| Literature DB >> 32948798 |
Rodolfo Liporoni1, Guaraci Duran Cordeiro2, Paulo Inácio Prado3, Clemens Schlindwein4, Eric James Warrant5, Isabel Alves-Dos-Santos3.
Abstract
The foraging activity of diurnal bees often relies on flower availability, light intensity and temperature. We do not know how nocturnal bees, which fly at night and twilight, cope with these factors, especially as light levels vary considerably from night to day and from night to night due to moon phase and cloud cover. Given that bee apposition compound eyes function at their limits in dim light, we expect a strong dependence of foraging activity on light intensity in nocturnal bees. Besides being limited by minimum light levels to forage, nocturnal bees should also avoid foraging at brighter intensities, which bring increased competition with other bees. We investigated how five factors (light intensity, flower availability, temperature, humidity, and wind) affect flower visitation by Neotropical nocturnal bees in cambuci (Campomanesia phaea, Myrtaceae). We counted visits per minute over 30 nights in 33 cambuci trees. Light intensity was the main variable explaining flower visitation of nocturnal bees, which peaked at intermediate light levels occurring 25 min before sunrise. The minimum light intensity threshold to visit flowers was 0.00024 cd/m2. Our results highlight the dependence of these nocturnal insects on adequate light levels to explore resources.Entities:
Year: 2020 PMID: 32948798 PMCID: PMC7501267 DOI: 10.1038/s41598-020-72047-x
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Nocturnal bee species that visit flowers of cambuci (Campomanesia phaea, Myrtaceae) in south-eastern Brazil. (A) Ptiloglossa latecalcarata (Colletidae), (B) Ptiloglossa sp. (Colletidae), (C) Megalopta sodalis (Halictidae), (D) Megommation insigne (Halictidae).
Visitation rate (mean ± SD) of five nocturnal bee species foraging in a commercial cambuci (Campomanesia phaea, Myrtaceae) orchard surrounded by secondary Atlantic forest fragments in Mogi das Cruzes, São Paulo State, Brazil.
| Bee family | Bee species | Visitation rate (× 10–2 visits/flower/min) | |
|---|---|---|---|
| Colletidae | 1.90 ± 6.12 | ||
| 0.03 ± 0.66 | |||
| 0.002 ± 0.15 | |||
| Halictidae | 0.03 ± 0.51 | ||
| 0.17 ± 1.39 | |||
| Total | 2.13 ± 6.46 | ||
Figure 2Visitation rate (visits/flower/min) by nocturnal bees on cambuci flowers and light intensity variation during twilight and for 30 min after sunrise. Black dots are average visitation rate values and black bars are standard errors of the mean (n = 30 twilight periods). The coloured curve represents mean light intensity for each minute during twilight and the shaded area the relative errors (n = 30 twilight periods). Background colours represent true night (dark grey), twilight (light grey) and daytime (white). The vertical dashed line approximately marks mid-twilight. Sunrise time (0 in the time axis) varied between 6:29 h on the first sampled twilight (17 Oct 2017) to 6:09 h on the last twilight (24 Nov 2017).
Model selection for factors affecting foraging activity of nocturnal bees, using generalized linear mixed models (GLMMs) with Poisson distribution.
| Models | logLikelihood | AICc | ∆AICc | DF | Weight |
|---|---|---|---|---|---|
| Light + light2 + all other variables | − 3,645.5 | 7,309.1 | 0.0 | 9 | 1 |
| Light + all other variables | − 4,379.6 | 8,775.1 | 1,466.1 | 8 | < 0.001 |
| All variables, except light | − 4,381.0 | 8,775.9 | 1,466.9 | 7 | < 0.001 |
| No fixed effects (null) | − 4,670.4 | 9,342.7 | 2033.6 | 1 | < 0.001 |
AICc corrected Akaike information criterion, DF degrees of freedom.
The response variable was the number of visits per minute, using the number of observed flowers as model offset. The best model includes all environmental variables (light intensity, air temperature, relative air humidity, maximum wind speed, orchard flower abundance) with a quadratic term for light intensity.
Figure 3Distribution of visitation rate (visits/flower/min) by nocturnal bees on cambuci flowers during twilight as a function of light intensity measured as luminance (cd/m2). Boxes delimit where 50% of the values for each light interval are concentrated, horizontal lines indicate the median (all of them are zero), and dots represent outliers. The red curve represents the predicted visitation rate by the best supported model, which includes a quadratic term for the light effect. The 95% confidence interval of predicted values is shown in light grey.
Figure 4The activity durations of nocturnal bees foraging on cambuci flowers measured during twilight periods over five weeks. Each horizontal line represents the time interval during which bees visited cambuci during each twilight period. Line colours indicate average light intensity—measured as the average luminance of an 18% grey card (cd/m2) during the first half of the twilight when light levels varied considerably between twilight periods (see this variation in Fig. S1). Grey horizontal lines are nights with missing light intensity data from the first half of the twilight. Circles at left represent moon phases (new moon = black circle; full moon = white circle). Other plot conventions as in Fig. 2.