000			03861nam a22004935i 4500
001			978-0-387-45088-9
003			DE-He213
005			20250710084000.0
007			cr nn 008mamaa
008			100301s2006 xxu| s |||| 0|eng d
020			_a9780387450889 _a99780387450889
024	7		_a10.1007/978-0-387-45088-9 _2doi
082	0	4	_a520 _223
100	1		_aKunow, H. _eauthor.
245	1	0	_aCoronal Mass Ejections _h[recurso electrónico] / _cby H. Kunow, N. U. Crooker, J. A. Linker, R. Schwenn, R. Steiger.
264		1	_aNew York, NY : _bSpringer New York, _c2006.
300			_aVI, 484 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aSpace Sciences Series of ISSI, _x1385-7525 ; _v21
505	0		_aA Brief History of CME Science -- Coronal Mass Ejections: Overview of Observations -- In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections -- An Introduction to CMEs and Energetic Particles -- An Introduction to Theory and Models of CMEs, Shocks, and Solar Energetic Particles -- An Introduction to the pre-CME Corona -- Solar Imprint on ICMEs, Their Magnetic Connectivity, and Heliospheric Evolution -- ICMEs in the Outer Heliosphere and at High Latitudes: an Introduction -- Coronal Observations of CMEs -- Understanding Interplanetary Coronal Mass Ejection Signatures -- Energetic Particle Observations -- CME Theory and Models -- The Pre-CME Sun -- Multi-Wavelength Observations of CMEs and Associated Phenomena -- ICMEs in the Inner Heliosphere: Origin, Evolution and Propagation Effects -- ICMEs at High Latitudes and in the Outer Heliosphere -- CME Disturbance Forecasting -- Coronal Mass Ejections.
520			_aIt is well known that the Sun gravitationally controls the orbits of planets and minor bodies. Much less known, however, is the domain of plasma fields and charged particles in which the Sun governs a heliosphere out to a distance of about 15 billion kilometers. What forces activates the Sun to maintain this power? Coronal Mass Ejections (CMEs) and their descendants are the troops serving the Sun during high solar activity periods. This volume offers a comprehensive and integrated overview of our present knowledge and understanding of Coronal Mass Ejections (CMEs) and their descendants, Interplanetary CMEs (ICMEs). It results from a series of workshops held between 2000 and 2004. An international team of about sixty experimenters involved e.g. in the SOHO, ULYSSES, VOYAGER, PIONEER, HELIOS, WIND, IMP, and ACE missions, ground observers, and theoreticians worked jointly on interpreting the observations and developing new models for CME initiations, development, and interplanetary propagation. The book provides researchers active in space physics with an overview of the current understanding of CMEs and ICMEs, and their effects in the heliosphere. It also provides the advanced graduate student with introductory material on this active field of research.
650		0	_aPHYSICS.
650		0	_aASTRONOMY.
650		0	_aASTROPHYSICS.
650	1	4	_aPHYSICS.
650	2	4	_aASTRONOMY.
650	2	4	_aASTROPHYSICS.
650	2	4	_aEXTRATERRESTRIAL PHYSICS, SPACE SCIENCES.
700	1		_aCrooker, N. U. _eauthor.
700	1		_aLinker, J. A. _eauthor.
700	1		_aSchwenn, R. _eauthor.
700	1		_aSteiger, R. _eauthor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9780387450865
830		0	_aSpace Sciences Series of ISSI, _x1385-7525 ; _v21
856	4	0	_uhttp://dx.doi.org/10.1007/978-0-387-45088-9 _zVer el texto completo en las instalaciones del CICY
912			_aZDB-2-PHA
942			_2ddc _cER
999			_c57665 _d57665