We examine the temperature structure of static coronal active region loops in regimes where
thermal conductive transport is driven by Coulomb collisions, by turbulent scattering, or by a …

We have expanded upon earlier work that investigates the relative importance of coronal
loops with isothermal versus multithermal cross-field temperature distributions. These results …

Due to their characteristic temperature and density, loop structures in active regions (ARs)
can be seen bright in extreme ultraviolet (EUV) and soft X-ray images. The semiempirical …

For understanding the physical processes in the solar corona, it is helpful to reconstruct the
3D-distribution of plasma density and temperature. We introduce a new iterative method that …