Quantifying the Uncertainty in CME Kinematics Derived From Geometric Modeling of Heliospheric Imager Data

Quantifying the Uncertainty in CME Kinematics Derived From Geometric Modeling of Heliospheric Imager Data

Abstract Geometric modeling of Coronal Mass Ejections (CMEs) is a widely used tool for assessing their kinematic evolution. Furthermore, techniques based on geometric modeling, such as ELEvoHI, are being developed into forecast tools for space weather prediction. These models assume that solar wind...

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Bibliographic Details
Main Authors: L. Barnard, M. J. Owens, C. J. Scott, M. Lockwood, C. A. deKoning, T. Amerstorfer, J. Hinterreiter, C. Möstl, J. A. Davies, P. Riley
Format: Article
Language:English
Published: Wiley 2022-01-01
Series:Space Weather
Subjects:
coronal mass ejections
geometric modeling
forecasting
ELEvoHI
HUXt
uncertainty
Online Access:https://doi.org/10.1029/2021SW002841
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