A Stealth CME Bracketed between Slow and Fast Wind Producing Unexpected Geo-effectiveness
Wen He, Ying D.Liu, Huidong Hu, Rui Wang, Xiaowei Zhao

TL;DR
This study examines how a weak CME, influenced by surrounding solar wind structures, unexpectedly caused a significant geomagnetic storm, highlighting the importance of background solar wind conditions in CME geo-effectiveness.
Contribution
It demonstrates the combined effect of slow and fast solar wind streams on the geo-effectiveness of a weak CME using multi-instrument observations and modeling.
Findings
Weak CME produced a strong geomagnetic storm due to solar wind interactions.
CME was bracketed between slow wind and high-speed streams, enhancing its geo-effectiveness.
Solar wind environment significantly influences CME impact on Earth.
Abstract
We investigate how a weak coronal mass ejection (CME) launched on 2016 October 8 without obvious signatures in the low corona produced a relatively intense geomagnetic storm. Remote sensing observations from SDO, STEREO and SOHO and in situ measurements from WIND are employed to track the CME from the Sun to the Earth. Using a graduated cylindrical shell (GCS) model, we estimate the propagation direction and the morphology of the CME near the Sun. CME kinematics are determined from the wide-angle imaging observations of STEREO A and are used to predict the CME arrival time and speed at the Earth. We compare ENLIL MHD simulation results with in situ measurements to illustrate the background solar wind where the CME was propagating. We also apply a Grad--Shafranov technique to reconstruct the flux rope structure from in situ measurements in order to understand the geo-effectiveness…
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