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Characterising and Testing Deep UV LEDs for Use in Space Applications

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arxiv 1508.00812 v1 pith:LL4OH2KU submitted 2015-08-04 astro-ph.IM physics.ins-det

Characterising and Testing Deep UV LEDs for Use in Space Applications

classification astro-ph.IM physics.ins-det
keywords ledsspaceavailabledeepgenerallampstesttesting
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Deep ultraviolet (DUV) light sources are used to neutralise isolated test masses in highly sensitive space-based gravitational experiments. An example is the LISA Pathfinder charge management system, which uses low-pressure mercury lamps. A future gravitational-wave observatory such as eLISA will use UV light-emitting diodes (UV LEDs), which offer numerous advantages over traditional discharge lamps. Such devices have limited space heritage but are are now available from a number of commercial suppliers. Here we report on a test campaign that was carried out to quantify the general properties of three types of commercially available UV LEDs and demonstrate their suitability for use in space. Testing included general electrical and UV output measurements, spectral stability, pulsed performance, temperature dependence as well as thermal vacuum, radiation and vibration survivability.

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