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Apex Dips of Experimental Flux Ropes: Helix or Cusp?

Wongwaitayakornkul, Pakorn and Haw, Magnus A. and Li, Hui and Li, Shengtai and Bellan, Paul M. (2017) Apex Dips of Experimental Flux Ropes: Helix or Cusp? Astrophysical Journal, 848 (2). Art. No. 89. ISSN 1538-4357. https://resolver.caltech.edu/CaltechAUTHORS:20171017-111654610

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Abstract

We present a new theory for the presence of apex dips in certain experimental flux ropes. Previously such dips were thought to be projections of a helical loop axis generated by the kink instability. However, new evidence from experiments and simulations suggest that the feature is a 2D cusp rather than a 3D helix. The proposed mechanism for cusp formation is a density pileup region generated by nonlinear interaction of neutral gas cones emitted from fast-gas nozzles. The results indicate that density perturbations can result in large distortions of an erupting flux rope, even in the absence of significant pressure or gravitational forces. The density pileup at the apex also suppresses the m = 1 kink mode by acting as a stationary node. Consequently, more accurate density profiles should be considered when attempting to model the stability and shape of solar and astrophysical flux ropes.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-4357/aa8990DOIArticle
http://iopscience.iop.org/article/10.3847/1538-4357/aa8990/metaPublisherArticle
ORCID:
AuthorORCID
Haw, Magnus A.0000-0001-5739-5160
Li, Hui0000-0003-3556-6568
Bellan, Paul M.0000-0002-0886-8782
Additional Information:© 2017 American Astronomical Society. Received 2017 June 8; revised 2017 August 28; accepted 2017 August 29; published 2017 October 17. This work was supported by NSF under award 1348393, AFOSR under award FA9550-11-1-0184, and DOE under awards DE-FG02-04ER54755 and DE-SC0010471. H.L. and S.L. acknowledge the support from DoE/OFES and LANL/LDRD programs.
Funders:
Funding AgencyGrant Number
NSFAGS-1348393
Air Force Office of Scientific Research (AFOSR)FA9550-11-1-0184
Department of Energy (DOE)DE-FG02-04ER54755
Department of Energy (DOE)DE-SC0010471
Subject Keywords:magnetohydrodynamics (MHD) ; methods: laboratory: atomic; methods: numerical; plasmas; Sun: filaments, prominences
Issue or Number:2
Record Number:CaltechAUTHORS:20171017-111654610
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20171017-111654610
Official Citation:Pakorn Wongwaitayakornkul et al 2017 ApJ 848 89
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:82421
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:17 Oct 2017 20:19
Last Modified:03 Oct 2019 18:54

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