CALCULATIONS OF SIGNAL-TO-NOISE RATIOS FOR SOLAR RADAR ECHOES
Abstract
The procedure for computing the signal-to-noise ratio of radar echoes from the sun is outlined. The radial distribution of electron density in the corona, the coronal temperature, solar noise, galactic noise, and radar-system parameters are taken into account. Examples are given of computations for two solar radar systems that will soon be in operation.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jul 18, 1961
- Accession Number
- AD0265347
Entities
People
- P. Yoh
Organizations
- Stanford University