Andrzej Fludra

TL;DR: The Coronal Diagnostic Spectrometer (CDS) as mentioned in this paper was designed to probe the solar atmosphere through the detection of spectral emission lines in the extreme ultraviolet wavelength range 150-800 A. By observing the intensities of selected lines and line profiles, the authors derived temperature, density, flow and abundance information for the plasmas in the solar ionosphere.

TL;DR: The first mission of ESA's Cosmic Vision 2015-2025 programme and a mission of international collaboration between ESA and NASA, was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and heliospheric physics pertaining to how the Sun creates and controls the Heliosphere, and why solar activity changes with time.

TL;DR: In this paper, the authors investigated the morphological and dynamical properties of the Kopp-Pneuman-type coronal mass ejection (CME) and found that the magnetic field strength in the vicinity of the current sheet is of the order of 1 G.

TL;DR: In this paper, the electron densities of the simplest symmetric solar minimum streamer structure observed during the Whole Sun Month (WSM) campaign were derived using coronal observations of both visible white light and extreme ultraviolet (EUV) emission.