Mirion/CANBERRA’s SAGe Well Detector has many novel features that sets it apart from similar detectors.
The SAGe Well Detector combines excellent energy resolution at low and high energies with maximum efficiency for small samples. Like Traditional Well Detectors, the SAGe Well is fabricated with a blind hole, leaving at least 20 mm of active detector thickness at the bottom of the well. The counting geometry therefore approaches 4π.
The low detector capacitance associated with the small anode technology gives the SAGe Well superior low and medium-energy resolution performance compared to Traditional Well or Coaxial Detectors, as well as excellent resolution for higher energy gamma rays.
Key features
Blind well approaches 4π counting geometry yielding high absolute efficiency
Superior resolution compared to Traditional Well Detectors at both low and high energies
Larger well diameter (28 mm) available with the same excellent resolution as the standard (16 mm) well sizes
Thin lithium diffused contact inside well allows spectroscopy from 20 keV up to 10 MeV
Full LabSOCS™ characterisation available, allowing True Coincidence Summing correction
Equipped with Intelligent PreamplifierUSB 2.0 Serial Interface
Applications
Environmental samples
Radiobioassay
Geology
Oceanography
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This presentation by our partner Mirion Technologies, focuses on techniques to reduce the background in your gamma spectroscopy system.
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This webinar reviewed the SAGe Well technology and innovations, use with LabSOCS and coincidence summing correction, as well as some applications for which the SAGe Well is particularly “well-suited.”