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Diploma thesis in Physics submitted by Florian Freundt born in ...

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1 Introduction<br />

on the pressure gradient and a parameter describ<strong>in</strong>g the hydraulic conductivity of the given<br />

soil. Flow rates and residence time of water with<strong>in</strong> aquifers therefore vary depend<strong>in</strong>g on the<br />

soil’s hydraulic properties an recharge rates. Water <strong>in</strong> conf<strong>in</strong>ed aquifers can reach an age of up<br />

to several 10 5 years [Sturchio et al., 2004]. Radiocarbon dat<strong>in</strong>g of dissolved <strong>in</strong>organic carbon<br />

<strong>in</strong> ground water is used to provide the age <strong>in</strong>formation for up to 50,000 year old water while<br />

different isotopic dat<strong>in</strong>g methods have to be used for older ground waters.<br />

Reconstruct<strong>in</strong>g paleotemperatures from ground water utilizes the dissolved noble gases neon,<br />

argon, krypton and xenon and requires conf<strong>in</strong>ed aquifers that limit gas exchange. The idea beh<strong>in</strong>d<br />

this paleorecord is the temperature dependency of gas solubility: the <strong>in</strong>filtrat<strong>in</strong>g meteoric<br />

water lead<strong>in</strong>g to ground water recharge is <strong>in</strong> contact with the soil atmosphere before enter<strong>in</strong>g<br />

the aquifer. Dur<strong>in</strong>g this contact the gaseous and aqueous phases equilibrate. This equilibration<br />

is dependent on soil temperature and the composition of the soil atmosphere. Due to temperature<br />

damp<strong>in</strong>g with<strong>in</strong> the soil, its temperature is closely related to annual mean atmospheric<br />

temperatures [Hillel, 1980]. The standard assumption on soil atmosphere noble gas composition<br />

is that it is close or equal to the atmospheric composition, show<strong>in</strong>g only <strong>in</strong>significant<br />

fluctuations [Stute and Schlosser, 1993]. This however neglects the fact that soil atmospheres<br />

greatly vary <strong>in</strong> O2 and CO2 composition spatially as well as temporally [Yamaguchi et al., 1967;<br />

Dowdell and Smith, 1974; Amundson and Davidson, 1990; Magnusson, 1992]. This likely affects<br />

the partial pressures of its rema<strong>in</strong><strong>in</strong>g components. These changes <strong>in</strong> soil air composition are<br />

ma<strong>in</strong>ly caused <strong>by</strong> microbiological activities and are <strong>in</strong>fluenced <strong>by</strong> a multitude of soil properties<br />

like temperature, precipitation, soil hydraulic properties and others <strong>in</strong> a complex relationship<br />

[Suarez and ˇ Sim˚unek, 1993; Welsch and Hornberger, 2004; Riveros-Iregui et al., 2011]. While<br />

paleotemperature studies have largely neglected this possibility so far and have nonetheless successfully<br />

employed model<strong>in</strong>g approaches to account for other factors affect<strong>in</strong>g the dissolved noble<br />

gases [Aeschbach-Hertig et al., 1999b; Kipfer et al., 2002; Peeters et al., 2003], studies on young<br />

ground water <strong>in</strong> recharge areas [Stute and Sonntag, 1992; Ma et al., 2004; Castro et al., 2007]<br />

have led to noble gas temperatures a few degrees below measured soil temperatures. Hall et al.<br />

[2005] proposed that this shift could be caused <strong>by</strong> a deviation of noble gas partial pressures <strong>in</strong><br />

the soil atmosphere from atmospheric values. As the cause for this change they suggest the<br />

process of oxygen depletion, mean<strong>in</strong>g that the O2 removed from the soil atmosphere <strong>by</strong> microorganisms<br />

is not replaced <strong>by</strong> an equimolar amount of CO2 produced <strong>by</strong> these organisms, lead<strong>in</strong>g<br />

to a pressure deficit affect<strong>in</strong>g the partial pressures of the rema<strong>in</strong><strong>in</strong>g gases. While their model<strong>in</strong>g<br />

approach <strong>in</strong>clud<strong>in</strong>g the proposed oxygen depletion effect successfully leads to match<strong>in</strong>g noble<br />

gas and mean atmospheric temperatures for their study area, an actual measurement of soil air<br />

composition was not executed to prove oxygen depletion has the suggested effect on noble gas<br />

partial pressures and could <strong>in</strong>deed be the ma<strong>in</strong> factor <strong>in</strong> caus<strong>in</strong>g the noble gas temperature shift.<br />

Extensive research has been done on the composition of soil atmospheres for various reasons,<br />

ma<strong>in</strong>ly ow<strong>in</strong>g to its importance <strong>in</strong> agricultural contexts. Modern climate research has also been<br />

<strong>in</strong>terested <strong>in</strong> soil atmospheres because of their part <strong>in</strong> the global atmospheric gas balance. Soils<br />

provide both s<strong>in</strong>ks and sources for CO2, CH4, N2O and various other gases relevant to the<br />

Earth’s radiation balance. These studies ma<strong>in</strong>ly focused on O2, CO2 and nitrogenous gases and<br />

usually their flux from the soil rather than <strong>in</strong> situ concentrations. Data on noble gases <strong>in</strong> the<br />

soil atmospheres relevant to noble gas temperatures is sparse at best, as little research on soil<br />

atmosphere composition focus<strong>in</strong>g on the noble gas components has been done so far. While<br />

12

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