Polarized skylight orientation in the desert antCataglyphis

Summary The desert antCataglyphis bicolor is able to use the pattern of polarized light in the sky as compass. By confronting the ant to single spots of artificially and naturally polarized light it is shown howCataglyphis uses the polarization pattern.When exposed to a horizontal e-vector,Cataglyphis was always oriented correctly. Orientation errors occurred, however, when other e-vector directions were presented. This indicates that the e-vector positions assumed by the ant do not coincide with the e-vector positions actually realized in the sky. From this it is concluded thatCataglyphis has no detailed knowledge of the actual azimuthal positions of the e-vectors. Instead, it is relying on a simplified celestial map of the polarization patterns in the sky (Fig. 7).Usually, the ant did not confuse celestial spots with identical e-vector directions. Even at sunset when the polarization pattern is completely ambiguous, correct orientation occurred. This suggests that the ant uses additional celestial cues such as the degree of polarization, the color or the intensity to find its way home when the sun is obscured.     

Integration of environmental stimuli in the migratory orientation of the savannah sparrow (Passerculus sandwichensis)

Two ‘cue-conflict’ experiments were designed to evaluate the role of (1) solar cues at sunset and stars, and (2) solar cues at sunset and geomagnetic stimuli, in the migratory orientation of the savannah sparrow (Passerculus sandwichensis). A sunset and stars experiment exposed birds in the experimental group to a mirror-reflected sunset followed by an unmanipulated view of stars. Experimental birds shifted their migratory activity in accordance with the setting sun despite exposure to a normal night sky. The sunset and geomagnetism experiment exposed birds in the experimental group to a simultaneous shift in both the position of sunset and the earth's magnetic field. Again experimentals shifted their activity in accordance with the setting sun rather than the artificially shifted magnetic field. Savannah sparrows probaly use stars as celestial landmarks to maintain a preferred direction and do not reorient their activity when exposed to an alternative cue once a direction is established. Moreover, savannah sparrows with experience of migration do not require geomagnetic information in order to use the solar cues available at sunset to select a migratory direction.     

Solar cues in the migratory orientation of the Savannah sparrow, Passerculus sandwichensis

Results clearly implicate the setting sun as a critical source of directional information in the migratory orientation of the savannah sparrow, Passerculus sandwichensis. Savannah sparrows allowed a view of both sunset and stars displayed oriented behaviour in biologically meaningful directions during spring and fall seasons. When the same individuals were denied a view of sunset, and tested under the stars alone, disorientation characterized their behaviour. Furthermore, birds allowed a view of sunset, but tested under ‘overcast’ night skies (no stars visible), displayed well-oriented behaviour indicating the sufficiency of sunset. Experiments in which the migrant's internal chronometer was shifted suggested a fixed-angle (menotactic) response to the sunset cue rather than a time-compensating compass mechanism. I believe stars are valuable to this migrant as celestial reference points. Orientational information gained at the time of sunset is transferred to stars on a nightly basis. The relationship between solar and stellar cues is apparently hierarchical in the savannah sparrow. Information necessary to select the appropriate migratory direction is gained from the primary cue, the setting sun, while maintenance of that heading is dependent on a secondary cue, probably the stars.     

Microorganisms collected during a solar eclipse in India

A solar eclipse was observed in India on 24 October, 1995. It was a total eclipse in some parts of the country while it was partial in other parts. The effect of the total or partial eclipse on the airspora was investigated. Airspora play an important role in various phenomena on the earth. Martins rose bengal agar plates were exposed at Kalpi (total eclipse) and at Aurangabad (partial eclipse). Both the quantitative and qualitative variations in the airspora were observed during different phases of the eclipse. At both places the number of fungal colonies were higher during the pre- and post-eclipse phase. There was a decrease at contact phase, total/partial or diamond ring eclipse phase. Thus, very minor changes were observed during the eclipse period. Bacterial colonies were higher at the post-eclipse phase at Kalpi but were less at Aurangabad during this phase. At Kalpi 23 fungal species were recorded while at Aurangabad 31 were recorded. Most of the fungal species are organic matter decomposers, while some of them are known to cause allergies in humans and also cause plant diseases.Aspergillus species were dominant. BothA. fumigatus (causing allergy and asthma) andA. flavus (producing aflatoxin) were the dominant species and they showed a definite trend in their occurrence. This was related to wind velocity and temperature changes in the atmosphere.     

Hierarchy of sun,beach slope,and landmarks as cues for Y-axis orientation of the supratidal amphipod Talorchestia longicornis (Say)

The semi-terrestrial amphipod Talorchestia longicornis (Say) undergoes Y-axis orientation and has a hierarchy among orientation cues. A previous study found that they used sun compass orientation and moved in the onshore direction of the home beach in both air and water. The present study determined whether this species could also use local landmarks and beach slope as orientation cues. They oriented upslope in simulated darkness in the laboratory on both dry and wet sand with threshold slopes of 2° and 4°, respectively. When tested outside in an arena in air on wet sand, they were disoriented when sun, slope, and landmarks were absent as cues. If presented with single cues, they moved upslope, toward landmarks and in the up-beach direction of the home beach during sun compass orientation. Using paired cues, sun was dominant over slope and landmarks, while slope was dominant over landmarks. In the presence of all three cues, amphipods displayed sun compass orientation in all test combinations except when slope and landmarks were paired together against the sun, which evoked a bimodal response. Thus, the hierarchy of cues for up-beach movement of T. longicornis during Y-axis orientation is the sun, then the slope, and finally the landmarks.     

Multiple sources of celestial compass information in the Central Australian desert ant Melophorus bagoti

The Central Australian desert ant Melophorus bagoti is known to use celestial cues for compass orientation. We manipulated the available celestial cues for compass orientation for ants that had arrived at a feeder, were captured and then released at a distant test site that had no useful terrestrial panoramic cues. When tested in an enclosed transparent box that blocked some or most of the ultraviolet light, the ants were still well oriented homewards. The ants were again significantly oriented homewards when most of the ultraviolet light as well as the sun was blocked, or when the box was covered with tracing paper that eliminated the pattern of polarised light, although in the latter case, their headings were more scattered than in control (full-cue) conditions. When the position of the sun was reflected 180° by a mirror, the ants headed off in an intermediate direction between the dictates of the sun and the dictates of unrotated cues. We conclude that M. bagoti uses all available celestial compass cues, including the pattern of polarised light, the position of the sun, and spectral and intensity gradients. They average multiple cues in a weighted fashion when these cues conflict.     

Integration of polarization and chromatic cues in the insect sky compass

Animals relying on a celestial compass for spatial orientation may use the position of the sun, the chromatic or intensity gradient of the sky, the polarization pattern of the sky, or a combination of these cues as compass signals. Behavioral experiments in bees and ants, indeed, showed that direct sunlight and sky polarization play a role in sky compass orientation, but the relative importance of these cues are species-specific. Intracellular recordings from polarization-sensitive interneurons in the desert locust and monarch butterfly suggest that inputs from different eye regions, including polarized-light input through the dorsal rim area of the eye and chromatic/intensity gradient input from the main eye, are combined at the level of the medulla to create a robust compass signal. Conflicting input from the polarization and chromatic/intensity channel, resulting from eccentric receptive fields, is eliminated at the level of the anterior optic tubercle and central complex through internal compensation for changing solar elevations, which requires input from a circadian clock. Across several species, the central complex likely serves as an internal sky compass, combining E-vector information with other celestial cues. Descending neurons, likewise, respond both to zenithal polarization and to unpolarized cues in an azimuth-dependent way.     

The role of the sun in the celestial compass of dung beetles

Recent research has focused on the different types of compass cues available to ball-rolling beetles for orientation, but little is known about the relative precision of each of these cues and how they interact. In this study, we find that the absolute orientation error of the celestial compass of the day-active dung beetle Scarabaeus lamarcki doubles from 16° at solar elevations below 60° to an error of 29° at solar elevations above 75°. As ball-rolling dung beetles rely solely on celestial compass cues for their orientation, these insects experience a large decrease in orientation precision towards the middle of the day. We also find that in the compass system of dung beetles, the solar cues and the skylight cues are used together and share the control of orientation behaviour. Finally, we demonstrate that the relative influence of the azimuthal position of the sun for straight-line orientation decreases as the sun draws closer to the horizon. In conclusion, ball-rolling dung beetles possess a dynamic celestial compass system in which the orientation precision and the relative influence of the solar compass cues change over the course of the day.     

Effect of solar eclipse on the behavior of a captive group of chimpanzees (Pan troglodytes)

A captive group of chimpanzees, housed in an outdoor compound at the Yerkes Regional Primate Research Center, was observed during the annular solar eclipse of May 30, 1984. The behavior of each animal was recorded using an instantaneous scan-sampling technique (Altmann: Behaviour 49:227–265, 1974). Beginning 2 days prior to the eclipse and continuing through the day following the eclipse, data were collected from 1100 to 1300 hours daily. At 1214 hours on the day of the eclipse, when the sky began to darken and the temperature began to decrease, solitary females and females with infants moved to the top of a climbing structure. As the eclipse progressed, additional chimpanzees began to congregate on the climbing structure and to orient their bodies in the direction of the sun and moon. At 1223 hours, during the period of maximum eclipse, the animals continued to orient their bodies toward the sun and moon and to turn their faces upward. One juvenile stood upright and gestured in the direction of the sun and moon. Sunlight began to increase at 1225 hours, and as it became brighter, the animals began to descend from the climbing structure. The behaviors exhibited by the group during the period of maximum eclipse were not observed prior to or following the eclipse nor as darkness approached at normal, daily sunset. These data indicate that a solar eclipse, a rare and uncommon environmental event, can influence and modulate the behavior of chimpanzees.     

Magnetic versus celestial cues: cue-conflict experiments with migrating silvereyes at dusk

To assess the relative importance of celestial and magnetic cues for orientation at dusk, Australian silvereyes, Zosterops l. lateralis, were subjected to artificial magnetic fields under the natural evening sky, beginning 30 min before sunset. Control birds tested in the local geomagnetic field preferred their normal south-southwesterly migratory direction. Birds tested in a magnetic field with north deflected counterclockwise to 240°WSW showed northeasterly tendencies from the first test onward. Birds subjected to a corresponding clockwise deflection to 120°ESE, in contrast, first showed southerly directions, but from the 7th test onward shifted towards the northwest. Hence, both experimental groups followed the shift in magnetic north, one immediately, the other after a delay. When the birds were later tested in a vertical magnetic field without directional information, the two experimental groups continued in the direction they had preferred in the artificial magnetic fields, presumably by celestial cues alone. This indicates that they had not simply ignored celestial cues, but had recalibrated them according to the altered magnetic fields. The reasons for the initial difference between the two experimental groups remain unclear. Delayed responses to deflections of magnetic north have also been observed in previous studies. They appear to be the main reason why studies that expose birds only once to a cue-conflict situation often seem to indicate a dominance of celestial cues, whereas studies exposing the birds repeatedly usually indicate a dominance of magnetic cues. Accepted: 17 September 1997     

Mechanisms of dance orientation in the Asian honey beeApis florea L.

Summary Early studies of dance communication inApis florea had shown that waggle dances are not performed on a vertical plane and oriented to gravity, as in the other species ofApis, but instead take place on the flattened top of the exposed comb and are oriented to celestial cues directly. More recent experiments showed thatA. florea can dance in the absence of a view of the sun or blue sky, but did not establish what mechanism permitted this orientation. I now report that dances can be oriented directly to landmarks visible from the nest, the first evidence of an environmental feature other than celestial cues or gravity being involved in dance orientation. Landmarks near the nest are probably used to refer to celestial cues, in a fashion analogous to the use of broad features of the landscape by honeybees in order to learn the sun's course, which permits them to determine their flight angle on overcast days or at night, and to compensate accurately for solar movement.Apis florea may therefore be able to learn the sun's course with respect to two sets of landmarks.In other experiments I have examined the influence of slope onA. florea's dance orientation to visual references. In the first extensive observations of its dances on a vertical plane, I have amply confirmed that this species cannot transpose light and gravity in setting its dance angle, as the other species ofApis can. Nor do dancers orient so as to match visual information seen during the dance with that remembered from the flight. Patterns in the data when the same patch of sky was presented from different angles suggest instead thatA. florea continues to orient to projections of celestial cues onto the horizontal plane even when dancing on a steep slope. This compensation for slope may involve an ability to detect gravity and factor it out in aligning the dance to celestial cues.These insights suggest thatA. florea's dance orientation system has been adapted to requirements imposed by its nesting behavior, and has diverged sharply from the system shared by the other species ofApis.     

昆虫定向机制研究进展

许多昆虫具有定向运动的行为。对部分社会性昆虫和迁飞性昆虫定向行为的大量研究已经初步阐明太阳、地磁场、天体、风及地面标志物等都可能成为昆虫返巢和迁飞定向的线索。社会性昆虫具有对不同定向线索进行整合而实现精确导航的能力。日间迁飞性昆虫利用时间补偿太阳罗盘进行定向的机制亦已明确,但夜间迁飞昆虫的定向机制尚需深入研究。迁飞性害虫定向机制的明确将有助于判断害虫迁飞路径及降落区域,为迁飞害虫的准确预测提供科学依据。本文对昆虫的定向机制研究进展进行了综述。     

Behavioural and physiological mechanisms of polarized light sensitivity in birds

Polarized light (PL) sensitivity is relatively well studied in a large number of invertebrates and some fish species, but in most other vertebrate classes, including birds, the behavioural and physiological mechanism of PL sensitivity remains one of the big mysteries in sensory biology. Many organisms use the skylight polarization pattern as part of a sun compass for orientation, navigation and in spatial orientation tasks. In birds, the available evidence for an involvement of the skylight polarization pattern in sun-compass orientation is very weak. Instead, cue-conflict and cue-calibration experiments have shown that the skylight polarization pattern near the horizon at sunrise and sunset provides birds with a seasonally and latitudinally independent compass calibration reference. Despite convincing evidence that birds use PL cues for orientation, direct experimental evidence for PL sensitivity is still lacking. Avian double cones have been proposed as putative PL receptors, but detailed anatomical and physiological evidence will be needed to conclusively describe the avian PL receptor. Intriguing parallels between the functional and physiological properties of PL reception and light-dependent magnetoreception could point to a common receptor system.     

Mechanisms of dusk orientation in white-throated sparrows (Zonotrichia albicollis): Clock-shift experiments

Summary Several species of night migrating birds, especially North American emberizines, exhibit markedly different orientation behaviour when tested in circular cages under clear skies at dusk as compared with tests performed after complete darkness. During the period between sunset and the first appearance of stars, birds tend to show high levels of well-oriented hopping; birds deprived of exposure to clear skies at dusk hop less and their activity is usually not oriented. There is evidence that visual cues available during the dusk period, but not later, are responsible for this difference, but details of the orientation mechanisms involved are unclear. We performed 3-h fast and slow clock shifts on white-throated sparrows (Zonotrichia albicollis) to address two questions concerning migratory orientation at dusk: (1) Is the better orientation of sparrows tested at dusk a function of the visual cues available at that time, or does it result from circadian changes in motivation?; and (2) Is the dusk orientation based on a time-compensated sun compass?Sparrows subjected to a 3-h slow clock shift were tested with controls on clear, moonless nights beginning immediately after lights-off in the clock shift room and thus about 3.5 h after local sunset. Individuals of both groups performed poorly oriented hopping typical of tests performed after complete darkness. The pooled data from each group were not significantly oriented. These results show that the visual cues available shortly after sunset, not temporal changes in the motivation of the birds, are responsible for the qualitative differences in orientation.Birds exposed to a 3-h fast clock shift were tested with controls on clear evenings between sunset and the first appearance of stars. Both groups showed well-oriented hopping. The mean direction of the pooled tests of controls was 325°, a typical spring orientation direction for this species. The mean direction of the pooled tests of the clock shifted birds (274°) was significantly different from that of controls and the 51° counterclockwise shift is consistent with that predicted by a time-compensated sun compass model.     

Orientation of males of sorghum midge,Contarinia sorghicola to sex pheromones from virgin females in the field

The orientation of males of the sorghum midge,Contarinia sorghicola Coq. (Diptera: Cecidomyiidae) towards virgin female baited sticky traps was studied in the field. Male response increased linearly with an increase in the number of virgin females in the sticky traps. Five females per vial were optimum for monitoring midge populations in the field. Numbers of males trapped were significantly greater in traps placed at 0.5 and 1.5 m above ground level compared with those placed at 2.5 m. Peak trap catches occurred at 0900 h. The number of males trapped decreased significantly after 1400 h; male catches continued till sunset. Trap catches followed the same pattern as the number of ovipositing females on sorghum panicles at the half-anthesis stage. Midge activity decreased with an increase in temperature and a decrease in relative humidity. Peak midge density was observed during the second fortnight of October in the rainy season and during February-March in the post-rainy season. Sex pheromones can be used to monitor midge population dynamics for integrated pest management and to screen for host plant resistance to this insect.     

Das Orientierungssystem der V?gel I. Kompa?mechanismen

Zusammenfassung V?gel stellen den Bezug zum Ziel indirekt über ein externes Referenzsystem her. Der Navigationsproze? besteht deshalb aus zwei Schritten: zun?chst wird die Richtung zum Ziel als Kompa?kurs festgelegt, dann wird dieser Kurs mit Hilfe eines Kompa?mechanismus aufgesucht. Das Magnetfeld der Erde und Himmelsfaktoren werden von den V?gel als Kompa? benutzt. In der vorliegenden Arbeit werden der Magnetkompa?, der Sonnenkompa? und der Sternkompa? der V?gel in ihrer Funktionsweise, ihrer Entstehung und ihrer biologischen Bedeutung vorgestellt. Der Magnetkompa? erwies sich als Inklinationskompa?, der nicht auf der Polarit?t, sondern auf der Neigung der Feldlinien im Raum beruht; er unterscheidet „polw?rts“ und „?quatorw?rts“ statt Nord und Süd. Er ist ein angeborener Mechanismus und wird beim Vogelzug und beim Heimfinden benutzt. Seine eigentliche Bedeutung liegt jedoch darin, da? er ein Referenzsystem bereitstellt, mit dessen Hilfe andere Orientierungsfaktoren zueinander in Beziehung gesetzt werden k?nnen. Der Sonnenkompa? beruht auf Erfahrung; Sonnenazimut, Tageszeit und Richtung werden durch Lernprozesse miteinander verknüpft, wobei der Magnetkompa? als Richtungsreferenzsystem dient. Sobald er verfügbar ist, wird der Sonnenkompa? bei der Orientierung im Heimbereich und beim Heimfinden bevorzugt benutzt; beim Vogelzug spielt er, wahrscheinlich wegen seiner Abh?ngigkeit von der geographischen Breite, kaum eine Rolle. Der Sternkompa? arbeitet ohne Beteiligung der Inneren Uhr; die V?gel leiten Richtungen aus den Konfigurationen der Sterne zueinander ab. Lernprozesse erstellen den Sternkompa? in der Phase vor dem ersten Zug; dabei fungiert die Himmelsrotation als Referenzsystem. Sp?ter, w?hrend des Zuges, übernimmt der Magnetkompa? diese Rolle. Die relative Bedeutung der verschiedenen Kompa?systeme wurde in Versuchen untersucht, bei denen Magnetfeld und Himmelsfaktoren einander widersprechende Richtungs-information gaben. Die erste Reaktion der V?gel war von Art zu Art verschieden; langfristig scheinen sich die V?gel jedoch nach dem Magnetkompa? zu richten. Dabei werden die Himmelsfaktoren umgeeicht, so da? magnetische Information und Himmelsinformation wieder im Einklang stehen. Der Magnetkompa? und die Himmelsfaktoren erg?nzen einander: der Magnetkompa? ersetzt Sonnen- und Sternkompa? bei bedecktem Himmel; die Himmelsfaktoren erleichtern den V?geln das Richtungseinhalten, zu dem der Magnetkompa? offenbar wenig geeignet ist. Magnetfeld und Himmelsfaktoren sollten deshalb als integrierte Komponenten eines multifaktoriellen Systems zur Richtungsorientierung betrachtet werden.

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The orientation system of birds — I. Compass mechanisms

Summary Because of the large distances involved, birds establish contact with their goal indirectly via an external reference. Hence any navigation is a two-step process: in the first step, the direction to the goal is determined as a compass course; in the second step, this course is located with a compass. The geomagnetic field and celestial cues provide birds with compass information. The magnetic compass of birds, the sun compass the star compass and the interactions between the compass mechanisms are described in the present paper. Magnetic compass orientation was first demonstrated by testing night-migrating birds in experimentally altered magnetic fields: the birds changed their directional tendencies according to the deflected North direction. The avian magnetic compass proved to be an inclination compass: it does not use polarity; instead it is based on the axial course of the field lines and their inclination in space, distinguishing “poleward” and “equatorward” rather than North and South. Its functional range is limited to intensities around the local field strength, but this biological window is flexible and can be adjusted to other intensities. The magnetic compass is an innate mechanism that is widely used in bird migration and in homing. Its most important role, however, is that of a basic reference system for calibrating other kinds of orientation cues. Sun compass orientation is demonstrated by clock-shift experiments: Shifting the birds' internal clock causes them to misjudge the position of the sun, thus leading to typical deflections which indicate sun compass use. The analysis of the avian sun compass revealed that it is based only on sun azimuth and the internal clock; the sun's altitude is not involved. The role of the pattern of polarized light associated with the sun is unclear; only at sunset has it been shown to be an important cue for nocturnal migrants, being part of the sun compass. The sun compass is based on experience; sun azimuth, time of day and direction are combined by learning processes during a sensitive period, with the magnetic compass serving as directional reference. When established, the sun compass becomes the preferred compass mechanism for orientation tasks within the home region and homing: in migration, however, its role is minimal, probably because of the changes of the sun's arc with geographic latitude. The star compass was demonstrated in night-migrating birds by projecting the northern stars in different directions in a planetarium. The analysis of the mechanism revealed that the internal clock is not involved; birds derive directions from the spatial relationship of the star configurations. The star compass is also established by experience; the directional reference is first provided by celestial rotation, later, during migration, by the magnetic compass. The relative importance of the various compass mechanisms has been tested in experiments in which celestial and magnetic cues gave conflicting information. The first response of birds to conflicting cues differs considerably between species; after repeated exposures, however, the birds oriented according to magnetic North, indicating a long-term dominance of the magnetic compass. Later tests in the absence of magnetic information showed that celestial cues were not simply ignored, but recalibrated so that they were again in agreement with magnetic cues. The magnetic compass and celestial cues complement each other: the magnetic field ensures orientation under overcast sky; celestial cues facilitate maintaining directions, for which the magnetic compass appears to be ill suited. In view of this, the magnetic field and celestial cues should be regarded as integrated components of a multifactorial system for directional orientation.

     

Coding of azimuthal directions via time-compensated combination of celestial compass cues

Many animals use the sun as a reference for spatial orientation [1-3]. In addition to sun position, the sky provides two other sources of directional information, a color gradient [4] and a polarization pattern [5]. Work on insects has predominantly focused on celestial polarization as an orientation cue [6, 7]. Relying on sky polarization alone, however, poses the following two problems: E vector orientations in the sky are not suited to distinguish between the solar and antisolar hemisphere of the sky, and the polarization pattern changes with changing solar elevation during the day [8, 9]. Here, we present neurons that overcome both problems in a locust's brain. The spiking activity of these neurons depends (1) on the E vector orientation of dorsally presented polarized light, (2) on the azimuthal, i.e., horizontal, direction, and (3) on the wavelength of an unpolarized light source. Their tuning to these stimuli matches the distribution of a UV/green chromatic contrast as well as the polarization of natural skylight and compensates for changes in solar elevation during the day. The neurons are, therefore, suited to code for solar azimuth by concurrent combination of signals from the spectral gradient, intensity gradient, and polarization pattern of the sky.     

Sunset and the orientation of European robins (Erithacus rubecula)

The migratory orientation of European robins (Erithacus rubecula) in autumn was tested immediately after sunset and also after the beginning of astronomical darkness. In twilight tests under clear skies, the birds selected an appropriate migratory direction. During the course of autumn, along with the shift of sunset azimuth, the orientation of birds also shifted, always in a counter-clockwise direction. Although this shift of orientation was not statistically significant, the difference between the mean direction and the sunset was the same for each autumn period. This suggests that the migratory direction was selected on the basis of menotactic orientation re the setting sun. Random directions were observed under solid overcast skies as well as during tests under starry skies, begun after all trace of the sunset position had disappeared.     

How dim is dim? Precision of the celestial compass in moonlight and sunlight

Prominent in the sky, but not visible to humans, is a pattern of polarized skylight formed around both the Sun and the Moon. Dung beetles are, at present, the only animal group known to use the much dimmer polarization pattern formed around the Moon as a compass cue for maintaining travel direction. However, the Moon is not visible every night and the intensity of the celestial polarization pattern gradually declines as the Moon wanes. Therefore, for nocturnal orientation on all moonlit nights, the absolute sensitivity of the dung beetle's polarization detector may limit the precision of this behaviour. To test this, we studied the straight-line foraging behaviour of the nocturnal ball-rolling dung beetle Scarabaeus satyrus to establish when the Moon is too dim--and the polarization pattern too weak--to provide a reliable cue for orientation. Our results show that celestial orientation is as accurate during crescent Moon as it is during full Moon. Moreover, this orientation accuracy is equal to that measured for diurnal species that orient under the 100 million times brighter polarization pattern formed around the Sun. This indicates that, in nocturnal species, the sensitivity of the optical polarization compass can be greatly increased without any loss of precision.     

Reed warbler orientation: initiation of nocturnal migratory flights in relation to visibility of celestial cues at dusk

We used radiotelemetry to investigate the time of migratory flight initiation relative to available celestial orientation cues and departure direction of a nocturnal passerine migrant, the reed warbler, Acrocephalus scirpaceus, during autumn migration. The study was carried out at Falsterbo, a coastal site in southwest Sweden. The warblers initiated migration from times well after local sunset and well into the night, corresponding to sun elevations between -4 degrees and -35 degrees, coinciding with the occurrence of stars at night. They departed in the expected migratory direction towards south of southwest with a few initiating migration in reverse directions towards northeast to east. Flight directions under overcast conditions (7-8/8) were more scattered than under clear sky conditions (0-4/8). There were fewer clouds on departure nights than on nights when the birds did not initiate migration. For birds staying longer than one night at stopover the horizontal visibility was higher and precipitation was less likely on departure nights than on the previous night. The results show that the visibility of celestial cues, and stars in particular, are important for the decision to initiate migration in reed warblers. However, cloud cover, horizontal visibility and precipitation might be correlated with other weather variables (i.e. wind or air pressure) that are also likely to be important for the decision to migrate. Copyright 2001 The Association for the Study of Animal Behaviour.