A procedure of selection of meteors from major streams for determination of mean orbits View Full Text


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Article Info

DATE

1995-01

AUTHORS

L. Neslušan, J. Svoreň, V. Porubčan

ABSTRACT

A procedure of selection of meteoroids from major streams is suggested and applied to the IAU Lund photographic database modified by a check for internal consistency among orbital elements (3411 orbits). Limits for choice of stream members were defined by break points on the plots of the cumulative numberNC vs. the Southworth-HawkinsD discriminant. For the break points were considered the points from which the dependenceNC vs.D changes to a quasi-linear one, and with the increasingD, NC changes only moderately. Except for the Taurids which desire a separate analysis, theNC vs.D diagrams are presented for the following major meteoroid streams: Quadrantids, Lyrids,η Aquarids,α Capricornids, N and Sδ Aquarids, Perseids, Orionids, Leonids and Geminids. The mean orbits, velocities and radiants of the streams are derived and compared with the osculating orbits of their parent bodies. The limitingDB was found to be a function of the number of the stream membersNCB. Omitting the exceptionally concentrated Geminids, the relation is in the formDB = 0.058 *ln(NCB) − 0.04. More... »

PAGES

427-433

References to SciGraph publications

  • 1994. Meteoroid Orbits Available from the IAU Meteor Data Center in ASTEROIDS, COMETS, METEORS 1993
  • 1995-01. On separation of major meteoroid streams from the sporadic background in EARTH, MOON, AND PLANETS
  • 1991. The IAU Meteor Data Center in Lund in ORIGIN AND EVOLUTION OF INTERPLANETARY DUST
  • Identifiers

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    http://scigraph.springernature.com/pub.10.1007/bf00671536

    DOI

    http://dx.doi.org/10.1007/bf00671536

    DIMENSIONS

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