Solar-Blind Diamond Detectors for Lyra, the Solar VUV Radiometer on Board Proba II View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2003-12

AUTHORS

A. Benmoussa, J.-F. Hochedez, W. K. Schmutz, U. SchÜhle, M. NeslÁdek, Y. Stockman, U. Kroth, M. Richter, A. Theissen, Z. Remes, K. Haenen, V. Mortet, S. Koller, J. P. Halain, R. Petersen, M. Dominique, M. D’Olieslaeger

ABSTRACT

Fabrication, packaging and experimental results on the calibration of metal-semiconductor-metal (MSM) photodetectors made on diamond are reported. LYRA (Lyman-α RAdiometer onboard PROBA-2) will use diamond detectors for the first time in space for a solar physics instrument. A set of measurement campaigns was designed to obtain the XUV-to-VIS responsivity of the devices and other characterizations. The measurements of responsivity in EUV and VUV spectral ranges (40–240 nm) have been carried out by the Physkalisch-Technische Bundesanstalt (PTB) in Germany at the electron storage ring BESSY II. The longer wavelength range from 210 to 1127 nm was measured with monochromatic light by using a Xe-lamp at IMO-IMOMEC. The diamond detectors exhibit a photoresponse which lie in the 35–65 mA/W range at 200 nm (corresponding to an external quantum efficiency of 20–40%) and indicate a visible rejection ratio (200–500 nm) higher than four orders of magnitude. More... »

PAGES

141-148

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10686-003-0035-3

DOI

http://dx.doi.org/10.1007/s10686-003-0035-3

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1012888691


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