Large-Scale Magnetic Structures Responsible for Coronal Disturbances
نویسندگان
چکیده
منابع مشابه
Large-scale Coronal Density and Abundance Structures and Their Association with Magnetic Field Structure
We construct subsynoptic maps of the ultraviolet-line fluxes, electron density, and elemental abundances for an east limb corona at 1.63 solar radii from 2000 September 20 to October 1. The data, covering position angles of 85 Y126 , were taken from the Ultraviolet Coronagraph Spectrometer (UVCS) on board the Solar and Heliospheric Observatory (SOHO), and the maps are based on the variation of ...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1974
ISSN: 0074-1809
DOI: 10.1017/s0074180900234116