Parker, E. N. Hydromagnetic dynamo models. Astrophys. J. 122, 293\u2013314 (1955).<\/p>\n
Article<\/a>\u00a0 Batchelor, G. K. & Proudman, I. The effects. of rapid distortion of a fluid in turbulent motion. Q. J. Mech. Appl. Math. 7, 83\u2013103 (1954).<\/p>\n Article<\/a>\u00a0 Terry, P. W. Suppression of turbulence and transport by sheared flow. Rev. Mod. Phys. 72, 109\u2013165 (2000).<\/p>\n Article<\/a>\u00a0 Yoshizawa, A. Self-consistent turbulent dynamo modeling of reversed field pinches and planetary magnetic fields. Phys. Fluids B 2, 1589\u20131600 (1990).<\/p>\n Article<\/a>\u00a0 Kiuchi, K., Cerd\u00e1-Dur\u00e1n, P., Kyutoku, K., Sekiguchi, Y. & Shibata, M. Efficient magnetic-field amplification due to the Kelvin\u2013Helmholtz instability in binary neutron star mergers. Phys. Rev. D 92, 124034 (2015).<\/p>\n Article<\/a>\u00a0 Kiuchi, K., Reboul-Salze, A., Shibata, M. & Sekiguchi, Y. A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers. Nat. Astron. 8, 298\u2013307 (2024).<\/p>\n Article<\/a>\u00a0 Price, D. J. & Rosswog, S. Producing ultrastrong magnetic fields in neutron star mergers. Science 312, 719\u2013722\u00a0(2006).<\/p>\n Article<\/a>\u00a0 Tsokaros, A., Bamber, J., Ruiz, M. & Shapiro, S. L. Masking the equation-of-state effects in binary neutron star mergers. Phys. Rev. Lett. 134, 121401 (2025).<\/p>\n Article<\/a>\u00a0 Basu, A. et al. Detection of an ~20 kpc coherent magnetic field in the outskirt of merging spirals: the Antennae galaxies. Mon. Not. R. Astron. Soc. 464, 1003\u20131017 (2017).<\/p>\n Article<\/a>\u00a0 Chandrasekhar, S. Hydrodynamic and Hydromagnetic Stability (Clarendon Press, 1961).<\/p>\n Palenzuela, C. et al. Turbulent magnetic field amplification in binary neutron star mergers. Phys. Rev. D 106, 023013 (2022).<\/p>\n Article<\/a>\u00a0 Vasil, G. M. et al. The solar dynamo begins near the surface. Nature 629, 769 (2024).<\/p>\n Article<\/a>\u00a0 Terry, P. W. in Zonal Jets (eds Galperin, B. & Read, P. L.) 181\u2013193 (Cambridge Univ. Press, 2019).<\/p>\n Hazra, G., Nandy, D., Kitchatinov, L. & Choudhuri, A. R. Mean field models of flux transport dynamo and meridional circulation in the Sun and stars. Space Sci. Rev. 219, 39 (2023).<\/p>\n Article<\/a>\u00a0 Gizon, L. et al. Meridional flow in the Sun\u2019s convection zone is a single cell in each hemisphere. Science 368, 1469\u20131472 (2020).<\/p>\n Article<\/a>\u00a0 Abramowicz, M. A., Lanza, A., Spiegel, E. A. & Szuszkiewicz, E. Vortices on accretion disks. Nature 356, 41\u201343 (1992).<\/p>\n Article<\/a>\u00a0 Chadayammuri, U. et al. Constraining merging galaxy clusters with X-ray and lensing simulations and observations: the case of Abell 2146. Mon. Not. R. Astron. Soc. 509, 1201\u20131216 (2021).<\/p>\n Article<\/a>\u00a0 Chadayammuri, U., ZuHone, J., Nulsen, P., Nagai, D. & Russell, H. Turbulent magnetic fields in merging clusters: a case study of Abell 2146. Mon. Not. R. Astron. Soc. 512, 2157\u20132170 (2022).<\/p>\n Article<\/a>\u00a0 Neronov, A. & Vovk, I. Evidence for strong extragalactic magnetic fields from Fermi observations of TeV blazars. Science 328, 73\u201375 (2010).<\/p>\n Article<\/a>\u00a0 Brandenburg, A. & Subramanian, K. Astrophysical magnetic fields and nonlinear dynamo theory. Phys. Rep. 417, 1\u2013209 (2005).<\/p>\n Article<\/a>\u00a0 Kulsrud, R. M. & Zweibel, E. G. On the origin of cosmic magnetic fields. Rep. Prog. Phys. 71, 046901 (2008).<\/p>\n Article<\/a>\u00a0 Tobias, S. M. & Cattaneo, F. Shear-driven dynamo waves at high magnetic Reynolds number. Nature 497, 463\u2013465 (2013).<\/p>\n Article<\/a>\u00a0 Squire, J. & Bhattacharjee, A. Generation of large-scale magnetic fields by small-scale dynamo in shear flows. Phys. Rev. Lett. 115, 175003 (2015).<\/p>\n Article<\/a>\u00a0 Steenbeck, M., Krause, F. & Radler, K.-H. Z. Naturforsch. 21a, 369\u2013376 (1966).<\/p>\n Article<\/a>\u00a0 Cattaneo, F. & Hughes, D. W. Nonlinear saturation of the turbulent \u03b1 effect. Phys. Rev. E 54, R4532 (1996).<\/p>\n Article<\/a>\u00a0 Vainshtein, S. & Cattaneo, F. Nonlinear restrictions on dynamo action. Astrophys. J. 393, 165\u2013171 (1992).<\/p>\n Article<\/a>\u00a0 Brandenburg, A., Elstner, D., Masada, Y. & Pipin, V. Turbulent processes and mean-field dynamo. Space Sci. Rev. 219, 55 (2023).<\/p>\n Article<\/a>\u00a0 Pouquet, A., Frisch, U. & Leorat, J. Strong MHD helical turbulence and the nonlinear dynamo effect. J. Fluid Mech. 77, 321\u2013354 (1976).<\/p>\n Article<\/a>\u00a0 Howe, R., Chaplin, W. J., Christensen-Dalsgaard, J., Elsworth, Y. P. & Schou, J. Update on global helioseismic observations of the solar torsional oscillation. Res. Notes AAS 6, 261 (2022).<\/p>\n Article<\/a>\u00a0 Smith, K. M., Caulfield, C. P. & Taylor, J. R. Turbulence in forced stratified shear flows. J. Fluid Mech. 910, A42 (2021).<\/p>\n Article<\/a>\u00a0 Hathaway, D. H. The solar cycle. Living Rev. Sol. Phys. 39, 227 (2015).<\/p>\n Ebrahimi, F. & Blackman, E. G. Radially dependent large-scale dynamos in global cylindrical shear flows and the local Cartesian limit. Mon. Not. R. Astron. Soc. 459, 1422\u20131431 (2016).<\/p>\n Article<\/a>\u00a0 Els\u00e4sser, W. M. The hydromagnetic equations. Phys. Rev. 79, 183 (1950).<\/p>\n Article<\/a>\u00a0 Bendre, A. B., Subramanian, K., Elstner, D. & Gressel, O. Turbulent transport coefficients in galactic dynamo simulations using singular value decomposition. Mon. Not. R. Astron. Soc. 491, 3870\u20133883 (2020).<\/p>\n Article<\/a>\u00a0 Lecoanet, D. et al. A validated non-linear Kelvin\u2013Helmholtz benchmark for numerical hydrodynamics. Mon. Not. R. Astron. Soc. 455, 4274\u20134288 (2016).<\/p>\n Article<\/a>\u00a0 Zhang, H. & Brandenburg, A. Solar kinetic energy and cross helicity spectra. Astrophys. J. Lett. 862, L17 (2018).<\/p>\n Article<\/a>\u00a0 Rahbarnia, K. et al. Direct observation of the turbulent EMF and transport of magnetic field in a liquid sodium experiment. Astrophys. J. 759, 80 (2012).<\/p>\n Article<\/a>\u00a0 Kaplan, E. J. et al. Reducing global turbulent resistivity by eliminating large eddies in a spherical liquid-sodium experiment. Phys. Rev. Lett. 106, 254502 (2011).<\/p>\n Article<\/a>\u00a0 Mondal, T. & Bhat, P. Unified treatment of mean-field dynamo and angular-momentum transport in magnetorotational instability-driven turbulence. Phys. Rev. E 108, 065201 (2023).<\/p>\n Article<\/a>\u00a0 Taylor, J. B. Relaxation of toroidal plasma and generation of reverse magnetic fields. Phys. Rev. Lett. 33, 1139\u20131141 (1974).<\/p>\n Article<\/a>\u00a0 Zrake, J. & MacFadyen, A. I. Magnetic energy production by turbulence in binary neutron star mergers. Astrophys. J. Lett. 769, L29 (2013).<\/p>\n Article<\/a>\u00a0 Kunnumkai, K. et al. Detecting electromagnetic counterparts to LIGO\/Virgo\/KAGRA gravitational-wave events with DECam: neutron star mergers. Astrophys. J. 993, 15 (2025).<\/p>\n Maggiore, M. et al. Science case for the Einstein Telescope. J. Cosmol. Astropart. Phys. 03, 050 (2020).<\/p>\n Article<\/a>\u00a0 Radice, D. General-relativistic large-eddy simulations of binary neutron star mergers. Astrophys. J. Lett. 838, L2 (2017).<\/p>\n Article<\/a>\u00a0 Mandal, K., Kosovichev, A. G. & Pipin, V. V. Helioseismic properties of dynamo waves in the variation of solar differential rotation. Astrophys. J. 973, 36 (2024).<\/p>\n Article<\/a>\u00a0 Yokoi, N. Unappreciated cross-helicity effects in plasma physics: anti-diffusion effects in dynamo and momentum transport. Rev. Mod. Plasma Phys. 7, e33 (2023).<\/p>\n Article<\/a>\u00a0 Chakraborty, S., Choudhuri, A. R. & Chatterjee, P. Why does the Sun\u2019s torsional oscillation begin before the sunspot cycle? Phys. Rev. Lett. 102, 041102 (2009).<\/p>\n Article<\/a>\u00a0 Yokoi, N., Schmitt, D., Pipin, V. & Hamba, F. A new simple dynamo model for stellar activity cycle. Astrophys. J. 824, 67 (2016).<\/p>\n Article<\/a>\u00a0 Pecora, F. et al. Relaxation of the turbulent magnetosheath. Mon. Not. R. Astron. Soc. 525, 67\u201372 (2023).<\/p>\n Article<\/a>\u00a0 Tripathi, B., Terry, P. W., Fraser, A. E., Zweibel, E. G. & Pueschel, M. J. Three-dimensional shear-flow instability saturation via stable modes. Phys. Fluids 35, 105151 (2023).<\/p>\n Article<\/a>\u00a0 Burns, K. J., Vasil, G. M., Oishi, J. S., Lecoanet, D. & Brown, B. P. Dedalus: a flexible framework for numerical simulations with spectral methods. Phys. Rev. Res. 2, 023068 (2020).<\/p>\n Article<\/a>\u00a0 Ascher, U. M., Ruuth, S. J. & Spiteri, R. J. Implicit-explicit Runge\u2013Kutta methods for time-dependent partial differential equations. Appl. Numer. Math. 25, 151\u2013167 (1997).<\/p>\n Article<\/a>\u00a0 Wang, D. & Ruuth, S. J. Variable step-size implicit-explicit linear multistep methods for time-dependent partial differential equations. J. Comput. Math. 26, 838\u2013855 (2008).<\/p>\n MathSciNet<\/a>\u00a0 Mininni, P. D., Alexakis, A. & Pouquet, A. Shell-to-shell energy transfer in magnetohydrodynamics II. Kinematic dynamo. Phys. Rev. E 72, 046302 (2005).<\/p>\n Article<\/a>\u00a0 Alexakis, A., Mininni, P. D. & Pouquet, A. Shell-to-shell energy transfer in magnetohydrodynamics. I. Steady state turbulence. Phys. Rev. E 72, 046301 (2005).<\/p>\n Article<\/a>\u00a0 Tripathi, B. et al. Codes, data, and additional materials for \u201cLarge-scale dynamos driven by shear-flow-induced jets\u201d. Zenodo https:\/\/doi.org\/10.5281\/zenodo.17162239<\/a> (2025).<\/p>\n Tripathi, B., Terry, P. W., Fraser, A. E., Zweibel, E. G. & Pueschel, M. J. Mechanism for sequestering magnetic energy at large scales in shear-flow turbulence. Phys. Plasmas 29, 070701 (2022).<\/p>\n Article<\/a>\u00a0 Marston, J. B., Conover, E. & Schneider, T. Statistics of an unstable barotropic jet from a cumulant expansion. J. Atmos. Sci. 65, 1955\u20131966 (2008).<\/p>\n Article<\/a>\u00a0 Cope, L., Garaud, P. & Caulfield, C. The dynamics of stratified horizontal shear flows at low P\u00e9clet number. J. Fluid Mech. 903, A1 (2020).<\/p>\n Article<\/a>\u00a0 Pueschel, M. J., Jenko, F., Told, D. & B\u00fcchner, J. Gyrokinetic simulations of magnetic reconnection. Phys. Plasmas 18, 112102 (2011).<\/p>\n Article<\/a>\u00a0 Pueschel, M. J. et al. Magnetic reconnection turbulence in strong guide fields: Basic properties and application to coronal heating. Astrophys. J. Suppl. Ser. 213, 30 (2014).<\/p>\n Article<\/a>\u00a0 Gruzinov, A. V. & Diamond, P. H. Self-consistent mean field electrodynamics of turbulent dynamos. Phys. Plasmas 2, 1941\u20131946 (1995).<\/p>\n Article<\/a>\u00a0 Biglari, H., Diamond, P. H. & Terry, P. W. Influence of sheared poloidal rotation on edge turbulence. Phys. Fluids B 2, 1\u20134 (1990).<\/p>\n Article<\/a>\u00a0 Townsend, A. A. The Structure of Turbulent Shear Flow 2nd edn (Cambridge Univ. Press, 1976).<\/p>\n Verma, M. K. Energy Transfers in Fluid Flows: Multiscale and Spectral Perspectives (Cambridge Univ. Press, 2019).<\/p>\n Reuter, K., Jenko, F. & Forest, C. B. Turbulent magnetohydrodynamic dynamo action in a spherically bounded von K\u00e1rm\u00e1n flow at small magnetic Prandtl numbers. N. J. Phys. 13, 073019 (2011).<\/p>\n Article<\/a>\u00a0 Baiotti, L., Giacomazzo, B. & Rezzolla, L. Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to a black hole. Phys. Rev. D 78, 084033 (2008).<\/p>\n Article<\/a>\u00a0 Most, E. R. & Quataert, E. Flares, jets, and quasiperiodic outbursts from neutron star merger remnants. Astrophys. J. Lett. 947, L15 (2023).<\/p>\n Article<\/a>\u00a0 Combi, L. & Siegel, D. M. Jets from neutron-star merger remnants and massive blue kilonovae. Phys. Rev. Lett. 131, 231402 (2023).<\/p>\n Article<\/a>\u00a0 Olausen, S. A. & Kaspi, V. M. The McGill Magnetar Catalog. Astrophys. J. Suppl. Ser. 212, 6 (2014).<\/p>\n Article<\/a>\u00a0 Bahramian, A. & Degenaar, N. Low-Mass X-ray Binaries (Springer Nature, 2022).<\/p>\n Anderson, M. et al. Magnetized neutron-star mergers and gravitational-wave signals. Phys. Rev. Lett.\u00a0100, 191101 (2008).<\/p>\n Article<\/a>\u00a0 Aguilera-Miret, R., Vigan\u00f2, D. & Palenzuela, C. Universality of the turbulent magnetic field in hypermassive neutron stars produced by binary mergers. Astrophys. J. Lett. 926, L31 (2022).<\/p>\n Article<\/a>\u00a0 Charbonneau, P. Dynamo models of the solar cycle. Living Rev. Sol. Phys. 17, 4 (2020).<\/p>\n Article<\/a>\u00a0 R\u00fcdiger, G., K\u00fcker, M. & Schnerr, R. S. Cross helicity at the solar surface by simulations and observations. Astron. Astrophys. 546, A23 (2012).<\/p>\n Article<\/a>\u00a0 Brandenburg, A. The case for a distributed solar dynamo shaped by near-surface shear. Astrophys. J. 625, 539\u2013547 (2005).<\/p>\n Article<\/a>\u00a0 Yousef, T. A. et al. Generation of magnetic field by combined action of turbulence and shear. Phys. Rev. Lett. 100, 184501 (2008).<\/p>\n Article<\/a>\u00a0 Blackman, E. G. Mean magnetic field generation in sheared rotators. Astrophys. J. 529, 138\u2013145 (2000).<\/p>\n Article<\/a>\u00a0 Brandenburg, A. & Urpin, V. Magnetic fields in young galaxies due to the cross-helicity effect. Astron. Astrophys. 332, L41\u2013L44 (1998).<\/p>\n Elias-L\u00f3pez, A., Del Sordo, F. & Vigan\u00f2, D. Vorticity and magnetic dynamo from subsonic expansion waves. Astron. Astrophys. 677, A46 (2023).<\/p>\n Article<\/a>\u00a0 Hughes, D. W. & Proctor, M. R. E. Large-scale dynamo action driven by velocity shear and rotating convection. Phys. Rev. Lett. 102, 044501 (2008).<\/p>\n Article<\/a>\u00a0
\n MathSciNet<\/a>\u00a0
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n MathSciNet<\/a>\u00a0
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\n PubMed Central<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n MathSciNet<\/a>\u00a0
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\n PubMed<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n MathSciNet<\/a>\u00a0
\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n MathSciNet<\/a>\u00a0
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\n PubMed<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n MathSciNet<\/a>\u00a0
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\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n CAS<\/a>\u00a0
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\n CAS<\/a>\u00a0
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n CAS<\/a>\u00a0
\n PubMed<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n PubMed<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n CAS<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n CAS<\/a>\u00a0
\n PubMed<\/a>\u00a0
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\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n
\n
\n Google Scholar<\/a>\u00a0\n <\/p>\n","protected":false},"excerpt":{"rendered":"Parker, E. N. Hydromagnetic dynamo models. Astrophys. J. 122, 293\u2013314 (1955). Article\u00a0 MathSciNet\u00a0 Google Scholar\u00a0 Batchelor, G. K.…\n","protected":false},"author":2,"featured_media":424348,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[24],"tags":[177503,35393,49,48,1099,1100,314,66],"class_list":{"0":"post-424347","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-physics","8":"tag-astrophysical-magnetic-fields","9":"tag-astrophysical-plasmas","10":"tag-ca","11":"tag-canada","12":"tag-humanities-and-social-sciences","13":"tag-multidisciplinary","14":"tag-physics","15":"tag-science"},"_links":{"self":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/424347","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/comments?post=424347"}],"version-history":[{"count":0,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/posts\/424347\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media\/424348"}],"wp:attachment":[{"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/media?parent=424347"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/categories?post=424347"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.newsbeep.com\/ca\/wp-json\/wp\/v2\/tags?post=424347"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}