Articles | Volume 34, issue 2
https://doi.org/10.5194/angeo-34-313-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/angeo-34-313-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Regular paper
| 
29 Feb 2016
Regular paper |
| 29 Feb 2016
Planar magnetic structures in coronal mass ejection-driven sheath regions
Erika Palmerio
CORRESPONDING AUTHOR
University of Helsinki, Department of Physics, P.O. Box 64, 00014 Helsinki, Finland
Emilia K. J. Kilpua
University of Helsinki, Department of Physics, P.O. Box 64, 00014 Helsinki, Finland
Neel P. Savani
Goddard Planetary Heliophysics Institute (GPHI), University of Maryland, Baltimore County, Maryland, USA
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
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Cited
44 citations as recorded by crossref.
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- Outer radiation belt and inner magnetospheric response to sheath regions of coronal mass ejections: a statistical analysis M. Kalliokoski et al. 10.5194/angeo-38-683-2020
- Geoeffectiveness of interplanetary shocks controlled by impact angles: A review D. Oliveira & A. Samsonov 10.1016/j.asr.2017.10.006
- Coexistence of a planar magnetic structure and an Alfvén wave in the shock-sheath of an interplanetary coronal mass ejection Z. Shaikh et al. 10.1093/mnras/stz2743
- The Effect of Stream Interaction Regions on ICME Structures Observed in Longitudinal Conjunction R. Winslow et al. 10.3847/1538-4357/ac0439
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- Thermospheric nitric oxide response to shock‐led storms D. Knipp et al. 10.1002/2016SW001567
- Coronal mass ejections and their sheath regions in interplanetary space E. Kilpua et al. 10.1007/s41116-017-0009-6
- Small-scale flux ropes in ICME sheaths J. Ruohotie et al. 10.3389/fspas.2022.943247
- Multi-Spacecraft Observations of an Interplanetary Coronal Mass Ejection Interacting with Two Solar-Wind Regimes Observed by the Ulysses and Twin-STEREO Spacecraft M. Maunder et al. 10.1007/s11207-022-02077-3
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- Spatial Coherence of Interplanetary Coronal Mass Ejection Sheaths at 1 AU M. Ala‐Lahti et al. 10.1029/2020JA028002
- The Compression of the Heliospheric Magnetic Structure by Interplanetary Shocks: Is the Structure at 1AU a Manifestation of Solar-Wind Turbulence or Is It Fossil Structure From the Sun? J. Borovsky 10.3389/fspas.2020.582564
- Anisotropic Heating and Cooling within Interplanetary Coronal Mass Ejection Sheath Plasma Z. Shaikh et al. 10.3847/1538-4357/ad782b
- Evolution of planar magnetic structure within the stream interaction region and its connection with a recurrent Forbush decrease Z. Shaikh et al. 10.1093/mnras/staa1039
- Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind E. Kilpua et al. 10.5194/angeo-38-999-2020
- Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection M. Ala-Lahti et al. 10.5194/angeo-36-793-2018
- The pancaking of coronal mass ejections: an in situ attestation A. Raghav & Z. Shaikh 10.1093/mnrasl/slz187
- Outer Radiation Belt Flux and Phase Space Density Response to Sheath Regions: Van Allen Probes and GPS Observations M. Kalliokoski et al. 10.1029/2022JA030708
- Alfvén Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections M. Ala‐Lahti et al. 10.1029/2019JA026579
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- Observation of a Fully-formed Forward–Reverse Shock Pair due to the Interaction between Two Coronal Mass Ejections at 0.5 au D. Trotta et al. 10.3847/2041-8213/ad68fa
- Radial Evolution of Magnetic Field Fluctuations in an Interplanetary Coronal Mass Ejection Sheath S. Good et al. 10.3847/1538-4357/ab7fa2
- Evolution of Earth’s magnetosheath as a planar magnetic structure Z. Shaikh & A. Raghav 10.1093/mnras/stac276
- Earth’s magnetosphere and outer radiation belt under sub-Alfvénic solar wind N. Lugaz et al. 10.1038/ncomms13001
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Latest update: 24 Apr 2025
Short summary
Coronal Mass Ejections (CMEs) are giant clouds of plasma and magnetic field that erupt from the Sun and travel though the solar wind. They can cause interplanetary shocks in the vicinity of Earth. We show in our paper that the region that follows CME-driven shocks, known as sheath region, can obtain a planar configuration of the magnetic field lines (planar magnetic structure, PMS) due to the compression resulting from the shock itself or from the draping of the magnetic field ahead of the CME.
Coronal Mass Ejections (CMEs) are giant clouds of plasma and magnetic field that erupt from the...
