scholarly journals Study of applying fiber based laser with the primary standard for optical power and improvement of spectral responsivity scales in near IR range

2013 ◽  
Author(s):  
Jing Zhang ◽  
Jia Jie Teo ◽  
Xuebo Huang
2011 ◽  
Vol 13 (38) ◽  
pp. 17304 ◽  
Author(s):  
Mickaël Four ◽  
Didier Riehl ◽  
Olivier Mongin ◽  
Mireille Blanchard-Desce ◽  
Latévi Max Lawson-Daku ◽  
...  

2022 ◽  
Vol 2149 (1) ◽  
pp. 012006
Author(s):  
Kinza Maham ◽  
Petri Kärhä ◽  
Farshid Manoocheri ◽  
Erkki Ikonen

Abstract We report realization of scales for optical power of lasers and spectral responsivity of laser power detectors based on a predictable quantum efficient detector (PQED) over the spectral range of 400 nm–800 nm. The PQED is characterized and used to measure optical power of a laser that is further used in calibration of the responsivities of a working standard trap detector at four distinct laser lines, with an expanded uncertainty of about 0.05%. We present a comparison of responsivities calibrated against the PQED at Aalto and the cryogenic radiometer at RISE, Sweden. The measurement results support the concept that the PQED can be used as a primary standard of optical power.


Metrologia ◽  
2014 ◽  
Vol 51 (3) ◽  
pp. 197-202 ◽  
Author(s):  
Timo Dönsberg ◽  
Meelis Sildoja ◽  
Farshid Manoocheri ◽  
Mikko Merimaa ◽  
Leo Petroff ◽  
...  

2002 ◽  
Vol 10 (1) ◽  
pp. 70 ◽  
Author(s):  
Didier Fussen ◽  
Filip Vanhellemont ◽  
Christine Bingen

2012 ◽  
Vol 42 (3) ◽  
pp. 244-249 ◽  
Author(s):  
A Yu Klimchuk ◽  
Aleksandr I Nadezhdinskii ◽  
Ya Ya Ponurovskii ◽  
Yu P Shapovalov ◽  
A V Rodin

2012 ◽  
Vol 8 (S293) ◽  
pp. 39-45 ◽  
Author(s):  
Tong Li ◽  
Feng Tian

AbstractHigh atmospheric abundances of oxygen has been widely considered to be a reliable biosignature for life on exoplanets in the habitable zones of all types of stars. Recently it was proposed that the unique UV spectra of observed planet-hosting M dwarfs could lead to the buildup of molecular oxygen in the atmospheres of habitable but lifeless planets around these stars (Tian et al. 2014). However, the detectability of the accumulated O2 was not modeled. In this work we developed a new line by line radiative transfer model based on HITRAN database and used the model to simulate the reflectivity in the visible and near IR range. We show that abiotically produced and maintained O2 in the 0.2% level is observable at 13105 cm−1 (0.76 μm) with the spectra resolution of 70.


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