Iridescent colored bands on clouds

Iridescence on clouds is often considered to be closely related to the rings of the atmospheric corona. Both phenomena are caused by near-forward scattering of sunlight. The colored rings of the corona are caused by diffraction from water droplets of fairly uniform size. Iridescence is often seen as bands of color along the edges of clouds. Mie theory shows that near-forward scattering of sunlight is a complicated function of droplet radius <i>r</i> and scattering angle <i>θ</i>. It is difficult to analyze photographs of iridescence because most photographers deliberately exclude the Sun, and hence, we do not know the value of <i>θ</i>. This paper uses indirect techniques to determine the relative position of the Sun, thereby revealing <i>θ</i> and allowing estimates of the droplet radius <i>r</i> at different points in the iridescent clouds. The results demonstrate that variations in <i>r</i> produce the narrow bands of color aligned with the edges of clouds.

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Publication Details

Journal
Applied Optics
Published
2025-11-24
DOI
https://doi.org/10.1364/ao.580006
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Iridescent colored bands on clouds

L. R. Hall, Philip Laven
Applied Optics
Solar and Space Plasma Dynamics
article

Iridescent colored bands on clouds

L. R. Hall, Philip Laven
article en

Abstract

Iridescence on clouds is often considered to be closely related to the rings of the atmospheric corona. Both phenomena are caused by near-forward scattering of sunlight. The colored rings of the corona are caused by diffraction from water droplets of fairly uniform size. Iridescence is often seen as bands of color along the edges of clouds. Mie theory shows that near-forward scattering of sunlight is a complicated function of droplet radius <i>r</i> and scattering angle <i>θ</i>. It is difficult to analyze photographs of iridescence because most photographers deliberately exclude the Sun, and hence, we do not know the value of <i>θ</i>. This paper uses indirect techniques to determine the relative position of the Sun, thereby revealing <i>θ</i> and allowing estimates of the droplet radius <i>r</i> at different points in the iridescent clouds. The results demonstrate that variations in <i>r</i> produce the narrow bands of color aligned with the edges of clouds.

Applied OpticsVol. 65(9)
Openalex Percentile: Top 75%
Solar and Space Plasma Dynamics
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