{"id":8057,"date":"2025-04-23T03:57:16","date_gmt":"2025-04-23T03:57:16","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8057"},"modified":"2025-09-30T02:51:45","modified_gmt":"2025-09-30T02:51:45","slug":"solnechno-zemnaya-fizika-tom-8-%e2%84%962-2022","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-8-%e2%84%962-2022\/","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 8, \u21162, 2022"},"content":{"rendered":"
\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/strong><\/td>\u0421\u0442\u0440.<\/strong><\/td><\/td>Pp.<\/strong><\/td><\/td><\/tr>
\u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418.<\/strong> <\/em>\u041a\u043e\u0433\u0435\u0440\u0435\u043d\u0442\u043d\u043e\u0435 \u043c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0435 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u0435 \u043a\u0430\u043a \u0438\u043d\u0434\u0438\u043a\u0430\u0442\u043e\u0440 \u043d\u0435\u0442\u0435\u043f\u043b\u043e\u0432\u043e\u0433\u043e \u044d\u043d\u0435\u0440\u0433\u043e\u0432\u044b\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0432 \u0440\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u0439 \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0439 \u0442\u043e\u0447\u043a\u0435 (Altyntsev A.T., Meshalkina N.S., Myshyakov<\/em><\/strong> I.I<\/strong><\/em>. <\/strong>Coherent microwave emission as an indicator of non-thermal energy release at a coronal X-ray point)<\/td>4\u201311<\/td>PDF<\/a><\/strong><\/td>3\u20139<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u0412.\u0413., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u041c.\u0412., \u0417\u0438\u043c\u043e\u0432\u0435\u0446 \u0418.\u0412.<\/em><\/strong> \u041e \u0432\u043e\u0437\u043c\u043e\u0436\u043d\u043e\u043c \u0440\u0430\u0437\u043b\u0438\u0447\u0438\u0438 \u0432 \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0438 \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u044b\u0445 \u0432\u044b\u0431\u0440\u043e\u0441\u043e\u0432 \u043c\u0430\u0441\u0441\u044b \u0434\u0432\u0443\u0445 \u0442\u0438\u043f\u043e\u0432 (Eselevich V.G., Eselevich M.V., Zimovets I.V.<\/em><\/strong> Possible difference in the formation of coronal mass <\/em>ejections of two types<\/em>)<\/td>12\u201322<\/td>PDF<\/a><\/strong><\/td>10\u201319<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0428\u0438\u0445\u043e\u0432\u0446\u0435\u0432 \u0410.\u042e., \u041a\u0438\u0441\u0435\u043b\u0435\u0432 \u0410.\u0412., \u041a\u043e\u0432\u0430\u0434\u043b\u043e \u041f.\u0413., \u041a\u043e\u043b\u043e\u0431\u043e\u0432 \u0414.\u042e., \u0420\u0443\u0441\u0441\u043a\u0438\u0445 \u0418.\u0412., \u0422\u043e\u043c\u0438\u043d \u0412.\u0415<\/em>. <\/strong>\u0424\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0438\u0441\u043a\u0430\u0436\u0435\u043d\u0438\u0439 \u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0433\u043e \u0444\u0440\u043e\u043d\u0442\u0430 \u043d\u0430 \u0440\u0430\u0437\u043d\u044b\u0445 \u0432\u044b\u0441\u043e\u0442\u0430\u0445 \u0432 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0435. \u0418\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u044f, \u0432\u044b\u043f\u043e\u043b\u043d\u0435\u043d\u043d\u044b\u0435 \u0441 \u043f\u043e\u043c\u043e\u0449\u044c\u044e \u0434\u0430\u0442\u0447\u0438\u043a\u0430 \u0428\u044d\u043a\u0430\u2014\u0413\u0430\u0440\u0442\u043c\u0430\u043d\u0430 (Shikhovtsev A.Yu., Kiselev A.V., Kovadlo P.G., Kolobov D.Yu., Russkikh I.V., Tomin V.E.<\/em> <\/strong>Turbulent parameters at different heights in the atmosphere. Shack\u2014Hartmann<\/em> wavefront sensor data)<\/td>23\u201328<\/td>PDF<\/a><\/strong><\/td>20\u201325<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041b\u0443\u043a\u043e\u0432\u043d\u0438\u043a\u043e\u0432\u0430 \u0410.\u0410., \u0421\u0434\u043e\u0431\u043d\u043e\u0432 \u0412.\u0415<\/em>. <\/strong>\u041f\u0438\u0442\u0447-\u0443\u0433\u043b\u043e\u0432\u0430\u044f \u0430\u043d\u0438\u0437\u043e\u0442\u0440\u043e\u043f\u0438\u044f \u0438 \u0434\u0438\u0444\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u0430\u043b\u044c\u043d\u044b\u0435 \u0436\u0435\u0441\u0442\u043a\u043e\u0441\u0442\u043d\u044b\u0435 \u0441\u043f\u0435\u043a\u0442\u0440\u044b \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 \u0432\u043e \u0432\u0440\u0435\u043c\u044f GLE 2 \u0438 6 \u043c\u0430\u044f 1998 \u0433. (Lukovnikova A.A., Sdobnov V.E.<\/em> <\/strong>Pitch-angle anisotropy and differential rigidity spectra of cosmic rays during GLE on May 2 and 6, 1998)<\/td>29\u201333<\/td>PDF<\/a><\/strong><\/td>26\u201330<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0414\u043c\u0438\u0442\u0440\u0438\u0435\u043d\u043a\u043e<\/em><\/strong> \u0418.\u0421.<\/strong><\/em> <\/strong>\u0412\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f \u0432\u0442\u043e\u0440\u043e\u0433\u043e \u043f\u043e\u0440\u044f\u0434\u043a\u0430 \u0432 \u0430\u043b\u044c\u0444\u0432\u0435\u043d\u043e\u0432\u0441\u043a\u0438\u0445 \u0432\u043e\u043b\u043d\u0430\u0445 \u0432 \u043f\u043b\u0430\u0437\u043c\u0435 \u0441 \u0434\u0430\u0432\u043b\u0435\u043d\u0438\u0435\u043c (Dmitrienko I.S<\/em>.<\/strong> Second-order perturbations in Alfv\u00e9n waves in finite pressure plasma)<\/td>34\u201340<\/td>PDF<\/a><\/strong><\/td>31\u201336<\/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., \u0426\u044d\u0433\u043c\u044d\u0434 \u0411., \u0425\u043e\u043c\u0443\u0442\u043e\u0432 \u0421.\u042e., \u0422\u0435\u0440\u043e \u0420\u0430\u0439\u0442\u0430, \u041f\u043e\u043f\u043e\u0432 \u0413.\u0412., \u041c\u043e\u0447\u0430\u043b\u043e\u0432 \u0410.\u0410., \u041f\u0438\u043b\u044c\u0433\u0430\u0435\u0432 \u0421.\u0412., \u0420\u0430\u0445\u043c\u0430\u0442\u0443\u043b\u0438\u043d<\/em><\/strong> \u0420.\u0410.<\/strong><\/em> \u041e \u0441\u043e\u043e\u0442\u0432\u0435\u0442\u0441\u0442\u0432\u0438\u0438 \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u043e\u0439 \u0438\u0437\u043e\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u043d\u043e\u0439 \u0441\u0443\u0431\u0431\u0443\u0440\u0438 \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043c\u043e\u0434\u0435\u043b\u0438 \u041c\u0430\u043a-\u0424\u0435\u0440\u0440\u043e\u043d\u0430 (Parkhomov V.A.<\/strong><\/em>, Eselevich V.G., Eselevich M.V., Tsegmed B., Khomutov S.Yu., Tero Raita, Popov G.V., Mochalov A.A., Pilgaev S.V., Rakhmatulin R.A<\/em>. <\/strong>Correspondence of a global isolated substorm to the McPherron statistical model)<\/td>41\u201351<\/td>PDF<\/a><\/strong><\/td>37\u201346<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u0440\u0447\u0443\u043a \u0420.\u0410., \u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421., \u041c\u0438\u0448\u0438\u043d \u0412.\u0412<\/em>. <\/strong>\u0421\u0438\u043d\u0445\u0440\u043e\u043d\u043d\u044b\u0435 \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u043e \u043d\u0430\u0431\u043b\u044e\u0434\u0430\u0435\u043c\u044b\u0435 \u0443\u043b\u044c\u0442\u0440\u0430\u043a\u043e\u0440\u043e\u0442\u043a\u043e\u043f\u0435\u0440\u0438\u043e\u0434\u043d\u044b\u0435 \u0438\u043c\u043f\u0443\u043b\u044c\u0441\u044b (Marchuk R.A., Potapov A.S., Mishin V.V<\/em>. <\/strong>Synchronous globally observable ultrashort-period pulses)<\/td>52\u201360<\/td>PDF<\/a><\/strong><\/td>47\u201355<\/td>PDF<\/a><\/strong><\/td><\/tr>
 \u0414\u0430\u0448\u043a\u0435\u0432\u0438\u0447 \u0416.\u0412., \u0418\u0432\u0430\u043d\u043e\u0432 \u0412.\u0415<\/em>. <\/strong>\u0414\u0438\u0430\u0433\u043d\u043e\u0441\u0442\u0438\u043a\u0430 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0435\u0439 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0438 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043d\u043e\u0439 \u043a\u043e\u043d\u0446\u0435\u043d\u0442\u0440\u0430\u0446\u0438\u0438 \u0432 \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u044f\u0445 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u044d\u043c\u043f\u0438\u0440\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043c\u043e\u0434\u0435\u043b\u0435\u0439 \u0432\u044b\u0441\u044b\u043f\u0430\u043d\u0438\u0439 (Dashkevich Zh.V., Ivanov V.E<\/em>. <\/strong>Diagnostics of emission intensities and electron density in auroras based on empirical precipitation models)<\/td>61\u201366<\/td>PDF<\/a><\/strong><\/td>56\u201360<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u0441\u044e\u043a\u0435\u0432\u0438\u0447 \u0410.\u0421., \u0412\u0435\u0441\u043d\u0438\u043d<\/em><\/strong> \u0410.\u041c<\/strong><\/em>.<\/strong> \u0421\u0440\u0430\u0432\u043d\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0432 \u0441\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0439 \u0441\u0442\u0440\u0430\u0442\u043e\u0441\u0444\u0435\u0440\u0435 \u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0435 \u0432 \u0437\u0438\u043c\u043d\u0438\u0435 \u043f\u0435\u0440\u0438\u043e\u0434\u044b (Yasyukevich A.S., Vesnin A.M.<\/em><\/strong> Comparative analysis of variability in the mid-latitude stratosphere and ionosphere in winter periods)<\/td>67\u201374<\/td>PDF<\/a><\/strong><\/td>61\u201368<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u041a\u043b\u0430\u0439\u043d \u0411.\u0418., \u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421<\/em>. <\/strong>\u0412\u043e\u043b\u043d\u044b \u0410\u043b\u044c\u0432\u0435\u043d\u0430: \u043a 80-\u043b\u0435\u0442\u0438\u044e \u043e\u0442\u043a\u0440\u044b\u0442\u0438\u044f (Guglielmi A.V., Klain B.I., Potapov<\/em><\/strong> A.S.<\/strong><\/em> <\/strong>Alfv\u00e9n waves: To the 80th<\/sup> anniversary of discovery)<\/td>75\u201377<\/td>PDF<\/a><\/strong><\/td>69\u201370<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0435\u043c\u043d\u0430\u0434\u0446\u0430\u0442\u0430\u044f \u0435\u0436\u0435\u0433\u043e\u0434\u043d\u0430\u044f \u043a\u043e\u043d\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u044f \u00ab\u0424\u0438\u0437\u0438\u043a\u0430 \u043f\u043b\u0430\u0437\u043c\u044b \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0441\u0438\u0441\u0442\u0435\u043c\u0435\u00bb,<\/strong> 7\u201311 \u0444\u0435\u0432\u0440\u0430\u043b\u044f 2022 \u0433., \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0439 \u0420\u0410\u041d, \u041c\u043e\u0441\u043a\u0432\u0430, \u0420\u043e\u0441\u0441\u0438\u044f<\/strong><\/td><\/td><\/td><\/td><\/td><\/tr>
\u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410<\/em>. <\/strong>\u041e \u0444\u043e\u0440\u043c\u0435 \u0441\u043f\u0435\u043a\u0442\u0440\u0430 \u0444\u043b\u0443\u043a\u0442\u0443\u0430\u0446\u0438\u0439 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0433\u0430\u043b\u0430\u043a\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Starodubtsev S.A<\/em>. <\/strong>Shape of spectrum of galactic cosmic ray intensity <\/strong>fluctuations)<\/td>78\u201383<\/td>PDF<\/a><\/strong><\/td>71\u201375<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u0433\u043e\u0432\u0430 \u041d.\u0412<\/em>., \u041a\u043e\u0437\u044b\u0440\u0435\u0432\u0430 \u041e.\u0412<\/em>., \u041d\u043e\u0441\u0438\u043a\u043e\u0432\u0430 \u041d.\u0421<\/em>. <\/strong>\u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0438 \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0430 1\u20134 \u043c\u0413\u0446 (Pc5\/Pi3) \u0432 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u043c \u0445\u0432\u043e\u0441\u0442\u0435 \u043f\u0440\u0438 \u0440\u0430\u0437\u043d\u043e\u043c \u0443\u0440\u043e\u0432\u043d\u0435 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0432 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u0441\u0440\u0435\u0434\u0435 (Yagova N.V., Kozyreva O.V., Nosikova N.S<\/em>. <\/strong>Geomagnetic pulsations in 1\u20134 mHz frequency range (Pc5\/Pi3) in the magnetotail at different levels of disturbances in the interplanetary medium)<\/td>84\u201392<\/td>PDF<\/a><\/strong><\/td>76\u201383<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432 \u0410.\u0412., \u0421\u043e\u043b\u043e\u0432\u044c\u0435\u0432 \u0410.\u0410., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u0412\u043e\u0440\u043e\u0431\u044c\u0435\u0432\u0430 \u0413.\u0420<\/em>. <\/strong>\u0418\u043d\u0442\u0435\u0440\u0430\u043a\u0442\u0438\u0432\u043d\u0430\u044f \u043a\u043e\u043c\u043f\u044c\u044e\u0442\u0435\u0440\u043d\u0430\u044f \u043c\u043e\u0434\u0435\u043b\u044c \u0434\u043b\u044f \u043f\u0440\u043e\u0433\u043d\u043e\u0437\u0430 \u0438 \u0430\u043d\u0430\u043b\u0438\u0437\u0430 \u043f\u043e\u043b\u044f\u0440\u043d\u044b\u0445 \u0441\u0438\u044f\u043d\u0438\u0439 (Vorobev A.V., Soloviev A.A., Pilipenko V.A., Vorobeva G.R<\/em>. <\/strong>Interactive computer model for aurora forecast and analysis)<\/td>93\u2013100<\/td>PDF<\/a><\/strong><\/td>84\u201390<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0422\u0438\u0449\u0435\u043d\u043a\u043e \u0412.\u041d., \u0411\u0435\u0440\u0435\u0437\u0443\u0446\u043a\u0438\u0439 \u0410.\u0413., \u0414\u043c\u0438\u0442\u0440\u0438\u0435\u0432\u0430 \u041b.\u0420., \u041c\u0438\u0440\u043e\u0448\u043d\u0438\u0447\u0435\u043d\u043a\u043e \u0418.\u0411., \u0428\u0430\u0439\u0445\u0438\u0441\u043b\u0430\u043c\u043e\u0432 \u0418.\u0424<\/em>. <\/strong>\u0413\u0435\u043d\u0435\u0440\u0430\u0446\u0438\u044f \u0430\u043b\u044c\u0444\u0432\u0435\u043d\u043e\u0432\u0441\u043a\u0438\u0445 \u0432\u043e\u043b\u043d \u0432 \u0437\u0430\u043c\u0430\u0433\u043d\u0438\u0447\u0435\u043d\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u0435 \u0441\u0433\u0443\u0441\u0442\u043a\u0430\u043c\u0438 \u043b\u0430\u0437\u0435\u0440\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b \u043f\u0440\u0438 \u0447\u0438\u0441\u043b\u0430\u0445 \u041c\u0430\u0445\u0430 \u043c\u043d\u043e\u0433\u043e \u043c\u0435\u043d\u044c\u0448\u0435 \u0435\u0434\u0438\u043d\u0438\u0446\u044b (Tishchenko V.N., Berezutsky A.G., Dmitrieva L.R., I.B. Miroshnichenko, Shaikhislamov I.F<\/em>. <\/strong>Generation of Alfv\u00e9n waves in magnetized plasma by laser plasma bunches at Mach numbers much less than unity)<\/td>101\u2013107<\/td>PDF<\/a><\/strong><\/td>91\u201397<\/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. \ufeff Pp. \ufeff \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u041c\u044b\u0448\u044c\u044f\u043a\u043e\u0432 \u0418.\u0418. \u041a\u043e\u0433\u0435\u0440\u0435\u043d\u0442\u043d\u043e\u0435 \u043c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0435 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u0435 \u043a\u0430\u043a \u0438\u043d\u0434\u0438\u043a\u0430\u0442\u043e\u0440 \u043d\u0435\u0442\u0435\u043f\u043b\u043e\u0432\u043e\u0433\u043e \u044d\u043d\u0435\u0440\u0433\u043e\u0432\u044b\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0432 \u0440\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u0439 \u043a\u043e\u0440\u043e\u043d\u0430\u043b\u044c\u043d\u043e\u0439 \u0442\u043e\u0447\u043a\u0435 (Altyntsev A.T., Meshalkina N.S., Myshyakov I.I. Coherent microwave emission as an indicator of non-thermal energy release at a coronal X-ray point) 4\u201311 PDF 3\u20139 PDF \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u0412.\u0413., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u041c.\u0412., \u0417\u0438\u043c\u043e\u0432\u0435\u0446 \u0418.\u0412. \u041e \u0432\u043e\u0437\u043c\u043e\u0436\u043d\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-8057","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8057","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=8057"}],"version-history":[{"count":29,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8057\/revisions"}],"predecessor-version":[{"id":9378,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8057\/revisions\/9378"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8057"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8057"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8057"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}