Article contents
Solar Flare Observations at Submm-waves
Published online by Cambridge University Press: 13 May 2016
Abstract
First 405 GHz and 212 GHz solar flare observations were obtained during short campaigns while the new solar submillimeter-wave telescope (SST) was still undergoing adjustments at the CASLEO El Leoncito observatory in the Argentina Andes. We show here preliminary results for a large X1.1 class X-ray event occurred on 2000 March 22, which exhibited a small submm-w continuum response to the slow (minutes) bulk flare emission, and numerous subsecond spikes (100-300 ms), the brightest spikes reaching about 180 and 50 s.f.u. at 405 and 212 GHz, respectively.
- Type
- Session III: Active Region Structure and Dynamics
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2001
References
- 3
- Cited by