Simulation of the Formation and Evolutio
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P. Brown; J. Jones
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Article
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1998
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Elsevier Science
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English
โ 945 KB
to shift the locations of the maximums to higher solar longitudes. A discrepancy which is present for both the 1993 and Four major models of cometary meteoroid ejection are devel-1994 peak locations of 1-2 h between the observed and modeled oped and used to simulate plausible starting conditions for