Determination of the wind velocity vector by a micropulse coherent Doppler wind lidar with a duo-beam method

Author(s):  
Andrey V. Falits ◽  
Igor N. Smalikho ◽  
Artem A. Sukharev ◽  
Evgenii V. Gordeev ◽  
Viktor A. Banakh
1996 ◽  
Author(s):  
Rodolphe Krawczyk ◽  
Jean-Bernard Ghibaudo ◽  
Jean-Yves Labandibar ◽  
David V. Willetts ◽  
M. Vaughan ◽  
...  

1995 ◽  
Author(s):  
Rodolphe Krawczyk ◽  
Jean-Bernard Ghibaudo ◽  
Jean-Yves Labandibar ◽  
David V. Willetts ◽  
M. Vaughan ◽  
...  

2015 ◽  
Vol 58 (4) ◽  
pp. 253-261
Author(s):  
M. A. Panfilova ◽  
M. B. Kanevsky ◽  
G. N. Balandina ◽  
V. Yu. Karaev ◽  
A. Stoffelen ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


2011 ◽  
Vol 9 (9) ◽  
pp. 090604-90607 ◽  
Author(s):  
刘源 Yuan Liu ◽  
刘继桥 Jiqiao Liu ◽  
陈卫标 Weibiao Chen

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