Author/Authors :
BenMoussa، نويسنده , , A. and Theissen، نويسنده , , A. and Scholze، نويسنده , , F. and Hochedez، نويسنده , , J.F. and Schühle، نويسنده , , U. and Schmutz، نويسنده , , W. and Haenen، نويسنده , , Nicole K. and Stockman، نويسنده , , Y. and Soltani، نويسنده , , A. and McMullin، نويسنده , , D. and Vest، نويسنده , , R.E. and Kroth، نويسنده , , U. and Laubis، نويسنده , , C. and Richter، نويسنده , , M. and Mortet، نويسنده , , V. and Gissot، نويسنده , , S. and Delouille، نويسنده , , V. and Dominique، نويسنده , , M. and Koller، نويسنده , , S. and Halain، نويسنده , , J.P and Remes، نويسنده , , Z. and Petersen، نويسنده , , R. and D’Olieslaeger، نويسنده , , M. and Defise، نويسنده , , J.-M.، نويسنده ,
Abstract :
We report on experimental results with photodetectors made of diamond. the Large Yield Radiometer (LYRA), will use such detectors for the first time for a solar physics space instrument. A (LYRA) set of measurement campaigns was carried out to obtain their XUV-to-VIS characterization (responsivity, linearity, stability, homogeneity). The responsivity has been measured from the XUV to the NIR, in the wavelength range 1–1127 nm (i.e. 1240–1.1 eV). The diamond detectors exhibit a photoresponse varying in the 40–75 mA/W range at 7 nm and demonstrate a visible rejection ratio (200 versus 500 nm) larger than four orders of magnitude. We show that diamond photodetectors are sensitive sensors for VUV photons, stable within a few percent, with a good linearity and moderate homogeneity.
