Depth profile of 236U/238U in soil samples in La Palma, Canary Islands Academic research paper on "Chemical sciences"

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Journal of Environmental Radioactivity

journal homepage: www.elsevier.com/locate/jenvrad

Depth profile of 236u/238U in soil samples in La Palma, Canary Islands

M. Srncika' *, P. Steierb, G. Wallner

a Department of Inorganic Chemistry, University of Vienna, Währinger Straße 42, A-1090 Vienna, Austria b VERA Institute, Faculty of Physics — Isotope Research, University of Vienna, Währinger Straße 17, A-1090 Vienna, Austria

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abstract

Article history:

Received 15 November 2010 Received in revised form 27 January 2011 Accepted 18 March 2011 Available online 9 April 2011

Keywords: Soil samples Global fallout

236y/238y

240Pu/239Pu 236U/239Pu

The vertical distribution of the 236u/238U isotopic ratio was investigated in soil samples from three different locations on La Palma (one of the seven Canary Islands, Spain). Additionally the 240Pu/239Pu atomic ratio, as it is a well establish tool for the source identification, was determined. The radiochemical procedure consisted of a U separation step by extraction chromatography using UTEVA® Resin (Eichrom Technologies, Inc.). Afterwards Pu was separated from Th and Np by anion exchange using Dowex 1x2 (Dow Chemical Co.). Furthermore a new chemical procedure with tandem columns to separate Pu and U from the matrix was tested. For the determination of the uranium and plutonium isotopes by alpha spectrometry thin sources were prepared by microprecipitation techniques. Additionally these fractions separated from the soil samples were measured by Accelerator Mass Spectrometry (AMS) to get information on the isotopic ratios 236u/238U, 240Pu/239Pu and 236U/239Pu, respectively. The 236U concentrations [atoms/g] in each surface layer (~2 cm) were surprisingly high compared to deeper layers where values around two orders of magnitude smaller were found. Since the isotopic ratio 240Pu/239Pu indicated a global fallout signature we assume the same origin as the probable source for 236U. Our measured 236U/239Pu value of around 0.2 is within the expected range for this contamination source.

© 2011 Elsevier Ltd. All rights reserved.

1. Introduction

The major source of actinides (as e.g. plutonium) in the environment is global fallout which arose from about 541 atmospheric nuclear explosions (UNSCEAR Report, 1993). Other sources are nuclear reactor accidents (Chernobyl), discharges of radioactive waste (Sellafield, La Hague, Mayak) and accidents with nuclear devices (e.g. Palomares, Thule) (Salbu, 2001). Soil samples from three different locations on La Palma, Canary Islands, (see Fig. 1) were collected in November 2007 and in February 2009. The emphasis on this work was the vertical distribution of 236U/238U in the soil and the measurement of Pu. In addition the determination of the 236U/239Pu isotopic ratio in these samples was carried out.

236U with a half life of 2.3 x 107 years is continuously produced by thermal neutron capture on 235U which is omnipresent in the environment. The natural 236U production results from neutrons produced by (a, n)-reactions on lighter nuclides (e.g. Na and Mg), spontaneous fission of 238U, induced fission of 235U and at the earth's surface from cosmic rays (Wilcken et al., 2008). A 236u/238U isotopic ratio between 1 x 10~14 and 5 x 10 14 can be expected for typical crustal rocks with a uranium and thorium content of a few

* Corresponding author. Tel.: +43 1 4277 52624; fax: +43 1 4277 52620. E-mail address: michaela.srncik@univie.ac.at (M. Srncik).

0265-931X/$ - see front matter © 2011 Elsevier Ltd. All rights reserved. doi:10.1016/j.jenvrad.2011.03.011

ppm (Steier et al., 2008). On the other hand, significant releases to the environment can be expected as 236U is a by-product in nuclear power plants. This potentially enhances the very low natural isotopic ratio, but the environmental distribution of anthropogenic 236U is not well investigated yet. The present work is part of a larger effort to assess the dispersion of anthropogenic 236U in different compartments of the environment. The summit of La Palma Island is chosen since it allows relatively easy access to a site with clean tropospheric air, far away from anthropogenic emissions. It is thus well suited for studying fallout at minimum risk of local contamination. The climate of the Canary Islands (Herrera et al., 2001) is dominated by the direct influence of the trade wind belt, which blows mainly against the northern of the islands. La Palma (2312 m a.s.l.) is the second highest island of the Canary archipelago, and the most humid (~ 1000 mm/year at the sampling sites). The exceptional steep topography of La Palma leads to condensation directly from high-altitude clean air. Since the deposition of global fallout is controlled by precipitation, a sufficient amount of radionuclides is expected. On the other hand, the high mountain ranges of La Palma are easily accessible on good roads, since they host several European astronomical observatories.

Measurements of 236U became possible only recently by AMS on very few facilities, as e.g. VERA (Vienna Environmental Research Accelerator); plutonium isotopes, on the contrary, are comparably well studied as tracer for anthropogenic actinides with alpha

Santa Cruz le La Palma

Fig. 1. Modified map from La Palma (Moss et al., 1999). The numbers with the respective cycles indicate the sampling sites (1 represents IIC, IID and LP_B1, LP_B2, number 2 stands for IA, IB and 3 for LP_A).

spectrometry and ICP-MS (Ketterer and Szechenyi, 2008) but also by AMS (Oughton et al., 2001). Although the environmental behaviour of U and Pu differs significantly, we consider plutonium as the best candidate for a methodical comparison. Also for Pu, AMS seems to have the best overall sensitivity (Fifield, 2008) but it can also be measured by other mass spectrometric techniques with partially higher detection efficiency (Steier et al., 2010). Recently soil samples from a site which was solely influenced by global fallout could be investigated for their 236U concentration. The amount ranged from 108—109 atoms/g dry soil (Sakaguchi et al., 2009). A constant 236U/239Pu ratio of ~0.2 was found, which was interpreted as the original fingerprint of global fallout. In the general environment, however, differences in the mobility of Pu and U will lead to deviations from this ratio.

In this paper the combined procedure for the determination of U and Pu in soil samples is presented. Two column chromatography methods were applied: at the beginning the sample solution was passed through a column filled with UTEVA® Resin (Eichrom Technologies, Inc.) to separate U, and then the Pu fraction was purified with a second anion exchange step by using Dowex 1x2 (100—200 mesh, Dow Chemical Co.). The second method consisted of a double column system. The first column was filled with Dowex 1x8 and the second one with UTEVA® Resin. The UTEVA column was placed directly below the anion exchange column.

The advantage of this method is that no further purification (i.e. additional column chromatography steps) of the Pu fraction was necessary.

We present first 236U/238U ratios from a clean air area as well as 240Pu/239Pu and 236U/239Pu atomic ratios, from which the contamination source (namely global fallout) can be derived.

2. Materials and methods

The samples were collected at three different sites on the island La Palma in the Atlantic Ocean. Despite samples were taken close to roads or trails, we looked out for an intact and site-typical vegetation cover as indication for the absence of anthropogenic disturbance. From the first sampling location (N 28° 45.233'/W 17° 53.4210, 2330 m a.s.l.) on the northern slope of Roque de los Muchachos two cores (IA and IB) were available which were separated into 2 cm layers and stored in plastic bags. The full length was 10 cm and 12 cm for IA and IB, respectively. At the second site several 100 m downhill (N 28° 46.191'/W 17° 54.224', 1970 m a.s.l.) again two cores with 8 cm length were collected (IIC and IID). IIC was separated into 2 cm layers whereas IID was taken as a bulk sample. Two years later two additional bulk samples (LP_B1 and LP_B2) were collected from the same site as IIC and IID: the depth of LP_B1 ranged from 0 to 5 cm. LP_B2 was sampled from an outcrop apparently exposed by road construction between 2007 and 2009. Approximately 10 cm of the vertical surface of the outcrop were removed, and then the material was taken from 15 to 40 cm below the horizontal surface. Additionally a third bulk sample (LP_A) was collected on Pico de La Nieve (N 28° 43.717'/W 17° 49.636', ~2000 m a.s.l.) with a depth down to 5 cm. In the time period between the two collection dates the sample procedure was improved. While the samples picked up in 2007 were prepared according to the chemical separation procedure A, the samples taken in 2009 were processed following the faster and more comfortable sample preparation B. The main difference of the second procedure is the usage of UTEVA® Resin coupled with Dowex 1x8 but few other changes are in the detail and therefore both sample treatments are described separately below. For spiking a stock solution of 236Pu was obtained from the University of Helsinki and calibrated against SRM 4334G (242Pu solution) by alpha spectrometry. Furthermore a stock solution of SRM 4324B (232U solution) was used. One reference sample (IAEA-135, Radionuclides in Irish Sea Sediment) was investigated with respect to Pu and U in order to check the validity of our results.

2.1. Chemical separation procedure A

After drying the samples by air, they were ashed in porcelain crucibles in an electric muffle furnace at 420 °C for 24 h. The radiochemical procedure applied to the analysis of U and Pu by alpha spectrometry followed the procedures given in (Eichrom Technologies, 2005; Hrnecek et al., 2002) with slight modifications which are discussed briefly below. Between 5 and 20 g soil were leached in 100 mL 65% HNO3 and 25 mL 37% HCl, 0.5 g NaNO2, 236Pu and 232U tracer solutions were added. After boiling the mixture for 3 h, the sample was centrifuged for 30 min at 4000 rpm (relative centrifugal force (RCF) is 1646). The soil residue was leached twice with 20 mL 65% HNO3 and 15 mL 48% HF for 1 h and was then rejected. The supernatant solutions were combined and evaporated to near dryness. The residue was fumed twice with 10 mL boric acid (c = 5 g/100 mL), three times with 10 mL 65% HNO3 and 4 mL 32% H2O2. The residue was taken up in 20 mL 3 M HNO3 — 1 M Al(NO3)3 and insoluble particles were removed by centrifugation.

2.1.1. Separation of uranium

0.5 g UTEVA® resin was pre-conditioned with 3 M HNO3, the sample solution was brought onto the column which was then washed with 35 mL 3 M HNO3. Pu was eluted with 10 mL 9 M HCl and 30 mL 5 M HCl — 0.05 M oxalic acid, and finally U was eluted with 30 mL 1 M HCl.

2.1.2. Purification of plutonium

The solution containing Pu was taken to dryness and fumed three times with 5 mL 65% HNO3 and 2 mL 32% H2O2. The residue was taken up with 20 mL 1 M HNO3 and 100 mg Mohr's salt [(NH4)2Fe(SO4)x6H2O] were added to reduce Pu to trivalent state. Afterwards the solution was adjusted to 8 M HNO3 by adding 20 mL 65% HNO3. Finally Pu was oxidized to tetravalent oxidation state by addition of 0.5 g NaNO2. The excess of nitrous acid was destroyed by gently boiling (NOx fumes). 6 g Dowex 1x2 were pre-conditioned with 8 M HNO3 and then the sample solution was loaded onto the column which was subsequently washed with 50 mL 8 M HNO3. Th was removed with 30 mL 37% HCl and Pu was eluted with 50 mL 0.36 M HCl — 0.014 M HF.

The U and Pu fractions were evaporated until dryness and fumed three times with 5 mL 65% HNO3 and 2 mL 32% H2O2. The U fraction was additionally fumed with 37% HCl (3x). Afterwards the Pu was dissolved in 20 mL 1 M HNO3 and U in 20 mL 1 M HCl to carry out the microprecipitation (description see Section 2.3) for the alpha source preparation.

2.2. Chemical separation procedure B

The procedure described below (modified from Eichrom Technologies, 2005; Moreno et al., 1997; Warneke et al., 2002) was used for the bulk samples collected in 2009. Samples of 20 g were dried in an electric oven at 100 °C to constant weight and afterwards ashed in porcelain crucibles in an electric muffle furnace at 420 °C for 24 h. The sample was transferred to a Teflon beaker and was leached according to 2.1 "Chemical separation procedure A". Afterwards the combined solutions were evaporated till dryness, fumed three times with 10 mL boric acid (c = 5 g/100 mL), with 10 mL 37% HCl (3x) and with 10 mL 65% HNO3 (3x). The residue was dissolved in 8 M HNO3 and a redox adjustment of Pu was carried out as described in Section 2.1. The insoluble part was removed by centrifugation (5 min at 4000 rpm). Two columns were prepared; the first one was filled with 6 g Dowex 1x8 (100—200 mesh, Dow Chemical Co.) and the second column with 0.5 g UTEVA® (Eichrom Technologies, Inc.). The UTEVA® column was placed directly under the anion exchange column and both were pre-conditioned with 8 M HNO3. The sample solution was transferred to the Dowex 1x8 column and the eluent passed directly onto the UTEVA® column. After washing with 60 mL 8 M HNO3 the columns were separated. The Dowex 1x8 column was washed with 50 mL 37% HCl to remove Th, and Pu was finally eluted with 50 mL 0.1 M NH4I — 9 M HCl. The iodide reduced Pu(IV) to Pu(III) which does not form chloride complexes and was no longer retained by the column. The UTEVA® resin was washed with 40 mL 3 M HNO3, traces of Th and Np were eluted with 10 mL 9 M HCl and 30 mL 5 M HCl — 0.05 M oxalic acid. Finally U was eluted with 30 mL 1 M HCl. The U and Pu fractions were treated according the last paragraph in Section 2.1.2.

23. Microprecipitation

To the plutonium fraction a tip of a spatula of Mohr's salt, 0.5 mL of a 25% NaNO2 solution and 50 mL of a Nd3+-solution (c = 1 mg/mL) were added.

To the U fraction 50 mL of a Nd3+-solution (c = 1 mg/mL) were added and U was reduced to tetravalent oxidation state by addition of 100 mL 15% TiCl3-solution. Afterwards 5 mL40% HF were added to both of the solutions. After 1 h the samples were filtered through a cellulose nitrate membrane filter (Whatman®, 0.1 mm pore size), washed three times with 2 mL 4% HF and twice with 2 mL Millipore water (18.2 MU cm).

2.4. Alpha measurement

Alpha spectrometry was performed with a PIPS (Passivated Implanted Planar Silicon) Detector, Model 7401 VR, Canberra/ Packard with an active area of 450 mm2. The counting time was 252 000 s and 604 800 s for U and Pu, respectively. For these measurements, the detection limits calculated according to Currie (1968) were 1.12 mBq/sample for 238U and 0.80 mBq/sample for 239(40)Pu. The software Genie 2.1 (Canberra, USA) was used for the evaluation of the spectra.

2.5. AMS measurement

The filters already analysed by alpha spectrometry were reprocessed for the AMS measurement according to Srncik et al. (2008). The filters were dissolved in HNO3, the nuclides of interest were co-precipitated with iron hydroxide, and combusted to oxides which are pressed into an aluminium sample holder either with or without silver as binder. The VERA setup as used for actinide measurements is described in Vockenhuber et al. (2003) and Steier et al. (2010).

PuO~ at 50 keV was produced in a Cs-sputter source, mass analysed, accelerated to 3 MeVand stripped to positive charge state in a gas cell. By these means, all interfering molecular isobars are destroyed. The 5+ charge state is selected in a second, high energy mass spectrometer, after acceleration to 18 MeV. A combination of an ionization chamber and a time-of-flight measurement allow a unique identification of the isotope of interest. Significant background exists for 240Pu5+, apparently from stable 144Nd3+, which shares the same mass-to-charge ratio and thus cannot be suppressed by the mass spectrometer. In the present measurement, the residual Nd concentration in the sputter samples was, however, low enough and could therefore be separated in the energy-resolving detector.

The machine was tuned with 238U16O~ as a pilot beam, and the parameters were than scaled to the different rare radioisotopes which do not provide sufficient beam current for tuning. Alternating measurements of 239Pu and 240Pu were performed, with duration of several 100 s each. By these means, one tries to minimize the impact of source output variations on the measured count rate results. For 236U, 238U16O- can be measured once per second as a current before the accelerator, which renders source output variations negligible. Our in-house standard Vienna-KkU, 236U/U = (6.98 ± 0.32)x 10 (Steier et al., 2008) was used to normalize the 236U measurements. However, no standard is available for Pu; this introduces an additional uncertainty, which is however expected to be in the range of a few percent. Measurement times per sample ranged from 30 min to several hours, depending mainly on the machine time availability. Generally, the prepared samples last for several hours, and an efficiency of ~ 10(counts in the detector per atom in sputter sample) is achieved if the samples are completely sputtered.

3. Results and discussion

The chemical separation A has been already applied in our laboratory but for sample preparation B the validity was checked by analysing an IAEA-135 reference material. The obtained result was

(225 ± 7) Bq/kg 239(40)Pu; this value is in good agreement with the recommended value of (205-226) Bq/kg for 239(40)Pu. The IAEA-135 standard was also measured for its 236u/238U ratio by AMS. Our value of (1.48 ± 0.04) x10-6 agrees with Hotchkis et al. (2000) who determined (1.48 ± 0.37)x10-6 viaAMS. Our result indicated a very good accuracy of the proposed method.

The isotopic ratios 236u/238U ranged from 10"

near the surface

In Table 1 the results of the 236u/238U isotopic ratios and 236U [atoms/g] for all core layers and also for the bulk samples are shown. In each core (IA, IB and IID) the main amount of 236U was found in the surface layer (between 109 and 1010 atoms/g dry soil). With increasing depth the number of atoms per gram measured was in the range of 107, except for the depth profile of IA. Here again an increase of two orders of magnitude was obtained for the deepest layer. As this value is so high and therefore implausible, we assume that a mistake during the sample collection occurred. According to the results that a relatively high value of 236U atoms/g in each surface layer was found in contrast to the deeper layers (decrease by two orders of magnitude), it seems that the anthropogenic 236U was not moving downwards. The layers below the "surface layer" show at all sites (IA, IB and IID) at least the same order of magnitude of 236U atoms/g. The result of the respective sub-samples of LP_B1 and LP_B2 are consistent with the exception of LP_B2_2 which was below the blank value. The result of sample LP_A_2 is higher but agrees with LP_A_1 and LP_A_3 within 2s. Both bulk samples LP_B1 (0-5 cm) and LP_B2 (15-40 cm) show a 236U concentration in the range of 108 atoms/g dry soil. For the LP_A bulk sample (0-5 cm depth) the results are one order of magnitude higher which reflects inhomogeneities in the 236U distribution at different sample sites.

Table 1

Results of the isotopic ratio 236u/238U and 236U [atoms/g] in soil samples from La Palma. The measurement uncertainties are given in ± 1a.

Sample Core, depth [cm] 236y/238y 236U [atoms/g]

Depth profile : — IA

LP01a IA, 2—6 (2.37 ± 0.07)x10~ -7 (9.69 ± 1.62)x109

LP02a IA, 6—8 (2.96 ± 0.20) x № 9 (6.08 ± 0.73)x107

LP03 IA, 8—10 (1.23 ± 0.04) x № 7 (1.93 ± 0.31)x109

Depth profile ! — IB

LP04 IB, 0—2 (3.15 ± 0.09) x 10" 7 (8.76 ± 1.62)x109

LP05a IB, 2—4 (3.01 ± 0.09) x 10" 9 (3.91 ± 0.56)x107

LP06 IB, 4—6 (3.90 ± 0.21) x № 9 (8.12 ± 1.24)x107

LP07 IB, 6—8 (2.10 ± 0.23)x10~ 9 (4.95 ± 1.12)x107

LP08a IB, 8—10 (1.00 ± 0.n)x10~ 9 (1.43 ± 0.33) x107

LP09 IB, 10—12 (2.13 ± 0.16)x10~ 9 (5.46 ± 0.89) x107

Depth profile : — IID

LP10 IID, 0—2 (2.54 ± 0.08) x № 7 (2.82 ± 0.48) x109

LP11 IID, 2—4 (4.93 ± 0.34) x № 9 (2.61 ± 0.48)x107

LP12a IID, 4—6 (3.25 ± 0.16) x 10- 9 (5.64 ± 0.96) x107

LP13 IID, 6—8 (3.54 ± 0.33)x10- 9 (2.85 ± 0.49) x107

LP14 IID, 8—10 (3.52 ± 0.29) x 10- 9 (4.41 ± 0.96)x107

IIC bulk sample

LP15a IIC, 0—8 (4.35 ± 0.24) x 10- 9 (5.75 ± 1.18)x107

Sample Depth [cm] 236y/238y 236U [atoms/g]

LP_B1 bulk sample, again from IIC/IID

LP_B1_1 LP_B1_2 LP_B1_3

0—5 0—5 0—5

(2.36 ± 0.07) x 10 (2.45 ± 0.07) x 10 (2.48 ± 0.07) x 10

LP_B2 bulk sample, again from IIC/IID LP_B2_1 15-40 LP_B2_2 15-40 LP_B2_3 15-40

(4.85 ± 1.69)x10 (3.25 ± 1.54)x10~9

LP_A bulk sample LP_A_1 0—5 LP_A_2 0—5 LP_A_3 0—5

(4.21 ± 0.13)x10~8 (3.41 ± 0.35) x10-8 (1.31 ± 0.57)x10-8

(4.44 ± 0.89) x108 (2.50 ± 0.41)x108 (3.22 ± 0.64) x108

(2.49 ± 0.92) x108 (1.78 ± 0.88) x108

(4.01 ± 0.48) x109 (2.20 ± 0.43) x109 (1.00 ± 0.46) x109

to 10 with increasing depth. The obtained ratios of 10 are not influenced by our blanks; this was proven by a blank correction. At the sample location LP_B1, (0-5 cm) the level of few parts in 10-8 was found and at LP_B2 (15-40 cm) the isotopic ratio is one order of magnitude lower. The value for LP_A is slightly higher than the bulk samples at the LP_B site.

Table 2 shows the vertical distribution of 239(40)Pu [Bq/kg] for each of the three sample locations (cores IA, IB and IID). At the sample site IA the surface layer (0-2 cm) got lost. The specific activities of 239(40)Pu in layer LP01a (2-6 cm) and LP02a (6-8 cm) at location IA are similar [(0.32 ± 0.05) Bq/kg and (0.35 ± 0.06) Bq/ kg, respectively]; in the deepest layer a decrease of one order of magnitude occurred. The highest specific activity at location IB of (0.46 ± 0.03) Bq/kg was found in the surface layer (0-2 cm). The values for LP05a (2-4 cm) and LP09 (10-12 cm) were below the limit of detection (<0.040 Bq/kg). At the sample location IID the highest value occurred in the layer between 2-4 cm and the decrease of the activity is less marked than at the other two locations. Also here two samples, LP12a (4-6 cm) and LP14 (8-10 cm), were below the detection limit (<0.080 Bq/kg).

The accumulated levels at site IB and IID were (36 ± 11) Bq 239(40)Pu m-2 and (22 ± 7) Bq 239(40)Pu m-2, respectively. These 239(40)Pu results are in the range of the expected value [(36 ± 3) Bq 239(40)Pu m-2] for global fallout in the Northern Hemisphere at latitude 20°-30° N (Hardy et al., 1973).

Buesseler (1997) reports for the global fallout 240Pu/239Pu isotopic ratio a typical interval of 0.175-0.19. According to Kelley et al. (1999) the average composition of fallout 240Pu/239Pu for the north equatorial region (latitude, 30°N-0) is 0.178 with a standard deviation of 0.019 (2a). The ratio for Chernobyl is 0.45-0.52 (Kutkov et al., 1995).

In the present work, for some samples the 240Pu/239Pu ratio could not be determined (indicated by "-" in Table 3) due to relatively small 239Pu and 240Pu count rates. One reason was the low Pu chemical yield (the average was 24.3 ± 0.7) determined by alpha spectrometry which is attributed to difficulties during the leaching and fuming steps before the column separation step. Additionally, sometimes problems during the Fe(OH)3 co-precipitation occurred which would further explain losses of Pu and therefore the low count rate by AMS. From Table 3 it can be seen that at the sample location IA only the first layer could by measured and is in agreement with global fallout, although the value was slightly higher.

Table 2

Vertical distribution of 239(40)Pu [Bq/kg] at the sample location IA, IB and IID and the measurement uncertainty is given ± 1s.

Sample Depth [cm] 239(40)Pu [Bq/kg]

Depth profile -LP01a IA IA, 2—6 0.322 ± 0.045

LP02a IA, 6—8 0.350 ± 0.055

LP03 IA, 8—10 0.026 ± 0.007

Depth profile -LP04 IB IB, 0—2 0.458 ± 0.028

LP05a IB, 2—4 —

LP06 IB, 4—6 0.088 ± 0.010

LP07 IB, 6—8 0.055 ± 0.011

LP08a IB, 8—10 0.037 ± 0.013

LP09 IB, 10—12 —

Depth profile -LP10 IID IID, 0—2 0.296 ± 0.065

LP11 IID, 2—4 0.601 ± 0.100

LP12a IID, 4—6 —

LP13 IID, 6—8 0.136 ± 0.025

LP14 IID, 8—10 —

The 240Pu count rates of both LP02a (6-8 cm) and LP03 (8-10 cm) were too low to determine the 240Pu/239Pu isotopic ratio. The 240Pu/239Pu results in all layers of location IB and IID showed a ratio indicating global fallout. The average isotopic ratio of bulk sample LP_B1 was 0.221 ± 0.029. For all three sub-samples of LP_B2 (15-40 cm below the surface) 239Pu was far below the blank value and therefore no atomic ratio could be determined. The mean 240Pu/239Pu ratio of bulk sample LP_A was 0.287 ± 0.025 which is slightly higher than the expected value for global fallout.

Table 4 shows the 236U/239Pu results for all layers and bulk samples, respectively. According to the isotopic ratios of 240Pu/239Pu found in the La Palma soil samples (Table 3), the source of contamination seems to be global fallout. Ketterer et al. (2007) reported 236U/239Pu atomic ratios between 0.05 and 0.5 for samples containing Pu of purely stratospheric fallout. The wide range was attributed to the evidently higher mobility of fallout 236U compared to Pu (Ketterer et al., 2007). However, this migration behaviour of U and Pu was not observed by Sakaguchi et al. (2009), who investigated at three sites 20 m apart from each other soil samples (0-30 cm) from Ishikawa Prefecture (Japan); here the 236U/239Pu isotopic ratios were in the much smaller range of 0.212-0.253. In our work (compare Table 1 and 2) the overwhelming part of 236U in the core samples was found in the surface layers, while the (unfortunately sparse) Pu data indicates a more even distribution. Consequently, the three topmost samples reveal an enhanced 236U/239Pu ratio higher than 3. All other values are in the range supposed by Ketterer et al. (2007) and for the bulk sub-samples LP_B1 (0-5 cm) a 236U/239Pu value of 0.2 similar to the bulk

samples of Sakaguchi et al. (2009) was found. We obtained for the bulk sample LP_A (0-5 cm) a higher average ratio (236U/239Pu = 0.5) but with a larger scatter between sub-samples.

4. Conclusion

Soil samples from a remote clean air site, the La Palma Island, were investigated with the emphasis on the 236U/238U ratio. A conventional and a new tandem column procedure were applied for the sequential and simultaneous separation of U and Pu, respectively. Samples were measured both by alpha spectrometry and AMS. The isotopic ratio of 236U/238U was between 10~7 for the surface samples and 10~9 for deeper layers. The 236U [atoms/g] results at each surface layer were surprisingly high and the decrease to deeper layers were around two orders of magnitude; this phenomenon was not observed for Pu. The isotopic ratio 240Pu/239Pu is a well established indicator for the identification of the contamination source. In our samples the 240Pu/239Pu atom ratios of 0.149-0.267 for site 1A, IB and IID indicate that global fallout is the probable source for the Pu isotopes similarly to site LP_B1 where the mean isotopic ratio is 0.221 ± 0.029. In accordance with the 240Pu/239Pu results, most of our measured 236U/239Pu isotopic ratios were in the order of 0.04 and 0.78 and agree with the sparse set of already published values for the global fallout signature.

Table 3 Table 4

Results of 240Pu/239Pu by AMS in soil samples from La Palma. The measurement Results of 236U/239Pu in La Palma soil samples. The measurement uncertainties are uncertainties are given in ± 1a. given in ± 1a.

Sample Core, depth [cm] 240Pu/239Pu Sample Core, depth [cm] 236U/239Pu

Depth profile - 1A LP01a IA, 2—6 0.267 ± 0.056 Depth profile - IA LP01a IA, 2—6 14 ± 3

LP02a IA, 6—8 — LP02a IA, 6—8 —

LP03 IA, 8—10 — LP03 IA, 8—10 —

Depth profile - IB LP04 IB, 0—2 0.149 ± 0.006 Depth profile - IB LP04 IB, 0—2 3.3 ± 0.5

LP05a IB, 2—4 0.178 ± 0.015 LP05a IB, 2—4 —

LP06 IB, 4—6 0.198 ± 0.050 LP06 IB, 4—6 0.38 ± 0.07

LP07 IB, 6—8 0.149 ± 0.051 LP07 IB, 6—8 0.27 ± 0.08

LP08a IB, 8—10 — LP08a IB, 8—10 —

LP09 IB, 10—12 — LP09 IB, 10—12 —

Depth profile - IID LP10 IID, 0—2 0.150 ± 0.018 Depth profile - IID LP10 IID, 0—2 4.6 ± 1.5

LP11 IID, 2—4 0.195 ± 0.089 LP11 IID, 2—4 0.04 ± 0.01

LP12a IID, 4—6 0.189 ± 0.035 LP12a IID, 4—6 —

LP13 IID, 6—8 — LP13 IID, 6—8 0.08 ± 0.02

LP14 IID, 8—10 — LP14 IID, 8—10 —

11C bulk sample LP15a IIC, 0—8 0.131 ± 0.029 IIC bulk sample LP15a IIC, 0—8 0.14 ± 0.03

Sample Depth [cm] 240Pu/239Pu Sample Depth [cm] 236U/239Pu

LP_B1 bulk sample, again from IIC/IID LP_B1_1 0—5 0.251 ± 0.060 LP_B1 bulk sample, again from IIC/IID LP_B1_1 0—5 0.23 ± 0.03

LP_B1_2 0—5 0.198 ± 0.027 LP_B1_2 0—5 0.17 ± 0.02

LP_B1_3 0—5 0.215 ± 0.055 LP_B1_3 0—5 0.21 ± 0.03

LP_B2 bulk sample, again from IIC/IID LP_B2_1 15—40 LP_B2 bulk sample, again from IIC/IID LP_B2_1 15—40

LP_B2_2 15—40 — LP_B2_2 15 — 40 —

LP_B2_3 15—40 — LP_B2_3 15 — 40 —

LP_A bulk sample LP_A_1 0—5 0.323 ± 0.041 LP_A bulk sample LP_A_1 0—5 0.78 ± 0.14

LP_A_2 0—5 0.222 ± 0.028 LP_A_2 0—5 0.43 ± 0.08

LP_A_3 0—5 0.315 ± 0.057 LP_A_3 0—5 0.23 ± 0.11

Acknowledgement

Financial support by the FWF Austrian Science Fund (project number P21403-N19) is gratefully acknowledged.

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