| Literature DB >> 32128152 |
Julian Klein1, Paul J Haverkamp2, Eva Lindberg3, Michael Griesser2,4, Sönke Eggers1.
Abstract
Habitat suitability models (HSM) based on remotely sensed data are useful tools in conservation work. However, they typically use species occurrence data rather than robust demographic variables, and their predictive power is rarely evaluated. These shortcomings can result in misleading guidance for conservation. Here, we develop and evaluate a HSM based on correlates of long-term breeding success of an open nest building boreal forest bird, the Siberian jay. In our study site in northern Sweden, nest failure of this permanent resident species is driven mainly by visually hunting corvids that are associated with human settlements. Parents rely on understory nesting cover as protection against these predators. Accordingly, our HSM includes a light detection and ranging (LiDAR) based metric of understory density around the nest and the distance of the nest to the closest human settlement to predict breeding success. It reveals that a high understory density 15-80 m around nests is associated with increased breeding success in territories close to settlements (<1.5 km). Farther away from human settlements breeding success is highest at nest sites with a more open understory providing a favorable warmer microclimate. We validated this HSM by comparing the predicted breeding success with landscape-wide census data on Siberian jay occurrence. The correlation between breeding success and occurrence was strong up to 40 km around the study site. However, the HSM appears to overestimate breeding success in regions with a milder climate and therefore higher corvid numbers. Our findings suggest that maintaining patches of small diameter trees may provide a cost-effective way to restore the breeding habitat for Siberian jays up to 1.5 km from human settlements. This distance is expected to increase in the warmer, southern, and coastal range of the Siberian jay where the presence of other corvids is to a lesser extent restricted to settlements.Entities:
Keywords: LiDAR; Perisoreus infaustus; airborne laser scanning; forest thinning; habitat suitability models; nest predation; understory
Year: 2020 PMID: 32128152 PMCID: PMC7042737 DOI: 10.1002/ece3.6062
Source DB: PubMed Journal: Ecol Evol ISSN: 2045-7758 Impact factor: 2.912
Annual increase in volume on productive stands (>1 m3 ha‐1 yr‐1) in the study site, supporting that ALS data from autumn 2010 were representative for the whole study period (Swedish NFI, 2015)
| Age class | 0–20 | 21–40 | 41–60 | 61–80 | 81–100 | 101–120 | 121+ | Total |
|---|---|---|---|---|---|---|---|---|
| Change in m3/ha | 0.5 | 2.6 | 3.6 | 3.1 | 2.8 | 1.9 | 1.6 | 2.4 |
Figure A1The probability of observing at least one Eurasian jay within 50 m from a Siberian jay nesting site during 26 ± 2 hr observation time. The probability is modeled as a response to the distance of the Siberian jay nest to the closest human settlement. The distance at which the predicted occurrence of Eurasian jays switches from 0 to 1 was 1,316 ± 151 m. The R 2‐value is .63
Corvid nest predators are observed mostly near human settlements during the breeding season of Siberian jays. Thus, their negative effect on Siberian jay breeding success is expected to decrease abruptly at a certain distance from year‐round inhabited human settlements. This creates clearly distinct areas of high and low nest predation risk. In the table below, the results of the categorisation of the distance of the Siberian jay nest to the closest settlement into close (high nest predation risk) and far (low nest predation risk) are shown. We selected this threshold distance according to the lowest AIC value. In order to not have an unbalanced data set, the threshold analysis included 80% of all nests, excluding the 10% closest and 10% furthest away
| Categorisation distance (m) | Estimate |
|
| Pr(>|z|) |
| AICc |
|---|---|---|---|---|---|---|
| 1,450 | 0.95 | 0.33 | 2.93 | 0.003 | 0.047 | 314.82 |
| 1,700 | 0.95 | 0.33 | 2.85 | 0.004 | 0.046 | 315.16 |
| 1,650 | 0.90 | 0.34 | 2.66 | 0.008 | 0.041 | 315.94 |
| 1,500 | 0.88 | 0.32 | 2.74 | 0.006 | 0.041 | 315.97 |
| 2,250 | 1.05 | 0.41 | 2.59 | 0.010 | 0.042 | 316.06 |
| 1,800 | 0.93 | 0.36 | 2.63 | 0.009 | 0.042 | 316.07 |
| 1,750 | 0.92 | 0.35 | 2.62 | 0.009 | 0.042 | 316.09 |
| 1,400 | 0.86 | 0.32 | 2.65 | 0.008 | 0.038 | 316.48 |
| 2,300 | 0.99 | 0.41 | 2.43 | 0.015 | 0.036 | 317.11 |
| 1,850 | 0.87 | 0.36 | 2.43 | 0.015 | 0.035 | 317.29 |
| 1,550 | 0.80 | 0.32 | 2.48 | 0.013 | 0.034 | 317.39 |
| 2,350 | 0.97 | 0.41 | 2.35 | 0.019 | 0.034 | 317.57 |
| 1,350 | 0.79 | 0.32 | 2.45 | 0.014 | 0.032 | 317.59 |
| 1,900 | 0.81 | 0.36 | 2.27 | 0.023 | 0.031 | 318.11 |
| 1,950 | 0.83 | 0.37 | 2.26 | 0.024 | 0.031 | 318.15 |
| 2,450 | 0.96 | 0.44 | 2.21 | 0.027 | 0.030 | 318.27 |
| 2,200 | 0.83 | 0.38 | 2.20 | 0.027 | 0.029 | 318.43 |
| 1,600 | 0.73 | 0.33 | 2.22 | 0.026 | 0.028 | 318.49 |
| 2,500 | 0.94 | 0.44 | 2.12 | 0.034 | 0.028 | 318.71 |
| 2,400 | 0.88 | 0.42 | 2.11 | 0.035 | 0.027 | 318.81 |
| 2,100 | 0.75 | 0.36 | 2.09 | 0.036 | 0.025 | 319.05 |
| 2,150 | 0.75 | 0.36 | 2.08 | 0.038 | 0.025 | 319.07 |
| 1,250 | 0.67 | 0.32 | 2.10 | 0.035 | 0.024 | 319.23 |
| 1,300 | 0.67 | 0.32 | 2.10 | 0.035 | 0.024 | 319.23 |
| 800 | 0.81 | 0.41 | 1.99 | 0.047 | 0.021 | 319.63 |
| 750 | 0.82 | 0.41 | 1.98 | 0.048 | 0.020 | 319.71 |
| 2,050 | 0.68 | 0.36 | 1.88 | 0.060 | 0.020 | 319.98 |
| 2,000 | 0.62 | 0.36 | 1.72 | 0.085 | 0.017 | 320.62 |
| 1,200 | 0.56 | 0.33 | 1.69 | 0.090 | 0.015 | 320.81 |
| 2,550 | 0.69 | 0.42 | 1.63 | 0.104 | 0.015 | 320.87 |
| 550 | 0.76 | 0.47 | 1.61 | 0.108 | 0.013 | 321.10 |
| 650 | 0.67 | 0.43 | 1.54 | 0.124 | 0.012 | 321.32 |
| 700 | 0.67 | 0.43 | 1.54 | 0.124 | 0.012 | 321.32 |
| 600 | 0.66 | 0.45 | 1.47 | 0.141 | 0.011 | 321.53 |
| 2,900 | 0.70 | 0.50 | 1.40 | 0.163 | 0.012 | 321.56 |
| 850 | 0.56 | 0.39 | 1.43 | 0.151 | 0.011 | 321.6 |
| 2,750 | 0.62 | 0.46 | 1.37 | 0.172 | 0.011 | 321.68 |
| 1,000 | 0.47 | 0.35 | 1.37 | 0.172 | 0.010 | 321.80 |
| 900 | 0.49 | 0.37 | 1.34 | 0.182 | 0.009 | 321.88 |
| 1,150 | 0.44 | 0.33 | 1.34 | 0.179 | 0.010 | 321.89 |
| 2,850 | 0.60 | 0.47 | 1.26 | 0.206 | 0.009 | 321.98 |
| 500 | 0.68 | 0.53 | 1.27 | 0.203 | 0.008 | 322.05 |
| 2,800 | 0.56 | 0.46 | 1.22 | 0.223 | 0.009 | 322.09 |
| 950 | 0.43 | 0.36 | 1.19 | 0.232 | 0.008 | 322.23 |
| 2,600 | 0.50 | 0.43 | 1.16 | 0.244 | 0.008 | 322.25 |
| 1,050 | 0.37 | 0.34 | 1.10 | 0.273 | 0.006 | 322.46 |
| 1,100 | 0.35 | 0.34 | 1.05 | 0.294 | 0.006 | 322.56 |
| 2,950 | 0.48 | 0.50 | 0.95 | 0.340 | 0.005 | 322.69 |
| 2,700 | 0.41 | 0.45 | 0.91 | 0.362 | 0.005 | 322.78 |
| 3,300 | 0.42 | 0.51 | 0.83 | 0.404 | 0.004 | 322.92 |
| 3,000 | 0.33 | 0.50 | 0.67 | 0.504 | 0.003 | 323.17 |
| 3,050 | 0.33 | 0.50 | 0.67 | 0.504 | 0.003 | 323.17 |
| 3,100 | 0.33 | 0.50 | 0.67 | 0.504 | 0.003 | 323.17 |
| 3,150 | 0.33 | 0.50 | 0.67 | 0.504 | 0.003 | 323.17 |
| 3,200 | 0.33 | 0.50 | 0.67 | 0.504 | 0.003 | 323.17 |
| 2,650 | 0.28 | 0.45 | 0.63 | 0.531 | 0.002 | 323.23 |
| 3,250 | 0.28 | 0.50 | 0.55 | 0.581 | 0.002 | 323.32 |
| 3,350 | 0.17 | 0.52 | 0.33 | 0.739 | 0.000 | 323.51 |
| 3,400 | 0.17 | 0.52 | 0.33 | 0.739 | 0.000 | 323.51 |
| 3,450 | 0.17 | 0.52 | 0.33 | 0.739 | 0.000 | 323.51 |
| 3,500 | 0.11 | 0.52 | 0.21 | 0.834 | 0.000 | 323.58 |
Summary of the GLMM (binomial error structure, logit link function) with breeding success (0 = failure, 1 = success) as the response and an interaction between the distance of the nest to the closest human settlement and understory density at the nest together with the study area as covariates
| Fixed effects | Estimate |
|
| Pr(>| |
|---|---|---|---|---|
| Intercept | 0.24 | 0.30 | 0.81 | 0.417 |
| Study area (unmanaged) | −0.52 | 0.36 | −1.46 | 0.143 |
| Distance to settlement (close) |
|
|
|
|
| Log(understory density) | 0.40 | 0.31 | 1.30 | 0.194 |
| Distance to settlement (close) × log(understory density) |
|
|
|
|
The year (1998–2013) and individual ID of both breeders were included as random effects. Significant (Pr(>|z|) < 0.05) effects are highlighted in bold (n = 235 nests).
Figure 1The effect of understory density at the nest on breeding success is shown for both high and low distance of the nest to the closest human settlement. The lines show predicted estimates while the ribbons show the standard error of the estimates. Data are back‐transformed for ease of viewing. Marginal and conditional R 2‐values = .10 resp. .18. Values of observed breeding success (0 = failure, 1 = success) of n = 235 nests are jittered to increase the visibility of individual data points
Figure 2The marginal R 2‐values of the model for breeding success with average understory density (ud) at i = nest (15 m) to within radius i = territory border (460 m) around the nest plotted against the correlation of the understory density at radius i, with understory density at the nest (n = 203 nests). The distance of the nest to the closest human settlement in the models for breeding success is the same for all radii. Understory density within radii <80 m has an effect on Siberian jay breeding success
We log‐transformed understory density since we expected that the same absolute change in understory density has a greater effect on breeding success at low understory densities compared to high densities. The results below verify that the model with log‐transformed understory density was more parsimonious than models with quadratic and linear relationships between understory density and breeding success. The table shows the evaluation results for the models with LiDAR data at the nest. Parsimony was measured with Akaike’s information criterion (n = 235 nests)
| Explanatory model | AICc | Delta |
|---|---|---|
| Distance to settlement * log(understory density) + study site | 302.0 | 0 |
| Distance to settlement * understory density + study site | 304.4 | 2.36 |
| Distance to settlement * understory density2 + study site | 305.1 | 3.08 |
| Distance to settlement + study site | 305.3 | 3.22 |
| Intercept | 309.0 | 6.96 |
| Study site | 311.1 | 9.04 |
| Understory density + study site | 312.7 | 10.64 |
We performed a sensitivity analysis of the main results to the categorisation of the distance of the Siberian jay nests to the closest human settlement, to verify that our results are not overly sensitive to the calculated threshold distance. The results of the interaction term between understory density and distance to settlement (close/far) is shown below. The results are sorted according to the AICc value
| Categorisation distance (m) | Estimate |
|
| Pr(>|z|) |
| AICc |
|---|---|---|---|---|---|---|
| 1,450 | −1.57 | 0.60 | −2.60 | 0.009 | 0.10 | 301.4 |
| 1,500 | −1.65 | 0.61 | −2.71 | 0.007 | 0.09 | 301.8 |
| 1,550 | −1.53 | 0.61 | −2.51 | 0.012 | 0.08 | 304.5 |
| 1,600 | −1.62 | 0.61 | −2.64 | 0.008 | 0.08 | 304.7 |
| 1,400 | −1.22 | 0.56 | −2.18 | 0.029 | 0.07 | 305.4 |
| 1,650 | −1.22 | 0.61 | −1.99 | 0.046 | 0.07 | 305.7 |
| 1,700 | −0.93 | 0.62 | −1.51 | 0.132 | 0.06 | 306.8 |
| 1,800 | −0.74 | 0.64 | −1.16 | 0.246 | 0.05 | 308.7 |
| 1,350 | −0.81 | 0.53 | −1.54 | 0.124 | 0.04 | 309.1 |
| 1,750 | −0.61 | 0.63 | −0.97 | 0.333 | 0.05 | 309.1 |
| 1,850 | −0.62 | 0.66 | −0.94 | 0.346 | 0.04 | 310.4 |
| 2,250 | −0.56 | 0.81 | −0.69 | 0.491 | 0.04 | 310.4 |
| 2,300 | −0.62 | 0.82 | −0.76 | 0.449 | 0.04 | 310.6 |
| 1,900 | −0.65 | 0.65 | −1.00 | 0.317 | 0.03 | 311.1 |
| 2,450 | −0.64 | 0.86 | −0.74 | 0.458 | 0.03 | 311.1 |
| 2,500 | −0.64 | 0.86 | −0.74 | 0.458 | 0.03 | 311.1 |
| 2,350 | −0.54 | 0.84 | −0.63 | 0.526 | 0.03 | 311.1 |
| 1,250 | −0.68 | 0.51 | −1.33 | 0.183 | 0.03 | 311.3 |
| 1,300 | −0.68 | 0.51 | −1.33 | 0.183 | 0.03 | 311.3 |
| 1,950 | −0.59 | 0.66 | −0.90 | 0.370 | 0.03 | 311.3 |
| 800 | −0.20 | 0.53 | −0.38 | 0.704 | 0.03 | 311.9 |
| 750 | −0.08 | 0.53 | −0.16 | 0.873 | 0.02 | 312.1 |
| 2,400 | −0.67 | 0.86 | −0.78 | 0.436 | 0.03 | 312.1 |
| 2,200 | −0.19 | 0.76 | −0.25 | 0.801 | 0.02 | 313.1 |
| 2,550 | −0.71 | 0.86 | −0.83 | 0.409 | 0.02 | 313.2 |
| 550 | −0.31 | 0.56 | −0.56 | 0.575 | 0.02 | 313.2 |
| 1,200 | −0.55 | 0.50 | −1.10 | 0.270 | 0.02 | 313.3 |
| 2,100 | −0.19 | 0.72 | −0.26 | 0.792 | 0.02 | 313.6 |
| 650 | −0.20 | 0.54 | −0.38 | 0.705 | 0.02 | 313.7 |
| 700 | −0.20 | 0.54 | −0.38 | 0.705 | 0.02 | 313.7 |
| 2,150 | 0.00 | 0.73 | 0.01 | 0.995 | 0.02 | 313.7 |
| 600 | −0.22 | 0.54 | −0.41 | 0.683 | 0.02 | 313.9 |
| 2,750 | −0.74 | 0.94 | −0.78 | 0.433 | 0.02 | 314.1 |
| 2,900 | −0.75 | 1.02 | −0.73 | 0.463 | 0.02 | 314.1 |
| 2,000 | −0.36 | 0.68 | −0.53 | 0.596 | 0.01 | 314.2 |
| 850 | −0.05 | 0.51 | −0.09 | 0.927 | 0.01 | 314.2 |
| 2,600 | −0.85 | 0.88 | −0.97 | 0.334 | 0.01 | 314.3 |
| 2,050 | −0.34 | 0.69 | −0.48 | 0.629 | 0.01 | 314.3 |
| 2,800 | −0.88 | 0.97 | −0.91 | 0.364 | 0.02 | 314.3 |
| 2,850 | −0.73 | 0.99 | −0.74 | 0.461 | 0.01 | 314.5 |
| 900 | 0.13 | 0.51 | 0.26 | 0.797 | 0.01 | 314.5 |
| 1,000 | 0.11 | 0.50 | 0.23 | 0.818 | 0.01 | 314.5 |
| 500 | −0.07 | 0.57 | −0.12 | 0.903 | 0.01 | 314.5 |
| 1,150 | −0.30 | 0.49 | −0.61 | 0.539 | 0.01 | 314.6 |
| 950 | 0.26 | 0.51 | 0.51 | 0.610 | 0.01 | 314.7 |
| 2,650 | −0.96 | 0.90 | −1.07 | 0.283 | 0.01 | 315.1 |
| 2,950 | −0.84 | 1.03 | −0.82 | 0.413 | 0.01 | 315.1 |
| 3,300 | −0.99 | 1.07 | −0.92 | 0.358 | 0.01 | 315.2 |
| 2,700 | −0.72 | 0.90 | −0.79 | 0.428 | 0.01 | 315.2 |
| 3,250 | −0.97 | 1.05 | −0.92 | 0.356 | 0.01 | 315.6 |
| 1,100 | −0.07 | 0.49 | −0.15 | 0.884 | 0.01 | 315.6 |
| 1,050 | −0.05 | 0.49 | −0.10 | 0.923 | 0.01 | 315.6 |
| 3,000 | −0.81 | 1.02 | −0.80 | 0.425 | 0.01 | 315.7 |
| 3,050 | −0.81 | 1.02 | −0.80 | 0.425 | 0.01 | 315.7 |
| 3,100 | −0.81 | 1.02 | −0.80 | 0.425 | 0.01 | 315.7 |
| 3,150 | −0.81 | 1.02 | −0.80 | 0.425 | 0.01 | 315.7 |
| 3,200 | −0.81 | 1.02 | −0.80 | 0.425 | 0.01 | 315.7 |
| 3,350 | −0.34 | 1.17 | −0.29 | 0.768 | 0.00 | 316.6 |
| 3,400 | −0.34 | 1.17 | −0.29 | 0.768 | 0.00 | 316.6 |
| 3,450 | −0.34 | 1.17 | −0.29 | 0.768 | 0.00 | 316.6 |
| 3,500 | −0.18 | 1.18 | −0.15 | 0.881 | 0.00 | 316.7 |
Figure 3(a) The difference between the normalized predictions of Siberian jay occurrence and probability of successful reproduction in a large part of its Swedish distribution. Disagreement is, in almost all cases, based on an overestimation of breeding success. The disagreement calculation in this map is based on understory density data within 15 m around the center of every pixel and is highly correlated (pmcc = 0.84) with using data within 80 m. (b) The density of the disagreement values split by the four municipalities used for this landscape comparison