Changes in the Stratosphere, Mesosphere and Lower Thermosphere Composition and Thermal Structure

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

Deadline for manuscript submissions: closed (15 September 2018) | Viewed by 10305

Special Issue Editor


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Guest Editor
Instituto de Astrofísica deAndalucía (IAA-CSIC), 18008 Granada, Spain
Interests: mesosphere and lower themosphere (MLT) thermal; chemical and dynamical structure; MLT variability; long-term trends; non-LTE modeling; IR observations; airglow; atmospheric variable retrievals
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Special Issue Information

Dear Colleagues,

The emission of gases at the surface impacts the atmosphere as a whole, from the ground to the upper thermosphere. There is a deep interest in the determination of the induced changes in the stratosphere, mesosphere and lower thermosphere (SMLT) composition and temperature, and the understanding of coupling processes with other atmospheric regions, feedback mechanisms and interactions with climate. Variations in atmospheric constituents affect the energy budget, modifying temperatures and, ultimately, the extension of the atmosphere. They may also eventually alter the dynamics and phenomena propagating from and to other regions in the atmosphere. Changes of anthropogenic origin are superimposed to the considerable natural variability of this atmospheric region. Above all else, all these are interconnected and interaction between large-scale processes and the regional behavior also play a role.

Over the past decades, spaceborne and groundbased instrumentation have provided a wealth of observations of the SMLT. These have allowed for an unprecedented perception of the variability in the SMLT composition and thermal structure at multiple timescales, the interconnection with lower and upper regions and the influence of the solar cycle. Nonetheless, the portrait of the changes in this region is not univocal. This is in part due to limitations in the observations, which lead to sampling biases and disagreements between instruments.

This Special Issue calls for papers addressing the study of the SMLT temperature and composition and providing insights on variations at any timescale and their evolution from an observational perspective, either from space, from the ground or from a combination of them, and either at a local or a global scale. Discussions on effects from sampling biases and other sources of uncertainties are more than welcome. Contributions may cover any of the following topics:

- SMLT monitoring, climatologies, observational evidence for long-term changes, identification of drivers;
- Characterization of diurnal, seasonal and interannual variability and their evolution;
- Effect of gravity waves, planetary waves and tides and its evolution;
- Influence of the sun on SMLT variability;
- SMLT coupling processes with lower and upper atmospheric regions and their variability;
- Comparisons between instruments, determination of sampling biases and uncertainties, effect on the interpretation of variabilities at any timescale;
- Role of natural variability in secular trends, impact of short and mid-term variations on long-term trend estimates.

Dr. Maya Garcia-Comas
Guest Editor

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Keywords

  • stratosphere, mesosphere, lower thermosphere observations
  • temperature and constituent abundances
  • atmospheric waves
  • atmospheric variability
  • climatologies and trends
  • atmospheric coupling

Published Papers (3 papers)

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Research

14 pages, 2827 KiB  
Article
A Case Study of the Stratospheric and Mesospheric Concentric Gravity Waves Excited by Thunderstorm in Northern China
by Ying Wen, Qilin Zhang, Haiyang Gao, Jiyao Xu and Qinzeng Li
Atmosphere 2018, 9(12), 489; https://0-doi-org.brum.beds.ac.uk/10.3390/atmos9120489 - 10 Dec 2018
Cited by 7 | Viewed by 3124
Abstract
In this paper, the complete process in which a concentric gravity wave (CGW), excited by a tropospheric thunderstorm, propagated into the stratosphere and mesosphere in Northern China is investigated. A strong thunderstorm developed in the middle of the Inner Mongolia autonomous region on [...] Read more.
In this paper, the complete process in which a concentric gravity wave (CGW), excited by a tropospheric thunderstorm, propagated into the stratosphere and mesosphere in Northern China is investigated. A strong thunderstorm developed in the middle of the Inner Mongolia autonomous region on the night of 10th August 2013. The stratospheric temperature perturbation, caused by the CGW, was observed by the Atmospheric Infrared Sounder (AIRS) at 02:11 LT 11th August 2013. An all-sky OH imager at the Shuozhou station (39.8° N, 112.1° E), supported by the Meridian Space Weather Monitoring Project, measured the mesospheric CGW between 22:00 LT to 23:00 LT on the night. It was certified that both the stratospheric and mesospheric CGWs were triggered by the aforementioned thunderstorm, and the excitation source was calculated to be located at (40.59° N, 108.67° E) by employing the dispersion relation. The CGWs were excited in the initial stage of the thunderstorm. The temperature and wind field data obtained by SABER and meteoric radar, respectively, were used to evaluate the background properties of the respective propagation regions. The result shows that an obvious thermal duct structure, with a positive squared vertical wavenumber (m2) existed around the OH layer. Full article
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14 pages, 2741 KiB  
Article
On the Roles of Advection and Solar Heating in Seasonal Variation of the Migrating Diurnal Tide in the Stratosphere, Mesosphere, and Lower Thermosphere
by Hongping Gu and Jian Du
Atmosphere 2018, 9(11), 440; https://0-doi-org.brum.beds.ac.uk/10.3390/atmos9110440 - 12 Nov 2018
Cited by 7 | Viewed by 3923
Abstract
The migrating diurnal tide (DW1) presents a unique latitudinal structure in the stratosphere, mesosphere, and lower thermosphere. In this paper, the physical mechanisms that govern its seasonal variation are examined in these three regions using the 31.5-year (1979–2010) output from the extended Canadian [...] Read more.
The migrating diurnal tide (DW1) presents a unique latitudinal structure in the stratosphere, mesosphere, and lower thermosphere. In this paper, the physical mechanisms that govern its seasonal variation are examined in these three regions using the 31.5-year (1979–2010) output from the extended Canadian Middle Atmosphere Model (eCMAM30). DW1 annual variation in the stratosphere is mainly controlled by the short-wave heating in the high latitudes, but by both the short-wave and adiabatic heating in the low latitudes. In the mesosphere, linear and nonlinear advection play important roles in the semiannual variation of the tide whereas short-wave heating does not. In the lower thermosphere, the annual variation of DW1 is mainly governed by the short-wave heating and linear advection. This study illustrates the complexity of the main physical mechanisms modulating the seasonal variations of DW1 in different regions of the atmosphere. Full article
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14 pages, 2526 KiB  
Article
Statistics on Nonmigrating Diurnal Tides Generated by Tide-Planetary Wave Interaction and Their Relationship to Sudden Stratospheric Warming
by Xiaojuan Niu, Jian Du and Xuwen Zhu
Atmosphere 2018, 9(11), 416; https://0-doi-org.brum.beds.ac.uk/10.3390/atmos9110416 - 25 Oct 2018
Cited by 3 | Viewed by 2744
Abstract
The nonmigrating diurnal tide, DW2, is known to have a source from the stationary planetary wave with wavenumber 1 (SPW1) and the migrating diurnal tide (DW1) interaction. Recent research has shown that DW2 time evolution in the equatorial mesopause tracks very well with [...] Read more.
The nonmigrating diurnal tide, DW2, is known to have a source from the stationary planetary wave with wavenumber 1 (SPW1) and the migrating diurnal tide (DW1) interaction. Recent research has shown that DW2 time evolution in the equatorial mesopause tracks very well with SPW1 in the polar stratosphere for the winter of 2009–2010, which contains a sudden stratospheric warming (SSW) vortex split event. This paper extends previous research and investigates the relationship between these two waves for 31 winters from 1979 to 2010 with the extended Canadian Middle Atmosphere Model (eCMAM) through correlation and composite analysis. Significant correlations are present between the two waves in 20 out of 31 winters (65%). We separate the 31 winters into four categories: SSW-displacement, SSW-split, minor-SSW, and no-SSW. Our results show that there is no significant difference among the four categories in terms of correlations between the two waves. Although SPW1 is usually stronger during a SSW-D winter, this does not warrant a stronger interaction with DW2. Full article
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