STANFORD MICROWAVE SPECTROHELIOGRAMS FOR 1960 JUNE
Abstract
By means of a microwave spectroheliograph, maps were made of the sun which show the disk distribution of solar radio emission at a wavelength of 9.1 cm by means of radioisophotes, or lines of constant brightness temperature. The contour interval, which varies from map to map, is usually about 80,000 K, and is determined after the map is drawn by reference to the measured flux density of the whole sun.
Document Details
- Document Type
- Technical Report
- Publication Date
- Apr 28, 1961
- Accession Number
- AD0257820
Entities
People
- G. Swarup
Organizations
- Stanford University