{"id":8046,"date":"2025-04-23T03:52:05","date_gmt":"2025-04-23T03:52:05","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8046"},"modified":"2025-10-16T05:33:55","modified_gmt":"2025-10-16T05:33:55","slug":"solnechno-zemnaya-fizika-tom-7-%e2%84%961-2021","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-7-%e2%84%961-2021\/","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 7, \u21161, 2021"},"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>
\u041a\u0443\u0434\u0440\u044f\u0432\u0446\u0435\u0432\u0430 \u0410.\u0412., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418., \u0423\u0440\u0430\u043b\u043e\u0432 \u0410.\u041c., \u0413\u0440\u0435\u0447\u043d\u0435\u0432 \u0412.\u0412<\/em>. <\/strong>\u041c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u044b\u0439 \u0438\u043d\u0434\u0438\u043a\u0430\u0442\u043e\u0440 \u043f\u043e\u0442\u0435\u043d\u0446\u0438\u0430\u043b\u044c\u043d\u043e\u0439 \u0433\u0435\u043e\u044d\u0444\u0444\u0435\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0438 \u0436\u0433\u0443\u0442\u043e\u0432\u0430\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u0430\u044f \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 (Kudriavtseva A.V., Myshyakov I.I., Uralov A.M., Grechnev<\/em>
V.V<\/em>. <\/strong>Microwave indicator of potential geoeffectiveness and magnetic flux-rope structure of a solar active region)<\/td>		3\u201312  <\/td>PDF<\/a><\/strong><\/td>3\u201310<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u043b\u043f\u0430\u043a \u0412.\u0418., \u041c\u043e\u0433\u0438\u043b\u0435\u0432\u0441\u043a\u0438\u0439 \u041c.\u041c., \u0427\u0443\u0433\u0443\u043d\u0438\u043d \u0414.\u0412., \u0427\u0435\u0440\u043d\u044b\u0448\u043e\u0432 \u0410.\u0410., \u041c\u043e\u0438\u0441\u0435\u0435\u043d\u043a\u043e \u0418.\u041b., \u041a\u0443\u043c\u0430\u043c\u043e\u0442\u043e \u0410., \u0422\u0441\u0443\u0447\u0438\u044f \u0424., \u041a\u0430\u0441\u0430\u0445\u0430\u0440\u0430 \u0415., \u0428\u043e\u0439\u0438 \u041c., \u041c\u0438\u0435\u0448\u0438 \u0415., \u0428\u0438\u043d\u043e\u0445\u0430\u0440\u0430 \u0418. <\/em><\/strong>\u0421\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u0441\u0432\u043e\u0439\u0441\u0442\u0432\u0430 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u043a\u0438\u043b\u043e\u043c\u0435\u0442\u0440\u043e\u0432\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u043f\u043e \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f\u043c \u043d\u0430 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u0435 ERG (ARASE) (Kolpak V.I., Mogilevsky M.M., Chugunin D.V., Chernyshov A.A., Moiseenko I.L., Kumamoto A., Tsuchiya F., Kasahara Y., Shoji M., Miyoshi Y., Shinohara I.<\/em> <\/strong>Statistical properties of auroral kilometer radiation: based on ERG (ARASE) satellite data)<\/td>13\u201320 <\/td>PDF<\/a><\/strong><\/td>11\u201316<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0438\u043d\u0435\u0432\u0438\u0447 \u0410.\u0410., \u0427\u0435\u0440\u043d\u044b\u0448\u043e\u0432 \u0410.\u0410., \u0427\u0443\u0433\u0443\u043d\u0438\u043d \u0414.\u0412., \u041c\u0438\u043b\u043e\u0445 \u0412.\u042f., \u041c\u043e\u0433\u0438\u043b\u0435\u0432\u0441\u043a\u0438\u0439 \u041c.\u041c. <\/em><\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u043c\u0435\u043b\u043a\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u043e\u0439 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u044b \u043f\u043e\u043b\u044f\u0440\u0438\u0437\u0430\u0446\u0438\u043e\u043d\u043d\u043e\u0433\u043e \u0434\u0436\u0435\u0442\u0430 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 20 \u0430\u043f\u0440\u0435\u043b\u044f 2018 \u0433. (Sinevich A.A., Chernyshov A.A., Chugunin D.V., Miloch W.J., Mogilevsky<\/em><\/strong> M.M.<\/strong><\/em> <\/strong>Studying the small-scale structure of a polarization jet during the April 20, 2018 geomagnetic storm)<\/td>21\u201333<\/td>PDF<\/a><\/strong><\/td>17\u201326<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0448\u0438\u043d \u0412.\u0412., \u041a\u0430\u0440\u0430\u0432\u0430\u0435\u0432 \u042e.\u0410., \u041b\u0443\u043d\u044e\u0448\u043a\u0438\u043d \u0421.\u0411., \u041f\u0435\u043d\u0441\u043a\u0438\u0445 \u042e.\u0412., \u041a\u0430\u043f\u0443\u0441\u0442\u0438\u043d \u0412.\u042d. <\/em><\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u043f\u0440\u043e\u0434\u043e\u043b\u044c\u043d\u044b\u0445 \u0442\u043e\u043a\u043e\u0432 \u0432 \u0434\u0432\u0443\u0445 \u043f\u043e\u043b\u0443\u0448\u0430\u0440\u0438\u044f\u0445 \u0417\u0435\u043c\u043b\u0438 \u0432 \u0445\u043e\u0434\u0435 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0442\u0435\u0445\u043d\u0438\u043a\u0438 \u0438\u043d\u0432\u0435\u0440\u0441\u0438\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0433\u0440\u0430\u043c\u043c (Mishin V.V., Karavaev Yu.A.,<\/em><\/strong> Silina A.S., Penskikh Yu.V., Kapustin V.E<\/strong><\/em>. <\/strong>Dynamics of field-aligned currents in two hemispheres during a magnetospheric storm from magnetogram inversion technique data)<\/td>34\u201339<\/td>PDF<\/a><\/strong><\/td>27\u201331<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0448\u0438\u043d \u0412.\u0412., \u041c\u0438\u0448\u0438\u043d \u0412.\u041c., \u041a\u0443\u0440\u0438\u043a\u0430\u043b\u043e\u0432\u0430 \u041c.\u0410<\/em>. <\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u0430\u0441\u0438\u043c\u043c\u0435\u0442\u0440\u0438\u0438 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u043f\u0440\u043e\u0434\u043e\u043b\u044c\u043d\u044b\u0445 \u0442\u043e\u043a\u043e\u0432 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0441\u0443\u0431\u0431\u0443\u0440\u044c \u0432 \u0441\u0435\u0437\u043e\u043d \u0440\u0430\u0432\u043d\u043e\u0434\u0435\u043d\u0441\u0442\u0432\u0438\u044f (Mishin V.V., Mishin V.M., Kurikalova M.A<\/em>. <\/strong>Dynamics of the field-aligned currents distribution asymmetry during substorms in the equinox season)<\/td>40\u201350<\/td>PDF<\/a><\/strong><\/td>32\u201340<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041d\u0438\u043a\u043e\u043b\u0430\u0435\u0432\u0430 \u0412.\u0414., \u0413\u043e\u0440\u0434\u0435\u0435\u0432 \u0415.\u0418., \u0420\u043e\u0433\u043e\u0432 \u0414.\u0414., \u041d\u0438\u043a\u043e\u043b\u0430\u0435\u0432 \u0410.\u0412. <\/em><\/strong>\u041a\u0430\u043b\u0438\u0431\u0440\u043e\u0432\u043a\u0430 \u043c\u043e\u0434\u0435\u043b\u0438 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b AIM-E \u0434\u043b\u044f \u0440\u0430\u0441\u0447\u0435\u0442\u0430 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0440\u0435\u0433\u0443\u043b\u044f\u0440\u043d\u043e\u0433\u043e E-\u0441\u043b\u043e\u044f (Nikolaeva V.D., Gordeev E.I., Rogov D.D., Nikolaev<\/em><\/strong> A.V<\/strong><\/em>. <\/strong>AIM-Eauroral ionosphere model adjustment for the regular E layer)<\/td>51\u201358<\/td>PDF<\/a><\/strong><\/td>41\u201346<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0424\u0435\u0434\u043e\u0440\u043e\u0432 \u0420.\u0420., \u0411\u0435\u0440\u043d\u0433\u0430\u0440\u0434\u0442 \u041e.\u0418. <\/em><\/strong>\u041c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433\u043e\u0432\u044b\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u043c\u0435\u0442\u0435\u043e\u0440\u043d\u043e\u0433\u043e \u044d\u0445\u0430 \u043d\u0430 \u0440\u0430\u0434\u0430\u0440\u0435 EKB \u0418\u0421\u0417\u0424 \u0421\u041e \u0420\u0410\u041d: \u0430\u043b\u0433\u043e\u0440\u0438\u0442\u043c\u044b, \u0432\u0430\u043b\u0438\u0434\u0430\u0446\u0438\u044f, \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u043a\u0430 (Fedorov R.R., Berngardt<\/em><\/strong> O.I<\/strong><\/em>. <\/strong>Monitoring observations of meteor echo at the EKB ISTP SB RAS radar: algorithms, validation, statistics)<\/td>59\u201373<\/td>PDF<\/a><\/strong><\/td>47\u201358<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u043e\u0442\u043e\u0432 \u041e.\u0414., \u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u0421\u0438\u043b\u0438\u043d\u0430 \u0410.\u0421<\/em>. <\/strong>\u041e \u0432\u043e\u0437\u043c\u043e\u0436\u043d\u043e\u0439 \u0441\u0432\u044f\u0437\u0438 \u0437\u0435\u043c\u043b\u0435\u0442\u0440\u044f\u0441\u0435\u043d\u0438\u0439 \u0441\u043e \u0441\u043c\u0435\u043d\u043e\u0439 \u0437\u043d\u0430\u043a\u0430 \u0440\u0430\u0434\u0438\u0430\u043b\u044c\u043d\u043e\u0439 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442\u044b \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f (Zotov O.D., Guglielmi A.V., Silina<\/em><\/strong> A.S.<\/strong><\/em> <\/strong>On possible relation of earthquakes with the sign change of the interplanetary magnetic field radial component)<\/td>74\u201383<\/td>PDF<\/a><\/strong><\/td>59\u201366<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u043d\u0447\u0443\u043a\u043e\u0432\u0441\u043a\u0438\u0439 \u0412.\u041b. <\/em><\/strong>\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u0430\u044f \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u044c \u0438 \u0441\u0435\u0439\u0441\u043c\u0438\u0447\u043d\u043e\u0441\u0442\u044c \u0417\u0435\u043c\u043b\u0438 (Yanchukovsky V.L.<\/em> <\/strong>Solar activity and Earth seismicity)<\/td>84\u201397 <\/td>PDF<\/a><\/strong><\/td>67\u201377<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0435\u043b\u0438\u043d\u0441\u043a\u0430\u044f \u0410.\u042e., \u041a\u043e\u0432\u0430\u043b\u0435\u0432 \u0410.\u0410., \u0421\u0435\u043c\u0430\u043a\u043e\u0432 \u041d.\u041d., \u0411\u0435\u043b\u0438\u043d\u0441\u043a\u0430\u044f \u0421.\u0418<\/em>. <\/strong>\u0412\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0411\u0430\u0447\u0430\u0442\u0441\u043a\u043e\u0433\u043e \u0437\u0435\u043c\u043b\u0435\u0442\u0440\u044f\u0441\u0435\u043d\u0438\u044f 18 \u0438\u044e\u043d\u044f 2013 \u0433. (Belinskaya A.Yu., Kovalev A.A., Semakov N.N., Belinskaya S.I.<\/em> <\/strong>Variations of ionospheric and geomagnetic field parameters during the June 18, 2013 Bachat earthquake)<\/td>98\u2013105<\/td>PDF<\/a><\/strong><\/td>78\u201384<\/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\u0443\u0434\u0440\u044f\u0432\u0446\u0435\u0432\u0430 \u0410.\u0412., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418., \u0423\u0440\u0430\u043b\u043e\u0432 \u0410.\u041c., \u0413\u0440\u0435\u0447\u043d\u0435\u0432 \u0412.\u0412. \u041c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u044b\u0439 \u0438\u043d\u0434\u0438\u043a\u0430\u0442\u043e\u0440 \u043f\u043e\u0442\u0435\u043d\u0446\u0438\u0430\u043b\u044c\u043d\u043e\u0439 \u0433\u0435\u043e\u044d\u0444\u0444\u0435\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0438 \u0436\u0433\u0443\u0442\u043e\u0432\u0430\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u0430\u044f \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 (Kudriavtseva A.V., Myshyakov I.I., Uralov A.M., GrechnevV.V. Microwave indicator of potential geoeffectiveness and magnetic flux-rope structure of a solar active region) 3\u201312   PDF 3\u201310 PDF \u041a\u043e\u043b\u043f\u0430\u043a \u0412.\u0418., \u041c\u043e\u0433\u0438\u043b\u0435\u0432\u0441\u043a\u0438\u0439 \u041c.\u041c., \u0427\u0443\u0433\u0443\u043d\u0438\u043d \u0414.\u0412., \u0427\u0435\u0440\u043d\u044b\u0448\u043e\u0432 \u0410.\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-8046","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8046","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=8046"}],"version-history":[{"count":7,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8046\/revisions"}],"predecessor-version":[{"id":9575,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8046\/revisions\/9575"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8046"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8046"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8046"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}