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Characterizing the Impacts of 2024 Total Solar Eclipse Using New York State Mesonet Data
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  • Junhong Wang,
  • Aiguo Dai,
  • Nathan Bain,
  • D.J. McGuinnes,
  • Bhupal Shrestha,
  • Chau Lam Yu
Junhong Wang
University at Albany, SUNY

Corresponding Author:[email protected]

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Aiguo Dai
University at Albany, State University of New York
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Nathan Bain
University at Albany, SUNY
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D.J. McGuinnes
University at Albany, SUNY
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Bhupal Shrestha
University at Albany SUNY
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Chau Lam Yu
SUNY Albany
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Abstract

On 8 April 2024, a rare total solar eclipse (TSE) passed over western New York State (NYS), the first since 1925 and the last one until 2079. The NYS Mesonet (NYSM) consisting of 126 weather stations with 55 on the totality path provides unprecedented surface, profile, and flux data and camera images during the TSE. Here we use NYSM observations to characterize the TSE’s impacts at the surface, in the planetary boundary layer (PBL), and on surface fluxes and CO2 concentrations. The TSE-induced surface cooling occurs 20 minutes after the totality and is 2.75°C on average with a maximum value of 6.9°C. It results in night-like surface inversion, calm winds, and reduced vertical motion and mixing, which leads to the shallowing of the PBL and its moistening due to reduced vertical mixing. Surface sensible, latent and ground heat fluxes all decrease whereas near-surface CO2 concentration rises as photosynthesis slows down.
10 Jul 2024Submitted to ESS Open Archive
15 Jul 2024Published in ESS Open Archive