Applying Landscape-Scale Habitat-Potential Models to Understand Deer Spatial Structure and Movement Patterns

2007 ◽  
Vol 71 (3) ◽  
pp. 804-810 ◽  
Author(s):  
ALEXANDRA B. FELIX ◽  
DANIEL P. WALSH ◽  
BRANDI D. HUGHEY ◽  
HENRY CAMPA ◽  
SCOTT R. WINTERSTEIN
2004 ◽  
Vol 32 (3) ◽  
pp. 795-806 ◽  
Author(s):  
Alexandra B. Felix ◽  
Henry Campa ◽  
Kelly F. Millenbah ◽  
Scott R. Winterstein ◽  
William E. Moritz

2006 ◽  
Vol 43 (6) ◽  
pp. 1087-1097 ◽  
Author(s):  
AUDREY ZANNÈSE ◽  
NICOLAS MORELLET ◽  
CHIARA TARGHETTA ◽  
AURÉLIE COULON ◽  
SIMONETTA FUSER ◽  
...  

2021 ◽  
Author(s):  
Camille Saade ◽  
Emanuel A. Fronhofer ◽  
Benoit Pichon ◽  
Sonia Kefi

Even when environments deteriorate gradually, ecosystems may shift abruptly from one state to another. Such catastrophic shifts are difficult to predict and reverse (hysteresis). While well studied in simplified contexts, we lack a general understanding of how catastrophic shifts spread in realistic spatial contexts. For different types of landscape structure, including typical terrestrial modular and riverine dendritic networks, we here investigate landscape-scale stability in metapopulations made of bistable patches. We find that such metapopulations usually exhibit large scale catastrophic shifts and hysteresis, and that the properties of these shifts depend strongly on metapopulation spatial structure and dispersal rate: intermediate dispersal rates and a riverine spatial structure can largely reduce hysteresis size. Interestingly, our study suggests that large-scale restoration is easier with spatially clustered restoration efforts and in populations characterized by an intermediate dispersal rate.


1967 ◽  
Vol 31 ◽  
pp. 45-46
Author(s):  
Carl Heiles

High-resolution 21-cm line observations in a region aroundlII= 120°,b11= +15°, have revealed four types of structure in the interstellar hydrogen: a smooth background, large sheets of density 2 atoms cm-3, clouds occurring mostly in groups, and ‘Cloudlets’ of a few solar masses and a few parsecs in size; the velocity dispersion in the Cloudlets is only 1 km/sec. Strong temperature variations in the gas are in evidence.


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