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Some results of bidimensional spectroscopic observations of solar active regions and flares.

B. Caccin, A. Donati-Falchi, R. Falciani, G. Roberti, and L.A. Smaldone

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Abstract

Bidimensional spectroscopy of solar chromospheric structures has been performed at the Sacramento Peak Observatory (SPO) for a collaborative study of active regions and flares together with radio and space-born NASA—SMM observations within the framework of the Solar Maximum Year activities.

© 1983 Optical Society of America

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