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

被引:0
|
作者
Wang, Junhong [1 ]
Dai, Aiguo [2 ]
Yu, Chau-Lam [1 ]
Shrestha, Bhupal [1 ]
Mcguinnes, D. J. [1 ]
Bain, Nathan [1 ]
机构
[1] SUNY Univ Albany, New York State Mesonet, Albany, NY 12222 USA
[2] SUNY Univ Albany, Dept Atmospher & Environm Sci, Albany, NY USA
基金
美国国家科学基金会;
关键词
total solar eclipse; New York State Mesonet; eclipse impacts; boundary layer; land-atmosphere interactions; PLANETARY BOUNDARY-LAYER; 29; MARCH; 2006; TEMPERATURE;
D O I
10.1029/2024GL112684
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
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 peak surface cooling occurs 17 min after the totality and is 2.8 degrees C on average with a maximum of 6.8 degrees C. It results in night-like surface inversion, calm winds, and reduced vertical motion and mixing, leading to the shallowing of the PBL and its moistening. Surface sensible, latent and ground heat fluxes all decrease whereas near-surface CO2 concentration rises as photosynthesis slows down.
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页数:10
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