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001 294653
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008 150903s2005 gw | o |||| 0|eng d
020 _a9783540307662
_99783540307662
024 7 _a10.1007/3540307664
_2doi
035 _avtls000347536
039 9 _a201509030436
_bVLOAD
_c201404121430
_dVLOAD
_c201404091207
_dVLOAD
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_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
100 1 _aAschwanden, Markus J.
_eautor
_9328391
245 1 0 _aPhysics of the Solar Corona :
_bAn Introduction with Problems and Solutions /
_cby Markus J Aschwanden.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c2005.
300 _axxii, 908 páginas
_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 _aSpringer Praxis Books
500 _aSpringer eBooks
505 0 _aThermal Radiation -- Hydrostatics -- Hydrodynamics -- Magnetic Fields -- Magneto-Hydrodynamics (MHD) -- MHD Oscillations -- Propagating MHD Waves -- Coronal Heating -- Magnetic Reconnection -- Particle Acceleration -- Particle Kinematics -- Hard X-Rays -- Gamma-Rays -- Radio Emission -- Flare Plasma Dynamics -- Coronal Mass Ejections (CMEs).
520 _aSolar science has evolved rapidly over the past ten years as the results of a new generation of solar space missions have become available. This book provides a thorough introduction to the subject of solar physics, based on those spacecraft observations. The author introduces the solar corona, which has a temperature of several million degrees, and sets it in the context of basic plasma physics before moving on to discuss plasma instabilities and plasma heating processes. The latest results on coronal heating and radiation,which are fundamental processes in all stars, are presented. Spectacular phenomena such as solar flares and coronal mass ejections are described in detail, together with their potential effects on the Earth. The author draws together observations made at many wavelengths from hard X-rays, soft X-rays, extreme UV and radio wavelengths. This paperback study edition of Markus Aschwanden’s highly acclaimed PHYSICS OF THE SOLAR CORONA will include 50 pages of problems and solutions which will much enhance the value of the book to students.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9783540307655
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/3-540-30766-4
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999 _c294653
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