Nonlinear Damping of Standing Kink Waves Computed With Elsasser Variables

被引:28
作者
Van Doorsselaere, Tom [1 ]
Goossens, Marcel [1 ]
Magyar, Norbert [2 ]
Ruderman, Michael S. [3 ,4 ]
Ismayilli, Rajab [1 ]
机构
[1] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B, B-3001 Leuven, Belgium
[2] Univ Warwick, Dept Phys, Ctr Fus Space & Astrophys, Coventry CV4 7AL, W Midlands, England
[3] Univ Sheffield, Sch Math & Stat SoMaS, Hicks Bldg,Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England
[4] Russian Acad Sci, Space Res Inst IKI, Moscow, Russia
基金
欧洲研究理事会;
关键词
Solar physics; Solar coronal waves; Solar corona; Magnetohydrodynamics; Solar active regions; Solar coronal loops; Solar coronal heating; CORONAL LOOP OSCILLATIONS; KELVIN-HELMHOLTZ INSTABILITY; TRANSVERSE-WAVES; SOLAR CORONA; TRANSITION-REGION; ALFVENIC WAVES; MHD WAVES; MODE; SEISMOLOGY; BEHAVIOR;
D O I
10.3847/1538-4357/abe630
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In a previous paper, we computed the energy density and the nonlinear energy cascade rate for transverse kink waves using Elsasser variables. In this paper, we focus on the standing kink waves, which are impulsively excited in coronal loops by external perturbations. We present an analytical calculation to compute the damping time due to the nonlinear development of the Kelvin-Helmholtz instability. The main result is that the damping time is inversely proportional to the oscillation amplitude. We compare the damping times from our formula with the results of numerical simulations and observations. In both cases we find a reasonably good match. The comparison with the simulations shows that the nonlinear damping dominates in the high amplitude regime, while the low amplitude regime shows damping by resonant absorption. In the comparison with the observations, we find a power law inversely proportional to the amplitude eta(-1) as an outer envelope for our Monte Carlo data points.
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页数:8
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