Some Results of Monitoring the Radiation Conditions onboard the International Space Station (2000–2003)

Tsetlin, V. V.; Akatov, Yu.A.; Archangelsky, V.V.; Mitrikas, V. G.; Бондаренко, В.А.; Teltsov, M. V.

doi:10.1007/s10604-005-0051-3

Cited by 2 publications

(1 citation statement)

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“…цей матеріал також широко застосовувався в якості одного з найкращих електричних ізоляторів [2]. Сьогодні його ізоляційні якості використовуються тільки у спеціальних проектах, наприклад у разі конструюванні космічних апаратів, оскільки, маючи найбільший питомий опір, бурштин має невелику густину, що є дуже важливим для досліджень космосу [3,4]. Крім того численні зразки бурштину належать до археологічних артефактів і мають історичну цінність, оскільки можуть бути джерелом інформацію щодо культурних аспектів різних суспільств.…”

Section: Eejp 4 2018unclassified

Two band structure of poleskiy amber photoluminescence

Skiba

Mysiura

Kalantaryan

et al. 2018

EEJP

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The paper presents the results of an experimental study of Poleskiy amber luminescence excited by narrow band UV radiation (7 nm) at the wavelength range of 310–410 nm with step of 10 nm. The purpose of the study was to determine the relation between an excitation of two luminescence centers, which we found earlier as a result of the mathematical treatment of the spectra obtained during a cycle of experiments on the photo- and X-ray luminescence of amber from the Poleskiy deposit. It was shown that for various samples the spectra of light excited by UV irradiation had a wide band of luminescence with some differences both in shapes and maximum positions. Increasing the exciting UV radiation wavelength, the monotonic displacement of the spectrum maximum position (from 2.62 to 2.5 eV) and the decrease of the full width at half maximum (from 0.92 to 0.62 eV) were observed. To analyze the spectra, we applied the mathematical treatment procedure that we successfully used earlier, namely fitting of experimental curves with Gaussian functions. It was demonstrated that the shape of our spectra could be with high accuracy deconvoluted by two peaks well described by Gaussian functions. The observed differences in shapes of the spectra can be explained by changes in the amplitudes of the two peaks with centers at 2.5 and 2.95 eV. The photoluminescence experiments with excitation by a narrow band UV radiation showed that light generation at wavelengths corresponding to these centers varied significantly by the change of primary UV radiation wavelength. The most intense excitation of the 2.5 eV band (496 nm) corresponds to the UV radiation wavelength of 384 nm (3.23 eV), and for the 2.95 eV band (420 nm) – 287.5 nm (4.32) eV. This led to the conclusion about an independent nature of the excitation of these centers. Spectrum changes can be explained by the different excitation efficiency of both centers.

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Section: Eejp 4 2018unclassified