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Zhurnal Tekhnicheskoi Fiziki, 2018 Volume 88, Issue 5, Pages 760–769 (Mi jtf5925)

This article is cited in 1 paper

Electrophysics, electron and ion beams, physics of accelerators

Content and isotope ratios of noble gases in congelation ice of lake Vostok

Yu. O. Chetverikova, N. N. Aruevb, S. A. Bulata, K. A. Gruzdovc, V. F. Ezhova, P. Jean-Baptisted, I. L. Kamenskiie, V. Ya. Lipenkovf, È. M. Prasolovc, V. A. Soloveia, R. V. Tyukal'tsevb, I. L. Fedichkinb

a The Petersburg Nuclear Physics Institute, The National Research Center "Kurchatov Institute"
b Ioffe Institute, St. Petersburg
c A.P. Karpinsky Russian Geological Research Institute, St. Petersburg
d Laboratoire des Sciences du Climat et l’Environnement (LSCE) CNRS Orme des Merisiers / Bat. 701 C.E. Saclay, Gif-sur-Yvette, France
e Kola Science Centre of the Russian Academy of Sciences, Apatity, Russia
f Federal Service for Hydrometeorology and Environmental Monitoring, Arctic and Antarctic Research Institute, St. Petersburg, Russia

Abstract: Isotope ratios of noble gases (He, Ne, Ar) were studied in samples collected by degassing of cores of water frozen over a glacier of Lake Vostok. The gases were collected into glass retorts during three days of degassing of cores, which have just been extracted from the borehole. Within the error, the isotope $^{3}$He/$^{4}$He ratios of 0.28 $\pm$ 0.08 $R_A$ ($R_A$ = 1.38 $\times$ 10$^{-6}$ is the ratio for air) correspond to those from [1]. The $^{4}$Íå/$^{20}$Ne and $^{40}$Ar/$^{36}$Ar ratios (12.4 $\pm$ 4.6 $R_A$ and 1.0074 $\pm$ 0.0023 $R_A$, respectively) exceed their contents in air ($^{4}$Íå/$^{20}$Ne$_{A}$ = 0.29; $^{40}$Ar/$^{36}$Ar$_{A}$ = 298.6) and may indicate some contribution of terrigenous gas to the gaseous balance of the lake, as well as the high content of ancient ground waters in the lake. The $^{3}$He/$^{4}$He ratio of 0.28 $R_A$ means low mantle $^{3}$He flux typical of continental platforms far from active rift zones.

Received: 02.10.2017

DOI: 10.21883/JTF.2018.05.45906.2500


 English version:
Technical Physics, 2018, 63:5, 738–746

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© Steklov Math. Inst. of RAS, 2024