Titlebook: Advances in Meteoroid and Meteor Science; J. M. Trigo-Rodríguez,F. J. M. Rietmeijer,D. Janch Book 2008 Springer-Verlag New York 2008 CCD.P

迷住

Hongyu Huang,Guijun Fan,Yantao Li,Nankun Mul theory provide us not only with a new method to forecast the occurrences and intensities of shower activities, but it is also offers a new approach to explore the history of past activities of the parent comet by retro-tracking its associated meteor showers. We introduce the result of an effort fo

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Teng Huang,Huiqun Yu,Guisheng Faning them forward to the present. Our aim is to determine the existence and characteristics of associated meteor showers at Mars and Venus and compare them with 1P/Halley’s two known showers at the Earth. We find that one shower should be present at Venus and two at Mars. The number of meteors in tho

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ICLE

teoroids 2007 conference held at the impressive CosmoCaixa Science Museum in Barcelona, Spain. The conference took place between the 11th and the 15th of June and was organized by the Institute of Space Sciences (Consejo Superior de Investigaciones Científicas, CSIC) and the Institut d‘Estudis Espac

Comprise

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Zhihui Cao,Haifeng Sun,Ning Zhang,Xiang Lvting value for the Southworth-Hawkins D-criterion, two distinct filaments in the stream, on a short and a long period orbit, are separated. To confirm their consistency as filaments, their orbital evolution over 5,000 years is investigated.

GLEAN

Jun Zeng,Juan Yao,Yang Yu,Yingbo Wu 2.5 of the average peak strength) resembled meteor showers connected with the returns of resonant meteoroids. An investigation of data dating back to 1928 yielded similar rate enhancements in 1936, further supporting the assumption that meteoroids trapped in the 1:6 resonance with Jupiter caused the unusual 2006 Orionid return.

Gentry

peritonitis

https://doi.org/10.1007/978-3-642-03354-4d once an ejection model has been assumed. Such calculations, if made for a range of ejection model parameters and compared with observed parameters of storms and outbursts, can be used to constrain quantitatively the process of meteoroid ejection from the nucleus, including the mass distribution of ejected meteoroids.