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The solar corona—the outermost layer of the Sun’s atmosphere—is extremely hot and very low in density. One of the main challenges in solar physics is understanding why the corona reaches temperatures of over a million degrees. This heating is believed to be closely related to the Sun’s magnetic field. However, quantifying the coronal magnetic field is difficult because the light emitted by the corona is extremely faint, and its polarization signals, which encode the information on the magnetic field, are subtle. Thanks to recent advances in technology, telescopes like the Daniel K. InouyeAdvertised on -
Del 10 al 13 de junio, las principales instalaciones astronómicas de España se dan cita en Granada para compartir conocimientos, tecnologías y estrategias de colaboración. Bajo el lema “Promoviendo sinergias entre grandes observatorios españoles”, este encuentro reúne a cerca de un centenar de expertos en tecnología, ingeniería y gestión que trabajan en las Infraestructuras Científicas y Técnicas Singulares (ICTS) en astronomía del país. El objetivo de esta segunda edición es consolidar los vínculos creados en la primera reunión, celebrada en La Palma en 2023, y seguir avanzando enAdvertised on -
The Canary Islands Institute of Astrophysics reinforces its commitment to scientific and cultural dissemination by participating in the literary event held in La Palma from September 22 to 27 The Instituto de Astrofísica de Canarias (IAC) renews its collaboration with the Spanish-American Writers’ Festival, which celebrates its seventh edition this year from September 22 to 27 in Los Llanos de Aridane, on the island of La Palma. This participation is part of the IAC's ongoing commitment to scientific and cultural outreach, connecting the world of astrophysics with literature and humanisticAdvertised on