Page
%P
![Loading...](https://link.springer.com/static/c4a417b97a76cc2980e3c25e2271af3129e08bbe/images/pdf-preview/spacer.gif)
-
Chapter and Conference Paper
Flows through the magnetically structured solar atmosphere
The upper solar atmosphere until three solar radii is controlled by the magnetic field. The plasma β (P kin/P magn) is decreasing with increasing altitude in the low coro...