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Solar cycle variations and cosmic rays

Author
POTGIETER, M. S1
[1] Unit for Space Physics, School of Physics, North-West University, 2520 Potchefstroom, South Africa
Source

Journal of atmospheric and solar-terrestrial physics. 2008, Vol 70, Num 2-4, pp 207-218, 12 p ; ref : 1 p.1/4

ISSN
1364-6826
Scientific domain
Astronomy earth cosmic environment
Publisher
Elsevier, Oxford
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
Cosmic ray modulation Cosmic rays Heliosphere Solar activity Solar cycles Space weather
Keyword (fr)
Activité solaire Barrière diffusion Champ magnétique solaire Champ magnétique Convection Couche courant Courbure Cycle 22 ans Cycle solaire Dynamique Effet Forbush Fluctuation Héliopause Héliosphère Intensité Long terme Maximum activité solaire Modélisation Processus diffusion Proton Rayonnement cosmique Région interaction corotative Turbulence Valeur extrême Variation temporelle Vent solaire
Keyword (en)
solar activity Diffusion barrier Solar magnetic field magnetic field convection Current sheet Curvature 22 year-Cycle solar cycles dynamics Forbush decrease fluctuations Heliopause Heliosphere intensity Long term Maximum solar activity Modeling Diffusion process protons cosmic rays Corotating interaction region turbulence extreme value time variations solar wind
Keyword (es)
Barrera difusión Campo magnético solar Campo magnético Convección Capa corriente Curvatura Ciclo 22 años Dinámica Efecto Forbush Fluctuación Heliosfera Intensidad Largo plazo Máximo actividad solar Modelización Proceso difusión Protón Región interacción corotativa Variación temporal Viento solar
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics / 001E02I Physics of the ionosphere

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E02 External geophysics / 001E02J Physics of the magnetosphere

Discipline
External geophysics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20140150

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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