Studies of the atmosphere with the NERC MST radar at Aberystwyth, UK

Introduction

I continue to work with data collected by the NERC MST radar and ancillary systems located at Aberystwyth, UK.  The long series of observations available in the database stored at the BADC allows a wide range of atmospheric conditions to be examined. The large database also  allows new techniques to be tested on a large high-quality dataset..

The NERC MST radar facility at Aberystwyth (52.4oN, 4.1oW) operates at a frequency of 46.5MHz and has a peak transmitted power of 160kW. The antenna consists of a 20 by 20 array of four element Yagi aerials covering an area of 104m by 104m. The radar beam has a one-way half power width of 1.5 degrees and can be directed in sixteen possible directions, these directions being vertical and at angles of 4.2, 6, 8.5 and 12 degrees. Each of the four off-vertical beams can be pointed into four azimuth directions, the four six degree off-vertical beams used in this study are rotated 17.3 degrees anti-clockwise from north-east, south-east, south-west and north-west, respectively.

Atmospheric Turbulence Identificiation with VHF Radar

Turbulence in the atmosphere has a broad range of consequences. Among other things it can pose a hazard to aircraft and give rise to mixing between air masses which would otherwise remain distinct. Identification of turbulent regions is therefore useful because of the importance of turbulence in the vertical diffusion of pollutants. As indicated previously intense turbulence is also a significant hazard to aviation and thus the determination of the frequency and distribution of intense turbulence relative to other atmospheric phenomena is also of significant importance. Although instrumented aircraft and balloon-borne probes have important roles to play in studies of this phenomenon, their usefulness is limited to specific events. Radars, by contrast, offer the potential for continuous observations to be made over a wide altitude extent.

Turbulent regions are usually identified by the  spread of velocities within the signal portion of a VHF radar return Doppler spectrum since they in part represent the variance of vertical velocities arising from turbulent motions. However, the spectral width is also influenced by the horizontal wind speed as a result of the finite beam width. This so-called beam-broadening component tends to dominate the observed spectral widths for high wind speeds. The technique is therefore of limited use in connection with frontal zones, for example, which are expected to be turbulent but which are characterised by high wind speeds. An additional indication of the presence of turbulence can be gained by considering the ratio of signal powers observed in the vertical direction and off-vertical direction. A small value of this so-called aspect sensitivity factor suggests that the radar signals are being scattered from isotropic irregularities of refractive index. A large value suggests that the signals are either being partially reflected from sharp, horizontally coherent changes in refractive index or being scattered from anisotropic irregularities.

An initial investigation has begun to evaluate the potential of the modified Rice parameter as a further diagnostic for the indentification of the presence of turbulence. This parameter is based on the statistical properties of the in-phase and quadrature components of the radar return signals. If the radar signals are scattered from an ensemble of roughly similar refractive index irregularities, which is expected from a region of turbulence, the signal components should have a Rayleigh distribution of amplitudes. If, on the other hand, the radar signals are predominantly returned from a single refractive index feature, such as might be expected under non-disturbed conditions, the signal components will tend to have a more Ricean distribution.

A PDF version of  a poster describing some initials results  of a study entitled "An examination of signal statistics and their analysis associated with clear air returns" which was presented at the UWERN2002 meeting in the UK can be found here (2.7MBytes).

 

 The possible effect of precipitation on clear air returns

A small number of recent studies have indicated that reductions in the signal strength of clear air returns can be observed at low altitudes in regions of precipitation. Data from the NERC MST radar facility in Aberystwyth and co-located tipping bucket rain gauge data are used to determine whether this effect can be observed for all periods where high rainfall rates were observed at the ground. The period selected for examination includes all of the days where a peak rainfall rate of 1mm/h was observed in 2001. The magnitude of the change in signal power and any variations in the spectral width of the Doppler spectra were examined and are shown to be statistically significant. Use can also be made of UHF wind profiler data to examine whether a relationship between enhanced UHF returns (signifying precipitation) and reduced VHF returns can be observed.

A PDF version of  a poster describing some initials results of a study entitled " The possible effect of precipitation on clear air returns" which was presented at the MST10 Conference in Piura, Peru can be found here (2.3MBytes). 

 

A PDF version of a draft of a paper submitted to a special edition of Annales of Geophysicae is available here (627kBytes).

Convection picture

Convective gravity wave paper draft

 

 


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