Enhancing the spatiotemporal features of polar mesosphere summer echoes using coherent MIMO and radar imaging at MAARSY

<p>Polar mesospheric summer echoes (PMSEs) are very strong radar echoes caused by the presence of ice particles, turbulence, and free electrons in the mesosphere over polar regions. For more than three decades, PMSEs have been used as natural tracers of the complicated atmospheric dynamics of...

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Bibliographic Details
Main Authors: J. M. Urco, J. L. Chau, T. Weber, R. Latteck
Format: Article
Language:English
Published: Copernicus Publications 2019-02-01
Series:Atmospheric Measurement Techniques
Online Access:https://www.atmos-meas-tech.net/12/955/2019/amt-12-955-2019.pdf
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Summary:<p>Polar mesospheric summer echoes (PMSEs) are very strong radar echoes caused by the presence of ice particles, turbulence, and free electrons in the mesosphere over polar regions. For more than three decades, PMSEs have been used as natural tracers of the complicated atmospheric dynamics of this region. Neutral winds and turbulence parameters have been obtained assuming PMSE horizontal homogeneity on scales of tens of kilometers. Recent radar imaging studies have shown that PMSEs are not homogeneous on these scales and instead they are composed of kilometer-scale structures. In this paper, we present a technique that allows PMSE observations with unprecedented angular resolution (<span class="inline-formula">∼0.6</span><span class="inline-formula"><sup>∘</sup></span>). The technique combines the concept of coherent MIMO (Multiple Input Multiple Output) and two high-resolution imaging techniques, i.e., Capon and maximum entropy (MaxEnt). The resulting resolution is evaluated by imaging specular meteor echoes. The gain in angular resolution compared to previous approaches using SIMO (Single Input Multiple Output) and Capon is at least a factor of 2; i.e., at 85&thinsp;km, we obtain a horizontal resolution of <span class="inline-formula">∼900</span>&thinsp;m. The advantage of the new technique is evaluated with two events of 3-D PMSE structures showing: (1) horizontal wavelengths of 8–10&thinsp;km and periods of 4–7&thinsp;min, drifting with the background wind, and (2) horizontal wavelengths of 12–16&thinsp;km and periods of 15–20&thinsp;min, not drifting with the background wind. Besides the advantages of the implemented technique, we discuss its current challenges, like the use of reduced power aperture and processing time, as well as the future opportunities for improving the understanding of the complex small-scale atmospheric dynamics behind PMSEs.</p>
ISSN:1867-1381
1867-8548