1994
DOI: 10.1016/0022-3093(94)90702-1
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Effects of exposure to photons of various energies on transmission of germanosilicate optical fiber in the visible to near IR spectral range

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Cited by 31 publications
(11 citation statements)
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“…The co-doping with Ge may induce Ge(1) centers contributing to the RIA of the tested wavelength [14] ; however, the induced absorption band of Ge(1) was unmeasurable at 1 310 nm in the present lowdose (100 Gy) experiment [15] . Several causative UV absorption centers may exist, forming the so-called UVabsorption tail.…”
Section: Fig 5 Ria Temperature-dependence After Accelerated Annealicontrasting
confidence: 57%
“…The co-doping with Ge may induce Ge(1) centers contributing to the RIA of the tested wavelength [14] ; however, the induced absorption band of Ge(1) was unmeasurable at 1 310 nm in the present lowdose (100 Gy) experiment [15] . Several causative UV absorption centers may exist, forming the so-called UVabsorption tail.…”
Section: Fig 5 Ria Temperature-dependence After Accelerated Annealicontrasting
confidence: 57%
“…Section 2.2.1). However, Anoikin et al [54] did not record their spectra to energies higher than 3.2 eV, so further research will be needed to find out what happens to the 5.8 eV band (associated with Ge(2); see Figure 2) in irradiated polymer-clad fibers subsequently exposed to the atmosphere for extended periods of time.…”
Section: What Are the Defects Responsible For The Radiationinduced Lomentioning
confidence: 99%
“…The nomenclature "GeX" was introduced by Anoikin and his coworkers [54] to express its unknown place in the Pantheon of Ge-doped-silica-glass defects. However, there was one clue.…”
Section: What Are the Defects Responsible For The Radiationinduced Lomentioning
confidence: 99%
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“…However, these defects with their absorption band at 6.2 eV (280 nm) negligibly contribute to induced losses in our studied range of wavelengths. Several authors showed that the absorption bands related to GeX (2.61 eV, 475 nm), Ge(1) (4.41 eV, 280 nm) and Ge-NBOHC (1.97 eV, 630 nm) can be used to correctly fit the RIA spectral curve after c-rays [6,7]. We recently showed [8] that these three defects also allow to correctly fit the c-ray and 14 MeV neutron RIA curves of our Ge-MMF fiber.…”
Section: Origin Of the Ria In The P-free Multimode Fibermentioning
confidence: 99%