# Migration, Habitat and Hunting Style Do Not Affect the Malar Stripe of Different Falcon Species

**Authors:** Celeste Polak, Jente Ottenburghs

PMC · DOI: 10.1002/ece3.71028 · Ecology and Evolution · 2025-04-27

## TL;DR

This study found that migration, habitat, and hunting style do not affect the malar stripe of falcons, suggesting other factors like camouflage or thermoregulation may be involved.

## Contribution

The study is the first to show that environmental variables do not significantly influence malar stripe traits in falcons.

## Key findings

- Malar stripe size and intensity do not differ between falcon species with different migratory strategies, habitats, or hunting styles.
- The relationship between malar stripe traits and solar radiation depends on species and habitat.
- Environmental variables like migration and habitat do not strongly influence malar stripe characteristics.

## Abstract

The solar glare hypothesis suggests that the malar stripe of a falcon decreases the sun's glare in the eye, possibly increasing their hunting success. The amount of sunlight an individual experiences could be affected by its migratory strategy, hunting style or main habitat. However, it is not known if these environmental variables impact the size and intensity of the malar stripe. Therefore, this study aimed to analyse differences in size and intensity of malar stripes between individuals of 12 falcon species with different migratory strategies, habitats, and hunting styles distributed worldwide. The malar stripes of 12 falcon species were measured and scored using more than 6000 photos from citizen science repositories. The measurements of the malar stripes were first reduced with a principal component analysis (PCA) and then analysed using a linear mixed model that included migratory strategy, habitat and hunting style as fixed factors and several posture variables as random factors. The relationships between the measurements of the malar stripe and solar radiation of the individual's location were also analyzed using linear mixed models. Overall, we found no differences in malar stripe size and intensity between species with differing migratory strategies, habitats, and hunting styles. The relationships between various characteristics of the malar stripe and solar radiation did depend on the species and the habitat the individual occupied. Therefore, migratory strategy, habitat and hunting style do not markedly influence the size and intensity of malar stripes across falcon species, suggesting that other mechanisms, such as thermoregulation or camouflage, also play a role.

Migratory strategy, habitat and hunting style do not markedly influence the size and intensity of malar stripes across falcon species, suggesting that other mechanisms, such as thermoregulation or camouflage, also play a role.

## Full-text entities

- **Chemicals:** black paint (-)
- **Species:** Eurillas virens (Little greenbul, species) [taxon 1743266], Falco berigora (species) [taxon 495972], Falco rupicoloides (species) [taxon 148597], Falco tinnunculus (common kestrel, species) [taxon 100819], Falco chicquera (red-necked falcon, species) [taxon 495941], Falco peregrinus (peregrine, species) [taxon 8954], Falco eleonorae (species) [taxon 495946], Falco rufigularis (species) [taxon 399590], Falco dickinsoni (species) [taxon 495939], Falco novaeseelandiae (species) [taxon 495971], Falco rusticolus (gyrfalcon, species) [taxon 120794], Falco rupicolus (South African kestrel, species) [taxon 1562128], Falco (falcons, genus) [taxon 8952], Lanius nubicus (masked shrike, species) [taxon 276759], Gyps fulvus (Eurasian griffon, species) [taxon 36247], Lemur catta (Ring-tailed lemur, species) [taxon 9447], Falco newtoni (species) [taxon 148595], Setophaga discolor (prairie warbler, species) [taxon 92120]

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12034159/full.md

## References

85 references — full list in the complete paper: https://tomesphere.com/paper/PMC12034159/full.md

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Source: https://tomesphere.com/paper/PMC12034159