{"id":8032,"date":"2025-04-23T00:27:46","date_gmt":"2025-04-23T00:27:46","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8032"},"modified":"2025-10-31T05:57:48","modified_gmt":"2025-10-31T05:57:48","slug":"solnechno-zemnaya-fizika-tom-5-%e2%84%963-2019-2","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-5-%e2%84%963-2019-2\/","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 5, \u21163, 2019"},"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>
\u041c\u0443\u0440\u0430\u0442\u043e\u0432\u0430 \u041d.\u041e., \u041c\u0443\u0440\u0430\u0442\u043e\u0432 \u0410.\u0410., \u041a\u0430\u0448\u0430\u043f\u043e\u0432\u0430 \u041b.\u041a.<\/em> <\/strong>\u0420\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u044b \u0440\u0430\u0431\u043e\u0442\u044b \u043d\u043e\u0432\u043e\u0433\u043e \u0441\u043f\u0435\u043a\u0442\u0440\u043e\u043f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0430 \u0434\u043b\u044f \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0432 \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0435 50\u2013500 \u041c\u0413\u0446 (Muratova N.O., Muratov A.A., Kashapova<\/em><\/strong> L.K<\/strong><\/em>. <\/strong>Results of work of new spectropolarimeter for solar radio emission observations in the range 50\u2013500 MHz)<\/td>3\u201310<\/td>PDF<\/a><\/strong><\/td>3\u20139<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0413.\u0421., \u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0422.\u041c., \u0422\u043e\u043c\u043e\u0437\u043e\u0432 \u0412.\u041c.<\/em> <\/strong>\u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u044f \u0434\u043b\u0438\u0442\u0435\u043b\u044c\u043d\u044b\u0445 \u043f\u043e\u0442\u043e\u043a\u043e\u0432 \u0432\u044b\u0441\u043e\u043a\u043e\u044d\u043d\u0435\u0440\u0433\u0438\u0447\u043d\u043e\u0433\u043e \u0433\u0430\u043c\u043c\u0430-\u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u043d\u0430 \u0440\u0430\u0437\u043d\u044b\u0445 \u0441\u0442\u0430\u0434\u0438\u044f\u0445 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u0435\u043a (Minasyants G.S., Minasyants T.M., Tomozov V.M.<\/em> <\/strong>Features of development of sustained fluxes of high-energy gamma-ray emission at different stages of solar flares)<\/td>11\u201320<\/td>PDF<\/a><\/strong><\/td>10\u201317<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0413\u043e\u043b\u043e\u0432\u043a\u043e \u0410.\u0410., \u041f\u043e\u043b\u044f\u043a\u043e\u0432 \u0412.\u0418., \u0422\u0440\u0438\u0444\u043e\u043d\u043e\u0432 \u0412.\u0414., \u042f\u0437\u0435\u0432 \u0421.\u0410.<\/em> <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u0432 \u0411\u0430\u0439\u043a\u0430\u043b\u044c\u0441\u043a\u043e\u0439 \u0430\u0441\u0442\u0440\u043e\u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043a\u043e\u0439 \u043e\u0431\u0441\u0435\u0440\u0432\u0430\u0442\u043e\u0440\u0438\u0438 \u0418\u0421\u0417\u0424 \u0421\u041e \u0420\u0410\u041d (Borovik \u0410.V., Golovko \u0410.\u0410., Polyakov V.I., \u0422rifonov V.D., Yazev S.\u0410.<\/em> <\/strong>Solar activity research at the Baikal Astrophysical Observatory of ISTP SB RAS)<\/td>21\u201335<\/td>PDF<\/a><\/strong><\/td>18\u201328<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447<\/em><\/strong> \u0412.\u0413.<\/strong><\/em> <\/strong>\u0414\u0438\u0430\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0435 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440\u044b \u2014 \u043e\u0441\u043d\u043e\u0432\u0430 \u043a\u0432\u0430\u0437\u0438\u0441\u0442\u0430\u0446\u0438\u043e\u043d\u0430\u0440\u043d\u043e\u0433\u043e \u043c\u0435\u0434\u043b\u0435\u043d\u043d\u043e\u0433\u043e \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 (Eselevich<\/em><\/strong> V.G<\/strong><\/em>. <\/strong>Diamagnetic structures as a basis of quasi-stationary slow solar wind)<\/td>36\u201349<\/td>PDF<\/a><\/strong><\/td>29\u201341<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0415\u0440\u043e\u0444\u0435\u0435\u0432 \u0414.\u0412<\/em>. <\/strong>\u0412\u043b\u0438\u044f\u043d\u0438\u0435 \u043a\u0440\u0443\u043f\u043d\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u043e\u0439 \u043d\u0435\u043e\u0434\u043d\u043e\u0440\u043e\u0434\u043d\u043e\u0441\u0442\u0438 \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u043d\u0430 \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u043d\u0430\u043f\u0440\u0430\u0432\u043b\u0435\u043d\u0438\u0439 \u0432\u0435\u043a\u0442\u043e\u0440\u0430 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0433\u043e \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u043f\u043e\u043b\u044f (Erofeev D.V.<\/em> <\/strong>Effect of large-scale inhomogeneity of solar wind velocity on distribution of directions of interplanetary magnetic field vector)<\/td>50\u201363<\/td>PDF<\/a><\/strong><\/td>42\u201353<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041b\u0443\u043a\u043e\u0432\u043d\u0438\u043a\u043e\u0432\u0430 \u0410.\u0410., \u0410\u043b\u0435\u0448\u043a\u043e\u0432 \u0412.\u041c., \u041b\u044b\u0441\u0430\u043a \u0410.\u0421.<\/em> <\/strong>\u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u0435 \u043d\u0435\u0439\u0442\u0440\u043e\u043d\u043d\u043e\u0439 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442\u044b \u0432 \u043f\u0435\u0440\u0438\u043e\u0434\u044b \u0433\u0440\u043e\u0437\u043e\u0432\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043d\u0430 \u0432\u044b\u0441\u043e\u043a\u043e\u0433\u043e\u0440\u043d\u043e\u0439 \u0441\u0442\u0430\u043d\u0446\u0438\u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Lukovnikova A.A., Aleshkov V.M., Lysak A.S.<\/em> <\/strong>Observing the neutron component during thunderstorm activity at a mountain CR station)<\/td>64\u201369<\/td>PDF<\/a><\/strong><\/td>54\u201358<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0430\u0440\u0445\u0430\u0442\u043e\u0432 \u041d.\u0410., \u0420\u0435\u0432\u0443\u043d\u043e\u0432\u0430 \u0415.\u0410.,. \u0420\u043e\u043c\u0430\u043d\u043e\u0432 \u0420.\u0412, \u0411\u0430\u0440\u0445\u0430\u0442\u043e\u0432\u0430 \u041e.\u041c., \u0420\u0435\u0432\u0443\u043d\u043e\u0432 \u0421.\u0415<\/em>. <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u0441\u0432\u044f\u0437\u0438 \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043b\u043e\u043a\u0430\u043b\u0438\u0437\u0430\u0446\u0438\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u043e\u0432 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u043e\u0431\u043b\u0430\u043a\u043e\u0432 \u0441 \u0438\u0445 \u0445\u0430\u0440\u0430\u043a\u0442\u0435\u0440\u0438\u0441\u0442\u0438\u043a\u0430\u043c\u0438 \u0438 \u0441\u0443\u0431\u0431\u0443\u0440\u0435\u0432\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u044c\u044e (Barkhatov N.A., Revunova E.A., Romanov R.V., Barkhatova O.M., Revunov S.E<\/em>. <\/strong>Studying the relationship of localization parameters of solar sources of magnetic clouds with their characteristics and substorm activity)<\/td>70\u201380<\/td>PDF<\/a><\/strong><\/td>59\u201367<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u0443\u0440\u0447\u0435\u0432 \u0415.\u0410., \u0411\u0430\u043b\u0430\u0431\u0438\u043d \u042e.\u0412., \u0413\u0435\u0440\u043c\u0430\u043d\u0435\u043d\u043a\u043e \u0410.\u0412., \u041c\u0438\u0445\u0430\u043b\u043a\u043e \u0415.\u0410., \u0413\u0432\u043e\u0437\u0434\u0435\u0432\u0441\u043a\u0438\u0439<\/em><\/strong> \u0411.\u0412.<\/strong><\/em> <\/strong>\u0420\u0430\u0441\u0447\u0435\u0442 \u0441\u043a\u043e\u0440\u043e\u0441\u0442\u0438 \u0438\u043e\u043d\u0438\u0437\u0430\u0446\u0438\u0438 \u0432\u0435\u0449\u0435\u0441\u0442\u0432\u0430 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u044b \u0417\u0435\u043c\u043b\u0438 \u043f\u0440\u043e\u0442\u043e\u043d\u0430\u043c\u0438 \u0433\u0430\u043b\u0430\u043a\u0442\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Maurchev E.A., Balabin Yu.V., Germanenko A.V., Mikhalko E.A., Gvozdevsky B.V.<\/em> <\/strong>Calculating the ionization rate induced by GCR and SCR protons in Earth\u2019s atmosphere)<\/td>81\u201388<\/td>PDF<\/a><\/strong><\/td>68\u201374<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u0440\u0441\u0443\u043d\u0441\u043a\u0430\u044f \u042e.\u0410.<\/em> <\/strong>\u042d\u0432\u0440\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u043c\u043e\u0434\u0435\u043b\u044c \u0434\u043b\u044f \u0432\u043e\u0441\u0441\u0442\u0430\u043d\u043e\u0432\u043b\u0435\u043d\u0438\u044f \u0440\u0435\u043d\u0442\u0433\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u0439 \u0447\u0430\u0441\u0442\u0438 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0441\u043f\u0435\u043a\u0442\u0440\u0430 \u043f\u043e \u0441\u043f\u0443\u0442\u043d\u0438\u043a\u043e\u0432\u044b\u043c \u0434\u0430\u043d\u043d\u044b\u043c \u0432 \u0438\u043d\u0442\u0435\u0440\u0435\u0441\u0430\u0445 \u0433\u0435\u043e\u0444\u0438\u0437\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043f\u0440\u0438\u043b\u043e\u0436\u0435\u043d\u0438\u0439 (Korsunskaja J.\u0410.<\/em> <\/strong>Heuristic model of solar X-ray spectrum according to satellite data for geophysical applications)<\/td>89\u2013101<\/td>PDF<\/a><\/strong><\/td>75\u201386<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u043b\u044c\u0435\u043b\u044c\u043c\u0438 \u0410.\u0412., \u041f\u043e\u0442\u0430\u043f\u043e\u0432 \u0410.\u0421.<\/em> <\/strong>\u041f\u0440\u043e\u0431\u043b\u0435\u043c\u044b \u0442\u0435\u043e\u0440\u0438\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u0432\u043e\u043b\u043d \u0420\u04411. \u041e\u0431\u0437\u043e\u0440 (Guglielmi A.V.,<\/em><\/strong> Potapov A.S.<\/strong><\/em> <\/strong>Problems of the Pc1 magnetospheric wave theory. A review)<\/td>102\u2013109<\/td>PDF<\/a><\/strong><\/td>87\u201392<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0440\u0438\u0433\u043e\u0440\u044c\u0435\u0432 \u0412.\u0413., \u0421\u0442\u0430\u0440\u043e\u0434\u0443\u0431\u0446\u0435\u0432 \u0421.\u0410., \u0413\u043e\u043b\u043e\u043b\u043e\u0431\u043e\u0432 \u041f.\u042e<\/em>. <\/strong>\u041c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u0439 \u043d\u0430 \u043e\u0441\u043d\u043e\u0432\u0435 \u043c\u0435\u0442\u043e\u0434\u0430 \u0433\u043b\u043e\u0431\u0430\u043b\u044c\u043d\u043e\u0439 \u0441\u044a\u0435\u043c\u043a\u0438 \u0432 \u0440\u0435\u0430\u043b\u044c\u043d\u043e\u043c \u0432\u0440\u0435\u043c\u0435\u043d\u0438 (Grigoryev V.G.,<\/em><\/strong> Starodubtsev S.A., Gololobov P.Yu. <\/strong><\/em>Monitoring of geomagnetic disturbances using the global survey method in real time)<\/td>110\u2013115<\/td>PDF<\/a><\/strong><\/td>93\u201397<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0443\u0431\u0435\u043d\u043a\u043e \u0412.\u041d., \u041a\u0438\u0440\u0438\u043b\u043b\u043e\u0432\u0438\u0447 \u0418.\u0410.<\/em> <\/strong>\u041c\u043e\u0434\u0443\u043b\u044f\u0446\u0438\u044f \u0441\u043f\u043e\u0440\u0430\u0434\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u0415-\u0441\u043b\u043e\u0435\u0432 \u043c\u0435\u043b\u043a\u043e\u043c\u0430\u0441\u0448\u0442\u0430\u0431\u043d\u044b\u043c\u0438 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u043c\u0438 \u0432\u043e\u043b\u043d\u0430\u043c\u0438 \u0432 \u0432\u044b\u0441\u043e\u043a\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u0435 \u0417\u0435\u043c\u043b\u0438 (Gubenko V.N., Kirillovich I.A<\/em>. <\/strong>Modulation of sporadic E layers by small-scale atmospheric waves in <\/strong>Earth\u2019s high-latitude ionosphere)<\/td>116\u2013129<\/td>PDF<\/a><\/strong><\/td>98\u2013108<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0438\u0445\u0430\u043b\u0435\u0432 \u0410.\u0412., \u0411\u0435\u043b\u0435\u0446\u043a\u0438\u0439 \u0410.\u0411., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u0415\u0441\u0435\u043b\u0435\u0432\u0438\u0447 \u041c.\u0412., \u0418\u0432\u0430\u043d\u043e\u0432 \u041a.\u0418., \u041a\u043e\u043c\u0430\u0440\u043e\u0432\u0430 \u0415.\u0421., \u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0410.\u0412., \u041f\u043e\u0434\u043b\u0435\u0441\u043d\u044b\u0439 \u0421.\u0412., \u0421\u044b\u0440\u0435\u043d\u043e\u0432\u0430 \u0422.\u0415. <\/em><\/strong>\u0414\u043e\u043b\u0433\u043e\u0436\u0438\u0432\u0443\u0449\u0438\u0435 \u043c\u0435\u0442\u0435\u043e\u0440\u043d\u044b\u0435 \u0441\u043b\u0435\u0434\u044b (Mikhalev A.V., Beletsky A.B., Vasilyev R.V., Eselevich M.V., Ivanov K.I., Komarova E.S., Podlesnyi A.V., Podlesny S.V., Syrenova T.E<\/em>. <\/strong>Long-lived meteor trails)<\/td>130\u2013139<\/td>PDF<\/a><\/strong><\/td>109\u2013116<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u043e\u043b\u0435\u0445 \u041d.\u041c., \u0427\u0435\u0440\u043d\u0438\u0433\u043e\u0432\u0441\u043a\u0430\u044f \u041c.\u0410., \u042f\u043a\u043e\u0432\u043b\u0435\u0432\u0430 \u041e.\u0415.<\/em> <\/strong>\u041a \u0432\u043e\u043f\u0440\u043e\u0441\u0443 \u043e \u0444\u043e\u0440\u043c\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u0438 \u0441\u043b\u043e\u044f F1 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0432\u043d\u0435\u0437\u0430\u043f\u043d\u044b\u0445 \u0441\u0442\u0440\u0430\u0442\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0445 \u043f\u043e\u0442\u0435\u043f\u043b\u0435\u043d\u0438\u0439 (Polekh N.M.,<\/em><\/strong> Chernigovskaya M.A., Yakovleva O.E.<\/strong><\/em> <\/strong>On the formation of the F1 layer during sudden stratospheric warming events)<\/td>140\u2013152<\/td>PDF<\/a><\/strong><\/td>117\u2013127<\/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. \u041c\u0443\u0440\u0430\u0442\u043e\u0432\u0430 \u041d.\u041e., \u041c\u0443\u0440\u0430\u0442\u043e\u0432 \u0410.\u0410., \u041a\u0430\u0448\u0430\u043f\u043e\u0432\u0430 \u041b.\u041a. \u0420\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u044b \u0440\u0430\u0431\u043e\u0442\u044b \u043d\u043e\u0432\u043e\u0433\u043e \u0441\u043f\u0435\u043a\u0442\u0440\u043e\u043f\u043e\u043b\u044f\u0440\u0438\u043c\u0435\u0442\u0440\u0430 \u0434\u043b\u044f \u043d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \u0432 \u0434\u0438\u0430\u043f\u0430\u0437\u043e\u043d\u0435 50\u2013500 \u041c\u0413\u0446 (Muratova N.O., Muratov A.A., Kashapova L.K. Results of work of new spectropolarimeter for solar radio emission observations in the range 50\u2013500 MHz) 3\u201310 PDF 3\u20139 PDF \u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0413.\u0421., \u041c\u0438\u043d\u0430\u0441\u044f\u043d\u0446 \u0422.\u041c., \u0422\u043e\u043c\u043e\u0437\u043e\u0432 \u0412.\u041c. \u041e\u0441\u043e\u0431\u0435\u043d\u043d\u043e\u0441\u0442\u0438 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u044f […]<\/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-8032","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8032","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=8032"}],"version-history":[{"count":6,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8032\/revisions"}],"predecessor-version":[{"id":9942,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8032\/revisions\/9942"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8032"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8032"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8032"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}