Results 101 to 110 of about 5,203 (216)
Context. The solar chromosphere is a dynamic and crucial interface between the solar interior and its interplanetary environment, regulating how energy is locally deposited into heat and transported into the upper atmospheric layers.
M. Carlsson, G. Aulanier, Q. Noraz
core +1 more source
The multi-thermal chromosphere: Inversions of ALMA and IRIS data
Context. Numerical simulations of the solar chromosphere predict a diverse thermal structure with both hot and cool regions. Observations of plage regions in particular typically feature broader and brighter chromospheric lines, which suggests that they ...
De Pontieu, Bart Walter +20 more
core +1 more source
3-D hydrodynamic simulations of the solar chromosphere
We present first results of three-dimensional numerical simulations ofthe non-magnetic solar chromosphere, computed with the radiationhydrodynamics code CO5BOLD.
Wedemeyer, S. +8 more
core +1 more source
The quiet chromosphere: old wisdom, new insights, future needs [PDF]
The introduction to this review summarizes chromosphere observation with two figures. The first part showcases the historical emphasis on the eclipse chromosphere in the development of NLTE line formation theory and criticizes 1D modeling.
Astrophysics +2 more
core
The Bright Rim Prominences according to 2.5D Radiative Transfer
Solar prominences observed close to the limb commonly include a bright feature that, from the perspective of the observer, runs along the interface between itself and the underlying chromosphere. Despite several idealized models being proposed to explain
Jack M. Jenkins +4 more
doaj +1 more source
Propagation of alfvénic waves from corona to chromosphere and consequences for solar flares
How do magnetohydrodynamic waves travel from the fully ionized corona, into and through the underlying partially ionized chromosphere, and what are the consequences for solar flares?
Fletcher, L. +2 more
core +1 more source
Observations of the Formation and Disappearance of a Funnel Prominence
We present an observational study of the formation and disappearance of a funnel prominence. Before the funnel prominence formed, cool materials from the top of a preexisting polar crown prominence flowed along saddle-shaped coronal loops to their base ...
Bo Yang +3 more
doaj +1 more source

