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Large-scale Dimmings Produced by Solar Coronal Mass Ejections According to SOHO/EIT Data in Four EUV Lines
DOI: 10.1134/1.1626196 Bibcode: 2003ARep...47..934C

Grechnev, V. V.; Chertok, I. M.

SOHO/EIT data are used to analyze dimmings, or transient coronal holes (regions of reduced soft-X-ray and EUV emission), which are observed on the solar disk after halo-type coronal mass ejections (CMEs). Simultaneous observations in the 171 Å FeIX/X, 195 Å FeXII, and 284 Å FeIX coronal lines, which are sensitive to temperatures of T e ≈1.2, 1.5, …

2003 Astronomy Reports
SOHO 24
Solar Large-Scale Channeled Dimmings Produced by Coronal Mass Ejections
DOI: 10.1134/1.1554517 Bibcode: 2003ARep...47..139C

Grechnev, V. V.; Chertok, I. M.

A new type of dimmings, or transient coronal holes (i.e., regions of reduced soft-X-ray and EUV emission), is revealed in analyses of difference solar images obtained with the SOHO EIT ultraviolet telescope at 195 Å. Such features can be observed on the solar disk after halo-type coronal mass ejections (CMEs). If several active regions, filaments,…

2003 Astronomy Reports
SOHO 16