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The double-gradient magnetic instability: Stabilizing effect of the guide field
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2015 (Engelska)Ingår i: Physics of Plasmas, ISSN 1070-664X, E-ISSN 1089-7674, Vol. 22, nr 1, artikel-id 012904Artikel i tidskrift (Refereegranskat) Published
Abstract [en]

The role of the dawn-dusk magnetic field component in stabilizing of the magnetotail flapping oscillations is investigated in the double-gradient model framework (Erkaev et al., Phys. Rev. Lett. 99, 235003 (2007)), extended for the magnetotail-like configurations with non-zero guide field By. Contribution of the guide field is examined both analytically and by means of linearized 2-dimensional (2D) and non-linear 3-dimensional (3D) MHD modeling. All three approaches demonstrate the same properties of the instability: stabilization of current sheet oscillations for short wavelength modes, appearing of the typical (fastest growing) wavelength lambda(peak) of the order of the current sheet width, decrease of the peak growth rate with increasing B-y value, and total decay of the mode for B-y similar to 0: 5 in the lobe magnetic field units. Analytical solution and 2D numerical simulations claim also the shift of lambda(peak) toward the longer wavelengths with increasing guide field. This result is barely visible in 3D simulations. It may be accounted for the specific background magnetic configuration, the pattern of tail-like equilibrium provided by approximated solution of the conventional Grad-Shafranov equation. The configuration demonstrates drastically changing radius of curvature of magnetic field lines, R-c. This, in turn, favors the "double-gradient" mode (lambda > R-c) in one part of the sheet and classical "ballooning" instability (lambda < R-c) in another part, which may result in generation of a "combined" unstable mode. (C) 2015 AIP Publishing LLC.

Ort, förlag, år, upplaga, sidor
2015. Vol. 22, nr 1, artikel-id 012904
Nationell ämneskategori
Fusion, plasma och rymdfysik
Identifikatorer
URN: urn:nbn:se:kth:diva-161152DOI: 10.1063/1.4905706ISI: 000349178100036Scopus ID: 2-s2.0-84923818507OAI: oai:DiVA.org:kth-161152DiVA, id: diva2:796503
Forskningsfinansiär
Swedish National Infrastructure for Computing (SNIC), 2014-1-176Swedish National Infrastructure for Computing (SNIC), 2014-8-38
Anmärkning

QC 20150319

Tillgänglig från: 2015-03-19 Skapad: 2015-03-09 Senast uppdaterad: 2017-12-04Bibliografiskt granskad

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Markidis, Stefano

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Markidis, Stefano
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High Performance Computing and Visualization (HPCViz)Parallelldatorcentrum, PDC
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Physics of Plasmas
Fusion, plasma och rymdfysik

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