Coronal partings
Coronal partings
- New search for: Nikulin, Igor F.
- New search for: Dumin, Yurii V.
- New search for: Nikulin, Igor F.
- New search for: Dumin, Yurii V.
Abstract The basic observational properties of “coronal partings”—the special type of quasi-one-dimensional magnetic structures, identified by a comparison of the coronal X-ray and EUV images with solar magnetograms—are investigated. They represent the channels of opposite polarity inside the unipolar large-scale magnetic fields, formed by the rows of magnetic arcs directed to the neighboring sources of the background polarity. The most important characteristics of the partings are discussed. It can be naturally assumed that—from the evolutionary and spatial points of view—the partings can transform into the coronal holes and visa versa. The classes of global, intersecting, and complex partings are identified.
Document information
Coronal partings
Advances in Space Research ; 57 , 3 ; 904-911
2015-11-19
8 pages
Article (Journal)
Electronic Resource
English
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