Solar VLBI of compact transient sources

Details Solar VLBI of compact transient sources Solar VLBI of compact transient sources

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..199t&link_type=abstract

(CNR, Workshop on Radio Continua during Solar Flares, Duino, Italy, May 27-31, 1985) Solar Physics (ISSN 0038-0938), vol. 104, M

Astronomy and Astrophysics

Astronomy

6

Radio Sources (Astronomy), Solar Flares, Solar Radio Bursts, Very Long Base Interferometry, Data Acquisition, Emission Spectra, Signal To Noise Ratios, Spectral Energy Distribution, Surges

Scientific paper

Very Long Baseline Interferometry offers the only technique for resolving the transient compact sources which, according to an increasing weight of observational and theoretical evidence, occur during solar flares. In this paper, the problems of applying VLBI to solar observation are discussed and the results obtained so far are presented. It is shown how the technique may be effectively employed in future studies of compact emission structures in solar flares.

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