31.2: Proposal of the Perceptive Parameter Motion Picture Response Time (MPRT)

2003 ◽  
Vol 34 (1) ◽  
pp. 1039 ◽  
Author(s):  
Youichi Igarashi ◽  
T. Yamamoto ◽  
Y. Tanaka ◽  
J. Someya ◽  
Y. Nakakura ◽  
...  
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2017 ◽  
Vol 32 (8) ◽  
pp. 581-589
Author(s):  
彭枫琳 PENG Feng-lin ◽  
陈海伟 CHEN Hai-wei ◽  
苟方旺 GOU Fang-wang ◽  
吴诗聪 WU Shin-Tson

Optica ◽  
2016 ◽  
Vol 3 (9) ◽  
pp. 1033 ◽  
Author(s):  
Haiwei Chen ◽  
Fenglin Peng ◽  
Fangwang Gou ◽  
Yun-Han Lee ◽  
Michael Wand ◽  
...  

2017 ◽  
Vol 48 (1) ◽  
pp. 1826-1829
Author(s):  
Fenglin Peng ◽  
Haiwei Chen ◽  
Fangwang Gou ◽  
Yun-Han Lee ◽  
Shin-Tson Wu ◽  
...  
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2017 ◽  
Vol 121 (2) ◽  
pp. 023108 ◽  
Author(s):  
Fenglin Peng ◽  
Haiwei Chen ◽  
Fangwang Gou ◽  
Yun-Han Lee ◽  
Michael Wand ◽  
...  

2017 ◽  
Vol 48 (1) ◽  
pp. 478-481 ◽  
Author(s):  
Fenglin Peng ◽  
Haiwei Chen ◽  
Shin-Tson Wu
Keyword(s):  

Optica ◽  
2016 ◽  
Vol 3 (10) ◽  
pp. 1114
Author(s):  
Haiwei Chen ◽  
Fenglin Peng ◽  
Fangwang Gou ◽  
Yun-Han Lee ◽  
Michael Wand ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 46-48 ◽  
Author(s):  
M. Lecar

“Dynamical mixing”, i.e. relaxation of a stellar phase space distribution through interaction with the mean gravitational field, is numerically investigated for a one-dimensional self-gravitating stellar gas. Qualitative results are presented in the form of a motion picture of the flow of phase points (representing homogeneous slabs of stars) in two-dimensional phase space.


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