{"id":8036,"date":"2025-04-23T00:29:03","date_gmt":"2025-04-23T00:29:03","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8036"},"modified":"2025-10-30T08:07:41","modified_gmt":"2025-10-30T08:07:41","slug":"solnechno-zemnaya-fizika-tom-6-%e2%84%961-2020","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-6-%e2%84%961-2020\/","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, \u21161, 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>
\u041a\u0443\u043f\u0440\u0438\u044f\u043d\u043e\u0432\u0430 \u0415.\u0413., \u041a\u043e\u043b\u043e\u0442\u043a\u043e\u0432 \u0414.\u042e., \u041d\u0430\u043a\u0430\u0440\u044f\u043a\u043e\u0432 \u0412.\u041c., \u041a\u0430\u0443\u0444\u043c\u0430\u043d<\/em><\/strong> \u0410.\u0421. <\/em><\/strong>\u041a\u0432\u0430\u0437\u0438\u043f\u0435\u0440\u0438\u043e\u0434\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0438 \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0438 \u0437\u0432\u0435\u0437\u0434\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u043a\u0430\u0445. \u041e\u0431\u0437\u043e\u0440 (Kupriyanova E.G.,<\/em><\/strong> Kolotkov D.Yu., Nakariakov V.M., Kaufman A.S.<\/strong><\/em> <\/strong>Quasi-periodic pulsations in solar and stellar flares. Review)<\/td>3\u201329<\/td>PDF<\/a><\/strong><\/td>3\u201323<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e., \u041a\u0440\u0438\u0432\u043e\u0448\u0430\u043f\u043a\u0438\u043d \u041f.\u0410., \u041a\u0440\u044b\u043c\u0441\u043a\u0438\u0439 \u0413.\u0424., \u0413\u0435\u0440\u0430\u0441\u0438\u043c\u043e\u0432\u0430 \u0421.\u041a<\/em>. <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0433\u043b\u0430\u0432\u043d\u044b\u0445 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442 \u0432\u043b\u0438\u044f\u043d\u0438\u044f \u0433\u0435\u043e\u043c\u0435\u0442\u0440\u0438\u0438 \u043d\u0435\u0439\u0442\u0440\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0442\u043e\u043a\u043e\u0432\u043e\u0433\u043e \u0441\u043b\u043e\u044f \u0433\u0435\u043b\u0438\u043e\u0441\u0444\u0435\u0440\u044b \u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043d\u0430 \u043c\u043e\u0434\u0443\u043b\u044f\u0446\u0438\u044e \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 (Gololobov P.Yu., Krivoshapkin P.A., Krymsky G.F., Gerasimova S.K.<\/em> <\/strong>Investigating the influence of geometry of the heliospheric neutral current sheet and solar activity on modulation of galactic cosmic rays with a method of main components)<\/td>30\u201335<\/td>PDF<\/a><\/strong><\/td>24\u201328<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0435\u0440\u0435\u0433\u0443\u0434\u043e\u0432 \u0414.\u0412., \u0421\u043e\u043b\u043e\u0432\u044c\u0435\u0432 \u0410.\u0410., \u042f\u0448\u0438\u043d \u0418.\u0418., \u0428\u0443\u0442\u0435\u043d\u043a\u043e \u0412.\u0412.<\/em> <\/strong>\u041c\u043e\u0434\u0435\u043b\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0435 \u0430\u043d\u0438\u0437\u043e\u0442\u0440\u043e\u043f\u0438\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 (Peregoudov D.V., Soloviev A.A., Yashin I.I., Shutenko V.V.<\/em> <\/strong>Galactic cosmic ray anisotropy modelling)<\/td>36\u201342<\/td>PDF<\/a><\/strong><\/td>29\u201334<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0435\u0432 \u0420.\u041d., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u041c.\u0421<\/em>. <\/strong>\u0421\u0432\u044f\u0437\u044c \u0438\u043d\u0434\u0435\u043a\u0441\u0430 ASY-H<\/em> \u0441 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430\u043c\u0438 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u0441\u0440\u0435\u0434\u044b \u0438 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u044c\u044e \u043d\u0430 \u0433\u043b\u0430\u0432\u043d\u044b\u0445 \u0444\u0430\u0437\u0430\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0441\u043e\u0431\u044b\u0442\u0438\u0439 CIR \u0438 ICME (Boroyev R.N., Vasiliev M.S.<\/em> <\/strong>Relationship of the ASY-H<\/em> index with interplanetary medium parameters and auroral activity in magnetic storm main phases during CIR and ICME events)<\/td>43\u201350<\/td>PDF<\/a><\/strong><\/td>35\u201340<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u0443\u0440\u0430\u0436\u043a\u043e\u0432\u0441\u043a\u0430\u044f \u041d.\u0410<\/em>. <\/strong>\u0413\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u0430\u044f \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0441\u0442\u044c \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b \u0417\u0435\u043c\u043b\u0438 \u0438 \u0435\u0435 \u0441\u0432\u044f\u0437\u044c \u0441 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043f\u043e\u0433\u043e\u0434\u043e\u0439 (Kurazhkovskaya N.A<\/em>. <\/strong>Global disturbance of Earth\u2019s magnetosphere and its connection with space weather)<\/td>51\u201362<\/td>PDF<\/a><\/strong><\/td>41\u201349<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0435\u0442\u0440\u0430\u0449\u0443\u043a \u0410.\u0412., \u041a\u043b\u0438\u043c\u0443\u0448\u043a\u0438\u043d \u0414.\u042e.<\/em> <\/strong>\u041f\u0440\u043e\u0441\u0442\u0440\u0430\u043d\u0441\u0442\u0432\u0435\u043d\u043d\u0430\u044f \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u0430 \u0430\u0437\u0438\u043c\u0443\u0442\u0430\u043b\u044c\u043d\u043e-\u043c\u0435\u043b\u043a\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u0445 \u041c\u0413\u0414-\u0432\u043e\u043b\u043d \u0432 \u043e\u0434\u043d\u043e\u043c\u0435\u0440\u043d\u043e-\u043d\u0435\u043e\u0434\u043d\u043e\u0440\u043e\u0434\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u0435 \u043a\u043e\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0434\u0430\u0432\u043b\u0435\u043d\u0438\u044f \u0441 \u043a\u0440\u0438\u0432\u044b\u043c\u0438 \u0441\u0438\u043b\u043e\u0432\u044b\u043c\u0438 \u043b\u0438\u043d\u0438\u044f\u043c\u0438 (Petrashchuk A.V., Klimushkin<\/em><\/strong> <\/em>D.Yu<\/em>. <\/strong>Spatial structure of azimuthally small-scale MHD waves in one-dimensionally inhomogeneous finite pressure plasma with curved field lines)<\/td>63\u201374<\/td>PDF<\/a><\/strong><\/td>50\u201359<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0420\u0443\u0431\u0446\u043e\u0432 \u0410.\u0412., \u041c\u0430\u043b\u0435\u0446\u043a\u0438\u0439 \u0411.\u041c., \u0414\u0430\u043d\u0438\u043b\u044c\u0447\u0443\u043a \u0415.\u0418., \u0421\u043c\u043e\u0442\u0440\u043e\u0432\u0430<\/em><\/strong> \u0415.\u0415., \u0428\u0435\u043b\u043a\u043e\u0432<\/strong> \u0410.\u0414., \u042f\u0441\u044e\u043a\u0435\u0432\u0438\u0447<\/strong> \u0410.\u0421<\/strong><\/em>. <\/strong>\u0412\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0430\u0434 \u0412\u043e\u0441\u0442\u043e\u0447\u043d\u043e\u0439 \u0421\u0438\u0431\u0438\u0440\u044c\u044e \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c 12\u201315 \u0430\u043f\u0440\u0435\u043b\u044f 2016 \u0433. (Rubtsov A.V., Maletckii B.M., Danilchuk E.I., Smotrova E.E., Shelkov A.D., Yasyukevich<\/em><\/strong> A.S.<\/strong><\/em> <\/strong>Ionospheric disturbances over Eastern Siberia during April 12\u201315, 2016 geomagnetic storms)<\/td>75\u201385<\/td>PDF<\/a><\/strong><\/td>60\u201368<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0410\u043a\u0441\u0435\u043d\u043e\u0432 \u041e.\u042e., \u041a\u043e\u0437\u043b\u043e\u0432 \u0421.\u0418., \u041b\u044f\u0445\u043e\u0432 \u0410.\u041d., \u0422\u0440\u0435\u043a\u0438\u043d \u0412.\u0412., \u041f\u0435\u0440\u0443\u043d\u043e\u0432 \u042e.\u041c., \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. I. \u041a\u043b\u0430\u0441\u0441\u0438\u0444\u0438\u043a\u0430\u0446\u0438\u044f \u043f\u0440\u0438\u043a\u043b\u0430\u0434\u043d\u044b\u0445 \u043c\u043e\u0434\u0435\u043b\u0435\u0439 \u0438 \u043e\u0441\u043d\u043e\u0432\u043d\u044b\u0435 \u0442\u0440\u0435\u0431\u043e\u0432\u0430\u043d\u0438\u044f, \u043f\u0440\u0435\u0434\u044a\u044f\u0432\u043b\u044f\u0435\u043c\u044b\u0435 \u043a \u043d\u0438\u043c \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\u0440\u0435\u0434\u0441\u0442\u0432 (Aksenov O.Yu., Kozlov S.I., Lyakhov A.N., Trekin V.V., Perunov Yu.M., Yakubovsky S.V. <\/em><\/strong>Analyzing existing applied models of the ionosphere for calculating radio wave propagation and possibility of their use for radar systems. I. Classification of applied models and the main requirements imposed on them for radar aids)<\/td>86\u201396<\/td>PDF<\/a><\/strong><\/td>69\u201376<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0410\u043b\u0441\u0430\u0442\u043a\u0438\u043d \u0421.\u0421., \u041c\u0435\u0434\u0432\u0435\u0434\u0435\u0432 \u0410.\u0412., \u0420\u0430\u0442\u043e\u0432\u0441\u043a\u0438\u0439<\/em><\/strong> \u041a.\u0413.<\/strong><\/em> <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u043c\u0435\u0442\u043e\u0434\u0430 \u0432\u043e\u0441\u0441\u0442\u0430\u043d\u043e\u0432\u043b\u0435\u043d\u0438\u044f N<\/em>e<\/sub> \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 (Alsatkin S.S., Medvedev A.V.,<\/em><\/strong> Ratovsky K.G.<\/strong><\/em> <\/strong>Features of N<\/em>e<\/sub> recovery at the Irkutsk Incoherent Scatter Radar)<\/td>97\u2013110<\/td>PDF<\/a><\/strong><\/td>77\u201388<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u041a\u043b\u0430\u0439\u043d \u0411.\u0418.<\/em> <\/strong>\u041e \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0438 \u0421\u043e\u043b\u043d\u0446\u0430 \u043d\u0430 \u0441\u0435\u0439\u0441\u043c\u0438\u0447\u043d\u043e\u0441\u0442\u044c \u0417\u0435\u043c\u043b\u0438 (Guglielmi A.V., Klain<\/em><\/strong> <\/em>B.I.<\/em> <\/strong>Effect of the Sun on Earth\u2019s seismicity)<\/td>111\u2013115<\/td>PDF<\/a><\/strong><\/td>89\u201392<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0420\u0443\u0436\u0438\u0447 \u0412.\u0412., \u041b\u0435\u0432\u0438\u043d\u0430 \u0415.\u0410.<\/em> <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u0441\u0435\u0439\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0432 \u0440\u0430\u0437\u043d\u044b\u0445 \u0440\u0435\u0433\u0438\u043e\u043d\u0430\u0445 \u0417\u0435\u043c\u043b\u0438 \u043f\u043e \u0444\u0430\u0437\u0430\u043c 11-\u043b\u0435\u0442\u043d\u0435\u0433\u043e \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0446\u0438\u043a\u043b\u0430 (Ruzhich V.V., Levina E.A.<\/em> <\/strong>Features of distribution of seismic activity in different regions of Earth over phases of the 11-year solar cycle)<\/td>116\u2013125<\/td>PDF<\/a><\/strong><\/td>93\u2013101<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0428\u0438\u0445\u043e\u0432\u0446\u0435\u0432 \u0410.\u042e., \u041a\u043e\u0432\u0430\u0434\u043b\u043e \u041f.\u0413., \u041a\u0438\u0441\u0435\u043b\u0435\u0432 \u0410.\u0412<\/em><\/strong>.<\/em> \u041e \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u043a\u0435 \u0430\u0441\u0442\u0440\u043e\u043a\u043b\u0438\u043c\u0430\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a \u0432 \u0421\u0430\u044f\u043d\u0441\u043a\u043e\u0439 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u043e\u0431\u0441\u0435\u0440\u0432\u0430\u0442\u043e\u0440\u0438\u0438 (Shikhovtsev A.Yu., Kovadlo P.G., Kiselev A.V<\/em>. <\/strong>Astroclimatic statistics at the Sayan Solar Observatory)<\/td>126\u2013133<\/td>PDF<\/a><\/strong><\/td>102\u2013107<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u043d\u0447\u0443\u043a\u043e\u0432\u0441\u043a\u0438\u0439<\/em><\/strong> \u0412.\u041b.<\/strong><\/em> <\/strong>\u0412\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0438\u043d\u0442\u0435\u043d\u0441\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043c\u044e\u043e\u043d\u043e\u0432 \u0438 \u0442\u0435\u043c\u043f\u0435\u0440\u0430\u0442\u0443\u0440\u0430 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b (Yanchukovskiy<\/em><\/strong> V.L<\/strong><\/em>. <\/strong>Muon intensity variations and atmospheric temperature)<\/td>134\u2013141<\/td>PDF<\/a><\/strong><\/td>108\u2013115<\/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. Pp. \u041a\u0443\u043f\u0440\u0438\u044f\u043d\u043e\u0432\u0430 \u0415.\u0413., \u041a\u043e\u043b\u043e\u0442\u043a\u043e\u0432 \u0414.\u042e., \u041d\u0430\u043a\u0430\u0440\u044f\u043a\u043e\u0432 \u0412.\u041c., \u041a\u0430\u0443\u0444\u043c\u0430\u043d \u0410.\u0421. \u041a\u0432\u0430\u0437\u0438\u043f\u0435\u0440\u0438\u043e\u0434\u0438\u0447\u0435\u0441\u043a\u0438\u0435 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0438 \u0432 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0438 \u0437\u0432\u0435\u0437\u0434\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u043a\u0430\u0445. \u041e\u0431\u0437\u043e\u0440 (Kupriyanova E.G., Kolotkov D.Yu., Nakariakov V.M., Kaufman A.S. Quasi-periodic pulsations in solar and stellar flares. Review) 3\u201329 PDF 3\u201323 PDF \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e., \u041a\u0440\u0438\u0432\u043e\u0448\u0430\u043f\u043a\u0438\u043d \u041f.\u0410., \u041a\u0440\u044b\u043c\u0441\u043a\u0438\u0439 \u0413.\u0424., \u0413\u0435\u0440\u0430\u0441\u0438\u043c\u043e\u0432\u0430 \u0421.\u041a. \u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0433\u043b\u0430\u0432\u043d\u044b\u0445 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442 \u0432\u043b\u0438\u044f\u043d\u0438\u044f \u0433\u0435\u043e\u043c\u0435\u0442\u0440\u0438\u0438 \u043d\u0435\u0439\u0442\u0440\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0442\u043e\u043a\u043e\u0432\u043e\u0433\u043e […]<\/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-8036","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8036","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=8036"}],"version-history":[{"count":7,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8036\/revisions"}],"predecessor-version":[{"id":9858,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8036\/revisions\/9858"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8036"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8036"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8036"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}