Kaiser M K, Hecht H
NASA Ames Research Center, Moffett Field, CA 94035-1000, USA.
Percept Psychophys. 1995 Aug;57(6):817-25. doi: 10.3758/bf03206797.
The time until an approaching object will pass an observer (time to passage, or TTP) is optically specified by a global flow field even in the absence of local expansion or size cues. Kaiser and Mowafy (1993) have demonstrated that observers are in fact sensitive to this global flow information. The present studies investigate two factors that are usually ignored in work related TTP: (1) non-constant motion functions and (2) concomitant eye rotation. Non-constant velocities violate an assumption of some TTP derivations, and eye rotations may complicate heading extraction. Such factors have practical significance, for example, in the case of a pilot accelerating an aircraft or executing a roll. In our studies, a flow field of constant-sized stars was presented monocularly on a large screen. TTP judgments had to be made on the basis of one target star. The flow field varied in its acceleration pattern and its roll component. Observers did not appear to utilize acceleration information. In particular, TTPs with decelerating motion were consistently underestimated. TTP judgments were fairly robust with respect to roll, even when roll axis and track vector were decoupled. However, substantial decoupling between heading and track vector led to a decrement in performance, in both the presence and the absence of roll.
即使在没有局部扩展或大小线索的情况下,接近物体经过观察者的时间(通过时间,或TTP)也可以由全局流场通过光学方式确定。凯泽和莫瓦菲(1993)已经证明,观察者实际上对这种全局流信息很敏感。本研究调查了在与TTP相关的工作中通常被忽视的两个因素:(1)非恒定运动函数和(2)伴随的眼球转动。非恒定速度违反了一些TTP推导的假设,并且眼球转动可能会使航向提取变得复杂。这些因素具有实际意义,例如,在飞行员加速飞机或执行侧滚动作的情况下。在我们的研究中,在大屏幕上以单眼方式呈现了大小恒定的恒星的流场。必须根据一颗目标恒星做出TTP判断。流场在其加速度模式和侧滚分量方面有所不同。观察者似乎没有利用加速度信息。特别是,减速运动的TTP一直被低估。即使侧滚轴和轨迹向量解耦,TTP判断对于侧滚也相当稳健。然而,航向和轨迹向量之间的大量解耦导致性能下降,无论是否存在侧滚。