Surface Mesonet and Upper Air Analysis of the 21 August 2017 Total Solar Eclipse

Author/Creator ORCID

Date

2023-09-07

Department

Program

Citation of Original Publication

Pasken, Robert, Jeffrey Halverson, and Peter Braunschweig. 2023. "Surface Mesonet and Upper Air Analysis of the 21 August 2017 Total Solar Eclipse" Atmosphere 14, no. 9: 1412. https://doi.org/10.3390/atmos14091412

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Attribution 4.0 International (CC BY 4.0)

Subjects

Abstract

The total solar eclipse of 21 August 2017 was unique in that the path of totality swept across the high spatial and temporal resolution QuantumWeather® mesonet and was very near the city of St. Louis Missouri. Thus, the meteorological response to the eclipse was complicated by the St. Louis urban heat island. Temperature changes of up 4 °C were observed across the network. Composite meteograms for rural, suburban, and urban stations displayed significant differences in the observed temperature and pressure response to the eclipse with a peak amplitude at the time of the eclipse. The differing response suggests that the urban heat island and changes in land surface characteristics alter the temperature and pressure response by the passage of the eclipse shadow. Oscillations in the composite meteograms appear to be the consequence of the passage of an outflow boundary across the network. As the outflow boundary moves north to south, the outflow boundary manifests its presence in the pressure field as a damped oscillation. Sounding data were collected along the center line of eclipse and along the southern edge of the eclipse before and during the eclipse. The soundings show that the eclipse altered the boundary layer height, the lowest layer of the atmosphere, in an unexpected way.