Simply recording water depth does not provide a reliable measure of water flow, for example, depth may vary while flow remains constant. In such cases it is essential to measure depth and velocity and then determine the flow measurement.
Unidata’s 6527 Starflow QSD Ultrasonic Doppler instrument is ideal for smaller open channel and pipe measurements as it is a complete hydrographic data collection system. Starflow QSD measures water velocity, depth, flow and temperature, enabling you to do a complete stream study with a single instrument.
Starflow operates in a wide range of water qualities from fresh streams to primary sewerage channels. It measures both forward and reverse flows, and is particularly useful at sites where a stable stage / velocity relationship does not exist. For very small flow monitoring the Unidata Tipping Bucket Flow Gauge can be used.
Open channels, partly filled pipes, and natural streams have very complex velocity characteristics. Turbulence, waves, stream slope, bed and wall unevenness, rocks and debris, all combine to create an unpredictable velocity profile. To account for these effects Starflow analyses up to one thousand separate velocity measurements and statistically determines the mean velocity. This approach provides a good “average velocity” even under difficult conditions.
Note, however, that Starflow is not a “current profiler”, that is, it does not record a detailed velocity profile.
The Starlog companion software allows a user to define the stream, channel or pipe profile, so that the velocity and depth readings can be converted to a true flow reading.
You will generally mount the Starflow QSD on (or near to) the bottom of the stream, pipe or culvert where you are measuring flow, however you can also mount it on the side of larger channels.
A single cable connects the instrument to a 12VDC power source. The unit also provides a control output for initiating a water-sampling unit. The sampling control is fully programmable and can be based on flow, velocity, depth or a combination of these conditions. By connecting a rain gauge you can make a complete storm water monitoring system.
A Neon Remote logger can be connected with the Starflow QSD Instrument in order to record and transmit measured perimeters to a Neon Server routinely. When the data arrives at the Neon Server, it can be viewed on a standard web browser. The data can be checked automatically for any out of limit readings and an appropriate alarm action can be issued.
