Several problems in astrophysics are examined where departures from purely thermal behavior are expected to produce effects which are detectable by a variety of NASA satellites. The problems identified as worthy of study include coronal heating in stars, deposition of non-thermal particle energy in stars from external sources, and turbulence in atmospheres and winds of stars. The progress in solving these problems is summarized
. Numerical simulations can lead to new insights into astrophysical processes that would be difficu...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...
The solar wind has been measured directly from 0.3 AU outward, and the Sun's atmosphere has been ima...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
Theoretical models describing solar coronal heating mechanisms are reviewed in some detail. The requ...
The identification of small-scale 3-D heating events in numerical simulations brought us a step clos...
The S055 EUV spectra was used to perform emission measure and line intensity ratio analyses of loop ...
The present state of development of the theory of coronal heating is summarized. Coronal heating is ...
Convective instability in the solar corona growth, especially linear growth, was studied. An investi...
Progress in the theory of stellar convection over the past decade is reviewed. The similarities and ...
The final report discusses work completed on proposals to construct state-of-the-art, theoretical, t...
A new three-dimensional hydrodynamics code has been developed to model the propagation of acoustical...
Observations of the corona and solar wind are analyzed and compared with generalized results derived...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
This paper presents work performed on the generation and physics of acoustic waves in the solar atmo...
. Numerical simulations can lead to new insights into astrophysical processes that would be difficu...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...
The solar wind has been measured directly from 0.3 AU outward, and the Sun's atmosphere has been ima...
The solar corona, the tenuous outer atmosphere of the Sun, is orders of magnitude hotter than the so...
Theoretical models describing solar coronal heating mechanisms are reviewed in some detail. The requ...
The identification of small-scale 3-D heating events in numerical simulations brought us a step clos...
The S055 EUV spectra was used to perform emission measure and line intensity ratio analyses of loop ...
The present state of development of the theory of coronal heating is summarized. Coronal heating is ...
Convective instability in the solar corona growth, especially linear growth, was studied. An investi...
Progress in the theory of stellar convection over the past decade is reviewed. The similarities and ...
The final report discusses work completed on proposals to construct state-of-the-art, theoretical, t...
A new three-dimensional hydrodynamics code has been developed to model the propagation of acoustical...
Observations of the corona and solar wind are analyzed and compared with generalized results derived...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
This paper presents work performed on the generation and physics of acoustic waves in the solar atmo...
. Numerical simulations can lead to new insights into astrophysical processes that would be difficu...
This paper discusses the possibility that heating of the solar corona in open field-line regions ema...
The solar wind has been measured directly from 0.3 AU outward, and the Sun's atmosphere has been ima...