An Astro-Archaeological Analysis
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The Conditions of Dramatic Production to the Death of Aeschylus Hammond, N G L Greek, Roman and Byzantine Studies; Winter 1972; 13, 4; Proquest Pg
The Conditions of Dramatic Production to the Death of Aeschylus Hammond, N G L Greek, Roman and Byzantine Studies; Winter 1972; 13, 4; ProQuest pg. 387 The Conditions of Dramatic Production to the Death of Aeschylus N. G. L. Hammond TUDENTS of ancient history sometimes fall into the error of read Sing their history backwards. They assume that the features of a fully developed institution were already there in its earliest form. Something similar seems to have happened recently in the study of the early Attic theatre. Thus T. B. L. Webster introduces his excellent list of monuments illustrating tragedy and satyr-play with the following sentences: "Nothing, except the remains of the old Dionysos temple, helps us to envisage the earliest tragic background. The references to the plays of Aeschylus are to the lines of the Loeb edition. I am most grateful to G. S. Kirk, H. D. F. Kitto, D. W. Lucas, F. H. Sandbach, B. A. Sparkes and Homer Thompson for their criticisms, which have contributed greatly to the final form of this article. The students of the Classical Society at Bristol produce a Greek play each year, and on one occasion they combined with the boys of Bristol Grammar School and the Cathedral School to produce Aeschylus' Oresteia; they have made me think about the problems of staging. The following abbreviations are used: AAG: The Athenian Agora, a Guide to the Excavation and Museum! (Athens 1962). ARNon, Conventions: P. D. Arnott, Greek Scenic Conventions in the Fifth Century B.C. (Oxford 1962). BIEBER, History: M. Bieber, The History of the Greek and Roman Theatre2 (Princeton 1961). -
LCROSS (Lunar Crater Observation and Sensing Satellite) Observation Campaign: Strategies, Implementation, and Lessons Learned
Space Sci Rev DOI 10.1007/s11214-011-9759-y LCROSS (Lunar Crater Observation and Sensing Satellite) Observation Campaign: Strategies, Implementation, and Lessons Learned Jennifer L. Heldmann · Anthony Colaprete · Diane H. Wooden · Robert F. Ackermann · David D. Acton · Peter R. Backus · Vanessa Bailey · Jesse G. Ball · William C. Barott · Samantha K. Blair · Marc W. Buie · Shawn Callahan · Nancy J. Chanover · Young-Jun Choi · Al Conrad · Dolores M. Coulson · Kirk B. Crawford · Russell DeHart · Imke de Pater · Michael Disanti · James R. Forster · Reiko Furusho · Tetsuharu Fuse · Tom Geballe · J. Duane Gibson · David Goldstein · Stephen A. Gregory · David J. Gutierrez · Ryan T. Hamilton · Taiga Hamura · David E. Harker · Gerry R. Harp · Junichi Haruyama · Morag Hastie · Yutaka Hayano · Phillip Hinz · Peng K. Hong · Steven P. James · Toshihiko Kadono · Hideyo Kawakita · Michael S. Kelley · Daryl L. Kim · Kosuke Kurosawa · Duk-Hang Lee · Michael Long · Paul G. Lucey · Keith Marach · Anthony C. Matulonis · Richard M. McDermid · Russet McMillan · Charles Miller · Hong-Kyu Moon · Ryosuke Nakamura · Hirotomo Noda · Natsuko Okamura · Lawrence Ong · Dallan Porter · Jeffery J. Puschell · John T. Rayner · J. Jedadiah Rembold · Katherine C. Roth · Richard J. Rudy · Ray W. Russell · Eileen V. Ryan · William H. Ryan · Tomohiko Sekiguchi · Yasuhito Sekine · Mark A. Skinner · Mitsuru Sôma · Andrew W. Stephens · Alex Storrs · Robert M. Suggs · Seiji Sugita · Eon-Chang Sung · Naruhisa Takatoh · Jill C. Tarter · Scott M. Taylor · Hiroshi Terada · Chadwick J. Trujillo · Vidhya Vaitheeswaran · Faith Vilas · Brian D. Walls · Jun-ihi Watanabe · William J. Welch · Charles E. Woodward · Hong-Suh Yim · Eliot F. Young Received: 9 October 2010 / Accepted: 8 February 2011 © The Author(s) 2011. -
Agorapicbk-17.Pdf
Excavations of the Athenian Agora Picture Book No. 17 Prepared by Mabel L. Lang Dedicated to Eugene Vanderpool o American School of Classical Studies at Athens ISBN 87661-617-1 Produced by the Meriden Gravure Company Meriden, Connecticut COVER: Bone figure of Socrates TITLE PAGE: Hemlock SOCRATES IN THE AGORA AMERICAN SCHOOL OF CLASSICAL STUDIES AT ATHENS PRINCETON, NEW JERSEY 1978 ‘Everything combines to make our knowledge of Socrates himself a subject of Socratic irony. The only thing we know definitely about him is that we know nothing.’ -L. Brunschvicg As FAR AS we know Socrates himselfwrote nothing, yet not only were his life and words given dramatic attention in his own time in the Clouds of Ar- istophanes, but they have also become the subject of many others’ writing in the centuries since his death. Fourth-century B.C. writers who had first-hand knowledge of him composed either dialogues in which he was the dominant figure (Plato and Aeschines) or memories of his teaching and activities (Xe- nophon). Later authors down even to the present day have written numerous biographies based on these early sources and considering this most protean of philosophers from every possible point of view except perhaps the topograph- ical one which is attempted here. Instead of putting Socrates in the context of 5th-century B.C. philosophy, politics, ethics or rhetoric, we shall look to find him in the material world and physical surroundings of his favorite stamping- grounds, the Athenian Agora. Just as ‘agora’ in its original sense meant ‘gathering place’ but came in time to mean ‘market place’, so the agora itself was originally a gathering place I. -
Alexander Jones Calendrica I: New Callippic Dates
ALEXANDER JONES CALENDRICA I: NEW CALLIPPIC DATES aus: Zeitschrift für Papyrologie und Epigraphik 129 (2000) 141–158 © Dr. Rudolf Habelt GmbH, Bonn 141 CALENDRICA I: NEW CALLIPPIC DATES 1. Introduction. Callippic dates are familiar to students of Greek chronology, even though up to the present they have been known to occur only in a single source, Ptolemy’s Almagest (c. A.D. 150).1 Ptolemy’s Callippic dates appear in the context of discussions of astronomical observations ranging from the early third century B.C. to the third quarter of the second century B.C. In the present article I will present new attestations of Callippic dates which extend the period of the known use of this system by almost two centuries, into the middle of the first century A.D. I also take the opportunity to attempt a fresh examination of what we can deduce about the Callippic calendar and its history, a topic that has lately been the subject of quite divergent treatments. The distinguishing mark of a Callippic date is the specification of the year by a numbered “period according to Callippus” and a year number within that period. Each Callippic period comprised 76 years, and year 1 of Callippic Period 1 began about midsummer of 330 B.C. It is an obvious, and very reasonable, supposition that this convention for counting years was instituted by Callippus, the fourth- century astronomer whose revisions of Eudoxus’ planetary theory are mentioned by Aristotle in Metaphysics Λ 1073b32–38, and who also is prominent among the authorities cited in astronomical weather calendars (parapegmata).2 The point of the cycles is that 76 years contain exactly four so-called Metonic cycles of 19 years. -
Stoa Poikile) Built About 475-450 BC
Arrangement Classical Greek cities – either result of continuous growth, or created at a single moment. Former – had streets –lines of communication, curving, bending- ease gradients. Later- had grid plans – straight streets crossing at right angles- ignoring obstacles became stairways where gradients were too steep. Despite these differences, certain features and principles of arrangement are common to both. Greek towns Towns had fixed boundaries. In 6th century BC some were surrounded by fortifications, later became more frequent., but even where there were no walls - demarcation of interior and exterior was clear. In most Greek towns availability of area- devoted to public use rather than private use. Agora- important gathering place – conveniently placed for communication and easily accessible from all directions. The Agora Of Athens • Agora originally meant "gathering place" but came to mean the market place and public square in an ancient Greek city. It was the political, civic, and commercial center of the city, near which were stoas, temples, administrative & public buildings, market places, monuments, shrines etc. • The agora in Athens had private housing, until it was reorganized by Peisistratus in the 6th century BC. • Although he may have lived on the agora himself, he removed the other houses, closed wells, and made it the centre of Athenian government. • He also built a drainage system, fountains and a temple to the Olympian gods. • Cimon later improved the agora by constructing new buildings and planting trees. • In the 5th century BC there were temples constructed to Hephaestus, Zeus and Apollo. • The Areopagus and the assembly of all citizens met elsewhere in Athens, but some public meetings, such as those to discuss ostracism, were held in the agora. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
Entrance Pupil Irradiance Estimating Model for a Moon-Based Earth Radiation Observatory Instrument
remote sensing Article Entrance Pupil Irradiance Estimating Model for a Moon-Based Earth Radiation Observatory Instrument Wentao Duan 1, Shaopeng Huang 2,3,* and Chenwei Nie 4 1 School of Human Settlements and Civil Engineering, Xi’an Jiaotong University, Xi’an 710054, China; [email protected] 2 Institute of Deep Earth Science and Green Energy, Shenzhen University, Shenzhen 518060, China 3 Department of Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI 48109, USA 4 Key Laboratory of Digital Earth Science, Institute of Remote Sensing and Digital Earth, Chinese Academy of Sciences, Beijing 100094, China; [email protected] * Correspondence: [email protected] Received: 26 January 2019; Accepted: 6 March 2019; Published: 10 March 2019 Abstract: A Moon-based Earth radiation observatory (MERO) could provide a longer-term continuous measurement of radiation exiting the Earth system compared to current satellite-based observatories. In order to parameterize the detector for such a newly-proposed MERO, the evaluation of the instrument’s entrance pupil irradiance (EPI) is of great importance. The motivation of this work is to build an EPI estimating model for a simplified single-pixel MERO instrument. The rationale of this model is to sum the contributions of every location in the MERO-viewed region on the Earth’s top of atmosphere (TOA) to the MERO sensor’s EPI, taking into account the anisotropy in the longwave radiance at the Earth TOA. Such anisotropy could be characterized by the TOA anisotropic factors, which can be derived from the Clouds and the Earth’s Radiant Energy System (CERES) angular distribution models (ADMs). -
The British Astronomical Association Handbook 2017
THE HANDBOOK OF THE BRITISH ASTRONOMICAL ASSOCIATION 2017 2016 October ISSN 0068–130–X CONTENTS PREFACE . 2 HIGHLIGHTS FOR 2017 . 3 CALENDAR 2017 . 4 SKY DIARY . .. 5-6 SUN . 7-9 ECLIPSES . 10-15 APPEARANCE OF PLANETS . 16 VISIBILITY OF PLANETS . 17 RISING AND SETTING OF THE PLANETS IN LATITUDES 52°N AND 35°S . 18-19 PLANETS – EXPLANATION OF TABLES . 20 ELEMENTS OF PLANETARY ORBITS . 21 MERCURY . 22-23 VENUS . 24 EARTH . 25 MOON . 25 LUNAR LIBRATION . 26 MOONRISE AND MOONSET . 27-31 SUN’S SELENOGRAPHIC COLONGITUDE . 32 LUNAR OCCULTATIONS . 33-39 GRAZING LUNAR OCCULTATIONS . 40-41 MARS . 42-43 ASTEROIDS . 44 ASTEROID EPHEMERIDES . 45-50 ASTEROID OCCULTATIONS .. ... 51-53 ASTEROIDS: FAVOURABLE OBSERVING OPPORTUNITIES . 54-56 NEO CLOSE APPROACHES TO EARTH . 57 JUPITER . .. 58-62 SATELLITES OF JUPITER . .. 62-66 JUPITER ECLIPSES, OCCULTATIONS AND TRANSITS . 67-76 SATURN . 77-80 SATELLITES OF SATURN . 81-84 URANUS . 85 NEPTUNE . 86 TRANS–NEPTUNIAN & SCATTERED-DISK OBJECTS . 87 DWARF PLANETS . 88-91 COMETS . 92-96 METEOR DIARY . 97-99 VARIABLE STARS (RZ Cassiopeiae; Algol; λ Tauri) . 100-101 MIRA STARS . 102 VARIABLE STAR OF THE YEAR (T Cassiopeiæ) . .. 103-105 EPHEMERIDES OF VISUAL BINARY STARS . 106-107 BRIGHT STARS . 108 ACTIVE GALAXIES . 109 TIME . 110-111 ASTRONOMICAL AND PHYSICAL CONSTANTS . 112-113 INTERNET RESOURCES . 114-115 GREEK ALPHABET . 115 ACKNOWLEDGEMENTS / ERRATA . 116 Front Cover: Northern Lights - taken from Mount Storsteinen, near Tromsø, on 2007 February 14. A great effort taking a 13 second exposure in a wind chill of -21C (Pete Lawrence) British Astronomical Association HANDBOOK FOR 2017 NINETY–SIXTH YEAR OF PUBLICATION BURLINGTON HOUSE, PICCADILLY, LONDON, W1J 0DU Telephone 020 7734 4145 PREFACE Welcome to the 96th Handbook of the British Astronomical Association. -
Vasemania: Neoclassical Form and Ornament
VOLUME: 4 WINTER, 2004 Vasemania: Neoclassical Form and Ornament: Selections from The Metropolitan Museum of Art at the Bard Graduate Center for Studies in the Decorative Arts, Design, and Culture Review by Nancy H. Ramage 1) is a copy of a vase that belonged to Ithaca College Hamilton, painted in Wedgwood’s “encaustic” technique that imitated red-figure with red, An unusual and worthwhile exhibit on the orange, and white painted on top of the “black passion for vases in the 18th century has been basalt” body, as he called it. But here, assembled at the Bard Graduate Center in Wedgwood’s artist has taken all the figures New York City. The show, entitled that encircle the entire vessel on the original, Vasemania: Neoclassical Form and and put them on the front of the pot, just as Ornament: Selections from The Metropolitan they appear in a plate in Hamilton’s first vol- Museum of Art, was curated by a group of ume in the publication of his first collection, graduate students, together with Stefanie sold to the British Museum in 1772. On the Walker at Bard and William Rieder at the Met. original Greek pot, the last two figures on the It aims to set out the different kinds of taste — left and right goût grec, goût étrusque, goût empire — that sides were Fig. 1 Wedgwood Hydria, developed over a period of decades across painted on the Etruria Works, Staffordshire, Britain, France, Italy, Spain, and Germany. back of the ves- ca. 1780. Black basalt with “encaustic” painting. The at the Bard Graduate Center. -
Lunar Motion Motion A
2 Lunar V. Lunar Motion Motion A. The Lunar Calendar Dr. Bill Pezzaglia B. Motion of Moon Updated 2012Oct30 C. Eclipses 3 1. Phases of Moon 4 A. The Lunar Calendar 1) Phases of the Moon 2) The Lunar Month 3) Calendars based on Moon b). Elongation Angle 5 b.2 Elongation Angle & Phase 6 Angle between moon and sun (measured eastward along ecliptic) Elongation Phase Configuration 0º New Conjunction 90º 1st Quarter Quadrature 180º Full Opposition 270º 3rd Quarter Quadrature 1 b.3 Elongation Angle & Phase 7 8 c). Aristarchus 275 BC Measures the elongation angle to be 87º when the moon is at first quarter. Using geometry he determines the sun is 19x further away than the moon. [Actually its 400x further !!] 9 Babylonians (3000 BC) note phases are 7 days apart 10 2. The Lunar Month They invent the 7 day “week” Start week on a) The “Week” “moon day” (Monday!) New Moon First Quarter b) Synodic Month (29.5 days) Time 0 Time 1 week c) Spring and Neap Tides Full Moon Third Quarter New Moon Time 2 weeks Time 3 weeks Time 4 weeks 11 b). Stone Circles 12 b). Synodic Month Stone circles often have 29 stones + 1 xtra one Full Moon to Full Moon off to side. Originally there were 30 “sarson The cycle of stone” in the outer ring of Stonehenge the Moon’s phases takes 29.53 days, or ~4 weeks Babylonians measure some months have 29 days (hollow), some have 30 (full). 2 13 c1). Tidal Forces 14 c). Tides This animation illustrates the origin of tidal forces. -
Great Waterworks in Roman Greece Aqueducts and Monumental Fountain Structures Function in Context
Great Waterworks in Roman Greece Aqueducts and Monumental Fountain Structures Function in Context Access edited by Open Georgia A. Aristodemou and Theodosios P. Tassios Archaeopress Archaeopress Roman Archaeology 35 © Archaeopress and the authors, 2017. Archaeopress Publishing Ltd Gordon House 276 Banbury Road Oxford OX2 7ED www.archaeopress.com ISBN 978 1 78491 764 7 ISBN 978 1 78491 765 4 (e-Pdf) © Archaeopress and the authors 2018 Cover: The monumental arcade bridge of Moria,Access Lesvos, courtesy of Dr Yannis Kourtzellis Creative idea of Tasos Lekkas (Graphics and Web Designer, International Hellenic University) Open All rights Archaeopressreserved. No part of this book may be reproduced, in any form or by any means, electronic, mechanical, photocopying or otherwise, without the prior written permission of the copyright owners. Printed in England by Oxuniprint, Oxford This book is available direct from Archaeopress or from our website www.archaeopress.com © Archaeopress and the authors, 2017. Contents Preface ��������������������������������������������������������������������������������������������������������������������������������������������� iii Georgia A. Aristodemou and Theodosios P. Tassios Introduction I� Roman Aqueducts in Greece �������������������������������������������������������������������������������������1 Theodosios P. Tassios Introduction II� Roman Monumental Fountains (Nymphaea) in Greece �����������������������������������������10 Georgia A. Aristodemou PART I: AQUEDUCTS Vaulted-roof aqueduct channels in Roman -
Th1rzne CEEK
HESPERIA 68.2, I999 "'ADYTO N ," "OPI STHO DOO S," AND THE INNER ROO/ OFr TH1rznECEEK/ T EMPLED For Lucy Shoe Meritt We know very little of what took place inside a Greek temple. Sacrifice, the focal act of communal religious observance,was enacted outside, on an open-air altar usually opposite the main, east, facade of the temple, while the interior contained objects dedicated to the deity, including a cult statue. In form most Greek temples had a single main interior room, or cella; some had an additional small room behind it, accessible only from the cella. Such a subdivision of interior space suggests that the inner chamber served a special function. This study is designed to ascertain why some temples had inner rooms and how these chambers were used, questions that shed light on the nature of the temple itself. Examination of termi- nology used for temple interiors and of archaeological remains of temples with inner rooms, together with literary and epigraphical references to activities that occurred in temples, indicates a larger economic role for many temples and less secret ritual than has been assumed.1 Nomenclature is a central issue here, as naming incorporates a set of 1. This article is dedicatedto Lucy Since the 19th century, the in- Shoe Meritt, with gratitude,for her assumptions and a specific interpretation. generosityin sharingher expertisein ner room has been called 'a'UTOV (adyton, "not to be entered"), a term and enthusiasmfor Greek architecture. known from ancient sources. The usage of "adyton" in literary and In the uncommonlylong develop- epigraphical testimonia led scholars to consider the inner room a locus of ment of this article,I have received cult ritual of a chthonian or oracular nature, mysterious rites conducted exceptionalassistance from Susan within the temple.