A model for stealth coronal mass ejections
B. J. Lynch, S. Masson, Y. Li, C. R. DeVore, J. G. Luhmann, S. K., Antiochos, and G. H. Fisher

TL;DR
This paper models a stealth coronal mass ejection using 3D MHD simulations, revealing how slow streamer blowouts can occur without observable low-corona signatures, aligning well with multi-viewpoint coronagraph observations.
Contribution
It introduces a novel 3D MHD simulation approach to explain the formation and evolution of stealth CMEs, matching observational data.
Findings
Simulation reproduces stealth CME features observed by SOHO and STEREO.
Slow streamer blowout results from shearing flows and magnetic reconnection.
Model provides insights into the initiation mechanism of stealth CMEs.
Abstract
Stealth coronal mass ejections (CMEs) are events in which there are almost no observable signatures of the CME eruption in the low corona but often a well-resolved slow flux rope CME observed in the coronagraph data. We present results from a three-dimensional numerical magnetohydrodynamics (MHD) simulation of the 1--2 June 2008 slow streamer blowout CME that Robbrecht et al. (2009) called "the CME from nowhere." We model the global coronal structure using a 1.4 MK isothermal solar wind and a low-order potential field source surface representation of the Carrington Rotation 2070 magnetogram synoptic map. The bipolar streamer belt arcade is energized by simple shearing flows applied in the vicinity of the helmet streamer's polarity inversion line. The flows are large scale and impart a shear typical of that expected from the differential rotation. The slow expansion of the energized…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Monetary Policy and Economic Impact
