Remote Sensing of Mesosphere and Lower Thermosphere Dynamical Tracers from Space

A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Atmospheric Techniques, Instruments, and Modeling".

Deadline for manuscript submissions: closed (30 October 2020) | Viewed by 2471

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,

Remote observations of long-lived trace gases in the mesosphere and lower thermosphere (MLT), depicting the dynamics of this atmospheric region, are often used to quantify dynamical phenomena that are otherwise difficult to measure (i.e., winds, waves, diffusion, etc.). Over the past few decades, satellite technology has provided a wealth of global measurements of tracers’ distributions in the MLT, which have already reached a continuous coverage over close to two solar cycles from single instruments in some cases. The availability of these datasets has resulted in a big step forward in understanding the dynamics of the MLT, i.e., global circulation, wave­–wave and wave–mean flow interactions, coupling to atmospheric regions below and above, name a few "after" response to sudden stratospheric warmings.

There are no clear prospects of a space mission being launched in the near future with the main objective of monitoring tracers with coverage from the lower mesosphere to the lower thermosphere. Providing continuity to the present observations is crucial for tracking variations of the MLT dynamics, particularly under a changing climate scenario. Moreover, it is critical to identify causes for disagreement between available measurements, not only in order to build up merged datasets to determine long-term variations, but also to provide recommendations for future instrumentation.

In the advent of a potential time gap in MLT tracer monitoring in the case of undesired failure of the space instruments currently in operation, it is timely to assess the quality of the available datasets, their drifts due to aging, the reasons for disagreement between datasets, and the pitfalls in their merging. This should be done for at least three reasons: (i) for an accurate evaluation of the climate change impact on MLT dynamics; (ii) because these datasets are used as diagnostics for accuracy of numerical model simulations and contribute to improvement of predictions; and (iii) with the ultimate aim of providing the scenario for future developments. In addition, it is also timely to highlight achievements in the knowledge of the dynamics of the MLT using available tracer datasets in order to demonstrate their need to decision makers.

In this Special Issue, we welcome manuscripts describing tracer measurements from space and evaluating their quality, more specifically related to the following aspects:

  • Retrievals, uncertainties, and error assessment;
  • Comparisons between datasets (including ground-based observations) and evaluation of biases or instrumental drifts;
  • Climatologies and variations at any time-scale;
  • Recommendations for future satellite instrumentation (and also ground-based instrumentation in support to satellite technology).

Manuscripts highlighting the value of tracers’ observations from space through comparisons with model simulations or including scientific analysis and broadening the knowledge on MLT dynamics are also more than welcome.

Dr. Maya Garcia Comas
Guest Editor

Manuscript Submission Information

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Keywords

  • Mesosphere and lower thermosphere
  • Dynamics
  • Tracers
  • Remote sensing
  • Future instrumentation
  • Climate change

Published Papers (1 paper)

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Research

17 pages, 5079 KiB  
Article
Initial Results of Meteor Wind with Langfang Medium Frequency Radar
by Bing Cai, Qingchen Xu, Xiong Hu and Junfeng Yang
Atmosphere 2020, 11(5), 507; https://doi.org/10.3390/atmos11050507 - 14 May 2020
Cited by 2 | Viewed by 2059
Abstract
We conducted meteor observations during the Leonid meteor shower on 16 November 2017 and 17 November 2018 with Langfang medium frequency (MF) radar (116° E, 40° N). This was the first nighttime meteor observation by MF radar in mid-latitude China. The observation period [...] Read more.
We conducted meteor observations during the Leonid meteor shower on 16 November 2017 and 17 November 2018 with Langfang medium frequency (MF) radar (116° E, 40° N). This was the first nighttime meteor observation by MF radar in mid-latitude China. The observation period was 12:00–22:00 (UT) and the observation range was 78–150 km. By using broad vertical beams, totally 94 and 92 meteor echoes were obtained, along with their spatial, time and height distribution. Quite a few meteor echoes are within 30° zenith angles, from the southwest direction, and with a mean height of 107 km which is almost 10 km higher than traditional VHF (Very High Frequency) meteor radar observations. Initial bi-hourly and nightly averaged wind profiles were calculated, and well fitted the wind estimations by co-located VHF meteor radar at the altitude of 100–110 km. On the other side, echoes around 140 km are successfully detected in our observation, which may suggest that for most running MF radars, meteor echoes around 140 km altitude could be detected with a sampling pulse frequency less than 100 Hz. Full article
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