(IEE) Installation of Wind Turbines, Crater Hill, Mcmu
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NITROGEN on MARS: INSIGHTS from CURIOSITY. J. C. Stern1 , B. Sutter2, W. A. Jackson3, Rafael Na- Varro-González4, Christopher P
Lunar and Planetary Science XLVIII (2017) 2726.pdf 1 2 3 NITROGEN ON MARS: INSIGHTS FROM CURIOSITY. J. C. Stern , B. Sutter , W. A. Jackson , Rafael Na- varro-González4, Christopher P. McKay5, Douglas W. Ming6, P. Douglas Archer2, D. P. Glavin1, A. G. Fairen7,8 and Paul R. Mahaffy1. 1NASA GSFC, Code 699, Greenbelt, MD 20771, [email protected], 2Jacobs, NASA Johnson Space Center, Houston, TX 77058, 3Texas Tech University, Lubbock, TX 79409, 4Universidad Nacional Autónoma de México, México, D.F. 04510, Mexico, 5NASA Ames Research Center, Moffett Field, CA 94035, 6NASA Johnson Space Center, Houston TX 77058, 7Centro de Astrobiologia, Madrid, Spain, 8Cornell University, Ithaca, NY 14853 Introduction: Recent detection of nitrate on Mars [1] indicates that nitrogen fixation processes occurred in early martian history. Data collected by the Sample Analysis at Mars (SAM) instrument on the Curiosity Rover can be integrated with Mars analog work in order to better understand the fixation and mobility of nitrogen on Mars, and thus its availability to putative biology. In particular, the relationship between nitrate and other soluble salts may help reveal the timing of nitrogen fixation and post-depositional behavior of nitrate on Mars. In addition, in situ measurements of nitrogen abundance and isotopic composition may be used to model atmospheric conditions on early Mars. Methods: The data presented are from analyses of solid Martian drilled and scooped samples by the Sam- ple Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory (MSL) Curiosity Rover. SAM performs evolved gas analysis (EGA), in which a 3 Figure 1. -
Non-Collider Searches for Stable Massive Particles
Non-collider searches for stable massive particles S. Burdina, M. Fairbairnb, P. Mermodc,, D. Milsteadd, J. Pinfolde, T. Sloanf, W. Taylorg aDepartment of Physics, University of Liverpool, Liverpool L69 7ZE, UK bDepartment of Physics, King's College London, London WC2R 2LS, UK cParticle Physics department, University of Geneva, 1211 Geneva 4, Switzerland dDepartment of Physics, Stockholm University, 106 91 Stockholm, Sweden ePhysics Department, University of Alberta, Edmonton, Alberta, Canada T6G 0V1 fDepartment of Physics, Lancaster University, Lancaster LA1 4YB, UK gDepartment of Physics and Astronomy, York University, Toronto, ON, Canada M3J 1P3 Abstract The theoretical motivation for exotic stable massive particles (SMPs) and the results of SMP searches at non-collider facilities are reviewed. SMPs are defined such that they would be suffi- ciently long-lived so as to still exist in the cosmos either as Big Bang relics or secondary collision products, and sufficiently massive such that they are typically beyond the reach of any conceiv- able accelerator-based experiment. The discovery of SMPs would address a number of important questions in modern physics, such as the origin and composition of dark matter and the unifi- cation of the fundamental forces. This review outlines the scenarios predicting SMPs and the techniques used at non-collider experiments to look for SMPs in cosmic rays and bound in mat- ter. The limits so far obtained on the fluxes and matter densities of SMPs which possess various detection-relevant properties such as electric and magnetic charge are given. Contents 1 Introduction 4 2 Theory and cosmology of various kinds of SMPs 4 2.1 New particle states (elementary or composite) . -
Perchlorate and Chlorate Biogeochemistry in Ice-Covered Lakes of the Mcmurdo Dry Valleys, Antarctica
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 98 (2012) 19–30 www.elsevier.com/locate/gca Perchlorate and chlorate biogeochemistry in ice-covered lakes of the McMurdo Dry Valleys, Antarctica W. Andrew Jackson a,⇑, Alfonso F. Davila b,c, Nubia Estrada a, W. Berry Lyons d, John D. Coates e, John C. Priscu f a Department of Civil and Environmental Engineering, Texas Tech University, Lubbock, TX 79409, USA b NASA Ames Research Center, Moffett Field, CA 95136, USA c SETI Institute, 189 Bernardo Ave., Suite 100, Mountain View, CA 94043-5203, USA d Byrd Polar Research Center, The Ohio State University, Columbus, OH 43210, USA e Department of Plant and Microbial Biology, University of California, Berkeley, CA 94720, USA f Department of Land Resources & Environmental Sciences, Montana State University, Bozeman, MT 59717, USA Received 15 February 2012; accepted in revised form 5 September 2012; available online 19 September 2012 Abstract À À We measured chlorate (ClO3 ) and perchlorate (ClO4 ) concentrations in ice covered lakes of the McMurdo Dry Valleys À À (MDVs) of Antarctica, to evaluate their role in the ecology and geochemical evolution of the lakes. ClO3 and ClO4 are À À present throughout the MDV Lakes, streams, and other surface water bodies. ClO3 and ClO4 originate in the atmosphere and are transported to the lakes by surface inflow of glacier melt that has been differentially impacted by interaction with soils À À and aeolian matter. Concentrations of ClO3 and ClO4 in the lakes and between lakes vary based on both total evaporative concentration, as well as biological activity within each lake. -
NO ONE KNOWS ABOUT US by Bridget Canning. a Creative Writing
NO ONE KNOWS ABOUT US By Bridget Canning. A Creative Writing Thesis submitted to the School of Graduate Studies in partial fulfillment of the requirements for the degree of Masters of Arts in English (Creative Writing) Department of English, Memorial University of Newfoundland Abstract: No One Knows about Us is a collection of twelve contemporary short stories. As the title suggests, the characters in each story deal with secrets: relationships, longings, grudges, addictions, and trickery. For them, these secrets are simultaneously overwhelming and futile; their importance within their small worlds reflect a deeper feeling of insignificance in the greater scheme of life in a small city in a northern province hemmed on to the side of a continent. Here are a range of characters and situations set in St. John’s, Newfoundland and Labrador. The stories are mapped out in different areas of the city and move chronologically over a year, starting in fall and ending in late summer. They work together to create a small sample of life in modern-day St. John’s – one that is informed by the influences of history, economy, and weather. i Acknowledgements: This thesis would not have been accomplished without the help of the English department faculty at Memorial such as Robert Finley, Robert Chafe, and especially my thesis advisor, Lisa Moore. Thanks to the Graduate Society for their financial support. Thanks to Jonathan Weir, Deirdre Snook, and the members of the Naked Parade Writing Collective for their guidance and encouragement. ii Contents: 1. Seen, p. 1 2. With Glowing Hearts, p. 19 3. -
Geology of Hut Point Peninsula, Ross Island
significantly below their Curie temperatures (approxi- Wilson, R. L., and N. D. Watkins. 1967. Correlation of mately 550°C.). petrology and natural magnetic polarity in Columbia Plateau basalts. Geophysical Journal of the Royal Astro- Previous work (Pucher, 1969; Stacey and Banerjee, nomical Society, 12(4): 405-424. 1974) indicates that the CRM intensity acquired in a low field is significantly less than the TRM intensity. It thus would appear that if a CRM induced at temperatures considerably below the Curie tempera- Geology of Hut Point Peninsula, ture, contributes a significant proportion to the ob- Ross Island served NRM intensity, too low an intensity value will be assigned to the ancient field. Although it is too early to report a firm value for PHILIP R. KYLE the intensity of the ancient field during the imprint- Department of Geology ing of unit 13 and related flows, we think that the Victoria University strength of the ambient field was more likely to Wellington, New Zealand have been about 0.5 oe (based on samples at about 141 meters) than about 0.1 oe (based on samples SAMUEL B. TREVES 122.18 and 126.06 meters). The virtual dipole Department of Geology moment (Smith, 1967b) calculated for an estimated University of Nebraska field intensity of 0.5 oe at the site is 7 X 10 25 gauss Lincoln, Nebraska 68508 cubic centimeters. This is larger than the value of 5.5 X 1025 gauss cubic centimeters (Smith, 1967b) Hut Point Peninsula is about 20 kilometers long calculated on the basis of paleointensity experiments and 2 to 4 kilometers wide. -
Clean Tech Handbook for Asia Pacific May 2010
Clean Tech Handbook for Asia Pacific May 2010 Asia Pacific Clean Tech Handbook 26-Apr-10 Table of Contents FOREWORD .................................................................................................................................................. 16 1 INTRODUCTION.................................................................................................................................... 19 1.1 WHAT IS CLEAN TECHNOLOGY? ........................................................................................................................ 19 1.2 WHY CLEAN TECHNOLOGY IN ASIA PACIFIC? .......................................................................................................19 1.3 FACTORS DRIVING THE CLEAN TECH MARKET IN ASIA PACIFIC .................................................................................20 1.4 KEY CHALLENGES FOR THE CLEAN TECH MARKET IN ASIA PACIFIC ............................................................................20 1.5 WHO WOULD BE INTERESTED IN THIS REPORT? ....................................................................................................21 1.6 STRUCTURE OF THE HANDBOOK ........................................................................................................................ 21 PART A – COUNTRY REVIEW.......................................................................................................................... 22 2 COUNTRY OVERVIEW.......................................................................................................................... -
Living and Working at USAP Facilities
Chapter 6: Living and Working at USAP Facilities CHAPTER 6: Living and Working at USAP Facilities McMurdo Station is the largest station in Antarctica and the southermost point to which a ship can sail. This photo faces south, with sea ice in front of the station, Observation Hill to the left (with White Island behind it), Minna Bluff and Black Island in the distance to the right, and the McMurdo Ice Shelf in between. Photo by Elaine Hood. USAP participants are required to put safety and environmental protection first while living and working in Antarctica. Extra individual responsibility for personal behavior is also expected. This chapter contains general information that applies to all Antarctic locations, as well as information specific to each station and research vessel. WORK REQUIREMENT At Antarctic stations and field camps, the work week is 54 hours (nine hours per day, Monday through Saturday). Aboard the research vessels, the work week is 84 hours (12 hours per day, Monday through Sunday). At times, everyone may be expected to work more hours, assist others in the performance of their duties, and/or assume community-related job responsibilities, such as washing dishes or cleaning the bathrooms. Due to the challenges of working in Antarctica, no guarantee can be made regarding the duties, location, or duration of work. The objective is to support science, maintain the station, and ensure the well-being of all station personnel. SAFETY The USAP is committed to safe work practices and safe work environments. There is no operation, activity, or research worth the loss of life or limb, no matter how important the future discovery may be, and all proactive safety measures shall be taken to ensure the protection of participants. -
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The Antarctic Sun, December 19, 1999
On the Web at http://www.asa.org December 19, 1999 Published during the austral summer at McMurdo Station, Antarctica, for the United States Antarctic Program Ski-plane crashes at AGO-6 By Aaron Spitzer The Antarctic Sun Two pilots escaped injury Sunday when their Twin Otter aircraft crashed during takeoff from an isolated landing site in East Antarctica. The plane, a deHavilland Twin Otter turboprop owned by Kenn Borek Air Ltd. and chartered to the U.S. Antarc- tic Program, was taking off around 3:15 p.m. Sunday when it caught a ski in the snow and tipped sideways. A wing hit the ground and the plane suffered Congratulations, it’s a helicopter! extensive damage. A New Zealand C-130 delivers a Bell 212 helicopter to the ice runway last week. The new The accident occurred on a tempo- arrival took the place of the Royal New Zealand Air Force helo used in the first part of the rary skiway at Automated Geophysical season. Photo by Ed Bowen. Observatory 6, located in Wilkes Land, about 800 miles northwest of McMurdo. The pilots had flown to the site earlier in the day from McMurdo Station to drop Testing tainted waters off two runway groomers, who were preparing the strip for the arrival of an By Josh Landis LC-130 Hercules ski-plane. The Antarctic Sun On Monday afternoon, another Kenn Borek Twin Otter, chartered to the Most scientists come to Antarctica because it gives them a chance to do their Italian Antarctic Program at Terra Nova work in the most pristine conditions on Earth. -
A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars
minerals Review A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars Joanna Clark 1,* , Brad Sutter 2, P. Douglas Archer Jr. 2, Douglas Ming 3, Elizabeth Rampe 3, Amy McAdam 4, Rafael Navarro-González 5,† , Jennifer Eigenbrode 4 , Daniel Glavin 4 , Maria-Paz Zorzano 6,7 , Javier Martin-Torres 7,8, Richard Morris 3, Valerie Tu 2, S. J. Ralston 2 and Paul Mahaffy 4 1 GeoControls Systems Inc—Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA 2 Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (B.S.); [email protected] (P.D.A.J.); [email protected] (V.T.); [email protected] (S.J.R.) 3 NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (D.M.); [email protected] (E.R.); [email protected] (R.M.) 4 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] (A.M.); [email protected] (J.E.); [email protected] (D.G.); [email protected] (P.M.) 5 Institito de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico City 04510, Mexico; [email protected] 6 Centro de Astrobiología (INTA-CSIC), Torrejon de Ardoz, 28850 Madrid, Spain; [email protected] 7 Department of Planetary Sciences, School of Geosciences, University of Aberdeen, Aberdeen AB24 3FX, UK; [email protected] 8 Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Armilla, 18100 Granada, Spain Citation: Clark, J.; Sutter, B.; Archer, * Correspondence: [email protected] P.D., Jr.; Ming, D.; Rampe, E.; † Deceased 28 January 2021. -
The Mcmurdo Dry Valleys of Antarctica As an Analog for Past and Present Martian Surface Processes
51st Lunar and Planetary Science Conference (2020) 1777.pdf THE MCMURDO DRY VALLEYS OF ANTARCTICA AS AN ANALOG FOR PAST AND PRESENT MARTIAN SURFACE PROCESSES. M. R. Salvatore1, J. S. Levy2, J. W. Head3, and J. L. Dickson4, 1Department of Astronomy and Planetary Science, Northern Arizona University, [email protected], 2Dept. of Geology, Colgate University, 3Dept. of Earth, Environmental, and Planetary Sciences, Brown University, 4Division of Geological and Planetary Sciences, Caltech. Introduction: The McMurdo Dry Valleys (MDV) of observed on Mars. We also highlight where additional Antarctica have been considered a valuable martian work in the MDV is necessary to address outstanding analog since the Viking era of Mars exploration [1]. Over questions in martian science. the past two decades, our understanding of martian Cold and Icy Early Mars?: The apparent environmental and geologic evolution has significantly disagreement between observed fluvial and lacustrine improved thanks to the plethora of orbital and landed landforms and the inability for global climate models to missions. New observations have raised many new produce mean annual temperatures greater than 0º C enigmatic questions about how cold and dry geological suggest that the martian surface was possibly never systems evolve, which has revitalized the MDV as an clement from a terrestrial perspective. Instead of a long- important terrestrial analog for Mars, from its earliest lived and continuously active hydrological system on recorded geologic history [2] to the present [3]. early Mars, is it possible that hydrological activity was Global martian climate models struggle to produce more episodic through punctuated climatic excursions on consistently warm and wet conditions at the martian an otherwise cold and icy early Mars? The fluvial and surface early in its history, even with the aid of additional lacustrine systems of the MDV are one possible analog greenhouse gases to offset the distance between Mars and where localized climatic optima drive local hydrological the faint young Sun [4]. -
Economic Benefits of Wind Farms in New Zealand
Report to: New Zealand Wind Energy Association ECONOMIC BENEFITS OF WIND FARMS IN NEW ZEALAND Final report Prepared by Jason Leung-Wai Amapola Generosa June 2012 Copyright© BERL BERL ref #5157 JEL Classification: Final report Economic benefits of wind farms in New Zealand 1 Summary .......................................................................................... 4 2 Introduction .................................................................................... 10 2.1 Methodology .......................................................................................... 10 2.1 Format of the report ............................................................................... 12 3 Electricity supply and forecasts ................................................... 13 3.1 New Zealand Energy Outlook, 2011 ..................................................... 13 3.2 Wind Energy Association growth target ................................................ 14 4 Analysis .......................................................................................... 15 4.1 Local and overseas studies ................................................................... 15 4.2 Survey ................................................................................................... 18 4.3 Case studies .......................................................................................... 18 4.4 Summary ............................................................................................... 18 5 The wind energy industry in New Zealand