| Literature DB >> 31834919 |
Michael A Patten1,2, Jutta C Burger3, Milan Mitrovich4.
Abstract
Direct effects of human disturbance on animal populations are well documented across habitats, biomes, and species, but indirect effects of diel have received less attention. An emerging field in applied ecology involves behavioral avoidance of or attraction to humans and their trappings. We posit trophic consequences, in terms of relative risk, for four species of mammals, each of which strongly avoids human activity, in urban reserves of coastal southern California. Two species, one predator and one prey, avoid human activity via a temporal shift to become "more nocturnal"-the species' activity is centered near dawn on days without human activity but nearer to midnight on days with human activity. Diel shifts have brought the species into greater overlap, respectively, with a key prey and a key predator, overlap that may increase encounter rate and thus increase relative risk of predation, with potential consequences for trophic dynamics and cascades: increased risk of predation may depress prey population, either directly (e.g., mortality) or indirectly (e.g., "landscape of fear"). Human use of reserves, especially in high population density regions, needs to be reconsidered either to reduce access or to restrict access entirely to areas that may provide refuge to both predators and prey.Entities:
Year: 2019 PMID: 31834919 PMCID: PMC6910683 DOI: 10.1371/journal.pone.0226418
Source DB: PubMed Journal: PLoS One ISSN: 1932-6203 Impact factor: 3.240
Temporal distribution across undisturbed and disturbed days for seven mammal species in coastal Orange County, California.
All means (from angle θ, with it and 95% confidence intervals, CI, converted to time of day, t, on a 24-h clock) differed significantly (Rayleigh test: P < 0.0001) from a random distribution of occurrences around the clock. Statistic r, which varies from 0 to 1, is a standardized measure of concentration at the mean. At the right, results are presented a rank sum test of temporal shift between undisturbed vs. disturbed occurrences.
| species | mean | mean | ||||||
|---|---|---|---|---|---|---|---|---|
| 00:24 | 0.20 | 2140 | 22:44 | 0.42 | 992 | -3.53 | <0.01 | |
| 00:15 | 0.40 | 514 | 22:58 | 0.59 | 157 | -1.36 | 0.17 | |
| 00:34 | 0.60 | 971 | 23:10 | 0.70 | 268 | -1.42 | 0.16 | |
| 04:04 | 0.26 | 3671 | 23:08 | 0.40 | 2440 | -9.04 | <0.01 | |
| 01:30 | 0.61 | 280 | 00:52 | 0.74 | 108 | -2.06 | 0.04 | |
| 00:23 | 0.55 | 599 | 23:59 | 0.62 | 91 | -1.65 | 0.10 | |
| 06:44 | 0.15 | 15689 | 20:56 | 0.24 | 2471 | -6.48 | <0.01 | |
Fig 1Diel activity of the Gray Fox (Urocyon cinereoargenteus) and Coyote (Canis latrans) with or without human disturbance.
Arrows indicate time (direction) and proportional magnitude (length) of mean activity, and the “net” displays the spread of activity on a 24-h clock, binned at 30-min. intervals. Note the predator’s (the Coyote) nocturnal shift when disturbance was present. The extent of overlap in activity increased from 33% to 45%.
Fig 2Diel activity of the Mule Deer (Odocoileus hemionus) and Puma (Puma concolor) with and without human disturbance; see Fig 1 for an explanation of the graphs.
Note the prey’s (the deer) nocturnal shift when disturbance was present. The extent of overlap in activity increased from 35% to 54%.
Fig 3Mean estimated abundance (from an N-mixture model, ±SE, and on a common log scale) of the Mule Deer (Odocoileus hemionus) and Puma (Puma concolor), as well as human disturbance for reference, with heuristic plots of mean slopes from a linear regression.
It is probable (Bayesian posterior P = 0.94) that deer occupancy (Ψ) has decreased over time whereas Puma occupancy has increased (Bayesian posterior P = 0.87). (Occupancy estimates for the Puma were unstable for 2007 and so abundance could not be estimated. Also, probability of detection was not correlated with year, although it may have increased slightly for the deer.).
Presence of the Mule Deer (Odocoileus hemionus) and the Puma (Puma concolor) across camera traps, with expected versus observed incidence of joint presence.
Data were aggregated by calendar day for the focal species alone (i.e., camera-trap records of species other than the deer and Puma were not considered) and restricted to cameras that had at least one presence of the Puma. Expected values were estimated from a joint probability under the assumption that the deer and Puma occur independently, meaning observed joint (i.e., same day) presence much lower than expected implies that occurrence is not independent.
| camera | Mule Deer | Puma | expected | observed | |
|---|---|---|---|---|---|
| AG CH | 77 | 0.675 | 0.325 | 17 | 0 |
| AU TR | 509 | 0.986 | 0.022 | 11 | 4 |
| BL ST | 66 | 0.924 | 0.091 | 6 | 1 |
| BO SP | 618 | 0.989 | 0.013 | 8 | 1 |
| BO TR | 582 | 0.930 | 0.124 | 67 | 31 |
| CO MI | 182 | 0.967 | 0.038 | 7 | 1 |
| CO TR | 173 | 0.908 | 0.104 | 16 | 2 |
| DO CA | 106 | 0.830 | 0.179 | 16 | 1 |
| DO CA2 | 50 | 0.900 | 0.120 | 5 | 1 |
| DO CA3 | 29 | 0.897 | 0.103 | 3 | 0 |
| DR SP | 207 | 0.807 | 0.232 | 39 | 8 |
| DR SP2 | 149 | 0.926 | 0.121 | 17 | 7 |
| EA MW | 445 | 0.971 | 0.043 | 18 | 6 |
| EA MW2 | 41 | 0.976 | 0.024 | 1 | 0 |
| FR RO | 231 | 0.939 | 0.087 | 19 | 6 |
| FU BR | 204 | 0.941 | 0.069 | 13 | 2 |
| GY FO | 243 | 0.930 | 0.119 | 27 | 12 |
| LA RO | 319 | 0.937 | 0.085 | 25 | 7 |
| LI ME | 131 | 0.832 | 0.198 | 22 | 4 |
| LI ME2 | 35 | 0.771 | 0.286 | 8 | 2 |
| LI SI | 141 | 0.816 | 0.270 | 31 | 12 |
| LO WE1 | 121 | 0.992 | 0.008 | 1 | 0 |
| LO WE2 | 274 | 0.737 | 0.281 | 57 | 5 |
| ME SP | 10 | 0.800 | 0.200 | 2 | 0 |
| MO FR1 | 215 | 0.837 | 0.181 | 33 | 4 |
| MO FR3 | 178 | 0.781 | 0.247 | 34 | 5 |
| OV TR | 195 | 0.964 | 0.036 | 7 | 0 |
| RA TR | 77 | 0.987 | 0.026 | 2 | 1 |
| RO CA | 134 | 0.993 | 0.007 | 1 | 0 |
| RO CA2 | 35 | 0.857 | 0.171 | 5 | 1 |
| SO GY | 204 | 0.868 | 0.157 | 28 | 5 |
| UP WE | 133 | 0.932 | 0.075 | 9 | 1 |
| WE SP | 458 | 0.985 | 0.026 | 12 | 5 |
| WE TR1 | 791 | 0.991 | 0.059 | 47 | 40 |
| WE TR2 | 627 | 0.994 | 0.038 | 24 | 20 |
| WE TR3 | 359 | 0.997 | 0.028 | 10 | 9 |
| WE WI | 71 | 0.930 | 0.070 | 5 | 0 |