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UAD Instance Chart 04.06.15 11:14
UAD Instance Chart 04.06.15 11:14 Search Site Hardware UAD-2 + Plug-Ins Store Blog Support About My.Uaudio Pressroom Contact Cart SUBSCRIBE TO THE Enter your email address Home > Support > UAD Support > UAD Compatibility > UAD Instance Chart UA NEWSLETTER UAD Instance Chart Online Support About This Chart The following table indicates DSP usage and instance counts for UAD Powered Plug-Ins. See bottom of page for more details about the chart. UAD Powered Plug-In DSP % SOLO DUO QUAD OCTO Contact Us Mono Stereo Mono Stereo Mono Stereo Mono Stereo Mono Stereo Phone Support 4K Buss Compressor 2.8% 3.4% 35 29 70 58 140 116 280 232 USA (toll free) 877-698-2834 4K Channel Strip * 7.4% 11.4% 17 11 34 22 68 44 136 88 International Ampex ATR-102 Mastering Tape Recorder 17.6% 29.0% 5 3 10 6 20 12 40 24 +1-831-440-1176 AMS RMX16 Digital Reverb 40.6% 41.1% 2 2 4 4 8 8 16 16 Germany, Austria, and Switzerland +31 (0) 20 800 4912 API 550A EQ 7.2% 11.7% 13 8 26 16 52 32 104 64 Fax +1-831-461-1550 API 560 EQ 9.2% 15.5% 10 6 20 12 40 24 80 48 Customer support is available from 9am to 5pm, Monday through Friday, PST API Vision Channel Strip * 22.4% 29.7% 4 3 8 6 16 12 32 24 Contact Support Bermuda Triangle 14.3% 28.4% 7 3 14 6 28 12 56 24 Submit a Request bx_digital V2 EQ & De-Esser 3.4% 4.9% N/A 20 N/A 40 N/A 80 N/A 160 Press, Review, and Advertising Inquiries Amanda Whiting bx_digital V2 Mono EQ & De-Esser 3.4% 3.8% 29 20 58 40 116 80 232 160 +1-831-440-1176 bx_refinement 12.3% 11.9% 7 7 14 14 28 28 56 56 Mailing Address Universal Audio, Inc. -
Annual Report COOPERATIVE INSTITUTE for RESEARCH in ENVIRONMENTAL SCIENCES
2015 Annual Report COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES 2015 annual report University of Colorado Boulder UCB 216 Boulder, CO 80309-0216 COOPERATIVE INSTITUTE FOR RESEARCH IN ENVIRONMENTAL SCIENCES University of Colorado Boulder 216 UCB Boulder, CO 80309-0216 303-492-1143 [email protected] http://cires.colorado.edu CIRES Director Waleed Abdalati Annual Report Staff Katy Human, Director of Communications, Editor Susan Lynds and Karin Vergoth, Editing Robin L. Strelow, Designer Agreement No. NA12OAR4320137 Cover photo: Mt. Cook in the Southern Alps, West Coast of New Zealand’s South Island Birgit Hassler, CIRES/NOAA table of contents Executive summary & research highlights 2 project reports 82 From the Director 2 Air Quality in a Changing Climate 83 CIRES: Science in Service to Society 3 Climate Forcing, Feedbacks, and Analysis 86 This is CIRES 6 Earth System Dynamics, Variability, and Change 94 Organization 7 Management and Exploitation of Geophysical Data 105 Council of Fellows 8 Regional Sciences and Applications 115 Governance 9 Scientific Outreach and Education 117 Finance 10 Space Weather Understanding and Prediction 120 Active NOAA Awards 11 Stratospheric Processes and Trends 124 Systems and Prediction Models Development 129 People & Programs 14 CIRES Starts with People 14 Appendices 136 Fellows 15 Table of Contents 136 CIRES Centers 50 Publications by the Numbers 136 Center for Limnology 50 Publications 137 Center for Science and Technology -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi. -
PEANUTS and SPACE FOUNDATION Apollo and Beyond
Reproducible Master PEANUTS and SPACE FOUNDATION Apollo and Beyond GRADE 4 – 5 OBJECTIVES PAGE 1 Students will: ö Read Snoopy, First Beagle on the Moon! and Shoot for the Moon, Snoopy! ö Learn facts about the Apollo Moon missions. ö Use this information to complete a fill-in-the-blank fact worksheet. ö Create mission objectives for a brand new mission to the moon. SUGGESTED GRADE LEVELS 4 – 5 SUBJECT AREAS Space Science, History TIMELINE 30 – 45 minutes NEXT GENERATION SCIENCE STANDARDS ö 5-ESS1 ESS1.B Earth and the Solar System ö 3-5-ETS1 ETS1.B Developing Possible Solutions 21st CENTURY ESSENTIAL SKILLS Collaboration and Teamwork, Communication, Information Literacy, Flexibility, Leadership, Initiative, Organizing Concepts, Obtaining/Evaluating/Communicating Ideas BACKGROUND ö According to NASA.gov, NASA has proudly shared an association with Charles M. Schulz and his American icon Snoopy since Apollo missions began in the 1960s. Schulz created comic strips depicting Snoopy on the Moon, capturing public excitement about America’s achievements in space. In May 1969, Apollo 10 astronauts traveled to the Moon for a final trial run before the lunar landings took place on later missions. Because that mission required the lunar module to skim within 50,000 feet of the Moon’s surface and “snoop around” to determine the landing site for Apollo 11, the crew named the lunar module Snoopy. The command module was named Charlie Brown, after Snoopy’s loyal owner. These books are a united effort between Peanuts Worldwide, NASA and Simon & Schuster to generate interest in space among today’s younger children. -
Worry Over Mistreating Clots Drove Push to Pause J&J Shot
P2JW109000-6-A00100-17FFFF5178F ****** MONDAY,APRIL 19,2021~VOL. CCLXXVII NO.90 WSJ.com HHHH $4.00 Last week: DJIA 34200.67 À 400.07 1.2% NASDAQ 14052.34 À 1.1% STOXX 600 442.49 À 1.2% 10-YR. TREASURY À 27/32 , yield 1.571% OIL $63.13 À $3.81 EURO $1.1982 YEN 108.81 Bull Run What’s News In Stocks Widens, Business&Finance Signaling More stocks have been propelling the U.S. market higher lately,asignal that fur- Strength ther gains could be ahead, but howsmooth the climb might be remains up fordebate. A1 Technical indicators WeWork’s plan to list suggestmoregains, stock by merging with a but some question how blank-check company has echoes of its approach in smooth theywill be 2019,when the shared-office provider’s IPO imploded. A1 BY CAITLIN MCCABE Citigroup plans to scale up its services to wealthy GES Agreater number of stocks entrepreneurs and their IMA have been propelling the U.S. businesses in Asia as the market higher lately,asignal bank refocuses its opera- GETTY that—if historyisany indica- tions in the region. B1 SE/ tor—moregains could be ahead. What remains up forde- A Maryland hotel mag- bate, however, is how smooth natebehind an 11th-hour bid ANCE-PRES FR the climb will be. to acquireTribune Publish- Indicatorsthat point to a ing is working to find new ENCE stronger and moreresilient financing and partnership AG stock market have been hitting options after his partner ON/ LL rare milestones recently as the withdrew from the deal. -
Turbulence and Aeolian Morphodynamics in Craters on Mars: Application to Gale Crater, Landing Site of the Curiosity Rover
16TH EUROPEAN TURBULENCE CONFERENCE, 21-24 AUGUST, 2017, STOCKHOLM,SWEDEN TURBULENCE AND AEOLIAN MORPHODYNAMICS IN CRATERS ON MARS: APPLICATION TO GALE CRATER, LANDING SITE OF THE CURIOSITY ROVER William Anderson1, Gary Kocurek2 & Kenzie Day2 1Mechanical Engineering Dept., Univ. Texas at Dallas, Richardson, Texas, USA 2Dept. Geological Sciences, Jackson School of Geosciences, Univ. Texas at Austin, Austin, Texas, USA Mars is a dry planet with a thin atmosphere. Aeolian processes – wind-driven mobilization of sediment and dust – are the dominant mode of landscape variability on the dessicated landscapes of Mars. Craters are common topographic features on the surface of Mars, and many craters on Mars contain a prominent central mound (NASA’s Curiosity rover was landed in Gale crater, shown in Figure 1a [1], while Figures 1b and 1c show Henry and Korolev crater, respectively). These mounds are composed of sedimentary fill and, therefore, they contain rich information on the evolution of climatic conditions on Mars embodied in the stratigraphic “layering” of sediments. Many other craters no longer house a mound, but contain sediment and dust from which dune fields and other features form (see, for example, Victoria Crater, Figure 1d). Using density-normalized large-eddy simulations, we have modeled turbulent flows over crater-like topographies that feature a central mound. Resultant datasets suggest a deflationary mechanism wherein vortices shed from the upwind crater rim are realigned to conform to the crater profile via stretching and tilting. This was accomplished using three- dimensional datasets (momentum and vorticity) retrieved from LES. As a result, helical vortices occupy the inner region of the crater and, therefore, are primarily responsible for aeolian morphodynamics in the crater (radial katabatic flows are also important to aeolian processes within the crater [2]). -
Volume 3, Number 3, November 2014
THE STAR THE NEWSLETTER OF THE MOUNT CUBA ASTRONOMICAL GROUP VOL. 3 NUM. 3 CONTACT US AT DAVE GROSKI [email protected] OR HANK BOUCHELLE [email protected] 302-983-7830 OUR PROGRAMS ARE HELD THE SECOND TUESDAY OF EACH MONTH AT 7:30 P.M. UNLESS INDICATED OTHERWISE MOUNT CUBA ASTRONOMICAL OBSERVATORY 1610 HILLSIDE MILL ROAD GREENVILLE DE. FOR DIRECTIONS PLEASE VISIT www.mountcuba.org PLEASE SEND ALL PHOTOS AND ARTICLES TO [email protected] 1 NOVEMBER MEETING TUESDAY THE 11TH 7:30 p.m. OCTOBER MEETING REVIEW: Dave Groski gave a presentation on the Spilhaus Space Clock. This is such an interesting devise that I shall cover it in more detail under the Points of Interest section of the STAR. Dr. Hank Bouchelle once again gave a truly informative talk on not one but several topics related to Astronomy and Physics in general. Since he covered such a varied group of topics, I shall also cover them in the Points of Interest section. Phenomena: Knock! Knock! Is Anyone home? Hank Bouchelle Cinematic depictions of the events accompanying an alien visit are almost uniformly dire. Alien intentions are almost always destructive, deadly, or intended to enslave. They destroy entire populations, and unleash weapons that easily turn Earth to dust. Reports of personal interactions with aliens frequently relate queasy adventures in proctology. It is a bit strange, then, that many people, especially among the scientific community, spare no effort or cost to detect alien messages or the electronic fingerprint of signals that are not produced by the nature. -
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. -
1 Reading Athenaios' Epigraphical Hymn to Apollo: Critical Edition And
Reading Athenaios’ Epigraphical Hymn to Apollo: Critical Edition and Commentaries DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Corey M. Hackworth Graduate Program in Greek and Latin The Ohio State University 2015 Dissertation Committee: Fritz Graf, Advisor Benjamin Acosta-Hughes Carolina López-Ruiz 1 Copyright by Corey M. Hackworth 2015 2 Abstract This dissertation is a study of the Epigraphical Hymn to Apollo that was found at Delphi in 1893, and since attributed to Athenaios. It is believed to have been performed as part of the Athenian Pythaïdes festival in the year 128/7 BCE. After a brief introduction to the hymn, I provide a survey and history of the most important editions of the text. I offer a new critical edition equipped with a detailed apparatus. This is followed by an extended epigraphical commentary which aims to describe the history of, and arguments for and and against, readings of the text as well as proposed supplements and restorations. The guiding principle of this edition is a conservative one—to indicate where there is uncertainty, and to avoid relying on other, similar, texts as a resource for textual restoration. A commentary follows, which traces word usage and history, in an attempt to explore how an audience might have responded to the various choices of vocabulary employed throughout the text. Emphasis is placed on Athenaios’ predilection to utilize new words, as well as words that are non-traditional for Apolline narrative. The commentary considers what role prior word usage (texts) may have played as intertexts, or sources of poetic resonance in the ears of an audience. -
Project: Apollo 8
v ._. I / I NATIONAL AERONAUTICS AND SPACE ADMINISTRATION TELS WO 2-4155 NEWS WASHINGTON,D.C.20546 • WO 3-6925 FOR RELEASE: SUNDAY December 15, 1968 RELEASE NO: 68.208 P PROJECT: APOLLO 8 R E contents GENERAL RELEASE----------~-------~·~-~-~--~~----~----~-~--~-l-lO MISSION OBJECTIVES------------------------------------------11 SEQUENCE OF EVENTS-------------~-------------~----~----~--~~12-14 5 Launch W1ndow~~-~----~--~-~--~-------~-----~---------w--~-14 MISSION DESCRIPTION-----------------------------------------15-19 FLIGHT PLAN--~---~-----·------------~------~----~---~----~--20-23 ALTERNATE MISSIONS---------------------------------~--------24-26 5 ABORT MODES-----~--------------~--~--~------------~---~~--~-27~29 PHOTOGRAPHIC TASKS------------------------------------------30-32 SPACECRAFT STRUCTURE SYSTEMS--------------------------------33-37 SATURN V LAUNCH VEHICLE-------------------------------------38-50 APOLLO 8 LAUNCH OPERATIONS----------------------------------51.64 MISSION CONTROL CENTER--------------------------------------65-66 MANNED SPACE FLIGHT NETWORK---------------------------------67-71 APOLLO 8 RECOVERY-------------------------------------------72-73 APOLLO 8 CREW-------------~--~--~~-~~---~---~~~-------------74-86 K LUNAR DESCRIPTION-------------------------------------------87-88 APOLLO PROGRAM MANAGEMENT/CONTRACTORS---~-------------------39-94 I APOLLO 8 GLOSSARY-------- -----------------------------------95-101 T -0- 12/6/68 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION WO 2-4155 NEWS WASHINGTON, D.C. 20546 TELS. -
Apollo 12 Photography Index
%uem%xed_ uo!:q.oe_ s1:s._l"e,d_e_em'I flxos'p_zedns O_q _/ " uo,re_ "O X_ pea-eden{ Z 0 (D I I 696L R_K_D._(I _ m,_ -4 0", _z 0', l',,o ._ rT1 0 X mm9t _ m_o& ]G[GNI XHdV_OOZOHd Z L 0T'I0_V 0 0 11_IdVdONI_OM T_OINHDZZ L6L_-6 GYM J_OV}KJ_IO0VSVN 0 C O_i_lOd-VJD_IfO1_d 0 _ •'_ i wO _U -4 -_" _ 0 _4 _O-69-gM& "oN GSVH/O_q / .-, Z9946T-_D-VSVN FOREWORD This working paper presents the screening results of Apollo 12, 70mmand 16mmphotography. Photographic frame descriptions, along with ground coverage footprints of the Apollo 12 Mission are inaluded within, by Appendix. This report was prepared by Lockheed Electronics Company,Houston Aerospace Systems Division, under Contract NAS9-5191 in response to Job Order 62-094 Action Document094.24-10, "Apollo 12 Screening IndeX', issued by the Mapping Sciences Laboratory, MannedSpacecraft Center, Houston, Texas. Acknowledgement is made to those membersof the Mapping Sciences Department, Image Analysis Section, who contributed to the results of this documentation. Messrs. H. Almond, G. Baron, F. Beatty, W. Daley, J. Disler, C. Dole, I. Duggan, D. Hixon, T. Johnson, A. Kryszewski, R. Pinter, F. Solomon, and S. Topiwalla. Acknowledgementis also made to R. Kassey and E. Mager of Raytheon Antometric Company ! I ii TABLE OF CONTENTS Section Forward ii I. Introduction I II. Procedures 1 III. Discussion 2 IV. Conclusions 3 V. Recommendations 3 VI. Appendix - Magazine Summary and Index 70mm Magazine Q II II R ii It S II II T II I! U II t! V tl It .X ,, ,, y II tl Z I! If EE S0-158 Experiment AA, BB, CC, & DD 16mm Magazines A through P VII.