scholarly journals Omnidirectional investigation of two-dimensional periodic nanostructure arrays by a two-axis Lloyd’s mirror interferometer

2020 ◽  
Vol 18 ◽  
pp. 103225
Author(s):  
Haitao Jiang ◽  
Zhe Zhuang ◽  
Xiong Zhang ◽  
Cheng Li ◽  
Hu Chen ◽  
...  
2008 ◽  
Author(s):  
Sungkwun Kenneth Lyo ◽  
Wei Pan ◽  
John Louis Reno ◽  
Joel Robert Wendt ◽  
Daniel Lee Barton

Nanomaterials ◽  
2020 ◽  
Vol 10 (9) ◽  
pp. 1820
Author(s):  
Yi-Hsien Liu ◽  
Shu-Chun Yeh ◽  
Chung-Wei Cheng

Laser-induced periodic surface structures (LIPSS) is the sub-wavelength periodic nanostructure, which is generally generated by the femtosecond laser. There are two kinds of LIPSS, low spatial frequency LIPSS (LSFL) and high spatial LIPSS (HSFL), and the period size is close and less than half of the laser wavelength, respectively. Fabrication of two-dimensional (2D) LSFL and HSFL on a titanium surface with a linear-polarized femtosecond green laser beam (wavelength 515 nm) and cross-scanning strategies is demonstrated in this study. Four types of LIPSS structures are obtained by controlling the laser fluence, irradiated pulses, and cross-scanning strategies: 1D-LSFL perpendicular to laser polarization with a period of 300–360 nm, 1D-HSFL parallel to laser polarization with a period of 55–75 nm, 2D-LSFL dot-like structures with a period ~200 nm, and 2D-HSFL net-like structures with a period of 50–100 nm.


2010 ◽  
Vol 22 (38) ◽  
pp. 4249-4269 ◽  
Author(s):  
Junhu Zhang ◽  
Yunfeng Li ◽  
Xuemin Zhang ◽  
Bai Yang

Nanoscale ◽  
2015 ◽  
Vol 7 (10) ◽  
pp. 4306-4324 ◽  
Author(s):  
Jia Lin Zhang ◽  
Shu Zhong ◽  
Jian Qiang Zhong ◽  
Tian Chao Niu ◽  
Wen Ping Hu ◽  
...  

2017 ◽  
Vol 696 ◽  
pp. 1180-1188 ◽  
Author(s):  
Hui Yun Tan ◽  
Bao Zhi Yu ◽  
Lin Li Cao ◽  
Tao Cheng ◽  
Xin Liang Zheng ◽  
...  

Nano Letters ◽  
2010 ◽  
Vol 10 (9) ◽  
pp. 3717-3721 ◽  
Author(s):  
Allon I. Hochbaum ◽  
Joanna Aizenberg

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.


1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.


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