Relative Effectiveness of Three Stimulus Variables for Locating a Moving Sound Source

Perception ◽  
1987 ◽  
Vol 16 (2) ◽  
pp. 175-186 ◽  
Author(s):  
Lawrence D Rosenblum ◽  
Claudia Carello ◽  
Richard E Pastore

A study is reported in which it is shown that observers can use at least three types of acoustic variables that indicate reliably when a moving sound source is passing: interaural temporal differences, the Doppler effect, and amplitude change. Each of these variables was presented in isolation and each was successful in indicating when a (simulated) moving sound source passed an observer. These three variables were put into competition (with each indicating that closest passage occurred at a different time) in an effort to determine their relative importance. It was found that amplitude change dominated interaural temporal differences which, in turn, dominated the Doppler effect stimulus variable. The results are discussed in terms of two interpretations. First, it is possible that subjects based their judgements on the potential discriminability of each stimulus variable. However, because the stimuli used involved easily discriminable changes, subjects may instead have based their judgements on the independence of a stimulus variable from different environmental situation conditions. The dominance ordering obtained supports the second interpretation.


Author(s):  
T. Usagawa ◽  
S. Nishimura ◽  
M. Ebata ◽  
J. Okda




2017 ◽  
Vol 142 (4) ◽  
pp. 2542-2542 ◽  
Author(s):  
Elizabeth McQueney ◽  
Maryam Landi ◽  
Likun Zhang


2003 ◽  
Vol 41 (2) ◽  
pp. 89-91 ◽  
Author(s):  
Marcelo M. F. Saba ◽  
Rafael Antônio da S. Rosa


2010 ◽  
Vol 59 (7) ◽  
pp. 4738
Author(s):  
Yang Dian-Ge ◽  
Luo Yu-Gong ◽  
Li Bing ◽  
Li Ke-Qiang ◽  
Lian Xiao-Min


2014 ◽  
Vol 64 (2) ◽  
pp. 162-169
Author(s):  
Ju-Hyun SON ◽  
Mun-Ho KWON ◽  
Ho-Meoyng CHOI*




Optik ◽  
2021 ◽  
pp. 167565
Author(s):  
Shukri Klinaku


1998 ◽  
Vol 13 (01) ◽  
pp. 1-6 ◽  
Author(s):  
BRUNO BERTOTTI

The increase in the accuracy of Doppler measurements in space requires a rigorous definition of the observed quantity when the propagation occurs in a moving, and possibly dispersive medium, like the solar wind. This is usually done in two divergent ways: in the phase viewpoint it is the time derivative of the correction to the optical path; in the ray viewpoint the signal is obtained form the deflection produced in the ray. They can be reconciled by using the time derivative of the optical path in the Lagrangian sense, i.e. differentiating from ray to ray. To rigorously derive this result an understanding, through relativistic Hamiltonian theory, of the delicate interplay between rays and phase is required; a general perturbation theorem which generalizes the concept of the Doppler effect as a Lagrangian derivative is proved. Relativistic retardation corrections O(v) are obtained, well within the expected sensitivity of Doppler experiments near solar conjunction.





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