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BIBTEX RIS

Radio-Echo Observations of the Major Night-Time Meteor Streams

1966; Oxford University Press; Volume: 132; Issue: 1 Linguagem: Inglês

10.1093/mnras/132.1.225

ISSN

1365-2966

Autores

Thomas Kaiser, L. M. G. Poole, A. R. Webster,

Tópico(s)

Solar and Space Plasma Dynamics

Resumo

The results of observations of the Perseid meteor shower during 1962 August are presented, and an attempt has been made to interpret the observed activity in terms of a radiant model comprising an intense discrete centre of activity, and a more diffuse component. The distribution in radio-magnitude in the range +8.4 to +6.8 m of the shower meteors has been studied as a function of solar longitude, and significant systematic variations, especially for the discrete component are indicated.

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