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Multiscale Filamentary Structures in the Solar Corona and their Implications for the Origin and Evolutions of the Solar WindA change in the paradigm of coronal structure has emerged as a result of definitive measurements made with radio occultation, white-light (SOHO/LASCO), ultraviolet (SOHO/UVCS), and soft X-ray (Yohkoh) measurements.
Document ID
20060041503
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/20492
Authors
Woo, R.
Habbal, S. R.
Date Acquired
August 23, 2013
Publication Date
June 22, 1998
Publication Information
Publication: AIP Conference Proceedings
Subject Category
Solar Physics
Distribution Limits
Public
Copyright
Other
Keywords
Filamentary Structures solar wind corona

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