The first high-spatial-resolution interferometric observations of solar flares at millimeter wavelengths are presented. They are of high sensitivity, and events ranging from subflares to X-class flares were detected. One to three baselines with fringe spacings of 2 to 5 arcsec were available, which demonstrated that generally source sizes were in excess of 2 arcsec, but in some events the sources may be about 1 arcsec.
High spatial resolution observations of solar flares at 3.3 mm wavelength
1991-01-01
Miscellaneous
No indication
English
Interferometric observations of solar flares at 3 mm wavelength
Elsevier | 1993
|Multi-Wavelength Observations of the Pre-Cursor Phase of Solar Flares
British Library Conference Proceedings | 2003
|Multi-wavelength observations of the pre-cursor phase of solar flares
Online Contents | 2003
|Extreme Ultraviolet Observations of Solar Flares
AIAA | 1972
|