Dear all,
you might be interested in the following paper that has just been
published on Science:
"Evidence of non-thermal particles in coronal loops heated
impulsively by nanoflares"
It can be downloaded from astro-ph: http://arxiv.org/abs/1410.6130
or directly
from the Science pages:
http://www.sciencemag.org/content/346/6207/1255724
The abstract is below.
cheers,
Paola
Abstract:
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 an interface region between the surface and the corona
that is highly sensitive to
the coronal heating mechanism. High-resolution observations with the
Interface Region
Imaging Spectrograph (IRIS) reveal rapid variability (~20 to 60
seconds) of intensity and
velocity on small spatial scales (≲500 kilometers) at the footpoints
of hot and dynamic
coronal loops. The observations are consistent with numerical
simulations of heating by
beams of nonthermal electrons, which are generated in small
impulsive (≲30 seconds)
heating events called “coronal nanoflares.” The accelerated
electrons deposit a sizable
fraction of their energy (≲10^25 erg) in the chromosphere and TR.
Our analysis provides tight
constraints on the properties of such electron beams and new
diagnostics for their
presence in the nonflaring corona.