Discriminative sensing of temperature and acoustic impedance by using forward Brillouin scattering in large effective area fiber

2021 ◽  
Vol 14 (4) ◽  
pp. 042004
Author(s):  
Zelin Zhang ◽  
Yuangang Lu ◽  
Yosuke Tanaka ◽  
Jianqin Peng ◽  
Zhikang Zhuang
Keyword(s):  
Acoustic Impedance ◽  
Brillouin Scattering ◽  
Effective Area ◽  
Large Effective Area

scholarly journals Large effective area highTc rf SQUID

2003 ◽  
Vol 52 (10) ◽  
pp. 2580
Author(s):  
Liu Xin-Yuan ◽  
Xie Fei-Xiang ◽  
Meng Shu-Chao ◽  
Ma Ping ◽  
Yang Tao ◽  
...  
Keyword(s):  
Effective Area ◽  
Rf Squid ◽  
Large Effective Area

Transmission over 5.6 km large effective area and low-loss (1.7 dB∕km) photonic crystal fibre

2003 ◽  
Vol 39 (10) ◽  
pp. 796 ◽  
Author(s):  
B. Zsigri ◽  
C. Peucheret ◽  
M.D. Nielsen ◽  
P. Jeppesen
Keyword(s):  
Photonic Crystal ◽  
Effective Area ◽  
Low Loss ◽  
Photonic Crystal Fibre ◽  
Large Effective Area

ASCA Observations of White Dwarfs, Neutron Stars and Black Holes

1996 ◽  
Vol 165 ◽  
pp. 321-331
Author(s):  
H. Inoue
Keyword(s):  
Black Holes ◽  
Focal Plane ◽  
Thin Foil ◽  
Effective Area ◽  
Wide Energy Range ◽  
Ccd Cameras ◽  
X Ray ◽  
Different Types ◽  
Wide Energy ◽  
Large Effective Area

ASCA, the fourth Japanese X-ray astronomy satellite, was launched by the Institute of Space and Astronautical Science (ISAS) on 1993 February 20. ASCA is designed to be a high-capability X-ray observatory (Tanaka et al. 1994). It is equipped with nested thin-foil mirrors which provide a large effective area over a wide energy range from 0.5 to 10 keV. Two different types of detectors, CCD cameras (SIS) and imaging gas scintillation proportional counters (GIS) are employed as the focal plane instruments.

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