A synoptic view of solar transient evolution in the inner heliosphere using the Heliospheric Imagers on STEREO

By J. Davies, R. Harrison, A. Rouillard, N. Sheeley, C. Perry, D. Bewsher, C. Davis, C. Eyles, S. Crothers, D. Brown. 2009

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Coronal Mass Ejections: Observations (2012, methodology): “In October 2006, the twin STEREO spacecraft were launched carrying the Heliospheric Imagers (HIs) (Howard et al., 2008a; Eyles et al., 2009).”
THE DEFLECTION OF THE TWO INTERACTING CORONAL MASS EJECTIONS OF 2010 MAY 23–24 AS REVEALED BY COMBINED IN SITU MEASUREMENTS AND HELIOSPHERIC IMAGING (2012, methodology): “J-maps are time-elongation maps created following the procedure explained in Sheeley et al. (1999) and Davies et al. (2009).”
GEOMETRIC TRIANGULATION OF IMAGING OBSERVATIONS TO TRACK CORONAL MASS EJECTIONS CONTINUOUSLY OUT TO 1 AU (2010, methodology): “…geometric triangulation for HI1 and HI2 data, relaxes various assumptions needed in a model fit (e.g., Sheeley et al. 1999, 2008; Rouillard et al. 2008; Davies et al. 2009), and can accurately determine CME kinematics (both propagation direction and radial distance) continuously in the heliosphere.”
ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, methodology): “Figure 2 displays two synoptic views of the CME (left) from STEREO A and B and the time-elongation maps (right) produced by stacking the running-difference images within a slit along the ecliptic (e.g., Sheeley et al. 2008; Davies et al. 2009; Liu et al. 2010a).”