000			03410nam a22004815i 4500
001			978-1-4020-5101-2
003			DE-He213
005			20251006084518.0
007			cr nn 008mamaa
008			100301s2006 ne | s |||| 0|eng d
020			_a9781402051012
020			_a99781402051012
024	7		_a10.1007/1-4020-5101-8 _2doi
082	0	4	_a520 _223
100	1		_aDorman, Lev I. _eauthor.
245	1	0	_aCosmic Ray Interactions, Propagation, and Acceleration in Space Plasmas _h[electronic resource] / _cby Lev I. Dorman.
264		1	_aDordrecht : _bSpringer Netherlands, _c2006.
300			_aXXXIII, 847 p. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aAstrophysics and Space Science Library ; _v339
505	0		_aCosmic Ray Interactions in Space Plasmas -- Cosmic Ray Propagation in Space Plasmas -- Nonlinear Cosmic Ray Effects in Space Plasmas -- Cosmic Ray Acceleration in Space Plasmas.
520			_aThe book consists of four Chapters. Chapter 1 shortly describes main properties of space plasmas and primary CR, different types of CR interactions with space plasmas components (matter, photons, and frozen in magnetic fields). Chapter 2 considers the problem of CR propagation in space plasmas described by the kinetic equation and different types of diffusion approximations (diffusion in momentum space and in pitch-angle space, anisotropic diffusion, anomaly CR diffusion and compound diffusion, the influence of magnetic clouds on CR propagation, non-diffusive CR particle pulse transport). Chapter 3 is devoted to CR non-linear effects in space plasmas caused by CR pressure and CR kinetic stream instabilities with the generation of Alfvèn turbulence (these effects are important in galaxies, in the Heliosphere, in CR and gamma-ray sources and in the processes of CR acceleration). In Chapter 4 different processes of CR acceleration in space plasmas are considered: the development of the Fermi statistical mechanism, acceleration in the turbulent plasma, Alfven mechanism of magnetic pumping, induction mechanisms, acceleration during magnetic collapse and compression, cumulative acceleration mechanism near the zero lines of a magnetic field, acceleration in shear flows, shock-wave diffusion (regular) acceleration. The book ends with a list providing more than 1,300 full references, a discussion on future developments and unsolved problems, as well as Object and Author indexes. This book will be useful for experts and students in CR research, Astrophysics and Geophysics, and in Space Physics.
650		0	_aPHYSICS.
650		0	_aASTRONOMY.
650		0	_aASTROPHYSICS.
650		0	_aPARTICLES (NUCLEAR PHYSICS).
650	1	4	_aPHYSICS.
650	2	4	_aASTRONOMY.
650	2	4	_aEXTRATERRESTRIAL PHYSICS, SPACE SCIENCES.
650	2	4	_aELEMENTARY PARTICLES AND NUCLEI.
650	2	4	_aASTRONOMY, ASTROPHYSICS AND COSMOLOGY.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9781402051005
830		0	_aAstrophysics and Space Science Library ; _v339
856	4	0	_uhttp://dx.doi.org/10.1007/1-4020-5101-8 _zVer el texto completo en las instalaciones del CICY
912			_aZDB-2-PHA
942			_2ddc _cER
999			_c61137 _d61137