Add to ORKGA study of stellar chromospheres based on the internal structure of particular stars is presented. Used are complex flow diagrams of the linkage paths between mass loss, angular momentum loss, magnetic field from the turbulent dynamo and its relations to differential rotations and the convection zone, and stellar evolution
In the first paper of this series we developed a method to construct theoretical, time-dependent an...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...
Context. The Sun and other cool stars harbouring outer convection zones manifest magnetic activity i...
The final report discusses work completed on proposals to construct state-of-the-art, theoretical, t...
The Sun, stars similar to it, and many rather dissimilar to it, have chromospheres, regions classica...
Abstract. The renewal of chromospheric activity in red giants and super-giants is interpreted in ter...
Direct observational evidence of stellar chromospheres is provided by H and K lines and their relati...
Stars constitute undoublty one of the elementary blocks of the Universe and play as such a central r...
Detailed theoretical studies of chromospheric inhomogeneities consider dynamics as well as radiative...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
This contribution is meant as a very brief introduction to the principal concepts of stellar physics...
Major advances in our understanding of non-radiative heating and other activity in stars cooler than...
In this work we try to establish a connection between the dynamo effect, which operates in the conve...
We computed chromospheric models of the Sun as a star and of nine solar analogues. The atmospheric m...
The activity in RS Canum Venaticorum (CVn) is investigated. Models for chromospheric structure are d...
In the first paper of this series we developed a method to construct theoretical, time-dependent an...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...
Context. The Sun and other cool stars harbouring outer convection zones manifest magnetic activity i...
The final report discusses work completed on proposals to construct state-of-the-art, theoretical, t...
The Sun, stars similar to it, and many rather dissimilar to it, have chromospheres, regions classica...
Abstract. The renewal of chromospheric activity in red giants and super-giants is interpreted in ter...
Direct observational evidence of stellar chromospheres is provided by H and K lines and their relati...
Stars constitute undoublty one of the elementary blocks of the Universe and play as such a central r...
Detailed theoretical studies of chromospheric inhomogeneities consider dynamics as well as radiative...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
This contribution is meant as a very brief introduction to the principal concepts of stellar physics...
Major advances in our understanding of non-radiative heating and other activity in stars cooler than...
In this work we try to establish a connection between the dynamo effect, which operates in the conve...
We computed chromospheric models of the Sun as a star and of nine solar analogues. The atmospheric m...
The activity in RS Canum Venaticorum (CVn) is investigated. Models for chromospheric structure are d...
In the first paper of this series we developed a method to construct theoretical, time-dependent an...
A dynamical model was proposed which is in agreement with the observations that suggest the solar ch...
Context. The Sun and other cool stars harbouring outer convection zones manifest magnetic activity i...