Characterizing the Impacts of 2024 Total Solar Eclipse Using New York
State Mesonet Data
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.