International Radiation Detectors, Inc.
AXUV Photodiodes with Directly Deposited
Filters
To avoid use of fragile freestanding thin filters during
XUV experiments and also in space missions, visible blind
AXUV photodiodes with integrated thin film filters have been
developed. The table below lists available AXUV diodes with
different filter materials and their passbands. Figures 1 and 2 plot a representative selection of quantum efficiencies
for the filtered diodes in the VUV region. These filtered diodes exhibit visible light blocking of at least
four orders of magnitude. Diodes with higher visible light
blocking can be specially selected if required. IRD is
continuously making AXUV diodes with many different filters.
Users are requested to contact us for their special filter
requirements.
The advantages of these integrated detector-filter devices
over presently used separate freestanding thin foil filters
and detectors are compactness, higher reliability, ease in
manufacturing and handling, more stable bandpass and
flexibility in design as the filter thicknesses are
determined by optical constants and not by the mechanical
strength requirement.
The filtered AXUV diodes have been successfully used in the
SNOE and SOHO satellites by scientists at the National
Center for Atmospheric Research and by scientists at
University of Southern California respectively. They are
also being used on the HBT-EP tokamak at Columbia University
as detectors for the soft X-ray tomography
system. We anticipate that these diodes will be
extremely useful in future space missions and other
applications like soft x-ray radiometry, x-ray lithography,
x-ray microscopy and XUV spectroscopy.
Fig. 1: Quantum Efficiencies, various AXUV filtered diodes, 0 - 110 nm
Fig. 2: Quantum Efficiencies, various AXUV filtered diodes, 5 - 35 nm
| Notes: |
* Developed Specifically for the Filtered Diode Ross
Spectrometer |
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# Developed for the Solar Measurements |
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