THE OBSERVATION OF 3.3-MM BURSTS AND THEIR CORRELATION WITH SOFT X-RAY BURSTS.
Abstract
Observations of 3.3-mm bursts show that in most cases these bursts have slower rise times and are longer lived than the impulsive centimeter bursts. There is a good temporal correlation between the 3.3-mm and soft x-ray bursts, indicating that these bursts have their origin in the same thermal source mechanism, although these emissions may not arise from the same electrons. (Author)
Document Details
- Document Type
- Technical Report
- Publication Date
- Sep 03, 1970
- Accession Number
- AD0711784
Entities
People
- Fred I. Shimabukuro
Organizations
- The Aerospace Corporation