Säm Krucker

TL;DR: In this paper, the authors investigated the solar source region of supra-thermal electron beams observed near Earth by combining in situ measurements of the three-dimensional Plasma and Energetic Particles experiment on the WIND spacecraft with remote-sensing hard X-ray observations by the Reuven Ramaty High Energy Solar Spectroscopic Imager.

TL;DR: In this article, the locations and spectra of solar microflares down to 3 kV were studied using the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) for the first time.

TL;DR: The Energetic Particle Detector (EPD) as discussed by the authors is an instrument suite that is part of the scientific payload aboard the Solar Orbiter mission, which is composed of four units: the SupraThermal Electrons and Protons (STEP), the Electron Proton Telescope (EPT), the Suprathermal Ion Spectrograph (SIS), and the High-Energy Telescope (HET).

TL;DR: In this paper, the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) was used for hard X-ray lightcurves, spectrograms, images, and spectra of three medium-sized flares observed by the RHESSI.

TL;DR: In this article, the authors present Nancay Radioheliograph observations of a moving source of broadband radio emission, commonly referred to as a type IV radio burst (type IVM), which occurred in association with a CME on the 14th of August 2010.