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This temporal relationship between the light and food can be preserved intact, but if the experimenter now arranges that food is equally available at other times (when the light is not on), the pigeon will not peck at the illuminated disk.
This was attributed to the existence of low local values of incident light intensity on the illuminated disk.
A pigeon, for example, will learn by classical conditioning to peck an illuminated disk in a Skinner box if, whenever the disk is illuminated, food is delivered.
Subsequently, the "Skinner box" was adapted for use with pigeons, who were required to peck at a small, illuminated disk on one wall of the box in order to obtain some grain.
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Similarly, a pigeon will learn to peck at a disk illuminated with red light even if a gap of several seconds separates this response from the delivery of food.
The dim flashes were spatially restricted by an adjustable slit ∼1-μm wide, set perpendicular to the length of the rod outer segment, illuminating ∼30 40 disks (Field and Rieke, 2002).
b Normalized optical extinction cross section of TiN nano-disk illuminated with plane wave at normal incidence.
In the quasi-static approximation, each nano-disk illuminated with incident light could be treated as a dipole with polarizability [42], alpha propto Vfrac{varepsilon_1-{varepsilon}_2}{varepsilon_2+Lleft({varepsilon}_1-{varepsilon}_2right)} (1) Fig. 4 a Absorption spectra without monolayer MoS2 for p x = 200 nm, d = 120 nm, and t 1 = t 2 = 50 nm.
A pigeon, for example, is required to choose between two disks, one illuminated with red light and the other with green light.
The effective PS II quantum yield (Y (II)) was calculated according to the formula [24]: <img src="http://journals.plos.org/plosone/article/asset?id=info?doi/10.1371/journal.pone.0008571.e001.PNG" class= inline-graphic"/> When the disks were illuminated, the maximum fluorescence yield (F'm) was detected, which was normally lower than Fm due to non-photochemical quenching (i.e. heat dissipation).
We present calculations of LTE model atmospheres of some ring on the accretion disk, which are illuminated by isotropic hard X-rays.
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