Extremely high speed solar wind: 29–30 October 2003

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Coronal Holes and the High-speed Solar Wind

Coronal holes are the lowest density plasma components of the Sun’s outer atmosphere, and are associated with rapidly expanding magnetic fields and the acceleration of the high-speed solar wind. Spectroscopic and polarimetric observations of the extended corona, coupled with interplanetary particle and radio sounding measurements going back several decades, have put strong constraints on possib...

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ژورنال

عنوان ژورنال: Journal of Geophysical Research

سال: 2004

ISSN: 0148-0227

DOI: 10.1029/2004ja010494