Microwave Spectroscopy of a Solar Active Region Observed during a Partial Eclipse.
Abstract
This work presents the first attempt at using microwave spectroscopy as a diagnostic tool for the study of complex solar active regions. Since the relevant emission mechanisms are gyroresonance opacity and thermal bremsstrahlung (free-free), the microwave emission is expected to depend on the values of temperature, density and magnetic fields in the solar corona.
Document Details
- Document Type
- Technical Report
- Publication Date
- Apr 01, 1976
- Accession Number
- ADA181468
Entities
People
- D. E. Gary
- G. J. Hurford
Organizations
- California Institute of Technology