Charla
The coronal heating problem: why MHD waves are trendy
The coronal heating problem has been with us for almost 70 years now. Among the different proposed explanations, wave-based heating mechanisms are recurrently...
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CharlaThe ESA/NASA mission Solar OrbiterSolar Orbiter is the first mission of the ESA Cosmic Vision program and that has recently been approved at implementation level. It is an M class mission with a...
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CharlaThe Magnetic Nature of Our SunThis talk will give an overview of our understanding of the Sun in the 1960's, the major discoveries since then, and the main questions that need to be answered...
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CharlaThe Solar ChromosphereThe chromosphere is the interface between the photospheric solar surface and the outer corona and wind. In this complex domain thesolar gas becomes transparent...
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CharlaThe wounded SunThe 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...
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PublicaciónTomographic Reconstruction of the Solar K-Corona Using Neural FieldsWe explore the application of neural fields for tomographic reconstructions of the solar corona using data from the Large Angle and Spectrometric Coronagraph...
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CharlaTurbulence and Particle Acceleration in Solar FlaresA solar flare involves the conversion of magnetic energy stored in the coronal magnetic field into the kinetic energy of thermal and non-thermal particles, mass...