Perseid meteor stream : cross and longitudinal structures from radar observations

1998 ◽  
Vol 47 (1-2) ◽  
pp. 281-289 ◽  
Author(s):  
M. Šimek ◽  
P. Pecina
1996 ◽  
Vol 150 ◽  
pp. 109-112 ◽  
Author(s):  
M. Šimek ◽  
P. Pecina

AbstractThe activity profile of the new filament in the Perseid meteor stream and its 1986-1994 levels were analyzed from Ondřejov radar observations. The filament was first detected in 1986 at its minimum activity level. Its maximum flux was observed in 1993. A secondary maximum appeared in the period 1988-1989. The cross-section profile of the new cloud shows an activity peak at L⊙ = 138°.87±0°.04 (equinox 1950.0).


1977 ◽  
Vol 39 ◽  
pp. 171-174
Author(s):  
B. A. McIntosh

In studying the evolution of meteor streams from cometary debris it is desirable to know the distribution of particles both around the orbit and in the cross section perpendicular to the orbit. Earth-based observations are limited to a once-per-year sample and also limited by the position of the observer on earth as it crosses the meteor stream. A continuous series, 11 years, of records of the Quadrantid meteor shower illustrates the problems and the results that can be achieved. International cooperation would greatly assist such studies.


2007 ◽  
Vol 66 (12) ◽  
pp. 1133-1141
Author(s):  
S. Ye. Yatsevich ◽  
V. B. Yefimov ◽  
I. A. Kalmykov

2006 ◽  
Vol 84A ◽  
pp. 295-304 ◽  
Author(s):  
Sundararajan SRIDHARAN ◽  
Toshitaka TSUDA ◽  
Takuji NAKAMURA ◽  
Robert A. VINCENT ◽  
EFFENDY

2021 ◽  
Vol 12 (6) ◽  
pp. 573-584
Author(s):  
Xinzhe Yuan ◽  
Weizeng Shao ◽  
Bing Han ◽  
Xiaochen Wang ◽  
Xiaoqing Wang ◽  
...  

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