Modeling the effect of meteor radiant distributions on the detection rate of meteor signals over forward-scatter links

Radio Science ◽  
1993 ◽  
Vol 28 (3) ◽  
pp. 428-440 ◽  
Author(s):  
R. S. Mawrey ◽  
A. D. Broadhurst
1957 ◽  
Vol 35 (6) ◽  
pp. 703-711 ◽  
Author(s):  
C. O. Hines ◽  
E. L. Vogan

The occurrence rate of meteoric signals, detected on a V.H.F. forward-scatter path, is analyzed for the time of the 1956 Quadrantid shower. The detection rate of the shower meteors is converted to an incidence rate, by use of the appropriate forward-scatter theory. The variation in the intrinsic strength of the shower is thereby determined, on an hour-to-hour basis, and it is compared with variations which have been obtained in other years by other methods. The comparison reveals a distinct secular shifting of the orbit of the Quadrantid meteor stream. It also illustrates the marked advantage of the new technique in assessing variations in the strengths of short-lived showers.


2007 ◽  
Vol 177 (4S) ◽  
pp. 651-651
Author(s):  
Nicolas B. Delongchamps ◽  
Vishal Chandan ◽  
Richard Jones ◽  
Gregory Threatte ◽  
Mary Jumbelic ◽  
...  

2004 ◽  
Vol 171 (4S) ◽  
pp. 479-479
Author(s):  
Roger Paul ◽  
Christian Korzineck ◽  
Ulrike Necknig ◽  
Herbert Leyh ◽  
Thomas Niesel ◽  
...  

2019 ◽  
Author(s):  
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G Axiaris ◽  
P Baxevanis ◽  
M Stoupaki ◽  
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2019 ◽  
Author(s):  
T Rath ◽  
F Vitali ◽  
E Klenske ◽  
J Siebler ◽  
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...  

2019 ◽  
Author(s):  
E Waldmann ◽  
H Sinkovec ◽  
G Heinze ◽  
D Penz ◽  
B Majcher ◽  
...  

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