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Measuring coronal magnetic fields with remote sensing observations of shock waves

Journal
Date Issued
2016
Author(s)
•
•
•
DOI
Abstract
Recent works demonstrated that remote sensing observations of shock waves propagating into the corona and associated with major solar eruptions can be used to derive the strength of coronal magnetic fields met by the shock over a very large interval of heliocentric distances and latitudes. This opinion article will summarize most recent results obtained on this topic and will discuss the weaknesses and strengths of these techniques to open a constructive discussion with the scientific community.
Volume
3
Start page
17
Uri
Url
Issn Identifier
2296-987X
Ads BibCode
2016FrASS...3...17B
Rights
open.access
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