Some magnetohydrodynamic aspects of the problem of solar surge formation and dynamics

Title:

Some magnetohydrodynamic aspects of the problem of solar surge formation and dynamics

Creator:

Dermendjiev, V. N.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:00d0efac-2989-4114-9b41-f1fe5f3a8303
uuid:00d0efac-2989-4114-9b41-f1fe5f3a8303

Subject:

magnetohydrodynamics and chromospheric plasma

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

Different modes of magnetic field - chromospheric plasma interaction are possible under the assumption that the energy is released impulsively. One of them leads to the creation of small-scale impulsive structures such as forced plume and dynamical stable current filaments. These structures we consider as basic MHD elements of the plasma of the solar active phenomena. We show that such a structuralization plays an important role in the process of solar surge formation and dynamics.

Language:

Czech

Rights:

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

Coverage:

138-138

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1998 Volume:87-88 | Number:88

Harvested from:

CDK

Metadata only:

false