Anisotropies and helicities in the solar wind inertial and dissipation ranges at 1 AU

Author:

Hamilton Kathleen1,Smith Charles W.1,Vasquez Bernard J.1,Leamon Robert J.2

Affiliation:

1. Space Science Center; University of New Hampshire; Durham New Hampshire USA

2. ADNET Systems, Inc.; NASA Goddard Space Flight Center; Greenbelt Maryland USA

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

Reference64 articles.

1. Behannon , K. W. 1975 Observations of the interplanetary magnetic field between 0.46 and 1 AU by the Mariner 10 spacecraft Catholic Univ. of Am. Washington, D. C.

2. Large-amplitude Alfvén waves in the interplanetary medium, 2;Belcher;J. Geophys. Res.,1971

3. Proton and electron mean free paths: The Palmer consensus revisited;Bieber;Astrophys. J.,1994

4. Dominant two-dimensional solar wind turbulence with implications for cosmic ray transport;Bieber;J. Geophys. Res.,1996

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