LEADER 03570nam 22005415 450 001 9910350229303321 005 20200702170752.0 010 $a981-13-7515-1 024 7 $a10.1007/978-981-13-7515-6 035 $a(CKB)4100000008525934 035 $a(DE-He213)978-981-13-7515-6 035 $a(MiAaPQ)EBC5755800 035 $a(PPN)235666521 035 $a(EXLCZ)994100000008525934 100 $a20190423d2019 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aStudy on Magnetohydrodynamic Turbulence and Its Astrophysical Applications /$fby Siyao Xu 205 $a1st ed. 2019. 210 1$aSingapore :$cSpringer Singapore :$cImprint: Springer,$d2019. 215 $a1 online resource (XIII, 157 p. 13 illus., 3 illus. in color.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 311 $a981-13-7514-3 330 $aTurbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence. These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aAstrophysics 606 $aPlasma (Ionized gases) 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 606 $aPlasma Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P24040 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 615 0$aAstrophysics. 615 0$aPlasma (Ionized gases). 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 14$aAstrophysics and Astroparticles. 615 24$aPlasma Physics. 615 24$aAstronomy, Observations and Techniques. 676 $a523.01 700 $aXu$b Siyao$4aut$4http://id.loc.gov/vocabulary/relators/aut$0839040 906 $aBOOK 912 $a9910350229303321 996 $aStudy on Magnetohydrodynamic Turbulence and Its Astrophysical Applications$91873819 997 $aUNINA