Abstract VLA observations at 91.6 cm wavelength describe large-scale features that either conicide with filaments, seen in emission rather than absorption, or act as large-scale magnetic loops that connect active regions and provide a conduit for relativistic electrons that trigger bursts at remote sites on the solar surface. VLA observations at 20.7 cm wavelength describe smaller, hotter coronal loops within active regions where impulsive bursts originate.
VLA observations of the inner corona
Advances in Space Research ; 11 , 1 ; 159-163
1991-01-01
5 pages
Article (Journal)
Electronic Resource
English
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