Planar magnetic structures in coronal mass ejection-driven sheath regions

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http://hdl.handle.net/10138/161486

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Palmerio , E , Kilpua , E K J & Savani , N P 2016 , ' Planar magnetic structures in coronal mass ejection-driven sheath regions ' Annales Geophysicae , vol. 34 , no. 2 , pp. 313-322 . DOI: 10.5194/angeo-34-313-2016

Title: Planar magnetic structures in coronal mass ejection-driven sheath regions
Author: Palmerio, Erika; Kilpua, Emilia K. J.; Savani, Neel P.
Contributor: University of Helsinki, Particle Physics and Astrophysics
University of Helsinki, Particle Physics and Astrophysics
Date: 2016
Language: eng
Number of pages: 10
Belongs to series: Annales Geophysicae
ISSN: 0992-7689
URI: http://hdl.handle.net/10138/161486
Abstract: Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic field vectors are nearly parallel to a single plane. One of the specific regions where PMSs have been reported are coronal mass ejection (CME)-driven sheaths. We use here an automated method to identify PMSs in 95 CME sheath regions observed in situ by the Wind and ACE spacecraft between 1997 and 2015. The occurrence and location of the PMSs are related to various shock, sheath, and CME properties. We find that PMSs are ubiquitous in CME sheaths; 85% of the studied sheath regions had PMSs with the mean duration of 6 h. In about one-third of the cases the magnetic field vectors followed a single PMS plane that covered a significant part (at least 67%) of the sheath region. Our analysis gives strong support for two suggested PMS formation mechanisms: the amplification and alignment of solar wind discontinuities near the CME-driven shock and the draping of the magnetic field lines around the CME ejecta. For example, we found that the shock and PMS plane normals generally coincided for the events where the PMSs occurred near the shock (68% of the PMS plane normals near the shock were separated by less than 20 degrees from the shock normal), while deviations were clearly larger when PMSs occurred close to the ejecta leading edge. In addition, PMSs near the shock were generally associated with lower upstream plasma beta than the cases where PMSs occurred near the leading edge of the CME. We also demonstrate that the planar parts of the sheath contain a higher amount of strong southward magnetic field than the non-planar parts, suggesting that planar sheaths are more likely to drive magnetospheric activity.
Subject: Interplanetary physics
interplanetary shocks
solar wind plasma
solar physics astrophysics and astronomy
flares and mass ejections
SOLAR-WIND
INTERPLANETARY SHOCKS
FIELDS
EARTH
EVOLUTION
MAXIMUM
CLOUDS
STORMS
115 Astronomy, Space science
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