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Confinement and anisotropy of ultrahigh-energy cosmic rays in isotropic plasma wave turbulence. I. Modification of the hillas limit due to turbulence geometry

Author
VUKCEVIC, M1 2 ; SCHLICKEISER, R1
[1] Institut für Theoretische Physik, Lehrstuhl IV: Weltraum-und Astrophysik, Ruhr-Universität Bochum, 44780 Bochum, Germany
[2] Department of Physics, University of Montenegro, Podgorica, Montenegro, Serbia and Montenegro
Source

Astronomy and astrophysics (Berlin. Print). 2007, Vol 467, Num 1, pp 15-20, 6 p ; ref : 1/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
ISM: cosmic rays ISM: magnetic fields plasmas scattering
Keyword (fr)
Amortissement Angle attaque Anisotropie Champ magnétique Confinement Dépendance énergie Galaxies Interaction rayon cosmique Onde magnétoacoustique Onde plasma Plasma isotrope Propagation onde Rayonnement cosmique galactique Rayonnement cosmique Turbulence faible Turbulence isotrope Turbulence plasma Voie lactée
Keyword (en)
Damping Pitch angle Anisotropy Magnetic fields Confinement Energy dependence Galaxies Cosmic ray interactions Magnetoacoustic waves Plasma waves Isotropic plasma Wave propagation Galactic cosmic rays Cosmic radiation Weak turbulence Isotropic turbulence Plasma turbulence Milky Way
Keyword (es)
Angulo ataque Plasma isótropo Turbulencia débil Turbulencia isótropa
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18734090

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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