1 Introduction

On the temperate Alpine glacier Vernagtferner, Ötztal Alps, Austria, core drillings were carried out in 1979 (bore holes I-III) (Reference Behrens, Oerter and ReinwarthOerter and others 1982) and again in 1983 (IV-VI). The sites of bore holes I-V (Fig.1) were located in the accumulation area, and bore hole VI was located near the mean equilibrium line (not shown in Figure 1). The investigations of the isotope content, fission products and structural parameters of the core material of bore holes I, II and III from 1979 are complete and the results published (Reference Drost and HofreiterDrost and Hofreiter 1982, Reference GoodGood 1982, Reference von Gunten, Rössler and Gäggelervon Gunten and others 1982, Reference Oerter and RauertOerter and Rauert 1982, Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982). The present paper deals with the isotope (³H, ¹⁸O, ²H) and electrical conductivity measurements of core IV, with the aim of investigating the variations in isotope contents during the period from 1979 to 1983.

Fig. 1 Map of the investigation area of Vernagtferner in the Ötztal Alps (Austria), and of the location of the drilling sites in 1979 (bore holes I, II, III) and 1983 (IV, V). The two positions of bore hole I show its movement from March 1979 to March 1983.

Bore hole IV was drilled on 5 and 6 March 1983, yielding a core of length 39.9 m, which corresponds to 30.1 m water equivalent (w.e.). The drilling site was only 10 m from the site of bore hole I in 1983 (Fig.1). Bore hole I has advanced 39.8 m since March 1979, corresponding to a mean surface flow velocity of the glacier in that time of 9.9 m a⁻¹. The vertical component of the movement was 7.7 m, corresponding to a mean value of 1.9 m a⁻¹. For the isotope measurements the core was cut parallel to its axis into two equal parts. One half, with a cross-section of about 22 cm², was further cut perpendicular to the axis into pieces 5 cm long. These pieces were melted, and the electrical conductivity measured, and afterwards ³H, ²H and ¹⁸O contents were determined.

2 Tritium Content and Electrical Conductivity of Core IV

2.1 Tritium content

The ³H contents of most of the samples were measured by direct liquid scintillation counting of 10 ml water samples for a time of 500 to 1000 min each, which yields a detection limit of about 10 TUFootnote *. Details of the measuring technique may be found in Reference Eichinger, Forster, Rast, Rauert and WolfEichinger and others (1981).

Figures 2(a) and (b) show the ³H content of core I (Reference Oerter and RauertOerter and Rauert 1982) in comparison with the ³H content of core IV plotted against the depth in meters of water equivalent.

Fig. 2 (a) ³H content of core I (1979) (Reference Oerter and RauertOerter and Rauert 1982), (b) ³H content of core IV (1983), (c) electrical conductivity (normalized to 20°C) of core 1 (1979) (running mean values of 10 samples, 2.5 cm long each, plotted), (d) electrical conductivity (normalized to 25°C) of core IV (running mean values of 5 samples, 5 cm long each, plotted).

Core IV displays high ³H values in the depth between 10 and 13 m w.e., as was expected from the ³H content of core I. This increase in ³H content in the deposited precipitation is due to the nuclear weapon tests performed mainly between 1953 and 1962. The high ³H values appear in core IV at about 0.9 m w.e. deeper than in core I. The lengths of the sections with high ³H contents in cores I and IV are in good agreement, but the amounts of ³H differ. The ³H content should have decreased by a factor of 0.8 due to radioactive decay during the period 1979–1983 (see also Fig.4), but in fact decreased by a factor of about 0.5. This means that in addition to the radioactive decay another decrease took place. This additional decrease is possibly due to the effects of the water table in the firn, and to the seepage of meltwater there. This point will be discussed in more detail in section 4.

Fig. 4 (a) ³H content of core IV and of core I (Reference Oerter and RauertOerter and Rauert 1982). The ³H contents of core I are referred to March 1983, and the depth scale for core I is shifted 0.9 m w.e. downwards to yield the best fit. The triangles mark the ³H peaks of which the flow lines are shown in Fig. 2 (b) Oxygen-18 content of core IV (running mean values over 5 samples, 5 cm long each) and of core I (Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982) (running mean values over 10 samples, 2.5 cm long each) The depth of core I is shifted 0.9 m downwards, as for the ³H content. The ¹⁸O content is indicated in terms of relative deviation δ¹⁸O from the international standard V-SMOW The measuring accuracy is ±0.15° /_°°. (c) Deuterium excess of core IV (running mean values over 5 samples 5 cm long each) and that of core I (Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982) (running mean values over 10 samples 2.5 cm long each). The depth of core I is shifted 0.9 m downwards, as for the ³H content The deuterium excess d was calculated by d = δ²H-8δ¹⁸O.

An unexpectedly high ³H content was measured in core IV between the depth of 19 to 21 m w.e. According to the dating of core I (Reference Oerter and RauertOerter and Rauert 1982, Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982) these firn and ice layers come from precipitation during the years 1951 to 1954. As the ³H values are about 200 TU (the original ³H content of the precipitation would have been at least 1000 TU), which is larger than expected for this period, we have to assume a contamination of the firn layers by meltwater. This meltwater must either originate from precipitation of the bomb-test period or have been in contact with firn layers from that time under equilibrium conditions. During the drilling these ice cores were wet and water was in the bore hole. At this stage in our investigations we have no definite explanation for the high ³H content at this depth.

We calculate a value of either 1.3 m w.e. or 0.9 m w.e. for the mean accumulation rate from March 1979 to March 1983, depending on whether the small peak at 1975 or the more pronounced peaks around 1963 are used as reference layers.

3 The Water Table in the Firn

Previous investigations of meltwater flow on and within the Vernagtferner demonstrated the build-up of a seasonal water table within the glacier at a depth of about 17 to 20 m below the glacier surface (Reference Oerter and MoserOerter and Moser 1982). The seasonal fluctuations of the water table are correlated with meltwater production on the glacier surface and with meltwater seepage through the firn (Fig.3). The thickness of the water-bearing firn layer increases at the beginning of the ablation season, up to 4 m thickness in some years, and decreases again at the end of the ablation season. The water table is also influenced by crevasses in the firn area which cause drainage of the water-bearing firn layer. Thus the water table drops in the proximity of a crevasse, This means that in the area around an ice core a large water-bearing layer could have existed during certain years, whereas in other years, when this area reached a crevasse, only a thin water-bearing layer might have existed, due to the draining effect of the crevasse.

Fig. 3 Record of water level (well hydrograph) in bore hole I from 1979 to 1982 and in bore hole IV for 1983. The elevation change of the well opening and of the snow surface is also plotted. Note that a pipe was put into bore hole I in May 1979 to reinforce the upper 4 m, and a water-level recorder was mounted on the well opening. The vertical uplift of the well opening in 1981 and 1982 is due to extra pieces of pipe being added. In 1983 a pipe was put into bore hole IV immediately after drilling. The triangles mark the flow lines of two pairs of ³H peaks (at 9.2 and 12.2 m w.e. in core I, and 10.1 and 13.1 m w.e. in core IV).

Tracer experiments on the Vernagtferner showed that intraglacial meltwater flow takes place, and that this meltwater finds its way to the glacier terminus within a few days (Reference Behrens, Oerter and ReinwarthBehrens and others 1982). The calculated flow velocity within the firn water body was about δ m d⁻¹. It is most likely that an isotopic and chemical exchange takes place between the passing meltwater and the porous firn, because the firn is assumed to be water saturated and the liquid and solid phases are in equilibrium. Such an exchange causes a damping of the original isotope content in the firn water body.

Figure 3 also shows the flow line of two firn layers containing two pairs of ³H peaks correlated between cores I and IV (see Fig.4).

4 Changes in the Isotope Content

Figure 4 shows the isotope content of core IV from 8 to 18 m depth w.e. The results for core I are also plotted, with the depth scale shifted 0.9 m w.e. downwards (this shift yields the best fit between the ³H content of both cores). The ³H content of core I (Fig.4(a)) was multiplied by a factor of 0.8 to compensate for the radioactive decay which took place between 1979 and 1983. The biggest changes in ³H are observed between 10 and 13 m w.e., as already mentioned above. From Figure 3 we note that the two peaks at 9.2 and 12.2 m w.e. in core I (Fig.2(a)), corresponding to the peaks at 10.1 and 13.1 m w.e. in core IV, were submerged beneath the firn water table several times in the intervening four years. Apparently, a higher dilution of the ³H content takes place in the more porous firn layers in the water table, and they thus display a greater decrease in the ³H content than do the more compact layers, which mostly coincide with dust layers (at 10.9, 12.0, and 13.05 m depth w.e. in core I).

Furthermore, the measurements of ²H and ¹⁸O contents over this depth range demonstrate a similar effect. In both cases the very marked minimum of core I (Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982) cannot be found in core IV (Fig.4(b)), where only a small peak appears at the corresponding depth. The remaining minimum at a depth of 10.9 m w.e. lies in a horizon with a marked dust layer, and is obviously not related to the original minimum peak of core I, Not only have the minimum values been damped since 1979, but also the maximum values in the firn layers below (these layers do not display the absolute maximum of the ¹⁸O content of core I (Reference Stichler, Baker, Oerter and TrimbornStichler and others 1982: fig.4)). This illustrates that the isotope content becomes more homogeneous in the firn water body. The mean ¹⁸O content of the core section shown (Fig.4(b)) decreased slightly from −14.3‰ (core I) to −14.6‰ (core IV).

The analysis of core I by Reference Stichler, Baker, Oerter and TrimbornStichler and others (1982) demonstrated that the variations of the deuterium excess d (d = δ²H – 8δ¹⁸O) can be used to determine yearly firn layers. In fact, along the section of core IV under discussion the variations of the excess are also present, with only a slightly smaller amplitude. This confirms the usefulness of the deuterium excess for the core analysis. The mean value of deuterium excess also increased from 6.7‰ in 1979 to 9.4‰ in 1983. An explanation for this effect cannot be given.

The downwards depth shift of 0.9 m w.e. which best fitted the results of the ³H measurement, does not yield best results at all depths for the ¹⁸O measurements or for the deuterium excess d. In general a shift of 1.1 m w.e. would be better for the comparison of ¹⁸O and excess d.

Besides an exchange between meltwater and firn, another effect could also appear to be yielding more homogeneous δ¹⁸O values as well as ³H and electrical conductivity values. If some amount of the meltwater remains in the liquid phase in the pores of the drained firn water body (density 0.75–0.85 g cm⁻³) during winter time, it will freeze and become part of the core when the core is removed from the bore hole in sub-freezing temperatures. In addition, small amounts of water remaining in firn pores can become trapped as the firn changes to ice.

In conclusion one can say that one possible reason for the changing isotope content within a temperate glacier is the firn water body, which appears on the Vernagtferner at a depth of about 10 to 12 m w.e. When using the ¹⁸O or ²H contents for analysis of an ice core from a temperate glacier emphasis should be laid on the deuterium excess.