Solar Large-Scale Emitting Chains: Evidences of Reality and Some Features,

by I.M. Chertok

Fig. The SOHO/EIT 171 Å image (a) illustrating a pronounced transequatorial inverted V-shaped chain 1-2-3-4 which appears to outline the large soft X-ray CH observed with the Yohkoh/SXT (b) on March 1-2, 1999.  The BBSO H-alpha (c) and MLSO/HAO He I 10830 Å (d) heliograms are shown to demonstrate relation of this and some other EUV chains to other large-scale structures such as H-alpha filaments and He I 10830 Å features.

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