Louise K. Harra

TL;DR: The Hinode satellite as discussed by the authors is the successor to the Yohkoh mission, which aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases.

TL;DR: The EUV Imaging Spectrometer (EIS) as mentioned in this paper is a two-element, normal incidence design with a backside-illuminated, thinned CCD, which has a significantly greater effective area than previous orbiting EUV spectrographs with typical active region 2 -5 s exposure times in the brightest lines.

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 investigate the properties of two "classical" EUV Imaging Telescope (EIT) coronal waves and observe deep core dimmings near the flare site and also widespread diffuse dimming, accompanying the expansion of the EIT wave, and propose a new mechanism where driven magnetic reconnections between the skirt of the expanding CME magnetic field and quiet-Sun magnetic loops generate the observed bright diffuse front.

TL;DR: A list of emission lines recommended to be included in EIS observation studies is presented in this article based on analysis of blending and diagnostic potential using the CHIANTI atomic database, identifying the most useful density diagnostics from the ions covered by EIS.