Moonlight Cannot Paint the Sky Blue: Evidence for Neutral Solar Wind Atmospheric Excitation

Earth's blue sky has been attributed to Rayleigh scattering for 150 years, yet moonlight—despite identical spectral composition—produces no detectable blue sky. We demonstrate that if scattering dominated, moonlight should create observable blue glow (0.04 lux, magnitude -9.7), contradicting astronomical observations. We propose that blue sky arises primarily from atmospheric excitation by neutral solar wind particles via auroral mechanisms. This explains: (1) the moonlight asymmetry, (2) diurnal color changes matching altitude-dependent auroral emissions, and (3) thermospheric heating at auroral altitudes (85-600 km). This paradigm shift implies neutral particles constitute a significant component of solar wind, with profound implications for solar-terrestrial physics and space weather.

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2025-10-13
DOI
https://doi.org/10.5281/zenodo.17342007
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00
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article

Moonlight Cannot Paint the Sky Blue: Evidence for Neutral Solar Wind Atmospheric Excitation

Zenodo (CERN European Organization for Nuclear Research)
Ionosphere and magnetosphere dynamics
article

Moonlight Cannot Paint the Sky Blue: Evidence for Neutral Solar Wind Atmospheric Excitation

article en

Abstract

Earth's blue sky has been attributed to Rayleigh scattering for 150 years, yet moonlight—despite identical spectral composition—produces no detectable blue sky. We demonstrate that if scattering dominated, moonlight should create observable blue glow (0.04 lux, magnitude -9.7), contradicting astronomical observations. We propose that blue sky arises primarily from atmospheric excitation by neutral solar wind particles via auroral mechanisms. This explains: (1) the moonlight asymmetry, (2) diurnal color changes matching altitude-dependent auroral emissions, and (3) thermospheric heating at auroral altitudes (85-600 km). This paradigm shift implies neutral particles constitute a significant component of solar wind, with profound implications for solar-terrestrial physics and space weather.

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 49%
Ionosphere and magnetosphere dynamics
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