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1 En Petkovic
Scientific paper Creation and Analysis of the Yugoslav Rock Song Lyrics Corpus from 1967 to 20031 UDC 811.163.41’322 DOI 10.18485/infotheca.2019.19.1.1 Ljudmila Petkovi´c ABSTRACT: The paper analyses the pro- [email protected] cess of creation and processing of the Yu- University of Belgrade goslav rock song lyrics corpus from 1967 to Belgrade, Serbia 2003, from the theoretical and practical per- spective. The data have been obtained and XML-annotated using the Python program- ming language and the libraries lyricsmas- ter/yattag. The corpus has been preprocessed and basic statistical data have been gener- ated by the XSL transformation. The diacritic restoration has been carried out in the Slovo Majstor and LeXimir tools (the latter appli- cation has also been used for generating the frequency analysis). The extraction of socio- cultural topics has been performed using the Unitex software, whereas the prevailing top- ics have been visualised with the TreeCloud software. KEYWORDS: corpus linguistics, Yugoslav rock and roll, web scraping, natural language processing, text mining. PAPER SUBMITTED: 15 April 2019 PAPER ACCEPTED: 19 June 2019 1 This paper originates from the author’s Master’s thesis “Creation and Analysis of the Yugoslav Rock Song Lyrics Corpus from 1945 to 2003”, which was defended at the University of Belgrade on March 18, 2019. The thesis was conducted under the supervision of the Prof. Dr Ranka Stankovi´c,who contributed to the topic’s formulation, with the remark that the year of 1945 was replaced by the year of 1967 in this paper. -
Tomma Abts Francis Alÿs Mamma Andersson Karla Black Michaël
Tomma Abts 2015 Books Zwirner David Francis Alÿs Mamma Andersson Karla Black Michaël Borremans Carol Bove R. Crumb Raoul De Keyser Philip-Lorca diCorcia Stan Douglas Marlene Dumas Marcel Dzama Dan Flavin Suzan Frecon Isa Genzken Donald Judd On Kawara Toba Khedoori Jeff Koons Yayoi Kusama Kerry James Marshall Gordon Matta-Clark John McCracken Oscar Murillo Alice Neel Jockum Nordström Chris Ofili Palermo Raymond Pettibon Neo Rauch Ad Reinhardt Jason Rhoades Michael Riedel Bridget Riley Thomas Ruff Fred Sandback Jan Schoonhoven Richard Serra Yutaka Sone Al Taylor Diana Thater Wolfgang Tillmans Luc Tuymans James Welling Doug Wheeler Christopher Williams Jordan Wolfson Lisa Yuskavage David Zwirner Books Recent and Forthcoming Publications No Problem: Cologne/New York – Bridget Riley: The Stripe Paintings – Yayoi Kusama: I Who Have Arrived In Heaven Jeff Koons: Gazing Ball Ad Reinhardt Ad Reinhardt: How To Look: Art Comics Richard Serra: Early Work Richard Serra: Vertical and Horizontal Reversals Jason Rhoades: PeaRoeFoam John McCracken: Works from – Donald Judd Dan Flavin: Series and Progressions Fred Sandback: Decades On Kawara: Date Paintings in New York and Other Cities Alice Neel: Drawings and Watercolors – Who is sleeping on my pillow: Mamma Andersson and Jockum Nordström Kerry James Marshall: Look See Neo Rauch: At the Well Raymond Pettibon: Surfers – Raymond Pettibon: Here’s Your Irony Back, Political Works – Raymond Pettibon: To Wit Jordan Wolfson: California Jordan Wolfson: Ecce Homo / le Poseur Marlene -
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2019 Asteroid Regolith Weathering: A Large-Scale Observational Investigation Eric Michael MacLennan University of Tennessee, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Recommended Citation MacLennan, Eric Michael, "Asteroid Regolith Weathering: A Large-Scale Observational Investigation. " PhD diss., University of Tennessee, 2019. https://trace.tennessee.edu/utk_graddiss/5467 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Eric Michael MacLennan entitled "Asteroid Regolith Weathering: A Large-Scale Observational Investigation." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Geology. Joshua P. Emery, Major Professor We have read this dissertation and recommend its acceptance: Jeffrey E. Moersch, Harry Y. McSween Jr., Liem T. Tran Accepted for the Council: Dixie L. Thompson Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Asteroid Regolith Weathering: A Large-Scale Observational Investigation A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Eric Michael MacLennan May 2019 © by Eric Michael MacLennan, 2019 All Rights Reserved. -
N Arieuican%Mllsellm
n ARieuican%Mllsellm PUBLISHED BY THE AMERICAN MUSEUM OF NATURAL HISTORY CENTRAL PARK WEST AT 79TH STREET, NEW YORK 24, N.Y. NUMBER 2I63 DECEMBER I9, I963 The Pallasites BY BRIAN MASON' INTRODUCTION The pallasites are a comparatively rare type of meteorite, but are remarkable in several respects. Historically, it was a pallasite for which an extraterrestrial origin was first postulated because of its unique compositional and structural features. The Krasnoyarsk pallasite was discovered in 1749 about 150 miles south of Krasnoyarsk, and seen by P. S. Pallas in 1772, who recognized these unique features and arranged for its removal to the Academy of Sciences in St. Petersburg. Chladni (1794) examined it and concluded it must have come from beyond the earth, at a time when the scientific community did not accept the reality of stones falling from the sky. Compositionally, the combination of olivine and nickel-iron in subequal amounts clearly distinguishes the pallasites from all other groups of meteorites, and the remarkable juxtaposition of a comparatively light silicate mineral and heavy metal poses a nice problem of origin. Several theories of the internal structure of the earth have postulated the presence of a pallasitic layer to account for the geophysical data. No apology is therefore required for an attempt to provide a comprehensive account of this remarkable group of meteorites. Some 40 pallasites are known, of which only two, Marjalahti and Zaisho, were seen to fall (table 1). Of these, some may be portions of a single meteorite. It has been suggested that the pallasite found in Indian mounds at Anderson, Ohio, may be fragments of the Brenham meteorite, I Chairman, Department of Mineralogy, the American Museum of Natural History. -
Meteorite Collections: Sample List
Meteorite Collections: Sample List Institute of Meteoritics Department of Earth and Planetary Sciences University of New Mexico October 01, 2021 Institute of Meteoritics Meteorite Collection The IOM meteorite collection includes samples from approximately 600 different meteorites, representative of most meteorite types. The last printed copy of the collection's Catalog was published in 1990. We will no longer publish a printed catalog, but instead have produced this web-based Online Catalog, which presents the current catalog in searchable and downloadable forms. The database will be updated periodically. The date on the front page of this version of the catalog is the date that it was downloaded from the worldwide web. The catalog website is: Although we have made every effort to avoid inaccuracies, the database may still contain errors. Please contact the collection's Curator, Dr. Rhian Jones, ([email protected]) if you have any questions or comments. Cover photos: Top left: Thin section photomicrograph of the martian shergottite, Zagami (crossed nicols). Brightly colored crystals are pyroxene; black material is maskelynite (a form of plagioclase feldspar that has been rendered amorphous by high shock pressures). Photo is 1.5 mm across. (Photo by R. Jones.) Top right: The Pasamonte, New Mexico, eucrite (basalt). This individual stone is covered with shiny black fusion crust that formed as the stone fell through the earth's atmosphere. Photo is 8 cm across. (Photo by K. Nicols.) Bottom left: The Dora, New Mexico, pallasite. Orange crystals of olivine are set in a matrix of iron, nickel metal. Photo is 10 cm across. (Photo by K. -
Domaće Popularne, Zabavne, Strane I Rok Pesme
DOMAĆE POPULARNE, ZABAVNE, STRANE I ROK PESME: o Aerodrom – Obična ljubavna pesma o Ambasadori – Dođi u 5 do 5 o Apsolutno Romantično – Đoletova pesma o Atomsko Sklonište – Olujni Mornar o Atomsko Sklonište – Pakleni vozači o Atomsko Sklonište – Za ljubav treba imat dušu o Azra – Balkan o Azra – Usne vrele višnje o Azra – Voljela me nijedna o Babe – Ko me ter’o o Babe – Noć bez sna o Baby Doll – Brazil o Bajaga – 220 u voltima o Bajaga – Godine prolaze o Bajaga – Moji su drugovi o Bajaga – Na vrhovima prstiju o Bajaga – Ti se ljubiš tako dobro o Bajaga – Tišina o Bajaga – Vratiće se rode o Bijelo Dugme – A i ti me iznevjeri o Bijelo Dugme – Ako ima Boga o Bijelo Dugme – Đurđevdan o Bijelo Dugme – Esma o Bijelo Dugme – Lažeš o Bijelo Dugme – Lipe cvatu o Bijelo Dugme – Na zadnjem sedištu moga auta o Bijelo Dugme – Napile se ulice o Bijelo Dugme – Padaju zvijezde o Bijelo Dugme – Pljuni i zapjevaj o Bijelo Dugme – Ružica si bila o Bijelo Dugme – Tako ti je mala moja kad ljubi o Boris Režak – Anđeo o Colonia – Ti da bu di bu da o Crvena Jabuka – Bacila je sve niz rijeku o Crvena Jabuka – Da nije ljubavi o Crvena Jabuka – Dirlija o Crvena Jabuka – Moje najmilije o Crvena Jabuka – Nekako s prolijeća o Crvena Jabuka – Stižu me sjećanja o Crvena Jabuka – Tamo gdje ljubav počinje o Crvena Jabuka – To mi radi o Crvena Jabuka – Tuga, ti i ja o Crvena Jabuka – Volio bi da si tu o Crvena Jabuka – Zovu nas ulice o Čutura – Voli me o Darko Domijan – Ulica jorgovana o Dado Topić I Slađana Milošević – Princeza o Dejan Cukić – Milica o Dejan Cukić – Nebo -
New Europe College Ştefan Odobleja Program Yearbook 2012-2013
New Europe College Ştefan Odobleja Program Yearbook 2012-2013 CONSTANTIN ARDELEANU CRISTIAN CERCEL ALEX CISTELECAN COSTIN MOISIL RALUCA MUŞAT MARIUS STAN IOAN ALEXANDRU TOFAN RĂZVAN VONCU Editor: Irina Vainovski-Mihai Copyright – New Europe College ISSN 1584-0298 New Europe College Str. Plantelor 21 023971 Bucharest Romania www.nec.ro; e-mail: [email protected] Tel. (+4) 021.307.99.10, Fax (+4) 021. 327.07.74 RĂZVAN VONCU Born in 1969 Ph.D., University of Bucharest, 2006 Thesis: Confessive Narrative in Romanian Medieval Literature Senior Lecturer, University of Bucharest, Faculty of Letters, Department of Literary Studies Scholarship of Open Society Foundation – Bulgarian and Balkanology Studies, Bansko – Blagoevgrad, Bulgaria (1993) Scholarship at “St. Kliment Ohridski” University of Sofia – Studies of Bulgarian Language and Literature (1990) Papers delivered at conferences in Romania, Serbia, Republic of Moldova Numerous articles published on Literary Studies, Balkan Studies, Cultural Studies Published three translated books (from Italian and Serbian) Author of 16 books among which: Secvenţe literare contemporane (Contemporary Literary Fragments), I, Viitorul Românesc, Bucharest, 2001 Secvenţe literare contemporane (Contemporary Literary Fragments), II, Viitorul Românesc, Bucharest, 2002 Orizonturi medievale (Medieval Horizons), Artemis, Bucharest, 2003 Despre Preda şi alte eseuri neconvenţionale (On Preda and Other Unconventional Essays), Semne, Bucharest, 2003 Eseuri critice (Critical Essays), Ed. Muzeului Naţional al Literaturii Române, -
(2000) Forging Asteroid-Meteorite Relationships Through Reflectance
Forging Asteroid-Meteorite Relationships through Reflectance Spectroscopy by Thomas H. Burbine Jr. B.S. Physics Rensselaer Polytechnic Institute, 1988 M.S. Geology and Planetary Science University of Pittsburgh, 1991 SUBMITTED TO THE DEPARTMENT OF EARTH, ATMOSPHERIC, AND PLANETARY SCIENCES IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN PLANETARY SCIENCES AT THE MASSACHUSETTS INSTITUTE OF TECHNOLOGY FEBRUARY 2000 © 2000 Massachusetts Institute of Technology. All rights reserved. Signature of Author: Department of Earth, Atmospheric, and Planetary Sciences December 30, 1999 Certified by: Richard P. Binzel Professor of Earth, Atmospheric, and Planetary Sciences Thesis Supervisor Accepted by: Ronald G. Prinn MASSACHUSES INSTMUTE Professor of Earth, Atmospheric, and Planetary Sciences Department Head JA N 0 1 2000 ARCHIVES LIBRARIES I 3 Forging Asteroid-Meteorite Relationships through Reflectance Spectroscopy by Thomas H. Burbine Jr. Submitted to the Department of Earth, Atmospheric, and Planetary Sciences on December 30, 1999 in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Planetary Sciences ABSTRACT Near-infrared spectra (-0.90 to ~1.65 microns) were obtained for 196 main-belt and near-Earth asteroids to determine plausible meteorite parent bodies. These spectra, when coupled with previously obtained visible data, allow for a better determination of asteroid mineralogies. Over half of the observed objects have estimated diameters less than 20 k-m. Many important results were obtained concerning the compositional structure of the asteroid belt. A number of small objects near asteroid 4 Vesta were found to have near-infrared spectra similar to the eucrite and howardite meteorites, which are believed to be derived from Vesta. -
Meteorite Collections: Catalog
Meteorite Collections: Catalog Institute of Meteoritics Department of Earth and Planetary Sciences University of New Mexico July 25, 2011 Institute of Meteoritics Meteorite Collection The IOM meteorite collection includes samples from approximately 600 different meteorites, representative of most meteorite types. The last printed copy of the collection's Catalog was published in 1990. We will no longer publish a printed catalog, but instead have produced this web-based Online Catalog, which presents the current catalog in searchable and downloadable forms. The database will be updated periodically. The date on the front page of this version of the catalog is the date that it was downloaded from the worldwide web. The catalog website is: Although we have made every effort to avoid inaccuracies, the database may still contain errors. Please contact the collection's Curator, Dr. Rhian Jones, ([email protected]) if you have any questions or comments. Cover photos: Top left: Thin section photomicrograph of the martian shergottite, Zagami (crossed nicols). Brightly colored crystals are pyroxene; black material is maskelynite (a form of plagioclase feldspar that has been rendered amorphous by high shock pressures). Photo is 1.5 mm across. (Photo by R. Jones.) Top right: The Pasamonte, New Mexico, eucrite (basalt). This individual stone is covered with shiny black fusion crust that formed as the stone fell through the earth's atmosphere. Photo is 8 cm across. (Photo by K. Nicols.) Bottom left: The Dora, New Mexico, pallasite. Orange crystals of olivine are set in a matrix of iron, nickel metal. Photo is 10 cm across. (Photo by K. -
Meteorite Auction - Macovich Collection
Meteorite Auction - Macovich Collection HOME l INTRO TO MACOVICH l METEORITES FOR SALE l MEDIA INFO l CONTACT US THE MACOVICH METEORITE AUCTION Sunday February 9, 2003 10:30 A.M. at the InnSuites — Courtyard Terrace 475 North Granada, Tucson (520) 622-3000 Previews & In-person Registration February 1 – February 9 (10:30AM – 6 PM) February 9 (9:30AM – 10:30AM) Room 404 at the InnSuites Hotel AUCTION NOTES You must register to participate. Dimensions of lots are approximate. There is a 12.5% buyer's commission on all lots. Low and high estimates are merely a guideline. Witnessed falls are denoted by an asterisk. A bullet to the left of the lot number indicates that the specimen carries a reserve. Meteorites of a more decorative or sculptural nature are designated by a green box around the lot number. LOT NAME DATE OF WEIGHT & TKW LOCALITY DESCRIPTION ESTIMATE # TYPE FALL/FIND DIMENSIONS CLICK ON METEORITE NAME TO VIEW IMAGE AND DESCRIPTION Naiman* Naiman Cnty, Encrusted fragment of an extremely difficult to obtain meteorite; 12.55 g 1 May/26/1982 1.05 Kg $150 – $250 L6 Mongolia Purple Mountain Observatory provenance 27 x 28 x 14 Kilabo* Complete specimen of Earth's most recent meteorite recovery 83.20 g 2 July/21/2002 ~24 Kg Hadejia, Nigeria $600 – $750 LL6 to date; ~90% fusion crust 48 x 35 x 35 Highly brecciated thin quarter slice of this much sought–after Honolulu* 1.99 g 3 Sep/27/1825 ~3 Kg Oahu, Hawaii meteorite; with fusion crust; Finnish Geological Museum $250 – $350 L5 27 x 21 x 1 provenance Partial slice; the most famous meteorite/auto -
Guillaume Bijl
GUILLAUME BIJL Born in Antwerp, Belgium in 1946. Lives and works in Antwerp, Belgium. SOLO SHOWS (a selection) : 2019 Collection presentation: 40 years installations (celebration) 1979 – 2019, M HKA, Antwerp, Belgium Guillaume Bijl presents Fraikin, art Center Hugo Voeten, Herentals, Belgium Zwin Natuur Park, Knokke-Heist, Belgium Compositions & Sorry’s, J. Allen Gallery, Paris, France Dogsalon ‘Daisy’, Pinkie Bowtie, Antwerp, Belgium Bruegelfeest in de Ponderosa, Dilbeek, Belgium 2018 Art’s Birthday, M HKA, Antwerp, Belgium Adriaen Brouwer Installation, Ronde van Vlaanderen Museum, Oudenaarde, Belgium Felicien Rops Installation, Musée Félicien Rops, Namur, Belgium 2017 Walk of Fame, Middelburg, The Netherlands Matrass Discount, ADNplatform, Barcelona, Spain PXL Mad Campus, Hasselt, Belgium The Politician = a Transformation - Installation, Mengi, Iceland 2016 Cultuurcentrum Mechelen, Mechelen, Belgium Dog Salon Bobby, Grieder Contemporary, MANIFESTA 11, Zürich, Switzerland Galerie Nagel Draxler, Berlin, Germany Galleri Nicolai Wallner, Copenhagen, Denmark Sculptures, Compositions & Sorries, KETELEER Gallery, Antwerp, Belgium Sorry, Le Carré – Scène nationale et Centre d’Art contemporain du pays de Château-Gontier, Château-Gontier, France 2014 Compositions, Lumen Trevor Gallery, Amsterdam, The Netherlands 2013 Chateau des Adhemar - centre d’art contemporain, Montelimar, France 2012 Compositions Trouvées, Galerie Christian Nagel, Berlin, Germany Extra Hair Shop, etablissement d’en face projects, Brussels, Belgium Galerie Hubert Winter, -
The Physical Propermes of Near Earth Asteroids
The Physical Properes of Near Earth Asteroids Dan Bri University of Central Florida What Do We Need to Know About NEA Physical Proper/es? • Asteroid Structure – Rubble pile? – Coherent object? • Material Strength – Tough? Weak? • Mineralogy • Thermal Properes • Surface texture – Dusty regolith? – Boulder field? Sources of Data • Meteorites – Strong? Weak? • Observaons of Bolides • Meteorite Strewnfields • Observaons of NEAs – Rota/on rates – Binaries • Physics – Microgravity – Cohesion – Thermal cycles Lets Start with Meteorites Meteorite Types • Chondrites (ordinary, enstatite) – Stones, chondrules, olivine, pyroxene, metal, sulfides, usually strong • Volatile-rich Carbonaceous Chondrites (CI, CM) Farmington (L5) Farmville (H4) – Hydrated silicates, carbon compounds, refractory grains, very weak. • Other Carbonaceous (CO, CV, CK, CR, CH) – Highly variable, chondules, refractory grains, often as strong as ordinary Allende (CV3) chondrites • Achondrites – Igneous rocks from partial melts or melt residues Bununu (Howardite) • Irons – Almost all FeNi metal Thiel Mountains (pallasite) • Stony-irons Cape York (IIIAB) – Mix of silicates and metal Meteorite Density Meteorite Compressive Strength Material Meteorite Type Compressive Strength (MPa) Concrete (Unreinforced) Typical Sidewalk 20 (3000 psi) Charcoal Briquee ~2 Granite 100–140 Medium dirt clod 0.2-0.4 La Lande, NM L5 373.4 Tsarev L5 160-420 Covert (porosity 13%) H5 75.3 Krymka LL3 160 Seminole H4 173 Holbrook, AZ (porosity 11%) L6 6.2 Tagish Lake C2 0.25-1.2 Murchison CM ~50 Bolides ? 0.1-1