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Published in: Environmental Earth Sciences 10/2019

01-05-2019 | Thematic Issue

Groundwater gravitational circulation of Karst Veliko Vrelo and Malo Vrelo springs by isotope and the noble gas method: case study of the Beljanica Massif

Authors: Ljiljana Vasić, Laszlo Palcsu, Huang Fen

Published in: Environmental Earth Sciences | Issue 10/2019

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Abstract

Defining groundwater circulation velocity and residence time in the karst is of particular importance, especially for purposes of water supply use. Investigations were performed at Veliko Vrelo and Malo Vrelo springs, which are typical gravitational circulation karst springs of the Beljanica massif, for determining groundwater residence time, both during the high-flow period, which is characterized by rapid water circulation (spring period), as well as in the recession period (end of summer) when water circulates significantly more slowly through smaller and relatively deeper karst channels. For purposes of defining the different groundwater residence times and circulation velocity, besides tracer test (Na-fluorescein), stable isotope methods 18O, 2H, 13C as well as radioactive isotopes 3H and 3H + 3He were used. Additionally, to determine the temperature conditions that prevail, as well as recharge duration in the vadose zone during the groundwater recharge period, the content of noble gases in groundwater was measured. The results reveal the dual development of karst conduits, where the first circulation zone is characterized by larger channel dimensions where groundwater rapidly circulates over a period of only several days, while the second zone consists of smaller channels and cracks, in which the waters reside 3 or 4 months during the recession period.

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Metadata
Title
Groundwater gravitational circulation of Karst Veliko Vrelo and Malo Vrelo springs by isotope and the noble gas method: case study of the Beljanica Massif
Authors
Ljiljana Vasić
Laszlo Palcsu
Huang Fen
Publication date
01-05-2019
Publisher
Springer Berlin Heidelberg
Published in
Environmental Earth Sciences / Issue 10/2019
Print ISSN: 1866-6280
Electronic ISSN: 1866-6299
DOI
https://doi.org/10.1007/s12665-019-8294-0

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