For Better Crops Benefits of Sulfate 3

Total Page:16

File Type:pdf, Size:1020Kb

For Better Crops Benefits of Sulfate 3 Benefits of sulfate New fertilizer Polysulphate Readily available sulfur plus potassium, magnesium and calcium for better crops Benefits of sulfate 3 19.2% S 14% K2O 3.6% Mg 12.2% Ca Mined in the UK, ICL is the first – and only – producer in The need for sulfur application the world to mine polyhalite, marketed as Polysulphate™. Sulfate is now established as a major fertilizer requirement for arable crops and grassland. Yet most farmland never receives a routine application. Sulfur fertility has historically not been a major concern for growers on most soils, as soil organic matter, atmospheric deposition, manure application and incidental sulfur contained in fertilizers have typically supplied sufficient sulfur for crop production. However, reductions in the amount of sulfur contributed by these factors combined with increased sulfur removal with greater crop yields have made sulfur deficiencies more common. According to The Sulphur Institute, it is estimated that about 20% of arable lands in North America suffers sulfur deficiency at present. Benefits of sulfate 5 Historically, in industrialized countries arable crops and grassland had never required sulfate applications. Coal-burning had always ensured plenty of sulphur was supplied via atmospheric deposition. Regulation has ensured this deposition is now a fraction of what it used to be. As a result, large areas of farmed land are sulphur deficient, particularly those with lighter soils or lower rainfall. NATIONAL EMISSIONS OF SULFUR DIOXIDE (SO2) IN USA 35,000 30,000 25,000 2 20,000 15,000 ‘000 tons SO ‘000 10,000 5,000 0 Livestock requirements 1970 1975 1980 1985 1990 1995 2000 2005 2010 2015 Like arable crops, grassland needs sulfate fertilizer – it’s a vital input to ensure a healthy ruminant diet. Even where manure Nitrogen (N) and sulfur (S) are both essential constituents of plant and animal protein, so now that sulfur is no longer freely available from the and slurry are returned to the land, extra applications are atmosphere, wherever nitrogen fertilizers are applied there is likely to be a often needed. need for a balancing sulfate fertilizer to ensure yield and quality. In the UK, only around 10% of grassland currently receives sulfate fertilizer. Legumes such as peas, beans, alfalfa/lucerne and clover, which rely on But a shortage will reduce grass yield and efficient nitrogen utilization, atmospheric nitrogen but are now deprived of similar sulfur, will now increase nitrate loss and reduce sugar content and digestibility1. Grass almost certainly respond to a sulfate fertilizer. grown for silage is particularly liable to sulfur deficiency. This booklet introduces a sulfate fertilizer, PolysulphateTM. This new product is mined in the UK, and with 19.2% S, provides a reliable and readily available new source of sulfate. 1 G. Fisher, J. Buss et al., 2011, Grassland Report, British Grassland Society, UK 4 Benefits of sulfate 7 As with arable crops, grass also requires a balance between nitrogen and DAILY LIVEWEIGHT GAIN OF LAMBS INCREASES sulfur for its protein content, and a lack of sulfur will lead to reduced yields AS FEED N:S RATIO IMPROVES and to increased levels of non-protein nitrogen in the feed (see chart). Source: Rendig and Weir, J. Anim. Sci. 16(2) BENEFICIAL EFFECT OF S-FERTILIZATION ON NON-PROTEIN 0.17 N CONTENT OF GRASS Source: Baker A.S. et al. Sulfur Inst J. 9(1), 14-16 0.15 25 R² = 0.85324 0.13 20 0.11 15 Daily liveweight gain – pounds 10 0.09 17:1 16:1 15:1 14:1 13:1 12:1 11:1 N : S ratio in grass 5 N:S ratio of feed 0 1.4 1.2 1.0 0.8 0.6 0.4 0.2 IMPROVED N:S RATIO INCREASES D-VALUE OF FEED FOR DAIRY COWS Source: Bouchard and Conrad, J. Dairy Sci. 56 Non-protein nitrogen content – NPN % Research on silage carried out by IGER at North Wyke (now part of 72 Rothamsted Research, UK) found dry matter yields increased by 35% over three cuts on sandy loam soil where sulfate was applied2. Nitrate losses were cut by up to 82%, while the true protein and soluble sugars content of 70 the silage were boosted by 25% and 30% respectively. Perhaps even more importantly, the microbes in the rumen also need the 68 correct balance of nitrogen and sulfur. If the grass is short of sulfur they will not be able to use all of its potential feed value. This means that the actual Apparent D-value of feed digestibility (D-value) of the feed is reduced and part of the feed value is 66 wasted (see charts). 36:1 20:1 14:1 12:1 N:S ratio of feed 2 L. Brown, D. Scholefieldet al., 2000, The effect of sulfur application on the efficiency of nitrogen use in two contrasting grassland soils, Journal of Agricultural Science, Vol 135 6 Sources of sulfate 9 Sulfur from manure and slurry Sulfur in soil and in the plant Farmyard manure and slurry contain significant quantities of sulfur. When fresh much of this becomes Sulfate behaves like nitrate in the soil. In the plant nitrogen available to the plant. But in storage the activity of and sulfur are both essential building blocks for proteins. anaerobic bacteria can reduce the sulfate to sulfide and Sulfur deficiency will severely reduce the efficient use of combine it into organic complexes. These cannot be nitrogen and limit protein synthesis. utilized by plants, but gradually oxidize back to sulfate Sulfur can only be taken up by plants from the soil solution as sulfate. over time. As with readily-available nitrate, it can be liable to loss through leaching. Spring application of sulfate fertilizer is therefore recommended so that There is little reliable data on the actual availability the plant can take it up during the period of active growth, as with nitrate. of sulfur in stored manures, so it is therefore best to Sulfur is required together with nitrogen for the formation of proteins and consider it as contributing to overall soil reserves, rather uptake timings are similar. than supplying sufficient nutrient for the current crop. Some atmospheric Sulfate in deposition of S fertilizer Uptake Dung/urine Crop residue Crop Mineral S Sulfate in S in organic in the soil soil solution material Desorption Immobilization Adsorption Mineralization Leaching 8 Sources of sulfate 11 Elemental sulfur While sulfate fertilizer is immediately available to the crop, applications of elemental sulfur must be converted to sulfate by bacterial activity in the soil before it becomes available. The time taken for this oxidation is unpredictable and may take many months, so the sulfate required by the crop may not be available when needed. Protein synthesis Sulfur is required for many growth functions in plants – like nitrogen it is principally an essential constituent of protein. There is therefore a close relationship between the quantities of nitrogen and sulfur in crops, with most taking up about 1 pound of sulfur for every 12 pounds of nitrogen. SULFUR UPTAKES BY WHEAT, POTATO AND CABBAGE 20 90 18 80 16 70 Once taken up, unlike nitrogen, sulfur does not move against the 14 60 transpiration stream and cannot be taken from older leaves, for example, 12 50 to support new growth. So a sufficient and continuous supply is needed in 10 40 the soil to satisfy all the needs of the growing crop. 8 30 6 Wheat Signs of deficiency include the yellowing of young leaves or new growth. By 4 Potato 20 contrast, yellowing from nitrogen deficiency affects the older leaves first. Wheat and potato – lb S/ac Wheat and potato – lb Cabbage Sulfur in Cabbage – lbS/ac 2 10 Sulfur-deficient oilseed rape can also have purpling and upward cupping of 0 0 1 2 3 4 5 6 7 9 8 10 11 12 13 14 15 16 17 18 19 young leaves, delayed and prolonged flowering, pale-colored flowers, and Week of sampling in spring fewer, smaller pods. Brassica crops, such as oilseed rape, cabbage and kale, require much more sulfate. They need extra sulfur for the production of glucosinolates, which are used within the plants as a defense mechanism. 10 Polysulphate 13 BOULBY MINE STRATIGRAPHY JURASSIC SURFACE 0 Sea level 100 200 Iias shales 300 Penarth Group 400 PERMIAN STRATA 190 million years 500 Mercia Mudstones 1000 Halite with mudstone interbeds TRIASSIC 600 Halite 700 Anhydrite POTASH Marl (clay) 800 MINE 1100 Halite Introducing Polysulphate Sherwood Sandstone LEVEL 900 Anhydrite Polysulphate is a new fertilizer, high in sulfate, available in its natural state, and mined in the UK. A unique benefit is its Dolomite PERMIAN 1000 Anhydrite additional natural content of other macronutrients. 225 million years 1200 1100 Halite POLYSULPHATE Polyhalite Polysulphate comes from the polyhalite layer of rock, over 3,300 ft below 1200 MINE LEVEL the North Sea off the North Yorkshire coast in the UK. Deposited 260 Anhydrite million years ago, it lies 490-560 ft below the potash seam at the Cleveland Permian Evaporites 1300 Potash Boulby Mine. 1300 1400 Dol/Lst The main Polysulphate seam was reached in September 2010, bringing the (lower evaps) first samples up to the surface. It is estimated there are one billion tons CARBONIFEROUS 1500 available from this one source. Polysulphate is available as both a granular and powder product. The 1400 2-4mm granular product has excellent spreading characteristics and is an ideal fertilizer to apply alongside straight nitrogen. Depth below surface in meters 1500 12 Trials information 15 Polysulphate contains How Polysulphate performs • 19.2% S as sulfate • 14% K2O as from sulfate of potash • 3.6% Mg as from magnesium sulfate Proprietary and independent trials work have shown • 12.2% Ca as from calcium sulfate Polysulphate to be as good as the best sources available of the principal nutrients it contains.
Recommended publications
  • Deep Science at Boulby Underground Laboratory
    Sean Paling STFC Boulby Underground Science Facility Hartlepool Nuclear Power Station Astroparticle Physics: the search for Dark Matter & beyond Earth and environmental science, Astrobiology and planetary exploration CYGNUS Directional Dark Matter search Deep Science at Boulby Underground Laboratory: Subterranean studies at the UK’s deep underground science facility Underground lab @ Boulby World antineutrino flux levels A WATer CHerenkov Monitor of ANtineutrinos Design, excavation, installation & operation 2019 to 2026(+) A 6kT Gd- loaded water detector looking at ~20 m anti-neutrinos from Hartlepool nuclear reactor • 3500 tons of gadoliniumVertices doped water within 50cm • 3000 photomultiplier tubes Funding: US (>$70M), UK (~£10M) • Signal: ~11 events/month/core confirmed in 2017 & 2018 respectively • ΔTBackground: ~30μs ~20 events/month NEW 6kT prototype detector: R&D for anti-neutrino monitoring of nuclear reactors for global nuclear non-proliferation purposes & more Deep Science @ Boulby Underground Laboratory… 1) About Boulby Mine and Boulby Underground Lab 2) Boulby Science Overview: • Astroparticle Physics & Low Background Science • Earth & Environmental Science • Astrobiology & Planetary Exploration Studies 3) The future: inc. AIT-NEO (WATCHMAN) Boulby Underground Laboratory The UK’s deep underground science facility operating in a working polyhalite & salt mine. 1.1km depth (2805 mwe). With low background surrounding rock-salt Operated by the UK’s Science & Technology Facilities Council (STFC) in partnership with the mine operators ICL Polyhalite Deepest mine in Britain Permian Evaporites Factor ~106 reduction in cosmic ray flux vs. surface A QUIET place in the Universe Boulby Geology & Mining Major local employer. Open since 1968. Originally mining potash (KCl) for fertiliser. Now first and only producers of polyhalite Excavations are in Salt (NaCl) & Potash (KCl) Permian evaporite layers left over from the Zechstein Sea.
    [Show full text]
  • IUPAP Report 41A
    IUPAP Report 41a A Report on Deep Underground Research Facilities Worldwide (updated version of August 8, 2018) Table of Contents INTRODUCTION 3 SNOLAB 4 SURF: Sanford Underground Research Facility 10 ANDES: AGUA NEGRA DEEP EXPERIMENT SITE 16 BOULBY UNDERGROUND LABORATORY 18 LSM: LABORATOIRE SOUTERRAIN DE MODANE 21 LSC: LABORATORIO SUBTERRANEO DE CANFRANC 23 LNGS: LABORATORI NAZIONALI DEL GRAN SASSO 26 CALLIO LAB 29 BNO: BAKSAN NEUTRINO OBSERVATORY 34 INO: INDIA BASED NEUTRINO OBSERVATORY 41 CJPL: CHINA JINPING UNDERGROUND LABORATORY 43 Y2L: YANGYANG UNDERGROUND LABORATORY 45 IBS ASTROPHYSICS RESEARCH FACILITY 48 KAMIOKA OBSERVATORY 50 SUPL: STAWELL UNDERGROUND PHYSICS LABORATORY 53 - 2 - __________________________________________________INTRODUCTION LABORATORY ENTRIES BY GEOGRAPHICAL REGION Deep Underground Laboratories and their associated infrastructures are indicated on the following map. These laboratories offer low background radiation for sensitive detection systems with an external users group for research in nuclear physics, astroparticle physics, and dark matter. The individual entries on the Deep Underground Laboratories are primarily the responses obtained through a questionnaire that was circulated. In a few cases, entries were taken from the public information supplied on the lab’s website. The information was provided on a voluntary basis and not all laboratories included in this list have completed construction, as a result, there are some unavoidable gaps. - 3 - ________________________________________________________SNOLAB (CANADA) SNOLAB 1039 Regional Road 24, Creighton Mine #9, Lively ON Canada P3Y 1N2 Telephone: 705-692-7000 Facsimile: 705-692-7001 Email: [email protected] Website: www.snolab.ca Oversight and governance of the SNOLAB facility and the operational management is through the SNOLAB Institute Board of Directors, whose member institutions are Carleton University, Laurentian University, Queen’s University, University of Alberta and the Université de Montréal.
    [Show full text]
  • The Current Status and Planned Developments for Deep Underground Astro-Particle Physics Science Facilities
    12th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2011) IOP Publishing Journal of Physics: Conference Series 375 (2012) 042059 doi:10.1088/1742-6596/375/4/042059 The Current Status and Planned Developments for Deep Underground Astro-particle Physics Science Facilities N.J.T.Smith SNOLAB, 1039 Regional Road 24, Lively, Ontario, P3Y 1N2, Canada E-mail: [email protected] Abstract. The rigorous radiation background constraints imposed by several studies in particle and astro-particle physics, such as Galactic dark matter searches, man-made, terrestrial, solar and supernova neutrino studies and 0νββ-decay studies, require deep underground science facilities to afford shielding from penetrating cosmic rays and their secondary by-products. New threads of research focused on deep sub-surface biology, chemistry, geology and engineering have also been developing rapidly at several sites, benefitting from the significant investment in underground access and infrastructure developed. In addition to planned, or completed, expansion at several of these deep underground facilities, additional new facilities are in early stages of construction or well advanced planning. These developments provide significant additional capability to these fields of study. This paper summarises the developments at these facilities, focused on those extremely deep uderground laboratories where expansion is underway or planned. 1. Introduction Searches for rare decay channels or weak interactions in particle or astro-particle physics studies require the observation of rare events in dedicated detector systems. These rare events need to be observed against the significant backgrounds created by cosmic-ray and radioactive- contaminant generated signals. To enable the observation of these exquisite signal events, experiments must therefore be operated in the quiet environment afforded by shielded facilities in deep underground laboratories.
    [Show full text]
  • Potash – Recent Exploration Developments in North Yorkshire
    F.W. Smith, J.P.L. Dearlove, S.J. Kemp, C.P. Bell, C.J. Milne and T.L. Pottas POTASH – RECENT EXPLORATION DEVELOPMENTS IN NORTH YORKSHIRE 1 1 2 1 2 3 F.W. SMITH , J.P.L. DEARLOVE , S.J. KEMP , C.P. BELL , C.J. MILNE AND T.L. POTTAS 1 FWS Consultants Ltd, Merrington House, Merrington Lane Trading Estate, Spennymoor DL16 7UT. 2 British Geological Survey, Nicker Hill, Keyworth, Nottingham. NG12 5GG. 3 York Potash Ltd, 7-10 Manor Court, Scarborough. YO11 3TU. ABSTRACT Polyhalite is not a rare mineral worldwide, but it rarely forms more than a minor component of evaporite sequences. York Potash Ltd is exploring an area of interest between Whitby and Scarborough, North Yorkshire, UK, in which an Exploration Target of 6.8 to 9.5 billion tonnes has been identified. Polyhalite exploration by York Potash has primarily been by drilling boreholes from surface, that are then cored through the Zechstein evaporite sequence. Assay samples have been analysed initially by quantitative X-ray diffraction, with subsequent analyses by Inductively Coupled Plasma Atomic Emission Spectroscopy. The assay results reported in this paper for the weighted average ore zone sections range from 78 to 97% polyhalite, with high grade sections in places exceeding 99% polyhalite. The exploration results have lead to a revised conceptual model for the Fordon Evaporites in North Yorkshire, in particular defining the differences between the three depositional environments of the Shelf, Basinal and intervening Transitional or Ramp facies and the occurrence of additional potash horizons in the region. Of particular significance was the discovery of accessory or exotic minerals associated with the polyhalite.
    [Show full text]
  • AIT/WATCHMAN @ Boulby Lab: Overview of Boulby Lab & Our Science
    Sean Paling STFC Boulby Underground Laboratory Hartlepool Nuclear Boulby Science – the search for Power Station Dark Matter & Beyond The Watchman Project AIT/WATCHMAN @ Boulby Lab: Overview of Boulby Lab & our Science. Progress & considerations for the new AIT/WATCHMAN project. New Underground lab @ Boulby Boulby Mine A working potash, polyhalite and rock- salt mine on the North East of England. Owned by Israel Chemicals Ltd. (ICL-UK) Major local employer - ~700 direct and 3000 indirect employment. Middlesborough Staithes Whitby Polyhalite York Deepest mine in Britain: 1100m Potash (KCl) Mines ~1 million tonnes of Potash / year. Supplies ~ 50% of the UK’s potash Whitby View from Staithes Boulby Geology & Mining Excavations are in Salt (NaCl) & Potash (KCl) Permian evaporite layers left over from the Zechstein Sea. Over 40 kms of tunnel mined each year (now >1,000kms in total), the long-lived roadways being cut in the lower NaCl layer. Typical Boulby U: 67 ± 6 ppb Salt Roadway Th: 125 ± 10 ppb Low γ & n backgrounds Zechstein Sea Low Rn (<3 Bqm-3) Potash Mine Shafts Rock-Salt New Lab (2017) Polyhalite Boulby Geology [email protected] Boulby Underground Laboratory The UK’s deep underground science facility operating in a working potash and salt mine. 1.1km depth (2805 mwe). With low background surrounding rock-salt Operated by the UK’s Science Outside & Technology Facilities Council Experimentation (STFC) in partnership with the Area (OEA) mine operators ICL-UK Permian Evaporites 4000m3 class 10k and 1k clean lab Factor ~106 space reduction in cosmic ray flux vs. surface A QUIET place in the Universe Underground Science @ Boulby Mine • DRIFT: Directional Dark Matter Search • BUGS: Ultra-low background material screening (for LUX-ZEPLIN and Super-K-Gd and more) • ERSaB: Environmental gamma spectroscopy DRIFT-II • Deep Carbon: Muon Tomography for CCS (etc) • SELLR: Life in Low background radiation • BISAL: Geomicrobiology / Astrobiology studies • MINAR: Space Exploration Tech.
    [Show full text]
  • 7 Underground Laboratory Capabilities
    7 Underground Laboratory Capabilities Convener: M. G. Gilchriese P. Cushman, K. Heeger, J. Klein, K. Scholberg, H. Sobel, M. Witherell 7.1 Introduction Many of the most compelling scientific issues in particle physics can only be addressed with experiments operating at underground facilities. For example, large underground facilities are needed for direct searches for dark matter and neutrinoless double-beta decay (0νββ), and the scale and complexity of these experiments will continue to increase for the foreseeable future. The importance of underground experiments using solar, reactor, atmospheric, supernova neutrinos and neutrinos from accelerators to elucidate neutrino properties is also expected to grow over the next decade and beyond. Underground facilities are located in North America, Europe, Asia and Antarctica (ice). In the last few years, new underground facilities have become operational in Canada (SNOLAB), China (China JinPing Deep Underground Laboratory { CJPL), Spain (Canfranc Laboratory, or Laboratorio Subterr´aneode Canfranc { LSC) and in the United States (Sanford Underground Research Facility { SURF). Experiments continue to be operated or assembled at older underground facilities in Asia, Europe, the United States and in ice at the South Pole. The world-wide particle physics community plans to expand underground capabilities over the next few years. Significant expansions are underway or planned in China (CJPL and JUNO), Korea (RENO50 and Yangyang Laboratory), Japan (Hyper-K), France (Modane extension), India (India Neutrino Observatory { INO), South America (Agua Negra Deep Experiment Site { ANDES) and possibly in Finland (Center for Underground Particle Physics { CUPP). If all of these plans are realized, general-purpose space for underground experiments would roughly double by the end of the decade.
    [Show full text]
  • Boulby Underground Laboratory: the UK's Multi-Disciplinary Deep
    Sean Paling STFC Boulby Underground Science Facility Hartlepool Nuclear Astroparticle physics & ultra Power Station low background studies Earth and environmental science, AIT-NEO Astrobiology and planetary (WATCHMAN) exploration Boulby Underground Laboratory: The UK’s multi-disciplinary deep underground science facility. Status, plans and opportunities for growth Underground lab @ Boulby Boulby Underground Laboratory The UK’s deep underground science facility operating in a working polyhalite & salt mine. 1.1km depth (2805 mwe). With low background surrounding rock-salt Rock-Salt Operated by the UK’s Science & Technology Facilities Council (STFC) in partnership with the mine operators ICL Polyhalite Deepest mine in Britain Permian Evaporites Factor ~106 reduction in cosmic ray flux vs. surface A QUIET place in the Universe Boulby Geology & Mining Major local employer. Open since 1968. Originally mining potash (KCl) for fertiliser. Now first and only producers of polyhalite Excavations are in Salt (NaCl) & Potash (KCl) Permian evaporite layers left over from the Zechstein Sea. Typical Boulby Salt Roadway Potash Zechstein Sea KCl Mine Shafts Rock-Salt NaCl New Lab Polyhalite (2017) K2Ca2Mg(SO4)4·2H2O Boulby Geology Office space, chemistry & clean prep lab, storage and staging space, IT room, conference room, SurFace support and 3 staging building 3000m Outside Outside ExperimentationExperimentation Area Area Boulby Underground Lab Facilities 2020: >4000m3 class 1k & 10k clean room lab space 100Mb Internet AC, Air filtration, 5T & 10T lifting,
    [Show full text]
  • Overview of Non-Liquid Noble Direct Detection Dark Matter Experiments
    Overview of Non-Liquid Noble Direct Detection Dark Matter Experiments J. Cooley Department of Physics, Southern Methodist University, Dallas, TX 75275, USA Abstract In the last few years many advances have been made in the field of dark matter direct detection. In this article I will review the progress and status of experiments that employ detection techniques that do not use noble liquids. First, I will give an introduction to the field of dark matter and discuss the background challenges that confront all dark matter experiments. I will also discuss various detection techniques employed by the current generation and the next generation of dark matter experiments. Finally, I will discuss recent results and the status of current and future direct detection experiments. Keywords: 1. Introduction The revolution in precision cosmology of the last decade has revealed con- clusively that about a quarter of our universe consists of dark matter [1, 2]. Despite the abundant evidence for the existence of dark matter, its con- stituents have eluded detection. Phenomenology at the intersection of particle physics, cosmology and astrophysics gives well-motivated candidates for dark matter. Dark matter candidates naturally arise from theories that explain the radiative stability of arXiv:1410.4960v2 [astro-ph.IM] 3 Nov 2014 the weak scale. These theories include supersymmetry [3] and the existence of extra dimensions [4, 5, 6]. Candidates from these theories are representative of a generic class of weakly interacting massive particles (WIMPs). In the hot early universe WIMPs would have been in thermal equilibrium. They would have decoupled as the universe expanded and cooled, leaving behind a relic abundance of these particles in the universe today.
    [Show full text]
  • Introduction Status and Plans in Europe in Canada in Asia Summary
    NeSS2002 workshop, Sep.2002, Washington DC Takaaki Kajita, ICRR, U.Tokyo Outline Introduction Status and plans in Europe in Canada in Asia Summary Many thanks to: A.Bettini, L.Mosca, N.Spooner, A.Morales, D.Sinclair, S.K. Kim, K.Kuroda, T.Kishimoto Apology: Some underground labs (especially those related to geosciences, dark matter, double beta decay or cosmic ray experiments) may not be mentioned. Introduction History of particle/astroparticle physics discoveries by underground experiments year 1950’s Discovery of neutrinos (12 m underground) 1965 Observation of atmospheric neutrinos 1968 Solar neutrino problem 1987 Observation of neutrinos from SN1987A 1988 Atmospheric neutrino anomaly 1989-92 Confirmation of solar neutrino problem 1998 Discovery of neutrino oscillations 2001,2 Solar neutrino oscillation Important scientific results from underground experiments! Much more (neutrinos, p-decay, double beta decay, dark matter…) ! Why underground? : Background However, importance is experiment dependent: VERY important for ) 1 - Solar neutrino exp, year 2 Canfranc (lab3) オ flux: - キ GNOオBG = 4% of the signal Boulby 1 106 / キ SNO オ induced n capture BG (after cuts) = 9% of the signal intensity (m Deeper is better for Atmospheric neutrino exp. Muon p-decay exp. supernova neutrino exp. ゚゚ exp. Depth (m.w.e.) Dark Matter exp. Status and Pyhasalmi Lab. plans in Europe Boulby mine Baksan Canfranc Frejus Gran Sasso INFN Gran Sasso National Laboratory •1400 m rock overburden •Flat cross-section •Underground area 18 000 m2 •Support facilities on the surface Scientific programme(1): Neutrino oscillations Neutrinos from CERN (CNGS) Neutrinos from the Sun OPERA GNO Low energy solar neutrino Observe exp with 30ton -decay t Ga.
    [Show full text]
  • The Canfranc Underground Laboratory. Present and Future
    November 17, 2004 9:47 Proceedings Trim Size: 9in x 6in LSC1 THE CANFRANC UNDERGROUND LABORATORY. PRESENT AND FUTURE J. MORALES, B. BELTRAN,´ J.M. CARMONA, S. CEBRIAN,´ E. GARC´IA, I.G. IRASTORZA, H. GOMEZ,´ G. LUZON,´ M. MART´INEZ, A. MORALES,¤ A. ORT´IZ DE SOLORZANO,´ C. POBES, J. PUIMEDON,´ A. RODR´IGUEZ, J. RUZ, M.L. SARSA, L. TORRES, J.A. VILLAR. Laboratory of Nuclear and High Energy Physics University of Zaragoza, 50009 Zaragoza, Spain E-mail: [email protected] A brief history of the Canfranc Underground Laboratory is presented together with its current status. The description of a new, enlarged underground facility with a main experimental hall of 40 £ 15 £ 11 m3 and a total surface of about 1; 500 m2 at a depth of 2,450 m.w.e. is outlined as well. 1. Introduction Underground science includes a wide range of exciting disciplines in both fundamental and practical subjects in fields as diverse as Elementary Par- ticle Physics, Nuclear Physics, Astrophysics, Cosmology, Geology, Biology, Material Science, etc. By using underground laboratories one reaches the low radioactive back- ground environment needed to look for rare event physics which allows us to study, amongst many other amazing research fields, the fundamental laws of physics such as those governing the stability of the proton or the particle-antiparticle properties of the neutrino; we can probe the interior of the Sun or determine the nature of the dark matter. Figure 1 shows an incomplete list of the underground laboratories around the world, the most outstanding ones in Europe being the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, the Laboratoire Souterrain de Modane (Frejus) (LSM) in France and The Boulby Mine Underground Physics Facility in UK.
    [Show full text]
  • Dark Matter Experiments at Boulby Mine
    28th International Cosmic Ray Conference 1693 Dark Matter Experiments At Boulby Mine M.J.Carson1 for the Boulby Dark Matter Collaboration (1) Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, UK. Email: [email protected] abstract The status of galactic dark matter searches currently underway at Boulby mine in the UK is reviewed. These experiments are searching for the elusive Weakly Interacting Massive Particles (WIMPs) and utilise both scintillator and low pressure gas detectors. NaIAD and ZEPLIN are scintillator based experi- ments. The DRIFT experiment uses a low pressure gas TPC to detect recoils due to WIMP events. Recent results from both NaIAD and ZEPLIN are presented and our future programme is discussed. 1. Introduction The UK Dark Matter Collaboration (UKDMC) has been operating NaI(Tl) detectors at the Boulby Mine underground site for several years [1]. Limits on the flux of weakly interacting massive particles (WIMPs), that may constitute up to 90% of the mass of the Galaxy, have been recently set using the data from the first NaIAD detectors [2]. In recent years emphasis has shifted toward the operation of liquid Xe based detectors (the ZEPLIN program) and TPCs (DRIFT). These are potentially more senstive to WIMP signatures and, in the case of DRIFT, can provide directional information on the WIMP flux. ZEPLIN I is a liquid Xe scintillation detector and is currently one of the most sensitive dark matter detectors in operation. The initial goal of each experiment is to determine a WIMP event rate (or to put an upper limit on this rate) measured in number of events per kg per day.
    [Show full text]
  • The New Experimental Hall at Callio Lab Underground Centre for Science and R & D in the Pyhäsalmi Mine, Finland
    Deeper understanding at Lab 2: the new experimental hall at Callio Lab underground centre for science and R & D in the Pyhäsalmi Mine, Finland Master’s thesis Jari Joutsenvaara Degree Programme in Physics Oulu University May 23, 2016 2 Contents 1 Introduction 5 1.1 History . 5 1.2 Motivation . 6 2 Deep underground physics laboratories (DULs) 9 2.1 Why to go deep? . 9 2.2 Deep (>2 000 m.w.e.) underground laboratories . 10 2.3 Callio Lab (CLAB), Finland . 15 3 Background sources for underground laboratories 21 3.1 High-energy cosmic muons . 21 3.1.1 Muon Depth-Intensity-Relation (DIR) . 21 3.1.2 Methods to reduce muon background . 23 3.2 Neutron background . 23 3.2.1 Neutrons from local radioactivity . 24 3.2.2 Cosmic ray muon induced neutron background . 24 3.2.3 Reduction on neutron background . 25 3.3 Neutrino background . 26 3.3.1 Neutrinos interfering with experiments . 28 3.4 Radioactive impurities. .29 3.4.1 Radioactivity. .30 3.4.2 Radioactive decay law . 31 3.4.3 Alpha decay . 32 3.4.4 Beta decay . 34 3.5 Problematic radon . 34 4 Radon 39 4.1 History . 39 4.2 Properties of radon . 39 4.3 Radon transport mechanisms . 40 4.4 Radon contamination . 41 4.5 Radon mitigation . 42 3 5 About activated carbon-based radon removal systems 43 5.1 Adsorption of radon with activated carbon . 43 5.1.1 Principles of adsorption . 43 5.2 Activated carbon as adsorbent . 44 5.3 Radon removal systems.
    [Show full text]