No unique solution to the seismological problem of standing kink magnetohydrodynamic waves

被引:20
作者
Arregui, I. [1 ,2 ]
Goossens, M. [3 ]
机构
[1] Inst Astrofis Canarias, Tenerife 38205, Spain
[2] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
[3] Katholieke Univ Leuven, Dept Math, Ctr Math Plasma Astrophys, Celestijnenlaan 200B Bus 2400, B-3001 Leuven, Belgium
关键词
magnetohydrodynamics (MHD); waves; methods: statistical; Sun: corona; Sun: oscillations; CORONAL LOOP OSCILLATIONS; PERIOD MAGNETIC PULSATIONS; MHD WAVES; RESONANT ABSORPTION; SURFACE-WAVES; ALFVEN WAVES; FLUX TUBES; EXCITATION; BEHAVIOR; MODES;
D O I
10.1051/0004-6361/201833813
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The aim of this paper is to point out that the classic seismological problem using observations and theoretical expressions for the periods and damping times of transverse standing magnetohydrodynamic waves in coronal loops is better referred to as a reduced seismological problem. "Reduced" emphasises the fact that only a small number of characteristic quantities of the equilibrium profiles can be determined. Reduced also implies that there is no unique solution to the full seismological problem. Even the reduced seismological problem does not allow a unique solution. Bayesian inference results support our mathematical arguments and offer insight into the relationship between the algebraic and the probabilistic inversions.
引用
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页数:10
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