Solar jets are observed as collimated plasma beams over a large range of temperatures and
wavelengths. They have been observed in H α and optical lines for more than 50 years and …

Previous studies have revealed that solar coronal jets triggered by the eruption of
minifilaments (MFs) conform to the famous magnetic-breakout mechanism. In such a …

Context. One of the main science questions of the Solar Orbiter and Parker Solar Probe
missions deals with understanding how electrons in the lower solar corona are accelerated …

Context. We study the solar energetic particle (SEP) event observed on 9 October 2021 by
multiple spacecraft, including Solar Orbiter. The event was associated with an M1. 6 flare, a …

Context. The Spectrometer/Telescope for Imaging X-rays (STIX) is the hard X-ray instrument
onboard Solar Orbiter designed to observe solar flares over a broad range of flare sizes …

We investigate the hard X-ray (HXR) flare-associated" prompt" solar energetic electron
(SEE) 2013 November 12 event with joint EUV jet observations from Solar Dynamics …

Magnetic reconnection is widely accepted to be a major contributor to nonthermal particle
acceleration in the solar atmosphere. In this paper we investigate particle acceleration …

A series of solar energetic electron (SEE) events was observed from 2022 November 9 to
November 15 by Solar Orbiter, STEREO-A, and near-Earth spacecraft. At least 32 SEE …

A series of 3He-rich solar energetic particle (SEP) events was observed by Solar Orbiter in
May 2021 at a radial distance of 0.95 AU. An isolated active region AR 12824 was likely the …

Solar flare electron acceleration is an efficient process, but its properties (mechanism,
location) are not well constrained. Via hard X-ray (HXR) emission, we routinely observe …