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020 _a9781402045578
_99781402045578
024 7 _a10.1007/1402045573
_2doi
035 _avtls000334818
039 9 _a201509030224
_bVLOAD
_c201404120850
_dVLOAD
_c201404090628
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_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB1-991
100 1 _aFrisch, Priscilla C.
_eeditor.
_9309372
245 1 0 _aSolar journey: The significance of our galactic environment for the heliosphere and earth /
_cedited by Priscilla C. Frisch.
264 1 _aDordrecht :
_bSpringer Netherlands,
_c2006.
300 _axxv, 413 páginas
_brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
500 _aSpringer eBooks
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.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9781402043970
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/1-4020-4557-3
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999 _c282550
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