000			03287nam a22005535i 4500
001			978-3-540-74302-6
003			DE-He213
005			20161121231051.0
007			cr nn 008mamaa
008			100301s2008 gw | s |||| 0|eng d
020			_a9783540743026 _9978-3-540-74302-6
024	7		_a10.1007/978-3-540-74302-6 _2doi
050		4	_aQB495-500.269
072		7	_aTTDS _2bicssc
072		7	_aSCI005000 _2bisacsh
082	0	4	_a520 _223
082	0	4	_a500.5 _223
100	1		_aBalogh, André. _eauthor.
245	1	4	_aThe Heliosphere through the Solar Activity Cycle _h[electronic resource] / _cby André Balogh, Louis J. Lanzerotti, Steven T. Suess.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c2008.
300			_aXXV, 286 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aSpringer Praxis Books
505	0		_aThe heliosphere: Its origin and exploration -- Solar cycle 23 -- The solar wind throughout the solar cycle -- The global heliospheric magnetic field -- Heliospheric energetic particle variations -- Galactic and anomalous cosmic rays through the solar cycle: New insights from Ulysses -- Overview: The heliosphere then and now.
520			_aUnderstanding how the Sun changes though its 11-year sunspot cycle and how these changes affect the vast space around the Sun – the heliosphere – has been one of the principal objectives of space research since the advent of the space age. This book presents the evolution of the heliosphere through an entire solar activity cycle. The last solar cycle (cycle 23) has been the best observed from both the Earth and from a fleet of spacecraft. Of these, the joint ESA-NASA Ulysses probe has provided continuous observations of the state of the heliosphere since 1990 from a unique vantage point, that of a nearly polar orbit around the Sun. Ulysses’ results affect our understanding of the heliosphere from the interior of the Sun to the interstellar medium - beyond the outer boundary of the heliosphere. Written by scientists closely associated with the Ulysses mission, the book describes and explains the many different aspects of changes in the heliosphere in response to solar activity. In particular, the authors describe the rise in solar activity from the last minimum in solar activity in 1996 to its maximum in 2000 and the subsequent decline in activity.
650		0	_aPhysics.
650		0	_aPlanetology.
650		0	_aAstrophysics.
650		0	_aSpace sciences.
650		0	_aAerospace engineering.
650		0	_aAstronautics.
650	1	4	_aPhysics.
650	2	4	_aExtraterrestrial Physics, Space Sciences.
650	2	4	_aAstrophysics and Astroparticles.
650	2	4	_aPlanetology.
650	2	4	_aAerospace Technology and Astronautics.
700	1		_aLanzerotti, Louis J. _eauthor.
700	1		_aSuess, Steven T. _eauthor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783540743019
830		0	_aSpringer Praxis Books
856	4	0	_uhttp://dx.doi.org/10.1007/978-3-540-74302-6
912			_aZDB-2-PHA
950			_aPhysics and Astronomy (Springer-11651)
999			_c508073 _d508073