VLA observations at 91.6 cm wavelength describe large-scale features that either coincide 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 19
1991-01-01
Miscellaneous
No indication
English
Inner corona from solar radio observations
Elsevier | 1991
|VLA observations of the inner corona
Elsevier | 1991
|Models for inner corona parameters
Elsevier | 1991
|Temperature Measurements in the Inner Corona
British Library Online Contents | 1992
|