Connection of the large-scale solar magnetic and velocity fields with the solar active phenomena

Title:

Connection of the large-scale solar magnetic and velocity fields with the solar active phenomena

Creator:

Ambrož, Pavel

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:24970825-7d55-47ab-8ff8-cdef6f4ecbbe
uuid:24970825-7d55-47ab-8ff8-cdef6f4ecbbe

Subject:

solar photosphere, large-scale solar magnetic fields, and large-scale solar velocity fields

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

The paper characterizes the evolution, structure and areal distribution of the large-scale background magnetic fields in the solar photosphere. The direction of the horizontal streaming of the solar photospheric plasma was found. Active regions are formed mainly in places where the global circulation displays maximum velocity. Filaments occur in the areas with a high value of velocity gradient perpendicular to the filament axis. The relationship between the weak background and the strong local magnetic fields is documented.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

117-127

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:66

Harvested from:

CDK

Metadata only:

false