26 citations · 145 across the 9 of their papers we have counts for
9 papers
A CHEOPS-enhanced view of the HD3167 system
V. Bourrier, A. Deline, A. Krenn +92
Much remains to be understood about the nature of exoplanets smaller than Neptune, most of which have been discovered in compact multi-planet systems. With its inner ultra-short pe…
Synchronization of Small-scale Magnetic Features, Blinkers, and Coronal Bright Points
Zahra Shokri, Nasibe Alipour, Hossein Safari +4
We investigate the relationship between different transients such as blinkers detected in images taken at 304~Å, extreme ultraviolet coronal bright points (ECBPs) at 193~Å, X-ray c…
A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude
Louise Harra, Vincenzo Andretta, Thierry Appourchaux +29
A mission to view the solar poles from high helio-latitudes (above 60) will build on the experience of Solar Orbiter as well as a long heritage of successful solar missions…
Sign singularity of the local energy transfer in space plasma turbulence
Luca Sorriso-Valvo, Gaetano De Vita, Federico Fraternale +18
In weakly collisional space plasmas, the turbulent cascade provides most of the energy that is dissipated at small scales by various kinetic processes. Understanding the characteri…
A fast algorithm for a three-dimensional synthetic model of intermittent turbulence
Francesco Malara, Francesca Di Mare, Giuseppina Nigro +1
Synthetic turbulence models are a useful tool that provide realistic representations of turbulence, necessary to test theoretical results, to serve as background fields in some num…
Heating Mechanisms for Intermittent Loops in Active Region Cores from AIA/SDO EUV Observations
A. C. Cadavid, J. K. Lawrence, D. J. Christian +2
We investigate intensity variations and energy deposition in five coronal loops in active region cores. These were selected for their strong variability in the AIA/SDO 94 Å intensi…
Study on the large scale dynamo transition
Giuseppina Nigro, Pierlugi Veltri
Using the magnetohydrodynamic (MHD) description, we develop a nonlinear dynamo model that couples the evolution of the large scale magnetic field with turbulent dynamics of the pla…
The chromosphere: gateway to the corona, or the purgatory of solar physics?
Philip G. Judge
I argue that one should attempt to understand the solar chromosphere not only for its own sake, but also if one is interested in the physics of: the corona; astrophysical dynamos;…
Modeling a coronal loop heated by MHD-turbulence nanoflares
F. Reale, G. Nigro, F. Malara +2
We model the hydrodynamic evolution of the plasma confined in a coronal loop, 30000 km long, subject to the heating of nanoflares due to intermittent magnetic dissipative events in…