Publication Date:
2013-08-31
Description:
A model of the spatial density distribution of large (m greater than 10(exp -3) g) cometary meteoroids in the inner solar system is obtained assuming that they have orbits closely associated with that of their parent comet. Distributions of the orbital parameters of the Taurid, Quadrantid and Perseid meteoroid streams are used in developing the model.
Keywords:
ASTROPHYSICS
Type:
Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991; p 403-406
Format:
application/pdf