DOCSLIB.ORG

O E a N U S P R C E L L a R U M M Ontes R O O K M O N Te S C O R D I Le

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
O E a N U S P R C E L L a R U M M Ontes R O O K M O N Te S C O R D I Le 100°W 90°W 80°W 70°W 60°W 50°W 40°W 30°W 20°W 10°W 0° 10°E 20°E 30°E 40°E 50°E 60°E 70°E 80°E 90°E 100°E 50°N 50°N Chapman Aristoteles Baily . Mitchell Galvani M . Trouvelot o M Maupertuis n t es e O lp Egede . Bianchini s A N lis ORIS J T T Val p U Montes Recti e LACUS r R ne E a r A e h if McLaughlin fe S Atlas S S ard Hercules s E Rima Mercurius a T LACUS Atla m . Dechen i Promontorium N R Sharp Laplace Mons Boss SINUS R Rimae Ger O g Pico r TEMPORIS ü SINUS Mont . B Zeno . Schönfeld Bürg M Blanc A e Chevallier a Gerard L Eudoxus im Promontorium SUS R . Louville Deville P . Harding MORTIS . Carrington IRIDUM E . Vashakidze S Oersted LACUS . Lamèch UCA Mason . Shuckburgh Schumacher SPEI Fabry Promontorium Piazzi Agassiz Plana . Smyth . Williams Bunsen von Mairan Braun Mons Mons Hooke Rümker Promontorium Piton Cepheus Heraclides . Helicon . Le Verrier Cassini Alexander . 40°N 40°N Avicenna Grove Riemann Harkhebi . Kirch LACUS SOMNIORUM Messala Rima Mair . Calippus O Franklin Rimae Daniell Lavoisier MARE C Dor s an Rima Beals . ppu . Maury E sum ali C . Mons Gruithuisen Gamma Theaetetus Berzelius S . Mons Gruithuisen Delta Gauss Nernst A . Naumann . Daniell N Bernoulli d en cilla n . C. Herschel g U o Geminus B Vestine . Carlini Montes Aristillus . Dor Hall G . Luther Berosus S MONTES CA sum Heim Spitzber Ulugh . Röntgen Aston Gruithuisen s Posidonius u R a Richardson Lorentz t imae . Heis P m Beigh e i IMBRIUM SINUS t osidonius . G. Bond e R . Nielsen . Lich tenberg a Landsteiner e . h Dor sum Burckhardt Hahn her Rupes Gaston LUNICUS T . Bo Linda Humason ris elisle abau e . Boris . Autolycus sa Whiston . a . Wollaston Dor . a D Gr Maxwell ma Buc . McDonald a Ri Rim sum m i 30°N Charles . Kirchhoff 30°N Cleopatr . Aloha . Delisle Caventou .Mavis Dor Dor R Chacornac . la Dor Mons . o Archimedes Debes Rayleigh ric Dor Annegrit Cha Newcomb Angström . Sampson Timochar . Ag Cate a Krieger Rimae m Nig s Rima Delisle sum Zirk Ri u Krieger Rocco sa Ar MONTES g m . na Promontorium Fresnel c li Samir or . .Ruth is Louise Tralles Van Biesbroeck . n R R Rima . Diophantus Cleomeimdeas . sum ac Isabel resnel Dor Rimae gand . Walter Laue Fedorov . el Dor MARE i Montes Agricola . Bancroft m Toscanelli er Urey Voskresenskiy . Mons . Spurr . Santos-Dumont Linné . T Higazy . Golgi Mons R P a TAURUS . h os Feuillée ALUS PUTRE Rupe . Diophantus v e sa Burnet .Herodotus La Hire . im inz vic Lomonosov c Rimae o istarchus ma Artsimovich sa .Beer a R anelli mo Dor n Delmotte i e Raman Ri Rimae F . Pr s Dor t ö s Ar . A DINIS Seneca Ar Timocharis Russell Zinner Ivan Stille . rc . Banting sum Azar m Cleomedes . h D . Le Monnier . Briggs s S D Lyapunov i e i O l . m Mons Hadley or l ch Vera r Montes o a e Julienne wen rö . sum M V Väisälä d r A t . sa Smir i . e e su R Ian y t Joliot . Lambert s Mons Hadley Delta d E r . Very F reud Prinz Dor Felix Archimedes ima e s . i Kathleen Rima Rima . m a n . R a g-Mei Römer Za ma Courtney Artemis V Ann Michael i n . Dor lad adl R u a Ar . Montes Harbing h . Joy G sum Verne im . S . ir i . Carlos H Dor a Patricia . Sung-Mei v Cat .Heinrich duino Yoshi Sarabhai Edison . Ther Taizo . Krishna Béla . o Y . su en . ur Christel . V Bartels . .Manuel r m .Jomo a i a y m d . e on dl u l E immart Plutarch MacMillan s SERENITATIS . y a Hornsby A A . r r . Struve le Aratus C . Aristarchus B o Finsch y Pupin . LACUS a w N o r D . Schiaparelli o B Euler tta .Brewster . r . t G t Herodotus a i BONITATIS R a s L i a U r im m . Franck . Borel e Mons Vinogradov R en w o Hubble a t o a a I y . Galen e m D D i C ittr S Bell S . Bessel L . R o a Mons . Conon MONTES u HAEMUS r . Littrow Eddington adle l r D m uler p s e Cle rke SINUS o i a E t . Esclangon Macrobius . Seleucus m ic u . Deseilligny Tisserand l r R Ri Br i m is . e s Moseley . us p a Dziewulski Brayley .Jehan G L p Ango a . D Catena . Pytheas l Hill Rosa Huxley lu Abetti O z . Akis . Wallace s Ching-Te Mons Maraldi i . C R . Rima Cono e ens Ampèr . a im r w 20°N 20°N Catena . M me T a .. Stella Cannon ulsk Pierre . f Natasha Mons n l e ons . ma o B i t u a .Mons Vitruvius LACUS ODII c s R Dor y Balboa Rima Wan-Yu Sulpicius Gallus Bobillier k r Mons Argaeus . Carmichael l i Huyg o Rud a . Swift D nd D Robert Rima . Maraldi a Dag or Ni Ma e Sorby . Isis Mons Agnes sa Mary . rc e . el LACUS . Osiris l Ina s Rimao m v .. c .Jerik . Fabbroni n um . Osama na Reik u ol te FELICITATIS o s . Peirce Rima Categit AMORIS . Fredholm Brackett ri Draper . B r R R i SINUS D m o Al-Biruni Draper . im aw a . e Eckert LACUS s Vitruvius Gardner ae . D . FIDEI Bowen Me Theophrastus ne . Dalton . DOLORIS la . Dawes Popov u R arius . Yangel' s Rimae Plinius im M Mons Wolff Einstein Krafft a MONTES CARP MONTES APENNIRimNa YaUngel' S LACUS . Franz MARE CRISIUM . Menelaus Tacquet . Beketov Marco GAUDII . Proclus r . Alhazen Daubrée Promontorium sa e . T. Mayer . k Polo Archerusia Plinius ow r LACUS Auwers Dor a afft A . H Goddard .Bessarion J Rim Barl Promontorium TUS HIEMALIS LACUS a Mons Esam Kr n . Yerkes .Curtis a Agarum Catena s Diana . Picard . Eratosthenes . Al-Bakri . PALUS Ginzel Vasco e .Grace . Lucian MARE Ibn er LENITATIS n y . Gay-Lussac MARE . Crile a . Hansen . Ma s Yunus da Gama T Manilius r ma . Jansen Lyell SOMNI . Cardanus Ri ima o . Sabatier .Theiler Rima Galilaei R sac . D Mees s . Glaisher Greaves Cajal . Fahrenheit -Lu ear Bohr y Dor VAPORUM V Ga Lick sum T acl a s Rimae u SINUS Rima Cauc ermie Mons Usov Condorcet MARGINIS l n Marius M l Carda . i . Ross s a HONORIS r im SINUS R R h B . Galilaei . Carrel e CONCORDIAE . Sundman Stadius c . Maclear MARE h Auzout i o y Dreyer m vi Boscovich . ma h . 10°N 10°N mae a co . r Ri Ri o da Gama M Copernicus Rupes Cauch c Milichius Cauchy . Tebbutt Krogh . Wildt Virchow as . Bos . van Albada i Shapley . l V i R Julius c Sinas h im . Watts Rim i Caesar u . Sosigenes Jansky . Elvey a a s Rim da Vinci Bo y Neper Glushko . Kepler . a us d H ac iae MARE e . y L ant Reiner e . ginu Rima Ar ver Hyginus . S SINUS AESTUUM s .Donna erse PLANITIA u P Olbers Gamma igenes . Lawrence Asada Firmicus . e Ukert . DESCENSUS . Reiner s Bode Rimae s . iadaeus MARE UNDARUM . Hortensius Sos Cameron . Fauth . Arago . Aryabhata . P r Rimae e Taruntius . Boethius Banachiewicz k Silberschlag ae c . Daly Erro Pallas . Zähringer . Abbot . Knox-Shaw im Taruntius . Bombelli . Cavalerius R R . Wallach . Maestlin esne INSULARUM Murchison i r Tacchini . Encke T .Ariadaeus . Manners Lamont . Nunn Apollonius Babcock . Suess Whewell . Dubyago . Triesnecker Agrippa . R . T Ri O Chladni . Cayley i Ap m ma r I a . Zasyadko Tempel oll e i Cartan R TRANQUILLITATIS o esn H nius imae e De Morgan .Menzel C T Ca Ameghino . Townley a . elius r ten Kunowsky . Reinhold Dorsa . ec un C . v Dor Rimae . Dembowski t a Liouville Dana C ius . C Dionysius E k . R u Maestlin Schubert . Peek S s sum er Respighi . Hedin . i h Schröter tt Petit ma . D . EDII . D'Arrest e . Maskelyne . Secchi r Ritter n Smithson Stewart . Hevelius M . o Sinus . McAdie r D E r Godin S . Condon s MARE e . Ca o Aldrin E a . .Armstrong T r Successus . Sabine . Anville su i C y .Bruce .Blagg Collins N e m Back Dorsum Rima . O a ux L t MARE Cloos . Gambart Schmidt Rimaecch o Jenkins Schröt M e SPUMANS . Pomortsev . .Statio Tranquillitatis S . Fox Rimae He Sömmering Nobili . R 0° L SINUS . im 0° ae Rima M Lohrmann . Lansberg Rhaeticus . A Hy . Moltke .Censorinus . Hermann . Mösting . Theon Senior patia Weierstrass er essier v . Webb . polz o Oppolzer ma Op Lade MARE us Avery R . Turner . Ri dr . Wyld on R n . Hargreaves . Van Vleck . Haldane v ri i . ma m . Delambre . Messier A Maclaurin lam Seeliger . Carrillo Purkyne F a . Theon Junior . Kramarov . R a . U ma é ie s . Morley . Geissler Runge Ri a k r um .Pickering i Talbot Riccioli o u e Slocum Flammarion Réaumur r . Leakey D Gilbert . G M SINUS Rim R i m . Horrocks . Lubbock . Warner ae . Riccio . Saunder . Hypatia ae Rankine SMYTHII . Spörer . Flamsteed Lalande . Hume . Torricelli l Damoiseau . Naonobu . Couder i . Gute Lebesgue Gyldén Hipparchus a . s . V Grimaldi . Taylor . Alfraganus .Amontons r . Lindbergh a . Acosta . Swasey . Herschel o Tucker l nber . Atwood . Hirayama l Bilharz Schlüter D . Fra Mauro i . Born Do ASPERITATIS s FECUNDITATIS Widmannstätten Hartwig rs y Kiess a r g R r ub a Kästner Kao P Ibn Battuta imaldi .
Load more

Recommended publications
  • 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.
    [Show full text]
  • Table of Exposures
    Table of Exposures Dole UT Focal Emulsion Exposure Moon's age Plate Nos. ralio sec. days 08.11.65 2132· f/29 Kodak 0.250 Plole 0.4 15.3 7e/2 08.01.66 2228 f/24 Kodak 0.250 Plate 0.31 17.0 3b, 15e 31.01.66 1947 1/24 Kodak 0.250 Plale 0.3 10.1 5b 02.02.66 1944 f/24 Kodak 0.250 Plote 0.25 12.1 7b, 8b 06.02.66 2326 1/24 Kodak 0.250 Plole 0.2 16.3 14c,16b 05.03.66 2259 1/41 IIford Zenith Plole 0.1 13 .5 lOe/l 27.04.66 2152 1/24 lIford G.30 Plate 0.5 6.9 150 28.04.66 2046 f/30 lIford G.30 Pia Ie 0.8 7.9 10,130 23.05.66 2033 f/24 Kodak 0.250 Plole 0.7 3.4 15e/2 23.05,66 2034 f/24 Kodak 0.250 Plate 0.7 3.4 3e/2,4b 23.05.66 2036 1/24 Kodak 0.250 Plate 0.7 3.4 16e 28.05.66 2122 1/30 IIford G.30 Plole 0.8 8.4 140 29.05.66 2103 1/30 IIford G.30 Plate 0.8 9.4 2e 23.06.66 2109 f/24 lIford G.30 Pia Ie 1.0 5.0 160 06.08.66 0211 f/30 Illord G.30 Pia Ie 0.7 18.9 2b 06.08.66 0215 1/30 IIford G.30 Plale 0.7 18.9 lb, 13b 09.08.66 0315 1/30 IIlord G.30 Plate 1.1 23.8 50,60 09.08.66 03 17 1/30 Ilford G.30 Plate 1.1 23.8 90, 91/2, 11 b, 12e/l 06.
    [Show full text]
  • Planetary Science : a Lunar Perspective
    APPENDICES APPENDIX I Reference Abbreviations AJS: American Journal of Science Ancient Sun: The Ancient Sun: Fossil Record in the Earth, Moon and Meteorites (Eds. R. 0.Pepin, et al.), Pergamon Press (1980) Geochim. Cosmochim. Acta Suppl. 13 Ap. J.: Astrophysical Journal Apollo 15: The Apollo 1.5 Lunar Samples, Lunar Science Insti- tute, Houston, Texas (1972) Apollo 16 Workshop: Workshop on Apollo 16, LPI Technical Report 81- 01, Lunar and Planetary Institute, Houston (1981) Basaltic Volcanism: Basaltic Volcanism on the Terrestrial Planets, Per- gamon Press (1981) Bull. GSA: Bulletin of the Geological Society of America EOS: EOS, Transactions of the American Geophysical Union EPSL: Earth and Planetary Science Letters GCA: Geochimica et Cosmochimica Acta GRL: Geophysical Research Letters Impact Cratering: Impact and Explosion Cratering (Eds. D. J. Roddy, et al.), 1301 pp., Pergamon Press (1977) JGR: Journal of Geophysical Research LS 111: Lunar Science III (Lunar Science Institute) see extended abstract of Lunar Science Conferences Appendix I1 LS IV: Lunar Science IV (Lunar Science Institute) LS V: Lunar Science V (Lunar Science Institute) LS VI: Lunar Science VI (Lunar Science Institute) LS VII: Lunar Science VII (Lunar Science Institute) LS VIII: Lunar Science VIII (Lunar Science Institute LPS IX: Lunar and Planetary Science IX (Lunar and Plane- tary Institute LPS X: Lunar and Planetary Science X (Lunar and Plane- tary Institute) LPS XI: Lunar and Planetary Science XI (Lunar and Plane- tary Institute) LPS XII: Lunar and Planetary Science XII (Lunar and Planetary Institute) 444 Appendix I Lunar Highlands Crust: Proceedings of the Conference in the Lunar High- lands Crust, 505 pp., Pergamon Press (1980) Geo- chim.
    [Show full text]
  • The Archaeology and Heritage of the Sudanese Red Sea Region: Importance, Findings, and Challenges
    The Archaeology and Heritage of the Sudanese Red Sea Region: Importance, Findings, and Challenges AHMED ADAM Head Department of Archaeology - University of Khartoum Director of the Red Sea Project for Archaeological Research Abstract This paper seeks to shed a high light on the archaeological sites discovered in the area of Suakin, Arkaweet, and Sinkat as a part of the project of the department of Archaeology ß university of Khartoum, so, the archaeological sites discovered in this region belong to different periods such as Pre-Historic, Medieval, Islamic, and others are unknown, which means that the region used to link the Red Sea Cultures with those on the central Sudan and Egypt far north and Eretria in the east. Through this study I am also seeking to evaluate the field work (Archaeological and Ethnographic) conducted in the area of Arkaweet and Sinkat town, and Suakin port, then to put a plan for the managing and protecting the archaeologi- cal sites and ethnographic materials. Therefore I will follow or apply a number of approaches in this study such as description, survey analysis of the sites and its contents as well a comparison will be made between the results of the present study with the results of the previous studies in the field of archeology and ethnography conducted on other sites in the Sudanese Red Sea Region. The historical sources will also be compared with the study findings. Keywords Red Sea, Archaeology, Heritage, Sudan, Survey, Suakin 188 1. INTRODUCTION The Red Sea lies in an ideal geographical location between eastern and west- ern seas in general, and between the Mediterranean Sea and the Indian Ocean in particular.
    [Show full text]
  • 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.
    [Show full text]
  • The Aristarchus Plateau on the Moon: Nature and Stratigraphy of the Substratum
    40th Lunar and Planetary Science Conference (2009) 1234.pdf THE ARISTARCHUS PLATEAU ON THE MOON: NATURE AND STRATIGRAPHY OF THE SUBSTRATUM. S.D. Chevrel1, P.C. Pinet1, Y. Daydou1, S. Le Mouélic2, Y. Langevin3, F. Costard4, S. Erard5 1UMR5562/CNRS, Observatoire Midi Pyrénées,Toulouse, France, 2UMR6112/CNRS, Université de Nantes, France, 3Institut d’Astrophysique Spatiale, Orsay, France, 4UMR 8148/CNRS, Université Paris-Sud, Orsay, France, 5LESIA, Observatoire de Paris, Meudon, France Introduction: The Aristarchus Plateau is one of give a comprehensive description (82% of the image the most complex regions on the Moon. It is an old modeled) of the distribution and amount of surface rectangular elevated crustal block about 170x220 km, mixing of the units present across the Plateau and its with its west and east borders approximately immediate surroundings [3]. concentric The first iteration, involving DMD (pyroclastic to the Imbrium basin, surrounded by younger mare glass-rich dark mantling materials), AER (anorthositic basalts of Oceanus Procellarum (e.g., [1]). The Plateau with clinopyroxene and orthopyroxene), NE shows extensive dark mantling deposits (DMD) of (pyroxene-rich materials) and OL (olivine-rich volcanic pyroclastic origin (e.g., [2]). The Aristarchus materials), describes surface regional mixtures crater (40 km in diameter), which formed at the edge associated with the Plateau setting (substratum, of the Plateau, permits to document the nature and the pyroclastic deposits) (Fig. 2). The second iteration, stratigraphy of the crust in this region of the Moon. involving AER, SC (anorthositic with pyroxene) and Data and analysis: We present here results [3] SW (mare basalt), describes mixtures of mare units from integrated UV-VISNIR (410-2000nm) lying outside the Plateau and ejecta materials from the Clementine spectral reflectance data (i.e.
    [Show full text]
  • Glossary of Lunar Terminology
    Glossary of Lunar Terminology albedo A measure of the reflectivity of the Moon's gabbro A coarse crystalline rock, often found in the visible surface. The Moon's albedo averages 0.07, which lunar highlands, containing plagioclase and pyroxene. means that its surface reflects, on average, 7% of the Anorthositic gabbros contain 65-78% calcium feldspar. light falling on it. gardening The process by which the Moon's surface is anorthosite A coarse-grained rock, largely composed of mixed with deeper layers, mainly as a result of meteor­ calcium feldspar, common on the Moon. itic bombardment. basalt A type of fine-grained volcanic rock containing ghost crater (ruined crater) The faint outline that remains the minerals pyroxene and plagioclase (calcium of a lunar crater that has been largely erased by some feldspar). Mare basalts are rich in iron and titanium, later action, usually lava flooding. while highland basalts are high in aluminum. glacis A gently sloping bank; an old term for the outer breccia A rock composed of a matrix oflarger, angular slope of a crater's walls. stony fragments and a finer, binding component. graben A sunken area between faults. caldera A type of volcanic crater formed primarily by a highlands The Moon's lighter-colored regions, which sinking of its floor rather than by the ejection of lava. are higher than their surroundings and thus not central peak A mountainous landform at or near the covered by dark lavas. Most highland features are the center of certain lunar craters, possibly formed by an rims or central peaks of impact sites.
    [Show full text]
  • User Guide to 1:250,000 Scale Lunar Maps
    CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west.
    [Show full text]
  • Zanzibar: Its History and Its People
    Zanzibar: its history and its people http://www.aluka.org/action/showMetadata?doi=10.5555/AL.CH.DOCUMENT.PUHC025 Use of the Aluka digital library is subject to Aluka’s Terms and Conditions, available at http://www.aluka.org/page/about/termsConditions.jsp. By using Aluka, you agree that you have read and will abide by the Terms and Conditions. Among other things, the Terms and Conditions provide that the content in the Aluka digital library is only for personal, non-commercial use by authorized users of Aluka in connection with research, scholarship, and education. The content in the Aluka digital library is subject to copyright, with the exception of certain governmental works and very old materials that may be in the public domain under applicable law. Permission must be sought from Aluka and/or the applicable copyright holder in connection with any duplication or distribution of these materials where required by applicable law. Aluka is a not-for-profit initiative dedicated to creating and preserving a digital archive of materials about and from the developing world. For more information about Aluka, please see http://www.aluka.org Zanzibar: its history and its people Author/Creator Ingrams, W.H. Publisher Frank Cass & Co., Ltd. Date 1967 Resource type Books Language English Subject Coverage (spatial) Northern Swahili Coast, Tanzania, United Republic of, Zanzibar Stone Town, Tanzania Source Princeton University Library 1855.991.49 Rights By kind permission of Leila Ingrams. Description Contents: Preface; Introductory; Zanzibar; The People; Historical; Early History and External Influences; Visitors from the Far East; The Rise and Fall of the Portuguese; Later History of the Native Tribes; History of Modern Zanzibar.
    [Show full text]
  • The History of the People's of the Eastern Desert
    The History of the Peoples of the Eastern Desert edited by Hans Barnard and Kim Duistermaat Monograph 73 Cotsen Institute of Archaeology University of California, Los Angeles THE COTSEN INSTITUTE OF ARCHAEOLOGY PRESS is the publishing unit of the Cotsen Institute of Archaeology at UCLA. The Cotsen Institute is a premier research organization dedicated to the creation, dissemination, and conservation of archaeological knowledge and heritage. It is home to both the Interdepartmental Archaeology Graduate Program and the UCLA/Getty Master’s Program in the Conservation of Archaeological and Ethnographic Materials. The Cotsen Institute provides a forum for innovative faculty research, graduate education, and public programs at UCLA in an effort to impact positively the academic, local and global communities. Established in 1973, the Cotsen Institute is at the forefront of archaeological research, education, conservation and publication and is an active contributor to interdisciplinary research at UCLA. The Cotsen Institute Press specializes in producing high-quality academic volumes in several different series, including Monographs, World Heritage and Monuments, Cotsen Advanced Seminars, and Ideas, Debates and Perspectives. The Press is committed to making the fruits of archaeological research accessible to professionals, scholars, students, and the general public. We are able to do this through the generosity of Lloyd E. Cotsen, longtime Institute volunteer and benefactor, who has provided an endowment that allows us to subsidize our publishing
    [Show full text]
  • Adams Adkinson Aeschlimann Aisslinger Akkermann
    BUSCAPRONTA www.buscapronta.com ARQUIVO 27 DE PESQUISAS GENEALÓGICAS 189 PÁGINAS – MÉDIA DE 60.800 SOBRENOMES/OCORRÊNCIA Para pesquisar, utilize a ferramenta EDITAR/LOCALIZAR do WORD. A cada vez que você clicar ENTER e aparecer o sobrenome pesquisado GRIFADO (FUNDO PRETO) corresponderá um endereço Internet correspondente que foi pesquisado por nossa equipe. Ao solicitar seus endereços de acesso Internet, informe o SOBRENOME PESQUISADO, o número do ARQUIVO BUSCAPRONTA DIV ou BUSCAPRONTA GEN correspondente e o número de vezes em que encontrou o SOBRENOME PESQUISADO. Número eventualmente existente à direita do sobrenome (e na mesma linha) indica número de pessoas com aquele sobrenome cujas informações genealógicas são apresentadas. O valor de cada endereço Internet solicitado está em nosso site www.buscapronta.com . Para dados especificamente de registros gerais pesquise nos arquivos BUSCAPRONTA DIV. ATENÇÃO: Quando pesquisar em nossos arquivos, ao digitar o sobrenome procurado, faça- o, sempre que julgar necessário, COM E SEM os acentos agudo, grave, circunflexo, crase, til e trema. Sobrenomes com (ç) cedilha, digite também somente com (c) ou com dois esses (ss). Sobrenomes com dois esses (ss), digite com somente um esse (s) e com (ç). (ZZ) digite, também (Z) e vice-versa. (LL) digite, também (L) e vice-versa. Van Wolfgang – pesquise Wolfgang (faça o mesmo com outros complementos: Van der, De la etc) Sobrenomes compostos ( Mendes Caldeira) pesquise separadamente: MENDES e depois CALDEIRA. Tendo dificuldade com caracter Ø HAMMERSHØY – pesquise HAMMERSH HØJBJERG – pesquise JBJERG BUSCAPRONTA não reproduz dados genealógicos das pessoas, sendo necessário acessar os documentos Internet correspondentes para obter tais dados e informações. DESEJAMOS PLENO SUCESSO EM SUA PESQUISA.
    [Show full text]
  • January 2021 Click on Images in This Issue for Hyperlinks
    A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Back issues: http://www.alpo-astronomy.org/ Online readers, January 2021 click on images In This Issue for hyperlinks Announcements 2 Lunar Calendar October 2020 3 An Invitation to Join ALPO 3 Observations Received 4 By the Numbers 6 Submission Through the ALPO Image Achieve 7 When Submitting Observations to the ALPO Lunar Section 8 page 83 Call For Observations Focus-On 8 Focus-On Announcement 9 Schickard Sunrise Patch, S. Berté 10 Another Dome Home, R. Hill 11 Some Wonders on the Shores of Mare Crisium, A. Anunziato 12 Lunar Topographic Studies Program: Banded Craters 14 A Fleet Vision of Posidonius Y on Dorsa Smirnov, A. Anunziato 20 Aristarchus Plateau Region, H. Eskildsen 21 Focus On: The Lunar 100, Features 41-50, J. Hubbell 22 Lunar 41-50, a Personal View, A. Anunziato 25 Wargentin, R. Hays, Jr. 37 Recent Topographic Studies 79 Lunar Geologic Change Detection Program, T. Cook 119 page 84 Key to Images in this Issue 131 A very Happy New Year to all. We look forward to a good year ahead. Thank you contributors for your many contributions to this issue of The Lunar Observer. Your excellent submissions is what makes this newsletter possible. If you are reading this issue, welcome aboard! Perhaps you would like to contribute your own lunar observations to us. You can contribute observations if you are not a member of ALPO, but we sure would like you to consider becoming a member (yearly rates start at only $18.00, a great deal!).
    [Show full text]