Magnetic turbulent diffusion and the problem of solar surge formation

Title:

Magnetic turbulent diffusion and the problem of solar surge formation

Creator:

Dermendjiev, V. N. and Buyukliev, G. T.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:ad8e017e-74bd-4c20-be39-3ec70e90d223
uuid:ad8e017e-74bd-4c20-be39-3ec70e90d223

Subject:

solar surge and magnetohydrodynamic - numeric simulation

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

The proces of solar eurge formation is atudied by means of computer simulations on the basis of a two-dimensional MHD model. It is assumed in the model that a small-scale magnetic field is penetrating in a compressible plasma medium with physical parameters near to those of the lower chromosphere. Computer simulations show that nonlinear effects lead to formation of relatively denser and hotter structures. This phenomenon is discussed as a link unifying the magnetic and nonmagnetic mechanisms of surge formation proposed by various authors.

Language:

Czech

Rights:

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

Coverage:

113-116

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