000 03722nam a22003735i 4500
001 284143
003 MX-SnUAN
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007 cr nn 008mamaa
008 150903s2009 ne | o |||| 0|eng d
020 _a9781402092398
_99781402092398
024 7 _a10.1007/9781402092398
_2doi
035 _avtls000336313
039 9 _a201509030258
_bVLOAD
_c201404300314
_dVLOAD
_y201402041346
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB495-500.269
100 1 _aDorman, Lev.
_eautor
_9312083
245 1 0 _aCosmic Rays in Magnetospheres of the Earth and other Planets /
_cby Lev Dorman.
264 1 _aDordrecht :
_bSpringer Netherlands,
_c2009.
300 _brecurso en línea.
336 _atexto
_btxt
_2rdacontent
337 _acomputadora
_bc
_2rdamedia
338 _arecurso en línea
_bcr
_2rdacarrier
347 _aarchivo de texto
_bPDF
_2rda
490 0 _aAstrophysics and Space Science Library,
_x0067-0057 ;
_v358
500 _aSpringer eBooks
505 0 _aFirst Measurements of Cosmic Ray Geomagnetic Effects and the Problem of CR Nature -- Cosmic Rays in the Dipole Geomagnetic Field -- Cosmic Rays in the Real Geomagnetic Field -- Cosmic Ray Planetary Surveys on Ships, Trains, Tracks, Planes, Balloons, and Satellites -- Main Results of Cosmic Ray Survey to Antarctica on the Ship Italica in 1996/97 -- Geomagnetic Variations of Cosmic Rays -- Magnetospheric Models and their Checking by Cosmic Rays -- Galactic Cosmic Rays in Atmospheres and Magnetospheres of Other Planets.
520 _aThis monograph describes the behaviour of cosmic rays in the magnetosphere of the Earth and of some other planets. Recently this has become an important topic both theoretically, because it is closely connected with the physics of the Earth’s magnetosphere, and practically, since cosmic rays determine a significant part of space weather effects on satellites and aircraft. The book contains eight chapters, dealing with – The history of the discovery of geomagnetic effects caused by cosmic rays and their importance for the determination of the nature of cosmic rays or gamma rays – The first explanations of geomagnetic effects within the framework of the dipole approximation of the Earth’s magnetic field – Trajectory computations of cutoff rigidities, transmittance functions, asymptotic directions, and acceptance cones in the real geomagnetic field taking into account higher harmonics – Cosmic ray latitude-longitude surveys on ships, trains, tracks, planes, balloons and satellites for determining the planetary distribution of the intensity of cosmic rays and how it changes with time – Geomagnetic time variations of cosmic rays caused by the changing of internal sources of Earth’s main magnetic field and variable magnetospheric current systems – Magnetospheric models and how to check them by galactic and solar cosmic rays – The behaviour of cosmic rays in the atmospheres and magnetospheres of Venus, Mars, and Jupiter. The work concludes with a discussion of future developments and unsolved problems and contains a list of about thousand full references. This book will be of great interest to experts and students in cosmic ray research, solar-terrestrial physics, magnetosphere physics, and space physics.
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:
_z9781402092381
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-1-4020-9239-8
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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