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No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
General Disclaimer One Or More of the Following Statements May Affect
https://ntrs.nasa.gov/search.jsp?R=19710025504 2020-03-11T22:36:49+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) 6 X t B ICC"m date: July 16, 1971 955 L'Enfant Plaza North, S. W Washington, D. C. 20024 to Distribution B71 07023 from. J. W. Head suhiecf Derivation of Topographic Feature Names in the Apollo 15 Landing Region - Case 340 ABSTRACT The topographic features in the region of the Apollo 15 landing site (Figure 1) are named for a number of philosophers, explorers and scientists (astronomers in particular) representing periods throughout recorded history. It is of particular interest that several of the individuals were responsible for specific discoveries, observations, or inventions which considerably advanced the study and under- standing of the moon (for instance, Hadley designed the first large reflecting telescope; Beer published classic maps and explanations of the moon's surface). -
DMAAC – February 1973
LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base. -
Annual Report 2008 – 2009
O L D S T U R B R I D G E Summer 2009 Special Annual VILLAGE Report Edition Visitor 2008-2009 2008--2009 Momentum and More The History of Fireworks Farms, Families, and Change Cooking with OSV Summer Events a member magazine that keeps you coming back Old Sturbridge Village, a museum and learning resource of 2008-2009 Building Momentum New England life, invites each visitor to find meaning, pleasure, a letter from President Jim Donahue relevance, and inspiration through the exploration of history. to our newly designed V I S I T O R magazine. We hope that you will learn new things and come to visit t is no secret around the Village that I like to keep my eye on the “dashboard” – a set of key the Village soon. There is always something fun to do at indicators that I am consistently checking to make sure we are steering OSV in the right direction. In fact, Welcome O l d S T u R b ri d g E V I l l a g E . I take a lot of good-natured kidding about how often I peek at the attendance figures each day, eager to see if we beat last year’s number. And I have to admit that I get energized when the daily mail brings in new donations, when the sun is shining, the parking lot is full, when I can hear happy children touring the Village, and the visitor comments are upbeat and favorable. Volume XlIX, No. 2 Summer 2009 Special Annual Report Edition I am happy to report these indicators have been overwhelmingly positive during the past year – solid proof that Old Sturbridge Village is building on last year’s successes and is poised to finish this decade much stronger There is nothing quite like learning about history from than when it started. -
List of Targets for the Lunar II Observing Program (PDF File)
Task or Task Description or Target Name Wood's Rükl Target LUNAR # 100 Atlas Catalog (chart) Create a sketch/map of the visible lunar surface: 1 Observe a Full Moon and sketch a large-scale (prominent features) L-1 map depicting the nearside; disk of visible surface should be drawn 2 at L-1 3 least 5-inches in diameter. Sketch itself should be created only by L-1 observing the Moon, but maps or guidebooks may be used when labeling sketched features. Label all maria, prominent craters, and major rays by the crater name they originated from. (Counts as 3 observations (OBSV): #1, #2 & #3) Observe these targets; provide brief descriptions: 4 Alpetragius 55 5 Arago 35 6 Arago Alpha & Arago Beta L-32 35 7 Aristarchus Plateau L-18 18 8 Baco L-55 74 9 Bailly L-37 71 10 Beer, Beer Catena & Feuillée 21 11 Bullialdus, Bullialdus A & Bullialdus B 53 12 Cassini, Cassini A & Cassini B 12 13 Cauchy, Cauchy Omega & Cauchy Tau L-48 36 14 Censorinus 47 15 Crüger 50 16 Dorsae Lister & Smirnov (A.K.A. Serpentine Ridge) L-33 24 17 Grimaldi Basin outer and inner rings L-36 39, etc. 18 Hainzel, Hainzel A & Hainzel C 63 19 Hercules, Hercules G, Hercules E 14 20 Hesiodus A L-81 54, 64 21 Hortensius dome field L-65 30 22 Julius Caesar 34 23 Kies 53 24 Kies Pi L-60 53 25 Lacus Mortis 14 26 Linne 23 27 Lamont L-53 35 28 Mairan 9 29 Mare Australe L-56 76 30 Mare Cognitum 42, etc. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Congressional Record—Senate S1186
S1186 CONGRESSIONAL RECORD — SENATE February 12, 2019 the inclusion of the Frank and Jeanne RECESS and Water Conservation Fund and the Moore Salmon Sanctuary. The PRESIDING OFFICER. Under protection of Paradise Valley. In fact, As anybody who works on public the previous order, the Senate stands Paradise Valley is the doorstep to Yel- lands legislation knows, sometimes it in recess until 2:15. lowstone National Park, our Nation’s is hard to find a balance in order to get Thereupon, the Senate, at 12 noon, first national park. That would be found in the Yellowstone Gateway Pro- public lands legislation passed. Nobody recessed until 2:15 p.m. and reassem- bled when called to order by the Pre- tection Act. gets everything they want. Nobody Growing up, I spent a lot of time in siding Officer (Mrs. CAPITO). gets everything they believe they that part of our State. I still do. I love ought to have. The question is, can you f fly fishing on the Yellowstone River. In bring people together. NATURAL RESOURCES fact, when I was in high school, I load- I am going to close by way of saying MANAGEMENT ACT—Continued ed up the station wagon—in fact, I I have highlighted a number of provi- think probably the Griswolds’ station The PRESIDING OFFICER. The Sen- sions that I am glad we got in here. It wagon by today’s standards—and, with ator from Montana. was 10 years earlier when then-Presi- a couple of my classmates from Boze- dent Obama signed seven pieces of pub- S. -
Get Smart with Art Is Made Possible with Support from the William K
From the Headlines About the Artist From the Artist Based on the critics’ comments, what aspects of Albert Bierstadt (1830–1902) is Germany in 1830, Albert Bierstadt Bierstadt’s paintings defined his popularity? best known for capturing majestic moved to Massachusetts when he western landscapes with his was a year old. He demonstrated an paintings of awe-inspiring mountain early interest in art and at the age The striking merit of Bierstadt in his treatment of ranges, vast canyons, and tumbling of twenty-one had his first exhibit Yosemite, as of other western landscapes, lies in his waterfalls. The sheer physical at the New England Art Union in power of grasping distances, handling wide spaces, beauty of the newly explored West Boston. After spending several years truthfully massing huge objects, and realizing splendid is evident in his paintings. Born in studying in Germany at the German atmospheric effects. The success with which he does Art Academy in Düsseldorf, Bierstadt this, and so reproduces the noblest aspects of grand returned to the United States. ALBERT BIERSTADT scenery, filling the mind of the spectator with the very (1830–1902) sentiment of the original, is the proof of his genius. A great adventurer with a pioneering California Spring, 1875 Oil on canvas, 54¼ x 84¼ in. There are others who are more literal, who realize details spirit, Bierstadt joined Frederick W. Lander’s Military Expeditionary Presented to the City and County of more carefully, who paint figures and animals better, San Francisco by Gordon Blanding force, traveling west on the overland who finish more smoothly; but none except Church, and 1941.6 he in a different manner, is so happy as Bierstadt in the wagon route from Saint Joseph, Watkins Yosemite Art Gallery, San Francisco. -
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America There are approximately 101,135sexual abuse claims filed. Of those claims, the Tort Claimants’ Committee estimates that there are approximately 83,807 unique claims if the amended and superseded and multiple claims filed on account of the same survivor are removed. The summary of sexual abuse claims below uses the set of 83,807 of claim for purposes of claims summary below.1 The Tort Claimants’ Committee has broken down the sexual abuse claims in various categories for the purpose of disclosing where and when the sexual abuse claims arose and the identity of certain of the parties that are implicated in the alleged sexual abuse. Attached hereto as Exhibit 1 is a chart that shows the sexual abuse claims broken down by the year in which they first arose. Please note that there approximately 10,500 claims did not provide a date for when the sexual abuse occurred. As a result, those claims have not been assigned a year in which the abuse first arose. Attached hereto as Exhibit 2 is a chart that shows the claims broken down by the state or jurisdiction in which they arose. Please note there are approximately 7,186 claims that did not provide a location of abuse. Those claims are reflected by YY or ZZ in the codes used to identify the applicable state or jurisdiction. Those claims have not been assigned a state or other jurisdiction. Attached hereto as Exhibit 3 is a chart that shows the claims broken down by the Local Council implicated in the sexual abuse. -
Northwest Plant Names and Symbols for Ecosystem Inventory and Analysis Fourth Edition
USDA Forest Service General Technical Report PNW-46 1976 NORTHWEST PLANT NAMES AND SYMBOLS FOR ECOSYSTEM INVENTORY AND ANALYSIS FOURTH EDITION PACIFIC NORTHWEST FOREST AND RANGE EXPERIMENT STATION U.S. DEPARTMENT OF AGRICULTURE FOREST SERVICE PORTLAND, OREGON This file was created by scanning the printed publication. Text errors identified by the software have been corrected; however, some errors may remain. CONTENTS Page . INTRODUCTION TO FOURTH EDITION ....... 1 Features and Additions. ......... 1 Inquiries ................ 2 History of Plant Code Development .... 3 MASTER LIST OF SPECIES AND SYMBOLS ..... 5 Grasses.. ............... 7 Grasslike Plants. ............ 29 Forbs.. ................ 43 Shrubs. .................203 Trees. .................225 ABSTRACT LIST OF SYNONYMS ..............233 This paper is basicafly'an alpha code and name 1 isting of forest and rangeland grasses, sedges, LIST OF SOIL SURFACE ITEMS .........261 rushes, forbs, shrubs, and trees of Oregon, Wash- ington, and Idaho. The code expedites recording of vegetation inventory data and is especially useful to those processing their data by contem- porary computer systems. Editorial and secretarial personnel will find the name and authorship lists i ' to be handy desk references. KEYWORDS: Plant nomenclature, vegetation survey, I Oregon, Washington, Idaho. G. A. GARRISON and J. M. SKOVLIN are Assistant Director and Project Leader, respectively, of Paci fic Northwest Forest and Range Experiment Station; C. E. POULTON is Director, Range and Resource Ecology Applications of Earth Sate1 1 ite Corporation; and A. H. WINWARD is Professor of Range Management at Oregon State University . and a fifth letter also appears in those instances where a varietal name is appended to the genus and INTRODUCTION species. (3) Some genera symbols consist of four letters or less, e.g., ACER, AIM, GEUM, IRIS, POA, TO FOURTH EDITION RHUS, ROSA. -
Graphical Evidence for the Solar Coronal Structure During the Maunder Minimum: Comparative Study of the Total Eclipse Drawings in 1706 and 1715
J. Space Weather Space Clim. 2021, 11,1 Ó H. Hayakawa et al., Published by EDP Sciences 2021 https://doi.org/10.1051/swsc/2020035 Available online at: www.swsc-journal.org Topical Issue - Space climate: The past and future of solar activity RESEARCH ARTICLE OPEN ACCESS Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 1715 Hisashi Hayakawa1,2,3,4,*, Mike Lockwood5,*, Matthew J. Owens5, Mitsuru Sôma6, Bruno P. Besser7, and Lidia van Driel – Gesztelyi8,9,10 1 Institute for Space-Earth Environmental Research, Nagoya University, 4648601 Nagoya, Japan 2 Institute for Advanced Researches, Nagoya University, 4648601 Nagoya, Japan 3 Science and Technology Facilities Council, RAL Space, Rutherford Appleton Laboratory, Harwell Campus, OX11 0QX Didcot, UK 4 Nishina Centre, Riken, 3510198 Wako, Japan 5 Department of Meteorology, University of Reading, RG6 6BB Reading, UK 6 National Astronomical Observatory of Japan, 1818588 Mitaka, Japan 7 Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria 8 Mullard Space Science Laboratory, University College London, RH5 6NT Dorking, UK 9 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 92195 Meudon, France 10 Konkoly Observatory, Hungarian Academy of Sciences, 1121 Budapest, Hungary Received 18 October 2019 / Accepted 29 June 2020 Abstract – We discuss the significant implications of three eye-witness drawings of the total solar eclipse on 1706 May 12 in comparison with two on 1715 May 3, for our understanding of space climate change. These events took place just after what has been termed the “deep Maunder Minimum” but fall within the “extended Maunder Minimum” being in an interval when the sunspot numbers start to recover.