... apply the widely used term ``transient coronalholes'' to avoid confusion between ... various solar features and phenomena from coronalholes to flares in the temperature ...
... The categorization CH (``coronalhole'') means high speed solar wind streams from coronalholes. ... heliospheric current sheet (HCS) position, evolving coronalholes, disappearing filaments, solar flares, coronal mass ejections ...
... accompanying phenomena (dimmings, transient coronalholes, and coronal waves) have ... the data from BST-1 (CrAO, Ukraine) to study the height structure of coronalholes ...
... They give an invaluable information about heating, structure and dynamics of the corona, and temperature distribution of quasi-stable coronal structures (active regions, coronalholes, bright points etc.) ...
... These are needed to construct theoretical models for various plasma structures of the solar corona--flares, active regions, coronalholes, off-limb structures, etc. ...
... These modes are commonly used dur ing target observations, when local structures are monitored (active regions, coronalholes, spicules in polar regions, etc.) ...
... The study of mechanisms of solar wind generation and coronal heating. ... of dynamics and spatial structure of coronal mass ejections up to the heights of 4 ... only instrument registering images of hot coronal plasma with temperatures about 10 ...
... and charged particles, emissions of the coronal mass, and the flow of solar wind all ... structures, i.e., flares, hot clouds, active regions, coronal mass ejections, etc ...