There have been years of discussion and controversy about the existence of
very thin and stable temperature sheets and their relationship to the VHF r
adar aspect sensitivity. It is only recently that very high-resolution insi
tu temperature observations have brought credence to the reality and ubiqui
ty 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 ob
tain outside of the planetary boundary layer. They have only been carried o
ut up to the lower stratosphere by Service d'Aeronomie (CNRS, France) for a
bout 10 years. The controversy also persisted due to the volume resolution
of the (Mesosphere)-Stratosphere-Troposphere VHF radars which is coarse wit
h respect to sheet thickness, although widely sufficient for meteorological
or meso-scale investigations. The contribution within the range gate of ma
ny of these structures, which are advected by the wind, and decay and grow
at different instants and could be distorted either by internal gravity wav
es or turbulence fields, could lead to radar echoes with statistical proper
ties similar to those produced by anisotropic turbulence. Some questions th
us remain regarding the manner in which temperature sheets contribute to VH
F radar echoes. In particular, the zenithal and azimuthal angular dependenc
e of the echo power may not only be produced by diffuse reflection on stabl
e distorted or corrugated sheets, but also by extra contributions from anis
otropic turbulence occurring in the stratified atmosphere. Thus, for severa
l years, efforts have been put forth to improve the radar height resolution
in order to better describe thin structures. Frequency interferometric tec
hniques are widely used and have been recently further developed with the i
mplementation of high-resolution data processings. We begin by reviewing br
iefly some characteristics of the ST radar echoes with a particular emphasi
s on recent works. Their possible coupling with stable sheets is then prese
nted and their known characteristics are described with some hypotheses con
cerning their generation mechanisms. Finally, measurement campaigns that to
ok recently place or will be carried out in the near future for improving o
ur knowledge of these small-scale structures are presented briefly.