{"id":8064,"date":"2025-04-23T04:08:20","date_gmt":"2025-04-23T04:08:20","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8064"},"modified":"2025-10-24T17:08:52","modified_gmt":"2025-10-24T17:08:52","slug":"solnechno-zemnaya-fizika-tom-9-%e2%84%964-2023","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-9-%e2%84%964-2023\/","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 9, \u21164, 2023"},"content":{"rendered":"
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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS<\/strong><\/strong><\/td>\u0421\u0442\u0440.<\/td><\/td>Pp.<\/td><\/td><\/tr>
\u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411., \u0411\u0430\u0437\u0438\u043b\u0435\u0432\u0441\u043a\u0430\u044f \u0413.A., \u041a\u0430\u043b\u0438\u043d\u0438\u043d \u041c.\u0421., \u041c\u0438\u0445\u0430\u0439\u043b\u043e\u0432 \u0412.\u0412., \u0421\u0432\u0438\u0440\u0436\u0435\u0432\u0441\u043a\u0430\u044f \u0410.\u041a., \u0421\u0432\u0438\u0440\u0436\u0435\u0432\u0441\u043a\u0438\u0439 \u041d.\u0421<\/em>. <\/strong>\u041f\u044f\u0442\u044c\u0434\u0435\u0441\u044f\u0442 \u043b\u0435\u0442 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043f\u043e\u0432\u0435\u0434\u0435\u043d\u0438\u044f \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0413\u041a\u041b \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0438\u043d\u0432\u0435\u0440\u0441\u0438\u0438 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f. I. \u041d\u0430\u0431\u043b\u044e\u0434\u0430\u0435\u043c\u044b\u0435 \u044d\u0444\u0444\u0435\u043a\u0442\u044b (Krainev M.B., Bazilevskaya G.A., Kalinin M.S., Mikhailov V.V., Svirzhevskaya A.K., Svirzhevsky<\/em><\/strong> <\/em>N.S<\/em>. <\/strong>Fifty years of studying the GCR intensity during inversion of heliospheric magnetic fields. I. Observations)<\/td>5\u201320<\/td>PDF<\/strong><\/a><\/td>3-16<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422<\/em>. <\/strong>\u042f\u0440\u043a\u0438\u0435 \u0443\u043b\u044c\u0442\u0440\u0430\u0444\u0438\u043e\u043b\u0435\u0442\u043e\u0432\u044b\u0435 \u0443\u0437\u043b\u044b \u043a\u0430\u043a \u0432\u043e\u0437\u043c\u043e\u0436\u043d\u044b\u0435 \u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u0438 \u043a\u043e\u0433\u0435\u0440\u0435\u043d\u0442\u043d\u043e\u0433\u043e \u043c\u0438\u043a\u0440\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0433\u043e \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f (Meshalkina N.S., Altyntsev A.T<\/em>. <\/strong>Bright ultraviolet knots as possible sources of coherent microwave radiation)<\/td>21\u201329<\/td>PDF<\/strong><\/a><\/td>17-24<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u041c., \u0415\u0440\u043c\u0430\u043a\u043e\u0432\u0430 \u041b.\u0412<\/em>. <\/strong>\u0410\u043a\u0442\u0438\u0432\u043d\u044b\u0435 \u0434\u043e\u043b\u0433\u043e\u0442\u044b \u0438 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0430 \u043a\u0440\u0443\u043f\u043d\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0432 \u043c\u0438\u043d\u0438\u043c\u0443\u043c\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Grigoriev V.M., Ermakova L.V<\/em>. <\/strong>Active longitudes and the structure of the large-scale magnetic field at solar minimum)<\/td>30\u201337<\/td>PDF<\/strong><\/a><\/td>25-31<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0422\u043e\u043c\u043e\u0437\u043e\u0432 \u0412.\u041c., \u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0413.\u0421., \u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0422.\u041c<\/em>. <\/strong>\u0421\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0435 \u0432\u0441\u043f\u044b\u0448\u043a\u0438 \u0441 \u043f\u0440\u043e\u0434\u043e\u043b\u0436\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u043c \u0433\u0430\u043c\u043c\u0430-\u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u0435\u043c \u0438 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0438 \u043f\u043e\u0442\u043e\u043a\u043e\u0432 \u043f\u0440\u043e\u0442\u043e\u043d\u043e\u0432 \u0432\u044b\u0441\u043e\u043a\u0438\u0445 \u044d\u043d\u0435\u0440\u0433\u0438\u0439 (Tomozov V.M., Minasyants G.S., Minasyants T.M<\/em>. <\/strong>Solar flares with sustained gamma-ray emission and some characteristics of high-energy proton fluxes)<\/td>38\u201343<\/td>PDF<\/strong><\/a><\/td>32-36<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410<\/em>. <\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u043c\u0435\u043b\u043a\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u043f\u043e\u043b\u0435\u0439 \u043f\u0435\u0440\u0435\u0434 \u043c\u0430\u043b\u044b\u043c\u0438 \u0438 \u043a\u0440\u0443\u043f\u043d\u044b\u043c\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u043c\u0438 \u0432\u0441\u043f\u044b\u0448\u043a\u0430\u043c\u0438 (Borovik A.V., Zhdanov A.A<\/em>. <\/strong>Dynamics of small-scale magnetic fields before small and large solar flares)<\/td>44\u201353<\/td>PDF<\/strong><\/a><\/td>37-45<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0421\u0435\u0442\u043e\u0432 \u0410.\u0413., \u041a\u0443\u0448\u043d\u0430\u0440\u0435\u0432 \u0414.\u0421<\/em>. <\/strong>\u041a\u043e\u0440\u0440\u0435\u043b\u044f\u0446\u0438\u043e\u043d\u043d\u044b\u0439 \u0430\u043d\u0430\u043b\u0438\u0437 \u0430\u0431\u0441\u043e\u043b\u044e\u0442\u043d\u044b\u0445 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u043f\u043e\u0442\u043e\u043a\u0430 \u043d\u0430 \u0447\u0430\u0441\u0442\u043e\u0442\u0430\u0445 161 \u0438 245 \u041c\u0413\u0446 (Setov A.G., Kushnarev D.S<\/em>. <\/strong>Correlation analysis of solar flux absolute measurements at 161 and 245 MHz)<\/td>54\u201362<\/td>PDF<\/strong><\/a><\/td>46-54<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0415\u0440\u043c\u043e\u043b\u0430\u0435\u0432 \u042e.\u0418., \u041b\u043e\u0434\u043a\u0438\u043d\u0430 \u0418.\u0413., \u0425\u043e\u0445\u043b\u0430\u0447\u0435\u0432 \u0410.\u0410., \u0415\u0440\u043c\u043e\u043b\u0430\u0435\u0432 \u041c.\u042e., \u0420\u044f\u0437\u0430\u043d\u0446\u0435\u0432\u0430 \u041c.\u041e., \u0420\u0430\u0445\u043c\u0430\u043d\u043e\u0432\u0430 \u041b.\u0421., \u0411\u043e\u0440\u043e\u0434\u043a\u043e\u0432\u0430 \u041d.\u041b., \u0421\u0430\u043f\u0443\u043d\u043e\u0432\u0430 \u041e.\u0412., \u041c\u043e\u0441\u043a\u0430\u043b\u0435\u0432\u0430 \u0410.\u0412<\/em>. <\/strong>\u041f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u044b \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u043d\u0430 \u0444\u0430\u0437\u0435 \u0440\u043e\u0441\u0442\u0430 25-\u0433\u043e \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0446\u0438\u043a\u043b\u0430: \u0441\u0445\u043e\u0434\u0441\u0442\u0432\u0430 \u0438 \u0440\u0430\u0437\u043b\u0438\u0447\u0438\u044f \u0441 23-\u043c \u0438 24-\u043c \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u043c\u0438 \u0446\u0438\u043a\u043b\u0430\u043c\u0438 (Yermolaev Yu.I., Lodkina I.G., Khokhlachev A.A., Yermolaev M.Yu., Riazantseva M.O., Rakhmanova L.S., Borodkova N.L., Sapunova O.V., Moskaleva A.V<\/em>. <\/strong>Solar wind parameters in rising phase of solar cycle 25: Similarities and differences with solar cycles 23 and 24)<\/td>63\u201370<\/td>PDF<\/strong><\/a><\/td>55-62<\/td>PDF<\/strong><\/a><\/td><\/tr>
 \u0414\u043e\u0440\u043e\u0444\u0435\u0435\u0432 \u0414.\u0410., \u0427\u0435\u0440\u043d\u044b\u0448\u043e\u0432 \u0410.\u0410., \u0427\u0443\u0433\u0443\u043d\u0438\u043d \u0414.\u0412., \u041c\u043e\u0433\u0438\u043b\u0435\u0432\u0441\u043a\u0438\u0439 \u041c.\u041c<\/em>. <\/strong>\u041e\u0441\u043d\u043e\u0432\u043d\u044b\u0435 \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u0441\u0432\u043e\u0439\u0441\u0442\u0432\u0430 \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0442\u0438\u043f\u0430 \u0433\u0435\u043a\u0442\u043e\u043c\u0435\u0442\u0440\u043e\u0432\u044b\u0439 \u043a\u043e\u043d\u0442\u0438\u043d\u0443\u0443\u043c \u0432 \u043e\u043a\u043e\u043b\u043e\u0437\u0435\u043c\u043d\u043e\u043c \u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435 (Dorofeev D.A., Chernyshov A.A., Chugunin D.V., Mogilevsky M.M<\/em>. <\/strong>Main statistical properties of hectometric continuum radiation in near-Earth space)<\/td>71\u201379<\/td>PDF<\/strong><\/a><\/td>63-71<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u042f\u043a\u0438\u043c\u0447\u0443\u043a \u0410.\u0418., \u0420\u0443\u0431\u0446\u043e\u0432 \u0410.\u0412., \u041a\u043b\u0438\u043c\u0443\u0448\u043a\u0438\u043d \u0414.\u042e<\/em>. <\/strong>\u0420\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u043f\u043e\u043b\u044f\u0440\u0438\u0437\u0430\u0446\u0438\u0438 \u043f\u043e\u043f\u0435\u0440\u0435\u0447\u043d\u044b\u0445 \u0423\u041d\u0427-\u0432\u043e\u043b\u043d \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c Van Allen Probe A: \u0441\u0443\u0449\u0435\u0441\u0442\u0432\u0443\u044e\u0442 \u043b\u0438 \u0440\u0430\u0437\u0434\u0435\u043b\u044c\u043d\u043e \u0442\u043e\u0440\u043e\u0438\u0434\u0430\u043b\u044c\u043d\u044b\u0435 \u0438 \u043f\u043e\u043b\u043e\u0438\u0434\u0430\u043b\u044c\u043d\u044b\u0435 \u0432\u043e\u043b\u043d\u044b \u0432 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u0435? (Yakimchuk A.I., Rubtsov A.V., Klimushkin D.Yu<\/em>. <\/strong>Polarization distribution of transverse ULF waves according to Van Allen Probe A data: Whether toroidal and poloidal waves exist separately in the magnetosphere?)<\/td>80\u201385<\/td>PDF<\/strong><\/a><\/td>72-77<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0411\u0430\u0438\u0448\u0435\u0432 \u0414.\u0413., \u041c\u0430\u043a\u0430\u0440\u043e\u0432 \u0413.\u0410<\/em>. <\/strong>\u0418\u0437\u043e\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u043d\u044b\u0435 \u0441\u0443\u0431\u0431\u0443\u0440\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u0439 \u0432 \u0422\u0438\u043a\u0441\u0438 \u0432 \u043f\u0435\u0440\u0438\u043e\u0434 \u043c\u0438\u043d\u0438\u043c\u0430\u043b\u044c\u043d\u043e\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 (Baishev D.G., Makarov G.A<\/em>. <\/strong>Isolated substorms according to magnetic measurement at Tixie during minimum solar activity)<\/td>86\u201390<\/td>PDF<\/strong><\/a><\/td>78\u201382<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u0418\u043b\u044c\u0438\u043d \u041d.\u0412., \u041f\u0435\u043d\u0437\u0438\u043d \u041c.\u0421., \u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d.<\/em>,<\/strong> \u0425\u0430\u0445\u0438\u043d\u043e\u0432<\/em> <\/strong>\u0412.\u0412<\/em>. <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u041a\u0412-\u0440\u0430\u0434\u0438\u043e\u043a\u0430\u043d\u0430\u043b\u0430 \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 (Kurkin V.I.<\/em>.<\/strong>, Ilyin N.V., Penzin M.S., Ponomarchuk S.N.<\/em>,<\/strong> Khakhinov<\/em> <\/strong>V.V<\/em>. <\/strong>HF radio channel modeling by a waveguide approach)<\/td>91\u2013103<\/td>PDF<\/strong><\/a><\/td>83\u201394<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041a\u043e\u0437\u043b\u043e\u0432 \u0421.\u0418., \u041b\u044f\u0445\u043e\u0432 \u0410.\u041d.<\/em> <\/strong>\u0420\u0430\u0441\u0447\u0435\u0442\u044b \u0444\u043e\u0442\u043e\u043e\u0442\u043b\u0438\u043f\u0430\u043d\u0438\u044f \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u043e\u0442 \u041e\u2013<\/sup> \u0438 \u041e2<\/sub>\u2013<\/sup> \u0432 \u043e\u0431\u043b\u0430\u0441\u0442\u0438 D \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u0437\u0430\u0432\u0438\u0441\u0438\u043c\u043e\u0441\u0442\u0438 \u043e\u0442 \u0432\u044b\u0441\u043e\u0442\u044b, \u0437\u0435\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u0443\u0433\u043b\u0430 \u0438 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0421\u043e\u043b\u043d\u0446\u0430 (Kozlov S.I., Laykhov<\/em><\/strong> A.N<\/strong><\/em>. <\/strong>Photodetachment rates for \u041e\u2013<\/sup> and \u041e2<\/sub>\u2013 <\/sup>in the D layer of the ionosphere as function of solar zenith angle and solar activity)<\/td>104\u2013107<\/td>PDF<\/strong><\/a><\/td>95\u201398<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0427\u0435\u0440\u043d\u0438\u0433\u043e\u0432\u0441\u043a\u0430\u044f \u041c.\u0410., \u042f\u0441\u044e\u043a\u0435\u0432\u0438\u0447 \u0410.\u0421., \u0425\u0430\u0431\u0438\u0442\u0443\u0435\u0432 \u0414.\u0421<\/em>. <\/strong>\u0414\u043e\u043b\u0433\u043e\u0442\u043d\u0430\u044f \u0438\u0437\u043c\u0435\u043d\u0447\u0438\u0432\u043e\u0441\u0442\u044c \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0421\u0435\u0432\u0435\u0440\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u0443\u0448\u0430\u0440\u0438\u044f \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0438\u043e\u043d\u043e\u0437\u043e\u043d\u0434\u043e\u0432 \u0438 GPS\/\u0413\u041b\u041e\u041d\u0410\u0421\u0421 (Chernigovskaya M.A., Yasyukevich A.S., Khabituev<\/em><\/strong> D.S<\/strong><\/em>. <\/strong>Ionospheric longitudinal variability in the Northern Hemisphere during magnetic storms in March 2012 from ionosonde and GPS\/GLONASS data)<\/td>108\u2013120<\/td>PDF<\/strong><\/a><\/td>99\u2013110<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u0411\u0435\u043b\u043e\u0432 \u0418.\u041e., \u0421\u043e\u043b\u043e\u0432\u044c\u0435\u0432 \u0410.\u0410., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410.,<\/em><\/strong> \u0414\u043e\u0431\u0440\u043e\u0432\u043e\u043b\u044c\u0441\u043a\u0438\u0439 \u041c.\u041d., \u0411\u043e\u0433\u043e\u0443\u0442\u0434\u0438\u043d\u043e\u0432 \u0428.\u0420., \u041a\u0430\u043b\u0438\u043d\u043a\u0438\u043d \u041a.\u0414<\/strong><\/em>. <\/strong>\u041e\u043d\u043b\u0430\u0439\u043d-\u0441\u0438\u0441\u0442\u0435\u043c\u0430 \u0434\u043b\u044f \u0430\u043d\u0430\u043b\u0438\u0437\u0430 \u0442\u043e\u043a\u043e\u0432 \u0432 \u0432\u0435\u0440\u0445\u043d\u0435\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0435 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432 Swarm (Belov I.O., Soloviev A.A., Pilipenko V.A., Bogoutdinov Sh.R., Kalinkin K.D<\/em>. <\/strong>Online system for analyzing currents in the upper ionosphere according to Swarm satellite data)<\/td>121\u2013133<\/td>PDF<\/strong><\/a><\/td>111\u2013122<\/td>PDF<\/strong><\/a><\/td><\/tr>
\u041c\u043e\u0440\u0434\u0432\u0438\u043d\u043e\u0432 \u0412.\u0418., \u0414\u0435\u0432\u044f\u0442\u043e\u0432\u0430 \u0415.\u0412., \u0422\u043e\u043c\u043e\u0437\u043e\u0432 \u0412.\u041c<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0438 \u043a\u043e\u043d\u0444\u0438\u0433\u0443\u0440\u0430\u0446\u0438\u0438 \u0441\u0440\u0435\u0434\u043d\u0435\u0433\u043e \u0442\u0435\u0447\u0435\u043d\u0438\u044f \u043d\u0430 \u043f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u0443\u044e \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0443 \u0438 \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u044c \u0440\u043e\u0441\u0442\u0430 \u043d\u043e\u0440\u043c\u0430\u043b\u044c\u043d\u044b\u0445 \u043c\u043e\u0434 (Mordvinov V.I., Devyatova E.V., Tomozov V.M<\/em>. <\/strong>Influence of the magnetic field and the mean flow configuration on spatial structure and growth rate of normal modes)<\/td>134\u2013146<\/td>PDF<\/strong><\/a><\/td>123\u2013135<\/td>PDF<\/strong><\/a><\/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. \ufeff Pp. \ufeff \u041a\u0440\u0430\u0439\u043d\u0435\u0432 \u041c.\u0411., \u0411\u0430\u0437\u0438\u043b\u0435\u0432\u0441\u043a\u0430\u044f \u0413.A., \u041a\u0430\u043b\u0438\u043d\u0438\u043d \u041c.\u0421., \u041c\u0438\u0445\u0430\u0439\u043b\u043e\u0432 \u0412.\u0412., \u0421\u0432\u0438\u0440\u0436\u0435\u0432\u0441\u043a\u0430\u044f \u0410.\u041a., \u0421\u0432\u0438\u0440\u0436\u0435\u0432\u0441\u043a\u0438\u0439 \u041d.\u0421. \u041f\u044f\u0442\u044c\u0434\u0435\u0441\u044f\u0442 \u043b\u0435\u0442 \u0438\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u043f\u043e\u0432\u0435\u0434\u0435\u043d\u0438\u044f \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0413\u041a\u041b \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0438\u043d\u0432\u0435\u0440\u0441\u0438\u0438 \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f. I. \u041d\u0430\u0431\u043b\u044e\u0434\u0430\u0435\u043c\u044b\u0435 \u044d\u0444\u0444\u0435\u043a\u0442\u044b (Krainev M.B., Bazilevskaya G.A., Kalinin M.S., Mikhailov V.V., Svirzhevskaya A.K., Svirzhevsky N.S. Fifty years of studying the GCR intensity during inversion of heliospheric […]<\/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-8064","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8064","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=8064"}],"version-history":[{"count":12,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8064\/revisions"}],"predecessor-version":[{"id":9709,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8064\/revisions\/9709"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8064"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8064"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8064"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}