Author:
Noyes R. W.,Foukal P. V.,Huber M. C. E.,Reeves E. M.,Schmahl E. J.,Timothy J. G.,Vernazza J. E.,Withbroe G. L.
Abstract
In this paper we review some preliminary results from the Harvard College Observatory Extreme Ultraviolet Spectroheliometer on ATM that pertain to solar activity. The results reviewed here are described in more detail in other papers referred to in the text. In the following paragraphs we first describe the instrument and its capabilities, and then turn to results on active regions, sunspots, flares, EUV bright points, coronal holes, and prominences.
Publisher
Cambridge University Press (CUP)
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1. 3.1.2.3 Sunspots;Landolt-Börnstein - Group VI Astronomy and Astrophysics