| Literature DB >> 36188521 |
Robert J Thomas1,2, Stephen P Davison3.
Abstract
Bat abundance, diversity, and behavior can be monitored by capturing bats for identification and measurement in the hand, but this has several disadvantages. These include disturbance to the bats, which limits the frequency with which captures can be made at an individual capture site, and potentially alters the behaviors being studied. Infrared video monitoring, passive acoustic recording and automated analysis and identification of bat calls offers an alternative set of noninvasive methods for monitoring bats. In this study, we examine the effectiveness of acoustic monitoring in comparison with capture-based and video monitoring of seasonal swarming behavior among several species of Myotis bats in southern Britain. We applied these complementary approaches to describe seasonal, overnight, and species-specific variation in swarming behavior in a multispecies community of Myotis bats. We show that the three monitoring approaches have advantages and disadvantages for different tasks, but can be viewed as highly complementary methods for addressing different types of research questions. In our study of swarming behavior, capture and examination of bats in the hand was necessary for measuring sex ratios, reproductive status, and even for confirmation of species identification for some difficult to separate taxa. Capture is also an essential aspect of tagging bats for individual identification and tracking studies. Video monitoring is useful for understanding the behavior of bats at swarming sites, and measuring the flux of individuals into and out of roosting or swarming sites. Passive acoustic monitoring is a valuable noninvasive method for continuous monitoring of within-night, seasonal, and between-year variation in the abundance of bat calls. These can be used as an index of variation in relative abundance within-but not between-bat species.Entities:
Keywords: acoustic monitoring; bats; myotis; swarming
Year: 2022 PMID: 36188521 PMCID: PMC9502064 DOI: 10.1002/ece3.9344
Source DB: PubMed Journal: Ecol Evol ISSN: 2045-7758 Impact factor: 3.167
FIGURE 2Seasonal variation in the activity of Myotis bats at “Middle Earth” cave in 2018. Panel (a) shows all Myotis species combined, detected as full spectrum sonograms and identified by automated identification to genus level using the Bat Classify software. The smoothed seasonal pattern (fitted using a GAM, effective degrees of freedom = 5) is shown in addition to the raw data. The temperature data shown in panel (b) were obtained from the mouth of the cave at dusk, and the smoothed seasonal pattern (fitted using a GAM, effective degrees of freedom = 5) is shown in addition to the raw data. Seasonal activity patterns of individual taxa are shown in panels (c)–(f); the smoothed seasonal pattern for each taxon (fitted using a GAM, effective degrees of freedom = 5) is shown in addition to the raw data. For all graphs, the upper and lower smoothed dotted lines show ±1 SE, respectively. The GAM analyses for these seasonal variations are shown in Tables A3 and A4.
FIGURE 1Seasonal variation in the activity of Myotis bats (all species combined) at “Hobbit Hole” cave in 2015–2017, measured as the number of zero crossing files, and identified to genus level by visual inspection of the resulting sonograms. Fitted lines show GAM analysis of activity in each year (Table A1). Standard errors not included for the sake of clarity.
A generalized additive model to explain variation in nightly abundance of different taxa of Myotis bats detected at “Hobbit Hole” cave in 2015–17 using automated acoustic monitoring.
| Independent variables | Category | df/edf | Parameter estimate | SE | Test statistic |
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| Intercept | 1 | 2.952 | 0.689 | 4.284 | <.0001 | |
| Year (reference category = 2015) | 2016 | 1 | 0.030 | 0.698 | 0.043 | .966 |
| 2017 | 1 | −0.156 | 0.693 | −0.225 | .822 | |
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| Julian day × 2015 | 18.94 | 278.4 | <.0001 | |||
| Julian day × 2016 | 28.23 | 429.5 | <.0001 | |||
| Julian day × 2017 | 27.29 | 292.2 | <.0001 |
Note: The model used a negative binomial error family (scale = 1) and a log‐link function. Max k = 40. Overdispersion statistic = 1.061, deviance explained = 61.7%. The prediction plot from this model is shown in Figure 1.
Abbreviation: edf, effective degrees of freedom.
FIGURE 4Catches of different Myotis species in 2017–2018. Captures are plotted against calendar date, but in each year, the timing of peak activity was different. Solid lines represent model fitted lines from the GAM model for each taxon described in Table A2 (negative binomial error family, log‐link function, maximum k‐value = 40). Dashed lines represent ±1SE.
A generalized additive model to explain variation in nightly activity of different taxa of Myotis bats (all taxa combined) at Middle Earth cave in 2018.
| Independent variables | Category | df/edf | Parameter estimate | SE | Test statistic |
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| Intercept | 1 | 4.205 | 0.0688 | 61.15 | <.0001 | |
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| Julian day | 23.94 | 785.6 | <.0001 |
Note: The model used a negative binomial error family (scale = 1) and a log‐link function. Max k = 40. Overdispersion statistic = 1.343, deviance explained = 69.6%. The prediction plot from this model is shown in Figure 4, panel (a).
Abbreviation: edf, effective degrees of freedom.
A generalized additive model to explain variation in nightly abundance of different taxa of Myotis bats detected at Middle Earth cave in 2018, using automated acoustic monitoring.
| Independent variables | Category | df/edf | Parameter estimate | SE | Test statistic |
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| Intercept | 1 | 0.322 | 0.107 | 3.019 | .003 | |
| Species (reference category = Bechstein's) | Daubenton's | 1 | 1.985 | 0.131 | 15.199 | <.0001 |
| Natterer's | 1 | 2.640 | 0.138 | 19.113 | <.0001 | |
| Whiskered/Brandt's | 1 | −0.631 | 0.402 | −1.567 | .117 | |
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| Julian day × Bechstein's | 10.17 | 160.7 | <.0001 | |||
| Julian day × Daubenton's | 29.95 | 387.0 | <.0001 | |||
| Julian day × Natterer's | 25.51 | 1153.4 | <.0001 | |||
| Julian day × Whiskered /Brandt's | 26.95 | 151.9 | <.0001 |
Note: The model used a negative binomial error family (scale = 1) and a log‐link function. Max k = 40. Overdispersion statistic = 1.208, deviance explained = 82%. The prediction plot from this model is shown in Figure 4 (panels c–f).
Abbreviation: edf, effective degrees of freedom.
FIGURE 3Hourly activity of different Myotis species across the night, across the 2018 peak swarming period. The vertical lines indicate the changing night lengths throughout the study period, and the colors indicate respective weeks. (a) Overnight distribution of Myotis nattereri calls. (b) Overnight distribution of Myotis daubentonii calls. Vertical lines and colors represent mean time of sunrise during each week of the study period. Fitted lines show GAM analysis for each week throughout the swarming period (Tables A5 and A6). Standard errors are not shown for the sake of clarity.
A generalized additive model to explain variation in hourly abundance of Daubenton's bats, detected at Middle Earth cave in 2018, using automated acoustic monitoring.
| Independent variables | Category | df/edf | Parameter estimate | SE | Test statistic |
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| Intercept | 1 | −0.739 | 0.573 | −1.290 | .197 | |
| Week (reference category = Week 5) | Week 1 | 1 | −0.713 | 0.816 | −0.873 | .383 |
| Week 2 | 1 | +1.565 | 1.035 | 1.512 | .131 | |
| Week 3 | 1 | −0.089 | 0.770 | −0.116 | .908 | |
| Week 4 | 1 | +0.777 | 1.434 | 0.542 | .588 | |
| Week 6 | 1 | +1.499 | 0.613 | 2.446 |
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| Week 7 | 1 | +0.806 | 0.638 | 1.264 | .206 | |
| Week 8 | 1 | −0.897 | 0.835 | −1.074 | .283 | |
| Week 9 | 1 | −2.054 | 1.538 | −1.336 | .182 | |
| Week 10 | 1 | −1.729 | 1.176 | −1.470 | .142 | |
| Week 11 | 1 | −0.993 | 0.948 | −1.047 | .295 | |
| Week 12 | 1 | −0.838 | 0.688 | −1.219 | .223 | |
| Week 13 | 1 | −4.878 | 2.998 | −1.627 | .104 | |
| Week 14 | 1 | −9.841 | 22.635 | −0.435 | .6637 | |
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| Hour × Week 1 | 3.178 | 56.091 | <.0001 | |||
| Hour × Week 2 | 7.232 | 100.614 | <.0001 | |||
| Hour × Week 3 | 3.980 | 68.257 | <.0001 | |||
| Hour × Week 4 | 8.995 | 104.527 | <.0001 | |||
| Hour × Week 5 | 4.330 | 118.014 | <.0001 | |||
| Hour × Week 6 | 3.518 | 109.619 | ||||
| Hour × Week 7 | 4.472 | 105.544 | ||||
| Hour × Week 8 | 6.120 | 34.072 | <.0001 | |||
| Hour × Week 9 | 6.782 | 31.353 | .0001 | |||
| Hour × Week 10 | 6.428 | 26.687 | .0005 | |||
| Hour × Week 11 | 7.620 | 21.382 | .0127 | |||
| Hour × Week 12 | 5.053 | 16.567 | .0178 | |||
| Hour × Week 13 | 3.204 | 10.979 | .0329 | |||
| Hour × Week 14 | 4.809 | 2.988 | .831 |
Note: The model used a negative binomial error family and a log‐link function. The prediction plot from this model is shown in Figure 5a. Max k = 15. Overdispersion statistic = 0.974, deviance explained = 71.6%.
Abbreviation: edf, effective degrees of freedom.
A generalized additive model to explain variation in hourly abundance of Natterer's bats, detected at Middle Earth cave in 2018, using automated acoustic monitoring.
| Independent variables | Category | df/edf | Parameter estimate | SE | Test statistic |
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| Intercept | 1 | 2.5575 | 0.221 | 11.576 | <.0001 | |
| Week (reference category = Week 7) | Week 1 | 1 | −20.058 | 2.230 | −0.393 | .694 |
| Week 2 | 1 | −12.048 | 27.384 | −3.325 | .660 | |
| Week 3 | 1 | −6.223 | 1.872 | −3.325 | .0009 | |
| Week 4 | 1 | −3.967 | 1.193 | −3.326 | .0009 | |
| Week 5 | 1 | −6.387 | 2.230 | −2.865 | .00417 | |
| Week 6 | 1 | −0.473 | 0.340 | −1.393 | .164 | |
| Week 8 | 1 | −0.658 | 0.391 | −1.685 | .092 | |
| Week 9 | 1 | −1.439 | 0.349 | −4.121 | <.0001 | |
| Week 10 | 1 | −0.412 | 0.522 | −0.789 | .430 | |
| Week 11 | 1 | 0.438 | 0.253 | 1.736 | .082 | |
| Week 12 | 1 | 0.153 | 0.256 | 0.597 | .550 | |
| Week 13 | 1 | −1.574 | 0.273 | −5.777 | <.0001 | |
| Week 14 | 1 | −1.744 | 0.277 | −6.302 | <.0001 | |
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| Hour × Week 1 | 4.240 | 2.179 | .754 | |||
| Hour × Week 2 | 7.675 | 24.682 | .0018 | |||
| Hour × Week 3 | 4.042 | 33.654 | <.0001 | |||
| Hour × Week 4 | 5.640 | 111.238 | <.0001 | |||
| Hour × Week 5 | 4.600 | 126.809 | <.0001 | |||
| Hour × Week 6 | 4.874 | 253.107 | <.0001 | |||
| Hour × Week 7 | 6.309 | 265.450 | <.0001 | |||
| Hour × Week 8 | 7.810 | 162.098 | <.0001 | |||
| Hour × Week 9 | 6.160 | 198.349 | <.0001 | |||
| Hour × Week 10 | 10.781 | 140.149 | <.0001 | |||
| Hour × Week 11 | 6.049 | 212.760 | <.0001 | |||
| Hour × Week 12 | 6.561 | 178.182 | <.0001 | |||
| Hour × Week 13 | 5.311 | 127.143 | <.0001 | |||
| Hour × Week 14 | 7.562 | 79.144 | <.0001 |
Note: The model used a negative binomial error family and a log‐link function. The prediction plot from this model is shown in Figure 5b. Max k = 15. Overdispersion statistic = 1.248, deviance explained = 77.2%.
Abbreviation: edf, effective degrees of freedom.
Sex ratios among Myotis bats captured at “Middle Earth” cave and in adjacent woodland in 2017 and 2018, using mist nets and harp traps.
| Species | 2017 | 2018 | Total 2017–18 | Between year sex ratio comparison | ||||||
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| M:F | % Male |
| M:F | % Male |
| M:F | % Male |
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| 19:2 | 90.5 | .006 | 21:5 | 80.8 | .040 | 40:7 | 85.1 | .0004 | .400 |
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| 39:9 | 81.2 | .002 | 62:5 | 92.5 | <.0001 | 101:14 | 87.8 | <.0001 | .090 |
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| 35:11 | 76.1 | .020 | 17:4 | 81.0 | .050 | 52:15 | 77.6 | .001 | .800 |
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| 4:3 | 74.3 | – | 1:0 | 100.0 | – | 5:3 | 62.5 | – | – |
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| 33:5 | 86.8 | .001 | 13:1 | 92.9 | .030 | 46:6 | 88.5 | <.0001 | 1.000 |
Note: Male: female ratios were compared using Fisher's exact test for sex‐ratio bias (null hypothesis of 1:1), and for differences in sex ratio between 2017 and 2018.
Generalized additive models to explain variation in nightly abundance of different taxa of Myotis bats captured at “Middle Earth” cave in 2018.
| Taxon | Independent variables | df/edf | Parameter estimate | SE | Test statistic |
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| (i) Bechstein's bat |
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| Intercept | 1 | 0.982 | 0.159 | 6.175 | <.0001 | |
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| Julian day | 2.421 | 6.529 | .0892 | |||
| (ii) Daubenton's bat |
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| Intercept | 1 | 1.116 | 0.160 | 6.991 | <.0001 | |
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| Julian day | 2.120 | 14.870 | .00133 | |||
| (iii) Natterer's bat |
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| Intercept | 1 | 1.998 | 0.203 | 5.914 | <.0001 | |
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| Julian day | 2.795 | 25.040 | <.0001 | |||
| (iv) Brandt's /Whiskered bat |
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| Intercept | 1 | 1.266 | 0.170 | 7.438 | <.0001 | |
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| Julian day | 2.199 | 0.006 |
Note: Each model used a negative binomial error family (scale = 1) and a log‐link function. Max k = 40.
Bechstein's bat. Overdispersion statistic = 1.907, deviance explained = 15.9%. The prediction plot from this model is shown in Figure 4a.
Daubenton's bat. Overdispersion statistic = 1.922, deviance explained = 26.9%. The prediction plot from this model is shown in Figure 4b.
Natterer's bat. Overdispersion statistic = 1.673, deviance explained = 45.9%. The prediction plot from this model is shown in Figure 4c.
Brandt's/Whiskered bat. Overdispersion statistic = 1.642, deviance explained = 25.5%. The prediction plot from this model is shown in Figure 4d.
Abbreviation: edf, effective degrees of freedom.
FIGURE 5Video‐evidence of bats entering and leaving the focal cave on August 28, 2017, and September 28, 2017, from half an hour before sunset, until 3.5 h after sunset.