TY - JOUR
T1 - Medium-scale gravity wave activity in the bottomside F region in tropical regions
AU - Liu, Huixin
AU - Pedatella, Nicholas
AU - Hocke, Klemens
N1 - Funding Information:
We thank E. Doornbos for providing the GOCE data, which is accessible at https://earth.esa.int/web/guest/ missions/esa-operational-missions/ goce/goce-thermospheric-data. This work is supported by JSPS KAKENHI grants 15K05301 and 15H02135. The National Center for Atmospheric Research is supported by the U.S. National Science Foundation.
Publisher Copyright:
©2017. American Geophysical Union. All Rights Reserved.
PY - 2017/7/28
Y1 - 2017/7/28
N2 - Thermospheric gravity waves (GWs) in the bottomside F region have been proposed to play a key role in the generation of equatorial plasma bubbles (EPBs). However, direct observations of such waves are scarce. This study provides a systematic survey of medium-scale (<620 km) neutral atmosphere perturbations at this critical altitude in the tropics, using 4 years of in situ Gravity Field and Steady-State Ocean Circulation Explorer satellite measurements of thermospheric density and zonal wind. The analysis reveals pronounced features on their global distribution and seasonal variability: (1) A prominent three-peak longitudinal structure exists in all seasons, with stronger perturbations over continents than over oceans. (2) Their seasonal variation consists of a primary semiannual oscillations (SAO) and a secondary annual oscillation (AO). The SAO component maximizes around solstices and minimizes around equinoxes, while the AO component maximizes around June solstice. These GW features resemble those of EPBs in spatial distribution but show opposite trend in climatological variations. This may imply that stronger medium-scale GW activity does not always lead to more EPBs. Possible origins of the bottomside GWs are discussed, among which tropical deep convection appears to be most plausible.
AB - Thermospheric gravity waves (GWs) in the bottomside F region have been proposed to play a key role in the generation of equatorial plasma bubbles (EPBs). However, direct observations of such waves are scarce. This study provides a systematic survey of medium-scale (<620 km) neutral atmosphere perturbations at this critical altitude in the tropics, using 4 years of in situ Gravity Field and Steady-State Ocean Circulation Explorer satellite measurements of thermospheric density and zonal wind. The analysis reveals pronounced features on their global distribution and seasonal variability: (1) A prominent three-peak longitudinal structure exists in all seasons, with stronger perturbations over continents than over oceans. (2) Their seasonal variation consists of a primary semiannual oscillations (SAO) and a secondary annual oscillation (AO). The SAO component maximizes around solstices and minimizes around equinoxes, while the AO component maximizes around June solstice. These GW features resemble those of EPBs in spatial distribution but show opposite trend in climatological variations. This may imply that stronger medium-scale GW activity does not always lead to more EPBs. Possible origins of the bottomside GWs are discussed, among which tropical deep convection appears to be most plausible.
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U2 - 10.1002/2017GL073855
DO - 10.1002/2017GL073855
M3 - Article
AN - SCOPUS:85028511355
SN - 0094-8276
VL - 44
SP - 7099
EP - 7105
JO - Geophysical Research Letters
JF - Geophysical Research Letters
IS - 14
ER -