \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0435 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u044f \u0438 \u0430\u043d\u0430\u043b\u0438\u0437 (Balabin Yu.V., Germanenko A.V., Gvozdevsky B.B., Maurchev E.A., Michalko E.A.<\/em> <\/strong>Precipitation-related increase events of the electromagnetic component of secondary cosmic rays: Spectral analysis)<\/td>41\u201351<\/td>PDF<\/a><\/strong><\/td>37\u201347<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u043a\u0441\u0438\u043c\u043e\u0432 \u0414.\u0421., \u041a\u043e\u0433\u043e\u0433\u0438\u043d \u0414.\u0410., \u041d\u0430\u0441\u044b\u0440\u043e\u0432 \u0418.\u0410., \u0417\u0430\u0433\u0440\u0435\u0442\u0434\u0438\u043d\u043e\u0432 \u0420.\u0412<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u0435\u043a 5\u201312 \u0441\u0435\u043d\u0442\u044f\u0431\u0440\u044f 2017 \u0433. \u043d\u0430 \u0440\u0435\u0433\u0438\u043e\u043d\u0430\u043b\u044c\u043d\u0443\u044e \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0441\u0442\u044c \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0417\u0435\u043c\u043b\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0413\u041d\u0421\u0421-\u0441\u0442\u0430\u043d\u0446\u0438\u0439, \u0440\u0430\u0441\u043f\u043e\u043b\u043e\u0436\u0435\u043d\u043d\u044b\u0445 \u0432 \u041f\u0440\u0438\u0432\u043e\u043b\u0436\u0441\u043a\u043e\u043c \u0444\u0435\u0434\u0435\u0440\u0430\u043b\u044c\u043d\u043e\u043c \u043e\u043a\u0440\u0443\u0433\u0435 \u0420\u043e\u0441\u0441\u0438\u0439\u0441\u043a\u043e\u0439 \u0424\u0435\u0434\u0435\u0440\u0430\u0446\u0438\u0438 (Maksimov D.S., Kogogin D.A., Nasyrov I.A., Zagretdinov R.V<\/em>. <\/strong>Effects of September 5\u201312, 2017 solar flares on regional disturbance of Earth\u2019s ionosphere as recorded by GNSS stations located in the Volga Federal District of the Russian Federation)<\/td>52\u201359<\/td>PDF<\/a><\/strong><\/td>48\u201354<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u043d\u0447\u0443\u043a\u043e\u0432\u0441\u043a\u0438\u0439 \u0412.\u041b.<\/em> <\/strong>\u0422\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u043d\u044b\u0439 \u044d\u0444\u0444\u0435\u043a\u0442 \u043c\u044e\u043e\u043d\u043e\u0432, \u0440\u0435\u0433\u0438\u0441\u0442\u0440\u0438\u0440\u0443\u0435\u043c\u044b\u0445 \u043f\u043e\u0434 \u0437\u0435\u043c\u043b\u0435\u0439 \u0432 \u042f\u043a\u0443\u0442\u0441\u043a\u0435 \u0441 \u043f\u043e\u043c\u043e\u0449\u044c\u044e \u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f\u043e\u0432 \u043d\u0430 \u0433\u0430\u0437\u043e\u0440\u0430\u0437\u0440\u044f\u0434\u043d\u044b\u0445 \u0441\u0447\u0435\u0442\u0447\u0438\u043a\u0430\u0445 (Yanchukovsky V.L<\/em>. <\/strong>Temperature effect of muons registered under the ground in Yakutsk by telescopes on GAS-discharge counters)<\/td>60\u201370<\/td>PDF<\/a><\/strong><\/td>55\u201365<\/td>PDF<\/a><\/strong><\/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<\/em>. <\/strong>\u0421\u043f\u043e\u043a\u043e\u0439\u043d\u0430\u044f \u043a\u043e\u0440\u043e\u043d\u0430 \u0421\u043e\u043b\u043d\u0446\u0430: \u0435\u0436\u0435\u0434\u043d\u0435\u0432\u043d\u044b\u0435 \u0438\u0437\u043e\u0431\u0440\u0430\u0436\u0435\u043d\u0438\u044f \u043d\u0430 \u0434\u043b\u0438\u043d\u0430\u0445 \u0432\u043e\u043b\u043d 8.8\u201310.7 \u0441\u043c (Altyntsev A.T., Globa M.V., Meshalkina N.S<\/em>. <\/strong>Quiet solar corona: daily images at 8.8\u201310.7 cm wavelengths)<\/td>71\u201377<\/td>PDF<\/a><\/strong><\/td>66\u201372<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410., \u0417\u0432\u0435\u0440\u0435\u0432 \u0410.\u0421., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u0413<\/em>. <\/strong>\u0424\u043b\u0443\u043a\u0442\u0443\u0430\u0446\u0438\u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0438 \u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u044b \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u043c \u0432\u0435\u0442\u0440\u0435 (Starodubtsev S.A., Zverev A.S., Gololobov P.Yu., Grigoryev V.G<\/em>. <\/strong>Cosmic ray fluctuations and MHD waves in the solar wind)<\/td>78\u201385<\/td>PDF<\/a><\/strong><\/td>73\u201380<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0414\u0430\u043d\u0438\u043b\u043e\u0432\u0430 \u041e.\u0410.,<\/em> \u041f\u0442\u0438\u0446\u044b\u043d\u0430 \u041d.\u0413., \u0422\u044f\u0441\u0442\u043e \u041c.\u0418., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.E.<\/em><\/strong> \u0418\u0437\u043c\u0435\u043d\u0435\u043d\u0438\u044f \u0436\u0435\u0441\u0442\u043a\u043e\u0441\u0442\u0435\u0439 \u043e\u0431\u0440\u0435\u0437\u0430\u043d\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0431\u0443\u0440\u0438 8\u201311 \u043c\u0430\u0440\u0442\u0430 2012 \u0433. \u0432 \u043f\u0435\u0440\u0438\u043e\u0434 CAWSES-II (Danilova O.A., Ptitsyna N.G., Tyasto M.I., Sdobnov V.E.<\/em><\/strong> Variations in cosmic ray cutoff rigidities during the March 8\u201311, 2012 magnetic storm (CAWSES II period))<\/td>86\u201393<\/td>PDF<\/a><\/strong><\/td>81\u201387<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0435\u0442\u0443\u0445\u043e\u0432\u0430 \u0410.\u0421., \u041f\u0435\u0442\u0443\u0445\u043e\u0432 \u0418.\u0421., \u041f\u0435\u0442\u0443\u0445\u043e\u0432 \u0421.\u0418., \u0413\u043e\u0442\u043e\u0432\u0446\u0435\u0432 \u0418.\u0421. <\/em><\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0434\u0438\u043d\u0430\u043c\u0438\u043a\u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0441\u0440\u0435\u0434\u044b \u0438 \u043f\u043b\u043e\u0442\u043d\u043e\u0441\u0442\u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432 \u0441\u0438\u043b\u044c\u043d\u044b\u0445 \u0444\u043e\u0440\u0431\u0443\u0448-\u043f\u043e\u043d\u0438\u0436\u0435\u043d\u0438\u044f\u0445, \u0441\u0432\u044f\u0437\u0430\u043d\u043d\u044b\u0445 \u0441 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u043c\u0438 \u043e\u0431\u043b\u0430\u043a\u0430\u043c\u0438 (Petukhova A.S., Petukhov I.S., Petukhov S.I., Gotovtsev I.S.<\/em><\/strong> Peculiarities of medium parameter dynamics and cosmic ray density in strong Forbush decreases associated with magnetic clouds)<\/td>94\u2013100<\/td>PDF<\/a><\/strong><\/td>88\u201393<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u0438\u0441\u043e\u0432\u0430 \u0422.\u0414., \u0411\u043b\u0430\u0433\u043e\u0432\u0435\u0449\u0435\u043d\u0441\u043a\u0430\u044f \u041d.\u0424., \u041a\u0430\u043b\u0438\u0448\u0438\u043d \u0410.C<\/em>. <\/strong>\u0421\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0435 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0438 \u043f\u043b\u0430\u0437\u043c\u0435\u043d\u043d\u044b\u0445 \u0432\u043e\u043b\u043d \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043f\u0440\u0438 \u0432\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u0438 \u043c\u043e\u0449\u043d\u044b\u043c\u0438 \u041a\u0412-\u0440\u0430\u0434\u0438\u043e\u0432\u043e\u043b\u043d\u0430\u043c\u0438 \u043d\u0430 \u0447\u0430\u0441\u0442\u043e\u0442\u0430\u0445 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0432\u0431\u043b\u0438\u0437\u0438 \u0433\u0438\u0440\u043e\u0433\u0430\u0440\u043c\u043e\u043d\u0438\u043a \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u0438 \u043a\u0440\u0438\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u0447\u0430\u0441\u0442\u043e\u0442\u044b \u0441\u043b\u043e\u044f F2 (Borisova T.D., Blagoveshchenskaya N.F., Kalishin A.S<\/em>.<\/strong> Spectral features of ionospheric plasma waves excited by powerful HF radio waves radiated at frequencies near electron gyroharmonics and F2-layer critical frequency)<\/td>101\u2013110<\/td>PDF<\/a><\/strong><\/td>94\u2013102<\/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> \u042d\u043b\u0435\u043a\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0439 \u043f\u043e\u0442\u0435\u043d\u0446\u0438\u0430\u043b \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u2014 \u0430\u043b\u044c\u0442\u0435\u0440\u043d\u0430\u0442\u0438\u0432\u043d\u044b\u0439 \u0438\u043d\u0434\u0438\u043a\u0430\u0442\u043e\u0440 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u044f \u043d\u0430 \u043d\u0438\u0436\u043d\u044e\u044e \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0443 (Karakhanyan A.A., Molodykh S.I.<\/em><\/strong> Ionospheric electric potential as an alternative indicator of solar effect on the lower atmosphere)<\/td>111\u2013115<\/td>PDF<\/a><\/strong><\/td>103\u2013106<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0430\u043c\u044f\u0442\u0438 \u0410\u043d\u0430\u0442\u043e\u043b\u0438\u044f \u0421\u0435\u0440\u0433\u0435\u0435\u0432\u0438\u0447\u0430 \u041b\u0435\u043e\u043d\u043e\u0432\u0438\u0447\u0430 (In memory of Anatoly S. Leonovich)<\/td>116<\/td>PDF<\/a><\/strong><\/td>107<\/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. \ufeff Pp. \ufeff \u041a\u0438\u0440\u0438\u0447\u0435\u043d\u043a\u043e \u0410.\u0421., \u041b\u043e\u0431\u043e\u0434\u0430 \u0418.\u041f., \u0420\u0435\u0432\u0430 \u0410.\u0410., \u0423\u043b\u044c\u044f\u043d\u043e\u0432 \u0410.\u0421., \u0411\u043e\u0433\u0430\u0447\u0435\u0432 \u0421.\u0410. \u0428\u0438\u0440\u043e\u0442\u043d\u044b\u0435 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u043c\u0438\u043a\u0440\u043e\u0432\u0441\u043f\u044b\u0448\u0435\u043a \u0438 \u0432\u044b\u0441\u043e\u043a\u043e\u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u043c\u0438\u043d\u0438\u043c\u0443\u043c\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Kirichenko A.S., Loboda I.P., Reva A.A., Ulyanov A.S., Bogachev S.A. Latitude distribution of solar microflares and high-temperature plasma at solar minimum) 5\u201311 PDF 3\u20138 PDF \u0422\u0443\u0440\u043e\u0432\u0430 \u0418.\u041f., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432\u0430 \u0421.\u0410., […]<\/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-8066","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8066","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=8066"}],"version-history":[{"count":11,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8066\/revisions"}],"predecessor-version":[{"id":9713,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8066\/revisions\/9713"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8066"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8066"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8066"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}