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Coronal partings

MPG-Autoren
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Dumin,  Yurii V.
Max Planck Institute for the Physics of Complex Systems, Max Planck Society;

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Zitation

Nikulin, I. F., & Dumin, Y. V. (2016). Coronal partings. ADVANCES IN SPACE RESEARCH, 57(3), 904-911. doi:10.1016/j.asr.2015.11.020.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0029-C7EF-3
Zusammenfassung
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.