{"id":8042,"date":"2025-04-23T00:31:30","date_gmt":"2025-04-23T00:31:30","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8042"},"modified":"2025-10-30T07:16:09","modified_gmt":"2025-10-30T07:16:09","slug":"solnechno-zemnaya-fizika-tom-6-%e2%84%963-2020","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-6-%e2%84%963-2020\/","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, \u21163, 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>
\u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u0412.\u0413., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 M.\u0412.<\/em> <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u043d\u0430\u0447\u0430\u043b\u044c\u043d\u043e\u0439 \u0441\u0442\u0430\u0434\u0438\u0438 \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0431\u044b\u0441\u0442\u0440\u043e\u0433\u043e \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0432\u044b\u0431\u0440\u043e\u0441\u0430 \u043c\u0430\u0441\u0441\u044b 25 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 2014 \u0433. (Eselevich V.G., Eselevich M.V. <\/em><\/strong>Features of the initial stage of formation of fast coronal mass ejection on February 25, 2014)<\/td>3\u201317<\/td>PDF<\/a><\/strong><\/td>3\u201315<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410.<\/em><\/strong> \u0421\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0435 \u0432\u0441\u043f\u044b\u0448\u043a\u0438 \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 \u0432 \u043e\u043f\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u043c \u0438 \u0440\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u043c \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0430\u0445 \u0434\u043b\u0438\u043d \u0432\u043e\u043b\u043d \u0432 21\u201324-\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0446\u0438\u043a\u043b\u0430\u0445 (Borovik A.V., Zhdanov A.A.<\/em> <\/strong>Low-power solar flares of optical and X-ray wavelengths for solar cycles 21\u201324)<\/td>18\u201325<\/td>PDF<\/a><\/strong><\/td>16\u201322<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0443\u0437\u044c\u043c\u0435\u043d\u043a\u043e \u0418.\u0412.<\/em> <\/strong>\u041a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u044b\u0435 \u0434\u0436\u0435\u0442\u044b \u043a\u0430\u043a \u043f\u0440\u0438\u0447\u0438\u043d\u0430 \u0432\u043e\u0437\u043d\u0438\u043a\u043d\u043e\u0432\u0435\u043d\u0438\u044f \u043c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u044b\u0445 \u043e\u0442\u0440\u0438\u0446\u0430\u0442\u0435\u043b\u044c\u043d\u044b\u0445 \u0432\u0441\u043f\u043b\u0435\u0441\u043a\u043e\u0432 (Kuzmenko I.V.<\/em><\/strong> Coronal jets as a cause of microwave negative bursts)<\/td>26\u201332<\/td>PDF<\/a><\/strong><\/td>23\u201328<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0435\u0442\u043e\u0432 \u0410.\u0413., \u041a\u0443\u0448\u043d\u0430\u0440\u0435\u0432 \u0414.\u0421., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u041c\u0435\u0434\u0432\u0435\u0434\u0435\u0432 \u0410.\u0412.<\/em> <\/strong>\u0414\u043b\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0435 \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u043f\u043e\u0442\u043e\u043a\u0430 \u0432 2011\u20132019 \u0433\u0433. \u043d\u0430 \u0418\u0440\u043a\u0443\u0442\u0441\u043a\u043e\u043c \u0440\u0430\u0434\u0430\u0440\u0435 \u043d\u0435\u043a\u043e\u0433\u0435\u0440\u0435\u043d\u0442\u043d\u043e\u0433\u043e \u0440\u0430\u0441\u0441\u0435\u044f\u043d\u0438\u044f (\u0418\u0420\u041d\u0420) (Setov A.G., Kushnarev D.S., Vasilyev R.V., Medvedev A.V<\/em>. <\/strong>Long-term solar flux observations with Irkutsk Incoherent Scatter Radar (IISR) in 2011\u20132019)<\/td>33\u201339<\/td>PDF<\/a><\/strong><\/td>29\u201333<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0414\u0430\u043d\u0438\u043b\u043e\u0432\u0430 \u041e.\u0410., \u041f\u0442\u0438\u0446\u044b\u043d\u0430 \u041d.\u0413., \u0422\u044f\u0441\u0442\u043e \u041c.\u0418., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.E<\/em>. <\/strong>\u0412\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u0430\u044f \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u0430 7\u20138 \u043d\u043e\u044f\u0431\u0440\u044f 2004 \u0433. \u0438 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0436\u0435\u0441\u0442\u043a\u043e\u0441\u0442\u0438 \u043e\u0431\u0440\u0435\u0437\u0430\u043d\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439: \u0448\u0438\u0440\u043e\u0442\u043d\u044b\u0435 \u044d\u0444\u0444\u0435\u043a\u0442\u044b (Danilova O.A., Ptitsyna N.G.<\/em><\/strong>, Tyasto M.I., Sdobnov V.E<\/strong><\/em>. <\/strong>Disturbed magnetosphere on November 7\u20138, 2004 and variations of cosmic ray cutoff rigidity: Latitude effects)<\/td>40\u201347<\/td>PDF<\/a><\/strong><\/td>34\u201339<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421., \u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u0414\u043e\u0432\u0431\u043d\u044f \u0411.\u0412<\/em>. <\/strong>\u0423\u043b\u044c\u0442\u0440\u0430\u043d\u0438\u0437\u043a\u043e\u0447\u0430\u0441\u0442\u043e\u0442\u043d\u044b\u0435 \u044d\u043c\u0438\u0441\u0441\u0438\u0438 \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0430 0.1\u20133 \u0413\u0446 \u0432 \u043f\u0440\u0438\u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u043e\u0431\u043b\u0430\u0441\u0442\u044f\u0445 (Potapov A.S., Guglielmi A.V., Dovbnya B.V.<\/em> <\/strong>Ultra low frequency emissions ranging from 0.1 to 3 Hz in circumpolar areas)<\/td>48\u201355<\/td>PDF<\/a><\/strong><\/td>40\u201345<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u043e\u0438\u0441\u0435\u0435\u0432 \u0410.\u0412., \u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410., \u041c\u0438\u0448\u0438\u043d \u0412.\u0412.<\/em><\/strong> \u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0432\u043e\u0437\u0431\u0443\u0436\u0434\u0435\u043d\u0438\u044f \u0438 \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u044f \u043f\u043e \u0430\u0437\u0438\u043c\u0443\u0442\u0443 \u0438 \u043c\u0435\u0440\u0438\u0434\u0438\u0430\u043d\u0443 \u0434\u043b\u0438\u043d\u043d\u043e\u043f\u0435\u0440\u0438\u043e\u0434\u043d\u044b\u0445 Pi3 \u043a\u043e\u043b\u0435\u0431\u0430\u043d\u0438\u0439 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f 8 \u0434\u0435\u043a\u0430\u0431\u0440\u044f 2017 \u0433. (Moiseev A.V., Starodubtsev S.A., Mishin V.V.<\/em> <\/strong>Features of excitation and azimuthal and meridional
propagation of long-period Pi3 oscillations of the geomagnetic field on December 8, 2017)<\/td>		56\u201372<\/td>PDF<\/a><\/strong><\/td>46\u201359<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0410\u043b\u043f\u0430\u0442\u043e\u0432 \u0412.\u0412., \u0411\u0435\u043a\u043a\u0435\u0440 \u0421.\u0417., \u041a\u043e\u0437\u043b\u043e\u0432 \u0421.\u0418., \u041b\u044f\u0445\u043e\u0432 \u0410.\u041d., \u042f\u043a\u0438\u043c \u0412.\u0412., \u042f\u043a\u0443\u0431\u043e\u0432\u0441\u043a\u0438\u0439 \u0421.\u0412<\/em>.<\/strong> \u0410\u043d\u0430\u043b\u0438\u0437 \u043f\u0440\u0438\u043a\u043b\u0430\u0434\u043d\u044b\u0445 \u043c\u043e\u0434\u0435\u043b\u0435\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0434\u043b\u044f \u0440\u0430\u0441\u0447\u0435\u0442\u0430 \u0440\u0430\u0441\u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0435\u043d\u0438\u044f \u0440\u0430\u0434\u0438\u043e\u0432\u043e\u043b\u043d \u0438 \u0432\u043e\u0437\u043c\u043e\u0436\u043d\u043e\u0441\u0442\u044c \u0438\u0445 \u0438\u0441\u043f\u043e\u043b\u044c\u0437\u043e\u0432\u0430\u043d\u0438\u044f \u0432 \u0438\u043d\u0442\u0435\u0440\u0435\u0441\u0430\u0445 \u0440\u0430\u0434\u0438\u043e\u043b\u043e\u043a\u0430\u0446\u0438\u043e\u043d\u043d\u044b\u0445 \u0441\u0438\u0441\u0442\u0435\u043c. II. \u041e\u0442\u0435\u0447\u0435\u0441\u0442\u0432\u0435\u043d\u043d\u044b\u0435 \u043c\u043e\u0434\u0435\u043b\u0438 (Alpatov V.V., Bekker S.Z., Kozlov S.I., Lyakhov A.N., Yakim V.V., Yakubovsky S.V<\/em>. <\/strong>Analyzing existing applied models of the ionosphere to calculate radio wave propagation and a possibility of their use for radar-tracking systems. II. Domestic models)<\/td>73\u201381<\/td>PDF<\/a><\/strong><\/td>60\u201366<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d., \u041f\u0435\u043d\u0437\u0438\u043d \u041c.\u0421<\/em>.<\/strong> \u0418\u043d\u0432\u0435\u0440\u0441\u0438\u044f \u0438\u043e\u043d\u043e\u0433\u0440\u0430\u043c\u043c \u0432\u043e\u0437\u0432\u0440\u0430\u0442\u043d\u043e-\u043d\u0430\u043a\u043b\u043e\u043d\u043d\u043e\u0433\u043e \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0432 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u044b \u043a\u0432\u0430\u0437\u0438-\u043f\u0430\u0440\u0430\u0431\u043e\u043b\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u0441\u043b\u043e\u044f (Ponomarchuk S.N., Penzin M.S<\/em>. <\/strong>Inversion of backscatter ionograms into quasiparabolic ionospheric layer parameters)<\/td>82\u201387<\/td>PDF<\/a><\/strong><\/td>67\u201371<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042e\u0441\u0443\u043f\u043e\u0432 \u041a.\u041c., \u041c\u044d\u0442\u044c\u044e\u0437 \u0414.\u0414., \u041c\u0430\u0440\u0443\u044f\u043c\u0430 \u0422., \u0410\u043a\u0447\u0443\u0440\u0438\u043d \u0410.\u0414., \u0422\u043e\u043b\u0441\u0442\u0438\u043a\u043e\u0432 \u041c.\u0412., \u0428\u0435\u0440\u0441\u0442\u044e\u043a\u043e\u0432 \u041e.\u041d.,<\/em><\/strong> \u0424\u0438\u043b\u0438\u043f\u043f\u043e\u0432\u0430 \u0415.\u0410.,<\/strong> \u0421\u0430\u0444\u0438\u0443\u043b\u043b\u0438\u043d \u0410.\u0421<\/strong><\/em>. <\/strong>\u0410\u043c\u043f\u043b\u0438\u0442\u0443\u0434\u043d\u044b\u0435 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u043e\u0442\u0440\u0430\u0436\u0435\u043d\u043d\u043e\u0433\u043e \u0441\u0438\u0433\u043d\u0430\u043b\u0430 \u043f\u0440\u0438 \u0432\u0435\u0440\u0442\u0438\u043a\u0430\u043b\u044c\u043d\u043e\u043c \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430 \u0441\u0440\u0435\u0434\u043d\u0438\u0445 \u0448\u0438\u0440\u043e\u0442\u0430\u0445 (Yusupov K.\u041c., Mathews J.D., Maruyama T., Akchurin A.D., Tolstikov M.V., Sherstyukov O.N., Filippova<\/em><\/strong> E.A.,<\/strong><\/em> Safiullin<\/em><\/strong> A.S<\/strong><\/em>. <\/strong>Amplitude variations of the reflected signal during vertical sounding of the ionosphere at middle latitudes)<\/td>88\u201398<\/td>PDF<\/a><\/strong><\/td>72\u201380<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412.<\/em> <\/strong>\u041f\u0440\u043e\u044f\u0432\u043b\u0435\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0438 \u0434\u0438\u043d\u0430\u043c\u0438\u043a\u0438 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u044f\u0445 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u044d\u043c\u0438\u0441\u0441\u0438\u0439 \u043d\u043e\u0447\u043d\u043e\u0433\u043e \u043d\u0435\u0431\u0430 557.7 \u0438 630.0 \u043d\u043c \u0432 24-\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u043c \u0446\u0438\u043a\u043b\u0435 (Mikhalev A.V.<\/em><\/strong> Manifestation of solar activity and dynamics of the atmosphere in variations of 577.7 and 630.0 nm atmospheric emissions in solar cycle 24)<\/td>99\u2013104<\/td>PDF<\/a><\/strong><\/td>81\u201385<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u043a\u043e\u0432\u043b\u0435\u0432\u0430 \u041e.\u0415., \u041a\u0443\u0448\u043d\u0430\u0440\u0435\u043d\u043a\u043e \u0413.\u041f., \u041a\u0443\u0437\u043d\u0435\u0446\u043e\u0432\u0430<\/em><\/strong> \u0413.\u041c.<\/strong><\/em> <\/strong>\u0410\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0430 \u043d\u0430\u0434 \u041d\u043e\u0440\u0438\u043b\u044c\u0441\u043a\u043e\u043c \u043d\u0438\u0436\u0435 200 \u043a\u043c \u0432 \u0443\u0441\u043b\u043e\u0432\u0438\u044f\u0445 \u043c\u0438\u043d\u0438\u043c\u0443\u043c\u0430 \u0438 \u043c\u0430\u043a\u0441\u0438\u043c\u0443\u043c\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Yakovleva O.E., Kushnarenko G.P., Kuznetsova<\/em><\/strong> G.M.<\/strong><\/em> <\/strong>The atmosphere below 200 km over Norilsk at solar minimum and maximum)<\/td>105\u2013109<\/td>PDF<\/a><\/strong><\/td>86\u201389<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0443\u0448\u043d\u0430\u0440\u0435\u043d\u043a\u043e \u0413.\u041f., \u042f\u043a\u043e\u0432\u043b\u0435\u0432\u0430 \u041e.\u0415., \u041a\u0443\u0437\u043d\u0435\u0446\u043e\u0432\u0430<\/em><\/strong> \u0413.\u041c<\/strong><\/em>. <\/strong>\u041e\u0446\u0435\u043d\u043a\u0430 \u043e\u0442\u043d\u043e\u0448\u0435\u043d\u0438\u0439 \u043e\u0441\u043d\u043e\u0432\u043d\u044b\u0445 \u043d\u0435\u0439\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0441\u043e\u0441\u0442\u0430\u0432\u043b\u044f\u044e\u0449\u0438\u0445 \u0442\u0435\u0440\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0432 2014\u20132017 \u0433\u0433. \u043d\u0430 \u0432\u044b\u0441\u043e\u0442\u0430\u0445 \u0441\u043b\u043e\u044f F1 \u043d\u0430\u0434 \u0418\u0440\u043a\u0443\u0442\u0441\u043a\u043e\u043c (Kushnarenko G.P., Yakovleva O.E., Kuznetsova<\/em><\/strong> G.M<\/strong><\/em>. <\/strong>Estimated relations between the main thermospheric neutral components at ionospheric F1-layer heights above Irkutsk in 2014\u20132017)<\/td>110\u2013114<\/td>PDF<\/a><\/strong><\/td>90\u201393<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0440\u043e\u0431\u0446\u0435\u0432 \u0418.\u0412., \u0426\u0443\u043a\u043a\u0435\u0440 \u0422.\u0413., \u041c\u0438\u0448\u0438\u043d\u0430 \u041c.\u041d., \u0413\u043e\u0440\u044f\u0448\u0438\u043d \u0412.\u0415.,<\/em> \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u041c.\u0412.<\/em> <\/strong>\u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043c\u0443\u0441\u043e\u0440\u0430 \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u043e\u0440\u0431\u0438\u0442 \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 (Korobtsev I.V., Tsukker T.G., Mishina M.N., Goryashin V.E., Eselevich M.V<\/em>. <\/strong>Observations of space debris in the vicinity of orbits of global navigation satellite systems)<\/td>115\u2013123<\/td>PDF<\/a><\/strong><\/td>94\u2013100<\/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. \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u0412.\u0413., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 M.\u0412. \u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u043d\u0430\u0447\u0430\u043b\u044c\u043d\u043e\u0439 \u0441\u0442\u0430\u0434\u0438\u0438 \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0431\u044b\u0441\u0442\u0440\u043e\u0433\u043e \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0432\u044b\u0431\u0440\u043e\u0441\u0430 \u043c\u0430\u0441\u0441\u044b 25 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 2014 \u0433. (Eselevich V.G., Eselevich M.V. Features of the initial stage of formation of fast coronal mass ejection on February 25, 2014) 3\u201317 PDF 3\u201315 PDF \u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410. \u0421\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0435 \u0432\u0441\u043f\u044b\u0448\u043a\u0438 \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 \u0432 \u043e\u043f\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u043c \u0438 \u0440\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u043c […]<\/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-8042","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8042","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=8042"}],"version-history":[{"count":7,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8042\/revisions"}],"predecessor-version":[{"id":9804,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8042\/revisions\/9804"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8042"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8042"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8042"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}