000 03026nam a22003855i 4500
001 287948
003 MX-SnUAN
005 20160429154607.0
007 cr nn 008mamaa
008 150903s2013 xxu| o |||| 0|eng d
020 _a9781461457824
_99781461457824
024 7 _a10.1007/9781461457824
_2doi
035 _avtls000341726
039 9 _a201509030335
_bVLOAD
_c201405050233
_dVLOAD
_y201402061106
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB460-466
100 1 _aFleishman, Gregory D.
_eautor
_9317421
245 1 0 _aCosmic Electrodynamics :
_bElectrodynamics and Magnetic Hydrodynamics of Cosmic Plasmas /
_cby Gregory D. Fleishman, Igor N. Toptygin.
264 1 _aNew York, NY :
_bSpringer New York :
_bImprint: Springer,
_c2013.
300 _axxii, 712 páginas 117 ilustraciones, 36 ilustraciones en color.
_brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
490 0 _aAstrophysics and Space Science Library,
_x0067-0057 ;
_v388
500 _aSpringer eBooks
505 0 _aMagnetohydrodynamics of the Cosmic Plasma -- Non-Linear MHD Waves and Discontinuities -- Instability of MHD motion and MHD turbulence -- Generation of magnetic field -- Plasma Dispersion -- Linear modes in the plasma -- Weak Turbulence and Magnetic Reconnection -- Wave-Particle Interactions -- Particle Transport -- Particle Acceleration -- Generation of linear modes by given electric current -- Microscopic Emission Processes in the Plasma -- Transport of Radiation -- Self-consistent models of astrophysical objects.
520 _aThis volume offers a deep and detailed overview of plasma behavior in diverse astrophysical conditions. The presentation is based on a solid science foundation that includes well established physical laws of electromagnetism, hydrodynamics, classical and quantum mechanics and other relevant fields of science. Qualitative ideas and descriptions are followed by quantitative derivations and estimates of key physical quantities, and the results of theories and models are confronted with modern observational data obtained from numerous international science programs. Fundamental astrophysical phenomena, such as charged particle acceleration and magnetic field generation, are presented along with spectacular phenomena, such as stellar winds (including ultra-relativistic pulsar wind), supernova explosions and evolution of its remnants, and solar flares.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700 1 _aToptygin, Igor N.
_eautor
_9317422
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9781461457817
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-1-4614-5782-4
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
942 _c14
999 _c287948
_d287948