Solar Atmospheric Dynamics,
Abstract
This study, aimed at calculating the heating of the solar chromosphere and corona, started with the analysis of magneto-acoustic-gravity wave vector surfaces. To permit non-linear calculation of the excitation and propagation of these waves the equations of motion were written for an imposed horizontal structure -- namely six waves of the same wavelength propagating in an hexagonal pattern. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Jan 01, 1976
- Accession Number
- ADA027512
Entities
People
- R. F. Stein
- S. H. Hsieh
Organizations
- Brandeis University