TV meteor streams searching
| dc.contributor.author | Jopek, Tadeusz J. | |
| dc.date.accessioned | 2015-09-04T14:36:01Z | |
| dc.date.available | 2015-09-04T14:36:01Z | |
| dc.date.issued | 1993 | |
| dc.description.abstract | Using a modified D-criterion (threshold Do=0.2), among 531 TV meteor orbits, 23 streams has been identified. Adout 30% of the orbits belongs to the stream component. Only 3 streams have orbits inclined more than 30deg. Four streams have reciprocal orbits. The major stream Herculids shown to be a complex structure, sensitive on the choice of the D- threshold value. The Taurids complex differs slightly from the photographic one. The theta Piscids stream has very small orbit, the mean semi-major axis equals to 0.79AU. This stream seems to be TV component of the Eccentrides system, but with Do=0.21 the theta Piscids have joined S. Taurids. The TV Orionids appeared in two branches. One of them includes a single orbit which belongs to the eta Aquariids. | pl_PL |
| dc.identifier.citation | Jopek T.J., 1993, in Meteoroids and their parent bodies, Proceedings of the International Astronomical Symposium held at Smolenice, Slovakia, July 6-12, 1992, Bratislava, eds Porubcan V., Williams I.P, 269-272 | pl_PL |
| dc.identifier.uri | http://hdl.handle.net/10593/13855 | |
| dc.language.iso | en_US | pl_PL |
| dc.publisher | Astronomical Institute Slovak Academy of Sciences, Bratislava | pl_PL |
| dc.rights | info:eu-repo/semantics/openAccess | pl_PL |
| dc.subject | TV meteor streams | pl_PL |
| dc.title | TV meteor streams searching | pl_PL |
| dc.type | Materiały konferencyjne | pl_PL |