z-logo
Premium
Long‐Term Trends in Tropical (10°N–15°N) Middle Atmosphere (40–110 km) CO 2 Cooling
Author(s) -
Ramesh K.,
Sridharan S.
Publication year - 2018
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2017ja025060
Subject(s) - thermosphere , atmospheric sciences , atmosphere (unit) , depth sounding , mesosphere , stratosphere , climatology , quasi biennial oscillation , ozone , environmental science , oscillation (cell signaling) , atmospheric temperature , ionosphere , physics , chemistry , geology , meteorology , biochemistry , astronomy , oceanography
Long‐term trends in middle atmosphere (~40–100 km; here extended up to 110 km), 15 μm carbon dioxide (CO 2 ) cooling rates, and their responses to solar cycle (SC), quasi‐biennial oscillation, and El Niño‐Southern Oscillation are investigated over Indian tropical region (10°N–15°N) using TIMED‐SABER (Thermosphere Ionosphere Mesosphere Energetics and Dynamics‐Sounding of the Atmosphere using Broadband Emission Radiometry) observations during 2002–2015 (23–24 SCs). The CO 2 cooling directly depends on temperature so that higher temperature causes more infrared emission from CO 2 at 15 μm band and thus provides larger CO 2 cooling. The 15 μm CO 2 cooling trends are relatively smaller below ~70–80 km, and their amplitude increases above this height. The trends are positive between ~40 and ~62 km peaking at ~47 km (0.06 ± 0.014 K/day/decade) and negative at ~63–74 and ~79–84 km. Further the positive trends increase sharply above ~84 km at the rate of ~0.1–3.0 K/day/decade between 85 and 110 km. The CO 2 cooling response to SC, El Niño‐Southern Oscillation, and quasi‐biennial oscillation is smaller below ~70–75 and stronger above this height. The 15 μm CO 2 heating exhibits semiannual variation with ~0.1–0.8 K/day during equinoxes between ~70 and 77 km. In addition, the increase in CO 2 cooling significantly influences the background temperature and thereby ozone concentration, neutral number density and layer thickness (width) in the stratosphere and mesosphere.

This content is not available in your region!

Continue researching here.

Having issues? You can contact us here