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)
First Light! The spectro-polarimeter of the world's largest solar telescope in Hawaii looks at the Sun for the first time. The instrument was developed in Germany.
Dr. Theodosios Chatzistergos receives award by the European Space Weather and Space Climate Association for his research findings on the historical activity of the Sun.
The Zdenĕk Švetska Senior Prize of the Solar Physics Division of the European Physical Society (EPS) recognizes Solanki’s pioneering contributions to solar research.
The magnetic field in the solar atmosphere exceeds the geomagnetic field strength by four orders of magnitude. It greatly influences the processes of energy transport within the solar atmosphere, and dominates the morphology of the solar chromosphere and corona. Kinetic energy from convective motions in the Sun can be efficiently stored in magnetic fields and subsequently released - to heat the solar corona to several million degrees or to blast off coronal mass ejections.
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...