Cairós, L. M.; González-Pérez, J. N.; Weilbacher, P. M.; Manso Sainz, R.: Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE. The diverse ionization mechanisms acting in low-mass starbursts. Astronomy and Astrophysics 664, p. A144 (2022)
Cairos, L. M.; Gonzalez-Perez, J. N.; Weilbacher, P. M.; Manso Sainz, R.: MUSE observations of the blue compact dwarf galaxy Haro 14: Data analysis and first results on morphology and stellar populations. Astronomy and Astrophysics 654, A142 (2021)
del Pino Alemán, T.; Trujillo Bueno, J.; Casini, R.; Manso Sainz, R.: The Magnetic Sensitivity of the Resonance and Subordinate Lines of Mg II in the Solar Chromosphere. The Astrophysical Journal 891 (1), 91 (2020)
Manso Sainz, R.; Alemán, T. d. P.; Casini, R.; McIntosh, S.: Spectropolarimetry of the Solar Mg II h and k Lines. Astrophysical Journal, Letters 883 (2), L30 (2019)
Casini, R.; Aleman, T. d. P.; Manso Sainz, R.: Explicit Form of the Radiative and Collisional Branching Ratios in Polarized Radiation Transport with Coherent Scattering. Astrophysical Journal 848 (2), 99 (2017)
Casini, R.; del Pino Alemán, T.; Manso Sainz, R.: A Note on the Radiative and Collisional Branching Ratios in Polarized Radiation Transport with Coherent Scattering. Astrophysical Journal 835, 114 (2017)
Casini, R.; Manso Sainz, R.; Pino Alemán, T. d.: Rayleigh Scattering in Spectral Series with L-term Interference. The Astrophysical Journal 850 (2), 162 (2017)
Casini, R.; Manso Sainz, R.: Frequency Redistribution of Polarized Light in the Λ-Type Multi-Term Polarized Atom. Astrophysical Journal 824, 135 (2016)
Casini, R.; Manso Sainz, R.: Laboratory Frequency Redistribution Function for the Polarized Λ -type Three-term Atom. Astrophysical Journal 833 (2), 197 (2016)
del Pino Alemán T. andCasini, R.; Manso Sainz, R.: Magnetic Diagnostics of the Solar Chromosphere with the Mg II h-k Lines. Astrophysical Journal 830, L24 (2016)
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.