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Solar Flare Observations at Submm-waves

Published online by Cambridge University Press:  13 May 2016

P. Kaufmann
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo Unicamp, Campinas
J.-P. Raulin
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo
E. Correia
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo Inpe, São José dos Campos, Brazil
J. E. R. Costa
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo Inpe, São José dos Campos, Brazil
C. G. Giménez de Castro
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo
A. V. R. Silva
Affiliation:
CRAAM/CRAAE, Universidade Presbiteriana Mackenzie, São Paulo
H. Levato
Affiliation:
Complejo Astronómico El Leoncito, San Juan, Argentina
M. Rovira
Affiliation:
Instituto de Astronomia y Física del Espacio, Buenos Aires, Argentina
C. Mandrini
Affiliation:
Instituto de Astronomia y Física del Espacio, Buenos Aires, Argentina
R. Fernández-Borda
Affiliation:
Instituto de Astronomia y Física del Espacio, Buenos Aires, Argentina
O. Bauer
Affiliation:
Max-Planck-Institut fur extraterrestrische Physik, Garching, Germany

Abstract

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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
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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