203 citations · 299 across the 5 of their papers we have counts for
9 papers
Plasma sloshing in pulse-heated solar and stellar coronal loops
F. Reale
There is evidence that coronal heating is highly intermittent, and flares are the high energy extreme. The properties of the heat pulses are difficult to constrain. Here hydrodynam…
Evidence of Non-Thermal Particles in Coronal Loops Heated Impulsively by Nanoflares
Paola Testa, Bart De Pontieu, Joel Allred +21
The physical processes causing energy exchange between the Sun's hot corona and its cool lower atmosphere remain poorly understood. The chromosphere and transition region (TR) form…
Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity
S. Orlando, F. Reale, G. Peres +1
According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion bui…
Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant
M. Miceli, S. Orlando, F. Reale +2
Many supernova remnants (SNRs) are characterized by a knotty ejecta structure. The Vela SNR is an excellent example of remnant in which detached clumps of ejecta are visible as X-r…
The role of radiative losses in the late evolution of pulse-heated coronal loops/strands
F. Reale, E. Landi
Radiative losses from optically thin plasma are an important ingredient for modeling plasma confined in the solar corona. Spectral models are continuously updated to include the em…
Sphinx measurements of the 2009 solar minimum x-ray emission
J. Sylwester, M. Kowalinski, S. Gburek +9
The SphinX X-ray spectrophotometer on the CORONAS-PHOTON spacecraft measured soft X-ray emission in the 1-15 keV energy range during the deep solar minimum of 2009 with a sensitivi…