Confirmation of a 152-Day Periodicity in the Occurrence of Solar Flares Inferred from Microwave Data,
Abstract
Evidence for a periodicity of about 155 + or - 5 days in the production of energetic solar flares has been reported by Rieger et al. (1984) and Kiplinger et al. (1984). The data on which these analyses were based are restricted to the years 1980 through early 1984. To see whether this periodicity is a persistent phenomenon, we have examined the occurrences of flares inferred from microwave data, which are available for most of the present and previous solar cycles. We find strong confirmation of a 152-day periodicity in the time interval previously studied, demonstrating that these flares are a useful indicator for the observed periodicity. We find evidence for persistence of the periodicity in the previous cycle (Cycle 20). In Cycle 20 the periodic modulation of the flare occurrence rate was weaker than in Cycle 21, but the phase has apparently remained coherent through both cycles.
Document Details
- Document Type
- Technical Report
- Publication Date
- Sep 01, 1985
- Accession Number
- ADA163091
Entities
People
- Richard S. Bogart
- Taeil Bai
Organizations
- Stanford University