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A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Meteorology".

Deadline for manuscript submissions: closed (1 October 2020) | Viewed by 48725

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Special Issue Editors

Dr. Xin Xu

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Guest Editor

School of Atmospheric Sciences, Nanjing University, Nanjing 210023, China
Interests: gravity wave dynamics; parameterization; mesoscale convective systems

Dr. Miguel Teixeira

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Guest Editor

Department of Meteorology, University of Reading, Reading RG6 6BB, UK
Interests: gravity waves; orographic flows; turbulence; fluid dynamics

Dr. Manuel Pulido

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Guest Editor

Department of Meteorology, University of Reading, Reading RG6 6BB, UK
Interests: data assimilation; atmospheric gravity waves; parameterizations

Dr. Junhong Wei

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Guest Editor

School of Atmospheric Sciences, Sun Yat-sen University, Guangzhou 510275, China
Interests: jet-front gravity wave dynamics; moist convection; gravity wave parameterization; ray tracing technique

Special Issue Information

Dear Colleagues,

Gravity waves in the atmosphere have a variety of sources, including topography, moist convection, and jet-frontal systems. The momentum transport by gravity waves is of great importance to the atmospheric circulation, structure and variability, especially in the middle atmosphere. Gravity waves are also closely related to various severe weather phenomena, such as downslope windstorms, orographic precipitation and clear-air turbulence. There are many open questions regarding the fundamental dynamics of gravity waves, namely their genesis, maintenance, propagation and breaking, as well as the interaction of gravity waves with boundary layer processes, larger-scale waves and the mean flow. Moreover, observations of gravity waves at all scales are critical for better constraining gravity wave drag parameterizations implemented in numerical weather prediction and climate models. The estimation of gravity wave parameters from observational information, using inverse or data assimilation techniques, is therefore an urgent need.

We invite you to submit your research for publication in this Special Issue, which aims to improve the understanding of atmospheric gravity waves through a selection of papers. Both original research and review papers are welcome. We encourage contributions to topics including but not limited to:

Gravity wave dynamics;
Observations of gravity waves by means of remote sensing and in situ instruments;
Climate effects of gravity waves;
Gravity waves and severe weather;
Parameterization of gravity waves;
Clear air turbulence generation by gravity waves;
Data assimilation of gravity waves.

Dr. Xin Xu
Dr. Miguel Teixeira
Dr. Manuel Pulido
Dr. Junhong Wei

Guest Editors

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Keywords

gravity wave dynamics
gravity wave observation
parameterization schemes
large-scale circulation and climate
convective systems
jet streams
polar vortex
tropical oscillations
boundary layer process
clear air turbulence
downslope windstorms
data assimilation

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Published Papers (13 papers)

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Research

27 pages, 5883 KiB

Open AccessArticle

Investigating the Spatio-Temporal Distribution of Gravity Wave Potential Energy over the Equatorial Region Using the ERA5 Reanalysis Data

by Shih-Sian Yang, Chen-Jeih Pan and Uma Das

Atmosphere 2021, 12(3), 311; https://doi.org/10.3390/atmos12030311 - 27 Feb 2021

Cited by 6 | Viewed by 2807

Abstract

Atmospheric gravity waves play a crucial role in affecting atmospheric circulation, energy transportation, thermal structure, and chemical composition. Using ERA5 temperature data, the present study investigates the tropospheric to the lower mesospheric gravity wave potential energy (E_P) over the equatorial region to understand the vertical coupling of the atmosphere. E_P is mainly controlled by two factors. The first is zonal wind through wave–mean flow interactions, and thus E_P has periodic variations that are correlated to the zonal wind oscillations and enhances around the altitudes of zero-wind shears where the zonal wind reverses. The second is the convections caused by atmospheric circulations and warm oceans, resulting in longitudinal variability in E_P. The lower stratospheric and the lower mesospheric E_P are negatively correlated. However, warm oceanic conditions can break this wave energy coupling and further enhance the lower mesospheric E_P. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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12 pages, 7978 KiB

Open AccessArticle

Performance Evaluation of Sub-Grid Orographic Parameterization in the WRF Model over Complex Terrain in Central Asia

by Huoqing Li, Junjian Liu, Hailiang Zhang, Chenxiang Ju, Junjie Shi, Junlan Zhang, Ali Mamtimin and Shuiyong Fan

Atmosphere 2020, 11(11), 1164; https://doi.org/10.3390/atmos11111164 - 28 Oct 2020

Cited by 2 | Viewed by 3099

Abstract

The terrain of Central Asia is complex and rugged over mountains. Consequently, wind speed is overestimated over mountains and plains when using the Weather Research Forecast (WRF) model in winter. To solve this problem, three different simulations (named as control simulation (CRTL), gravity waves (GWD), and flow-blocking drag (FBD), respectively) were designed to investigate the impact of sub-grid orography (gravity waves and flow-blocking drag) on wind forecasts. The results illustrated that near-surface wind-speed overestimations were alleviated when sub-grid orographic drag was used in GWD, though the upper-level wind fields at 500 hPa were excessively reduced compared to CRTL. Thus, we propose eliminating the gravity wave breaking at the upper level to improve upper-level wind underestimations and surface wind speeds at the same time. The sub-grid orographic drag stress of the vertical profile over mountains was reduced when only the flow-blocking drag was retained in FBD. This alleviated underestimations of the upper-level wind speed and near-surface wind, which both have the same positive effects as the gravity wave and flow-blocking total. The mean bias and root mean squared error reduced by 32.76% and 9.39%, respectively, compared to CRTL. Moreover, the temperature and specific humidity in the lower troposphere were indirectly improved. The results of the study demonstrate that it is better to remove sub-grid orographic gravity wave drag when using the gravity wave drag scheme of the WRF model. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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15 pages, 4521 KiB

Open AccessFeature PaperArticle

The Response of Parameterized Orographic Gravity Waves to Rapid Warming over the Tibetan Plateau

by Runqiu Li, Xin Xu, Yuan Wang, Miguel A. C. Teixeira, Jianping Tang and Yixiong Lu

Atmosphere 2020, 11(9), 1016; https://doi.org/10.3390/atmos11091016 - 22 Sep 2020

Cited by 4 | Viewed by 3751

Abstract

Using the ERA-Interim reanalysis during 1979–2017, this work for the first time investigates the climatology and long-term trend of orographic gravity waves (OGWs) in the Tibetan Plateau (TP). The linkage between the trends of OGWs and the rapid warming over the TP is also studied. Climatologically, the most prominent surface wave momentum flux (SWMF) of OGWs occurs in the western and southeastern TP, while it is weak in the central TP. The SWMF is stronger in winter and spring than in autumn and summer. Overall, the mean SWMF over the TP experienced a weak decreasing trend. The decrease of SWMF mainly took place in the western and southeastern TP in spring. However, increasing trends were found in the central TP in winter. Changes of SWMF are mainly caused by the changes of horizontal wind near the surface, while buoyancy frequency and air density play a minor role. In response to the inhomogeneous warming over the TP, the surface winds were adjusted through thermal wind balance. In spring (winter), the most remarkable warming occurred in the northern (southern) TP, which reduced (enhanced) the meridional temperature gradient across the plateau, and thus led to a deceleration (acceleration) of the horizontal wind. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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12 pages, 2281 KiB

Open AccessEditor’s ChoiceArticle

Dynamics of Mechanical Oscillator Mechanism for Stratospheric Gravity Waves Generated by Convection

by Shiwang Yu, Lifeng Zhang, Ming Zhang and Yuan Wang

Atmosphere 2020, 11(9), 942; https://doi.org/10.3390/atmos11090942 - 3 Sep 2020

Cited by 1 | Viewed by 2353

Abstract

The mechanical oscillator mechanism (MOM) for stratospheric gravity waves generated by convection is investigated with a dynamics model using the two-dimensional, nonhydrostatic and linear governing equations based on the Boussinesq approximation. The model is solved analytically with a fixed buoyancy oscillation (BO) at the tropopause as the boundary conditions. Results show that this BO is the source of stratospheric gravity waves and the MOM is the generation mechanism. The characteristics of the stratospheric gravity waves not only depend on the BO, but also rely on the stratospheric state, such as the background wind and the buoyancy frequency. When the vertical wavenumbers of the stratospheric gravity waves are close to those of the intrinsic characteristic waves (ICWs), which are the model solution without BO forcing at the tropopause, resonance occurs. Under the resonance conditions, the amplitudes of the stratospheric gravity waves increase significantly, even for low BO intensity. The background wind in the stratosphere has a large effect on wave resonance. Finally, numerical simulation results of a low-vortex system also verify that the MOM is the generation mechanism of stratospheric gravity waves generated by convection. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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13 pages, 1828 KiB

Open AccessArticle

Diurnal Characteristics of Gravity Waves over the Tibetan Plateau in 2015 Summer Using 10-km Downscaled Simulations from WRF-EnKF Regional Reanalysis

by Tingting Qian, Fuqing Zhang, Junhong Wei, Jie He and Yinghui Lu

Atmosphere 2020, 11(6), 631; https://doi.org/10.3390/atmos11060631 - 14 Jun 2020

Cited by 7 | Viewed by 2811

Abstract

Diurnal variations of gravity waves over the Tibetan Plateau (TP) in summer 2015 were investigated based on high-resolution downscaled simulations from WRF-EnKF (Weather Research and Forecasting model and an ensemble Kalman filter) regional reanalysis data with particular emphasis on wave source, wave momentum fluxes and wave energies. Strong diurnal precipitations, which mainly happen along the south slope of the TP, tend to excite upward-propagating gravity waves. The spatial and temporal distributions of the momentum fluxes of small-scale (10–200 km) and meso-scale (200–500 km) gravity waves agree well with the diurnal precipitation distributions. The power spectra of momentum fluxes also show that the small- and meso-scale atmospheric processes become important during the period of the strongest rainfall. Eastward momentum fluxes and northward momentum fluxes are dominant. Wave energies are described in terms of kinetic energy (KE), potential energy (PE) and vertical fluctuation energy (VE). The diurnal variation and spatial distribution of VE in the lower stratosphere correspond to the diurnal rainfall in the troposphere. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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14 pages, 8114 KiB

Open AccessArticle

Extraction of Quasi-Monochromatic Gravity Waves from an Airglow Imager Network

by Chang Lai, Wei Li, Jiyao Xu, Xiao Liu, Wei Yuan, Jia Yue and Qinzeng Li

Atmosphere 2020, 11(6), 615; https://doi.org/10.3390/atmos11060615 - 10 Jun 2020

Cited by 2 | Viewed by 2952

Abstract

An algorithm has been developed to isolate the gravity waves (GWs) of different scales from airglow images. Based on the discrete wavelet transform, the images are decomposed and then reconstructed in a series of mutually orthogonal spaces, each of which takes a Daubechies (db) wavelet of a certain scale as a basis vector. The GWs in the original airglow image are stripped to the peeled image reconstructed in each space, and the scale of wave patterns in a peeled image corresponds to the scale of the db wavelet as a basis vector. In each reconstructed image, the extracted GW is quasi-monochromatic. An adaptive band-pass filter is applied to enhance the GW structures. From an ensembled airglow image with a coverage of 2100 km × 1200 km using an all-sky airglow imager (ASAI) network, the quasi-monochromatic wave patterns are extracted using this algorithm. GWs range from ripples with short wavelength of 20 km to medium-scale GWs with a wavelength of 590 km. The images are denoised, and the propagating characteristics of GWs with different wavelengths are derived separately. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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17 pages, 12839 KiB

Open AccessArticle

Improved Simulation of the Antarctic Stratospheric Final Warming by Modifying the Orographic Gravity Wave Parameterization in the Beijing Climate Center Atmospheric General Circulation Model

by Yixiong Lu, Tongwen Wu, Xin Xu, Li Zhang and Min Chu

Atmosphere 2020, 11(6), 576; https://doi.org/10.3390/atmos11060576 - 1 Jun 2020

Cited by 6 | Viewed by 5972

Abstract

The Antarctic stratospheric final warming (SFW) is usually simulated with a substantial delay in climate models, and the corresponding temperatures in austral spring are lower than observations, implying insufficient stratospheric wave drag. To investigate the role of orographic gravity wave drag (GWD) in modeling the Antarctic SFW, in this study the orographic GWD parameterization scheme is modified in the middle-atmosphere version of the Beijing Climate Center Atmospheric General Circulation Model. A pair of simulations are conducted to compare two orographic GWD schemes in simulating the breakdown of the stratospheric polar vortex over Antarctica. The control simulation with the default orographic GWD scheme exhibits delayed vortex breakdown and the cold-pole bias seen in most climate models. In the simulation with modified orographic GWD scheme, the simulated vortex breaks down earlier by 8 days, and the associated cold-pole bias is reduced by more than 2 K. The modified scheme provides stronger orographic GWD in the lower stratosphere, which drives an accelerated polar downwelling branch of the Brewer–Dobson circulation and, in turn, produces adiabatic warming. Our study suggests that modifying orographic GWD parameterizations in climate models would be a valid way of improving the SFW simulation over Antarctica. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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26 pages, 11617 KiB

Open AccessArticle

Morphology of the Wavenumber 1 and Wavenumber 2 Stratospheric Kelvin Waves Using the Long-Term Era-Interim Reanalysis Dataset

by Chen-Jeih Pan, Shih-Sian Yang, Uma Das and Wei-Sheng Chen

Atmosphere 2020, 11(4), 421; https://doi.org/10.3390/atmos11040421 - 22 Apr 2020

Cited by 2 | Viewed by 2778

Abstract

The atmospheric Kelvin wave has been widely studied due to its importance in atmospheric dynamics. Since a long-term climatological study is absent in the literature, we have employed the two-dimensional fast Fourier transform (2D-FFT) method for the 40-year long-term reanalysis of the dataset, ERA-Interim, to investigate the properties of Kelvin waves with wavenumbers 1 (E1) and 2 (E2) at 6–24 days wave periods over the equatorial region of ±10° latitude between a 15 and 45 km altitude during the period 1979–2019. The spatio-temporal variations of the E1 and E2 wave amplitudes were compared to the information of stratospheric quasi-biennial oscillation (QBO), and the wave amplitudes were found to have an inter-QBO cycle variation that was related to sea surface temperature and convections, as well as an intra-QBO cycle variation that was caused by interactions between the waves and stratospheric mean flows. Also, the E1 waves with 6–10 day periods and the E2 waves with 6 days period were observed to penetrate the westerly regime of QBO, which has a thickness less than the vertical wavelengths of those waves, and the waves could further propagate upward to higher altitudes. In a case study of the period 2006–2013, the wave amplitudes showed a good correlation with the Niño 3.4 index, outgoing longwave radiation (OLR), and precipitation during 2006–2013, though this was not the case for the full time series. The present paper is the first report on the 40-year climatology of Kelvin waves, and the morphology of Kelvin waves will help us diagnose the anomalies of wave activity and QBO in the future. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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20 pages, 6577 KiB

Open AccessArticle

Statistical Analysis of Turbulence Characteristics over the Tropical Western Pacific Based on Radiosonde Data

by Yang He, Zheng Sheng, Lesong Zhou, Mingyuan He and Shudao Zhou

Atmosphere 2020, 11(4), 386; https://doi.org/10.3390/atmos11040386 - 14 Apr 2020

Cited by 10 | Viewed by 3390

Abstract

The tropical region is a key area for the interaction between the stratosphere and troposphere. The strong convective activity in the troposphere produces a series of gravity wave activities, which result in strong and widespread turbulence over the region. Therefore, studying the turbulent activity in the western Pacific is essential for understanding the characteristics of atmospheric disturbance over this region, which has the world’s most complex circulation system. In this paper, we explore the characteristics of atmospheric turbulence distribution over Guam in this region, and the Thorpe sorting method is used to study one-second resolution radiosonde data from the US. On the basis of the background field and local instability, the turbulence generation mechanism is discussed in detail. Results show that the US high-resolution balloon data are efficacious for tropospheric turbulence retrieval but increasingly affected by instrument noise as altitude increases. It is also found that there is a strong turbulent mixing band caused by both shear instability and static instability near the tropopause, where the turbulence activity is markedly enhanced and characterized by annual oscillation, reaching the maximum from July to September. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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14 pages, 2950 KiB

Open AccessArticle

Retrieval and Analysis of the Strongest Mixed Layer in the Troposphere

by Zheng Sheng, Lesong Zhou and Yang He

Atmosphere 2020, 11(3), 264; https://doi.org/10.3390/atmos11030264 - 6 Mar 2020

Cited by 13 | Viewed by 3132

Abstract

In this article, Thorpe analysis, which often retrieves the characteristics of mixing in the free atmosphere from balloon sounding data, is applied to the data of the Constellation Observing System for Meteorology, Ionosphere and Climate (COSMIC). We find that the COSMIC data can well retrieve the strongest mixed layer in the troposphere (SMLT) altitude, and can reveal the basic variation trend of the SMLT thickness and Thorpe scale

L_{T}

. We use COSMIC data to reveal the global spatial and temporal distribution of the SMLT from 2007 to 2015 and analyze the fluctuation period of the SMLT altitude with Hilbert–Huang transform (HHT), we find that the variation of the SMLT altitude is influenced by the dual effects of terrain and solar radiation. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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17 pages, 3023 KiB

Open AccessArticle

Spectral Analysis of Gravity Waves from Near Space High-Resolution Balloon Data in Northwest China

by Yang He, Zheng Sheng and Mingyuan He

Atmosphere 2020, 11(2), 133; https://doi.org/10.3390/atmos11020133 - 24 Jan 2020

Cited by 32 | Viewed by 4962

Abstract

Using a set of near space high-resolution balloon data released in Hami, Xinjiang, we explored the spectral characteristics of temperature fluctuations and three-dimensional wind field fluctuations. As different from previous studies, which were based on radiosondes, we have increased the height range of spectral analysis to the stratosphere (38 km), which can explore the variation of spectral features with altitude, and can analyze higher wavenumber regions. The results show that horizontal wind field disturbances are isotropic, meridional and zonal winds have relatively consistent spectral structures, while vertical wind fluctuations have completely different spectral structures, which cannot be explained by the existing “universal spectrum” theory. The observed spectrum of horizontal wind field can be explained well by the “wind-shifting” theory. The ratio of spectral kinetic energy to potential energy is approximately constant only in the high wavenumber region but it varies at different height intervals. This study is a necessary extension of the observation for the characteristics of the vertical wavenumber spectrum in northwestern China, and it is also an experimental observation of spectral characteristics using radiosonde data at higher altitudes. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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10 pages, 3313 KiB

Open AccessArticle

Sampling Errors in Observed Gravity Wave Momentum Fluxes from Vertical and Tilted Profiles

by Simon B. Vosper and Andrew N. Ross

Atmosphere 2020, 11(1), 57; https://doi.org/10.3390/atmos11010057 - 2 Jan 2020

Cited by 4 | Viewed by 3447

Abstract

Observations from radiosondes or from vertically pointing remote sensing profilers are often used to estimate the vertical flux of momentum due to gravity waves. For planar, monochromatic waves, these vertically integrated fluxes are equal to the phase averaged flux and equivalent to the horizontal averaging used to deduce momentum flux from aircraft data or in numerical models. Using a simple analytical solution for two-dimensional hydrostatic gravity waves over an isolated ridge, it is shown that this equivalence does not hold for mountain waves. For a vertical profile, the vertically integrated flux estimate is proportional to the horizontally integrated flux and decays with increasing distance of the profile location from the mountain. For tilted profiles, such as those obtained from radiosonde ascents, there is a further sampling error that increases as the trajectory extends beyond the localised wave field. The same sampling issues are seen when the effects of the Coriolis force on the gravity waves are taken into account. The conclusion of this work is that caution must be taken when using radiosondes or other vertical profiles to deduce mountain wave momentum fluxes. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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11 pages, 1200 KiB

Open AccessArticle

The Influence of Gravity Waves on Ice Saturation in the Tropical Tropopause Layer over Darwin, Australia

by Andrew M. Dzambo, Matthew H. Hitchman and Kai-Wei Chang

Atmosphere 2019, 10(12), 778; https://doi.org/10.3390/atmos10120778 - 5 Dec 2019

Cited by 1 | Viewed by 3144

Abstract

Gravity waves (GWs) in the tropical tropopause layer (TTL) can help dehydrate the lower stratosphere through rapid cooling events, but observational studies of GWs in the TTL are limited. Using a long-term, high-resolution radiosonde temperature dataset, an atmospheric state classification technique, and wavelet analysis, we characterize temperature perturbations generated by GWs in the TTL over Darwin, Australia across eight atmospheric states. We find a peak in GW power just above the tropical tropopause and a climatological maximum during peak monsoon season. While accounting for a chronic negative temperature bias near the tropical tropopause, we estimate that, in the upper troposphere, GWs impose a 2 K temperature perturbation during non-monsoon states and a 3 K temperature perturbation during the monsoon states, with corresponding values of 5 K and 6 K in the upper TTL. A 3 K negative temperature perturbation will lead to significant perturbations in relative humidity with respect to ice, which has implications for environmental ice number concentrations and TTL cloud fraction. Full article

(This article belongs to the Special Issue Gravity Waves in the Atmosphere)

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