{"id":6112,"date":"2025-01-14T17:32:10","date_gmt":"2025-01-14T17:32:10","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=6112"},"modified":"2025-11-17T07:07:20","modified_gmt":"2025-11-17T07:07:20","slug":"solnechno-zemnaya-fizika-zhurnal-tom-1-%e2%84%961-2015","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-zhurnal-tom-1-%e2%84%961-2015\/","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 1, \u21161, 2015"},"content":{"rendered":"

\u0421\u043e\u0434\u0435\u0440\u0436\u0430\u043d\u0438\u0435<\/h2>\n\n\n\n
\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/td>\u0421\u0442\u0440.<\/strong><\/td><\/td><\/tr>
\u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432 \u0413.\u0410.<\/em><\/strong>\u00a0\u041f\u0440\u0435\u0434\u0438\u0441\u043b\u043e\u0432\u0438\u0435 \u0433\u043b\u0430\u0432\u043d\u043e\u0433\u043e \u0440\u0435\u0434\u0430\u043a\u0442\u043e\u0440\u0430 \u043a \u043f\u0435\u0440\u0432\u043e\u043c\u0443 \u043d\u043e\u043c\u0435\u0440\u0443 \u0436\u0443\u0440\u043d\u0430\u043b\u0430 \u00ab\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u0430\u044f \u0444\u0438\u0437\u0438\u043a\u0430\u00bb (Zherebtsov G.A.<\/em><\/strong>\u00a0Introduction to the first issue of «Solar-Terrestrial Physics» from the Editor-in-Chief)<\/td>3<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041b\u0435\u043e\u043d\u043e\u0432\u0438\u0447 \u0410.\u0421., \u041c\u0430\u0437\u0443\u0440 \u0412.\u0410., \u041a\u043e\u0437\u043b\u043e\u0432 \u0414.\u0410.<\/em><\/strong>\u00a0\u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u044b \u0432 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u043c \u0445\u0432\u043e\u0441\u0442\u0435: \u043e\u0431\u0437\u043e\u0440(Leonovich A.S., Mazur V.A., Kozlov D.A.<\/strong>\u00a0<\/em>MHD waves in the geomagnetic tail: A review)<\/td>4-22<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041b\u0430\u0437\u0443\u0442\u0438\u043d \u041b.\u041b.<\/em><\/strong>\u00a0\u041e\u0432\u0430\u043b \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u0439 \u2014 \u043f\u0440\u0435\u043a\u0440\u0430\u0441\u043d\u0430\u044f, \u043d\u043e \u0443\u0441\u0442\u0430\u0440\u0435\u0432\u0448\u0430\u044f \u043f\u0430\u0440\u0430\u0434\u0438\u0433\u043c\u0430 (Lazutin L.L.<\/em><\/strong>\u00a0Auroral oval as a beautiful but outdated paradigm)<\/td>23-35<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u0430\u0437\u0443\u0440 \u0412.\u0410., \u0427\u0443\u0439\u043a\u043e \u0414.\u0410.<\/em><\/strong>\u00a0\u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0434 \u0432\u043e \u0432\u043d\u0435\u0448\u043d\u0435\u0439 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u0435 \u0438 \u043c\u0435\u0445\u0430\u043d\u0438\u0437\u043c\u044b \u0435\u0433\u043e \u0432\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u044f (Mazur V.A., Chuiko D.A.<\/em><\/strong>\u00a0MHD waveguide in the outermagnetosphere and mechanisms of its excitation)<\/td>36-55<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0414\u0435\u043c\u0438\u043d\u043e\u0432 \u041c.\u0413., \u0414\u0435\u043c\u0438\u043d\u043e\u0432\u0430 \u0413.\u0424., \u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432 \u0413.\u0410., \u041f\u043e\u043b\u0435\u0445 \u041d.\u041c.<\/em><\/strong>\u00a0\u0421\u0432\u043e\u0439\u0441\u0442\u0432\u0430 \u0438\u0437\u043c\u0435\u043d\u0447\u0438\u0432\u043e\u0441\u0442\u0438 \u043a\u043e\u043d\u0446\u0435\u043d\u0442\u0440\u0430\u0446\u0438\u0438 \u043c\u0430\u043a\u0441\u0438\u043c\u0443\u043c\u0430 F2-\u0441\u043b\u043e\u044f \u043d\u0430\u0434 \u0418\u0440\u043a\u0443\u0442\u0441\u043a\u043e\u043c \u043f\u0440\u0438 \u0440\u0430\u0437\u043d\u044b\u0445 \u0443\u0440\u043e\u0432\u043d\u044f\u0445 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Deminov M.G., Deminova G.F., Zherebtsov G.A., Polekh N.M.<\/em><\/strong>\u00a0Properties of the F2-layer maximum density variability over Irkutsk under different levels ofthe solar and geomagnetic activity)<\/td>56-62<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041f\u043e\u043b\u044f\u043a\u043e\u0432\u0430 \u0410.\u0421., \u041f\u0435\u0440\u0435\u0432\u0430\u043b\u043e\u0432\u0430 \u041d.\u041f.<\/em><\/strong>\u00a0\u0421\u0440\u0430\u0432\u043d\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u0439 \u041f\u042d\u0421 \u043d\u0430\u0434 \u0437\u043e\u043d\u0430\u043c\u0438 \u0434\u0435\u0439\u0441\u0442\u0432\u0438\u044f \u0442\u0440\u043e\u043f\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0446\u0438\u043a\u043b\u043e\u043d\u043e\u0432 \u0432 \u0441\u0435\u0432\u0435\u0440\u043e-\u0437\u0430\u043f\u0430\u0434\u043d\u043e\u0439 \u0447\u0430\u0441\u0442\u0438 \u0422\u0438\u0445\u043e\u0433\u043e \u043e\u043a\u0435\u0430\u043d\u0430 (Polyakova A.S.,Perevalova N.P.<\/em><\/strong>\u00a0Comparative analysis of TEC disturbances above regions of tropical cyclonesin the north-west Pacific Ocean)<\/td>63-74<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0425\u043b\u044b\u0441\u0442\u043e\u0432\u0430 \u0410.\u0418.<\/em><\/strong>\u00a0\u0421\u0432\u044f\u0437\u044c \u0434\u043e\u043f\u043b\u0435\u0440\u043e\u0432\u0441\u043a\u0438\u0445 \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0435\u0439 \u0441 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430\u043c\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u043f\u0440\u0438 \u043f\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u0438 \u0430\u043a\u0442\u0438\u0432\u043d\u044b\u0445 \u043e\u0431\u043b\u0430\u0441\u0442\u0435\u0439 \u0432 \u0444\u043e\u0442\u043e\u0441\u0444\u0435\u0440\u0435 \u0421\u043e\u043b\u043d\u0446\u0430 (Khlystova A.I.<\/em><\/strong>\u00a0Relationship betweenplasma flow Doppler velocities and magnetic field parameters during the appearance ofactive regions at the solar photospheric level)<\/td>75-84<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0425\u043b\u044b\u0441\u0442\u043e\u0432\u0430 \u0410.\u0418.<\/em><\/strong>\u00a0\u0413\u043e\u0440\u0438\u0437\u043e\u043d\u0442\u0430\u043b\u044c\u043d\u0430\u044f \u0441\u043e\u0441\u0442\u0430\u0432\u043b\u044f\u044e\u0449\u0430\u044f \u0442\u0435\u0447\u0435\u043d\u0438\u0439 \u0444\u043e\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u043f\u0440\u0438 \u0432\u043e\u0437\u043d\u0438\u043a\u043d\u043e\u0432\u0435\u043d\u0438\u0438 \u0430\u043a\u0442\u0438\u0432\u043d\u044b\u0445 \u043e\u0431\u043b\u0430\u0441\u0442\u0435\u0439 \u043d\u0430 \u0421\u043e\u043b\u043d\u0446\u0435 (Khlystova A.I.<\/em><\/strong>\u00a0Horizontal component ofphotospheric plasma flows during the emergence of active regions on the Sun)<\/td>85-97<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u041b\u0430\u0432\u0440\u043e\u0432 \u0418.\u041f., \u0421\u043e\u0431\u0438\u0441\u0435\u0432\u0438\u0447 \u0410.\u041b.<\/em><\/strong>\u00a0\u0412\u043d\u0435\u0437\u0430\u043f\u043d\u044b\u0435 \u043d\u0430\u0447\u0430\u043b\u0430 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c \u0438 \u0437\u0435\u043c\u043b\u0435\u0442\u0440\u044f\u0441\u0435\u043d\u0438\u044f (Guglielmi \u0410.V., Lavrov I.P., Sobisevich A.L.<\/strong>\u00a0<\/em>Storm sudden commencementsand earthquakes)<\/td>98-103<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0414\u0435\u043d\u0438\u0441\u0435\u043d\u043a\u043e \u0412.\u0412., \u042f\u043a\u0443\u0431\u0430\u0439\u043b\u0438\u043a \u041e.\u042d.<\/strong>\u00a0<\/em>\u0423\u0447\u0435\u0442 \u0440\u0435\u043b\u044c\u0435\u0444\u0430 \u043f\u0440\u0438 \u0432\u044b\u0447\u0438\u0441\u043b\u0435\u043d\u0438\u0438 \u0441\u043e\u043f\u0440\u043e\u0442\u0438\u0432\u043b\u0435\u043d\u0438\u044f \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043f\u0440\u043e\u0432\u043e\u0434\u043d\u0438\u043a\u0430 (Denisenko V.V., Yakubailik O.E.<\/em><\/strong>\u00a0Taking accountof topography when calculating the resistance of the global atmospheric conductor)<\/td>104-108<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u0438\u0447\u0438\u0433\u0438\u043d \u0413.\u041d.<\/em><\/strong>\u00a0\u0423\u0434\u0430\u0440\u043d\u044b\u0435 \u0432\u043e\u043b\u043d\u044b, \u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u043d\u044b\u0435 \u0432\u0437\u0440\u044b\u0432\u0430\u043c\u0438 \u0432 \u043a\u043e\u0441\u043c\u043e\u0441\u0435, \u2014 \u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0441\u0432\u0435\u0440\u0445\u0432\u044b\u0441\u043e\u043a\u0438\u0445 \u044d\u043d\u0435\u0440\u0433\u0438\u0439 (Kichigin G.N.<\/em><\/strong>\u00a0Shock waves raised by explosionsin space as sources of ultra-high-energy cosmic rays)<\/td>109-114<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u0440\u0430\u0432\u0446\u043e\u0432\u0430 \u041c.\u0412., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.\u0415.<\/em><\/strong>\u00a0\u0421\u043f\u0435\u043a\u0442\u0440\u044b \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0439 \u0438 \u0430\u043d\u0438\u0437\u043e\u0442\u0440\u043e\u043f\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432 \u043f\u0435\u0440\u0438\u043e\u0434 GLE 11 \u0438\u044e\u043d\u044f 1991 \u0433. (Kravtsova M.V., Sdobnov V.E.<\/em><\/strong>\u00a0Spectra of variations andcosmic ray anisotropy during GLE of June 11, 1991)<\/td>115-120
<\/td>		PDF<\/strong><\/a><\/td><\/tr>
\u041f\u0430\u043c\u044f\u0442\u0438 \u0412.\u0410. \u041c\u0430\u0437\u0443\u0440\u0430 (In memory of V.A. Mazur)<\/td>121<\/td>PDF<\/strong><\/a><\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

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\u0421\u043e\u0434\u0435\u0440\u0436\u0430\u043d\u0438\u0435 \u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. \u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432 \u0413.\u0410.\u00a0\u041f\u0440\u0435\u0434\u0438\u0441\u043b\u043e\u0432\u0438\u0435 \u0433\u043b\u0430\u0432\u043d\u043e\u0433\u043e \u0440\u0435\u0434\u0430\u043a\u0442\u043e\u0440\u0430 \u043a \u043f\u0435\u0440\u0432\u043e\u043c\u0443 \u043d\u043e\u043c\u0435\u0440\u0443 \u0436\u0443\u0440\u043d\u0430\u043b\u0430 \u00ab\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u0430\u044f \u0444\u0438\u0437\u0438\u043a\u0430\u00bb (Zherebtsov G.A.\u00a0Introduction to the first issue of «Solar-Terrestrial Physics» from the Editor-in-Chief) 3 PDF \u041b\u0435\u043e\u043d\u043e\u0432\u0438\u0447 \u0410.\u0421., \u041c\u0430\u0437\u0443\u0440 \u0412.\u0410., \u041a\u043e\u0437\u043b\u043e\u0432 \u0414.\u0410.\u00a0\u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u044b \u0432 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u043c \u0445\u0432\u043e\u0441\u0442\u0435: \u043e\u0431\u0437\u043e\u0440(Leonovich A.S., Mazur V.A., Kozlov D.A.\u00a0MHD waves in the geomagnetic tail: A review) 4-22 PDF \u041b\u0430\u0437\u0443\u0442\u0438\u043d \u041b.\u041b.\u00a0\u041e\u0432\u0430\u043b \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u0439 […]<\/p>","protected":false},"author":13,"featured_media":0,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[],"tags":[],"class_list":["post-6112","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/6112","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\/13"}],"replies":[{"embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/comments?post=6112"}],"version-history":[{"count":8,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/6112\/revisions"}],"predecessor-version":[{"id":10395,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/6112\/revisions\/10395"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=6112"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=6112"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=6112"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}