Solar coronal loop oscillations: theory of resonantly damped oscillations and comparison with observations
One of the proposed damping mechanisms of coronal transverse loop oscillations in the kink mode is resonant absorption as a result of the spatial variation of...
Data obtained at Izaña (Tenerife) and Haleakala (Maui), using optical resonant scattering with a potassium vapour cell over the years 1980 - 84, are used to...
Solar cycle variations of oscillation mode parameters from LOWL and MARK-I instruments
The signature of the Solar-Cycle appears clearly in the p-mode parameters (Jiménez-Reyes et al. 1998, Libbrecht & Woodard 1990, and Anguera et al. 1992). At...
The prime objectives of the workshop were to: inform the community about the science opportunities of the Solar Orbiter mission; to provide a forum for...
A statistical analysis of the frequency spectrum of 85 days of data obtained from integral solar velocity signals, has shown that significant signals exist in...
Gravity modes are the best probes to study the solar radiative zone, in particular the nuclear core and to follow its potential variability with time and...