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ELECTORAL DISTRICTS Proposal for the Province of Ontario Published
ELECTORAL DISTRICTS Proposal for the Province of Ontario Published pursuant to the Electoral Boundaries Readjustment Act Table of Contents Preamble ......................................................................................................................................... 3 Process for Electoral Readjustment ................................................................................................ 3 Notice of Sittings for the Hearing of Representations .................................................................... 4 Requirements for Making Submissions During Commission Hearings ......................................... 5 Rules for Making Representations .................................................................................................. 6 Reasons for the Proposed Electoral Boundaries ............................................................................. 8 Schedule A – Electoral District Population Tables....................................................................... 31 Schedule B – Maps, Proposed Boundaries and Names of Electoral Districts .............................. 37 2 FEDERAL ELECTORAL BOUNDARIES COMMISSION FOR THE PROVINCE OF ONTARIO PROPOSAL Preamble The number of electoral districts represented in the House of Commons is derived from the formula and rules set out in sections 51 and 51A of the Constitution Act, 1867. This formula takes into account changes to provincial population, as reflected in population estimates in the year of the most recent decennial census. The increase -
Mixed Use High Density Development Site 81-85 Bridgeport Road E, Waterloo, Ontario
MIXED USE HIGH DENSITY DEVELOPMENT SITE 81-85 BRIDGEPORT ROAD E, WATERLOO, ONTARIO 81 85 BRIDGEPORT ROAD 4 executive summary property 6 overview location 8 overview offering 10 process 81-85 BRIDGEPORT ROAD EAST 3 THE OFFERING CBRE Limited is pleased to offer for sale 81-85 Bridgeport Road E, Waterloo, ON (the “Property” or the “Site”), a ±2.5 acre parcel currently improved with a 23,500 sq. ft furnature retail building and 4,000 sq.ft. automotive building. The Site has significant intensification potential and is situated in a tremendous location opposite a grocery-anchored retail centre, and within a desirable neighborhood flanking Uptown Waterloo. The Site further offers excellent transit accessibility and efficient access to the Conestoga Parkway (Highway #7/8 and Highway #85). The Toronto Waterloo Region is now internationally recognized as “The Corridor” (https://thecorridor.ca/) given the substantial local presence of advanced technology and manufacturing firms and proximity to the GTA. Kitchener-Waterloo has matured to incorporate more than 1,000 technology firms, 150 research centres and more than 100,000 post-secondary students. The property is an ideal location for mixed-use high density intensification due to its proximity to the Bridgeport Plaza consisting of Walmart, Sobeys, Tim Hortons, Bulk Barn and Petro Canada. The property is also a short walk away from Uptown Waterloo where significant tech employment growth is occurring (Shopify, SSIMWAVE, Kiite, etc.) As well as boasting restaurants and premium boutique shopping in the area (Beertown, Abe Erb, Channer’s & SASS) 81-85 LRT Station 4 MIXED USE DEVELOPMENT SITE BRIDGEPORT ROAD E PROPERTY DETAILS ADDRESS 81-85 Bridgeport Road E Site Size ±2.50 acres Buillding Size ±23,500 sq. -
Mars Mapping, Data Mining, Change Detection, GIS Mapping, Time Series Analysis
ISPRS Technical Commission IV Symposium on Geospatial Databases and Location Based Services, 14 – 16 May 2014, Suzhou, China, MTSTC4-2014-172-2 TEMPORAL ANALYSIS OF ALL AVAILABLE HIGH-RESOLUTION MARS IMAGING PRODUCTS SINCE 1976 Panagiotis Sidiropoulos1 and Jan-Peter Muller Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey, RH56NT, UK [email protected], [email protected] Commission KEY WORDS: Mars mapping, data mining, change detection, GIS mapping, time series analysis ABSTRACT: Starting from Viking Orbiter 1, launched in August 1975, several mainly NASA orbiters have been sent to Mars to accomplish the robotic tasks of imaging its surface. Initial analyses of these early images indicated a planet with similar characteristics to the Moon pitted with craters and large volcanic and tectonic features but dead from a geological perspective. Recently, scientific interest has shifted towards high-resolution imaging, which allows the identification of previously undiscovered geological phenomena and surface features as well as the examination of surface composition and geological history. The increasing frequency of Mars orbiters, carrying high-resolution cameras, allows the dynamic analysis of Martian surface, i.e. the analysis of the temporal evolution of certain areas that reveal natural processes that happen over time. The latter can be roughly classified into two major categories; processes that happen periodically each and every Martian season (e.g. seasonal flows in high latitude areas (McEwen et al., 2011) and events that do not follow some iterative pattern but are rather sporadic (e.g. new impact craters (Byrne et al., 2009)). Consequently, it is beneficial to conduct a twin temporal grouping of Mars imaging products, the first examining product distribution through time, so as to point out areas that favor the search for sporadic events, and the second product distribution per season, to identify areas favouring the search for periodic events. -
Community Profile 2019
“Proudly remembering our past; Confidently embracing our future.” Community Profile & Development Information 2019 Township of Woolwich Region of Waterloo Ontario, Canada Located in the heart of South Western Ontario, the Township of Woolwich surrounds the Cities of Waterloo, Kitchener and Cambridge, and is within minutes of the City of Guelph. Woolwich is not only known for its farms and farm markets, but also its industry, trails and providing a rural lifestyle with all the conveniences of the city. The Township contains an area of approximately 31,912 hectares (78,854 acres), with a population of approximately 25,000 people. Woolwich is comprised of an extensive rural area along with residential communities and industrial/commercial areas which 0 62.5 125 250 Miles include Elmira, St. Jacobs, and 0 100 200 400 / Kilometers National Geographic, Esri, DeLorme, NAVTEQ, UNEP-WCMC, USGS, Breslau. NASA, ESA, METI, NRCAN, GEBCO, NOAA, iPC Elmira 1:7,909,724 Township of Woolwich St. Jacobs Breslau Cambridge 0 4 8 Sources: Esri, DeLorme, NAVTEQ, USGS, Intermap, iPC, NRCAN, Esri Japan, METI, Esri China (Hong Kong), Esri . Kilometers (Thailand), TomTom, 2013 OUR VISION A vision reflects the aspirations of the organization and its activities providing a panoramic view of “where we are going”. It points an organization in a particular direction and charts a strategic path for everyone to follow. “Woolwich will be known as a Community of Choice in the Province of Ontario because of its: • Sustainable Growth Practices; • Forward-Looking Investment in Infrastructure Maintenance & Transportation Planning; • Effective Communication Strategies; • Responsible Fiscal Planning; • Safe, Active, and Environmentally Friendly Communities; and • Solid Governance, Progressive Administration, and Community Engagement Practices” OUR MISSION While a vision paints a picture of a final destination, the destination pre-supposes a starting point. -
Ancient Fluid Escape and Related Features in Equatorial Arabia Terra (Mars)
EPSC Abstracts Vol. 7 EPSC2012-132-3 2012 European Planetary Science Congress 2012 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2012 Ancient fluid escape and related features in equatorial Arabia Terra (Mars) F. Franchi(1), A. P. Rossi(2), M. Pondrelli(3), B. Cavalazzi(1), R. Barbieri(1), Dipartimento di Scienze della Terra e Geologico Ambientali, Università di Bologna, via Zamboni 67, 40129 Bologna, Italy ([email protected]). 2Jacobs University, Bremen, Germany. 3IRSPS, Università D’Annunzio, Pescara, Italy. Abstract Noachian [1]. The ELDs are composed by light rocks showing a polygonal pattern, described elsewhere on Arabia Terra, in the equatorial region of Mars, is Mars [4], and is characterized by a high sinuosity of long-time studied area especially for the abundance the strata that locally follows a concentric trend of fluid related features. Detailed stratigraphic and informally called “pool and rim” structures (Fig. morphological study of the succession exposed in the 1A). Crommelin and Firsoff craters evidenced the occurrences of flow structures and spring deposits that endorse the presence of fluids circulation in the Late Noachian. All the morphologies in these two proto-basins occur within the Equatorial Layered Deposits (ELDs). 1. Introduction Martian layered spring deposits are of considerable interest for their supposed relationship with water and high potential of microbial signatures preservation. Their supposed fluid-related origin [1] makes the Equatorial Layered Deposits attractive targets for future missions with astrobiological purposes. In this study we report the occurrence of mounds fields and flow structures in Firsoff and Crommelin craters and summarize the result of a detailed study of the remote-sensing data sets available in this region. -
1 Fluids Mobilization in Arabia Terra, Mars
Fluids mobilization in Arabia Terra, Mars: depth of pressurized reservoir from mounds self- similar clustering Riccardo Pozzobon1, Francesco Mazzarini2, Matteo Massironi1, Angelo Pio Rossi3, Monica Pondrelli4, Gabriele Cremonese5, Lucia Marinangeli6 1 Department of Geosciences, Università degli Studi di Padova, Via Gradenigo 6 - 35131, Padova, Italy 2 Istituto Nazionale di Geofisica e Vulcanologia (INGV), Via Della Faggiola, 32 - 56100 Pisa, Italy 3 Department of Physics and Earth Sciences, Jacobs University Bremen, Campus Ring 1 -28759 Bremen, Germany 4 International Research School of Planetary Sciences, Università d'Annunzio, viale Pindaro 42 – 65127, Pescara, Italy 5 INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5 - 35122, Padova, Italy 6 Laboratorio di Telerilevamento e Planetologia, DISPUTer, Universita' G. d'Annunzio, Via Vestini 31 - 66013 Chieti, Italy Abstract Arabia Terra is a region of Mars where signs of past-water occurrence are recorded in several landforms. Broad and local scale geomorphological, compositional and hydrological analyses point towards pervasive fluid circulation through time. In this work we focus on mound fields located in the interior of three casters larger than 40 km (Firsoff, Kotido and unnamed crater 20 km to the east) and showing strong morphological and textural resemblance to terrestrial mud volcanoes and spring-related features. We infer that these landforms likely testify the presence of a pressurized fluid reservoir at depth and past fluid upwelling. We have performed morphometric analyses to characterize the mound morphologies and consequently retrieve an accurate automated mapping of the mounds within the craters for spatial distribution and fractal clustering analysis. The outcome of the fractal clustering yields information about the possible extent of the percolating fracture network at depth below the craters. -
Near Earth Asteroid Rendezvous: Mission Summary 351
Cheng: Near Earth Asteroid Rendezvous: Mission Summary 351 Near Earth Asteroid Rendezvous: Mission Summary Andrew F. Cheng The Johns Hopkins Applied Physics Laboratory On February 14, 2000, the Near Earth Asteroid Rendezvous spacecraft (NEAR Shoemaker) began the first orbital study of an asteroid, the near-Earth object 433 Eros. Almost a year later, on February 12, 2001, NEAR Shoemaker completed its mission by landing on the asteroid and acquiring data from its surface. NEAR Shoemaker’s intensive study has found an average density of 2.67 ± 0.03, almost uniform within the asteroid. Based upon solar fluorescence X-ray spectra obtained from orbit, the abundance of major rock-forming elements at Eros may be consistent with that of ordinary chondrite meteorites except for a depletion in S. Such a composition would be consistent with spatially resolved, visible and near-infrared (NIR) spectra of the surface. Gamma-ray spectra from the surface show Fe to be depleted from chondritic values, but not K. Eros is not a highly differentiated body, but some degree of partial melting or differentiation cannot be ruled out. No evidence has been found for compositional heterogeneity or an intrinsic magnetic field. The surface is covered by a regolith estimated at tens of meters thick, formed by successive impacts. Some areas have lesser surface age and were apparently more recently dis- turbed or covered by regolith. A small center of mass offset from the center of figure suggests regionally nonuniform regolith thickness or internal density variation. Blocks have a nonuniform distribution consistent with emplacement of ejecta from the youngest large crater. -
41 Ardelt Place for Lease
41 ARDELT PLACE Kitchener, Ontario SITE FOR LEASE For more information, please contact: HIGH EXPOSURE OFFICE SPACE :: Chris Kotseff* :: Mitchell Blaine* :: Joe Benninger* CCIM Sales Representative Senior Sales Associate Senior Sales Associate 519.340.2321 519.340.2309 519.340.2323 ±14,464 Square Feet Available at 41 Ardelt Place in Kitchener, Ontario. Fully Finished with Upgraded Interior. Beautiful Finishes [email protected] [email protected] [email protected] Throughout. Substantial Natural Lighting Through Windows and Skylights. Ample On-Site Surface Parking. Close Proximity to the Fairway Road Retail Corridor. Accessible to the Highway #7/8 and Highway #401 via Courtland Avenue East and Homer Watson Boulevard. www.cbre.ca/chris.kotseff Kitchener, Ontario is Located in the Heart of Canada’s Most Populous Province. With a Current Population of Over 500,000, the Waterloo Region is now the 10th Largest Urban Area in Canada and the 4th Largest in Ontario. There Are 2.7 Million People Living Within a 45 Minute Drive and 5.1 Million People Living With a One Hour Drive. This disclaimer shall apply to CB Richard Ellis Limited, Brokerage, and to all other divisions of the Corporation (“CBRE”). The information set out herein (the “Information”) has not been verified by CBRE, and CBRE does not represent, warrant or guarantee the accuracy, correctness and completeness of the Information. CBRE does not accept or assume any responsibility or liability, direct or consequential, for the Information or the recipient’s reliance upon the Information. The recipient of the Information should take such steps as the recipient may deem necessary to verify the Information prior to placing any reliance upon the Information. -
ONTARIO ROAD SAFETY: Annual Report 2016
ONTARIO ROAD SAFETY Annual Report 2016 Printed on paper with recycled content. ISSN #0832-8269 (Printed Version) ISSN #1710-2480 (Internet Version) ONTARIO ROAD SAFETY ANNUAL REPORT 2016 This document is available online at: www.ontario.ca/orsar If you are seeking information on how to reduce your risk of being in a collision, visit your local DriveTest Centre, or visit the Ministry of Transportation website at ontario.ca/transportation. For all other road safety public education materials please go to the ServiceOntario Publications website at www.serviceontario.ca/publications, or call 416-326-5300 or 1-800-668-9938. The Ministry of Transportation’s Official Driver’s Handbook is available online at www.mto.gov.on.ca/english/publications/handbooks.shtml. You can also purchase 1 hardcopies at DriveTest Centres, and at various department stores, automotive retail outlets and book stores. For more information on the data in this publication, please contact the Road Safety Research Office at 416-235-3585. Produced by: Road Safety Research Office Safety Policy & Education Branch Ministry of Transportation 87 Sir William Hearst Avenue Room 212 Toronto, Ontario M3M 0B4 Phone: 416-235-3585 Fax: 416-235-5129 Ontario Road Safety Annual Report 2016 CONTENTS Section/Title Page Foreword 6 1. Overview 20 1a Synopsis 22 1b Health Perspective 23 2. The People 24 2a People in Collisions 26 2b Putting The People In Context 37 3. The Collision 44 3a Types of Collisions 46 3b Time and Environment 49 2 3c The Collision Location 52 4. Place of Collision 54 Contents 5. The Vehicle 72 5a Vehicles in Collisions 74 5b Putting the Vehicle in Context 76 6. -
2016 Annual Report
2016 The Federal Gas Tax Fund Annual Report – Part II Table of Contents Compliance and Financial Audit Statements, Federal Gas Tax Fund ............. A 1-9 Audit Based Attestation .................................................................................................... B 1 Municipal Compliance Audit Reports ........................................................................... C 1-44 2016 to 2018 Federal Gas Tax Fund Allocations ....................................................... D 1-11 2016 Federal Gas Tax Fund Projects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
R. M. E. Williams, 2017, Shaler: a Fluvial Sedimentary Deposit on Mars, Sedimentology
Rebecca M. (Eby) Williams Planetary Science Institute (p) 608-729-7786 (e) [email protected] Education: PhD., 2000, Planetary Sciences, Washington University, St. Louis, MO B.A., 1995, Cum Laude, Physics and Geology, Franklin & Marshall College, Lancaster, PA Relevant Work History: Planetary Science Institute, Tucson, AZ 2011-Present Senior Scientist 2005-2010 Research Scientist Smithsonian Institution, Center for Earth and Planetary Science, Washington, DC 2004-2006 Research Associate, Lindbergh Fellow Malin Space Science Systems, Inc., San Diego, CA 2002-2004 Staff Scientist 2001-2002 Post-Doctoral Research Associate Awards & Service: 2006 NASA Carl Sagan Fellowship for Early Career Researchers 2011 MRO CTX Science Team NASA Group Achievement Award 2013 MSL Science Office Development and Operations Team, NASA Group Achievement Award 2013-Present ESA ExoMars Landing Site Selection Working Group (LSSWG) Member 2015 NASA Next Orbiter to Mars Science Advisory Group (NEX-SAG) Member 2015 MSL Prime Mission Science and Operations Team, NASA Group Achievement Award 2017 Friend of Education, Waunakee Teachers Association Field Experience: Deltas in Patagonia, Chile, PI, November 2018. Inverted paleochannels & alluvial fans, Pampa del Tamarugal region, Atacama Desert, Chile, PI, Nov 2010, June 2012, May 2016, Nov. 2017. Inverted paleochannels, Ebro Basin, Spain, Co-I, Feb. 2017 (PI Michael Lamb). Rover operations testing, Co-I, near Vernal, UT, Oct. 2017; Green River, UT, April 2016 (GeoHeuristic Operational Strategies Testing, GHOST, PI Aileen Yingst). Inverted paleochannels near Baker, CA, PI, Sep 2014, April 2016. Inverted paleochannels near Cadney, South Australia, PI, May 2011. Meandering channels of the Quinn River, Nevada, Co-I, July 2010, Oct. 2011. Inverted paleochannels, Cape York Peninsula, Queensland, Australia, PI, July 2009. -
Scent Theory Store List
Store Address City State Zip Phone 1158 2473 HACKWORTH RD ADAMSVILLE AL 35214 2057989721 423 630 COLONIAL PROMENADE PKWY ALABASTER AL 35007 2056200360 4756 9085 HWY 119 ALABASTER AL 35007 2056246229 726 2643 HIGHWAY 280 ALEXANDER CITY AL 35010 2562340316 1091 1991 DR M L K JR EXPY ANDALUSIA AL 36420 3342226561 329 5560 MCCLELLAN BLVD ANNISTON AL 36206 2568203326 306 1450 N BRINDLEE MOUN ARAB AL 35016 2565868168 661 1011 US HIGHWAY 72 E ATHENS AL 35611 2562302981 7247 911 N MAIN STREET ATMORE AL 36502 2513681403 316 973 GILBERT FERRY RD SE ATTALLA AL 35954 2565383811 356 1717 S COLLEGE ST AUBURN AL 36832 3348212493 4673 1810 SHUG JORDAN PARKWAY AUBURN AL 36832 3345396318 5062 2047 E UNIVERSITY DR AUBURN AL 36830 3345396214 2739 701 MCMEANS AVE BAY MINETTE AL 36507 2519375558 764 750 ACADEMY DR BESSEMER AL 35022 2054245890 762 9248 PARKWAY E BIRMINGHAM AL 35206 2058337676 1711 1600 MONTCLAIR RD BIRMINGHAM AL 35210 2059560416 2111 5335 HIGHWAY 280 BIRMINGHAM AL 35242 2059805156 3424 2653 VALLEYDALE ROAD BIRMINGHAM AL 35244 2055826183 4504 312 PALISADES BLVD BIRMINGHAM AL 35209 2058708101 5100 1916 CENTER POINT PKWY BIRMINGHAM AL 35215 2055200269 298 1972 HIGHWAY 431 BOAZ AL 35957 2565930195 425 PO BOX 270 BRENT AL 35034 2059264878 1620 2578 DOUGLAS AVE BREWTON AL 36426 2518674680 3271 5100 HIGHWAY 31 CALERA AL 35040 2056680831 5126 1950 W MAIN ST CENTRE AL 35960 2569279900 4330 16077 HIGHWAY 280 CHELSEA AL 35043 2056782222 424 1415 7TH ST S CLANTON AL 35045 2057557574 670 626 OLIVE ST SW CULLMAN AL 35055 2567391664 7280 5601 HIGHWAY 157 CULLMAN