Heliospheric pick-up ions influencing thermodynamics and dynamics of the distant solar wind

Nonlinear Processes in Geophysics

Volumn 9, Issue 3-4, 2002, Pages 377-386

  Fahr, H J ^a   Rucinski, D ^b  

^a UNIVERSITY OF BONN   (Germany)

^b Polish Academy of Sciences ^*  (Poland)

Author keywords

[No Author keywords available]

Indexed keywords

SOLAR ACTIVITY; SOLAR WIND; THERMODYNAMICS;

EID: 0036319322     PISSN: 10235809     EISSN: None     Source Type: Journal    
DOI: 10.5194/npg-9-377-2002     Document Type: Article

References (41)

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4. A three-fluid model of the solar wind termination shock including a continuous production of anomalous cosmic rays
5. The three-fluid structure of the particle modulated solar wind termination shock
6. Spectra of energized pick-up ions upstream of the heliospheric termination shock I. The role of Alfvénic turbulences
7. Spectra of energized pick-up ions upstream of the two-dimensional heliospheric termination shock. II. Acceleration by Alfvénic and by large-scale solar wind turbulences
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20. o electromagnetic instabilities
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22. Conductive solar wind models in rapidly diverging flow geometries
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24. Velocity space diffusion from weak plasma turbulence in a magnetic field
25. Effects of cosmic rays and interstellar gas on the dynamics of a wind
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35. The termination shock 1979-1996
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37. Diffuse ions produced by electromagnetic ion beam instabilities
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