Modeling Global Cosmogenic Nuclide Production Through 1St Principles

Total Page:16

File Type:pdf, Size:1020Kb

Modeling Global Cosmogenic Nuclide Production Through 1St Principles Modeling global cosmogenic nuclide production through 1st principles David C. Argento A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Washington 2013 Reading Committee: Dr. John O. Stone, Chair Dr. Erika Harnett Dr. Eric Steig Program Authorized to Offer Degree: Earth and Space Sciences ©Copyright 2013 David C. Argento University of Washington Abstract Modeling global cosmogenic nuclide production through 1st principles David C. Argento Chair of the Supervisory Committee: Dr. John O. Stone, Associate Professor Earth and Space Science The work contained in this thesis is focused on utilizing radiation transport code software as the basis for developing a well validated, first-principles model of global terrestrial cosmogenic nuclide production rates. The state-of-the-art radiation transport code, MCNPX, is utilized to model the terrestrial radiation field. Folding the radiation field neutron and proton results with cosmogenic nuclide production cross-sections yields production rates. This comprehensive, first- principles model is used to investigate characteristics of cosmogenic nuclide production. The goal of the work is to constrain uncertainties in cosmogenic nuclides by better understanding production systematics. Greater understanding of cosmogenic nuclide production rate systematics will assist in constraining uncertainties in cosmogenic nuclide production rate scaling, thereby reducing uncertainties in calculations based on sample nuclide concentrations iii exposure ages, erosion rates, and burial dating. Furthermore, novel uses of cosmogenic nuclides, currently unachievable due to uncertainties, will be enabled by further constraining these. The model is benchmarked against Dr. Paul Goldhagen’s ER-2 aircraft neutron monitor measurements, the Knyahinya meteorite in-situ cosmogenic nuclides, the Beacon Heights sandstone core measurements, and estimated sea level production rates. In this work, I examine: the production rates of each commonly used cosmogenic nuclide as a function of altitude and latitude; the angular distribution of nuclide-producing cosmic-ray particles as a function of altitude and latitude; subsurface production rate systematics; and the production of 36Cl in both the atmosphere and the oceans. iv Acknowledgments I would like to thank my advisor, Dr, John Stone, for his time, energy and guidance in developing my skills as a thorough and effective researcher. John played a critical role in my growth and provided essential perspective throughout this process. I would like to thank the members of my committee: Drs. Erika Harnett, Eric Steig, Bruce Nelson, and Greg Hakim for their guidance and insight. I would also like to thank Dr. Robert Winglee, the Chair of the Earth and Space Sciences Department for his support. I owe a debt of gratitude to Drs. Paul Goldhagen, Gregg McKinney and Laurie Waters whose MCNPX modeling expertise was essential to the success of this project. This work benefited greatly from collaborations with Dr. Robert C. Reedy, Keran O’Brien and Dr. L. Keith Fifield. I would also like to thank the members of CRONUS-Earth who were supportive of my efforts and leant advice and knowledge regarding cosmogenic nuclide formation and applications. My gratitude goes to my colleagues in the Earth and Space Sciences Department, my friends and my family who have supported me through this journey. Above all, I am grateful to my wife, Valerie, for her support, mentoring and love. Finally, I would like to dedicate this dissertation to my parents, Joseph Argento and Susan Millington, particularly my father who passed away before seeing me finish this journey. For their unwavering faith in me, their generosity, their never-ending support, and especially their unconditional love, I am deeply grateful. This work was supported by the CRONUS-Earth Graduate Fellowship (NSF EAR-0345949). v Table of Contents Acknowledgments ................................................................................................... v Table of Contents .................................................................................................. vi Chapter 1- A model of global cosmogenic nuclide production .......................... 1 THESIS STATEMENT ............................................................................................................ 2 BACKGROUND ...................................................................................................................... 2 GOALS & OBJECTIVES ........................................................................................................ 5 CONTRIBUTIONS .................................................................................................................. 6 OUTLINE OF THESIS............................................................................................................. 9 REFERENCES ....................................................................................................................... 11 Chapter 2 - Modeling the Earth’s cosmic radiation ..........................................14 ABSTRACT ............................................................................................................................ 15 INTRODUCTION .................................................................................................................. 16 METHODS ............................................................................................................................. 18 RESULTS ............................................................................................................................... 20 Deep atmosphere ............................................................................................................... 20 Simple planet .................................................................................................................... 24 DISCUSSION ......................................................................................................................... 26 CONCLUSION ....................................................................................................................... 28 REFERENCES ....................................................................................................................... 30 Chapter 3 - A physics-based system for determining cosmic-ray produced nuclide production rates .............................................................................33 ABSTRACT ............................................................................................................................ 34 INTRODUCTION .................................................................................................................. 35 METHODS ............................................................................................................................. 37 GCR models ...................................................................................................................... 37 Radiation transport ............................................................................................................ 40 Application of angular rigidity cut-offs ............................................................................ 42 Normalizations .................................................................................................................. 44 Model geometry ................................................................................................................ 45 Importance values ............................................................................................................. 47 MCNPX Physics options .................................................................................................. 48 MCNPX particle flux output tallies .................................................................................. 48 Atmospheric composition ................................................................................................. 49 Production rates: cross section folding ............................................................................. 49 RESULTS ............................................................................................................................... 50 vi Validations ........................................................................................................................ 50 Terrestrial cosmogenic production results ........................................................................ 57 DISCUSSION ......................................................................................................................... 60 Validations ........................................................................................................................ 60 CONCLUSION ....................................................................................................................... 65 APPENDIX A – MCNPX settings ......................................................................................... 67 REFERENCES ....................................................................................................................... 71 Chapter 4 - Key aspects of in-situ cosmogenic nuclide production: Insights from a physics based model ........................................................................74 ABSTRACT ...........................................................................................................................
Recommended publications
  • EXTRACTION of BERYLLIUM-10 from SOIL by FUSION Summary
    EXTRACTION OF BERYLLIUM-10 FROM SOIL BY FUSION Summary This method is used to separate Be from soil and sediment samples, for AMS analysis. After adding Be carrier, the sample is fused with KHF2. Be is extracted from the fusion cake with hot water. K is removed by precipitation, the sample is dried to expel fluoride, and Be is recovered as Be(OH)2. Yields are typically 70-80 %, but can be increased by additional leaching of the fusion cake. Version Written by John Stone, 1996-2002. This version revised May 2004 by Greg Balco. Available at: http://depts.washington.edu/cosmolab/chem.html References If you use this method, please cite: Stone, J.O.H. (1998). A rapid fusion method for the extraction of Be-10 from soils and silicates. Geochimica et Cosmochimica Acta (Scientific comment) 62, 555-561. Sampling and grinding Mix and grind an unbiased ∼ 50-100 g sample of the material. If possible, mix the original sample bag before opening and take representative proportions of coarse and fine material. Fine soil, carbonate nodules, clay lumps, rock fragments, etc., all have different 10Be concentrations. Grinding homogenises the sample and ensures that these components are evenly represented in the small subsample used for the analysis. If the sample is wet, you will need to dry it before grinding. Initial sample drying Samples are best run in batches of four. This is because we currently have four Pt crucibles. Given more crucibles and sufficient hotplate space, batches of 8 or even 12 are equally feasible. ————————————————— UW Cosmogenic Nuclide Lab – 10Be fusion process 1 – Label and tare four disposable aluminum foil drying dishes and transfer a few grams of ground sediment to each with a steel spatula.
    [Show full text]
  • Isotopegeochemistry Chapter4
    Isotope Geochemistry W. M. White Chapter 4 GEOCHRONOLOGY III: OTHER DATING METHODS 4.1 COSMOGENIC NUCLIDES 4.1.1 Cosmic Rays in the Atmosphere As the name implies, cosmogenic nuclides are produced by cosmic rays colliding with atoms in the atmosphere and the surface of the solid Earth. Nuclides so created may be stable or radioactive. Radio- active cosmogenic nuclides, like the U decay series nuclides, have half-lives sufficiently short that they would not exist in the Earth if they were not continually produced. Assuming that the production rate is constant through time, then the abundance of a cosmogenic nuclide in a reservoir isolated from cos- mic ray production is simply given by: −λt N = N0e 4.1 Hence if we know N0 and measure N, we can calculate t. Table 4.1 lists the radioactive cosmogenic nu- clides of principal interest. As we shall, cosmic ray interactions can also produce rare stable nuclides, and their abundance can also be used to measure geologic time. A number of different nuclear reactions create cosmogenic nuclides. “Cosmic rays” are high-energy (several GeV up to 1019 eV!) atomic nuclei, mainly of H and He (because these constitute most of the matter in the universe), but nuclei of all the elements have been recognized. To put these kinds of ener- gies in perspective, the previous gen- eration of accelerators for physics ex- Table 4.1. Data on Cosmogenic Nuclides periments, such as the Cornell Elec- -1 tron Storage Ring produce energies in Nuclide Half-life, years Decay constant, yr the 10’s of GeV (1010 eV); while 14C 5730 1.209x 10-4 CERN’s Large Hadron Collider, 3H 12.33 5.62 x 10-2 mankind’s most powerful accelerator, 10Be 1.500 × 106 4.62 x 10-7 located on the Franco-Swiss border 26Al 7.16 × 105 9.68x 10-5 near Geneva produces energies of 36Cl 3.08 × 105 2.25x 10-6 ~10 TeV range (1013 eV).
    [Show full text]
  • Meteoric Be and Be As Process Tracers in the Environment
    Chapter 5 Meteoric 7Be and 10Be as Process Tracers in the Environment James M. Kaste and Mark Baskaran 7 10 Abstract Be (T1/2 ¼ 53 days) and Be (T1/2 ¼ occurring Be isotopes of use to Earth scientists are the 7 1.4 Ma) form via natural cosmogenic reactions in the short-lived Be (T1/2 ¼ 53.1 days) and the longer- 10 atmosphere and are delivered to Earth’s surface by wet lived Be (T1/2 ¼ 1.4 Ma; Nishiizumi et al. 2007). and dry deposition. The distinct source term and near- Because cosmic rays that cause the initial cascade of constant fallout of these radionuclides onto soils, vege- neutrons and protons in the upper atmosphere respon- tation, waters, ice, and sediments makes them valuable sible for the spallation reactions are attenuated by tracers of a wide range of environmental processes the mass of the atmosphere itself, production rates of operating over timescales from weeks to millions of comsogenic Be are three orders of magnitude higher in years. Beryllium tends to form strong bonds with oxygen the stratosphere than they are at sea-level (Masarik and atoms, so 7Be and 10Be adsorb rapidly to organic and Beer 1999, 2009). Most of the production of cosmo- inorganic solid phases in the terrestrial and marine envi- genic Be therefore occurs in the upper atmosphere ronment. Thus, cosmogenic isotopes of beryllium can be (5–30 km), although there is trace, but measurable used to quantify surface age, sediment source, mixing production as oxygen atoms in minerals at the Earth’s rates, and particle residence and transit times in soils, surface are spallated (in situ produced; see Lal 2011, streams, lakes, and the oceans.
    [Show full text]
  • Beryllium-10 Terrestrial Cosmogenic Nuclide Surface Exposure Dating of Quaternary Landforms in Death Valley
    Geomorphology 125 (2011) 541–557 Contents lists available at ScienceDirect Geomorphology journal homepage: www.elsevier.com/locate/geomorph Beryllium-10 terrestrial cosmogenic nuclide surface exposure dating of Quaternary landforms in Death Valley Lewis A. Owen a,⁎, Kurt L. Frankel b, Jeffrey R. Knott c, Scott Reynhout a, Robert C. Finkel d,e, James F. Dolan f, Jeffrey Lee g a Department of Geology, University of Cincinnati, Cincinnati, Ohio, USA b School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA 30332, USA c Department of Geological Sciences, California State University, Fullerton, California, USA d Department of Earth and Planetary Science Department, University of California, Berkeley, Berkeley, CA 94720-4767, USA e CEREGE, BP 80 Europole Méditerranéen de l'Arbois, 13545 Aix en Provence Cedex 4, France f Department of Earth Sciences, University of Southern California, Los Angeles, California, USA g Department of Geological Sciences, Central Washington University, Ellensburg, Washington, USA article info abstract Article history: Quaternary alluvial fans, and shorelines, spits and beach bars were dated using 10Be terrestrial cosmogenic Received 10 March 2010 nuclide (TCN) surface exposure methods in Death Valley. The 10Be TCN ages show considerable variance on Received in revised form 3 October 2010 individual surfaces. Samples collected in the active channels date from ~6 ka to ~93 ka, showing that there is Accepted 18 October 2010 significant 10Be TCN inheritance within cobbles and boulders. This
    [Show full text]
  • Polar Desert Chronologies Through Quantitative Measurements of Salt Accumulation
    Polar desert chronologies through quantitative measurements of salt accumulation Joseph A. Graly1, Kathy J. Licht1, Gregory K. Druschel1, and Michael R. Kaplan2 1Department of Earth Sciences, Indiana University–Purdue University Indianapolis, Indianapolis, Indiana 46202, USA 2Lamont–Doherty Earth Observatory, Palisades, New York 10964, USA ABSTRACT isotopes suggest a primarily atmospheric ori- We measured salt concentration and speciation in the top horizons of moraine sediments gin, with some trace mineral boron (Leslie et from the Transantarctic Mountains (Antarctica) and compared the salt data to cosmogenic- al., 2014). However, the Dry Valleys boron iso- nuclide exposure ages on the same moraine. Because the salts are primarily of atmospheric tope values that suggest a trace mineral compo- origin, and their delivery to the sediment is constant over relevant time scales, a linear rate of nent could also form from Rayleigh distillation accumulation is expected. When salts are measured in a consistent grain-size fraction and at during the precipitation of atmospheric boron a consistent position within the soil column, a linear correlation between salt concentration (Rose-Koga et al., 2006). and exposure age is evident. This correlation is strongest for boron-containing salts (R2 > 0.99), Atmospheric aerosols exist either as acid 2 but is also strong (R ≈ 0.9) for most other water-extracted salt species. The relative mobility vapors and gases (e.g., HNO3, N2O5, etc.) or of salts in the soil column does not correspond to species solubility (borate is highly soluble). as anion-cation pairs, commonly adhering to Instead, the highly consistent behavior of boron within the soil column is best explained by particulate matter.
    [Show full text]
  • Calibration of the Production Rates of Cosmogenic 36C1 from Potassium
    CALIBRATION OF THE PRODUCTION RATES OF COSMOGENIC 36C1 FROM POTASSIUM Jodie Manderson Evans A thesis submitted for the degree of Doctor of Philosophy at The Australian National University July, 2001 daran and Heather Preface This thesis describes the complete calibration of J6C1 produced in-situ from potassium. This project was suggested by Dr John Stone and Dr Keith Fifield, and carried out at the Australian National University (ANU) jointly between the Research School of Earth Sciences (RSES), and the Department of Nuclear Physics, RSPhysSE. The author has taken primary responsibility from the beginning of this project to its conclusion. This has involved collecting the samples, performing mineral separations, preparing them for many different measurements, performing the measurements, and finally, carrying out the analysis and interpreting the data. During this process the author was assisted and advised by many people, as discussed below. With the exception of the samples AT-10, AT-11, AT-12 and AT-13, which were collected by Dr Stone, all the Scottish samples were collected by the author with advice from Dr Colin Ballantyne and assistance from Keith Salt, Matt Franks, Angela Lamb and Dr Greg Lane. The samples for the depth profile from Wyangala were collected by the author with Dr Stone, Dr Fifield, Dr Richard Cresswell, Dr Mariana Di Tada and Dr Kexin Liu. The original trace element measurements were made by ICP-MS at RSES with assistance from Mr Leslie Kinsley. X-ray fluorescence measurements (major element whole rock concentrations and some whole rock uranium and thorium concentrations) were made by Dr Bruce Chappell in the Geology Department at ANU.
    [Show full text]
  • Chlorine-36/Beryllium-10 Burial Dating of Alluvial Fan Sediments Associated with the Mission Creek Strand of the San Andreas Fault System, California, USA
    Geochronology, 1, 1–16, 2019 https://doi.org/10.5194/gchron-1-1-2019 © Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License. Chlorine-36=beryllium-10 burial dating of alluvial fan sediments associated with the Mission Creek strand of the San Andreas Fault system, California, USA Greg Balco1, Kimberly Blisniuk2, and Alan Hidy3 1Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94550, USA 2Department of Geology, San Jose State University, San Jose, CA, USA 3Center for Accelerator Mass Spectrometry, Lawrence Livermore National Laboratory, Livermore, CA, USA Correspondence: Greg Balco ([email protected]) Received: 23 April 2019 – Discussion started: 30 April 2019 Revised: 3 July 2019 – Accepted: 5 July 2019 – Published: 18 July 2019 Abstract. We apply cosmogenic-nuclide burial dating using with stratigraphic age constraints as well as independent es- the 36Cl-in-K-feldspar=10Be-in-quartz pair in fluvially trans- timates of long-term fault slip rates, and it highlights the po- ported granitoid clasts to determine the age of alluvial sedi- tential usefulness of the 36Cl=10Be pair for dating Upper and ment displaced by the Mission Creek strand of the San An- Middle Pleistocene clastic sediments. dreas Fault in southern California. Because the half-lives of 36Cl and 10Be are more different than those of the commonly used 26Al=10Be pair, 36Cl=10Be burial dating should be ap- 36 10 plicable to sediments in the range ca. 0.2–0.5 Ma, which is 1 Introduction: Cl= Be burial dating too young to be accurately dated with the 26Al=10Be pair, and should be more precise for Middle and Late Pleistocene sed- In this paper we apply the method of cosmogenic-nuclide 36 iments in general.
    [Show full text]
  • Third Nordic Workshop on Cosmogenic Nuclide Techniques
    Third Nordic Workshop on cosmogenic nuclide techniques Third Nordic Workshop June 8–10, 2016 Workshop hosted by Department of Physical Geography, Stockholm University co-sponsored by Svensk Kärnbränslehantering (SKB) Third Nordic Workshop on cosmogenic nuclide techniques Celebrating 30 years of counting cosmogenic atoms Editors Robin Blomdin June 8–10, 2016 June 8–10, Ping Fu Bradley W. Goodfellow Natacha Gribenski Jakob Heyman Jennifer C. Newall Arjen P. Stroeven SVENSK KÄRNBRÄNSLEHANTERING ISBN 978-91-980362-7-5 SKB ID 1545666 June 8–10, 2016 Third Nordic Workshop on cosmogenic nuclide techniques Celebrating 30 years of counting cosmogenic atoms Editors Robin Blomdin1, Ping Fu2, Bradley W. Goodfellow1,3,4, Natacha Gribenski1, Jakob Heyman5, Jennifer C. Newall1,6, Arjen P. Stroeven1 1 Geomorphology and Glaciology, Department of Physical Geography & Bolin Centre for Climate Research, Stockholm University, Sweden 2 School of Geographical Sciences, The University of Nottingham Ningbo, China 3 Department of Geological Sciences & Bolin Centre for Climate Research, Stockholm University, Sweden 4 Department of Geology, Lund University 5 Department of Earth Sciences, University of Gothenburg, Sweden 6 Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, USA Keywords: Glacial erosion, Cosmogenic nuclides, Cosmogenic dating, Forsmark, Excursion guide, Third Nordic Workshop on Cosmogenic Nuclide Techniques A pdf version of this document can be downloaded from www.skb.se. © 2015 Svensk Kärnbränslehantering AB Preface This proceedings volume contains the extended abstracts presented at the Third Nordic Workshop on Cosmogenic Nuclide Techniques: Celebrating 30 years of counting cosmogenic atoms, arranged by Stockholm University, June 8–10, 2016, and co-sponsored by SKB. It also contains the field guide for the post-workshop excursion to Forsmark, held on June 11, 2016.
    [Show full text]
  • Extraction and Measurement of Cosmogenic in Situ 14C from Quartz
    EXTRACTION AND MEASUREMENT OF COSMOGENIC IN SITU 14C FROM QUARTZ PHILIP NAYSMITH Thesis presented for the degree of Master of Science University of Glasgow Scottish Universities Environmental Research Centre East Kilbride © P. Naysmith 2007 TABLE OF CONTENTS ACKNOWLEDGEMENTS ........................................................................................ iv DECLARATION......................................................................................................... v ABSTRACT .............................................................................................................. vi CHAPTER 1: INTRODUCTION................................................................................. 1 1.1. Introduction ..................................................................................................... 1 1.2. History of Surface Exposure Dating ................................................................ 4 1.3. Formation of Cosmogenic Nuclides ................................................................ 5 14 1.4. Advantages of In Situ C for Surface Exposure Dating .................................. 7 14 1.5. Previous Studies of In Situ C........................................................................ 9 14 1.6. Production Rates for In situ C..................................................................... 18 1.7. Measurement Techniques............................................................................. 20 14 1.8. Applications using In Situ C.......................................................................
    [Show full text]
  • Cosmogenic Nuclide Analysis
    ISSN 2047-0371 Cosmogenic nuclide analysis Christopher M. Darvill1 1 Department of Geography, Durham University, South Road, Durham, DH1 3LE, UK ([email protected]) ABSTRACT: Cosmogenic nuclides can be used to directly determine the timing of events and rates of change in the Earth’s surface by measuring their production due to cosmic ray-induced reactions in rocks and sediment. The technique has been widely adopted by the geomorphological community because it can be used on a wide range of landforms across an age range spanning hundreds to millions of years. Consequently, it has been used to successfully analyse exposure and burial events; rates of erosion, denudation and uplift; soil dynamics; and palaeo-altimetric change. This paper offers a brief outline of the theory and application of the technique and necessary considerations when using it. KEYWORDS: Cosmogenic nuclide, dating, chronology, landscape change, Quaternary Introduction by the geomorphological community in addressing issues such as the timing of Geochronology allows the quantification of glacial advances, fault-slip rates, rates of landscape change and timing of bedrock/basin erosion and sediment burial geomorphic events, bridging the gap between (Cockburn and Summerfield, 2004). geomorphological evidence and However, there are a number of practical and environmental or climatic variability over time. theoretical concerns that need to be Cosmogenic nuclide analysis involves the considered when applying the technique. measurement of rare isotopes which build-up in rock minerals predictably over time due to This chapter will briefly explain how bombardment of the upper few metres of the cosmogenic nuclides are produced, describe Earth’s surface by cosmic rays.
    [Show full text]
  • Cosmogenic Nuclide Dating of the Sediments of Bulmer Cavern: Implications for the Uplift History of Southern Northwest Nelson, South Island New Zealand
    Cosmogenic nuclide dating of the sediments of Bulmer Cavern: implications for the uplift history of southern Northwest Nelson, South Island New Zealand Gavin Holden A thesis submitted to Victoria University of Wellington in partial fulfilment of the requirements for the degree of Master of Science in Geology School of Geography, Environment and Earth Sciences Victoria University of Wellington November 2018 1 Frontispiece: A caver in the Wildcat Series, lower levels of Bulmer cavern. 2 Abstract The landscape of Northwest Nelson shows evidence of significant tectonic activity since the inception of the Austro-Pacific plate boundary in the Eocene. Evidence of subsidence followed by rapid uplift from the Eocene to the late Miocene is preserved in the sedimentary basins of Northwest Nelson. However, the effects of erosion mean there is very little evidence of post-Miocene tectonic activity preserved in the Northwest Nelson area. This is a period of particular interest, because it coincides with the onset of rapid uplift along the Alpine Fault, which is located to the south, and the very sparse published data for this period suggest very low uplift rates compared to other areas close to the Alpine Fault. Cosmogenic nuclide burial dating of sediments preserved in Bulmer Cavern, indicate an uplift rate of 0.13mm/a from the mid-Pliocene to the start of the Pleistocene and 0.067mm/a since the start of the Pleistocene. The Pleistocene uplift rate is similar to other published uplift rates for this period from the northern parts of Northwest Nelson, suggesting that the whole of Northwest Nelson has experienced relative tectonic stability compared to other areas close to the Alpine Fault during this period.
    [Show full text]
  • Determination Limits for Cosmogenic 10Be and Their Importance for Geomorphic Applications
    Determination limits for cosmogenic 10Be and their importance for geomorphic applications 1 S1 – Supplementary Text Cosmogenic nuclides are widely used for studying and quantifying geomorphic processes. Because of the broadness and complexity of the topic, we do not intend this text to be an exhaustive review of the method, because many detailed papers already exist on this argument (Nishiizumi et al. 1989; Lal, 1991; Brown et al., 1992; Biermann et al., 1996; Gosse and Phillips, 2001; von Blanckenburg, 2005; Dunai 2010; Balco 2011 among others). Instead, we provide a general and simplified description of how the technique can be used in rapidly eroding landscapes, particularly in the case of samples with low 10Be content. Additionally, we provide a description of how to estimate the amount of material to be collected in the field, and suggestions on how to minimize the loss of quartz during the chemical treatment of samples (Portenga et al., 2015; Corbett et al., 2016). S2 – Challenges arising from samples with low 10Be/9Be ratios In a sample with low 10Be content, the sample’s 10Be/9Be ratio can be very low, and potentially drop below the range that can be precisely measured by an AMS. In cases where a low 10Be content is anticipated, higher 10Be/9Be ratios can be achieved in two ways: 1) by increasing the 10Be content in the sample, and/or 2) by reducing the amount of added 9Be carrier. However, too little carrier added to the samples can result in problematic AMS measurements, so this option may be discarded for samples with low 10Be content.
    [Show full text]