The Sun is a magnetic star, not as magnetic as some stars, or as it was when itwas younger, but nonetheless magnetic fields dominate and even construct...
Theoretical Modeling of Propagation of Magnetoacoustic Waves in Magnetic Regions Below Sunspots
We use two-dimensional numerical simulations and eikonal approximation to study properties of magnetohydrodynamic (MHD) waves traveling below the solar surface...
Tracing p-mode Waves from the Photosphere to the Corona in Active Regions
Atmosphere above sunspots is abundant with different types of waves. Among these waves are running penumbral waves in the chromosphere, quasi-periodic...
Tracing the ``Acoustic'' Solar Cycle: A Direct Comparison of BiSON and GOLF Low-l p-Mode Variations
We present a detailed, comparative study of low angular degree solar p-mode variations extracted by analyses of two sets of observational data. These were...
Una estrella masiva pulsante facilita claves para calibrar los modelos de evolución estelar
Una colaboración internacional, en la que participa el Instituto de Astrofísica de Canarias (IAC), consigue determinar con un nivel de precisión sin precedentes...
Since the beginning of this century we have attended a blooming of the gravity-mode research thanks to the unprecedented quality of the data available, either...
VIRGO: Experiment for Helioseismology and Solar Irradiance Monitoring
The scientific objective of the VIRGO experiment (Variability of solar IRradiance and Gravity Oscillations) is to determine the characteristics of pressure and...
The VIRGO Experiment (Variability of solar IRradiance and Gravity Oscillations) contains two types of active cavity radiometers for monitoring of the solar...