Particle mass distribution in the new Perseid 1987-1994 filament

Planetary and Space Science

Volumn 45, Issue 5, 1997, Pages 525-527

  Simek, M ^a   Pecina, P ^a  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0040803106     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/s0032-0633(96)00150-x     Document Type: Review

References (5)

1. Jones, J., McIntosh, B. A. and Šimek, M. (1990) Ozone and the duration of overdense radio meteors. J. Atmos. Terr. Phys. 52, 253-258.
2. Roggemans, P. (1989) The Perseid meteor stream in 1988: a double maximum! WGN 20, 127-137.
3. Šimek, M. (1985) Regression method for long-term meteor shower radar data analysis. Bull. Astron. Inst. Czechosl. 36, 270-278.
4. Šimek, M. (1993) Diurnal variations of some meteor echoduration parameters. In Meteoroids and their Parent Bodies, eds J. Štohl and I. P. Williams, pp. 277-280. Astron. Inst. Slovak Academy of Sciences, Bratislava.
5. Šimek, M. and Pecina, P. (1996) Activity of the new filament in the Perseid meteor stream. In Physics, Chemistry, and Dynamics of Interplanetary Dust, eds B. A. S. Gustafson and M. S. Hanner, pp. 109-112. Astr. Soc. Pacific, San Francisco.