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Self‐similarity of ICME flux ropes: Observations by radially aligned spacecraft in the inner Heliosphere

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Title: Self‐similarity of ICME flux ropes: Observations by radially aligned spacecraft in the inner Heliosphere
Authors: Good, SW
Kilpua, EKJ
LaMoury, AT
Forsyth, RJ
Eastwood, JP
Möstl, C
Item Type: Journal Article
Abstract: Interplanetary coronal mass ejections (ICMEs) are a significant feature of the heliospheric environment and the primary cause of adverse space weather at the Earth. ICME propagation and the evolution of ICME magnetic field structure during propagation are still not fully understood. We analyze the magnetic field structures of 18 ICME magnetic flux ropes observed by radially aligned spacecraft in the inner heliosphere. Similarity in the underlying flux rope structures is determined through the application of a simple technique that maps the magnetic field profile from one spacecraft to the other. In many cases, the flux ropes show very strong underlying similarities at the different spacecraft. The mapping technique reveals similarities that are not readily apparent in the unmapped data and is a useful tool when determining whether magnetic field time series observed at different spacecraft are associated with the same ICME. Lundquist fitting has been applied to the flux ropes, and the rope orientations have been determined; macroscale differences in the profiles at the aligned spacecraft may be ascribed to differences in flux rope orientation. Assuming that the same region of the ICME was observed by the aligned spacecraft in each case, the fitting indicates some weak tendency for the rope axes to reduce in inclination relative to the solar equatorial plane and to align with the solar east‐west direction with heliocentric distance. Plain Language Summary Coronal mass ejections (CMEs) are large eruptions of magnetic field and plasma from the Sun. When they arrive at the Earth, these eruptions can cause significant damage to ground and orbital infrastructure; forecasting this “space weather” impact of CMEs at the Earth remains a difficult task. The impact of individual CMEs is largely dependent on their magnetic field configurations, and an important aspect of space weather forecasting is understanding how CME field configuration changes with distance from the Sun. We have analyzed the signatures of 18 CMEs observed by pairs of lined‐up spacecraft and show that their basic magnetic field structures often display significant self‐similarities, that is, they do not often show significant reordering of field features with heliocentric distance. This similarity points to the general usefulness of placing spacecraft between the Sun and Earth to act as early‐warning space weather monitors. CME signatures observed at such monitors would likely be similar to the signatures subsequently arriving at the Earth and could be used to produce space weather forecasts with longer lead times.
Issue Date: Jul-2019
Date of Acceptance: 6-May-2019
URI: http://hdl.handle.net/10044/1/72605
DOI: 10.1029/2019ja026475
ISSN: 2169-9380
Publisher: American Geophysical Union (AGU)
Start Page: 4960
End Page: 4982
Journal / Book Title: Journal of Geophysical Research: Space Physics
Volume: 124
Issue: 7
Copyright Statement: ©2019. American Geophysical Union. All Rights Reserved. This is the pre-peer reviewed version of the following article: Good, S. W., Kilpua, E. K. J., LaMoury, A. T., Forsyth, R. J., Eastwood, J. P., & Möstl, C. ( 2019). Self‐similarity of ICME flux ropes: Observations by radially aligned spacecraft in the inner heliosphere. Journal of Geophysical Research: Space Physics, 124, which has been published in final form at https://doi.org/10.1029/2019JA026475
Sponsor/Funder: Commission of the European Communities
Funder's Grant Number: 606692
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
coronal mass ejections
flux ropes
radially aligned spacecraft
inner heliosphere
CORONAL MASS EJECTIONS
INTERPLANETARY MAGNETIC CLOUDS
SOLAR-WIND
VENUS-EXPRESS
FIELD
CMES
EVOLUTION
MESSENGER
STEREO
MAGNETOSHEATH
physics.space-ph
physics.space-ph
Publication Status: Published
Article Number: 2019JA026475
Online Publication Date: 2019-05-16
Appears in Collections:Space and Atmospheric Physics
Physics
Faculty of Natural Sciences



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