000			03183nam a22003855i 4500
001			283123
003			MX-SnUAN
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007			cr nn 008mamaa
008			150903s2008 ne | o |||| 0|eng d
020			_a9781402088681 _99781402088681
024	7		_a10.1007/9781402088681 _2doi
035			_avtls000336186
039		9	_a201509030257 _bVLOAD _c201404300312 _dVLOAD _y201402041343 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB1-991
100	1		_aHasan, S. S. _eeditor. _9310404
245	1	0	_aTurbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes : _bFirst Kodai-Trieste Workshop on Plasma Astrophysics Held at the Kodaikanal Observatory Kodaikanal, India, August 27 – September 7, 2007 / _cedited by S. S. Hasan, R. T. Gangadhara, V. Krishan.
264		1	_aDordrecht : _bSpringer Netherlands, _c2008.
300			_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 Proceedings, _x1570-6591
500			_aSpringer eBooks
520			_aIt is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling variety of configurations in the form of filaments, loops , jets and arches. The plasma structures that cannot last for more than a second or less in a laboratory remain intact for astronomical time and spatial scales in an astrophysical setting. The case in point is the well known extragalactic jets whose collimation and stability has remained an enigma inspite of the efforts of many for many long years. The high energy radiation sources such as the active galactic nuclei again summon the coherent plasma radiation processes for their exceptionally large output from regions of relatively small physical sizes. The generation of magnetic field, anomalous transport of angular momentum with decisive bearing on star formation processes, the ubiquitous MHD turbulence under conditions irreproducible in terrestrial laboratories are some of the generic issues still awaiting a concerted effort for their understanding. Quantum Plasmas, pair plasmas and pair-ion plasmas exist under extreme conditions in planetary interiors and exotic stars. In this workshop plasma physicists, astrophysicists and plasma astrophysicists are brought together to discuss these issues.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aGangadhara, R. T. _eeditor. _9310405
700	1		_aKrishan, V. _eeditor. _9310406
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9781402088674
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-1-4020-8868-1 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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