A model of solar wind fluctuations with two components: Alfvén waves and convective structures-Reference-Cited by-同舟云学术

A model of solar wind fluctuations with two components: Alfvén waves and convective structures

Published:1993-02-01 Issue:A2 Volume:98 Page:1257-1276
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res.

Author:

Tu C.-Y.,Marsch E.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/92JA01947/fullpdf

Reference73 articles.

1. Evidence of local generation of Alfvénic turbulence in the solar wind;Bavassano;J. Geophys. Res.,1989

2. Solar wind fluctuations at large scale: A comparison between low and high solar activity conditions;Bavassano;J. Geophys. Res.,1991

3. On the role of interplanetary sources in the evolution of low-frequency Alfvénic turbulence in the solar wind;Bavassano;J. Geophys. Res.,1992

4. Radial variation of interplanetary Alfvénic fluctuations: Pioneer 10 and 11 observations between 1 and 5 AU;Bavassano;J. Geophys. Res.,1986

5. Radial evolution of power spectra of interplanetary Alfvénic turbulence;Bavassano;J. Geophys. Res.,1982

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