Add to ORKGLong-period acoustic waves generated in the solar convection zone can propagate radially outward through the overlying atmosphere and get resonantly absorbed in the magnetic arches of the low-lying chromospheric canopy. The resulting Poynting and acoustic flux that enters the magnetic canopy in the network regions is demonstrated to be adequate to account for the observed chromospheric emission
Observations show the increase of high-frequency wave power near magnetic network cores and active r...
The direct propagation of acoustic waves, driven harmonically at the solar photosphere, into the thr...
Context. We present evidence for the conversion and transmission of wave modes on the magn...
Long-period acoustic waves generated in the solar convection zone can propagate radially outward thr...
Acoustic and magnetoacoustic waves play an important role in the chromospheric heating, exhibiting t...
Aims. Our aim is to investigate the role of acoustic and magneto-acoustic waves in heating the solar...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Abstract. Several mechanisms may heat the solar chromosphere: acoustic waves, magne-toacoustic waves...
Several mechanisms may heat the solar chromosphere: acoustic waves, magnetoacoustic waves (slow, fas...
Aims. To study the heating of solar chromospheric magnetic and nonmagnetic regions by acoustic and m...
We perform numerical simulations of magnetoacoustic waves (MAWs) in the solar atmosphere, which is g...
Acoustic and magnetoacoustic waves are considered to be possible agents of chromospheric heating. We...
AbstractIn this paper, upward propagating Magnetoacoustic waves in an ideal atmosphere are considere...
Aims. We study the properties of slow magneto-acoustic waves that are naturally excited as a result ...
Observations show the increase of high-frequency wave power near magnetic network cores and active r...
The direct propagation of acoustic waves, driven harmonically at the solar photosphere, into the thr...
Context. We present evidence for the conversion and transmission of wave modes on the magn...
Long-period acoustic waves generated in the solar convection zone can propagate radially outward thr...
Acoustic and magnetoacoustic waves play an important role in the chromospheric heating, exhibiting t...
Aims. Our aim is to investigate the role of acoustic and magneto-acoustic waves in heating the solar...
Acoustic and magnetoacoustic waves are among the possible candidate mechanisms that heat the upper l...
We show that inclined magnetic field lines at the boundaries of large-scale convective cells (superg...
Abstract. Several mechanisms may heat the solar chromosphere: acoustic waves, magne-toacoustic waves...
Several mechanisms may heat the solar chromosphere: acoustic waves, magnetoacoustic waves (slow, fas...
Aims. To study the heating of solar chromospheric magnetic and nonmagnetic regions by acoustic and m...
We perform numerical simulations of magnetoacoustic waves (MAWs) in the solar atmosphere, which is g...
Acoustic and magnetoacoustic waves are considered to be possible agents of chromospheric heating. We...
AbstractIn this paper, upward propagating Magnetoacoustic waves in an ideal atmosphere are considere...
Aims. We study the properties of slow magneto-acoustic waves that are naturally excited as a result ...
Observations show the increase of high-frequency wave power near magnetic network cores and active r...
The direct propagation of acoustic waves, driven harmonically at the solar photosphere, into the thr...
Context. We present evidence for the conversion and transmission of wave modes on the magn...