Temporal structure of meteoroid stream and lunar seismicity according to Nakamura's catalogue

Details Temporal structure of meteoroid stream and lunar seismicity according to Nakamura's catalogue Temporal structure of meteoroid stream and lunar seismicity according to Nakamura's catalogue

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495...95k&link_type=abstract

In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August 2001, Kiruna, Sweden. Ed.: Barbara Warmbein. ESA SP-495, Noordw

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Meteoroid Streams

Scientific paper

Nakamura and Oberst pioneered in receiving data on the problem of meteoroid clustering streams which require analysing of wide range their temporal time structure. As a continuation of their research we have derived some types of temporal series. All series were studied by spectral analysis and as a result, common periodicity for all series and supplementary peaks in only two series were obtained. Spectrum of the series (1969 - 1977) disclosed time peaks on Mercury, Venus and Earth orbital periodictiy (88; 115; 225; 365; 27.3 days). Comparative analysis of spectra for other series disclosed following periodicity peaks: 44; 27; 5,5; 3,7 and others. The 10 and 5-days peaks are exceptionally interesting, because magnetic solar storms have the same periodicity. The dust component of meteoroid streams similar to dust plasma probably is modulated by variation of solar magnetic fields. Thin temporal structure of temporal variation of meteoroid streams has the peaks which coincide with half-periods of neighbourhood binary star systems (2.2 day - UW CMa; 3.6 days - h Aql).

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