Introduction
The purpose of this study is to estimate the snow accumulation rate at “Byrd” station, at the location of the first core hole to bedrock in Antarctica (Reference Gow, Gow, Ueda and GarfieldGow and others, 1968).
This knowledge, together with that of dynamic factors, is essential to the establishment of a time scale most useful for the interpretation of the data obtained by other investigators.
We report here the results obtained by surface measurements and by two radiometric methods based respectively on the distribution of the fission products and of 210Pb with depth in the firn.
Surface measurements
Two 10 km long accumulation stake lines were established in February 1962 and have been monitored each year since. One line was oriented in an east–west direction, the other in a north–south direction (Fig. 1); measurements at these stakes have provided the most reliable record of accumulation variations within a 10 km radius of “Byrd” station.
Results of the first 3 years’ observations (Reference Gow and RowlandGow and Rowland, 1965) indicated a strong topographic control on accumulation rates which all subsequent measurements continue to reflect, namely, that surface depressions accumulate appreciably more snow than the exposed ridges or crests. These relationships are clearly demonstrated in Figure 2, depicting measurements from the east–west line.
Snow stakes were originally emplaced on 16 February 1962, the distance between stakes being set at 0.5 km. A total of 43 stakes was planted but records are incomplete at two stakes. Snow accumulation at 41 slakes for the past 8 years has averaged 117 kg m−2 year−1 The stake showing the greatest accumulation in 8 years averaged 157 kg m−2 year−1; that with the least accumulation averaged 86 kg m−2 year−1 The largest accumulation recorded at any one stake in a given accumulation year (February to February) was 195 kg m−2 year−1.
Measurements made by R. L. Cameron (personal communication) at 100 snow stakes, laid out in a 1 km grid near the eastern corner of the east–west line, have yielded an average accumulation of 103 kg m−2 year−1 based on 2 years’ measurements.
Fission products distribution in the firn
The observation, by Reference Picciotto and WilgainPicciotto and Wilgain (1963) and Reference VickersVickers (1963), that a well-defined reference level in the upper layers of the Antarctic ice sheet has been formed by the stratospheric fall-out of radioactive debris released from the first large thermonuclear bomb test has provided a criterion for measuring the average accumulation rate since 1955. This 1955 horizon (Reference Wilgain, Wilgain and PicciottoWilgain and others, 1965), easily identified by a sudden and large increase in 90Sr or in gross β activity, has been used systematically to estimate snow accumulation rates at 75 stations on the east Antarctic plateau (Reference Picciotto, Picciotto, Crozaz and BreuckPicciotto and others, in press).
An additional reference level, in January 1965, corresponding to the fall-out. of the atmospheric thermonuclear bombs detonated in 1962 has been recognized by Reference CrozazCrozaz (1969).
The firn analysed here was collected in December 1967 near the northern corner of the north-south line. Five bulk samples were used for the depth interval from 0 to 1 m, and seven 1 m cores (7.6 cm diameter hand-augered cores) from 1 m down to 8 m. Each core was cut in five pieces and 300 g samples were treated. The samples were kept frozen until analysed. The gross β activity was measured after coprecipitation of the fission products with suitable carriers (see Reference Picciotto, Picciotto, Crozaz and BreuckPicciotto and others, in press).
The distribution of the gross β activity with depth is shown in Figure 3. The interpretation of these data is straightforward; the low, almost constant, activity below 240 cm is essentially due to the detector background and partially to the natural activity of 210Pb. The jump at 220 ± 10 cm is attributed to the January 1955 (±1 month) precipitations; above this level the usual decrease in activity is followed by a second important increase which culminates in January 1965, at 80 ± 10 cm.
The resulting mean accumulation rates are 67 ± 4 kg m−2 year−1 for the time period 1955–68 and 100 ± 10 kg m–2 year–1 for 1965–68. The errors on the accumulation rates include the uncertainties on the β surges, due to the finite thickness of the samples and the uncertainty on the time of occurrence of the respective horizons (± 1 month).
210Pb
The 210Pb method (Reference GoldbergGoldberg, 1963; Reference Crozaz, Crozaz, Picciotto and BreuckCrozaz and others, 1964) is based on the radioactive decay of the 210Pb occurring naturally in the atmosphere as a decay product of 222Ra. Its 22 year half life allows dating of firn samples up to 100 years old. This method has previously been applied at “Byrd” station by Windom (1969), who derived a mean accumulation rate of 98 kg m−2 year−1.
The 210Pb activity as a function of depth was measured on hand-drilled cores from the same location, from the surface down to 10 m. Two additional 16 cm diameter cores (covering the depth intervals 9.68–10.64 m and 43.36–44.01 m) were obtained from the deep drill hole at “Byrd” station.
The radiochemical procedure has been described in Reference Crozaz and FabriCrozaz and Fabri (1966) and Reference Picciotto, Picciotto, Crozaz and BreuckPicciotto and others (in press). It is based on the α counting of 210Po in equilibrium with 210Pb. The chemical recovery yield is controlled by the use of a 208Po tracer.
The concentrations of 210Po as a function of the depth in water equivalent are shown in Table I. The results are expressed in 210Po/208Po activity ratios; the activities measured are taken to represent the activity at the middle of the depth interval covered by each sample.
A blank correction was applied by subtracting the activity found in the deepest sample, from 43.36 to 44.01 m (which is more than 200 years old).
From the slope of the best straight-line fit through the corrected values (Fig. 4) an accumulation rate of 120 ±10 kg m−2 year−1, averaged over the last 50 years, is deduced.
Conclusion
The results are summarized in Table II.
Consideration of surface stake measurements indicates that the average snow accumulation for the time interval 1962–70, within a 10 km radius of “Byrd” station, varies from 86 to 157 kg m–2 year–1 with a mean value of 117 kg m–2 year–1.
The value for the time interval 1955–68, inferred from the fission products, is rather low but still compatible with the stake measurements since the cores used were from the same general area as the stakes with the lowest accumulation.
The accumulation derived from the 210Pb is in reasonable agreement with the one found by Windom at the same location. Combining both results, we conclude that the average accumulation at “Byrd” station for the time interval 1910–68 is 110 ± 10 kg m−2 year−1.
Acknowledgements
The support of the Office of Antarctic Programs, National Science Foundation and of Task Force 43, U.S. Navy is gratefully acknowledged.