TY - JOUR
T1 - Vertical Transport of Sensible Heat and Meteoric Na by the Complete Temporal Spectrum of Gravity Waves in the MLT Above McMurdo (77.84°S, 166.67°E), Antarctica
AU - Chu, Xinzhao
AU - Gardner, Chester S.
AU - Li, Xianxin
AU - Lin, Cissi Ying Tsen
N1 - We sincerely appreciate Dr. Sharon Vadas and Dr. Erich Becker for their advice and invaluable discussion on the compressible polarization relations for gravity waves and on energetics and wave dynamics of the middle and upper atmosphere. We are grateful to Jackson Jandreau for his assistance in compiling satellite and WACCM data of minor species for chemical flux calculation, to Wuhu Feng for providing WACCM KZZ data, to Tao Li for providing the Hefei flux measurements, and to Juan Diego Carrillo-Sanchez for providing CABMOD meteoric injection rates. We gratefully acknowledge Dr. Art Richmond, Dr. Yasunobu Ogawa, Dr. Zhonghua Xu, and Dr. Yukitoshi Nishimura for invaluable discussions on heat sources and heat balance in the lower thermosphere. We are grateful to Dr. Yasunobu Ogawa for providing aurora observations at McMurdo. We sincerely appreciate the staff of United States Antarctic Program, McMurdo Station, Antarctica New Zealand, and Scott Base for their superb support to the McMurdo lidar observations. The McMurdo lidar projects were supported by the National Science Foundation (NSF) grants OPP-1246405, OPP-1443726, and OPP-2110428. This work was partially supported by NSF grants AGS-2029162 and AGS-1452351. The auroral images were obtained with supports from NSF (ANT-1643700) and the Japanese Antarctic Research Expedition program (AP0927).
We sincerely appreciate Dr. Sharon Vadas and Dr. Erich Becker for their advice and invaluable discussion on the compressible polarization relations for gravity waves and on energetics and wave dynamics of the middle and upper atmosphere. We are grateful to Jackson Jandreau for his assistance in compiling satellite and WACCM data of minor species for chemical flux calculation, to Wuhu Feng for providing WACCM K data, to Tao Li for providing the Hefei flux measurements, and to Juan Diego Carrillo‐Sanchez for providing CABMOD meteoric injection rates. We gratefully acknowledge Dr. Art Richmond, Dr. Yasunobu Ogawa, Dr. Zhonghua Xu, and Dr. Yukitoshi Nishimura for invaluable discussions on heat sources and heat balance in the lower thermosphere. We are grateful to Dr. Yasunobu Ogawa for providing aurora observations at McMurdo. We sincerely appreciate the staff of United States Antarctic Program, McMurdo Station, Antarctica New Zealand, and Scott Base for their superb support to the McMurdo lidar observations. The McMurdo lidar projects were supported by the National Science Foundation (NSF) grants OPP‐1246405, OPP‐1443726, and OPP‐2110428. This work was partially supported by NSF grants AGS‐2029162 and AGS‐1452351. The auroral images were obtained with supports from NSF (ANT‐1643700) and the Japanese Antarctic Research Expedition program (AP0927). ZZ
PY - 2022/8/27
Y1 - 2022/8/27
N2 - We report the first lidar observations of vertical fluxes of sensible heat and meteoric Na from 78 to 110 km in late May 2020 at McMurdo, Antarctica. The measurements include contributions from the complete temporal spectrum of gravity waves and demonstrate that wave-induced vertical transport associated with atmospheric mixing by non-breaking gravity waves, Stokes drift imparted by the wave spectrum, and perturbed chemistry of reactive species, can make significant contributions to constituent and heat transport in the mesosphere and lower thermosphere (MLT). The measured sensible heat and Na fluxes exhibit downward peaks at 84 km (−3.0 Kms−1 and −5.5 × 104 cm−2s−1) that are ∼4 km lower than the flux peak altitudes observed at midlatitudes. This is likely caused by the strong downwelling over McMurdo in late May. The Na flux magnitude is double the maximum at midlatitudes, which we believe is related to strong persistent gravity waves in the MLT at McMurdo. To achieve good agreement between the measured Na flux and theory, it was necessary to infer that a large fraction of gravity wave energy was propagating downward, especially between 80 and 95 km where the Na flux and wave dissipation were largest. These downward propagating waves are likely secondary waves generated in-situ by the dissipation of primary waves that originate from lower altitudes. The sensible heat flux transitions from downward below 90 km to upward from 97 to 106 km. The observations are explained with the fully compressible solutions for polarization relations of primary and secondary gravity waves with λ z > 10 km.
AB - We report the first lidar observations of vertical fluxes of sensible heat and meteoric Na from 78 to 110 km in late May 2020 at McMurdo, Antarctica. The measurements include contributions from the complete temporal spectrum of gravity waves and demonstrate that wave-induced vertical transport associated with atmospheric mixing by non-breaking gravity waves, Stokes drift imparted by the wave spectrum, and perturbed chemistry of reactive species, can make significant contributions to constituent and heat transport in the mesosphere and lower thermosphere (MLT). The measured sensible heat and Na fluxes exhibit downward peaks at 84 km (−3.0 Kms−1 and −5.5 × 104 cm−2s−1) that are ∼4 km lower than the flux peak altitudes observed at midlatitudes. This is likely caused by the strong downwelling over McMurdo in late May. The Na flux magnitude is double the maximum at midlatitudes, which we believe is related to strong persistent gravity waves in the MLT at McMurdo. To achieve good agreement between the measured Na flux and theory, it was necessary to infer that a large fraction of gravity wave energy was propagating downward, especially between 80 and 95 km where the Na flux and wave dissipation were largest. These downward propagating waves are likely secondary waves generated in-situ by the dissipation of primary waves that originate from lower altitudes. The sensible heat flux transitions from downward below 90 km to upward from 97 to 106 km. The observations are explained with the fully compressible solutions for polarization relations of primary and secondary gravity waves with λ z > 10 km.
KW - Antarctica gravity waves
KW - constituent and heat transport
KW - fully compressible polarization relations
KW - lidar
KW - secondary gravity wave generation
KW - vertical fluxes of sensible heat and meteoric Na
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U2 - 10.1029/2021JD035728
DO - 10.1029/2021JD035728
M3 - Article
AN - SCOPUS:85137989334
SN - 2169-897X
VL - 127
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
IS - 16
M1 - e2021JD035728
ER -