INNER HELIOSPHERE OBSERVATIONS OF MHD TURBULENCE IN THE SOLAR WIND. CHALLENGES TO THEORY-Reference-Cited by-同舟云学术

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INNER HELIOSPHERE OBSERVATIONS OF MHD TURBULENCE IN THE SOLAR WIND. CHALLENGES TO THEORY

Published:1992 Issue: Volume: Page:423-428
ISSN:
Container-title:Solar Wind Seven
language:
Short-container-title:

Author:

Bruno R.

Publisher

Elsevier

Reference6 articles.

1. Origin of low cross-helicity regions in the solar wind;Bruno;J. Geophys. Res.,1991

2. “Alfvénic” versus “standard” turbulence in the solar wind;Grappin;Ann. Geophys.,1991

3. MHD turbulence in the solar wind;Marsch,1991

4. Turbulence and waves in the solar wind, U.S. National Report 1987–1990;Roberts;Rev. Geophys., suppl.,1991

5. Large-scale structure of interplanetary medium;Schwenn,1991

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1. Turbulence transport in the solar corona: Theory, modeling, and Parker Solar Probe;Physics of Plasmas;2021-08

2. Boundary of the Slow Solar Wind;The Astrophysical Journal;2018-09-10

3. Turbulence Studied via Elsässer Variables;Turbulence in the Solar Wind;2016

4. Early Observations of MHD Turbulence;Turbulence in the Solar Wind;2016

5. Observations of magnetohydrodynamic turbulence in the 3D heliosphere;Advances in Space Research;2005-01

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