The development of NASA's Crustal Dynamics Project

Author(s):  
John M. Bosworth ◽  
Robert J. Coates ◽  
Thomas L. Fischetti
Keyword(s):  
2019 ◽  
Vol 71 (1) ◽  
Author(s):  
Yoshihisa Iio ◽  
Richard H. Sibson ◽  
Toru Takeshita ◽  
Takeshi Sagiya ◽  
Bunichiro Shibazaki ◽  
...  

Science ◽  
1931 ◽  
Vol 73 (1900) ◽  
pp. 590-590
Author(s):  
J. S. DeLury
Keyword(s):  

2012 ◽  
Vol 13 (9) ◽  
Author(s):  
Eugénie Pérouse ◽  
Nicolas Chamot-Rooke ◽  
Alain Rabaute ◽  
Pierre Briole ◽  
François Jouanne ◽  
...  

Author(s):  
R. E. Price ◽  
M. J. Chandler ◽  
B. R. Schupler ◽  
P. R. Dachel

Author(s):  
Patrick Charlot ◽  
Jean-François Lestrade ◽  
Claude Boucher
Keyword(s):  

1988 ◽  
Vol 129 ◽  
pp. 505-506
Author(s):  
R. E. Price ◽  
M. J. Chandler ◽  
B. R. Schupler ◽  
P. R. Dachel

For the NASA Crustal Dynamics Project VLBI network, signals from quasars are recorded simultaneously at widely separated antennas. It is well known that hydrogen maser frequency standards provide the stable frequency reference used to precisely measure the difference in arrival time of the radio signals at the different antennas, enabling the determination of precise distances between the antennas. This paper reviews the practical requirements for maser support of VLBI for the Crustal Dynamics Project and describes the means used to meet these requirements for a network of eight fixed and three mobile stations which participate in approximately 200 VLBI experiments per year at locations in North America and the Pacific.


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