The Parker spiral configuration of the interplanetary magnetic field between 1 and 8.5 AU-Reference-Cited by-同舟云学术

The Parker spiral configuration of the interplanetary magnetic field between 1 and 8.5 AU

Published:1980 Issue:A12 Volume:85 Page:6861
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Thomas Barry T.,Smith Edward J.

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://www.agu.org/journals/ja/v085/iA12/JA085iA12p06861/JA085iA12p06861.pdf

Reference20 articles.

1. Evidence of a structure free state at high solar wind speeds;Bame;J. Geophys. Res.,1977

2. Heliocentric distance dependence of the interplanetary magnetic field;Behannon;Rev. Geophys. Space Phys.,1978

3. Interplanetary acceleration of nucleons at 15° solar latitude by plasma stream-stream interaction regions corotating with the sun;Cherneff;Astrophys. J. Lett.,1980

4. Measurements of the interplanetary magnetic field in relation to the modulation of cosmic rays;Hedgecock;Solar Phys.,1975

5. The heliographic latitude dependence and sector structure of the interplanetary magnetic field 1969–1974: Results from the Heos satellites;Hedgecock;Solar Phys.,1975

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