Topics
magnetic fieldDisease
sound waveLanguage
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres of late type stars which have significant convective envelopes. Principle wave modes are studied for their generation, propagation, and heating properties in the presence of a magnetic field, and various approximations on when a sound wave becomes strong enough to produce heating in the atmosphere are presented
Abstract. Several mechanisms may heat the solar chromosphere: acoustic waves, magne-toacoustic waves...
Stably stratified fluids, such as stellar and planetary atmospheres, can support and propagate gravi...
Abstract. This review focuses on acoustic oscillations in the solar at-mosphere. There is much debat...
This paper presents work performed on the generation and physics of acoustic waves in the solar atmo...
Theoretical models describing solar coronal heating mechanisms are reviewed in some detail. The requ...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Acoustic and magnetoacoustic waves are considered to be possible agents of chromospheric heating. We...
In the first paper of this series we developed a method to construct theoretical, time-dependent an...
The efficiency of non-modal self-heating by acoustic wave perturbations is examined. Considering dif...
In a qualitative sense, the heating of chromospheres and coronae has long been ascribed to either ac...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
Abstract. In a recent paper (Straus et al. 2008) we determined the energy flux of internal gravity w...
Several mechanisms may heat the solar chromosphere: acoustic waves, magnetoacoustic waves (slow, fas...
Physical processes that may lead to solar chromospheric heating are analyzed using high-resolution 1...
Acoustic and magnetoacoustic waves play an important role in the chromospheric heating, exhibiting t...
Abstract. Several mechanisms may heat the solar chromosphere: acoustic waves, magne-toacoustic waves...
Stably stratified fluids, such as stellar and planetary atmospheres, can support and propagate gravi...
Abstract. This review focuses on acoustic oscillations in the solar at-mosphere. There is much debat...
This paper presents work performed on the generation and physics of acoustic waves in the solar atmo...
Theoretical models describing solar coronal heating mechanisms are reviewed in some detail. The requ...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Acoustic and magnetoacoustic waves are considered to be possible agents of chromospheric heating. We...
In the first paper of this series we developed a method to construct theoretical, time-dependent an...
The efficiency of non-modal self-heating by acoustic wave perturbations is examined. Considering dif...
In a qualitative sense, the heating of chromospheres and coronae has long been ascribed to either ac...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
Abstract. In a recent paper (Straus et al. 2008) we determined the energy flux of internal gravity w...
Several mechanisms may heat the solar chromosphere: acoustic waves, magnetoacoustic waves (slow, fas...
Physical processes that may lead to solar chromospheric heating are analyzed using high-resolution 1...
Acoustic and magnetoacoustic waves play an important role in the chromospheric heating, exhibiting t...
Abstract. Several mechanisms may heat the solar chromosphere: acoustic waves, magne-toacoustic waves...
Stably stratified fluids, such as stellar and planetary atmospheres, can support and propagate gravi...
Abstract. This review focuses on acoustic oscillations in the solar at-mosphere. There is much debat...
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