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| Hauptseite > Publikationsdatenbank > Secondary Gravity Waves From the Stratospheric Polar Vortex Over ALOMAR Observatory on 12–14 January 2016: Observations and Modeling > print |
| Hauptseite > Publikationsdatenbank > Secondary Gravity Waves From the Stratospheric Polar Vortex Over ALOMAR Observatory on 12–14 January 2016: Observations and Modeling > print |
| 001 | 943409 | ||
| 005 | 20260122224323.0 | ||
| 024 | 7 | _ | |2 doi |a 10.1029/2022JD036985 |
| 024 | 7 | _ | |2 ISSN |a 0148-0227 |
| 024 | 7 | _ | |2 ISSN |a 2156-2202 |
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| 100 | 1 | _ | |0 0000-0002-6459-005X |a Vadas, Sharon L. |b 0 |e Corresponding author |
| 245 | _ | _ | |a Secondary Gravity Waves From the Stratospheric Polar Vortex Over ALOMAR Observatory on 12–14 January 2016: Observations and Modeling |
| 260 | _ | _ | |a Hoboken, NJ |b Wiley |c 2023 |
| 336 | 7 | _ | |2 DRIVER |a article |
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| 520 | _ | _ | |a We analyze the gravity waves (GWs) observed by a Rayleigh lidar at the Arctic Lidar Observatory for Middle Atmosphere Research (ALOMAR) (16.08°E, 69.38°N) in Norway at z ∼ 20–85 km on 12–14 January 2016. These GWs propagate upward and downward away from zknee = 57 and 64 km at a horizontally-displaced location with periods τr ∼ 5–10 hr and vertical wavelengths λz ∼ 9–20 km. Because the hodographs are distorted, we introduce an alternative method to determine the GW parameters. We find that these GWs are medium to large-scale, and propagate north/northwestward with intrinsic horizontal phase speeds of ∼35–65 m/s. Since the GW parameters are similar above and below zknee, these are secondary GWs created by local body forces (LBFs) south/southeast of ALOMAR. We use the nudged HIAMCM (HIgh Altitude Mechanistic general Circulation Model) to model these events. Remarkably, the model reproduces similar GW structures over ALOMAR, with zknee = 58 and 66 km. The event #1 GWs are created by a LBF at ∼35°E, ∼60°N, and z ∼ 58 km. This LBF is created by the breaking and dissipation of primary GWs generated and amplified by the imbalance of the polar night jet below the wind maximum; the primary GWs for this event are created at z ∼ 25–35 km at 49–53°N. We also find that the HIAMCM GWs agree well with those observed by the Atmospheric InfraRed Sounder (AIRS) satellite, and that those AIRS GWs south and north of ∼50°N over Europe are mainly mountain waves and GWs from the polar vortex, respectively. |
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| 773 | _ | _ | |0 PERI:(DE-600)2969341-X |a 10.1029/2022JD036985 |g Vol. 128, no. 2 |n 2 |p e2022JD036985 |t JGR / Atmospheres |v 128 |x 0148-0227 |y 2023 |
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