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The cosmic radiation in the heliosphere at successive solar minima : steady state no-drift solutions of the transport equation

Author
REINECKE, J. P. L1 ; MORAAL, H1 ; MCDONALD, F. B
[1] Potchefstroom univ. Christian higher eduction, dep. physics, Potchefstroom 2520, South Africa
Source

Journal of geophysical research. 1993, Vol 98, Num A6, pp 9417-9431 ; ref : 37 ref

ISSN
0148-0227
Scientific domain
Astronomy earth cosmic environment; Geology; Geophysics; Climatology, meteorology; Oceanography
Publisher
American Geophysical Union, Washington, DC
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Equation transport Gradient densité Gradient radial Hydrogène Atome Héliosphère Hélium Ion atomique Intensité Minimum activité solaire Modèle 2 dimensions Observation par sonde spatiale Oxygène Ion atomique Rayonnement cosmique galactique Satellite IMP-8 Sonde Pioneer-10 Sonde Pioneer-11 Sonde Voyager-1 Sonde Voyager-2
Keyword (en)
Transport equation Density gradient Radial gradient Hydrogen Atoms Heliosphere Helium Atomic ions Intensity Minimum solar activity Two dimensional model Space probe observation Oxygen Atomic ions Galactic cosmic ray
Keyword (es)
Ecuación transporte Gradiente densidad Gradiente radial Hidrógeno Atomo Heliosfera Helio Ión atómico Intensidad Mínimo actividad solar Modelo 2 dimensiones Observación por sonda espacial Oxígeno Ión atómico Radiación cósmica galáctica
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B50 Interplanetary space

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
4787750

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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