{"id":8044,"date":"2025-04-23T00:32:23","date_gmt":"2025-04-23T00:32:23","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8044"},"modified":"2025-10-20T03:49:08","modified_gmt":"2025-10-20T03:49:08","slug":"solnechno-zemnaya-fizika-tom-6-%e2%84%964-2020","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-6-%e2%84%964-2020\/","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 6, \u21164, 2020"},"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>
\u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u041c., \u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u041b.\u0412., \u0425\u043b\u044b\u0441\u0442\u043e\u0432\u0430 \u0410.\u0418.<\/em> <\/strong>\u0410\u0441\u0438\u043c\u043c\u0435\u0442\u0440\u0438\u044f \u0432 \u043f\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u0438 \u043b\u0438\u0434\u0438\u0440\u0443\u044e\u0449\u0435\u0439 \u0438 \u043f\u043e\u0441\u043b\u0435\u0434\u0443\u044e\u0449\u0435\u0439 \u043f\u043e\u043b\u044f\u0440\u043d\u043e\u0441\u0442\u0435\u0439 \u0432 \u0444\u043e\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u043c \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u043c \u043f\u043e\u043b\u0435 \u043d\u0430 \u0440\u0430\u043d\u043d\u0435\u0439 \u0441\u0442\u0430\u0434\u0438\u0438 \u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u0438\u044f \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 (Grigoryev V.M., Ermakova L.V., Khlystova A.I<\/em>. <\/strong>Asymmetry in occurrence of the leading and following polarities in the photospheric magnetic field at the early stage of active region formation)<\/td>3\u20139<\/td>PDF<\/a><\/strong><\/td>3\u20139<\/td>PDF<\/a><\/strong><\/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 \u041e.\u0410.<\/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. II. \u041c\u0435\u0442\u043e\u0434\u0438\u043a\u0430 \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0438 \u043a\u043e\u0440\u0440\u0435\u043b\u044f\u0446\u0438\u043e\u043d\u043d\u044b\u0435 \u0441\u043e\u043e\u0442\u043d\u043e\u0448\u0435\u043d\u0438\u044f \u043c\u0435\u0436\u0434\u0443 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430\u043c\u0438 \u043b\u0438\u043d\u0438\u0438 \u0434\u043b\u044f \u0443\u0447\u0430\u0441\u0442\u043a\u043e\u0432 K1<\/sub> \u0438 K2<\/sub> (Turova I.P., Grigoryeva S.A., Ozhogina O.A.<\/em><\/strong> Spatial and temporal variations of K CA II line profile shapes in different structures of the solar chromosphere. II. Determination technique and correlation relationships between the K CA II line parameters for K1<\/sub> and K2<\/sub> features)<\/td>10\u201317<\/td>PDF<\/a><\/strong><\/td>10\u201316<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041d\u0435\u043a\u0440\u0430\u0441\u043e\u0432 \u0410.\u041a., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e<\/em><\/strong> \u0412.\u0410.<\/strong><\/em> <\/strong>\u041c\u0413\u0414-\u0432\u043e\u043b\u043d\u044b \u0432 \u0441\u0442\u043e\u043b\u043a\u043d\u043e\u0432\u0438\u0442\u0435\u043b\u044c\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u043a\u043e\u0440\u043e\u043d\u044b \u0438 \u0437\u0435\u043c\u043d\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b (Nekrasov A.K., Pilipenko V.A.<\/em><\/strong> MHD waves in the collisional plasma of the solar corona and terrestrial ionosphere)<\/td>18\u201325<\/td>PDF<\/a><\/strong><\/td>17\u201323<\/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., \u0421\u0443\u0432\u043e\u0440\u043e\u0432\u0430 \u0410.\u0412., \u0412\u0435\u0434\u0435\u0440\u043d\u0438\u043a\u043e\u0432\u0430 \u0422.\u0418<\/em>. <\/strong>\u041a\u043b\u0430\u0441\u0441\u0438\u0444\u0438\u043a\u0430\u0446\u0438\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u043e\u0442\u043a\u043b\u0438\u043a\u043e\u0432 \u043d\u0430 \u0432\u0437\u0430\u0438\u043c\u043e\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435 \u0441 \u0434\u0438\u0430\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u043c\u0438 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0430\u043c\u0438 \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 (Parkhomov V.A., Eselevich V.G.,<\/em><\/strong> Eselevich M.V., Dmitriev A.V., Suvorova A.V., Vedernikova T.I.<\/strong><\/em> <\/strong>Classification of magnetospheric responses to interaction with diamagnetic structures of slow solar wind)<\/td>26\u201341<\/td>PDF<\/a><\/strong><\/td>24\u201336<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u0432\u0435\u0440\u0435\u0432 \u0410.\u0421., \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u0413., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e., \u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410<\/em>. <\/strong>\u041c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432<\/a> \u0430\u043d\u0438\u0437\u043e\u0442\u0440\u043e\u043f\u0438\u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432 \u0440\u0435\u0430\u043b\u044c\u043d\u043e\u043c \u0432\u0440\u0435\u043c\u0435\u043d\u0438 \u0438 \u043a\u0440\u0430\u0442\u043a\u043e\u0441\u0440\u043e\u0447\u043d\u044b\u0439 \u043f\u0440\u043e\u0433\u043d\u043e\u0437 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u0439 (Zverev A.S., Grigoryev V.G., Gololobov P.Yu., Starodubtsev S.A.<\/em> <\/strong>Real-time monitoring of cosmic ray anisotropy parameters and short-term forecasting of geomagnetic disturbances)<\/td>42\u201345<\/td>PDF<\/a><\/strong><\/td>37\u201339<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041b\u0430\u0437\u0443\u0442\u0438\u043d \u041b.\u041b<\/em>. <\/strong>\u0412\u043e\u0437\u0440\u0430\u0441\u0442\u0430\u043d\u0438\u044f \u044d\u043d\u0435\u0440\u0433\u0438\u0447\u043d\u044b\u0445 \u043f\u0440\u043e\u0442\u043e\u043d\u043e\u0432 \u0421\u041a\u041b \u043d\u0430 \u0417\u0435\u043c\u043b\u0435 \u0438 \u0438\u0445 \u0441\u0432\u044f\u0437\u044c \u0441 \u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u0430\u043c\u0438    \u043d\u0430 \u0421\u043e\u043b\u043d\u0446\u0435 (Lazutin L.L.<\/em><\/strong> Increases in SCR energetic proton fluxes on Earth and their relation to solar sources)<\/td>46\u201350<\/td>PDF<\/a><\/strong><\/td>40\u201343<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0442\u043e\u0432\u0430 \u0413.\u0410., \u0412\u0435\u0440\u0438\u0433\u0438\u043d \u041c.\u0418., \u0413\u043e\u043c\u0431\u043e\u0448\u0438 \u0422.,<\/em><\/strong> \u041a\u0430\u0431\u0438\u043d \u041a<\/strong><\/em>. <\/strong>\u0410\u043d\u0430\u043b\u0438\u0442\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u043c\u043e\u0434\u0435\u043b\u044c \u043e\u043a\u043e\u043b\u043e\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u0443\u0434\u0430\u0440\u043d\u043e\u0439 \u0432\u043e\u043b\u043d\u044b \u0434\u043b\u044f \u0440\u0430\u0437\u043b\u0438\u0447\u043d\u044b\u0445 \u043d\u0430\u043f\u0440\u0430\u0432\u043b\u0435\u043d\u0438\u0439 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f, \u043e\u0441\u043d\u043e\u0432\u0430\u043d\u043d\u0430\u044f \u043d\u0430 \u041c\u0413\u0414-\u0440\u0430\u0441\u0447\u0435\u0442\u0430\u0445 (Kotova G.A., Verigin M.I., Gombosi T.,<\/em><\/strong> Kabin K.<\/strong><\/em> <\/strong>Analytical model of the planetary bow shock for various magnetic field directions based on MHD calculations)<\/td>51\u201358<\/td>PDF<\/a><\/strong><\/td>44\u201349<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u043a\u0430\u0440\u043e\u0432 \u0413.\u0410<\/em>. <\/strong>\u0413\u0435\u043e\u043c\u0435\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0439 \u0444\u0430\u043a\u0442\u043e\u0440 \u0432 \u0441\u0435\u0437\u043e\u043d\u043d\u044b\u0445 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u044f\u0445 \u0441\u0440\u0435\u0434\u043d\u0435\u0441\u0443\u0442\u043e\u0447\u043d\u044b\u0445 \u0437\u043d\u0430\u0447\u0435\u043d\u0438\u0439 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u0438\u043d\u0434\u0435\u043a\u0441\u0430 Dst<\/em> (Makarov G.A.<\/em><\/strong> Geometric factor in seasonal variations of daily average values of the geomagnetic index Dst<\/em>)<\/td>59\u201366<\/td>PDF<\/a><\/strong><\/td>50\u201356<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0435\u043d\u0441\u043a\u0438\u0445 \u042e.\u0412.<\/em> <\/strong>\u041f\u0440\u0438\u043c\u0435\u043d\u0435\u043d\u0438\u0435 \u043c\u0435\u0442\u043e\u0434\u0430 \u043d\u0430\u0438\u0431\u043e\u043b\u044c\u0448\u0438\u0445 \u0432\u043a\u043b\u0430\u0434\u043e\u0432 \u0432 \u0442\u0435\u0445\u043d\u0438\u043a\u0435 \u0438\u043d\u0432\u0435\u0440\u0441\u0438\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0433\u0440\u0430\u043c\u043c (Penskikh Yu.V.<\/em> <\/strong>Applying the method of maximum contributions to the magnetogram inversion technique)<\/td>67\u201376<\/td>PDF<\/a><\/strong><\/td>57\u201365<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0410\u0444\u0430\u043d\u0430\u0441\u044c\u0435\u0432 \u041d.\u0422., \u0427\u0443\u0434\u0430\u0435\u0432 \u0421.\u041e.<\/em> <\/strong>\u0414\u0438\u0430\u0433\u043d\u043e\u0441\u0442\u0438\u043a\u0430 \u0441\u0442\u043e\u0445\u0430\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043a\u0430\u043d\u0430\u043b\u0430 \u0432 \u0434\u0435\u043a\u0430\u043c\u0435\u0442\u0440\u043e\u0432\u043e\u043c \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0435 \u0440\u0430\u0434\u0438\u043e\u0432\u043e\u043b\u043d (Afanasiev N.T., Chudaev S.\u041e.<\/em> <\/strong>Diagnostics of the stochastic ionospheric channel in the decameter band of radio waves)<\/td>77\u201385<\/td>PDF<\/a><\/strong><\/td>66\u201373<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u0447\u0435\u0432\u043a\u0438\u043d\u0430 \u041e.\u041f., \u041a\u0430\u0440\u043f\u043e\u0432 \u0418.\u0412., \u041a\u0430\u0440\u043f\u043e\u0432 \u041c.\u0418., \u041a\u043e\u0440\u0435\u043d\u044c\u043a\u043e\u0432\u0430 \u041d.\u0410., \u0412\u043b\u0430\u0441\u043e\u0432 \u0412.\u0418., \u041b\u0435\u0449\u0435\u043d\u043a\u043e \u0412.\u0421.<\/em> <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043c\u0435\u0442\u0435\u043e\u0440\u043e\u043b\u043e\u0433\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0448\u0442\u043e\u0440\u043c\u043e\u0432 \u043d\u0430 \u043e\u0431\u043b\u0430\u0441\u0442\u044c \u0415 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0432 2017\u20132018 \u0433\u0433. (Borchevkina O.P., Karpov I.V., Karpov M.I., Korenkova N.A., Vlasov V.I., Leshchenko V.S<\/em>. <\/strong>Impact of meteorological storms on the E-region of the ionosphere in 2017\u20132018)<\/td>86\u201392<\/td>PDF<\/a><\/strong><\/td>74\u201379<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u041a\u043b\u0430\u0439\u043d \u0411.\u0418., \u041a\u0443\u0440\u0430\u0436\u043a\u043e\u0432\u0441\u043a\u0430\u044f \u041d.\u0410.<\/em> <\/strong>\u0417\u0435\u043c\u043b\u0435\u0442\u0440\u044f\u0441\u0435\u043d\u0438\u044f \u0438 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f (Guglielmi V., Klain B.I., Kurazhkovskaya N.A.<\/em> <\/strong>Earthquakes and geomagnetic disturbances)<\/td>93\u201398<\/td>PDF<\/a><\/strong><\/td>80\u201383<\/td>PDF<\/a><\/strong><\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. Pp. \u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u041c., \u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u041b.\u0412., \u0425\u043b\u044b\u0441\u0442\u043e\u0432\u0430 \u0410.\u0418. \u0410\u0441\u0438\u043c\u043c\u0435\u0442\u0440\u0438\u044f \u0432 \u043f\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u0438 \u043b\u0438\u0434\u0438\u0440\u0443\u044e\u0449\u0435\u0439 \u0438 \u043f\u043e\u0441\u043b\u0435\u0434\u0443\u044e\u0449\u0435\u0439 \u043f\u043e\u043b\u044f\u0440\u043d\u043e\u0441\u0442\u0435\u0439 \u0432 \u0444\u043e\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u043c \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u043c \u043f\u043e\u043b\u0435 \u043d\u0430 \u0440\u0430\u043d\u043d\u0435\u0439 \u0441\u0442\u0430\u0434\u0438\u0438 \u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u0438\u044f \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0439 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 (Grigoryev V.M., Ermakova L.V., Khlystova A.I. Asymmetry in occurrence of the leading and following polarities in the photospheric magnetic field at the early stage of active region formation) 3\u20139 […]<\/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-8044","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8044","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=8044"}],"version-history":[{"count":7,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8044\/revisions"}],"predecessor-version":[{"id":9621,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8044\/revisions\/9621"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8044"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8044"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8044"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}