Add to ORKGAbstract. This review focuses on acoustic oscillations in the solar at-mosphere. There is much debate on photospheric pistons to chromo-spheric oscillations, on the penetration height of acoustic shocks, and on their contribution to chromospheric heating, with new input coming from space observations and from numerical simulations. Less progress is made in identifying wave modes or wave heating in magnetic structures, but it seems that umbral flashes are ripe for understanding. 1
Context. The exact nature of the quiet solar chromosphere and especially its temporal variation, ar...
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
This review focuses on acoustic oscillations n the solar at- mosphere.There s much debate on photos...
Aims.This paper aims to look at the propagation of synthetic photospheric oscillations from a point ...
Abstract. We analyze oscillations in the solar atmosphere using image sequences from the Transition ...
The solar chromosphere has never been static although it was often modeled so.Even the quiet-sun in...
Abstract The direct propagation of acoustic waves, driven harmonically at the solar photo-sphere, in...
The leakage and coupling of solar global oscillations to the overlaying magnetized solar atmosphere ...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
Both the interior and the atmosphere of the Sun give a wide range of oscillations and waves. Interac...
We have studied the nonlinear response of the solar atmosphere to a single event of excitation of os...
Aims. Our aim is to investigate the role of acoustic and magneto-acoustic waves in heating the solar...
Abstract. The dynamical behavior of upper cool-star photospheres constitutes the next step in realis...
Abstract. In a recent paper (Straus et al. 2008) we determined the energy flux of internal gravity w...
Context. The exact nature of the quiet solar chromosphere and especially its temporal variation, ar...
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
This review focuses on acoustic oscillations n the solar at- mosphere.There s much debate on photos...
Aims.This paper aims to look at the propagation of synthetic photospheric oscillations from a point ...
Abstract. We analyze oscillations in the solar atmosphere using image sequences from the Transition ...
The solar chromosphere has never been static although it was often modeled so.Even the quiet-sun in...
Abstract The direct propagation of acoustic waves, driven harmonically at the solar photo-sphere, in...
The leakage and coupling of solar global oscillations to the overlaying magnetized solar atmosphere ...
The shock dissipation hypothesis for solar atmospheric heating is extended to stellar chromospheres ...
Both the interior and the atmosphere of the Sun give a wide range of oscillations and waves. Interac...
We have studied the nonlinear response of the solar atmosphere to a single event of excitation of os...
Aims. Our aim is to investigate the role of acoustic and magneto-acoustic waves in heating the solar...
Abstract. The dynamical behavior of upper cool-star photospheres constitutes the next step in realis...
Abstract. In a recent paper (Straus et al. 2008) we determined the energy flux of internal gravity w...
Context. The exact nature of the quiet solar chromosphere and especially its temporal variation, ar...
Global helioseismic oscillation modes are a window to the solar interior. They are acoustic waves tr...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...