{"id":8022,"date":"2025-04-23T00:22:29","date_gmt":"2025-04-23T00:22:29","guid":{"rendered":"https:\/\/iszf.irk.ru\/?p=8022"},"modified":"2025-11-01T02:03:19","modified_gmt":"2025-11-01T02:03:19","slug":"solnechno-zemnaya-fizika-tom-4-%e2%84%963-2018","status":"publish","type":"post","link":"https:\/\/iszf.irk.ru\/en\/uncategorized\/solnechno-zemnaya-fizika-tom-4-%e2%84%963-2018\/","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 4, \u21163, 2018"},"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>
\u0413\u0435\u043b\u0438\u044e \u0410\u043b\u0435\u043a\u0441\u0430\u043d\u0434\u0440\u043e\u0432\u0438\u0447\u0443 \u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432\u0443 \u2014 80 \u043b\u0435\u0442<\/td>3\u20134<\/td>PDF<\/a><\/strong><\/td><\/td><\/td><\/tr>
\u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410.<\/em> <\/strong>\u0420\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u0435\u043a \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 \u043f\u043e \u0432\u0440\u0435\u043c\u0435\u043d\u0438 \u043f\u043e\u0434\u044a\u0435\u043c\u0430 \u044f\u0440\u043a\u043e\u0441\u0442\u0438 \u043a \u043c\u0430\u043a\u0441\u0438\u043c\u0443\u043c\u0443 (Borovik A.V., Zhdanov A.A<\/em>. <\/strong>Distribution of low-power solar flares by brightness rise time)<\/td>5\u201316<\/td>PDF<\/a><\/strong><\/td>3\u201312<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0424\u0435\u0434\u043e\u0442\u043e\u0432\u0430 \u0410.\u042e., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041a\u043e\u0447\u0430\u043d\u043e\u0432 \u0410.\u0410., \u041b\u0435\u0441\u043e\u0432\u043e\u0439 \u0421.\u0412., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421.<\/em><\/strong> \u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u044d\u0440\u0443\u043f\u0442\u0438\u0432\u043d\u044b\u0445 \u0441\u043e\u0431\u044b\u0442\u0438\u0439 \u0441 \u043f\u043e\u043c\u043e\u0449\u044c\u044e \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 (Fedotova<\/em><\/strong> A.Yu., Altyntsev A.T., Kochanov A.A., Lesovoi S.V., Meshalkina N.S.<\/strong><\/em> <\/strong>Observation of eruptive events with the Siberian Radioheliograph)<\/td>17\u201327<\/td>PDF<\/a><\/strong><\/td>13\u201319<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041c\u0430\u043a\u0430\u0440\u043e\u0432 \u0413.\u0410.<\/em> <\/strong>\u0413\u0435\u043b\u0438\u043e\u0448\u0438\u0440\u043e\u0442\u043d\u044b\u0435 \u0437\u0430\u043a\u043e\u043d\u043e\u043c\u0435\u0440\u043d\u043e\u0441\u0442\u0438 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e-\u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u044b\u0445 \u0434\u043d\u0435\u0439 \u0441\u043e \u0441\u0440\u0435\u0434\u043d\u0435\u0441\u0443\u0442\u043e\u0447\u043d\u044b\u043c \u0437\u043d\u0430\u0447\u0435\u043d\u0438\u0435\u043c \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u043e\u0433\u043e \u0438\u043d\u0434\u0435\u043a\u0441\u0430 Dst<\/em><\u2013100 \u043d\u0422\u043b (Makarov<\/em><\/strong> G.A.<\/strong><\/em> <\/strong>Heliolatitude regularities of magnetically disturbed days with daily average geomagnetic index Dst<\/em><\u2013100 nT)<\/td>28\u201332<\/td>PDF<\/a><\/strong><\/td>20\u201323<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0421\u0435\u0442\u043e\u0432 \u0410.\u0413., \u0413\u043b\u043e\u0431\u0430 \u041c.\u0412., \u041c\u0435\u0434\u0432\u0435\u0434\u0435\u0432<\/em><\/strong> \u0410.\u0412., \u0412\u0430\u0441\u0438\u043b\u044c\u0435\u0432 \u0420.\u0412., \u041a\u0443\u0448\u043d\u0430\u0440\u0435\u0432 \u0414.\u0421<\/strong><\/em>. <\/strong>\u041f\u0435\u0440\u0432\u044b\u0435 \u0440\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u044b \u0430\u0431\u0441\u043e\u043b\u044e\u0442\u043d\u044b\u0445 \u0438\u0437\u043c\u0435\u0440\u0435\u043d\u0438\u0439 \u043f\u043e\u0442\u043e\u043a\u0430 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u043e\u0433\u043e \u0438\u0437\u043b\u0443\u0447\u0435\u043d\u0438\u044f \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 (\u0418\u0420\u041d\u0420) (Setov A.G., Globa M.V., Medvedev A.V., Vasilyev R.V., Kushnarev D.S.<\/em> <\/strong>First results of absolute measurements of solar flux at the Irkutsk Incoherent Scatter Radar (IISR))<\/td>33\u201338<\/td>PDF<\/a><\/strong><\/td>24\u201327<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0417\u043e\u043b\u043e\u0442\u0443\u0445\u0438\u043d\u0430 \u041d.\u0410., \u041a\u0443\u0440\u043a\u0438\u043d \u0412.\u0418., \u041f\u043e\u043b\u0435\u0445 \u041d.\u041c.<\/em> <\/strong>\u0418\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0435 \u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u0438\u044f \u043d\u0430\u0434 \u0412\u043e\u0441\u0442\u043e\u0447\u043d\u043e\u0439 \u0410\u0437\u0438\u0435\u0439 \u0432\u043e \u0432\u0440\u0435\u043c\u044f \u0441\u0438\u043b\u044c\u043d\u044b\u0445 \u0434\u0435\u043a\u0430\u0431\u0440\u044c\u0441\u043a\u0438\u0445 \u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u0431\u0443\u0440\u044c 2006 \u0438 2015 \u0433\u0433.: \u0441\u0445\u043e\u0434\u0441\u0442\u0432o \u0438 \u0440\u0430\u0437\u043b\u0438\u0447\u0438e (Zolotukhina N.A.,<\/em><\/strong> Kurkin V.I.,<\/strong> Polekh N.M.<\/strong><\/em> <\/strong>Ionospheric disturbances over East Asia during intense December magnetic storms of 2006 and 2015: similarities and differences)<\/td>39\u201356<\/td>PDF<\/a><\/strong><\/td>28\u201342<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0440\u0438\u043a\u043d\u0435\u0440 \u041a., \u0424\u0435\u0439\u0433\u0438\u043d \u0424.\u0417., \u0425\u0430\u0431\u0430\u0437\u0438\u043d \u042e.\u0413.<\/em> <\/strong>\u0418\u0441\u0441\u043b\u0435\u0434\u043e\u0432\u0430\u043d\u0438\u0435 \u0441\u0432\u044f\u0437\u0438 \u0441\u043f\u0435\u043a\u0442\u0440\u0430\u043b\u044c\u043d\u044b\u0445 \u0440\u0435\u0437\u043e\u043d\u0430\u043d\u0441\u043d\u044b\u0445 \u0441\u0442\u0440\u0443\u043a\u0442\u0443\u0440 \u0441 \u0433\u0430\u0440\u043c\u043e\u043d\u0438\u043a\u0430\u043c\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u043d\u043e\u0433\u043e \u0430\u043b\u044c\u0444\u0432\u0435\u043d\u043e\u0432\u0441\u043a\u043e\u0433\u043e \u0440\u0435\u0437\u043e\u043d\u0430\u0442\u043e\u0440\u0430 (Prikner K., Feygin F.Z., Khabazin<\/em><\/strong> Yu.G<\/strong><\/em>. <\/strong>Research into connection between spectral resonance structures and harmonics of ionospheric Alfv\u00e9n resonator)<\/td>57\u201360<\/td>PDF<\/a><\/strong><\/td>43\u201345<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0420\u0430\u0445\u043c\u0430\u0442\u0443\u043b\u0438\u043d \u0420.\u0410., \u041f\u0430\u0448\u0438\u043d\u0438\u043d<\/em><\/strong> \u0410.\u042e.<\/strong><\/em> <\/strong>\u0414\u0438\u043d\u0430\u043c\u0438\u043a\u0430 \u043f\u043e\u043b\u044f\u0440\u0438\u0437\u0430\u0446\u0438\u0438 Pi2-\u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u0439 \u0432 \u0441\u0440\u0435\u0434\u043d\u0438\u0445 \u0448\u0438\u0440\u043e\u0442\u0430\u0445 \u043f\u0440\u0438 \u0440\u0430\u0437\u0432\u0438\u0442\u0438\u0438 \u0441\u0443\u0431\u0431\u0443\u0440\u044c \u0432 \u0430\u0432\u0440\u043e\u0440\u0430\u043b\u044c\u043d\u043e\u0439 \u0437\u043e\u043d\u0435 (Rakhmatulin R.A., Pashinin<\/em><\/strong> A.Yu.<\/strong><\/em> <\/strong>Polarization dynamics of Pi2 pulsations at midlatitudes during development of substorms in the auroral zone)<\/td>61\u201367<\/td>PDF<\/a><\/strong><\/td>46\u201351<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u041f\u0430\u0440\u0445\u043e\u043c\u043e\u0432 \u0412.\u0410., \u0411\u043e\u0440\u043e\u0434\u043a\u043e\u0432\u0430 \u041d.\u041b., \u042f\u0445\u043d\u0438\u043d \u0410.\u0412., \u0422\u0435\u0440\u043e \u0420\u0430\u0439\u0442\u0430, \u0426\u044d\u0433\u043c\u044d\u0434 \u0411., \u0425\u043e\u043c\u0443\u0442\u043e\u0432 \u0421.\u042e., \u041f\u0430\u0448\u0438\u043d\u0438\u043d \u0410.\u042e., \u0427\u0438\u043b\u0438\u043a\u0438\u043d \u0412.\u042d., \u041c\u043e\u0447\u0430\u043b\u043e\u0432 \u0410.\u0410.<\/em> <\/strong>\u0414\u0432\u0430 \u0442\u0438\u043f\u0430 \u043e\u0442\u043a\u043b\u0438\u043a\u0430 \u043c\u0430\u0433\u043d\u0438\u0442\u043e\u0441\u0444\u0435\u0440\u044b \u0432 \u0433\u0435\u043e\u043c\u0430\u0433\u043d\u0438\u0442\u043d\u044b\u0445 \u043f\u0443\u043b\u044c\u0441\u0430\u0446\u0438\u044f\u0445 PSc \u043d\u0430 \u0432\u0437\u0430\u0438\u043c\u043e\u0434\u0435\u0439\u0441\u0442\u0432\u0438\u0435 \u0441 \u043c\u0435\u0436\u043f\u043b\u0430\u043d\u0435\u0442\u043d\u044b\u043c\u0438 \u0443\u0434\u0430\u0440\u043d\u044b\u043c\u0438 \u0432\u043e\u043b\u043d\u0430\u043c\u0438 (Parkhomov V.A., Borodkova N.L., Yahnin<\/em><\/strong> A.G., Tero Raita, Tsegmed B., Khomutov<\/strong> S.Yu.,<\/strong><\/em> Pashinin A.Yu., Chilikin V.E., Mochalov A.A.<\/em> <\/strong>Magnetospheric response of two types in PSc geomagnetic pulsations to interaction with interplanetary shock waves)<\/td>68\u201383<\/td>PDF<\/a><\/strong><\/td>52\u201366<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0411\u0435\u043a\u043a\u0435\u0440 \u0421.\u0417<\/em>.<\/strong> \u0410\u043d\u0430\u043b\u0438\u0437 \u0440\u0435\u0437\u0443\u043b\u044c\u0442\u0430\u0442\u043e\u0432 \u0440\u0430\u0441\u0447\u0435\u0442\u043e\u0432 \u043a\u043e\u043d\u0446\u0435\u043d\u0442\u0440\u0430\u0446\u0438\u0438 \u044d\u043b\u0435\u043a\u0442\u0440\u043e\u043d\u043e\u0432 \u043f\u043e \u0434\u0435\u0442\u0435\u0440\u043c\u0438\u043d\u0438\u0440\u043e\u0432\u0430\u043d\u043d\u043e-\u0432\u0435\u0440\u043e\u044f\u0442\u043d\u043e\u0441\u0442\u043d\u043e\u0439 \u043c\u043e\u0434\u0435\u043b\u0438 \u0441\u0440\u0435\u0434\u043d\u0435\u0448\u0438\u0440\u043e\u0442\u043d\u043e\u0439 \u043d\u0435\u0432\u043e\u0437\u043c\u0443\u0449\u0435\u043d\u043d\u043e\u0439 D-\u043e\u0431\u043b\u0430\u0441\u0442\u0438 \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b (Bekker<\/em><\/strong> S.Z.<\/strong><\/em> <\/strong>Analysis of electron density calculations using deterministic-probabilistic model of the ionospheric D-region)<\/td>84\u201394<\/td>PDF<\/a><\/strong><\/td>67\u201375<\/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.<\/em> <\/strong>\u0410\u0442\u043c\u043e\u0441\u0444\u0435\u0440\u043d\u044b\u0435 \u044d\u0444\u0444\u0435\u043a\u0442\u044b \u043c\u044e\u043e\u043d\u043d\u043e\u0439 \u043a\u043e\u043c\u043f\u043e\u043d\u0435\u043d\u0442\u044b \u043a\u043e\u0441\u043c\u0438\u0447\u0435\u0441\u043a\u0438\u0445 \u043b\u0443\u0447\u0435\u0439 (Yanchukovsky V.L., Kuzmenko V.S.<\/em> <\/strong>Atmospheric effects of the cosmic-ray mu-meson component)<\/td>95\u2013102<\/td>PDF<\/a><\/strong><\/td>76\u201382<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0418\u043b\u044c\u0438\u043d \u041d.\u0412., \u0411\u0443\u0431\u043d\u043e\u0432\u0430 \u0422.\u0412., \u0413\u0440\u043e\u0437\u043e\u0432 \u0412.\u041f., \u041f\u0435\u043d\u0437\u0438\u043d \u041c.\u0421., \u041f\u043e\u043d\u043e\u043c\u0430\u0440\u0447\u0443\u043a \u0421.\u041d.<\/em><\/strong> \u041e\u043f\u0435\u0440\u0430\u0442\u0438\u0432\u043d\u044b\u0439 \u043f\u0440\u043e\u0433\u043d\u043e\u0437 \u041c\u041f\u0427 \u0440\u0430\u0434\u0438\u043e\u0442\u0440\u0430\u0441\u0441 \u043f\u043e \u0442\u0435\u043a\u0443\u0449\u0438\u043c \u0434\u0430\u043d\u043d\u044b\u043c \u043d\u0430\u043a\u043b\u043e\u043d\u043d\u043e\u0433\u043e \u0437\u043e\u043d\u0434\u0438\u0440\u043e\u0432\u0430\u043d\u0438\u044f \u0438\u043e\u043d\u043e\u0441\u0444\u0435\u0440\u044b \u043d\u0435\u043f\u0440\u0435\u0440\u044b\u0432\u043d\u044b\u043c \u041b\u0427\u041c-\u0441\u0438\u0433\u043d\u0430\u043b\u043e\u043c (Ilyin N.V., Bubnova T.V., Grozov V.P., Penzin M.S., Ponomarchuk S.N.<\/em> <\/strong>Real-time forecast of MUF for radio paths from current data obtained from oblique sounding with continuous chirp signal)<\/td>103\u2013113<\/td>PDF<\/a><\/strong><\/td>83\u201391<\/td>PDF<\/a><\/strong><\/td><\/tr>
\u0425\u0430\u0445\u0438\u043d\u043e\u0432 \u0412.\u0412<\/em><\/strong>.<\/em> \u042d\u043b\u0435\u043a\u0442\u0440\u043e\u0434\u0438\u043d\u0430\u043c\u0438\u0447\u0435\u0441\u043a\u0430\u044f \u043c\u043e\u0434\u0435\u043b\u044c \u043f\u0440\u0438\u0435\u043c\u043d\u043e\u0439 \u0430\u043d\u0442\u0435\u043d\u043d\u044b \u0432 \u0440\u0430\u043c\u043a\u0430\u0445 \u0432\u043e\u043b\u043d\u043e\u0432\u043e\u0434\u043d\u043e\u0433\u043e \u043f\u0440\u0435\u0434\u0441\u0442\u0430\u0432\u043b\u0435\u043d\u0438\u044f \u041a\u0412-\u043f\u043e\u043b\u044f (Khakhinov V.V<\/em><\/strong>.<\/em> Receiving antenna electrodynamic model in terms of waveguide representation of HF field)<\/td>114\u2013118<\/td>PDF<\/a><\/strong><\/td>92\u201395<\/td>PDF<\/a><\/strong><\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

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\u0421\u041e\u0414\u0415\u0420\u0416\u0410\u041d\u0418\u0415\/CONTENTS \u0421\u0442\u0440. Pp. \u0413\u0435\u043b\u0438\u044e \u0410\u043b\u0435\u043a\u0441\u0430\u043d\u0434\u0440\u043e\u0432\u0438\u0447\u0443 \u0416\u0435\u0440\u0435\u0431\u0446\u043e\u0432\u0443 \u2014 80 \u043b\u0435\u0442 3\u20134 PDF \u0411\u043e\u0440\u043e\u0432\u0438\u043a \u0410.\u0412., \u0416\u0434\u0430\u043d\u043e\u0432 \u0410.\u0410. \u0420\u0430\u0441\u043f\u0440\u0435\u0434\u0435\u043b\u0435\u043d\u0438\u0435 \u0441\u043e\u043b\u043d\u0435\u0447\u043d\u044b\u0445 \u0432\u0441\u043f\u044b\u0448\u0435\u043a \u043c\u0430\u043b\u043e\u0439 \u043c\u043e\u0449\u043d\u043e\u0441\u0442\u0438 \u043f\u043e \u0432\u0440\u0435\u043c\u0435\u043d\u0438 \u043f\u043e\u0434\u044a\u0435\u043c\u0430 \u044f\u0440\u043a\u043e\u0441\u0442\u0438 \u043a \u043c\u0430\u043a\u0441\u0438\u043c\u0443\u043c\u0443 (Borovik A.V., Zhdanov A.A. Distribution of low-power solar flares by brightness rise time) 5\u201316 PDF 3\u201312 PDF \u0424\u0435\u0434\u043e\u0442\u043e\u0432\u0430 \u0410.\u042e., \u0410\u043b\u0442\u044b\u043d\u0446\u0435\u0432 \u0410.\u0422., \u041a\u043e\u0447\u0430\u043d\u043e\u0432 \u0410.\u0410., \u041b\u0435\u0441\u043e\u0432\u043e\u0439 \u0421.\u0412., \u041c\u0435\u0448\u0430\u043b\u043a\u0438\u043d\u0430 \u041d.\u0421. \u041d\u0430\u0431\u043b\u044e\u0434\u0435\u043d\u0438\u044f \u044d\u0440\u0443\u043f\u0442\u0438\u0432\u043d\u044b\u0445 […]<\/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-8022","post","type-post","status-publish","format-standard","hentry"],"_links":{"self":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8022","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=8022"}],"version-history":[{"count":6,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8022\/revisions"}],"predecessor-version":[{"id":10073,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/posts\/8022\/revisions\/10073"}],"wp:attachment":[{"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/media?parent=8022"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/categories?post=8022"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/iszf.irk.ru\/en\/wp-json\/wp\/v2\/tags?post=8022"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}