CosmicGuard™

Cosmic Veto Background Reduction System
Manufactured by: The Spectroscopy Divison
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CosmicGuard™

Cosmic Veto Background Reduction System
Manufactured by: The Spectroscopy Division
Favorite this Product

CosmicGuard device is a simple add-on to any new or existing High Purity Germanium (HPGe) counting system that includes a Lynx® Digital Signal Analyzer and Genie™ 2000 or Apex-Gamma™ spectroscopy software.

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Features

  • Performs Cosmic background reduction that can’t be done with lead shielding alone
  • Typical background reduction by 15–40% resulting in lower MDA’s and count times
  • Turnkey solution that can be added to new or existing HPGe detector/shield configurations
  • Compatible with most standard HPGe Lead Shields – split or solid top
  • Electronics for Veto Guard Detector built into detector module – no NIM modules or other additional signal processing electronics required
  • Single cable connection to the acquisition PC or network hub
  • Simple software interface for set-up
  • Requires Lynx Digital Signal Analyzer and Genie 2000 or Apex-Gamma software of current firmware/software versions

Description

The Mirion CosmicGuard device is a simple add-on to any new or existing High Purity Germanium (HPGe) counting system that includes a Lynx Digital Signal Analyzer and Genie 2000 or Apex-Gamma spectroscopy software. The fully self-contained guard detector/electronics module either mounts directly onto a lead shield with a solid 50.8 or 55.9 cm (20 or 22 in.) diameter circular lid or via a lift mechanism that clamps to the shield table for top-opening or non-circular shields. The system connects directly to the HPGe detector’s Lynx DSA and a controlling Genie or Apex® computer – no NIM or other electronics is needed.

Why is cosmic background reduction important?

Background in gamma spectroscopy systems comes from three main sources: Terrestrial Radiation, Internal Radiation and Cosmic Radiation. 

Terrestrial Radiation is driven by K-40, Uranium, and Thorium decay products and is greatly reduced by passive lead shielding. 

Internal Radiation can come from the HPGe detector components or from the sample itself due to incomplete energy deposition in the detector (scattering) and from some of the detector/shield components themselves. In many counting systems, the scattering component will be present, although Compton suppression solutions can be applied in some instances to reduce this form of background. Mirion detectors are already built using selected materials to minimize the detector’s contribution to the radiation background. To further reduce this background component Mirion offers cryostat options like Remote Detector Chamber (RDC) or Ultra-Low Background (ULB) materials.

Cosmic Radiation consists of high energy charged particles (such as muons) originating from extraterrestrial sources. This form of background radiation cannot be significantly reduced by passive lead shielding. It is omnidirectional, but primarily vertically oriented. Therefore, a guard detector placed over an HPGe detector’s shield and equipped with anti-coincidence logic can eliminate much of the cosmic contribution to background. In this case, radiation detected in both the guard detector and HPGe detector at the same time can cause those counts from the HPGe detector to be discarded, thus reducing the cosmic background contribution.

Background reduction achieved by the CosmicGuard system ranges from 15 to 40 percent. In fact, a higher background reduction ratio is seen on HPGe detector systems that already have shielding, especially those that include ULB™ cryostat configurations and shields (like the Mirion 777). With other sources of background minimized, the cosmic component of the remaining background can only be reduced with a guard detector-type set-up.

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