{"id":8034,"date":"2025-04-23T00:28:28","date_gmt":"2025-04-23T00:28:28","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8034"},"modified":"2025-10-31T05:09:59","modified_gmt":"2025-10-31T05:09:59","slug":"solnechno-zemnaya-fizika-tom-5-%e2%84%964-2019","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-5-%e2%84%964-2019\/","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 5, \u21164, 2019"},"content":{"rendered":"
\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/td>\u0421\u0442\u0440.<\/strong><\/td><\/td>Pp.<\/strong><\/td><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410<\/em>. <\/strong>\u041f\u0440\u043e\u0446\u0435\u0441\u0441\u044b \u044d\u043d\u0435\u0440\u0433\u043e\u0432\u044b\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u043a\u0430\u0445 \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 (Borovik A.V., Zhdanov A.A<\/em>. <\/strong>Processes of energy release in low-power solar flares)<\/td>3\u201311<\/td>PDF<\/a><\/strong><\/td>3-9<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411.<\/em> <\/strong>\u041f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u044f \u0432 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u0435 \u0438 \u0432 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0413\u041a\u041b \u0434\u0432\u0443\u0445 \u0432\u0435\u0442\u0432\u0435\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Krainev M.B.<\/em><\/strong> Manifestations of two branches of solar activity in the heliosphere and GCR intensity)<\/td>12\u201325<\/td>PDF<\/a><\/strong><\/td>10-20<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0418\u0432\u0430\u043d\u043e\u0432 \u0415.\u0424., \u0413\u0443\u0431\u0438\u043d \u0410.\u0412., \u041b\u0435\u0441\u043e\u0432\u043e\u0439 \u0421.\u0412., \u0420\u0430\u043c\u0437\u0435\u0441 \u0421\u0430\u043b\u044c\u0434\u0438\u0432\u0430\u0440 \u042d\u0441\u0442\u0440\u0430\u0434\u0430.<\/em> <\/strong>\u041f\u0440\u043e\u0435\u043a\u0442 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0441\u043f\u0435\u043a\u0442\u0440\u043e\u043f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0430 \u0434\u043b\u044f \u043f\u0440\u043e\u0433\u043d\u043e\u0437\u0430 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043f\u043e\u0433\u043e\u0434\u044b (Ivanov E.F., Gubin A.V., Lesovoi S.V., Ramses Zaldivar Estrada.<\/em> <\/strong>Solar spectropolarimeter for space weather forecast)<\/td>26\u201333<\/td>PDF<\/a><\/strong><\/td>21-26<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0424\u0435\u0434\u043e\u0442\u043e\u0432\u0430 \u0410.\u042e., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041a\u043e\u0447\u0430\u043d\u043e\u0432 \u0410.\u0410., \u041b\u0435\u0441\u043e\u0432\u043e\u0439 \u0421.\u0412., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421.<\/em><\/strong> \u041e \u043a\u0430\u043b\u0438\u0431\u0440\u043e\u0432\u043a\u0435 \u0438\u0437\u043e\u0431\u0440\u0430\u0436\u0435\u043d\u0438\u0439 \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u0430 (Fedotova A.Yu., Altyntsev A.T.,<\/em><\/strong> Kochanov A.A.,<\/strong> Lesovoi S.V., Meshalkina<\/strong> N.S.<\/strong><\/em> <\/strong>Calibration of Siberian Radioheliograph images)<\/td>34\u201341<\/td>PDF<\/a><\/strong><\/td>27-33<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0430\u0440\u0445\u043e\u043c\u043e\u0432 \u0412.\u0410., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u0412.\u0413., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u041c.\u0412., \u0414\u043c\u0438\u0442\u0440\u0438\u0435\u0432 \u0410.\u0412., \u0412\u0435\u0434\u0435\u0440\u043d\u0438\u043a\u043e\u0432\u0430 \u0422.\u0418<\/em>. <\/strong>\u0414\u0438\u0430\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u043f\u043b\u0430\u0437\u043c\u043e\u0438\u0434\u044b \u043a\u0430\u043a \u0441\u043e\u0441\u0442\u0430\u0432\u043d\u0430\u044f \u0447\u0430\u0441\u0442\u044c \u0434\u0438\u0430\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440 \u043c\u0435\u0434\u043b\u0435\u043d\u043d\u043e\u0433\u043e \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u0438 \u0438\u0445 \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435 \u043d\u0430 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u0443 <\/strong>(Parkhomov V.A., Eselevich V.G., Eselevich \u041c.V., Dmitriev A.V., Vedernikova T.I.<\/em> <\/strong>Diamagnetic plasmoids as part of diamagnetic structures of the slow solar wind and their impact on Earth\u2019s magnetosphere)<\/td>42\u201354<\/td>PDF<\/a><\/strong><\/td>34-45<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u043e\u0442\u043e\u0432 \u041e.\u0414., \u041a\u043b\u0430\u0439\u043d \u0411.\u0418., \u041a\u0443\u0440\u0430\u0436\u043a\u043e\u0432\u0441\u043a\u0430\u044f \u041d.\u0410<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430 b \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u043d\u0430 \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0438 A<\/em>p<\/sub>-\u0438\u043d\u0434\u0435\u043a\u0441\u0430 \u0432 \u0446\u0438\u043a\u043b\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Zotov O.D., Klain B.I., Kurazhkovskaya N.A.<\/em> <\/strong>Influence of the b solar wind parameter on statistical characteristics of the A<\/em>p<\/sub> index in the solar activity cycle)<\/td>55\u201363<\/td>PDF<\/a><\/strong><\/td>46-52<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0432\u0430\u043b\u044c \u0410.\u0412.<\/em><\/strong> \u0421\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0438 \u0437\u043d\u0430\u0447\u0438\u043c\u044b\u0435 \u043e\u0446\u0435\u043d\u043a\u0438 \u0432\u043b\u0438\u044f\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043d\u0430 \u043f\u043b\u0430\u043d\u0435\u0442\u0430\u0440\u043d\u044b\u0435 \u0432\u043e\u043b\u043d\u044b \u0432 \u0441\u0440\u0435\u0434\u043d\u0435\u0439 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0435 \u0421\u0435\u0432\u0435\u0440\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u0443\u0448\u0430\u0440\u0438\u044f \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043c\u043e\u0434\u0435\u043b\u0438 \u041c\u0421\u0412\u0410 (Koval A.V.<\/em><\/strong> Statistically significant estimates of influence of solar activity on planetary waves in the middle atmosphere of the Northern Hemisphere as derived from MUAM model data)<\/td>64\u201372<\/td>PDF<\/a><\/strong><\/td>53-59<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0415., \u041a\u043e\u0431\u044f\u043a\u043e\u0432\u0430 \u0421.\u0415., \u0425\u0430\u043b\u0438\u043f\u043e\u0432 \u0412.\u041b<\/em>. <\/strong>\u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0435 \u0431\u044b\u0441\u0442\u0440\u044b\u0445 \u0441\u0443\u0431\u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0434\u0440\u0435\u0439\u0444\u043e\u0432 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u042f\u043a\u0443\u0442\u0441\u043a\u043e\u0439 \u043c\u0435\u0440\u0438\u0434\u0438\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0439 \u0446\u0435\u043f\u043e\u0447\u043a\u0438 \u0441\u0442\u0430\u043d\u0446\u0438\u0439 (Stepanov A.E., Kobyakova S.E., Khalipov V.L.<\/em> <\/strong>Fast subauroral drifts of ionospheric plasma according to data from Yakut meridional chain of stations)<\/td>73\u201379<\/td>PDF<\/a><\/strong><\/td>60-65<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412<\/em>. <\/strong>\u0421\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u044b\u0435 \u0441\u0438\u044f\u043d\u0438\u044f \u0432 23\u201324-\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0446\u0438\u043a\u043b\u0430\u0445 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0439 \u043d\u0430 \u044e\u0433\u0435 \u0412\u043e\u0441\u0442\u043e\u0447\u043d\u043e\u0439 \u0421\u0438\u0431\u0438\u0440\u0438 (Mikhalev A.V<\/em>. <\/strong>Mid-latitude aurora in solar cycles 23\u201324 from observations in the south of Eastern Siberia)<\/td>80\u201389<\/td>PDF<\/a><\/strong><\/td>66-73<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u0440\u0442\u0438\u043d\u0435\u0441-\u0411\u0435\u0434\u0435\u043d\u043a\u043e \u0412.\u0410., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0417\u0430\u0445\u0430\u0440\u043e\u0432 \u0412.\u0418., \u0413\u0440\u0443\u0448\u0438\u043d \u0412.\u0410<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u0442\u0430\u0439\u0444\u0443\u043d\u0430 Vongfong 2014 \u0433. \u043d\u0430 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0443 \u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0435 \u043f\u043e\u043b\u0435 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432 Swarm: 2. \u0413\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f (Martines-Bedenko V.A.,<\/em><\/strong> Pilipenko V.A., Zakharov<\/strong> V.I., Grushin<\/strong> V.A<\/strong><\/em>. <\/strong>Influence of the Vongfong 2014 hurricane on the ionosphere and geomagnetic field as detected by SWARM satellites: 2. Geomagnetic disturbances)<\/td>90\u201398<\/td>PDF<\/a><\/strong><\/td>74-80<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0410\u0445\u043c\u0435\u0442\u043e\u0432 \u041e.\u0418., \u041c\u0438\u043d\u0433\u0430\u043b\u0435\u0432 \u0418.\u0412., \u041c\u0438\u043d\u0433\u0430\u043b\u0435\u0432 \u041e.\u0412., \u0421\u0443\u0432\u043e\u0440\u043e\u0432\u0430 \u0417.\u0412., \u0411\u0435\u043b\u0430\u0445\u043e\u0432\u0441\u043a\u0438\u0439 \u0412.\u0411., \u0427\u0435\u0440\u043d\u044f\u043a\u043e\u0432<\/em><\/strong> \u0421.\u041c.<\/strong><\/em> <\/strong>\u041e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a \u0418\u041d\u0427-\u0432\u043e\u043b\u043d, \u043d\u0430\u0438\u0431\u043e\u043b\u0435\u0435 \u0441\u0438\u043b\u044c\u043d\u043e \u0440\u0435\u0430\u0433\u0438\u0440\u0443\u044e\u0449\u0438\u0445 \u043d\u0430 \u043d\u0435\u0437\u043d\u0430\u0447\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0435 \u0438\u0437\u043c\u0435\u043d\u0435\u043d\u0438\u044f \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043d\u043e\u0439 \u043f\u043b\u043e\u0442\u043d\u043e\u0441\u0442\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u0432\u044b\u0441\u043e\u043a\u0438\u0445 \u0448\u0438\u0440\u043e\u0442 (Akhmetov O.I.,<\/em><\/strong> Mingalev I.V., Mingalev O.V., Suvorova Z.V., Belakhovsky V.B., Chernyakov S.M<\/strong><\/em>. <\/strong>Determination of ULF-wave characteristics most strongly reacting to minor changes of ionospheric electron density in a high-latitude region)<\/td>99\u2013109<\/td>PDF<\/a><\/strong><\/td>81-90<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0443\u043a\u0430\u0448\u0435\u0432\u0430 \u0421.\u041d., \u041a\u0430\u043f\u044b\u0442\u0438\u043d \u0412.\u0418., \u041c\u0430\u043b\u0438\u043c\u0431\u0430\u0435\u0432 \u0410.\u041c<\/em>. <\/strong>\u0412\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043d\u0430\u0434 \u0410\u043b\u043c\u0430-\u0410\u0442\u043e\u0439 (\u041a\u0430\u0437\u0430\u0445\u0441\u0442\u0430\u043d) \u0432 1999\u20132013 \u0433\u0433. (Mukasheva S.N., Kapytin V.I.<\/em><\/strong>, Malimbayev A.M<\/strong><\/em>. <\/strong>Variations of ionospheric parameters over Almaty (Kazakhstan) in 1999\u20132013)<\/td>110\u2013116<\/td>PDF<\/a><\/strong><\/td>91-96<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0440\u043e\u0431\u0446\u0435\u0432 \u0418.\u0412., \u041c\u0438\u0448\u0438\u043d\u0430 \u041c.\u041d<\/em>. <\/strong>\u041e\u043f\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u043c\u0430\u043b\u044b\u0445 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0430\u043f\u043f\u0430\u0440\u0430\u0442\u043e\u0432 \u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043c\u0443\u0441\u043e\u0440\u0430 \u0432 \u0421\u0430\u044f\u043d\u0441\u043a\u043e\u0439 \u043e\u0431\u0441\u0435\u0440\u0432\u0430\u0442\u043e\u0440\u0438\u0438 \u0418\u0421\u0417\u0424 \u0421\u041e \u0420\u0410\u041d (Korobtsev I.V., Mishina M.N.<\/em> <\/strong>Optical observations of small spacecraft and space debris at ISTP SB RAS Sayan Observatory)<\/td>117\u2013121<\/td>PDF<\/a><\/strong><\/td>97-100<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0410.\u0412., \u041d\u0430\u0443\u043c\u0435\u043d\u043a\u043e \u0410.\u0410., \u0426\u0435\u0434\u0440\u0438\u043a \u041c.\u0412.<\/em> <\/strong>\u041e\u0446\u0435\u043d\u043a\u0430 \u043a\u043e\u044d\u0444\u0444\u0438\u0446\u0438\u0435\u043d\u0442\u0430 \u0441\u0432\u044f\u0437\u0438 \u0430\u043d\u0442\u0435\u043d\u043d \u043f\u0440\u0438 \u0438\u0441\u043f\u043e\u043b\u044c\u0437\u043e\u0432\u0430\u043d\u0438\u0438 \u043d\u0435\u043f\u0440\u0435\u0440\u044b\u0432\u043d\u044b\u0445 \u041b\u0427\u041c-\u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432 \u0432 \u0443\u0441\u0442\u0430\u043d\u043e\u0432\u043a\u0430\u0445 \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0432\u043d\u0435\u0448\u043d\u0435\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b (Podlesnyi A.V.,<\/em><\/strong> Naumenko A.A., Cedrik M.V.<\/strong><\/em> <\/strong>Estimating antenna coupling factor for problem of topside ionosphere sounding from space with using chirp signals)<\/td>122\u2013129<\/td>PDF<\/a><\/strong><\/td>101-107<\/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. \u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410. \u041f\u0440\u043e\u0446\u0435\u0441\u0441\u044b \u044d\u043d\u0435\u0440\u0433\u043e\u0432\u044b\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u043a\u0430\u0445 \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 (Borovik A.V., Zhdanov A.A. Processes of energy release in low-power solar flares) 3\u201311 PDF 3-9 PDF \u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411. \u041f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u044f \u0432 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u0435 \u0438 \u0432 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0413\u041a\u041b \u0434\u0432\u0443\u0445 \u0432\u0435\u0442\u0432\u0435\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Krainev M.B. Manifestations of two branches of solar activity in the heliosphere […]<\/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-8034","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8034","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=8034"}],"version-history":[{"count":6,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8034\/revisions"}],"predecessor-version":[{"id":9909,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8034\/revisions\/9909"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8034"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8034"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8034"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}