National Camping School’S Annual Theme Program Experiments
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Saving the Information Commons a New Public Intere S T Agenda in Digital Media
Saving the Information Commons A New Public Intere s t Agenda in Digital Media By David Bollier and Tim Watts NEW AMERICA FOUNDA T I O N PUBLIC KNOWLEDGE Saving the Information Commons A Public Intere s t Agenda in Digital Media By David Bollier and Tim Watts Washington, DC Ack n owl e d g m e n t s This report required the support and collaboration of many people. It is our pleasure to acknowledge their generous advice, encouragement, financial support and friendship. Recognizing the value of the “information commons” as a new paradigm in public policy, the Ford Foundation generously supported New America Foundation’s Public Assets Program, which was the incubator for this report. We are grateful to Gigi Sohn for helping us develop this new line of analysis and advocacy. We also wish to thank The Open Society Institute for its important support of this work at the New America Foundation, and the Center for the Public Domain for its valuable role in helping Public Knowledge in this area. Within the New America Foundation, Michael Calabrese was an attentive, helpful colleague, pointing us to useful literature and knowledgeable experts. A special thanks to him for improv- ing the rigor of this report. We are also grateful to Steve Clemons and Ted Halstead of the New America Foundation for their role in launching the Information Commons Project. Our research and writing of this report owes a great deal to a network of friends and allies in diverse realms. For their expert advice, we would like to thank Yochai Benkler, Jeff Chester, Rob Courtney, Henry Geller, Lawrence Grossman, Reed Hundt, Benn Kobb, David Lange, Jessica Litman, Eben Moglen, John Morris, Laurie Racine and Carrie Russell. -
Acton Liquor Store
1966 Experience The Colonial Difference02 Holiday Spirits from Around the World! 02 Special Savings on Our original location Beer and Wine! 04 Add Some Sparkle: in 1966 Champagne Deals! 07 How Much of What? Party Planning from Colonial Spirits the Experts 08 Come celebrate our 46th season Wine Matches for Every Family Favorite! 010 Serve Wine Like a Sommelier! 015 Beer and Food, Done Right! 016 Moonshine North of the Mason-Dixon! 019 Finding Your Way in Whisk[e]y! 022 The New (Old) Wine Fashions! 024 4th Annual Big Red Tasting 026 Touching the Roots of Wine: Blends! 028 2012 87 Great Road, Acton, MA 01720 978.263.7775 Order Online at: www.ColonialSpiritsDelivers.com Colonial Spirits began its service as a but its popularity and the choices available to enthusiasts developed wine shop to the Acton, Concord, Carlisle and surrounding communi- quickly. Colonial Spirits went through several expansions over the ties over 40 years ago. Along a lightly developed and traveled route years to keep up with the ever growing demand for selection and the 2A in East Acton, Colonial Spirits began in the 19th century building diverse and changing tastes of people in the community. Wine proved next to the street. In its early days Colonial Spirits’ selection would to be a major source of enjoyment for people as new wineries from all seem quite limited in comparison to what can be found in the shop over the world continued to become available in Colonial Spirits. What today. Wine was just beginning to become a major consumer product, is most prominent in our recent history is the time spent at 69 Great Rd and the major expansion into 87 Great Rd in 2003. -
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography on the Occasion of the 50Th Anniversary of Apollo 11 Moon Landing
Special Catalogue Milestones of Lunar Mapping and Photography Four Centuries of Selenography On the occasion of the 50th anniversary of Apollo 11 moon landing Please note: A specific item in this catalogue may be sold or is on hold if the provided link to our online inventory (by clicking on the blue-highlighted author name) doesn't work! Milestones of Science Books phone +49 (0) 177 – 2 41 0006 www.milestone-books.de [email protected] Member of ILAB and VDA Catalogue 07-2019 Copyright © 2019 Milestones of Science Books. All rights reserved Page 2 of 71 Authors in Chronological Order Author Year No. Author Year No. BIRT, William 1869 7 SCHEINER, Christoph 1614 72 PROCTOR, Richard 1873 66 WILKINS, John 1640 87 NASMYTH, James 1874 58, 59, 60, 61 SCHYRLEUS DE RHEITA, Anton 1645 77 NEISON, Edmund 1876 62, 63 HEVELIUS, Johannes 1647 29 LOHRMANN, Wilhelm 1878 42, 43, 44 RICCIOLI, Giambattista 1651 67 SCHMIDT, Johann 1878 75 GALILEI, Galileo 1653 22 WEINEK, Ladislaus 1885 84 KIRCHER, Athanasius 1660 31 PRINZ, Wilhelm 1894 65 CHERUBIN D'ORLEANS, Capuchin 1671 8 ELGER, Thomas Gwyn 1895 15 EIMMART, Georg Christoph 1696 14 FAUTH, Philipp 1895 17 KEILL, John 1718 30 KRIEGER, Johann 1898 33 BIANCHINI, Francesco 1728 6 LOEWY, Maurice 1899 39, 40 DOPPELMAYR, Johann Gabriel 1730 11 FRANZ, Julius Heinrich 1901 21 MAUPERTUIS, Pierre Louis 1741 50 PICKERING, William 1904 64 WOLFF, Christian von 1747 88 FAUTH, Philipp 1907 18 CLAIRAUT, Alexis-Claude 1765 9 GOODACRE, Walter 1910 23 MAYER, Johann Tobias 1770 51 KRIEGER, Johann 1912 34 SAVOY, Gaspare 1770 71 LE MORVAN, Charles 1914 37 EULER, Leonhard 1772 16 WEGENER, Alfred 1921 83 MAYER, Johann Tobias 1775 52 GOODACRE, Walter 1931 24 SCHRÖTER, Johann Hieronymus 1791 76 FAUTH, Philipp 1932 19 GRUITHUISEN, Franz von Paula 1825 25 WILKINS, Hugh Percy 1937 86 LOHRMANN, Wilhelm Gotthelf 1824 41 USSR ACADEMY 1959 1 BEER, Wilhelm 1834 4 ARTHUR, David 1960 3 BEER, Wilhelm 1837 5 HACKMAN, Robert 1960 27 MÄDLER, Johann Heinrich 1837 49 KUIPER Gerard P. -
The BG News April 15, 1999
Bowling Green State University ScholarWorks@BGSU BG News (Student Newspaper) University Publications 4-15-1999 The BG News April 15, 1999 Bowling Green State University Follow this and additional works at: https://scholarworks.bgsu.edu/bg-news Recommended Citation Bowling Green State University, "The BG News April 15, 1999" (1999). BG News (Student Newspaper). 6484. https://scholarworks.bgsu.edu/bg-news/6484 This work is licensed under a Creative Commons Attribution-Noncommercial-No Derivative Works 4.0 License. This Article is brought to you for free and open access by the University Publications at ScholarWorks@BGSU. It has been accepted for inclusion in BG News (Student Newspaper) by an authorized administrator of ScholarWorks@BGSU. ■" * he BG News Women rally to 'take back the night' sexual assault. istration vivors, they will be able to relate her family. By WENDY SUTO Celesta Haras/ti, a resident of buildings, rain to parts of her story, Kissinger "The more I tell my story, the The BG News BG and a W4W member, said the or shine. The said. less shame and guilt I feel," Kissinger said. "For my situa- Women (and some men) will rally is about issues that are con- keynote "When I decided to disclose tion, I'm glad I didn't tell my take to the streets tonight, pro- sidered taboo by society, such as speaker, my sexual abuse to my family, I parents right away because I claiming a public statement in an rape and incest. She has attended Kendel came out of the closet complete- think it would have been a worse attempt to "Take Back the Night" several TBTN marches at the Kissinger, a ly," Kissinger said. -
How Does the Diver Work? Preparing the Plastic Soda Bottle
How Does the Diver Work? Preparing the Plastic Soda Bottle Vv'hen you build a Cartesian diver, you are exploring three scientific properties of air: You will need to start collecting plastic soda bottles with caps. While (1) Air has weight almost any size bottle will work, the most popular sizes are 1 liter, 1.5 liter, and 2 liter bottles. Smaller children will find that the 1 and 1.5 liter (2) Air occupies space bottles are easiest to squeeze. The best soda bottles are those that are (3) Air exerts pressure. clear from top to bottom so that you can see everything that is happening in the bottle. Generally speaking, an object will float in a fluid if its density is less than that of the fluid (densltyemass/volume). If the object is more dense than the fluid, then the object will sink. For example, an empty bottle will float in a bathtub that is filled with water if the bottle is less dense than the water. However, as you start filling the bottle with water, its Here's an easy method for density increases and its buoyancy decreases. Eventually, the bottle will sink if it is filled too full with water. ~ cleaning the plastic The Cartesian diver, consisting of a plastic medicine dropper and soda bottles: a metal hex nut, will float or sink in the bottle of water depending on the water level in the bulb of the dropper. Vv'hen pressure is applied to the outside of the bottle, water is pushed up inside the diver, and the air • Rinse out the bottle using warm water. -
A Ballistics Analysis of the Deep Impact Ejecta Plume: Determining Comet Tempel 1’S Gravity, Mass, and Density
Icarus 190 (2007) 357–390 www.elsevier.com/locate/icarus A ballistics analysis of the Deep Impact ejecta plume: Determining Comet Tempel 1’s gravity, mass, and density James E. Richardson a,∗,H.JayMeloshb, Carey M. Lisse c, Brian Carcich d a Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721-0092, USA c Planetary Exploration Group, Space Department, Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA d Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA Received 31 March 2006; revised 8 August 2007 Available online 15 August 2007 Abstract − In July of 2005, the Deep Impact mission collided a 366 kg impactor with the nucleus of Comet 9P/Tempel 1, at a closing speed of 10.2 km s 1. In this work, we develop a first-order, three-dimensional, forward model of the ejecta plume behavior resulting from this cratering event, and then adjust the model parameters to match the flyby-spacecraft observations of the actual ejecta plume, image by image. This modeling exercise indicates Deep Impact to have been a reasonably “well-behaved” oblique impact, in which the impactor–spacecraft apparently struck a small, westward-facing slope of roughly 1/3–1/2 the size of the final crater produced (determined from initial ejecta plume geometry), and possessing an effective strength of not more than Y¯ = 1–10 kPa. The resulting ejecta plume followed well-established scaling relationships for cratering in a medium-to-high porosity target, consistent with a transient crater of not more than 85–140 m diameter, formed in not more than 250–550 s, for the case of Y¯ = 0 Pa (gravity-dominated cratering); and not less than 22–26 m diameter, formed in not less than 1–3 s, for the case of Y¯ = 10 kPa (strength-dominated cratering). -
[Japan] SALA GIOCHI ARCADE 1000 Miglia
SCHEDA NEW PLATINUM PI4 EDITION La seguente lista elenca la maggior parte dei titoli emulati dalla scheda NEW PLATINUM Pi4 (20.000). - I giochi per computer (Amiga, Commodore, Pc, etc) richiedono una tastiera per computer e talvolta un mouse USB da collegare alla console (in quanto tali sistemi funzionavano con mouse e tastiera). - I giochi che richiedono spinner (es. Arkanoid), volanti (giochi di corse), pistole (es. Duck Hunt) potrebbero non essere controllabili con joystick, ma richiedono periferiche ad hoc, al momento non configurabili. - I giochi che richiedono controller analogici (Playstation, Nintendo 64, etc etc) potrebbero non essere controllabili con plance a levetta singola, ma richiedono, appunto, un joypad con analogici (venduto separatamente). - Questo elenco è relativo alla scheda NEW PLATINUM EDITION basata su Raspberry Pi4. - Gli emulatori di sistemi 3D (Playstation, Nintendo64, Dreamcast) e PC (Amiga, Commodore) sono presenti SOLO nella NEW PLATINUM Pi4 e non sulle versioni Pi3 Plus e Gold. - Gli emulatori Atomiswave, Sega Naomi (Virtua Tennis, Virtua Striker, etc.) sono presenti SOLO nelle schede Pi4. - La versione PLUS Pi3B+ emula solo 550 titoli ARCADE, generati casualmente al momento dell'acquisto e non modificabile. Ultimo aggiornamento 2 Settembre 2020 NOME GIOCO EMULATORE 005 SALA GIOCHI ARCADE 1 On 1 Government [Japan] SALA GIOCHI ARCADE 1000 Miglia: Great 1000 Miles Rally SALA GIOCHI ARCADE 10-Yard Fight SALA GIOCHI ARCADE 18 Holes Pro Golf SALA GIOCHI ARCADE 1941: Counter Attack SALA GIOCHI ARCADE 1942 SALA GIOCHI ARCADE 1943 Kai: Midway Kaisen SALA GIOCHI ARCADE 1943: The Battle of Midway [Europe] SALA GIOCHI ARCADE 1944 : The Loop Master [USA] SALA GIOCHI ARCADE 1945k III SALA GIOCHI ARCADE 19XX : The War Against Destiny [USA] SALA GIOCHI ARCADE 2 On 2 Open Ice Challenge SALA GIOCHI ARCADE 4-D Warriors SALA GIOCHI ARCADE 64th. -
Aeroastro-2011-12.Pdf
ANNUAL 2011-12 • MASSACHUSETTS INSTITUTE OF TECHNOLOGY Editors Department Head Associate Head Editor & Director of Communications Jaime Peraire Karen Willcox William T.G. Litant [email protected] [email protected] [email protected] AeroAstro is published annually by the Massachusetts Institute of Technology Department of Aeronautics and Astronautics, 33-240, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA. http://www.mit.aero AeroAstro No. 9, July 2012 ©2012 The Massachusetts Institute of Technology. All rights reserved. Except where noted, photographs by William Litant/MIT DESIGN Opus Design www.opusdesign.us Cover: Alumni astronauts (from left) Mike Fincke (AeroAstro, BSc ’89), Cady Coleman (ChemE, BSc ’83), and Greg Chamitoff (AeroAstro, PhD ’82), wearing MIT 150 anniversary t-shirts, send video greetings from the International Space Station to high school students around the world participating in AeroAstro’s 2011 Zero Robotics competition. Each is accom- panied by a Space System’s Lab SPHERE microsatellite. For more on Zero Robotics and SPHERES, turn to page 25 (Video grab via NASA). Cert no. XXX-XXX-000 THESE ARE EXCITING TIMES FOR AEROASTRO. Our research funding has risen by 40 percent over the past three years: there are more than 170 research projects in our labs and centers repre- senting $28 million in expenditures by the Department of Defense, NASA, other federal agencies and departments, and the aerospace industry. Our incoming sophomore class size is up by 48 percent over last year. Our faculty now includes a former secretary to the Air Force, a former astronaut, a former NASA associate administrator, a former USAF chief scientist, nine National Academy of Engineering members, nine Amer- ican Institute of Aeronautics and Astronautics Fellows, two Guggenheim Indeed, we have a number of great projects and initiatives ramping Medal recipients, and two AIAA Reed Aeronautics Award recipients. -
Science Concept 5: Lunar Volcanism Provides a Window Into the Thermal and Compositional Evolution of the Moon
Science Concept 5: Lunar Volcanism Provides a Window into the Thermal and Compositional Evolution of the Moon Science Concept 5: Lunar volcanism provides a window into the thermal and compositional evolution of the Moon Science Goals: a. Determine the origin and variability of lunar basalts. b. Determine the age of the youngest and oldest mare basalts. c. Determine the compositional range and extent of lunar pyroclastic deposits. d. Determine the flux of lunar volcanism and its evolution through space and time. INTRODUCTION Features of Lunar Volcanism The most prominent volcanic features on the lunar surface are the low albedo mare regions, which cover approximately 17% of the lunar surface (Fig. 5.1). Mare regions are generally considered to be made up of flood basalts, which are the product of highly voluminous basaltic volcanism. On the Moon, such flood basalts typically fill topographically-low impact basins up to 2000 m below the global mean elevation (Wilhelms, 1987). The mare regions are asymmetrically distributed on the lunar surface and cover about 33% of the nearside and only ~3% of the far-side (Wilhelms, 1987). Other volcanic surface features include pyroclastic deposits, domes, and rilles. These features occur on a much smaller scale than the mare flood basalts, but are no less important in understanding lunar volcanism and the internal evolution of the Moon. Table 5.1 outlines different types of volcanic features and their interpreted formational processes. TABLE 5.1 Lunar Volcanic Features Volcanic Feature Interpreted Process -
EARTH SCIENCE ACTIVITY #1 Tsunami in a Bottle
EARTH SCIENCE ACTIVITY #1 Grades 3 and Up Tsunami in a Bottle This activity is one of several in a basic curriculum designed to increase student knowledge about earthquake science and preparedness. The activities can be done at any time in the weeks leading up to the ShakeOut drill. Each activity can be used in classrooms, museums, and other educational settings. They are not sequence-bound, but when used together they provide an overview of earthquake information for children and students of various ages. All activities can be found at www.shakeout.org/schools/resources/. Please review the content background (page 3) to gain a full understanding of the material conducted in this activity. OBJECTIVE: For students to learn that tsunamis can be caused by earthquakes and to understand the effects of tsunamis on the shoreline MATERIALS/RESOURCES NEEDED: 2-liter plastic soda bottles Small gravel (fish tank gravel) Water source Empty water bottle (16 oz) Overhead projector Transparency of Tsunami Facts “What Do I See?” handout PRIOR KNOWLEDGE: In order to conduct this activity, students need to know how fault slippage can generate earthquakes. ACTIVITY: Set-Up (Time varies) Collect as many 2-liter soda bottles as possible or ask students to bring in bottles for this activity (3 students can share one bottle). Obtain an empty water bottle (about 16 oz). Remove labels from all bottles. Purchase or gather enough small gravel to fit through the mouth of the soda bottles. Students will fill up their soda bottles with gravel to create at least a 2 inch layer on the bottom of the bottle. -
USGS Professional Paper 1692
USG S Eruptive History and Chemical Evolution of the Precaldera and Postcaldera Basalt-Dacite Sequences, Long Valley, California: Implications for Magma Sources, Current Seismic Unrest, and Future Volcanism Professional Paper 1692 U.S. Department of the Interior U.S. Geological Survey This page intentionally left blank Eruptive History and Chemical Evolution of the Precaldera and Postcaldera Basalt-Dacite Sequences, Long Valley, California: Implications for Magma Sources, Current Seismic Unrest, and Future Volcanism By Roy A. Bailey Professional Paper 1692 U.S. Department of the Interior U.S. Geological Survey ii U.S. Department of the Interior Gale A. Norton, Secretary U.S. Geological Survey Charles G. Groat, Director U.S. Geological Survey, Reston, Virginia: 2004 For sale by U.S. Geological Survey Information Services Box 25286, Denver Federal Center Denver, CO 80225 This report and any updates to it are available online at: http://pubs.usgs.gov//pp/p1692/ Additional USGS publications can be found at: http://geology.usgs.gov/products.html For more information about the USGS and its products: Telephone: 1–888–ASK–USGS (1–888–275–8747) World Wide Web: http://www.usgs.gov/ Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement of the U.S. Government. Although this report is in the public domain, it contains copyrighted materials that are noted in the text. Permission to reproduce those items must be secured from the individual copyright owners. Cataloging-in-publication data are on file with the Library of Congress (URL http://www.loc.gov/). -
October 2006
OCTOBER 2 0 0 6 �������������� http://www.universetoday.com �������������� TAMMY PLOTNER WITH JEFF BARBOUR 283 SUNDAY, OCTOBER 1 In 1897, the world’s largest refractor (40”) debuted at the University of Chica- go’s Yerkes Observatory. Also today in 1958, NASA was established by an act of Congress. More? In 1962, the 300-foot radio telescope of the National Ra- dio Astronomy Observatory (NRAO) went live at Green Bank, West Virginia. It held place as the world’s second largest radio scope until it collapsed in 1988. Tonight let’s visit with an old lunar favorite. Easily seen in binoculars, the hexagonal walled plain of Albategnius ap- pears near the terminator about one-third the way north of the south limb. Look north of Albategnius for even larger and more ancient Hipparchus giving an almost “figure 8” view in binoculars. Between Hipparchus and Albategnius to the east are mid-sized craters Halley and Hind. Note the curious ALBATEGNIUS AND HIPPARCHUS ON THE relationship between impact crater Klein on Albategnius’ southwestern wall and TERMINATOR CREDIT: ROGER WARNER that of crater Horrocks on the northeastern wall of Hipparchus. Now let’s power up and “crater hop”... Just northwest of Hipparchus’ wall are the beginnings of the Sinus Medii area. Look for the deep imprint of Seeliger - named for a Dutch astronomer. Due north of Hipparchus is Rhaeticus, and here’s where things really get interesting. If the terminator has progressed far enough, you might spot tiny Blagg and Bruce to its west, the rough location of the Surveyor 4 and Surveyor 6 landing area.