1983
DOI: 10.1088/0022-3735/16/1/015
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A capillary discharge tube for the production of intense VUV resonance radiation

Abstract: Abstract. Design and operational characteristics of a line source with very high intensity in the vacuum u v are described. The source generates rare-gas resonance radiation in a lowpressure. cold-cathode, DC glow discharge up to 200 mA. The windowless lamp is differentially pumped and can be installed inside a vacuum chamber. During operation it is water cooled and can be mildly baked because it contains metal seals only. In a light beam of 2.5 mm diameter the photon flux for the strongest He1 and Ne1 emissio… Show more

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Cited by 39 publications
(10 citation statements)
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“…Figure 1 shows the schematic setup of the apparatus. The vacuum ultraviolet (VUV) lamp 15 and the cylindrical-mirror-analyzer electron spectrometer are necessary for photoelectron spectroscopy. The main parts of the source of oriented molecules are the supersonic beam source, the electrostatic hexapole, and the guiding field; in between a buffer field is placed.…”
mentioning
confidence: 99%
“…Figure 1 shows the schematic setup of the apparatus. The vacuum ultraviolet (VUV) lamp 15 and the cylindrical-mirror-analyzer electron spectrometer are necessary for photoelectron spectroscopy. The main parts of the source of oriented molecules are the supersonic beam source, the electrostatic hexapole, and the guiding field; in between a buffer field is placed.…”
mentioning
confidence: 99%
“…The 40.8 eV lines which are most intensive of the He II radiation are close to the electron-electron scattering threshold in solid Ne and fit, thus, the expected minimum of the photoemission line shape. Moreover, comparison of the 21.22 eV He I and 40.8 eV He II photon fluxes reported in the literature [54,57,58] shows that the latter one is 1-3 orders below the former one, making negligible contribution to the photoemission from solid Ne.…”
Section: Resultsmentioning
confidence: 79%
“…The spectrum in Fig. 2 of the paper [57] shows no signs of 61-62 nm emission lines thus testifying their low intensity. In Ref.…”
Section: Resultsmentioning
confidence: 86%
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“…Please note that the background subtraction routine for the measurement with the He-II line is slightly modified by first subtracting a background of spinresolved photoelectrons, which are excited by satellite spectral lines. 37 The measured spectra (I ± ) have been fitted with the convolution of a Gaussian peak function and the product of a Fermi-Dirac distribution (T = 300 K) with another Gaussian peak function. Here, the first Gaussian function represents the combined energy resolution due to the spectrometer and the light source.…”
Section: Fig 2 (A)mentioning
confidence: 99%