| Literature DB >> 34782664 |
Szymon Smoliński1, Aleksandra Langowska2, Adam Glazaczow3.
Abstract
Varroa destructor is the main pest of the honey bee Apis mellifera, causing colony losses. We investigated the effect of temperature on the autumn abundance of V. destructor in bee colonies over 1991-2020 in Central Europe. We tested the hypothesis that temperature can affect autumn mite populations with different time-lags modulating the bee abundance and brood availability. We showed that raised spring (March-May) and autumn (October) temperatures reinforce autumn V. destructor infestation in the bee colonies. The critical temperature signals embrace periods of bee activity, i.e., just after the first cleansing flights and just before the last observed bee flights, but no direct effects of phenological changes on V. destructor abundance were found. These effects were potentially associated with increased bee reproduction in the specific periods of the year and not with the extended period of activity or accelerated spring onset. We found significant effects of autumn bee abundance, autumn capped brood abundance, and the number of colonies merged on autumn mite infestation. We also observed differences in V. destructor abundance between bees derived from different subspecies. We indicated that climatic effects, through influence on the bee abundance and brood availability, are one of the main drivers regulating V. destructor abundance.Entities:
Mesh:
Year: 2021 PMID: 34782664 PMCID: PMC8593171 DOI: 10.1038/s41598-021-01369-1
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
List of variables used in the modelling of the autumn V. destructor abundance in the A. mellifera colony. The type of the variable, detailed description and proposed hypotheses are specified.
| Variable (abbreviation) | Description | Hypothesis |
|---|---|---|
| Response, continuous (No. individuals) | – | |
| Bee abundance in autumn (BA) | Fixed, continuous (No. frames) | Mite abundance increases with adult bee abundance[ |
| Capped brood in autumn (CB) | Fixed, continuous (No. frames) | Mite abundance increases with bee brood availability[ |
| Number of colonies merged (NC) | Fixed, continuous (No. colonies) | Mite abundance can be influenced, through “reinfestation”[ |
| Spring swarming (SS) | Fixed, factor (yes:1 or no:0) | Colony fission does not lower |
| Type of bees (TB) | Fixed, factor (3 levels: derived from Carniolan, Caucasian or Buckfast honey bees) | Mite abundance can be dependent on the type-specific factors acting directly, e.g. the attractiveness of the brood, grooming or hygienic behaviour[ |
| Age of queen (AQ) | Fixed, factor (3 levels: 1, 2, 3) | Mite abundance can be indirectly affected by the reproductive potential of the honey bee colony depending negatively upon the age of the queen[ |
| Year (YE) | Random, factor (22 levels) | Mite abundance can show interannual variation due to the external environmental drivers and repeated measurements in a year can be internally correlated |
| Temperature (TE) | Fixed, continuous (°C) | Mite abundance increases with a decrease of temperature—within a certain range—during reproduction of mites[ |
| First spring cleansing fligts (SP) | Fixed, continuous (Julian days) | Earlier spring cleansing flights extend the period of activity of bees, therefore can extend the brood-rearing period and availability of brood[ |
| Last autumn flights (AU) | Fixed, continuous (Julian days) | Later last autumn flights extend the period of activity of bees, therefore can extend the brood-rearing period and availability of brood[ |
| Number of active days of bees (DA) | Fixed, continuous (number of days) | Period of activity of bees extends the brood-rearing period and availability of brood[ |
Parameter estimates of the baseline, temperature, and final model for V. destructor abundance. Estimates are given for all fixed effects with standard errors (SE). For the random effects residual variance (σ), the variance associated with tested effects (τ), and intraclass correlation coefficient (ICC) are given. Fixed effects of the final model were selected based on the AICc comparisons. Abbreviations of predictors are given in Table 1. TE is an optimal and TE2 is a suboptimal temperature signal. The number of observations used to fit the models was N = 206 and number of years NYEAR = 22.
| Predictors | Baseline model | Temperature model | Final model | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Estimates | SE | p | Estimates | SE | p | Estimates | SE | p | |
| Intercept | − 3.39 | 5.77 | 0.557 | − 73.10 | 24.12 | − 72.69 | 23.86 | ||
| BA | 4.10 | 0.90 | 4.21 | 0.89 | 4.31 | 0.86 | |||
| CB | 1.50 | 0.68 | 1.63 | 0.69 | 1.51 | 0.67 | |||
| NC | 2.07 | 0.83 | 1.93 | 0.83 | 1.67 | 0.81 | |||
| SS [1] | 0.29 | 2.05 | 0.889 | 0.47 | 2.05 | 0.817 | |||
| TB [Caucasian] | − 6.96 | 3.71 | 0.061 | − 6.96 | 3.70 | 0.060 | − 7.63 | 3.68 | |
| TB [Carniolan] | − 2.43 | 1.78 | 0.171 | − 2.37 | 1.77 | 0.181 | − 2.99 | 1.73 | 0.084 |
| AQ [2] | 2.98 | 1.93 | 0.121 | 2.86 | 1.92 | 0.137 | |||
| AQ [3] | 4.98 | 5.38 | 0.355 | 4.57 | 5.38 | 0.395 | |||
| TE | 4.77 | 2.22 | 4.87 | 2.19 | |||||
| TE2 | 2.87 | 1.50 | 0.055 | 2.87 | 1.48 | 0.052 | |||
| σ2 | 100.71 | 100.59 | 100.68 | ||||||
| τYEAR | 140.45 | 101.51 | 98.80 | ||||||
| ICC | 0.58 | 0.50 | 0.50 | ||||||
| Marginal R2/conditional R2 | 0.131/0.637 | 0.287/0.645 | 0.288/0.640 | ||||||
Figure 1Predicted interannual variation in the V. destructor abundance. Estimates of the baseline model for the random effect of the year were used. Shaded areas indicate standard errors of the estimates.
Figure 2Results of the sliding window analysis indicating optimal and suboptimal signals of the temperature for the prediction of the autumn V. destructor abundance. Colour gradient indicate AICc changes in relation to the baseline model (lower AICc indicates a better model), black boxes show identified optimal and suboptimal signals, vertical grey lines indicate the multi-year average date of first spring cleansing flights (dashed) and last autumn flights (dotted). Notice that average March–May temperature obtained lower AICc than averages from single months (AICc for March–May temperature is indicated in the upper part of the rectangle that shows optimal signal).
Figure 3Spatial correlation between estimates of random effects of year and air temperature in the identified critical time windows: March–May (a) and October (b). Locations of the bee colony are indicated with points. Only cells with significant correlations (p < 0.1) are presented.
Figure 4Predicted effect of (a) autumn bee abundance; (b) autumn capped brood abundance; (c) number of colonies merged; (d) type of bees; (e) identified signal of spring temperature; (f) identified signal of autumn temperature on V. destructor abundance. Confidence intervals are indicated with shaded areas and bars.
Figure 5Phenology of the first spring cleansing flights (a) and last autumn flights (b) of the bees in relation to the temperature conditions during the first (a) and the second (b) critical time windows.