Published November 1989
| Version v1
Journal article
Computer simulation of Alfven resonance in a cylindrical, axially bounded flux tube
Description
The resonant absorption of Alfven waves in an axially bounded cylindrical flux tube is investigated in a dissipative MHD simulation. It is found that in an axially bounded flux tube, in contrast to an infinite periodic model, the resonant frequency is nearly independent of the poloidal component of the magnetic field. This is a consequence of the 'ballooning' structure of the resonant Alfven waves. The scaling with resistivity and viscosity of the width of the resonance layer, the dissipation rate, and the time for steady state absorption to occur, are all in agreement with theory. 19 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 346
- Series
- Astrophys. J.
- Journal Page Range
- 1035-1040
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21038208
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION; ALFVEN WAVES; COMPUTERIZED SIMULATION; HYDROMAGNETIC WAVES; MAGNETIC FIELD CONFIGURATIONS; MAGNETIC FLUX; MAGNETOHYDRODYNAMICS; RESONANCE; SOLAR CORONA
- Descriptors DEC
- ATMOSPHERES; FLUID MECHANICS; HYDRODYNAMICS; MECHANICS; SIMULATION; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE