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Three-dimensional structure of the coronal magnetic field and the solar wind speed distribution projected on the photosphere in 1974

✍ Scribed by Hakamada, Kazuyuki

Book ID: 119715448
Publisher: American Geophysical Union
Year: 1987
Tongue: English
Weight: 856 KB
Volume: 92
Category: Article
ISSN: 0148-0227
DOI: 10.1029/ja092ia05p04339

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