Physical data and processes: MHD;
Physical data and processes: waves;
Sun: chromosphere;
Sun: magnetic fields;
D O I:
10.1016/j.newast.2015.07.008
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Nonlinear modulated both axisymmetric and non-axisymmetric MHD wave propagation in magnetic flux tubes is studied. In the cylindrical coordinates, ordinary differential equation with cubic nonlinearity is derived. In both cases of symmetry, the equation has solitary solutions. Modulation stability of the solutions is studied. The results of the study show that the propagation of axisymmetric soliton causes rising of plasma temperature in peripheral regions of a magnetic flux tube. In the non-axisymmetric case, it gives also temperature rising effect. Results of theoretical study are examined on idealized model of chromospheric spicule. (C) 2015 Elsevier B.V. All rights reserved.
机构:
Osserv Astrofis Catania, INAF, I-95123 Catania, Italy
Ist Nazl Fis Nucl, Sez Catania, I-95123 Catania, ItalyOsserv Astrofis Catania, INAF, I-95123 Catania, Italy
Bonanno, A.
Urpin, V.
论文数: 0引用数: 0
h-index: 0
机构:
Osserv Astrofis Catania, INAF, I-95123 Catania, Italy
AF Ioffe Phys Tech Inst, St Petersburg 194021, Russia
Isaac Newton Inst Chile, Branch St Petersburg, St Petersburg 194021, RussiaOsserv Astrofis Catania, INAF, I-95123 Catania, Italy