000			03306nam a22004935i 4500
001			978-3-540-48053-2
003			DE-He213
005			20160624101853.0
007			cr nn 008mamaa
008			100730s1987 gw | s |||| 0|eng d
020			_a9783540480532 _9978-3-540-48053-2
024	7		_a10.1007/BFb0032307 _2doi
050		4	_aQC801-809
072		7	_aPHVG _2bicssc
072		7	_aSCI032000 _2bisacsh
082	0	4	_a550 _223
082	0	4	_a526.1 _223
245	1	0	_aSolar and Stellar Physics _h[electronic resource] : _bProceedings of the 5th European Solar Meeting Held in Titisee/Schwarzwald, Germany, April 27–30, 1987 / _cedited by Egon-Horst Schröter, Manfred Schüssler.
260		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1987.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1987.
300			_aV, 234 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aLecture Notes in Physics, _x0075-8450 ; _v292
505	0		_aWhat can the sun tell us about stellar activity? -- On the origin of stellar magnetism -- Stellar activity and rotation -- Solar and stellar convection -- Photospheric structure in solar-type stars -- Solar and stellar chromospheres -- Solar an stellar coronae -- Stellar vs. solar activity: The case of pre-main sequence stars -- Winds in late type stars and the solar wind -- Observations from space vs. ground based observations: Advantages and disadvantages -- New ideas about granulation based on data from the solar optical universal polarimeter instrument on spacelab 2 and magnetic data from big bear solar observatory -- Future prospects of stellar and solar physics from space.
520			_aThese proceedings bring together ideas from solar and stellar physics. The sun is near enough for rather detailed observations and one chapter is devoted to the more recent experimental data from observations from space. On the other hand the multitude of stars provides a wide range of physical parameters to test hypotheses in solar and stellar astrophysics. The reader will find an illuminating overview of these fields ranging from the dynamo in the convection zone to the stellar envelopes and winds in the outer regions. In particular the importance of small-scale magnetohydrodynamic processes for the activity phenomena plays an important role in the contributions to this volume. For both students and researchers the general introduction by N. O. Weiss makes an excellent guide to this very active field of research. (See also Lecture Notes in Physics Vol. 291.).
650		0	_aPhysical geography.
650		0	_aAstrophysics.
650	1	4	_aGeosciences.
650	2	4	_aGeophysics/Geodesy.
650	2	4	_aExtraterrestrial Physics, Space Sciences.
700	1		_aSchröter, Egon-Horst. _eeditor.
700	1		_aSchüssler, Manfred. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783540186786
786			_dSpringer
830		0	_aLecture Notes in Physics, _x0075-8450 ; _v292
856	4	0	_uhttp://dx.doi.org/10.1007/BFb0032307
942			_2EBK2680 _cEBK
999			_c31974 _d31974