Solar type III radio bursts are an important diagnostic tool in the understanding of solar
accelerated electron beams. They are a signature of propagating beams of nonthermal …

Solar radio emission provides valuable information on the structure and dynamics of the
solar atmosphere above the temperature minimum. We review the background and most …

We report on the 2017 September 10 ground-level enhancement (GLE) event associated
with a coronal mass ejection whose initial acceleration (∼ 9.1 km s− 2) and initial speed (∼ …

Context. Solar observatories are providing the world-wide community with a wealth of data,
covering wide time ranges (eg Solar and Heliospheric Observatory, SOHO), multiple …

We present SDO/AIA observations of an eruptive X-class flare of 2012 July 12, and compare
its evolution with the predictions of a three-dimensional (3D) numerical simulation. We focus …

This paper presents SunPy (version 0.5), a community-developed Python package for solar
physics. Python, a free, cross-platform, general-purpose, high-level programming language …

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 …

The article discusses characteristics, fundamental and applied tasks of the Siberian
Radioheliograph that is developed at the ISTP SB RAS Radio Astrophysical Observatory …

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 …

Abstract Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of
the total flux, are frequently detected in the light curves of solar/stellar flares. In this study, we …