Latent heating of coronal loops

被引:12
作者
Zhugzhda, YD
Nakariakov, VM
机构
[1] RUSSIAN ACAD SCI,INST TERR MAGNETISM IONOSPHERE & RADIO WAVE P,TROITSK 142092,MOSCOW REGION,RUSSIA
[2] UNIV ST ANDREWS,DEPT MATH & COMPUTAT SCI,ST ANDREWS KY16 9SS,FIFE,SCOTLAND
关键词
D O I
10.1023/A:1004909603871
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The theory of weakly nonlinear slow magnetosonic waves in thin flux tubes is developed. A Korteweg-de Vries equation is derived for slow body waves. The analysis of solitary and periodic solutions shows that the nonlinear waves produce running narrowings of the tube. The similarity of the shallow-water theory and the thin-flux-tube approximation helps to outline the peaking and breaking of the nonlinear slow body waves. It appears that the running narrowing of the tube works as the de Laval nozzle in generating a cool supersonic jet and a subsequent shock that heats the plasma. The presented theory of nonlinear slow body waves suggests a mechanism of coronal loop heating, which meets many of the observational constraints.
引用
收藏
页码:107 / 121
页数:15
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