Performance and Contributions of the Green Industry to Utah's Economy
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2014 Utah State Comprehensive Outdoor Recreation Plan 2014 Utah
2014 Utah State Comprehensive Outdoor Recreation Plan UTAH STATE PARKS Division of Utah State Parks and Recreation Planning Section 1594 West North Temple, Ste. 116 P.O. Box 146001 Salt Lake City, UT 84116-6001 (877) UT-PARKS stateparks.utah.gov State of Utah Figure 1. Public land ownership in Utah. ii 2014 SCORP ACKNOWLEDGEMENTS The research and publication of the 2014 Utah State Comprehensive Outdoor Recreation Plan (SCORP) is a product of a team effort. The Utah Department of Natural Resources, Division of Utah State Parks and Recreation, Utah Division of Wildlife Resources, Utah Department of Transportation, Utah Division of Water Resources, Governor’s Office of Planning and Budget, National Park Service (Omaha Regional Office), U.S. Department of Agriculture Forest Service, U.S. Department of the Interior Bureau of Land Management, U.S. Department of the Interior Bureau of Reclamation, Utah League of Cities and Towns, Utah Association of Counties, Utah Recreation and Parks Association, and others provided data, information, advice, recommendations, and encouragement. The 2014 Utah SCORP was completed under contract by BIO-WEST, Inc. (BIO-WEST), with survey work completed by Dan Jones & Associates. Key project contributors include Gary Armstrong, project manager for BIO-WEST, and David Howard, lead survey research associate for Dan Jones & Associates. Susan Zarekarizi of the Division of Utah State Parks and Recreation served as the overall project manager and provided contractor oversight. Additional staff contributing to the project include Sean Keenan of BIO-WEST, and Tyson Chapman and Kjersten Adams of Dan Jones & Associates. The 2014 Utah SCORP represents demand for future recreation facilities as identified in a series of public opinion surveys, special reports, park surveys, federal and local plans, technical reports, and other data. -
Economic Contribution of Agriclture to the Utah Economy 2014
The Economic Contribution of Agriculture to the Utah Economy in 2014 Ruby A. Ward Professor Karli Salisbury Research Assistant Dept. of Applied Economics Utah State University UMC 4835 Logan, UT 84322-4835 Prepared for Utah Department of Agriculture and Food Utah State University Economic Research Institute Report #2016-01 October 2016 Situation • The study of the economic contribution of agriculture to the Utah economy defines agriculture as the combination of the agriculture production sectors (NAICS codes 111, 112 and 115) and the agriculture processing sectors (NAICS codes 311 and 312). • Our economic analysis captures the direct sales (output) of agriculturally oriented businesses within the state, as well as the indirect and induced (multiplier) effects of these expenditures. Analysis was conducted using Version 3 of the Impact Analysis for Planning (IMPLAN) model and its 2014 database. • In 2014, production agriculture, including farming, ranching, dairy, and other related support industries, accounted for over $2.4 billion in direct output (sales), with a total of $3.5 billion in total economic output after adjustment for multiplier effects. - Based on Utah’s 2014 Gross State Product of $140 billion, production agriculture directly accounts for 1.7% of total state output and accounts for 2.5% with multiplying effects. - The production agriculture sector directly employs 18,000 people in either full or part-time positions. When including the multiplying effect, production agriculture accounts for roughly 26,000 jobs with an income compensation of $583 million. • Total direct output by the agricultural processing sector was approximately $10.7 billion in 2014. • The agriculture processing sector and the production agriculture sector combined account for $21.2 billion in total economic output in Utah after adjusting for multiplier effects. -
“Mining” Water Ice on Mars an Assessment of ISRU Options in Support of Future Human Missions
National Aeronautics and Space Administration “Mining” Water Ice on Mars An Assessment of ISRU Options in Support of Future Human Missions Stephen Hoffman, Alida Andrews, Kevin Watts July 2016 Agenda • Introduction • What kind of water ice are we talking about • Options for accessing the water ice • Drilling Options • “Mining” Options • EMC scenario and requirements • Recommendations and future work Acknowledgement • The authors of this report learned much during the process of researching the technologies and operations associated with drilling into icy deposits and extract water from those deposits. We would like to acknowledge the support and advice provided by the following individuals and their organizations: – Brian Glass, PhD, NASA Ames Research Center – Robert Haehnel, PhD, U.S. Army Corps of Engineers/Cold Regions Research and Engineering Laboratory – Patrick Haggerty, National Science Foundation/Geosciences/Polar Programs – Jennifer Mercer, PhD, National Science Foundation/Geosciences/Polar Programs – Frank Rack, PhD, University of Nebraska-Lincoln – Jason Weale, U.S. Army Corps of Engineers/Cold Regions Research and Engineering Laboratory Mining Water Ice on Mars INTRODUCTION Background • Addendum to M-WIP study, addressing one of the areas not fully covered in this report: accessing and mining water ice if it is present in certain glacier-like forms – The M-WIP report is available at http://mepag.nasa.gov/reports.cfm • The First Landing Site/Exploration Zone Workshop for Human Missions to Mars (October 2015) set the target -
Airport Report.Indd
SALT LAKE CITY INTERNATIONAL AIRPORT AIRPORT REDEVELOPMENT PROGRAM ECONOMIC IMPACT ANALYSIS September 2018 Table of Contents i TABLE OF CONTENTS I. Introduction and Summary 1 A. Project Background 1 B. State of the Utah Economy 2 C. Past Studies Summary 2 II. Methodology and Findings 3 A. Data Sources 3 B. Airport Redevelopment Program Description 3 C. Impact of Airport Redevelopment Program 4 D. Direct, Indirect and Induced Impacts of the Airport Redevelopment Program 5 i. Direct 5 ii. Indirect 5 iii. Induced 5 iv. Indirect and Induced 5 E. Estimated Benefit by Industry 6 III. Conclusion 7 IV. Appendix A – Economic Impacts Inputs 8 V. Appendix B – Annual Impacts by Sub-Project 9-12 A. Direct 9 B. Indirect 10 C. Induced 11 D. Indirect and Induced 12 VI. Appendix C - Past Studies of the Airport’s Economic Impact 13-14 Airport Redevelopment Program Economic Impact Analysis // GSBS Consulting Table of Tables iii TABLE OF TABLES TABLE 1 Terminal Redevelopment Program Analysis vs Airport Redevelopment Program Analysis TABLE 2 Annualized ARP Impact TABLE 3 ARP Annual Average Impact by Year TABLE 4 ARP Total Induced and Indirect Impact 2013-2025 TABLE 5 Total Impact Airport Redevelopment Program 2013-2025 TABLE 6 Top Ten Industries Impacted Statewide by Employment TABLE 7 Top Ten Industries Impacted Statewide by Total Output TABLE 8 Total Estimated Annual Direct Spending from All Projects TABLE 9 Total Annual Indirect Spending from All Projects TABLE 10 Total Annual Induced Spending from All Projects TABLE 11 Total Annual Indirect and Induced Spending from All Projects Airport Redevelopment Program Economic Impact Analysis // GSBS Consulting Introduction and Summary 1 I. -
Pacing Early Mars Fluvial Activity at Aeolis Dorsa: Implications for Mars
1 Pacing Early Mars fluvial activity at Aeolis Dorsa: Implications for Mars 2 Science Laboratory observations at Gale Crater and Aeolis Mons 3 4 Edwin S. Kitea ([email protected]), Antoine Lucasa, Caleb I. Fassettb 5 a Caltech, Division of Geological and Planetary Sciences, Pasadena, CA 91125 6 b Mount Holyoke College, Department of Astronomy, South Hadley, MA 01075 7 8 Abstract: The impactor flux early in Mars history was much higher than today, so sedimentary 9 sequences include many buried craters. In combination with models for the impactor flux, 10 observations of the number of buried craters can constrain sedimentation rates. Using the 11 frequency of crater-river interactions, we find net sedimentation rate ≲20-300 μm/yr at Aeolis 12 Dorsa. This sets a lower bound of 1-15 Myr on the total interval spanned by fluvial activity 13 around the Noachian-Hesperian transition. We predict that Gale Crater’s mound (Aeolis Mons) 14 took at least 10-100 Myr to accumulate, which is testable by the Mars Science Laboratory. 15 16 1. Introduction. 17 On Mars, many craters are embedded within sedimentary sequences, leading to the 18 recognition that the planet’s geological history is recorded in “cratered volumes”, rather than 19 just cratered surfaces (Edgett and Malin, 2002). For a given impact flux, the density of craters 20 interbedded within a geologic unit is inversely proportional to the deposition rate of that 21 geologic unit (Smith et al. 2008). To use embedded-crater statistics to constrain deposition 22 rate, it is necessary to distinguish the population of interbedded craters from a (usually much 23 more numerous) population of craters formed during and after exhumation. -
FROM WET PLANET to RED PLANET Current and Future Exploration Is Shaping Our Understanding of How the Climate of Mars Changed
FROM WET PLANET TO RED PLANET Current and future exploration is shaping our understanding of how the climate of Mars changed. Joel Davis deciphers the planet’s ancient, drying climate 14 DECEMBER 2020 | WWW.GEOLSOC.ORG.UK/GEOSCIENTIST WWW.GEOLSOC.ORG.UK/GEOSCIENTIST | DECEMBER 2020 | 15 FEATURE GEOSCIENTIST t has been an exciting year for Mars exploration. 2020 saw three spacecraft launches to the Red Planet, each by diff erent space agencies—NASA, the Chinese INational Space Administration, and the United Arab Emirates (UAE) Space Agency. NASA’s latest rover, Perseverance, is the fi rst step in a decade-long campaign for the eventual return of samples from Mars, which has the potential to truly transform our understanding of the still scientifi cally elusive Red Planet. On this side of the Atlantic, UK, European and Russian scientists are also getting ready for the launch of the European Space Agency (ESA) and Roscosmos Rosalind Franklin rover mission in 2022. The last 20 years have been a golden era for Mars exploration, with ever increasing amounts of data being returned from a variety of landed and orbital spacecraft. Such data help planetary geologists like me to unravel the complicated yet fascinating history of our celestial neighbour. As planetary geologists, we can apply our understanding of Earth to decipher the geological history of Mars, which is key to guiding future exploration. But why is planetary exploration so focused on Mars in particular? Until recently, the mantra of Mars exploration has been to follow the water, which has played an important role in shaping the surface of Mars. -
Collaborative Development of Narratives and Models for Steering Inter-Organizational Networks Philip C
Collaborative Development of Narratives and Models for Steering Inter-Organizational Networks Philip C. Emmi, Craig B. Forster, Jim I. Mills, Tarla Rai Peterson, Jessica L. Durfee and Frank X. Lilly University of Utah College of Architecture + Planning 375 S. 1530 East, Room 235 AAC Phone: 1-801-581-4255 Fax: 1-801-581-8217 [email protected] Abstract The power to direct and manage change within metropolitan areas is increasingly dispersed among a loosely interconnected set of mostly local organizations, agencies and actors that form a special type of urban inter-organizational network. Increasingly, the quality of metropolitan regional governance depends upon IO network capacity to articulate systemically insightful urban development strategies, i.e., to exercise a capacity for network steering. We outline an IO network steering capacity-support process that combines collaborative learning, narrative storytelling, and system dynamics modeling with the goal of deepening insights into urban human/biophysical processes and securing greater resilience in metropolitan regional governance. Our process promotes comprehension of complex urban processes through stories about past trajectories and future growth scenarios that frame issues within collaborative learning workshops for deliberation by local opinion leaders. This initiative is part of a larger research study on greenhouse gas emissions in relation to human and biological activities within metropolitan areas. Keywords: Collaborative learning, narratives, system dynamics, steering inter- organizational networks Introduction As our conception of government and its capacity for societal guidance changes, so too, does our approach to planning and decision-making. Increasingly, we recognize that the power to guide and direct change is dispersed among a variety of loosely interconnected organizations, agencies and actors. -
CURRICULUM VITAE Bradley J
CURRICULUM VITAE Bradley J. Thomson Assistant Professor Department of Earth & Planetary Sciences Phone: 865.974.2699 University of Tennessee Fax: 865.974.2368 1621 Cumberland Ave., Room 602 Email: [email protected] Knoxville, TN 37996-1410 Website: https://lunatic.utk.edu EDUCATION Ph.D. Geological Sciences, Brown University, 2006 Dissertation title: Recognizing impact glass on Mars using surface texture, mechanical properties, and mid-infrared spectroscopic properties Advisor: Peter H. SchultZ M.Sc. Geological Sciences, Brown University, 2001 Thesis title: Utopia Basin, Mars: Origin and evolution of basin internal structure Advisor: James W. Head III B.S. Harvey Mudd College, 1999, Geology major at Pomona College Thesis title: Thickness of basalts in Mare Imbrium Advisor: Eric B. Grosfils PROFESSIONAL EXPERIENCE Assistant Professor, Department of Earth and Planetary Sciences (EPS), University of Tennessee, Knoxville TN, 2020–present Research Associate Professor, Department of Earth and Planetary Sciences (EPS), University of Tennessee, Knoxville TN, 2016–2020 Senior Research Scientist, Boston University Center for Remote Sensing, 2011–2016 Co-Investigator, Mini-RF radar on the Lunar Reconnaissance Orbiter, 2009–present Co-Investigator, Mini-SAR radar on Chandrayaan-1, 2008–2009 Senior Staff Scientist, JHU Applied Physics Lab, 2008–2011 NASA Postdoctoral Program Fellow, Jet Propulsion Lab, 2006–2008 Science Theme Lead for mass wasting processes HiRISE camera on Mars Reconnaissance Orbiter, 2007–2010 Postdoctoral Fellow, Lunar and Planetary -
Origin and Evolution of the Peace Vallis Fan System That Drains Into the Curiosity Landing Area, Gale Crater
44th Lunar and Planetary Science Conference (2013) 1607.pdf ORIGIN AND EVOLUTION OF THE PEACE VALLIS FAN SYSTEM THAT DRAINS INTO THE CURIOSITY LANDING AREA, GALE CRATER. M. C. Palucis1, W. E. Dietrich1, A. Hayes1,2, R.M.E. Wil- liams3, F. Calef4, D.Y. Sumner5, S. Gupta6, C. Hardgrove7, and the MSL Science Team, 1Department of Earth and Planetary Science, University of California, Berkeley, CA, [email protected] and [email protected], 2Department of Astronomy, Cornell University, Ithaca, NY, [email protected], 3Planetary Science Institute, Tucson, AZ, [email protected], 4Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, [email protected], 5Department of Geology, University of California, Davis, Davis, CA, [email protected], 6Department of Earth Science, Imperial College, London, UK, [email protected], 7Malin Space Science Systems, San Diego, CA, [email protected] Introduction: Alluvial fans are depositional land- forms consisting of unconsolidated, water-transported sediment, whose fan shape is the result of sediment deposition downstream of an upland sediment point source. Three mechanisms have been identified, on Earth, for sediment deposition on a fan: avulsing river channels, sheet flows, and debris flows [e.g. 1-3]. Elu- cidating the dominant transport mechanism is im- portant for predicting water sources and volumes to the fan, estimating minimum timescales for fan formation, and understanding the regional climate at the time of fan building. This is especially relevant at Gale Crater (5.3oS 137.7oE), which contains a large alluvial fan, Peace Vallis fan, within the vicinity of the Bradbury Figure 1: HiRISE image of Peace Vallis Fan with smoothed 5-m landing site of the Mars Science Laboratory (MSL) contours. -
Workshop Schedule
Learn to Live Green. IT PAYS. Workshop Schedule TRADITIONAL YARD 9:00-9:20 Water Wise & Native Plants and Their Uses (New Horizons Nursery) Faye Rutishauser 9:30-9:50 Drip Irrigation Demonstration (The Gardening Coach) Kathlyn Collins 10:00-10:20 Fundamentals of Ecological Gardening (Mountain Bear Inc) Fred Montague 10:30-10:50 The Many Uses of Ornamental Grass (Growing Empire) Ruth McAngus 11:00-11:20 Benefits of Using a Geothermal System for Your Home (Comfort Tech) Becky Robbins 11:30-11:50 Fundamentals of Ecological Gardening (Mountain Bear Inc) Fred Montague 12:00-12:20 Drip Irrigation Demonstration (The Gardening Coach) Kathlyn Collins 12:30-12:50 Green Building is Better Building (G-Build) Brett Moyer 1:00-1:20 Socially Responsible Trading & Investing in the new economy (Locals Have More Fun) Brian Kahn 1:30-1:50 Water Wise & Native Plants and Their Uses (New Horizons Nursery) Faye Rutishauser 2:00-2:20 Brick paver installation techniques using recycled products (O’Brien Landscaping & Construction) Kevin O’Brien NORTH GATHERING AREA – JVWCD STAFF 9:00 Garden Tour 10:00 Garden Tour 11:00 Garden Tour 12:00 Garden Tour 1:00 Garden Tour NORTH GATHERING AREA 9:00 - 9:20 Water conservation for your system (Sprinkler World) Gig Bunnell 9:30 - 9:50 Water Management and Rebates (Innovative Management Solutions) Phil Fabry 10:00 -10:20 Sustainable Marketplace (Re-Direct Guide) Lara Gale 10:30 -10:50 Water Management and Rebates (Innovative Management Solutions) Phil Fabry 11:00 -11:20 Solar Electric Technology 101 (Wind Springs Energy) Mark Price 11:30 -11:50 Rebates For Attic Insulation Upgrade (Energy Savers Insulation) Jeff Dimond 12:00 -12:20 Enhancing Vegetation With Trace Mineral Supplementation (Int’l Institutue for Health & Wellness) Dr. -
A Noachian/Hesperian Hiatus and Erosive Reactivation of Martian Valley Networks
Lunar and Planetary Science XXXVI (2005) 2221.pdf A NOACHIAN/HESPERIAN HIATUS AND EROSIVE REACTIVATION OF MARTIAN VALLEY NETWORKS. R. P. Irwin III1,2, T. A. Maxwell1, A. D. Howard2, R. A. Craddock1, and J. M. Moore3, 1Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, MRC 315, 6th St. and Inde- pendence Ave. SW, Washington DC 20013-7012, [email protected], [email protected], [email protected]. 2Dept. of Environmental Sciences, P.O. Box 400123, University of Virginia, Charlottesville, VA 22904, [email protected]. 3NASA Ames Research Center, MS 245-3 Moffett Field, CA 94035-1000, [email protected]. Introduction: Despite new evidence for persistent rary in degraded craters of the southern equatorial lati- flow and sedimentation on early Mars [1−3], it remains tudes. All of these deposits likely formed during the unclear whether valley networks were active over long last stage of valley network activity, which appears to geologic timescales (105−108 yr), or if flows were per- have declined rapidly. sistent only during multiple discrete episodes [4] of Gale crater: Gale crater is an important strati- moderate (≈104 yr) to short (<10 yr) duration [5]. Un- graphic marker between discrete episodes of valley derstanding the long-term stability/variability of valley network activity. Gale retains most of the characteris- network hydrology would provide an important control tics of a fresh impact crater [15]: a rough ejecta blan- on paleoclimate and groundwater models. Here we ket, raised rim, hummocky interior walls, secondary describe geologic evidence for a hiatus in highland crater chains, and a (partially buried) central peak valley network activity while the fretted terrain (Figure 2). -
Comment on Liquid Water and Life on Mars
obiolog str y & f A O u o l t a r e n Chandra Wickramasinghe, Astrobiol Outreach 2015, 3:5 a r c u h o J Journal of Astrobiology & Outreach DOI: 10.4172/2332-2519.1000e111 ISSN: 2332-2519 Editorial Open Access Comment on Liquid Water and Life on Mars Chandra Wickramasinghe N*,1,2,3 1Buckingham Centre for Astrobiology (BCAB), Buckingham University, UK 2Institute for the Study of Panspermia and Astroeconomics, Gifu, Japan 3University of Peradeniya, Peradeniya, Sri Lanka *Corresponding author: Wickramasinghe NC, Buckingham Centre for Astrobiology (BCAB), Buckingham University, UK, Tel: +44-777-838-9243; E-mail: [email protected] Rec date: October 01, 2015; Acc date: October 05, 2015; Pub date: October 07, 2015 Copyright: © 2015 Chandra Wickramasinghe N, et al. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. Editorial but it was quickly rejected on grounds of alleged uncertainties of interpretation, as well as the lack of organic molecules detectable at the The announcement this week of the detection of liquid water on landing site. A year later, in1977, a major dust storm enveloped the Mars has come close on 4 decades after the arrival of the first Viking planet and H. Abadi and the present writer reported evidence of landers at the red planet in 1976 [1]. The temperatures at the two absorption properties of the Martian dust that was consistent with the original landing sites of the Viking spacecraft in 1976 ranged between a presence of aromatic hydrocarbons [3].