Phase-shifting interferometry with equal phase steps by use of a frequency-tunable diode laser and a Fabry–Perot cavity

2005 ◽  
Vol 44 (26) ◽  
pp. 5403 ◽  
Author(s):  
Youichi Bitou ◽  
Hajime Inaba ◽  
Feng-Lei Hong ◽  
Toshiyuki Takatsuji ◽  
Atsushi Onae
2009 ◽  
Vol 17 (3) ◽  
pp. 1442 ◽  
Author(s):  
Chu-Shik Kang ◽  
Jong-Ahn Kim ◽  
Tae Bong Eom ◽  
Roma Jang ◽  
Hae Yong Park ◽  
...  

2008 ◽  
Vol 47 (8) ◽  
pp. 6327-6332 ◽  
Author(s):  
Ying Li ◽  
Shigeo Nagano ◽  
Kensuke Matsubara ◽  
Hiroyuki Ito ◽  
Masatoshi Kajita ◽  
...  

2008 ◽  
Vol 28 (7) ◽  
pp. 1296-1300
Author(s):  
马骥驰 Ma Jichi ◽  
李岩 Li Yan ◽  
孙文科 Sun Wenke ◽  
许婕 Xu Jie

1988 ◽  
Vol 123 ◽  
pp. 475-479
Author(s):  
D. M. Rust ◽  
T. Appourchaux ◽  
F. Hill

A unique solar lineshift analyzer described by Rust, Burton and Leistner (1986) has been used at the Sacramento Peak Observatory to study solar oscillations. Operation of this “Stablized Solar Analyzer” (SSA) depends on the electro-optic effect in crystalline lithium niobate, the substrate of the solid Fabry-Perot etalon. Voltage on the etalon shifts the passband by ∼ 4.5 × 10−4 Å/V. The etalon has a passband of 0.175 Å at 6102.7 Å. The stabilization system uses a tunable diode laser to relate the Fabry-Perot passband to the D2 line of atomic Cs 133, at 8521.46 Å. This system reduced instrumental noise to less than Δλ/λ = 10−9 over a six-hour interval.


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