High-resolution white light and H-alpha observations are used to study the development of 15 large active solar regions. The behavior of the magnetic fragments...
Frequency shift of solar p-modes as seen by cross correlation analysis
Data obtained at the Observatorio del Teide (Tenerife) during the years 1978 to 1988 using a resonant scattering spectrophotometer, is analyzed to look for...
The principal objectives of this project are: 1) to study the structure and dynamics of the solar interior, 2) to extend this study to other stars (either...
Instability and eruption of magnetic flux tubes in the solar convection zone
We present a consistent model of storage, instability and dynamical eruption of magnetic flux tubes in the solar convection zone and underlying overshoot region...
Long-term Spatial and Temporal Variations of Aurora Borealis Events in the Period 1700 - 1905
Catalogues and other records of aurora-borealis events were used to study the long-term spatial and temporal variation of these phenomena in the period from...
Long-Term Trends and Gleissberg Cycles in Aurora Borealis Records (1600 - 2015)
The long-term spatial and temporal variation of aurora borealis events from 1600 to the present were studied using catalogues and other records of these...
Long-term Variation of Solar Activity by a Dynamo Based on Magnetic Flux Tubes
We show that cyclic activity and Maunder-type grand minima can be explained by a dynamo driven by the instability of magnetic flux tubes in the overshoot layer...
We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, which are structures though to trace intense kG magnetic...
Modeling of integrated sunlight velocity measurements: The effect of surface darkening by magnetic fields
It has been known since the work by Claverie et al. (1982) that integrated-sunlight velocities measured with the resonance scattering technique show variations...