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Estimation of a coronal mass ejection magnetic field strength using radio observations of gyrosynchrotron radiation
DOI: 10.1051/0004-6361/201731368 Bibcode: 2017A&A...608A.137C

Carley, Eoin P.; Vilmer, Nicole; Simões, Paulo J. A. +1 more

Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the low solar corona into interplanetary space. These eruptions are often associated with the acceleration of energetic electrons which produce various sources of high intensity plasma emission. In relatively rare cases, the energetic electrons may also produce gyr…

2017 Astronomy and Astrophysics
PROBA-2 60
Segmentation of photospheric magnetic elements corresponding to coronal features to understand the EUV and UV irradiance variability
DOI: 10.1051/0004-6361/201629924 Bibcode: 2017A&A...605A..41Z

Giono, G.; Zender, J. J.; Kariyappa, R. +5 more

Context. The magnetic field plays a dominant role in the solar irradiance variability. Determining the contribution of various magnetic features to this variability is important in the context of heliospheric studies and Sun-Earth connection.
Aims: We studied the solar irradiance variability and its association with the underlying magnetic fi…

2017 Astronomy and Astrophysics
PROBA-2 10