1980Geophysical Research LettersRequires access

VHF‐radar measurements of dynamical processes in the stratosphere and mesosphere

R. Rüster, P. Czechowsky, Gerhard Schmidt

Open publisher page 25 citations

Abstract

Radar observations in the stratosphere and mesosphere have been carried out during a minor stratospheric warming in February 1980 using the SOUSY‐VHF‐Doppler‐Radar (Germany). Enhanced echoes have been received from the stratosphere up to an altitude of about 36 km and from the mesosphere in the height range between 58 and 96 km. Aspect sensitivity has been observed at stratospheric heights, where the signal power can decrease by 10 dB between the vertical and 7° off‐vertical directions. No such effect has been observed in the mesosphere. The background wind speed and the wind direction have been deduced from Doppler measurements made in three different beam directions. The observed 3‐hour average wind speed in the stratosphere reaches a maximum of 60 m s−1, while that in the mesosphere reaches 40 m s−1. In particular, quasi‐periodic signal power variations, which are associated with vertical velocity oscillations at periods of about 12 to 15 min, have been observed in the mesosphere.

About this research paper

What this paper is about

Radar observations in the stratosphere and mesosphere have been carried out during a minor stratospheric warming in February 1980 using the SOUSY‐VHF‐Doppler‐Radar (Germany). Enhanced echoes have been received from the stratosphere up to an altitude of about 36 km and from the mesosphere in the height range between 58 and 96 km. Aspect sensitivity has been observed at stratospheric heights, where the signal power can decrease by 10 dB between the vertical and 7° off‐vertical directions. No such effect has been observed in the mesosphere. The background wind speed and the wind direction have been deduced from Doppler measurements made in three different beam directions. The observed 3‐hour average wind speed in the stratosphere reaches a maximum of 60 m s−1, while that in the mesosphere reaches 40 m s−1. In particular, quasi‐periodic signal power variations, which are associated with vertical velocity oscillations at periods of about 12 to 15 min, have been observed in the mesosphere.

Why it matters

OpenAlex reports 25 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

Radar observations in the stratosphere and mesosphere have been carried out during a minor stratospheric warming in February 1980 using the SOUSY‐VHF‐Doppler‐Radar (Germany). Enhanced echoes have been received from the stratosphere up to an altitude of about 36 km and from the mesosphere in the height range between 58 and 96 km. Aspect sensitivity has been observed at stratospheric heights, where the signal power can decrease by 10 dB between the vertical and 7° off‐vertical directions. No such effect has been observed in the mesosphere. The background wind speed and the wind direction have been deduced from Doppler measurements made in three different beam directions. The observed 3‐hour average wind speed in the stratosphere reaches a maximum of 60 m s−1, while that in the mesosphere reaches 40 m s−1. In particular, quasi‐periodic signal power variations, which are associated with vertical velocity oscillations at periods of about 12 to 15 min, have been observed in the mesosphere.

Key concepts: Mesosphere, Stratosphere, Atmospheric sciences, Altitude (triangle), Doppler effect, Radar, Wind speed, Doppler radar

Related papers

Back to paper searchBrowse research topicsOriginal source
VHF‐radar measurements of dynamical processes in the stratosphere and mesosphere — Research Paper | ScholarLens