MHD compressive turbulence in the solar wind and the nearly incompressible approach

Astrophysics and Space Science

Volumn 243, Issue 1, 1996, Pages 159-162

  Bavassano, B ^a   Bruno, R ^a   Rosenbauer, H ^b  

^a CNR   (Italy)

^b MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Density Fluctuations; MHD Turbulence; Solar Wind

Indexed keywords

EID: 0346674425     PISSN: 0004640X     EISSN: None     Source Type: Journal    
DOI: 10.1007/BF00644047     Document Type: Article

References (4)

1. Bavassano, B. and Bruno, R.: 1995, 'Density fluctuations and turbulent Mach numbers in the inner solar wind', J. Geophys. Res. , in press
2. Bavassano, B., Bruno, R. and Klein, L. W.: 1995, 'Density-temperature correlation in solar wind MHD fluctuations: A test for nearly incompressible models', J. Geophys. Res. , in press
3. Tu, C.-Y. and Marsch, E.: 1994, 'On the nature of compressive fluctuations in the solar wind', J. Geophys. Res. 99, 21,481-21,509
4. Zank, G. P. and Matthaeus, W. H.: 1992, 'Waves and turbulence in the solar wind', J. Geophys. Res. 97, 17,189-17,194