{"id":8003,"date":"2025-04-22T16:01:43","date_gmt":"2025-04-22T16:01:43","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8003"},"modified":"2025-11-17T03:12:01","modified_gmt":"2025-11-17T03:12:01","slug":"solnechno-zemnaya-fizika-zhurnal-tom-2-%e2%84%964-2016","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-zhurnal-tom-2-%e2%84%964-2016\/","title":{"rendered":"\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u0430\u044f \u0444\u0438\u0437\u0438\u043a\u0430. \u0416\u0443\u0440\u043d\u0430\u043b. \u0422\u043e\u043c 2, \u21164, 2016"},"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>
\u041c\u0430\u0443\u0440\u0447\u0435\u0432 \u0415.\u0410., \u0411\u0430\u043b\u0430\u0431\u0438\u043d \u042e.\u0412.<\/em> <\/strong>\u041c\u043e\u0434\u0435\u043b\u044c\u043d\u044b\u0439 \u043a\u043e\u043c\u043f\u043b\u0435\u043a\u0441 \u0434\u043b\u044f \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 RUSCOSMIC (Maurchev E.A., Balabin Yu.V.<\/em> <\/strong>RUSCOSMIC \u2014 the new software toolbox for detailed analysis of cosmic ray interactions with matter)<\/td>3\u20138<\/td>PDF<\/a><\/strong><\/td>3-10<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0435\u0432 \u0420.\u041d.<\/em> <\/strong>\u041a\u043e\u0440\u0440\u0435\u043b\u044f\u0446\u0438\u044f \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0438 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 \u043d\u0430 \u0433\u043b\u0430\u0432\u043d\u043e\u0439 \u0444\u0430\u0437\u0435 \u0438 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Boroyev R.N.<\/em><\/strong> Correlation between auroral activity and rate of development of a storm in its main phase)<\/td>9\u201312<\/td>PDF<\/a><\/strong><\/td>11\u201315<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421., \u0414\u043e\u0432\u0431\u043d\u044f \u0411.\u0412., \u0411\u0430\u0438\u0448\u0435\u0432<\/em><\/strong> \u0414.\u0413., \u041f\u043e\u043b\u044e\u0448\u043a\u0438\u043d\u0430 \u0422.\u041d., \u0420\u0430\u0445\u043c\u0430\u0442\u0443\u043b\u0438\u043d \u0420.\u0410.<\/strong><\/em> <\/strong>\u0423\u0437\u043a\u043e\u043f\u043e\u043b\u043e\u0441\u043d\u043e\u0435 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u0435 \u0441 \u0438\u0437\u043c\u0435\u043d\u044f\u044e\u0449\u0435\u0439\u0441\u044f \u043e\u0442 0.5 \u0434\u043e 3.5 \u0413\u0446 \u0447\u0430\u0441\u0442\u043e\u0442\u043e\u0439 \u043d\u0430 \u0444\u043e\u043d\u0435 \u0433\u043b\u0430\u0432\u043d\u043e\u0439 \u0444\u0430\u0437\u044b \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 17 \u043c\u0430\u0440\u0442\u0430 2013 \u0433. (Potapov A.S., Dovbnya B.V., Baishev D.G., Polyushkina T.N., Rakhmatulin R.A.<\/em> <\/strong>Narrow-band emission with 0.5 to 3.5 Hz varying frequency in the background of the main phase of the 17 March 2013 magnetic storm)<\/td>13\u201323<\/td>PDF<\/a><\/strong><\/td>16\u201330<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u043e\u043b\u043e\u0442\u0443\u0445\u0438\u043d\u0430 \u041d.\u0410., \u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u041f\u043e\u043b\u0435\u0445 \u041d.\u041c., \u0420\u043e\u043c\u0430\u043d\u043e\u0432\u0430 \u0415.\u0411.<\/em> <\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u043e\u0431\u0440\u0430\u0442\u043d\u043e\u0433\u043e \u0440\u0430\u0441\u0441\u0435\u044f\u043d\u0438\u044f \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0431\u043e\u043b\u044c\u0448\u043e\u0439 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0415\u043a\u0430\u0442\u0435\u0440\u0438\u043d\u0431\u0443\u0440\u0433\u0441\u043a\u043e\u0433\u043e \u0440\u0430\u0434\u0430\u0440\u0430: 17\u201322 \u043c\u0430\u0440\u0442\u0430 2015 \u0433. (Zolotukhina N.A., Kurkin V.I., Polekh N.M., Romanova E.B.<\/em> <\/strong>Backscattering dynamics during intense geomagnetic storm as deduced from Yekaterinburg radar data: March 17\u201322, 2015)<\/td>24\u201342<\/td>PDF<\/a><\/strong><\/td>31\u201354<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0438\u043c \u0410.\u0413., \u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u041a\u043e\u0442\u043e\u0432\u0438\u0447 \u0413.\u0412., \u0420\u043e\u043c\u0430\u043d\u043e\u0432\u0430 \u0415.\u0411. <\/em><\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 z-\u043e\u0431\u0440\u0430\u0437\u043d\u043e\u0433\u043e \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f \u043d\u0430 \u043b\u0443\u0447\u0435 \u041f\u0435\u0434\u0435\u0440\u0441\u0435\u043d\u0430 \u0434\u0438\u0441\u0442\u0430\u043d\u0446\u0438\u043e\u043d\u043d\u043e-\u0447\u0430\u0441\u0442\u043e\u0442\u043d\u043e\u0439 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0438 \u043d\u0430\u043a\u043b\u043e\u043d\u043d\u043e\u0433\u043e \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0441 \u0438\u0441\u043f\u043e\u043b\u044c\u0437\u043e\u0432\u0430\u043d\u0438\u0435\u043c \u043c\u043e\u0434\u0435\u043b\u0435\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b (Kim \u0410.G., Ponomarchuk S.N., Kotovich G.V., Romanova E.B.<\/em><\/strong> Modeling z-shaped disturbance at the Pedersen ray of oblique sounding ionogram using adaptation of IRI to experimental data)<\/td>43\u201353<\/td>PDF<\/a><\/strong><\/td>55\u201369<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u043e\u043b\u0438\u043a\u043e\u0432<\/em><\/strong> \u0418.\u0410., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432<\/strong> \u0410.\u042e., \u041f\u043e\u043f\u043e\u0432 \u0412.\u0418<\/strong><\/em>. <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u044b \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 F2 \u0432\u044b\u0441\u043e\u043a\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0434\u043b\u044f \u0443\u0441\u043b\u043e\u0432\u0438\u0439 \u0437\u0438\u043c\u043d\u0435\u0433\u043e \u0441\u043e\u043b\u043d\u0446\u0435\u0441\u0442\u043e\u044f\u043d\u0438\u044f (Golikov I.A., Gololobov A.Yu., Popov V.I.<\/em> <\/strong>Modeling the electron temperature distribution in F2 region of high-latitude ionosphere for winter solstice conditions)<\/td>54\u201362<\/td>PDF<\/a><\/strong><\/td>70\u201380<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0442\u043e\u0432\u0430 \u0414.\u0421., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e \u041c.\u0412., \u041a\u043b\u0438\u043c\u0435\u043d\u043a\u043e<\/em><\/strong> \u0412.\u0412., \u0417\u0430\u0445\u0430\u0440\u043e\u0432 \u0412.\u0415., \u0411\u0435\u0441\u0441\u0430\u0440\u0430\u0431 \u0424.\u0421., \u041a\u043e\u0440\u0435\u043d\u044c\u043a\u043e\u0432 \u042e.\u041d.<\/strong><\/em> <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \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 2009 \u0433. \u043d\u0430 \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u0435 \u043a\u043e\u0440\u043e\u0442\u043a\u0438\u0445 \u0440\u0430\u0434\u0438\u043e\u0432\u043e\u043b\u043d \u0432 \u044d\u043a\u0432\u0430\u0442\u043e\u0440\u0438\u0430\u043b\u044c\u043d\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0435 (Kotova D.S., Klimenko<\/em><\/strong> M.V., Klimenko<\/strong> V.V., Zakharov V.E., Bessarab<\/strong> F.S., Korenkov<\/strong> Yu.N<\/strong><\/em>. <\/strong>Influence of January 2009 stratospheric warming on HF radio wave propagation in the low-latitude ionosphere)<\/td>63\u201375<\/td>PDF<\/a><\/strong><\/td>81\u201393<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0422\u0430\u0449\u0438\u043b\u0438\u043d<\/em><\/strong> \u0410.\u0412., \u041b\u0435\u043e\u043d\u043e\u0432\u0438\u0447<\/strong> \u041b.\u0410.<\/strong><\/em> <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u043d\u043e\u0447\u043d\u044b\u0445 \u0441\u0432\u0435\u0447\u0435\u043d\u0438\u0439 \u043a\u0440\u0430\u0441\u043d\u043e\u0439 \u0438 \u0437\u0435\u043b\u0435\u043d\u043e\u0439 \u043b\u0438\u043d\u0438\u0439 \u0430\u0442\u043e\u043c\u0430\u0440\u043d\u043e\u0433\u043e \u043a\u0438\u0441\u043b\u043e\u0440\u043e\u0434\u0430 \u0434\u043b\u044f \u0443\u043c\u0435\u0440\u0435\u043d\u043d\u043e-\u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u044b\u0445 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0443\u0441\u043b\u043e\u0432\u0438\u0439 \u043d\u0430 \u0441\u0440\u0435\u0434\u043d\u0438\u0445 \u0448\u0438\u0440\u043e\u0442\u0430\u0445 (Tashchilin A.V., Leonovich L.A.<\/em> <\/strong>Modeling nightglow in atomic oxygen red and green lines under moderate disturbed geomagnetic conditions at midlatitudes)<\/td>76\u201384<\/td>PDF<\/a><\/strong><\/td>94\u2013106<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0435\u043b\u0435\u0446\u043a\u0438\u0439 \u0410.\u0411., \u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412., \u0425\u0430\u0445\u0438\u043d\u043e\u0432<\/em><\/strong> \u0412.\u0412., \u041b\u0435\u0431\u0435\u0434\u0435\u0432 \u0412.\u041f.<\/strong><\/em> <\/strong>\u041e\u043f\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0435 \u043f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u0435 \u0440\u0430\u0431\u043e\u0442\u044b \u0431\u043e\u0440\u0442\u043e\u0432\u044b\u0445 \u0434\u0432\u0438\u0433\u0430\u0442\u0435\u043b\u0435\u0439 \u043d\u0438\u0437\u043a\u043e\u043e\u0440\u0431\u0438\u0442\u0430\u043b\u044c\u043d\u044b\u0445 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0430\u043f\u043f\u0430\u0440\u0430\u0442\u043e\u0432 (Beletsky A.B., Mikhalev \u0410.V., Khakhinov V.V., Lebedev<\/em><\/strong> V.P<\/strong><\/em>. <\/strong>Optical effects produced by running onboard engines of low-earth-orbit spacecraft)<\/td>85\u201391<\/td>PDF<\/a><\/strong><\/td>107\u2013117<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0443\u0448\u043d\u0430\u0440\u0435\u043d\u043a\u043e \u0413.\u041f.,<\/em> \u042f\u043a\u043e\u0432\u043b\u0435\u0432\u0430 \u041e.\u0415., \u041a\u0443\u0437\u043d\u0435\u0446\u043e\u0432\u0430 \u0413.\u041c<\/em>. <\/strong>\u0414\u043e\u043b\u0433\u043e\u0432\u0440\u0435\u043c\u0435\u043d\u043d\u044b\u0435 \u0438\u0437\u043c\u0435\u043d\u0435\u043d\u0438\u044f \u0432 \u043d\u0435\u0439\u0442\u0440\u0430\u043b\u044c\u043d\u043e\u043c \u0433\u0430\u0437\u043e\u0432\u043e\u043c \u0441\u043e\u0441\u0442\u0430\u0432\u0435 \u0442\u0435\u0440\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430\u0434 \u041d\u043e\u0440\u0438\u043b\u044c\u0441\u043a\u043e\u043c (2003\u20132013 \u0433\u0433.) (Kushnarenko G.P., Yakovleva O.E., Kuznetsova G.M.<\/em> <\/strong>Long-term variations in the neutral gas composition of the thermosphere over Norilsk (2003\u20132013))<\/td>92\u201397<\/td>PDF<\/a><\/strong><\/td>118\u2013125<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438<\/em><\/strong> \u0410.\u0412., \u0420\u0443\u0431\u0430\u043d<\/strong> \u0412.\u0424. <\/strong><\/em>\u041a 120-\u043b\u0435\u0442\u0438\u044e \u0441\u043e \u0434\u043d\u044f \u0440\u043e\u0436\u0434\u0435\u043d\u0438\u044f \u0410.\u041b. \u0427\u0438\u0436\u0435\u0432\u0441\u043a\u043e\u0433\u043e (Guglielmi A.V., Ruban V.F.<\/em> <\/strong>To the 120th<\/sup> anniversary of A.L. Chizhevsky\u2019s birth)<\/td>98\u2013103<\/td>PDF<\/a><\/strong><\/td>126\u2013133<\/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. \u041c\u0430\u0443\u0440\u0447\u0435\u0432 \u0415.\u0410., \u0411\u0430\u043b\u0430\u0431\u0438\u043d \u042e.\u0412. \u041c\u043e\u0434\u0435\u043b\u044c\u043d\u044b\u0439 \u043a\u043e\u043c\u043f\u043b\u0435\u043a\u0441 \u0434\u043b\u044f \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 RUSCOSMIC (Maurchev E.A., Balabin Yu.V. RUSCOSMIC \u2014 the new software toolbox for detailed analysis of cosmic ray interactions with matter) 3\u20138 PDF 3-10 PDF \u0411\u043e\u0440\u043e\u0435\u0432 \u0420.\u041d. \u041a\u043e\u0440\u0440\u0435\u043b\u044f\u0446\u0438\u044f \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0438 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0439 \u0431\u0443\u0440\u0438 \u043d\u0430 \u0433\u043b\u0430\u0432\u043d\u043e\u0439 \u0444\u0430\u0437\u0435 \u0438 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Boroyev R.N. Correlation between auroral […]<\/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-8003","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8003","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=8003"}],"version-history":[{"count":6,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8003\/revisions"}],"predecessor-version":[{"id":10292,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8003\/revisions\/10292"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8003"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8003"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8003"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}