перевести предложения.
If a magnetic field is present with its lines of field running parallel to the filaments, then coronal material can easily flow in this direction but magnetic pressure will prevent it from expanding sideways. So we can picture a filament as a flexible tube, something like an airport windsock whose direction indicates where the coronal gas is following. The radial structure of the filaments that is observed is, in fact, strong evidence for the existence of a solar wind always blowing outwards from the Sun.

Дайяник    1   25.03.2020 08:22    1