In this study, we used a variety of Kestrel devices (DROP and 5400 Heat Stress Tracker), and QuantAQ MODULAIRs to measure the surface level composition at three unique sites across North and Central Texas. We aimed to study the changes of atmosphere conditions throughout the progression of a total solar eclipse and the concentrations of surface-level pollutants due to variations in solar radiation and atmospheric dynamics.
Our results show that an increase in NO2 by 200% and a decrease in NO by 85% and O3 by 33% were observed during the eclipse. Wind speeds experienced an explicit decrease of 95% when totality was occurring at our locations. This led to a very significant decrease in the dispersion of NO2, NO, and O3 at all three of our sites.
In conclusion, with the rise in NO2 observed during the eclipse, we can expect this increasing trend to continue if there were a solar blockage for a longer period, causing negative repercussions and uncommon behaviors in pollutants. The work found in this study can be used to show the impacts of UV-obstructing chemicals on objects such as clouds and future eclipses, which can also be used to strengthen chemical models.
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