Hostname: page-component-7479d7b7d-fwgfc Total loading time: 0 Render date: 2024-07-12T14:20:40.598Z Has data issue: false hasContentIssue false
  • English
  • Français

On the Determination of Velocities of Radar Meteors

Published online by Cambridge University Press:  27 February 2018

P. Pecina
P. Pecina*
Affiliation:
Astronomical Institute of the Czech Academy of Sciences, 251 65 Ondřejov, Czech Republic, e-mail:ppecina@asu.cas.cz

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The results of testing the classical method of velocity determination based on the positions of the extrema of Fresnel diffraction patterns (FDP) in radio echo amplitude, is presented. This technique is compared to the method of nonlinear least squares fitting (NLSF) of the theoretical patterns to the observed those. It is shown that while the classical method can fail in yielding correct values for the velocity of radar meteors, the NLSF method always yields good results.

Type
II. Meteors
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 71 - 74
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Baggaley, W. J., Bennett, R. G. T., Steel, D. L., & Taylor, A. D. 1994, Q. J. R. astr. Soc, 35, 293 Google Scholar
Pecina, P. 1988, Bull Astron. Inst, CzechosL, 39, 193 Google Scholar
Šimek, M. 1968, Canad. J. Phys., 46, 1563 Google Scholar