{"id":11874,"date":"2026-06-11T11:43:28","date_gmt":"2026-06-11T03:43:28","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=11874"},"modified":"2026-06-18T13:40:39","modified_gmt":"2026-06-18T05:40:39","slug":"solnechno-zemnaya-fizika-tom-12-%e2%84%962-2026","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-12-%e2%84%962-2026\/","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 12, \u21162, 2026"},"content":{"rendered":"
\"\"<\/figure>\n\n\n\n

<\/p>\n\n\n\n

\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\u0438\u0447\u0430\u0442\u0438\u043d\u043e\u0432<\/em><\/strong> \u041b.\u041b.<\/strong><\/em> \u041f\u0440\u0430\u0432\u0438\u043b\u043e \u0412\u0430\u043b\u044c\u0434\u043c\u0430\u0439\u0435\u0440\u0430 \u0434\u043b\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0446\u0438\u043a\u043b\u043e\u0432: \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u0434\u043e\u0441\u0442\u043e\u0432\u0435\u0440\u043d\u043e\u0441\u0442\u044c \u0438  \u0437\u043d\u0430\u0447\u0435\u043d\u0438\u0435 \u0434\u043b\u044f \u0434\u0438\u043d\u0430\u043c\u043e (Kitchatinov<\/em><\/strong> L.L<\/strong><\/em>.<\/strong> Waldmeier law for sunspot cycles: Statistical significance and implications for dynamo)<\/td>5\u20139<\/td>PDF<\/a><\/strong><\/td>3\u20137<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u0440\u0435\u0447\u043d\u0435\u0432 \u0412.\u0412., \u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u0423\u0440\u0430\u043b\u043e\u0432 \u0410.\u041c<\/em>.<\/strong> \u042d\u0440\u0443\u043f\u0446\u0438\u044f \u0432\u044b\u0441\u043e\u043a\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0433\u043e \u043f\u0440\u043e\u0442\u0443\u0431\u0435\u0440\u0430\u043d\u0446\u0430, \u043d\u0430\u0431\u043b\u044e\u0434\u0430\u0432\u0448\u0430\u044f\u0441\u044f \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u0438\u043c \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u043e\u043c \u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u043c\u0438 \u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f\u0430\u043c\u0438: I. \u0422\u043e\u0440\u043e\u0438\u0434\u0430\u043b\u044c\u043d\u0430\u044f \u0438 \u0432\u0438\u043d\u0442\u043e\u0432\u0430\u044f \u043d\u0435\u0443\u0441\u0442\u043e\u0439\u0447\u0438\u0432\u043e\u0441\u0442\u0438 \u0432 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u0438 \u041a\u0412\u041c (Grechnev V.V., Globa M.V., Uralov<\/em><\/strong> A.M<\/strong><\/em>. <\/strong>Eruption of a high-latitude prominence observed by the Siberian Radioheliograph and space-borne telescopes: I. Torus and helical kink instabilities in CME development)<\/td>10\u201323<\/td>PDF<\/a><\/strong><\/td>8\u201320<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0430\u0432\u0435\u043b\u044c\u0435\u0432\u0430 \u041d.\u0412., \u041f\u0438\u043b\u0438\u043f\u0435\u043d\u043a\u043e \u0412.\u0410., \u042f\u0433\u043e\u0434\u043a\u0438\u043d\u0430 \u041e.\u0418<\/em>.<\/strong> \u041a\u0430\u043a\u0438\u0435 \u0448\u0438\u0440\u043e\u0442\u044b \u0420\u043e\u0441\u0441\u0438\u0439\u0441\u043a\u043e\u0439 \u0424\u0435\u0434\u0435\u0440\u0430\u0446\u0438\u0438 \u043c\u043e\u0433\u0443\u0442 \u0431\u044b\u0442\u044c \u043f\u043e\u0434\u0432\u0435\u0440\u0436\u0435\u043d\u044b \u0432\u043e\u0437\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u044e \u044d\u043a\u0441\u0442\u0440\u0435\u043c\u0430\u043b\u044c\u043d\u044b\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c? (Savelyeva N.V., Pilipenko V.A., Yagodkina O.I<\/em>. <\/strong>Which latitudes of the Russian Federation may be affected by extreme magnetic storms?)<\/td>24\u201337<\/td>PDF<\/a><\/strong><\/td>21\u201333<\/td>PDF<\/a><\/strong><\/td><\/tr>
Tsegmed B., Namuun B<\/em>.<\/strong> Statistical study of predictive parameters for geomagnetic storms during solar cycles 23\u201324 (Tsegmed B., Namuun B<\/em>.<\/strong> Statistical study of predictive parameters for geomagnetic storms during solar cycles 23\u201324)<\/td>38\u201346<\/td>PDF<\/a><\/strong><\/td>34\u201342<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041a\u043e\u043b\u0435\u0441\u043d\u0438\u043a \u0421.\u0410., \u0411\u043e\u0440\u0438\u0441\u0435\u0432\u0438\u0447 \u0410.\u041d<\/em>.<\/strong> \u0421\u0435\u0437\u043e\u043d\u043d\u044b\u0435 \u0432\u0430\u0440\u0438\u0430\u0446\u0438\u0438 \u0434\u043d\u0435\u0432\u043d\u043e\u0433\u043e \u043c\u0430\u043a\u0441\u0438\u043c\u0443\u043c\u0430 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043d\u043e\u0439 \u043a\u043e\u043d\u0446\u0435\u043d\u0442\u0440\u0430\u0446\u0438\u0438 \u0441\u043b\u043e\u044f F2 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u0437\u0430\u0432\u0438\u0441\u0438\u043c\u043e\u0441\u0442\u0438 \u043e\u0442 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0439 \u0430\u043a\u0442\u0438\u0432\u043d\u043e\u0441\u0442\u0438 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0422\u043e\u043c\u0441\u043a\u043e\u0439 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0439 \u0441\u0442\u0430\u043d\u0446\u0438\u0438 (Kolesnik S.A., Borisevich A.N<\/em>. <\/strong>Seasonal variations in daily maximum of electron density in the F2 ionospheric layer depending on solar activity according to the Tomsk ionospheric station data)<\/td>47\u201353<\/td>PDF<\/a><\/strong><\/td>43\u201348<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u042f\u043d\u0447\u0443\u043a\u043e\u0432\u0441\u043a\u0438\u0439 \u0412.\u041b., \u041a\u0443\u0437\u044c\u043c\u0435\u043d\u043a\u043e \u0412.\u0421., \u0425\u0438\u0441\u0430\u043c\u043e\u0432 \u0420.\u0417<\/em>. <\/strong>\u0421\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u0430\u044f \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u0430 \u0415\u0432\u0440\u043e\u043f\u0435\u0439\u0441\u043a\u043e-\u0410\u0437\u0438\u0430\u0442\u0441\u043a\u043e\u0433\u043e \u0440\u0435\u0433\u0438\u043e\u043d\u0430  \u0432 \u043f\u0435\u0440\u0438\u043e\u0434 \u0444\u043e\u0440\u0431\u0443\u0448-\u043f\u043e\u043d\u0438\u0436\u0435\u043d\u0438\u0439 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Yanchukovsky V.L., Kuzmenko V.S., Khisamov R.Z<\/em>. <\/strong>The mid-altitude atmosphere of the European-Asian Region during Forbush decreases in cosmic rays)<\/td>54\u201362<\/td>PDF<\/a><\/strong><\/td>49\u201356<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0443\u0434\u043e\u0432\u043a\u0438\u043d\u0430 \u0410.\u0410., \u0415\u0434\u0435\u043c\u0441\u043a\u0438\u0439 \u0418.\u041a., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u0410\u0440\u0442\u0430\u043c\u043e\u043d\u043e\u0432 \u041c.\u0424<\/em>. <\/strong>\u0421\u0435\u0437\u043e\u043d\u043d\u0430\u044f \u0434\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u0433\u043e\u0440\u0438\u0437\u043e\u043d\u0442\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u043d\u0435\u0439\u0442\u0440\u0430\u043b\u044c\u043d\u043e\u0433\u043e \u0432\u0435\u0442\u0440\u0430 \u0432 \u0411\u0430\u0439\u043a\u0430\u043b\u044c\u0441\u043a\u043e\u043c \u0440\u0435\u0433\u0438\u043e\u043d\u0435 \u043f\u043e \u0434\u0430\u043d\u043d\u044b\u043c \u0438\u043d\u0442\u0435\u0440\u0444\u0435\u0440\u043e\u043c\u0435\u0442\u0440\u0430 \u0424\u0430\u0431\u0440\u0438\u2014\u041f\u0435\u0440\u043e \u0438 \u0440\u0430\u0437\u043b\u0438\u0447\u043d\u044b\u043c \u0432\u0435\u0440\u0441\u0438\u044f\u043c \u043c\u043e\u0434\u0435\u043b\u0438 HWM (Budovkina A.A., Edemskiy I.K., Vasilyev R.V., Artamonov M.F<\/em>.<\/strong> Seasonal variability of horizontal neutral wind in the Baikal Region from Fabry\u2014Perot interferometer observations and different versions of HWM)<\/td>63\u201375<\/td>PDF<\/a><\/strong><\/td>57\u201368<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0414\u0435\u043d\u0438\u0441\u0435\u043d\u043a\u043e \u0412.\u0412., \u0421\u043c\u0438\u0440\u043d\u043e\u0432 \u0421.\u042d<\/em>. <\/strong>\u041e\u0431 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u0438 \u0430\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u044d\u043b\u0435\u043a\u0442\u0440\u0438\u0447\u0435\u0441\u043a\u043e\u0433\u043e \u043f\u043e\u043b\u044f \u0432 \u043e\u0431\u0441\u0435\u0440\u0432\u0430\u0442\u043e\u0440\u0438\u0438 \u00ab\u041f\u0430\u0440\u0430\u0442\u0443\u043d\u043a\u0430\u00bb (Denisenko V.V., Smirnov S.E<\/em>. <\/strong>Measurement of the atmospheric electric field at the Paratunka Observatory)<\/td>76\u201383<\/td>PDF<\/a><\/strong><\/td>69\u201375<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0435\u0440\u043d\u0433\u0430\u0440\u0434\u0442 \u041e.\u0418<\/em>. <\/strong>\u041c\u0435\u0442\u043e\u0434 \u043e\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u043e\u0432 \u043c\u043d\u043e\u0433\u043e\u043c\u043e\u0434\u043e\u0432\u044b\u0445 \u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432, \u0440\u0435\u0433\u0438\u0441\u0442\u0440\u0438\u0440\u0443\u0435\u043c\u044b\u0445 \u043d\u0430 \u0440\u0430\u0434\u0430\u0440\u0430\u0445 \u0421\u0415\u041a\u0418\u0420\u0410 (Berngardt O.I<\/em>. <\/strong>Method for estimating parameters of multi-mode signals measured at SECIRA radars)<\/td>84\u201396<\/td>PDF<\/a><\/strong><\/td>76\u201388<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0412\u0441\u0435\u0440\u043e\u0441\u0441\u0438\u0439\u0441\u043a\u0430\u044f \u0440\u0430\u0434\u0438\u043e\u0430\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u043a\u043e\u043d\u0444\u0435\u0440\u0435\u043d\u0446\u0438\u044f \u00ab\u0410\u043f\u043f\u0430\u0440\u0430\u0442\u0443\u0440\u0430 \u0438 \u043c\u0435\u0442\u043e\u0434\u044b \u0440\u0430\u0434\u0438\u043e\u0430\u0441\u0442\u0440\u043e\u043d\u043e\u043c\u0438\u0438\u00bb <\/strong>
18\u201322 \u0430\u0432\u0433\u0443\u0441\u0442\u0430 2025 \u0433., \u0418\u043d\u0441\u0442\u0438\u0442\u0443\u0442 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e-\u0437\u0435\u043c\u043d\u043e\u0439 \u0444\u0438\u0437\u0438\u043a\u0438 \u0421\u041e \u0420\u0410\u041d, \u0418\u0440\u043a\u0443\u0442\u0441\u043a, \u0420\u043e\u0441\u0441\u0438\u044f<\/strong>
(All-Russian Radio Astronomy Conference \u201cApparatus and Methods of Radio Astronomy\u201d<\/strong>,
August 18\u201322, 2025, Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia)<\/strong><\/td>		<\/td><\/td><\/td><\/td><\/tr>
\u0416\u0435\u043b\u0435\u043d\u043a\u043e\u0432\u0430 \u041e.\u041f., \u0425\u043e\u0440\u0443\u0436\u0435\u043d\u043a\u043e \u041c.\u0412<\/em>. <\/strong>\u0410\u043d\u0430\u043b\u0438\u0437 \u043a\u0430\u043d\u0434\u0438\u0434\u0430\u0442\u043e\u0432 \u0432 \u0433\u0438\u0433\u0430\u043d\u0442\u0441\u043a\u0438\u0435 \u0440\u0430\u0434\u0438\u043e\u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u0438 \u043d\u0430 \u043e\u0441\u043d\u043e\u0432\u0435 \u043c\u043d\u043e\u0433\u043e\u0432\u043e\u043b\u043d\u043e\u0432\u044b\u0445 \u0434\u0430\u043d\u043d\u044b\u0445 (Zhelenkova O.P., Khoruzhenko M.V<\/em>. <\/strong>Analysis of giant radio source candidates based on multiwavelength data)<\/td>97\u2013104<\/td>PDF<\/a><\/strong><\/td>89\u201395<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041e\u0440\u0435\u0448\u043a\u043e \u0412.\u0412., \u0422\u044e\u043b\u044c\u0431\u0430\u0448\u0435\u0432 \u0421.\u0410<\/a><\/em>. <\/strong>\u0420\u0430\u0434\u0438\u043e\u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f \u0434\u043b\u044f \u043c\u043e\u043d\u0438\u0442\u043e\u0440\u0438\u043d\u0433\u0430 \u0441\u043e\u0441\u0442\u043e\u044f\u043d\u0438\u044f \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u043e\u0439 \u043f\u043b\u0430\u0437\u043c\u044b (Oreshko V.V., Tyul\u2019bashev<\/em><\/strong> S.A<\/strong><\/em>. <\/strong>Radio telescope for monitoring the state of interplanetary plasma)<\/td>105\u2013118<\/td>PDF<\/a><\/strong><\/td>96\u2013108<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u043c\u0438\u0440\u043d\u043e\u0432 \u0414.\u0410., \u041c\u0435\u043b\u044c\u043d\u0438\u043a\u043e\u0432<\/em><\/strong> \u0412.\u0424<\/strong><\/em>. <\/strong>\u0412\u043e\u0437\u043c\u043e\u0436\u043d\u044b\u0435 \u043f\u043e\u0433\u0440\u0435\u0448\u043d\u043e\u0441\u0442\u0438 \u0432 \u0432\u043e\u0441\u0441\u0442\u0430\u043d\u043e\u0432\u043b\u0435\u043d\u043d\u044b\u0445 \u043c\u0435\u0442\u043e\u0434\u043e\u043c \u0444\u0438\u0442\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u043f\u0430\u0440\u0430\u043c\u0435\u0442\u0440\u0430\u0445 \u0440\u0430\u0434\u0438\u043e\u0438\u0441\u0442\u043e\u0447\u043d\u0438\u043a\u0430, \u0441\u0432\u044f\u0437\u0430\u043d\u043d\u044b\u0435 \u0441 \u0430\u043d\u0438\u0437\u043e\u0442\u0440\u043e\u043f\u043d\u043e\u0441\u0442\u044c\u044e \u0440\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u044f \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 (Smirnov D.A., Melnikov V.F<\/em>. <\/strong>Possible errors in radio source parameters recovered by the fitting method related to anisotropy of the electron distribution)<\/td>119\u2013123<\/td>PDF<\/a><\/strong><\/td>109\u2013113<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u0413\u0443\u0431\u0438\u043d \u0410.\u0412., \u041b\u0435\u0441\u043e\u0432\u043e\u0439 \u0421.\u0412<\/em>. <\/strong>\u041a\u043e\u0440\u0440\u0435\u043a\u0446\u0438\u044f \u043d\u0430\u0432\u0435\u0434\u0435\u043d\u0438\u044f \u0430\u043d\u0442\u0435\u043d\u043d \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u043e\u0433\u043e \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u0430 (Globa M.V., Gubin A.V., Lesovoi S.V<\/em>. <\/strong>Correction for pointing errors of Siberian Radioheliograph antennas)<\/td>124\u2013129<\/td>PDF<\/a><\/strong><\/td>114\u2013118<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u0440\u0448\u0430\u043b\u043e\u0432 \u0414.\u0410., \u0413\u0440\u0435\u043d\u043a\u043e\u0432 \u0421.\u0410., \u0411\u0435\u0440\u0434\u043d\u0438\u043a\u043e\u0432 \u0410.\u0421., \u0424\u0435\u0434\u043e\u0442\u043e\u0432 \u041b.\u0412<\/em>. <\/strong>\u0421\u043e\u0432\u0440\u0435\u043c\u0435\u043d\u043d\u044b\u0435 \u0446\u0438\u0444\u0440\u043e\u0432\u044b\u0435 \u0441\u0438\u0441\u0442\u0435\u043c\u044b \u043f\u0440\u0435\u043e\u0431\u0440\u0430\u0437\u043e\u0432\u0430\u043d\u0438\u044f \u0441\u0438\u0433\u043d\u0430\u043b\u043e\u0432 \u0440\u0430\u0434\u0438\u043e\u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f\u043e\u0432 \u043a\u043e\u043c\u043f\u043b\u0435\u043a\u0441\u0430 \u00ab\u041a\u0432\u0430\u0437\u0430\u0440-\u041a\u0412\u041e\u00bb (Marshalov D.A., Grenkov S.A., Berdnikov A.S., Fedotov L.V<\/em><\/strong>. <\/em>Modern digital backend systems for the radio telescopes of the Quasar VLBI network)<\/td>130\u2013136<\/td>PDF<\/a><\/strong><\/td>119\u2013124<\/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. \u041a\u0438\u0447\u0430\u0442\u0438\u043d\u043e\u0432 \u041b.\u041b. \u041f\u0440\u0430\u0432\u0438\u043b\u043e \u0412\u0430\u043b\u044c\u0434\u043c\u0430\u0439\u0435\u0440\u0430 \u0434\u043b\u044f \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0446\u0438\u043a\u043b\u043e\u0432: \u0441\u0442\u0430\u0442\u0438\u0441\u0442\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u0434\u043e\u0441\u0442\u043e\u0432\u0435\u0440\u043d\u043e\u0441\u0442\u044c \u0438  \u0437\u043d\u0430\u0447\u0435\u043d\u0438\u0435 \u0434\u043b\u044f \u0434\u0438\u043d\u0430\u043c\u043e (Kitchatinov L.L. Waldmeier law for sunspot cycles: Statistical significance and implications for dynamo) 5\u20139 PDF 3\u20137 PDF \u0413\u0440\u0435\u0447\u043d\u0435\u0432 \u0412.\u0412., \u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u0423\u0440\u0430\u043b\u043e\u0432 \u0410.\u041c. \u042d\u0440\u0443\u043f\u0446\u0438\u044f \u0432\u044b\u0441\u043e\u043a\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0433\u043e \u043f\u0440\u043e\u0442\u0443\u0431\u0435\u0440\u0430\u043d\u0446\u0430, \u043d\u0430\u0431\u043b\u044e\u0434\u0430\u0432\u0448\u0430\u044f\u0441\u044f \u0421\u0438\u0431\u0438\u0440\u0441\u043a\u0438\u043c \u0440\u0430\u0434\u0438\u043e\u0433\u0435\u043b\u0438\u043e\u0433\u0440\u0430\u0444\u043e\u043c \u0438 \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u043c\u0438 \u0442\u0435\u043b\u0435\u0441\u043a\u043e\u043f\u0430\u043c\u0438: I. \u0422\u043e\u0440\u043e\u0438\u0434\u0430\u043b\u044c\u043d\u0430\u044f \u0438 \u0432\u0438\u043d\u0442\u043e\u0432\u0430\u044f \u043d\u0435\u0443\u0441\u0442\u043e\u0439\u0447\u0438\u0432\u043e\u0441\u0442\u0438 \u0432 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u0438 […]<\/p>\n","protected":false},"author":54,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[],"tags":[],"class_list":["post-11874","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11874","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=11874"}],"version-history":[{"count":24,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11874\/revisions"}],"predecessor-version":[{"id":12153,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/11874\/revisions\/12153"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=11874"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=11874"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=11874"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}