The ν13 fundamental band of benzene

1983 ◽  
Vol 61 (2) ◽  
pp. 269-277 ◽  
Author(s):  
Josef Plíva ◽  
J. W. C. Johns

The perpendicular band of the E1u vibration ν13 of benzene, occurring near 6.7 μm, has been measured on a BOMEM high-resolution Fourier transform spectrometer with a 246 cm optical path difference. The observed linewidth (full width at half height) of ~ 0.0048 cm−1 was reduced by deconvolution to ~ 0.0020 cm−1, which is slightly below the Doppler limit. The dense rotational structure was well resolved, and it was possible to assign over 125 subbands in the region 1466.5 to 1503 cm−1. A perturbation, identified as a third-order Jx,y-Coriolis interaction with a state located only ~ 0.055 cm−1 above the fundamental (presumably the A2u component of ν4 + 2ν20), causes distortion of the rotational structure and formation of subband heads in the low-KpQ-branches, which exhibit a striking line-like shape. The spectrum was analyzed in detail with the aid of the computer program SYMTOP for the treatment of symmetric top bands whose upper states are involved in arbitrary interactions. The Hamiltonian included, in addition to the Jx.y -Coriolis perturbation, the l-type resonance [Formula: see text]. A set of accurate spectroscopic constants was obtained for the perturbed ν13 upper state. Using these constants, 2750 lines of the ν13 band, which could be assigned nonzero weights, were reproduced with an overall standard deviation of ~ 0.00046 cm−1.


2019 ◽  
pp. 215-248
Author(s):  
B. D. Guenther

Using simple ray tracinig technliques presented in Chapter 6, we demonstrate that a general ray is not focused to the position predicted by paraxial theory. The aberration displayed is spherical aberration. Two methods of measuring aberration: the use of optical path difference to characterize wavefront aberration. The transverse ray coefficients to generate a ray intercept plot. Experimental examples of all the third order aberrations are given. In addition to spherical aberration, they include coma, astigmatism, field curvature, and distortion Only two types of aberration correction are discussed, removal of spherical aberration in the Hubble Space telescope and chromatic aberration. A detailed example of chromatic aberration is given.







Optik ◽  
2015 ◽  
Vol 126 (24) ◽  
pp. 5420-5422
Author(s):  
H.H. Ley ◽  
A. Yahaya ◽  
Y. Munajat


Measurement ◽  
2017 ◽  
Vol 109 ◽  
pp. 233-241 ◽  
Author(s):  
Fuqiang Zhou ◽  
Xin Chen ◽  
Haishu Tan ◽  
Xinghua Chai


1963 ◽  
Vol 1 (6) ◽  
Author(s):  
Francis E. Washer ◽  
Walter R. Darling


Author(s):  
Vinod Singh ◽  
Gaurav Singhal ◽  
Prabal Talukdar

Abstract CFD based thermal design of a transverse flow optical cavity is carried out for 1 kW Nd3+ POCl3 liquid laser source to investigate temperature and velocity distribution in the optical pumping region of the cavity. Temperature gradient and turbulence both affect the refractive index of the liquid gain medium, which results in optical path difference, divergence and hence, poorer quality of the laser beam. The main purpose of this design is to achieve uniform flow and least temperature gradient in the optical pumping region so that the optical path difference can be minimized and a good beam quality can be achieved. CFD model has been developed for carrying out thermo-fluid simulations for this thermal system and based on these simulations, an optimum geometry of inlet ports along with their position from optical pumping region have been proposed. A user defined function (UDF) is incorporated for the input of spatially varying heat source term in each cell of the optical pumping region of the cavity. Variations in refractive index and optical path difference are estimated from the temperature data using another UDF. Simulation reveals that mass flow rate between 1.5 kg/s to 2.0 kg/s maintains the optical homogeneity of gain medium. Preliminary experiments have been carried out to demonstrate the effect of flow rate on the beam divergence and thereby exhibiting the importance of present simulation work.





2012 ◽  
Author(s):  
Ming-Ying Hsu ◽  
Yu-Chuan Lin ◽  
Chia-Yen Chan ◽  
Wei-Cheng Lin ◽  
Shenq-Tsong Chan ◽  
...  


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