Abstract

Abstract. here have been years of discussion and controversy about the existence of very thin and stable temperature sheets and their relationship to the VHF radar aspect sensitivity. It is only recently that very high-resolution in situ temperature observations have brought credence to the reality and ubiquity of these structures in the free atmosphere and to their contribution to radar echo enhancements along the vertical. Indeed, measurements with very high-resolution sensors are still extremely rare and rather difficult to obtain outside of the planetary boundary layer. They have only been carried out up to the lower stratosphere by Service d’A´ eronomie (CNRS, France) for about 10 years. The controversy also persisted due to the volume resolution of the (Mesosphere)-Stratosphere-Troposphere VHF radars which is coarse with respect to sheet thickness, although widely sufficient for meteorological or mesoscale investigations. The contribution within the range gate of many of these structures, which are advected by the wind, and decay and grow at different instants and could be distorted either by internal gravity waves or turbulence fields, could lead to radar echoes with statistical properties similar to those produced by anisotropic turbulence. Some questions thus remain regarding the manner in which temperature sheets contribute to VHF radar echoes. In particular, the zenithal and azimuthal angular dependence of the echo power may not only be produced by diffuse reflection on stable distorted or corrugated sheets, but also by extra contributions from anisotropic turbulence occurring in the stratified atmosphere. Thus, for several years, efforts have been put forth to improve the radar height resolution in order to better describe thin structures. Frequency interferometric techniques are widely used and have been recently further developed with the implementation of high-resolution data processings. We begin by reviewing briefly some characteristics of the ST radar echoes with a particular emphasis on recent works. Their possible coupling with stable sheets is then presented and their known characteristics are described with some hypotheses concerning their generation mechanisms. Finally, measurement campaigns that took recently place or will be carried out in the near future for improving our knowledge of these small-scale structures are presented briefly.Key words. Meteorology and atmospheric dynamics (turbulence; instruments and techniques) – Radio Science (remote sensing)

Highlights

  • The Very High Frequency (VHF) Mesosphere-StratosphereTroposphere (MST) radars are dedicated to studying lower and middle atmosphere physics

  • Using the theoretical developments proposed by Hocking and Hamza (1997), many recent studies on the origin of aspect sensitivity indirectly point to the dominant contribution of atmospheric sheets to VHF radar echoes (e.g. Chen et al, 2000)

  • Most of the aspect sensitive echoing layers seen by ST radars in vertical incidence and in standard or imaging modes are very likely produced by these very thin sheets at least in the lower stratosphere

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Summary

Introduction

The Very High Frequency (VHF) Mesosphere-StratosphereTroposphere (MST) radars are dedicated to studying lower and middle atmosphere physics. We use the very broad definition introduced recently by Nastrom and Eaton (2001) which is based on the vertical domain of enhanced echo power and on the persistance of echoes as a signature of their horizontal extent Such a definition can be generalized to any direction of observation, but it is worth noting that it includes features of very different scales and of entirely different origins with a wide range of physical processes. For studies making use of in-situ observations, the vertical extent of atmospheric structures are essentially defined by the vertical gradient of the temperature (or refractive index). We introduce experiments that took place or will be carried out in the near future for improving our knowledge of these thin atmospheric structures

Aspect sensitivity of the VHF radar echoes
Biases on horizontal and vertical wind velocity measurements
Errors in isotropic turbulence parameter measurements
Stability measurements
Improved sensitivity along the vertical
Aspect sensitivity factor
Main characteristics of echo power
Height dependence
Frequency dependence of aspect sensitivity
Coherence of the aspect sensitive echoes
Azimuthal dependence of echo power
Aspect sensitivity associated with maximum echo power off zenith
Observations of echoing layers in standard mode
Observations at VHF with other modes
Observations with oversampling
Observations with dual Frequency Domain Interferometry technique
Observations with multi-Frequency Domain Interferometry technique
Various interpretations of aspect sensitive echoing layers
Observations in the free atmosphere
How are the temperature sheets generated?
Conclusions and perpectives
Doppler Beam Swinging technique
Beam Scanning technique
Broad-beam technique
Preset Multi-Beam Forming technique
Postset Beam Forming technique
Findings
Radar Imaging techniques with High-Resolution methods
Full Text
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