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Satellite observations of surface temperature during the March 2015 total solar eclipse
1Met Office Hadley Centre, FitzRoy Road, Exeter EX1 3PB, UK elizabeth.good@metoffice.gov.uk.
During a total solar eclipse, remotely sensed land surface temperatures (LSTs) dropped significantly, exceeding air temperature decreases. Factors like solar obscuration and eclipse duration influenced the LST drop.
Area of Science:
- Earth Observation
- Atmospheric Science
- Remote Sensing
Background:
- Total solar eclipses cause temporary reductions in solar radiation reaching the Earth's surface.
- Land surface temperature (LST) is a key variable influenced by surface energy balance.
- Previous studies have documented localized temperature drops during eclipses, but comprehensive satellite-based analyses are limited.
Purpose of the Study:
- To analyze the behavior of remotely sensed LST during the 20 March 2015 total solar eclipse over Europe.
- To quantify the relationship between LST drop and factors such as solar obscuration, eclipse duration, and time.
- To investigate local variations in LST drop related to surface characteristics like vegetation, proximity to coast, and elevation.
Main Methods:
- Utilized land surface temperature (LST) data from the Spinning-Enhanced Visible and Infrared Imager (SEVIRI).
- Analyzed LST changes during the 20 March 2015 total solar eclipse across Europe.
- Correlated LST drop magnitude with solar obscuration, eclipse duration, time, vegetation cover, coastal proximity, and elevation.
Main Results:
- LST decreased by up to several degrees Celsius during the eclipse, with minimums occurring shortly after the midpoint.
- The LST drop was generally larger than concurrent near-surface air temperature drops.
- LST drop magnitude showed significant correlations with solar obscuration (r=-0.47), eclipse duration (r=-0.62), and time (r=+0.37).
- Vegetation cover (up to r=+0.6), coastal proximity, and elevation influenced the localized LST drop, with less impact on vegetated, coastal, or higher-elevation areas.
Conclusions:
- Satellite-derived LST provides a robust measure of surface temperature response to solar eclipses.
- The study provides the most extensive characterization to date of satellite LST during an eclipse.
- The methodology can be applied to analyze LST data from other geostationary satellites, such as GOES, during future eclipses.
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