000			04149nam a22004815i 4500
001			978-1-4020-4557-8
003			DE-He213
005			20161121230944.0
007			cr nn 008mamaa
008			100301s2006 ne | s |||| 0|eng d
020			_a9781402045578 _9978-1-4020-4557-8
024	7		_a10.1007/1-4020-4557-3 _2doi
050		4	_aQB600-701
072		7	_aPGS _2bicssc
072		7	_aSCI031000 _2bisacsh
082	0	4	_a523.4 _223
245	1	0	_aSolar journey: The significance of our galactic environment for the heliosphere and earth _h[electronic resource] / _cedited by Priscilla C. Frisch.
264		1	_aDordrecht : _bSpringer Netherlands, _c2006.
300			_aXXV, 413 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
505	0		_aIntroduction: Paleoheliosphere versus PaleoLISM -- Heliospheric Variation in Response to Changing Interstellar Environments -- The Influence of the Interstellar Magnetic Field on the Heliospheric Interface -- Interstellar Conditions and Planetary Magnetospheres -- Long-term Variations in the Galactic Environment of the Sun -- Short-term Variations in the Galactic Environment of the Sun -- Variations of the Interstellar Dust Distribution in the Heliosphere -- Effects in the Inner Heliosphere Caused by Changing Conditions in the Galactic Environment -- Variable Terrestrial Particle Environments During the Galactic Orbit of the Sun -- The Galactic Cosmic Ray Intensity in the Heliosphere in Response to Variable Interstellar Environments -- Accretion of Interstellar Material into the Heliosphere and onto Earth -- Variations of Galactic Cosmic Rays and the Earth's Climate.
520			_aHumans evolved when the Sun was in the great void of the Local Bubble. The Sun entered the present environment of interstellar clouds only during the late Quaternary. Astronomical data reveal these long and short term changes in our galactic environment. Theoretical models then tell us how these changes affect interplanetary particles, planetary magnetospheres, and the Earth itself. Cosmic rays leave an isotopic signature in the paleoclimate record that helps trace the solar journey through space. "Solar Journey: The Significance of Our Galactic Environment for the Heliosphere and Earth" lays the foundation for an interdisciplinary study of the influence of interstellar material on the solar system and Earth as we travel through the Milky Way Galaxy. The solar wind bubble responds dynamically to interstellar material flowing past the Sun, regulating interstellar gas, dust, and cosmic particle fluxes in the interplanetary medium and the Earth. Cones of interstellar gas and dust focused by solar gravity, the magnetospheres of the outer planets, and cosmic rays at Earth all might yield the first hints of changes in our galactic environment. Twelve articles from leading experts in diverse fields discuss the physical changes expected as the heliosphere adjusts to its galactic environment. Topics include the interaction between the solar wind and interstellar dust and gas, cosmic ray modulation, magnetospheres, temporal variations in the solar environment, and the cosmic ray isotope record preserved in paleoclimate data. The breadth of processes discussed in this book make it a valuable resource for scientists and students doing research in the fields of Space Physics, Astronomy and the Paleoclimate. .
650		0	_aEarth sciences.
650		0	_aPlanetology.
650		0	_aAstronomy.
650		0	_aAstrophysics.
650		0	_aCosmology.
650		0	_aSpace sciences.
650	1	4	_aEarth Sciences.
650	2	4	_aPlanetology.
650	2	4	_aAstronomy, Astrophysics and Cosmology.
650	2	4	_aExtraterrestrial Physics, Space Sciences.
700	1		_aFrisch, Priscilla C. _eeditor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9781402043970
856	4	0	_uhttp://dx.doi.org/10.1007/1-4020-4557-3
912			_aZDB-2-PHA
950			_aPhysics and Astronomy (Springer-11651)
999			_c506405 _d506405