Abstract
Correlative and regression analyses of daily ERA-Interim reanalysis data for three separate solar maximum periods confirm the existence of a temperature response to short-term (mainly ∼27 day) solar ultraviolet variations at tropical latitudes in both the lower stratosphere and troposphere. The response, which occurs at a phase lag of 6-10 days after the solar forcing peak, consists of a warming in the lower stratosphere, consistent with relative downwelling and a slowing of the mean meridional (Brewer-Dobson) circulation, and a cooling in the troposphere. The midtropospheric cooling response is most significant in the tropical Pacific, especially under positive El Niño-Southern Oscillation conditions and may be related to a reduction in the number of Madden-Julian oscillation events that propagate eastward into the central Pacific following peaks in short-term solar forcing.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 4066-4075 |
| Number of pages | 10 |
| Journal | Geophysical Research Letters |
| Volume | 43 |
| Issue number | 8 |
| DOIs | |
| State | Published - Apr 28 2016 |
Keywords
- lower stratosphere
- solar ultraviolet radiation
- tropospheric temperature
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences
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