At hillslopes, arid ecosystems tend to form characteristic spatial patterns consisting of alternating vegetated and bare stripes. As such patterns form autogenously, they can potentially provide insight into the ecosystem functioning, health, and resilience. While the spectral properties of striped patterns are well understood, less is known about the stripe width. To fill this gap, I address several essential questions: 1) What is the general form of the stripe width distribution (SWD)? 2) How do exogenous random spatial heterogeneities modulate the SWD? 3) How can the regularity of patterns be measured based on the SWD? 4) What can the SWD reveal about the health and resilience of ecosystems? 5) What caveats complicate the estimation and interpretation of the SWD? To answer these questions, I first derive a theoretical SWD based on a parsimonious stochastic model for anisotropic patterns, and second, systematically explore the stripe width distributions of patterns generated with the more complex Rietkerk model which explicitly accounts for pattern forming processes. I ensure variation of the stripe width in the simulations by simulations by perturbing the infiltration capacity randomly in space. I find that the theoretical SWD agrees very well with the SWD of patterns generated in one-dimensional simulations, and after a small extension, also agrees reasonably well with that of patterns generated in two dimensions. Finally, I compare the theoretical SWD to that of natural striped vegetation patterns.
How to cite:
Kästner, K.: On the stripe width distribution of regular vegetation patterns, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14495, https://doi.org/10.5194/egusphere-egu26-14495, 2026.
Please use the buttons below to download the display or to visit the external website where the presentation is linked. Regarding the external link, please note that Copernicus Meetings cannot accept any liability for the content and the website you will visit.
You are going to open an external link to the presentation as indicated by the authors. Copernicus Meetings cannot accept any liability for the content and the website you will visit.