The Coronal Analysis of SHocks and Waves (CASHeW) framework
Coronal bright fronts (CBF) are large-scale wavelike disturbances in the solar corona, related to solar eruptions. They are observed (mostly in extreme ultraviolet (EUV) light) as transient bright fronts of finite width, propagating away from the eruption source location. Recent studies of individua...
| Main Authors: | , , , , |
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| Other Authors: | |
| Language: | en |
| Published: |
EDP SCIENCES S A
2017
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| Online Access: | http://hdl.handle.net/10150/626293 http://arizona.openrepository.com/arizona/handle/10150/626293 |