{"id":8073,"date":"2025-04-23T04:13:14","date_gmt":"2025-04-23T04:13:14","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8073"},"modified":"2025-10-24T17:03:12","modified_gmt":"2025-10-24T17:03:12","slug":"solnechno-zemnaya-fizika-tom-10-%e2%84%962-2024","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-10-%e2%84%962-2024\/","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 10, \u21162, 2024"},"content":{"rendered":"
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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/td>\u0421\u0442\u0440.<\/td><\/td>Pp.<\/td><\/td><\/tr>
\u0411\u0435\u043b\u043e\u0432 \u0421.\u0410., \u041b\u0435\u0434\u0435\u043d\u0446\u043e\u0432 \u041b.\u0421., \u0417\u0430\u0432\u0435\u0440\u0448\u0438\u043d\u0441\u043a\u0438\u0439 \u0414.\u0418., \u0411\u043e\u0433\u0430\u0447\u0451\u0432 \u0421.\u0410<\/em>. <\/strong>\u0414\u0438\u0444\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u0430\u043b\u044c\u043d\u0430\u044f \u043c\u0435\u0440\u0430 \u044d\u043c\u0438\u0441\u0441\u0438\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u043d\u0430\u043d\u043e\u0432\u0441\u043f\u044b\u0448\u0435\u043a, \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u043d\u0430\u044f \u0441 \u043f\u043e\u043c\u043e\u0449\u044c\u044e \u0430\u043b\u0433\u043e\u0440\u0438\u0442\u043c\u0430 SITES (Belov S.A., Ledentsov L.S., Zavershinskii D.I., Bogachev S.A<\/em>. <\/strong>Differential emission measure of solar nanoflares measured with the SITES algorithm)<\/td>4\u201314<\/td>PDF<\/strong><\/a><\/td>3\u201312<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0420\u0430\u0445\u043c\u0430\u043d\u043e\u0432\u0430 \u041b.\u0421., \u0425\u043e\u0445\u043b\u0430\u0447\u0435\u0432 \u0410.\u0410., \u0420\u044f\u0437\u0430\u043d\u0446\u0435\u0432\u0430 \u041c.\u041e., \u0415\u0440\u043c\u043e\u043b\u0430\u0435\u0432 \u042e.\u0418., \u0417\u0430\u0441\u0442\u0435\u043d\u043a\u0435\u0440 \u0413.\u041d<\/em>. <\/strong>\u0420\u0430\u0437\u0432\u0438\u0442\u0438\u0435 \u0442\u0443\u0440\u0431\u0443\u043b\u0435\u043d\u0442\u043d\u043e\u0441\u0442\u0438 \u0437\u0430 \u043e\u043a\u043e\u043b\u043e\u0437\u0435\u043c\u043d\u043e\u0439 \u0443\u0434\u0430\u0440\u043d\u043e\u0439 \u0432\u043e\u043b\u043d\u043e\u0439 \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0441\u043f\u043e\u043a\u043e\u0439\u043d\u043e\u0433\u043e \u0438 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0433\u043e \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 (Rakhmanova L.S., Khokhlachev A.A., Riazantseva M.O., Yermolaev Yu.I., Zastenker G.N<\/em>. <\/strong>Turbulence development behind the bow shock during disturbed and undisturbed solar wind)<\/td>15\u201328<\/td>PDF<\/strong><\/a><\/td>13\u201325<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u043e\u0432\u0430\u043b\u0435\u0432 \u0418.\u0418., \u041a\u0440\u0430\u0432\u0446\u043e\u0432\u0430 \u041c.\u0412., \u041e\u043b\u0435\u043c\u0441\u043a\u043e\u0439 \u0421.\u0412., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.\u0415., \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 \u043e\u043a\u043e\u043b\u043e\u0437\u0435\u043c\u043d\u043e\u0433\u043e \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0430, \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b \u0438 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0417\u0435\u043c\u043b\u0438 \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0444\u043e\u0440\u0431\u0443\u0448-\u044d\u0444\u0444\u0435\u043a\u0442\u043e\u0432 \u0432 \u043a\u043e\u043d\u0446\u0435 \u0430\u0432\u0433\u0443\u0441\u0442\u0430 2005 \u0433. (Kovalev I.I., Kravtsova M.V., Olemskoy S.V., Sdobnov V.E., Starodubtsev S.A<\/em>. <\/strong>Monitoring of near-Earth space, Earth\u2019s magnetosphere and atmosphere during Forbush decreases in August 2005)<\/td>29\u201337<\/td>PDF<\/strong><\/a><\/td>26\u201333<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0427\u0435\u0440\u043d\u0438\u0433\u043e\u0432\u0441\u043a\u0430\u044f \u041c.\u0410., \u0421\u0435\u0442\u043e\u0432 \u0410.\u0413., \u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439 \u041a.\u0413., \u041a\u0430\u043b\u0438\u0448\u0438\u043d \u0410.C., \u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0415<\/em>. <\/strong>\u0418\u0437\u043c\u0435\u043d\u0447\u0438\u0432\u043e\u0441\u0442\u044c \u0438\u043e\u043d\u0438\u0437\u0430\u0446\u0438\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430\u0434 \u0415\u0432\u0440\u0430\u0437\u0438\u0435\u0439 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0446\u0435\u043f\u0438 \u0432\u044b\u0441\u043e\u043a\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u044b\u0445 \u0438\u043e\u043d\u043e\u0437\u043e\u043d\u0434\u043e\u0432 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u044d\u043a\u0441\u0442\u0440\u0435\u043c\u0430\u043b\u044c\u043d\u044b\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c 2015 \u0433. (Chernigovskaya M.A., Setov A.G., Ratovsky K.G., Kalishin A.S., Stepanov A.E<\/em>. <\/strong>Variability of ionospheric ionization over Eurasia according to data from a high-latitude ionosonde chain during extreme magnetic storms in 2015)<\/td>38\u201352<\/td>PDF<\/strong><\/a><\/td>34\u201347<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0442\u0435\u043f\u0430\u043d\u043e\u0432 \u0410.\u0415., \u0414\u0430\u043d\u0438\u043b\u043e\u0432 \u0421.\u0418., \u0411\u0430\u0438\u0448\u0435\u0432 \u0414.\u0413., \u0425\u0430\u043b\u0438\u043f\u043e\u0432 \u0412.\u041b., \u041a\u043e\u0442\u043e\u0432\u0430 \u0413.\u0410., \u041a\u043e\u0431\u044f\u043a\u043e\u0432\u0430 \u0421.\u0415<\/em>. <\/strong>\u0412\u0440\u0435\u043c\u044f \u0436\u0438\u0437\u043d\u0438 \u043f\u043e\u043b\u044f\u0440\u0438\u0437\u0430\u0446\u0438\u043e\u043d\u043d\u043e\u0433\u043e \u0434\u0436\u0435\u0442\u0430 \u043f\u0440\u0438 \u0434\u043b\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044f\u0445 (Stepanov A.E., Danilov S.I., Baishev D.G., Khalipov V.L., Kotova G.A., Kobyakova S.E<\/em>. <\/strong>Lifetime of a polarization jet during long-term magnetic storms)<\/td>53\u201359<\/td>PDF<\/strong><\/a><\/td>48\u201354<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412<\/em>. <\/strong>\u041f\u043e\u043b\u044f\u0440\u043d\u044b\u0435 \u0441\u0438\u044f\u043d\u0438\u044f \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u044d\u043a\u0441\u0442\u0440\u0435\u043c\u0430\u043b\u044c\u043d\u044b\u0445 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c: \u043e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0441\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0433\u043e \u0441\u0438\u044f\u043d\u0438\u044f 11 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 1958 \u0433. (Mikhalev \u0410.V<\/em>. <\/strong>Auroras during extreme geomagnetic storms: some features of mid-latitude aurora on February 11, 1958)<\/td>60\u201366<\/td>PDF<\/strong><\/a><\/td>55\u201361<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u0415.\u041d., \u0420\u044f\u0431\u043e\u0432 \u0410.\u0412<\/em>.<\/strong> \u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u0440\u0435\u0437\u043e\u043d\u0430\u0442\u043e\u0440\u043e\u0432 \u043d\u0430 \u0441\u0443\u0442\u043e\u0447\u043d\u0443\u044e \u0434\u0438\u043d\u0430\u043c\u0438\u043a\u0443 \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043f\u0435\u0440\u0432\u043e\u0433\u043e \u0448\u0443\u043c\u0430\u043d\u043e\u0432\u0441\u043a\u043e\u0433\u043e \u0440\u0435\u0437\u043e\u043d\u0430\u043d\u0441\u0430 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043c\u0435\u0440\u0438\u0434\u0438\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0439 \u0441\u0435\u0442\u0438 \u0423\u041d\u0427-\u043c\u0430\u0433\u043d\u0438\u0442\u043e\u043c\u0435\u0442\u0440\u043e\u0432 (Ermakova E.N., Ryabov A.V<\/em>. <\/strong>Influence of ionospheric resonators on daily dynamics of the first Schumann resonance spectral parameters according to data from a meridional chain of ULF magnetometers)<\/td>67\u201378<\/td>PDF<\/strong><\/a><\/td>62\u201373<\/td>PDF<\/strong><\/a><\/td><\/tr>
 \u0411\u043e\u0440\u0438\u0441\u043e\u0432\u0430 \u0422.\u0414., \u0411\u043b\u0430\u0433\u043e\u0432\u0435\u0449\u0435\u043d\u0441\u043a\u0430\u044f \u041d.\u0424., \u041a\u0430\u043b\u0438\u0448\u0438\u043d \u0410.C., \u041a\u043e\u0432\u0430\u043b\u0435\u0432 \u0410.\u0421<\/em>. <\/strong>\u041e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u0432\u0435\u043a\u0442\u043e\u0440\u0430 \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0438 \u0438\u0441\u043a\u0443\u0441\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0445 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u043d\u0435\u043e\u0434\u043d\u043e\u0440\u043e\u0434\u043d\u043e\u0441\u0442\u0435\u0439 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0434\u043e\u043f\u043b\u0435\u0440\u043e\u0432\u0441\u043a\u0438\u0445 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u0439 \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0440\u0430\u043a\u0443\u0440\u0441\u043d\u043e\u0433\u043e \u0440\u0430\u0441\u0441\u0435\u044f\u043d\u0438\u044f \u041a\u0412-\u0440\u0430\u0434\u0438\u043e\u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432, \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u044f\u044e\u0449\u0438\u0445\u0441\u044f \u043d\u0430 \u043f\u0440\u043e\u0442\u044f\u0436\u0435\u043d\u043d\u044b\u0445 \u0440\u0430\u0434\u0438\u043e\u0442\u0440\u0430\u0441\u0441\u0430\u0445 (Borisova T.D., Blagoveshchenskaya N.F., Kalishin A.S., Kovalev A.S<\/em>. <\/strong>Determination of the vector velocity of artificial ionospheric irregularities based on Doppler measurements by the bistatic scatter method of HF radio signals propagating over long radio paths)<\/td>79\u201398<\/td>PDF<\/strong><\/a><\/td>74\u201392<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u0418\u043b\u044c\u0438\u043d \u041d.\u0412.<\/em>, \u041f\u0435\u043d\u0437\u0438\u043d \u041c.\u0421.<\/em> <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u041a\u0412-\u0440\u0430\u0434\u0438\u043e\u0442\u0440\u0430\u0441\u0441 \u043d\u0430 \u043e\u0441\u043d\u043e\u0432\u0435 \u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0434\u043d\u043e\u0433\u043e \u043f\u043e\u0434\u0445\u043e\u0434\u0430 (Ponomarchuk S.N., Kurkin V.I., Ilyin N.V., Penzin M.S.<\/em> <\/strong>HF radio path modeling by waveguide approach)<\/td>99\u2013108<\/td>PDF<\/strong><\/a><\/td>93\u2013101<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u0413\u0440\u043e\u0437\u043e\u0432 \u0412.\u041f<\/em>. <\/strong>\u0410\u0432\u0442\u043e\u043c\u0430\u0442\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u0438\u043d\u0442\u0435\u0440\u043f\u0440\u0435\u0442\u0430\u0446\u0438\u044f \u0438\u043e\u043d\u043e\u0433\u0440\u0430\u043c\u043c \u043d\u0430\u043a\u043b\u043e\u043d\u043d\u043e\u0433\u043e \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u043d\u0430 \u043e\u0441\u043d\u043e\u0432\u0435 \u0433\u0438\u0431\u0440\u0438\u0434\u043d\u044b\u0445 \u0430\u043b\u0433\u043e\u0440\u0438\u0442\u043c\u043e\u0432 (Ponomarchuk S.N., Grozov V.P<\/em>. <\/strong>Automatic interpretation of oblique sounding ionograms based on hybrid algorithms)<\/td>109\u2013118<\/td>PDF<\/strong><\/a><\/td>102\u2013110<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u043e\u0432\u0430\u043b\u044c \u0410.\u0412., \u0413\u0430\u0432\u0440\u0438\u043b\u043e\u0432 \u041d.\u041c., \u0413\u043e\u043b\u043e\u0432\u043a\u043e \u0410.\u0413., \u0414\u0438\u0434\u0435\u043d\u043a\u043e \u041a.\u0410., \u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u0422.\u0421<\/em>. <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0432\u043b\u0438\u044f\u043d\u0438\u044f \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043d\u0430 \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u0443\u044e \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u0443\u044e \u0446\u0438\u0440\u043a\u0443\u043b\u044f\u0446\u0438\u044e (Koval A.V., Gavrilov N.M., Didenko K.A., Ermakova T.S<\/em>. <\/strong>Modeling the impact of solar activity variations on global atmospheric circulation)<\/td>119\u2013126<\/td>PDF<\/strong><\/a><\/td>111\u2013118<\/td>PDF<\/strong><\/a><\/td><\/tr><\/tbody><\/table><\/figure>","protected":false},"excerpt":{"rendered":"

\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. \ufeff Pp. \ufeff \u0411\u0435\u043b\u043e\u0432 \u0421.\u0410., \u041b\u0435\u0434\u0435\u043d\u0446\u043e\u0432 \u041b.\u0421., \u0417\u0430\u0432\u0435\u0440\u0448\u0438\u043d\u0441\u043a\u0438\u0439 \u0414.\u0418., \u0411\u043e\u0433\u0430\u0447\u0451\u0432 \u0421.\u0410. \u0414\u0438\u0444\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u0430\u043b\u044c\u043d\u0430\u044f \u043c\u0435\u0440\u0430 \u044d\u043c\u0438\u0441\u0441\u0438\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u043d\u0430\u043d\u043e\u0432\u0441\u043f\u044b\u0448\u0435\u043a, \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u043d\u0430\u044f \u0441 \u043f\u043e\u043c\u043e\u0449\u044c\u044e \u0430\u043b\u0433\u043e\u0440\u0438\u0442\u043c\u0430 SITES (Belov S.A., Ledentsov L.S., Zavershinskii D.I., Bogachev S.A. Differential emission measure of solar nanoflares measured with the SITES algorithm) 4\u201314 PDF 3\u201312 PDF \u0420\u0430\u0445\u043c\u0430\u043d\u043e\u0432\u0430 \u041b.\u0421., \u0425\u043e\u0445\u043b\u0430\u0447\u0435\u0432 \u0410.\u0410., \u0420\u044f\u0437\u0430\u043d\u0446\u0435\u0432\u0430 \u041c.\u041e., \u0415\u0440\u043c\u043e\u043b\u0430\u0435\u0432 \u042e.\u0418., \u0417\u0430\u0441\u0442\u0435\u043d\u043a\u0435\u0440 […]<\/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-8073","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8073","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=8073"}],"version-history":[{"count":12,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8073\/revisions"}],"predecessor-version":[{"id":9704,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8073\/revisions\/9704"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8073"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8073"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8073"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}