Published June 1990 | Version v1
Journal article

Magnetohydrodynamic mode coupling at a large-density jump

Creators

  • 1. Maryland Univ., College Park (USA)

Description

Reflection and transmission of MHD waves when a fast wave is incident on an interface across which the density changes by a factor on the order of 100 is investigated. The gas pressure is assumed to be negligible in comparison with the pressure of a uniform magnetic field. Rather than lengthy computations of the exact reflection and transmission coefficients, the results can be approximated by the use of some simple physical concepts. That is, the transformation of the fast mode to the Alfven mode at the interface can be explained in terms of polarization matching. The transmitted wave (or reflected wave) whose electric and magnetic vectors best match the incident perturbations should carry a larger portion of the flux than the other secondary waves. Using only the continuity of the electric field, the efficiency of coupling is adequately gaged by considering how well wave's electric field matches the incident wave's electric field. This polarization matching of the electric fields is refined, and an intuitively appealing method for estimating reflection and transmission coefficients is developed. This method is accurate and much faster than an exact numerical code. 8 refs

Additional details

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
356
Series
Astrophys. J.
Journal Page Range
693-703
ISSN
0004-637X
CODEN
ASJOA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
21084904
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ELECTRIC FIELDS; HYDROMAGNETIC WAVES; MAGNETIC FIELDS; PLASMA DENSITY; POLARIZATION; REFLECTION; SOLAR CORONA; WAVE PROPAGATION
Descriptors DEC
ATMOSPHERES; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE