The rate profile of the Geminid meteor shower

  • Fox K
  • Williams I
  • Hughes D
N/ACitations
Citations of this article
5Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

A model for the formation of the Geminid meteor stream is developed. It is shown that this formation mechanism causes certain features to develop in the model stream which will result in both the rate profile being skew and mass segregation being observable. Such features are in fact observed in the Geminid shower and the magnitude of the features in the model are compared with those observed.

Cite

CITATION STYLE

APA

Fox, K., Williams, I. P., & Hughes, D. W. (1983). The rate profile of the Geminid meteor shower. Monthly Notices of the Royal Astronomical Society, 205(4), 1155–1169. https://doi.org/10.1093/mnras/205.4.1155

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free