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|Title: ||Multiscale Filamentary Structures in the Solar Corona and their Implications for the Origin and Evolutions of the Solar Wind|
|Authors: ||Woo, R.|
Habbal, S. R.
|Issue Date: ||22-Jun-1998 |
|Citation: ||MTG: AIP Conference Proceedings|
|Abstract: ||A 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.|
|Appears in Collections:||JPL TRS 1992+|
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