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Meteoroid orbits from video meteors. The case of the Geminid stream

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00478695" target="_blank" >RIV/67985815:_____/17:00478695 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.pss.2017.01.004" target="_blank" >http://dx.doi.org/10.1016/j.pss.2017.01.004</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.pss.2017.01.004" target="_blank" >10.1016/j.pss.2017.01.004</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Meteoroid orbits from video meteors. The case of the Geminid stream

  • Original language description

    The observed orbital dispersions in the Geminid stream described by the median absolute deviation range from 0.029 to 0.042 AU(-1) for the video catalogues. The distribution of the semi-major axes of video meteors in all the databases, except for the Ondrejov (Czech) data, seem to be systematically biased in comparison with the photographic and radio meteors. The determined velocities of the video data are underestimated, probably as a consequence of the methods used for the positional and velocity measurements. The largest shift is observed in the EDMOND and SonotaCo catalogues. Except for the measurement errors which influence the analyses and their interpretations, we also point out the problem of the uncertainties of the numerical integration procedures that influence the simulations' results. Several experimental integrations of the Geminids parent asteroid, which we performed from the present to the past and then back to the year 2015, showed that a complete reproduction, including also the mean anomaly, is only possible for a time span of about 2700 years.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/GA14-25251S" target="_blank" >GA14-25251S: Nonlinear imaging systems with spatially variant point spread function</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2017

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Planetary and Space Science

  • ISSN

    0032-0633

  • e-ISSN

  • Volume of the periodical

    143

  • Issue of the periodical within the volume

    SI

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    10

  • Pages from-to

    89-98

  • UT code for WoS article

    000405050600015

  • EID of the result in the Scopus database

    2-s2.0-85009740783