EUVI: the STEREO-SECCHI extreme ultraviolet imager

By J. Wuelser, J. Lemen, T. Tarbell, C. J. Wolfson, Joseph C. Cannon, B. A. Carpenter, D. Duncan, Glenn S. Gradwohl, S. Meyer, A. Moore and 24 more. SPIE Optics + Photonics, 2004

492 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Electrical and Electronic Engineering

View Paper: https://www.semanticscholar.org/paper/84346e5da7952fc08d1ecd3240424c1a6870c139

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In Aerospace Engineering

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Citations in the corpus

COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “It includes among others the Extreme Ultraviolet Imager (EUVI; Wuelser et al. 2004) and the white-light inner coronagraph COR1 (Thompson et al. 2003).”
DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE (2012, background): “…(AIA; Lemen et al. 2012) aboard the Solar Dynamics Observatory (SDO) since 2010 and the multiviewpoint observations from the EUV Imager (EUVI; Wuelser et al. 2004) in the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI; Howard et al. 2008) imaging suite aboard the STEREO…”
The Kinematics of a Globally Propagating Disturbance in the Solar Corona (2008, background): “Each image has a pixel scale of 1.6′′ (Wuelser et al. 2004) and the peak sensitivities for each passband are approximately 0.07 MK (304 Å), 1 MK (171 Å), 1.5 MK (195 Å) and 2.25 MK (284 Å).”
STEREO SECCHI Stereoscopic Observations Constraining the Initiation of Polar Coronal Jets (2008, background): “The SECCHI data used here were produced by an international consortium of the Naval Research Laboratory (USA), Lockheed Martin Solar and Astrophysics Lab (USA), NASA Goddard Space Flight Center (USA), Rutherford Appleton Laboratory (UK), University of Birmingham (UK), Max−Planck−Institut for Solar S”
SIMULTANEOUS OBSERVATION OF RECONNECTION INFLOW AND OUTFLOW ASSOCIATED WITH THE 2010 AUGUST 18 SOLAR FLARE (2011, methodology): “The EUV images of this flare were obtained by the Extreme Ultraviolet Imager (EUVI; Howard et al. 2008; Wüelser et al. 2004) on the Solar Terrestrial Relation Observatory spacecraft Ahead (STEREO-A; Kaiser et al. 2008) and the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory…”
NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, methodology): “Following the launch of the Solar Terrestrial Relations Observatory (STEREO; Kaiser et al. 2008), coronal waves are now observed with increased temporal and spatial resolution, and have now been seen from two perspectives using the Extreme Ultra-Violet Imagers (EUVI; Wuelser et al. 2004).”
OBSERVATIONS AND INTERPRETATION OF A LOW CORONAL SHOCK WAVE OBSERVED IN THE EUV BY THE SDO/AIA (2011, background): “′′6 pixel−1 (Wuelser et al. 2004).”
ON A CORONAL BLOWOUT JET: THE FIRST OBSERVATION OF A SIMULTANEOUSLY PRODUCED BUBBLE-LIKE CME AND A JET-LIKE CME IN A SOLAR EVENT (2011, methodology): “The full-disk 195 Å and 304 Å images taken by the Extreme Ultraviolet Imager (EUVI; Wuelser et al. (2004)) of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI; Howard et al. (2008)) on board STEREO Ahead are used in this paper.”
The Large Longitudinal Spread of Solar Energetic Particles During the 17 January 2010 Solar Event (2012, background): “er spiral to the Sun (SUN), and away from the Sun (ANTISUN), respectively. The SECCHI investigation (Howard etal., 2008) provides remote sensing observations of the Sun in extreme ultra violet (EUVI, Wuelser (2004)) as well as coronagraphic observations (COR1 and COR2 instruments), which allow to li”