64 citations · 171 across the 7 of their papers we have counts for
7 papers
Association of radio polar cap brightening with bright patches and coronal holes
Caius L. Selhorst, Paulo J. A. Simoes, Alexandre J. Oliveira e Silva +3
Radio-bright regions near the solar poles are frequently observed in Nobeyama Radioheliograph (NoRH) maps at 17 GHz, and often in association with coronal holes. However, the origi…
H and H emission in a C3.3 solar flare: comparison between observations and simulations
Vincenzo Capparelli, Francesca Zuccarello, Paolo Romano +7
The Hydrogen Balmer series is a basic radiative loss channel from the flaring solar chromosphere. We report here on the analysis of an extremely rare set of simultaneous observatio…
Estimation of a Coronal Mass Ejection Magnetic Field Strength using Radio Observations of Gyrosynchrotron Radiation
Eoin P. Carley, Nicole Vilmer, Paulo J. A. Simões +1
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 ac…
Observations of Reconnection Flows in a Flare on the Solar Disk
Juntao Wang, P. J. A. Simoes, N. L. S. Jeffrey +3
Magnetic reconnection is a well-accepted part of the theory of solar eruptive events, though the evidence is still circumstantial. Intrinsic to the reconnection picture of a solar…
Formation of the thermal infrared continuum in solar flares
Paulo J. A. Simões, Graham S. Kerr, Lyndsay Fletcher +3
Observations of the Sun with the Atacama Large Millimeter Array have now started, and the thermal infrared will regularly be accessible from the NSF's Daniel K. Inouye Solar Telesc…
Analysis of intermittency in submillimeter radio and hard X-Rays during the impulsive phase of a solar flare
C. Guillermo Giménez de Castro, Paulo J. A. Simões, Jean-Pierre Raulin +1
We present an analysis of intermittent processes occurred during the impulsive phase of the flare SOL2012-03-13, using hard X-rays and submillimeter radio data. Intermittency is a…