F. Portier-Fozzani

TL;DR: The Extreme Ultraviolet Imaging Telescope (EIT) on board the SOHO spacecraft has been operational since 2 January 1996 and has been used to observe the Sun over a 45 × 45 arc min field of view in four emission line groups: Fe IX, X, Fe XIIi, Fe xv, and He II.

TL;DR: In this paper, a new method of dynamic stereoscopy is developed to reconstruct the three-dimensional geometry of dynamically changing loops, which allows us to determine the orientation of the mean loop plane with respect to the line of sight, a prerequisite to correct properly for projection effects in 3D loop models.

TL;DR: In this paper, the authors examined two relatively cool features as recorded in EIT's Fe ix/x (171 A) and Fe xii (195 A) bands in a decaying active region and found that downward thermal conductive losses (at heights above the transition region) are inadequate to support local radiative losses.

TL;DR: In this article, the EIT (Extreme ultraviolet Imaging Telescope) images the Sun's corona in 4 EUV wavelengths, including the chromosphere and the base of the transition region at a temperature of 5 − 8 × 104 K.

TL;DR: In this paper, the 3D geometry of dynamic changing loops is reconstructed using dynamic stereoscopy to determine the orientation of the loop plane with respect to the line-of-sight.