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Multiscale Filamentary Structures in the Solar Corona and their Implications for the Origin and Evolutions of the Solar Wind

Multiscale Filamentary Structures in the Solar Corona and their Implications for the Origin and Evolutions of the Solar Wind

Woo, R.; Habbal, S. R.
URI: http://hdl.handle.net/2014/20492
Date: 1998-06-22
Citation: MTG: AIP Conference Proceedings
Lisbou, Portugal

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.

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