1977
DOI: 10.1007/bf00655873
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The superposition image in the eye ofEphestia k�hniella

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Cited by 32 publications
(26 citation statements)
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“…The two curves are presented as a function of the angle of incidence, ␣. Because the maximum angle of incidence ␣ max for E. kühniella is 22.5° ( Cleary et al, 1977) and for P. tristifica ␣ max =11.4° (Land, 1984), the curves virtually coincide when plotted as a function of the exit angle, ␤. The difference in optical path length, ⌬OPL, of rays through facets 2 with respect to those through facet 1 appears to be distinctly smaller than the coherence length l c =2.8·m for green receptors (see Materials and methods), but the ⌬OPLs for the other adjacent facets in a meridional section (4, 6, 9, etc.)…”
Section: Optical Path Length Differencementioning
confidence: 90%
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“…The two curves are presented as a function of the angle of incidence, ␣. Because the maximum angle of incidence ␣ max for E. kühniella is 22.5° ( Cleary et al, 1977) and for P. tristifica ␣ max =11.4° (Land, 1984), the curves virtually coincide when plotted as a function of the exit angle, ␤. The difference in optical path length, ⌬OPL, of rays through facets 2 with respect to those through facet 1 appears to be distinctly smaller than the coherence length l c =2.8·m for green receptors (see Materials and methods), but the ⌬OPLs for the other adjacent facets in a meridional section (4, 6, 9, etc.)…”
Section: Optical Path Length Differencementioning
confidence: 90%
“…The results can be compared with published experimental data for the nocturnal moth Ephestia kühniella and the skipper Toxidia peroni. For E. kühniella, Fig.·3 predicts m=2.3-2.0, but ray tracing calculations based on refractive index measurements yielded a constant m=1.32 (Cleary et al, 1977). For T. peroni, Fig.·3 predicts m=1.0-0.6, but direct measurements yielded a fairly constant m=1.6.…”
Section: Angular Magnification and Defocusmentioning
confidence: 97%
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“…The non-target rhabdoms may produce an error signal and inevitably blur the image, causing a loss in resolving power. Although we do not have optical data on the position of the superposition image formed by the dioptric apparatus in the eye of O. antiqua, the superposition images from other moths like Ephestia kühniella (Cleary et al, 1977;Kunze, 1979) and Phalaenoides tristifica (Narvarro & Franceschini, 1998) are located deep in the eyes at distances of 125 µm and 137 µm respectively. The widths of the clearzone of Ephestia kühniella and Phalaeoides tristifica are about 100 µm (Fischer & Horstmann, 1971) and 137 µm, respectively (Narvarro & Franceschini, 1998) and thus agree with values from the eye of male O. antiqua (99-106 µm, Table 2).…”
Section: The Retinula and Its Photoreceptorsmentioning
confidence: 99%