Why are ELEvoHI CME arrival predictions different if based on STEREO-A or STEREO-B heliospheric imager observations?
J\"urgen Hinterreiter, Tanja Amerstorfer, Martin A. Reiss, Christian, M\"ostl, Manuela Temmer, Maike Bauer, Ute V. Amerstorfer, Rachel L. Bailey,, Andreas J. Weiss, Jackie A. Davies, Luke A. Barnard, Mathew J. Owens

TL;DR
This study compares CME arrival time and speed predictions based on STEREO-A and STEREO-B observations using ELEvoHI, revealing differences influenced by ambient solar wind conditions and highlighting the challenges in space weather forecasting.
Contribution
It provides a systematic comparison of CME predictions from two vantage points, quantifies prediction discrepancies, and assesses the influence of solar wind variability on forecast accuracy.
Findings
Mean arrival time difference of 6.5 hours between viewpoints
Prediction errors of approximately 7.5 hours in arrival time
No significant accuracy advantage of one spacecraft over the other
Abstract
Accurate forecasting of the arrival time and arrival speed of coronal mass ejections (CMEs) is a unsolved problem in space weather research. In this study, a comparison of the predicted arrival times and speeds for each CME based, independently, on the inputs from the two STEREO vantage points is carried out. We perform hindcasts using ELlipse Evolution model based on Heliospheric Imager observations (ELEvoHI) ensemble modelling. An estimate of the ambient solar wind conditions is obtained by the Wang-Sheeley-Arge/Heliospheric Upwind eXtrapolation (WSA/HUX) model combination that serves as input to ELEvoHI. We carefully select 12 CMEs between February 2010 and July 2012 that show clear signatures in both STEREO-A and STEREO-B HI time-elongation maps, that propagate close to the ecliptic plane, and that have corresponding in situ signatures at Earth. We find a mean arrival time…
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