FRESQUALI

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VDemo-Fresnel II
FRESQUALI

“Fresquali” – Qualification of Linear Fresnel Collec-tors; Adaptation and Development of Optical and Thermal Testing Techniques

Participants:

  • Fraunhofer ISE

Contact:

  • Dr. Werner Platzer, Fraunhofer Institute for Solar Energy Systems ISE, Heidenhofstr. 2, 79110 Freiburg, Germany

Duration:

  • 3/2003 – 9/2006

Funding:  

  • German Ministry for Environment, Nature Conservation and Nuclear Safety (BMU): 390 t€
 

Strip reflection testing of primary mirror in a laboratory setup with screenshot of software evaluation tool

 

The Linear Fresnel Collector is an attractive option for solar thermal power stations, as shown by previous projects and fea-sibility studies. MAN Ferrostaal Power Industries is currently erect-ing a demonstration collector in cooperation with Fraunhofer ISE and DLR at the Plataforma Solar de Almeria. To ensure industrial production lines and qualification, Fraunhofer ISE is developing measurement techniques for industrial application of Fresnel collectors and adapting them to their special properties and geometries in a German national project called FRESQUALI.
Optical and thermal qualification will help manufacturers and construction companies to control collector performance as stipulated in the specifications. Some properties of the key components, i.e., thermal receiver, secondary and primary mir-rors, still have to be determined.
the first months of the project, a reflectometric technique was adapted to the requirements of solar field characterization. With strip reflection, the shape and optical aberrations of curved mirrors can be determined from camera pictures. Laboratory measurements using active pattern generation with projectors or flat screens have been developed to qualify the primary and secondary mirrors during production at the PSA. At the moment, a passive pattern technique using a printed pattern with sinusoidal grey strips is being developed for outdoor characterization of mounted mirrors. The technique is very flexible and may be adapted to parabolic mirror fields also.
Dust and dirt as well as degradation of mirrors may also re-duce the output of solar thermal fields and have a noticeable impact on their economics. A mobile spectrometer is to be used for fast reflectometric characterization in a handheld device.
A special 3.4 µm wavelength thermal infrared camera can be used to study the temperature distribution of solar receivers behind the glass cover for non-destructive testing of absorber properties.
 

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