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Detailed Reference Information |
Hakamada, K. (1987). Three-dimensional structure of the coronal magnetic field and the solar wind speed distribution projected on the photosphere in 1974. Journal of Geophysical Research 92: doi: 10.1029/JA092iA05p04339. issn: 0148-0227. |
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Keywords
Interplanetary Physics, Interplanetary magnetic fields, Interplanetary Physics, Sources of the solar wind, Solar Physics, Astrophysics, and Astronomy, Corona and transition region |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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