{"id":8024,"date":"2025-04-23T00:23:11","date_gmt":"2025-04-23T00:23:11","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8024"},"modified":"2025-11-01T01:09:38","modified_gmt":"2025-11-01T01:09:38","slug":"solnechno-zemnaya-fizika-tom-4-%e2%84%964-2018","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-4-%e2%84%964-2018\/","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 4, \u21164, 2018"},"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>
\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<\/em><\/strong> \u041e.\u0410.<\/strong><\/em> <\/strong>\u041f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0435 \u0438 \u0432\u0440\u0435\u043c\u0435\u043d\u043d\u044b\u0435 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0444\u043e\u0440\u043c\u044b \u043a\u043e\u043d\u0442\u0443\u0440\u043e\u0432 \u043b\u0438\u043d\u0438\u0438 K Ca II \u0432 \u0440\u0430\u0437\u043b\u0438\u0447\u043d\u044b\u0445 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u043d\u044b\u0445 \u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u0438\u044f\u0445 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0445\u0440\u043e\u043c\u043e\u0441\u0444\u0435\u0440\u044b. I. \u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0438\u043d\u0434\u0438\u0432\u0438\u0434\u0443\u0430\u043b\u044c\u043d\u044b\u0445 \u043a\u043e\u043d\u0442\u0443\u0440\u043e\u0432 (Turova I.P., Grigoryeva S.A., Ozhogina<\/em><\/strong> O.A. <\/strong>Spatial and temporal variations of Ca II K line profile shapes in different structures of solar chromosphere. I. Features of individual profiles)<\/td>3\u201313<\/td>PDF<\/a><\/strong><\/td>3\u201311<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0427\u0435\u043b\u043f\u0430\u043d\u043e\u0432 \u0410.\u0410., \u0427\u0435\u043b\u043f\u0430\u043d\u043e\u0432 \u041c.\u0410., \u041a\u043e\u0431\u0430\u043d\u043e\u0432 \u041d.\u0418., \u0421\u043e\u0442\u043d\u0438\u043a\u043e\u0432\u0430<\/em><\/strong> \u0420.\u0422.<\/strong><\/em> <\/strong>\u0421\u0440\u0430\u0432\u043d\u0435\u043d\u0438\u0435 \u043e\u0441\u043d\u043e\u0432\u043d\u044b\u0445 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a \u043a\u043e\u043b\u0435\u0431\u0430\u043d\u0438\u0439 \u0445\u0440\u043e\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0421\u043e\u043b\u043d\u0446\u0430 \u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b \u043f\u043e \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f\u043c, \u0432\u044b\u043f\u043e\u043b\u043d\u0435\u043d\u043d\u044b\u043c \u0432 \u0418\u0421\u0417\u0424 \u0421\u041e \u0420\u0410\u041d (Chelpanov A.A., Chelpanov M.A., Kobanov N.I., Sotnikova R.T. <\/em><\/strong>Comparing the main oscillation characteristics in the solar chromosphere and magnetosphere based on studies made in ISTP SB RAS)<\/td>14\u201322<\/td>PDF<\/a><\/strong><\/td>12\u201318<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0438\u0447\u0438\u0433\u0438\u043d \u0413.\u041d.<\/em> <\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u0438\u043e\u043d\u043e\u0432 \u0432\u043e \u0444\u0440\u043e\u043d\u0442\u0435 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0437\u0432\u0443\u043a\u043e\u0432\u044b\u0445 \u0443\u0434\u0430\u0440\u043d\u044b\u0445 \u0432\u043e\u043b\u043d (Kichigin G.N.<\/em> <\/strong>Ion dynamics in magnetosonic shock front)<\/td>23\u201331<\/td>PDF<\/a><\/strong><\/td>19\u201325<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439 \u041a.\u0413., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e \u041c.\u0412., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e \u0412.\u0412., \u0427\u0438\u0440\u0438\u043a \u041d.\u0412., \u041a\u043e\u0440\u0435\u043d\u044c\u043a\u043e\u0432\u0430 \u041d.\u0410., \u041a\u043e\u0442\u043e\u0432\u0430 \u0414.\u0421.<\/em> <\/strong>\u042d\u0444\u0444\u0435\u043a\u0442\u044b \u043f\u043e\u0441\u043b\u0435\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0439 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c: \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u0438 \u0442\u0435\u043e\u0440\u0435\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0435 \u043e\u0431\u044a\u044f\u0441\u043d\u0435\u043d\u0438\u0435 (Ratovsky K.G., Klimenko M.V., Klimenko V.V., Chirik N.V., Korenkova N.A., Kotova D.S.<\/em> <\/strong>After-effects of geomagnetic storms: statistical analysis and theoretical explanation)<\/td>32\u201342<\/td>PDF<\/a><\/strong><\/td>26\u201332<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u043b\u044f\u043a\u043e\u0432 \u0410.\u0420.<\/em> <\/strong>\u0414\u0435\u0442\u0435\u043a\u0442\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0433\u0440\u0443\u043f\u043f \u044d\u043a\u0432\u0438\u0434\u0438\u0441\u0442\u0430\u043d\u0442\u043d\u044b\u0445 \u0447\u0430\u0441\u0442\u043e\u0442 \u0432 \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u0445 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0439 (Polyakov A.R.<\/em> <\/strong>Detecting groups of equidistant frequencies in spectra of geomagnetic pulsations)<\/td>43\u201353<\/td>PDF<\/a><\/strong><\/td>33\u201341<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412., \u0411\u0435\u043b\u0435\u0446\u043a\u0438\u0439 \u0410.\u0411., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432 \u0413.\u0410., \u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0421.\u0412., \u0422\u0430\u0449\u0438\u043b\u0438\u043d \u041c.\u0410., \u0410\u0440\u0442\u0430\u043c\u043e\u043d\u043e\u0432 \u041c.\u0424.<\/em> <\/strong>\u0421\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0435 \u0438 \u0444\u043e\u0442\u043e\u043c\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0438 \u0441\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0433\u043e \u0441\u0438\u044f\u043d\u0438\u044f \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 17 \u043c\u0430\u0440\u0442\u0430 2015 \u0433 (Mikhalev A.V., Beletsky A.B., Vasilyev R.V., Zherebtsov G.A., Podlesny S.V., Tashchilin M.A., Artamonov M.F.<\/em> <\/strong>Spectral and photometric characteristics of mid-latitude auroras during the magnetic storm of March 17, 2015)<\/td>54\u201361<\/td>PDF<\/a><\/strong><\/td>42\u201347<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u0441\u044e\u043a\u0435\u0432\u0438\u0447 \u0410.\u0421., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e \u041c.\u0412., \u041a\u0443\u043b\u0438\u043a\u043e\u0432 \u042e.\u042e., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e \u0412.\u0412., \u0411\u0435\u0441\u0441\u0430\u0440\u0430\u0431 \u0424.\u0421., \u041a\u043e\u0440\u0435\u043d\u044c\u043a\u043e\u0432 \u042e.\u041d., \u041c\u0430\u0440\u0438\u0447\u0435\u0432 \u0412.\u041d., \u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439 \u041a.\u0413., \u041a\u043e\u043b\u0435\u0441\u043d\u0438\u043a \u0421.\u0410.<\/em> <\/strong>\u0418\u0437\u043c\u0435\u043d\u0435\u043d\u0438\u044f \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u0441\u0440\u0435\u0434\u043d\u0435\u0439 \u0438 \u0432\u0435\u0440\u0445\u043d\u0435\u0439 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0432\u043d\u0435\u0437\u0430\u043f\u043d\u043e\u0433\u043e \u0441\u0442\u0440\u0430\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043f\u043e\u0442\u0435\u043f\u043b\u0435\u043d\u0438\u044f \u0432 \u044f\u043d\u0432\u0430\u0440\u0435 2013 \u0433. (Yasyukevich A.S., Klimenko M.V., Kulikov Yu.Yu., Klimenko V.V., Bessarab F.S., Korenkov Yu.N., Marichev V.N., Ratovsky K.G., Kolesnik S.A.<\/em> <\/strong>Changes in the middle and upper atmosphere parameters during the January 2013 sudden stratospheric warming)<\/td>62\u201375<\/td>PDF<\/a><\/strong><\/td>48\u201358<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0430\u0440\u0430\u0445\u0430\u043d\u044f\u043d \u0410.\u0410., \u041c\u043e\u043b\u043e\u0434\u044b\u0445<\/em><\/strong> \u0421.\u0418.<\/strong><\/em> <\/strong>\u041f\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 \u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u044b \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u0439 (Karakhanyan A.A., Molodykh S.I.<\/em> <\/strong>Spatial distribution of temperature during geomagnetic disturbances)<\/td>76\u201381<\/td>PDF<\/a><\/strong><\/td>59\u201362<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u0441\u044e\u043a\u0435\u0432\u0438\u0447 \u042e.\u0412., \u0412\u0435\u0441\u043d\u0438\u043d \u0410.\u041c., \u041f\u0435\u0440\u0435\u0432\u0430\u043b\u043e\u0432\u0430 \u041d.\u041f.<\/em> <\/strong>\u0421\u0438\u0431\u0438\u0440\u0441\u043a\u0430\u044f \u0441\u0435\u0442\u044c \u043f\u0440\u0438\u0435\u043c\u043d\u0438\u043a\u043e\u0432 \u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432 \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u044b\u0445 \u043d\u0430\u0432\u0438\u0433\u0430\u0446\u0438\u043e\u043d\u043d\u044b\u0445 \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432\u044b\u0445 \u0441\u0438\u0441\u0442\u0435\u043c SibNet: \u0442\u0435\u043a\u0443\u0449\u0435\u0435 \u0441\u043e\u0441\u0442\u043e\u044f\u043d\u0438\u0435 (Yasyukevich Yu.V., Vesnin A.M., Perevalova N.P<\/em>. <\/strong>SibNet \u2014 Siberian Global Navigation Satellite System Network: Current state)<\/td>82\u201394<\/td>PDF<\/a><\/strong><\/td>63\u201372<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u043e\u0440\u043e\u043a\u0438\u043d \u0410.\u0413., \u041a\u043b\u044e\u0447\u0435\u0432\u0441\u043a\u0438\u0439 \u0410.\u0412., \u0414\u0435\u043c\u044c\u044f\u043d\u043e\u0432\u0438\u0447<\/em><\/strong> \u0412.\u041c.<\/strong><\/em> <\/strong>\u041e \u0433\u0435\u043d\u0435\u0440\u0430\u0446\u0438\u0438 \u0438\u043d\u0444\u0440\u0430\u0437\u0432\u0443\u043a\u043e\u0432\u044b\u0445 \u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432 \u043f\u0440\u0438 \u0437\u0435\u043c\u043b\u0435\u0442\u0440\u044f\u0441\u0435\u043d\u0438\u044f\u0445 5 \u0434\u0435\u043a\u0430\u0431\u0440\u044f 2014 \u0433. \u0432 \u0430\u043a\u0432\u0430\u0442\u043e\u0440\u0438\u0438 \u043e\u0437\u0435\u0440\u0430 \u0425\u0443\u0431\u0441\u0443\u0433\u0443\u043b (\u0421\u0435\u0432\u0435\u0440\u043d\u0430\u044f \u041c\u043e\u043d\u0433\u043e\u043b\u0438\u044f)(Sorokin A.G., Klyuchevskii \u0410.V., Demyanovich V.M.<\/em> <\/strong>Generation of infrasonic signals during earthquakes under Lake Hovsgool (Northern Mongolia) on December 5, 2014)<\/td>95\u2013105<\/td>PDF<\/a><\/strong><\/td>73\u201381<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041b\u0435\u0441\u043e\u0432\u043e\u0439<\/em><\/strong> <\/em>\u0421.\u0412., \u041a\u043e\u0431\u0435\u0446 \u0412.\u0421.<\/em> <\/strong>\u041c\u043e\u0434\u0435\u043b\u044c \u043e\u0442\u043a\u043b\u0438\u043a\u0430 \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 \u043d\u0430 \u0441\u043f\u043e\u043a\u043e\u0439\u043d\u043e\u0435 \u0421\u043e\u043b\u043d\u0446\u0435 (Lesovoi S.V., Kobets V.S. <\/em><\/strong>Simulating Siberian Radioheliograph response to the quiet Sun)<\/td>106\u2013113<\/td>PDF<\/a><\/strong><\/td>82\u201387<\/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. Pp. \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. \u041f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0435 \u0438 \u0432\u0440\u0435\u043c\u0435\u043d\u043d\u044b\u0435 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0444\u043e\u0440\u043c\u044b \u043a\u043e\u043d\u0442\u0443\u0440\u043e\u0432 \u043b\u0438\u043d\u0438\u0438 K Ca II \u0432 \u0440\u0430\u0437\u043b\u0438\u0447\u043d\u044b\u0445 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u043d\u044b\u0445 \u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u0438\u044f\u0445 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0445\u0440\u043e\u043c\u043e\u0441\u0444\u0435\u0440\u044b. I. \u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0438\u043d\u0434\u0438\u0432\u0438\u0434\u0443\u0430\u043b\u044c\u043d\u044b\u0445 \u043a\u043e\u043d\u0442\u0443\u0440\u043e\u0432 (Turova I.P., Grigoryeva S.A., Ozhogina O.A. Spatial and temporal variations of Ca II K line profile shapes in different structures of solar chromosphere. I. Features of […]<\/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-8024","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8024","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=8024"}],"version-history":[{"count":6,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8024\/revisions"}],"predecessor-version":[{"id":10043,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8024\/revisions\/10043"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8024"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8024"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8024"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}