Abstract The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for
observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can …

Where particle acceleration and plasma heating take place in relation to magnetic
reconnection is a fundamental question for solar flares. We report analysis of an M7. 7 flare …

Recent observations from RHESSI have revealed that the number of non-thermal electrons
in the coronal part of a flaring loop can exceed the number of electrons required to explain …

Aims. We constrain energy release and particle acceleration processes in solar flares by
means of comprehensively characterizing the physical parameters of both the thermal …

ABSTRACT The limb flare SOL2012-07-19T05: 58 (M7. 7) provides the best example of a
non-thermal above-the-loop-top hard X-ray source with simultaneous observations by the …

We report analysis of three solar flares that occur within 1 of limb passage, with the goal to
investigate the source height of chromospheric footpoints in white light (WL) and hard X-rays …

ABSTRACT A statistical study of the correlation between hard X-ray and white light emission
in solar flares is performed in order to search for a link between flare-accelerated electrons …

Understanding electron acceleration associated with magnetic energy release at subsecond
scales presents major challenges in solar physics. Solar radio spikes observed as …

Using observations by the Solar Dynamics Observatory from 2010 June to 2017 December,
we have performed the first statistical investigation of circular-ribbon flares (CFs) and …

Context. Twisted magnetic fields should be ubiquitous in the solar corona, particularly in
flare-producing active regions where the magnetic fields are strongly non-potential. The …