A long-term high-resolution study of the visual activity curve of the Perseid meteor stream 1953-1983
Perseid and sporadic meteor hourly rates and magnitudes observed in 1953-1983 by a team of visual observers at the Onsala Space Observatory, Sweden, are analysed. A high-resolution study of the zenithal hourly rates of bright Perseid meteors /(m<=2.5) versus solar longitude has been made using a step length of /0.05° in solar longitude. The present study, which is based on 147 Perseid hourly rates
