Document Type
Article
Publication Date
2-5-2026
Department
Department of Biological Sciences
Abstract
The search for predictors of plant diversity has challenged scientists for decades. Here we identify intense photosynthetically active radiation (PAR) as a major factor constraining plant species richness in global grasslands. We show that the strength of the negative relationship between species richness and PAR increases with increasing elevation and that species richness is more strongly correlated with intense PAR than with UV-B radiation, climate variables, and atmospheric nitrogen deposition. In addition to species richness, plant biomass was also negatively correlated with PAR at higher elevations, indicating that intense PAR also constrains plant biomass in montane grasslands. Furthermore, we show that the decrease in plant species richness with increasing PAR is mainly caused by a decrease in species richness of forbs, sedges, and rushes. In contrast, species richness of grasses was only negatively correlated with PAR at high elevations, and species richness of legumes was not significantly correlated with PAR. Our results suggest that PAR constrains plant species richness in global grasslands and limits the extent to which plant species of specific functional groups can migrate uphill in response to climate warming.
Publication Title
Proceedings of the National Academy of Sciences of the United States of America
Recommended Citation
Spohn, M.,
Arnillas, C.,
Bakker, J.,
Borer, E.,
Bråthen, K.,
Cadotte, M.,
Hersch-Green, E.,
&
et al.
(2026).
Intense solar radiation constrains plant species richness in global grasslands.
Proceedings of the National Academy of Sciences of the United States of America,
123(6).
http://doi.org/10.1073/pnas.2527128123
Retrieved from: https://digitalcommons.mtu.edu/michigantech-p2/2382
Creative Commons License

This work is licensed under a Creative Commons Attribution-NonCommercial-No Derivative Works 4.0 International License.
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Publisher's PDF
Publisher's Statement
Copyright © 2026 the Author(s). Published by PNAS. Publisher’s version of record: https://doi.org/10.1073/pnas.2527128123