Descriptions of Planetary and He1 Iocent R Ic Spacecraft and Investigations
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Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
Thematic Forest Dictionary
Elżbieta Kloc THEMATIC FOREST DICTIONARY TEMATYCZNY SŁOWNIK LEÂNY Wydano na zlecenie Dyrekcji Generalnej Lasów Państwowych Warszawa 2015 © Centrum Informacyjne Lasów Państwowych ul. Grójecka 127 02-124 Warszawa tel. 22 18 55 353 e-mail: [email protected] www.lasy.gov.pl © Elżbieta Kloc Konsultacja merytoryczna: dr inż. Krzysztof Michalec Konsultacja i współautorstwo haseł z zakresu hodowli lasu: dr inż. Maciej Pach Recenzja: dr Ewa Bandura Ilustracje: Bartłomiej Gaczorek Zdjęcia na okładce Paweł Fabijański Korekta Anna Wikło ISBN 978-83-63895-48-8 Projek graficzny i przygotowanie do druku PLUPART Druk i oprawa Ośrodek Rozwojowo-Wdrożeniowy Lasów Państwowych w Bedoniu TABLE OF CONTENTS – SPIS TREÂCI ENGLISH-POLISH THEMATIC FOREST DICTIONARY ANGIELSKO-POLSKI TEMATYCZNY SŁOWNIK LEÂNY OD AUTORKI ................................................... 9 WYKAZ OBJAŚNIEŃ I SKRÓTÓW ................................... 10 PLANTS – ROŚLINY ............................................ 13 1. Taxa – jednostki taksonomiczne .................................. 14 2. Plant classification – klasyfikacja roślin ............................. 14 3. List of forest plant species – lista gatunków roślin leśnych .............. 17 4. List of tree and shrub species – lista gatunków drzew i krzewów ......... 19 5. Plant morphology – morfologia roślin .............................. 22 6. Plant cells, tissues and their compounds – komórki i tkanki roślinne oraz ich części składowe .................. 30 7. Plant habitat preferences – preferencje środowiskowe roślin -
The Quest to Understand the Pioneer Anomaly
The quest to understand the Pioneer anomaly I Michael Martin Nieto, Theoretical Division (MS-8285) Los Alamos National Laboratory Los Alarnos, New Mexico 87545 USA E-mail: [email protected] +a l1 l I l uring the 1960's, when the Jet Propulsion Laboratory (JPL) Pioneer 10 was launched on 2 March 1972 local time, aboard D first started thinking about what eventually became the an Atlas/Centaur/TE364-4launch vehicle (see Fig. l).It was the "Grand Tours" of the outer planets (the Voyager missions of the first craft launched into deep space and was the first to reach an 1970's and 1980's),the use of planetary flybys for gravity assists of outer giant planet, Jupiter,on 4 Dec. 1973 [l, 21. Later it was the first spacecraft became of great interest. The concept was to use flybys to leave the "solar system" (past the orbit of Pluto or, should we now of the major planets to both mowthe direction of the spacecraft say, Neptune). The Pioneer project, eventually extending over and also to add to its heliocentric velocity in a manner that was decades, was managed at NASAIAMES Research Center under the unfeasible using only chemical fuels. The first time these ideas were hands of four successive project managers, the legendary Charlie put into practice in deep space was with the Pioneers. Hall, Richard Fimrnel, Fred Wirth, and the current Larry Lasher. While in its Earth-Jupiter cruise, Pioneer 10 was still bound to the solar system. By 9 January 1973 Pjoneer l0 was at a distance of 3.40 AU (Astronomical Units'), beyond the asteroid belt. -
Radial Variation of the Interplanetary Magnetic Field Between 0.3 AU and 1.0 AU
|00000575|| J. Geophys. 42, 591 - 598, 1977 Journal of Geophysics Radial Variation of the Interplanetary Magnetic Field between 0.3 AU and 1.0 AU Observations by the Helios-I Spacecraft G. Musmann, F.M. Neubauer and E. Lammers Institut for Geophysik and Meteorologie, Technische Universitiit Braunschweig, Mendelssohnstr. lA, D-3300 Braunschweig, Federal Republic of Germany Abstract. We have investigated the radial dependence of the radial and azimuthal components and the magnitude of the interplanetary magnetic field obtained by the Technical University of Braunschweig magnetometer experiment on-board of Helios-1 from December 10, 1974 to first perihelion on March 15, 1975. Absolute values of daily averages of each quantity have been employed. The regression analysis based on power laws leads to 2.55 y x r- 2 · 0 , 2.26 y x r- i.o and F = 5.53 y x r- i. 6 with standard deviations of 2.5 y, 2.0 y and 3.2 y for the radial and azimuthal components and magnitude, respectively. Here r is the radial distance from the sun in astronomical units. The results are compared with results obtained for Mariners 4, 5 and 10 and Pioneers 6 and 10. The differences are probably due to different epochs in the solar cycle and the different statistical techniques used. Key words: Interplanetary magnetic field - Helios-1 results. Introduction The study of the vanat10n of the components and magnitude of the in terplanetary magnetic field with heliocentric distance is very intersting at the present time. The mission of Mariner 10 to the inner solar system to a heliocentric distance of 0.46 AU and the missions of Pioneer 10 and Pioneer 11 to the outer solar system to heliocentric distances beyond 5 AU have provided new data over a wide range of heliocentric distance. -
Space and Astrophysical Plasmas: Pervasive Problems
PRAMANA c Indian Academy of Sciences Vol. 55, Nos 5 & 6 — journal of Nov. & Dec. 2000 physics pp. 645–654 Space and astrophysical plasmas: Pervasive problems CHANCHAL UBEROI Department of Mathematics, Indian Institute of Science, Bangalore 560 012, India Abstract. The observations and measurements given by Earth orbiting satellites, deep space probes, sub-orbital systems and orbiting astronomical observatories point out that there are impor- tant physical processes which are responsible for a wide variety of phenomena in solar-terrestrial, solar-system and astrophysical plasmas. In this review these topics are exemplified both from an observational and a theoretical point of view. Keywords. Heliosphere; solar corona; Alfven resonances; magnetic reconnection. PACS Nos 95.30 Q; 96.50 R 1. Introduction Space science is generally defined as investigations that are conducted by scientists using earth orbiting satellites, deep space probes like Pioneer series and sub-orbital systems. Space plasma sciences are now a very highly developed multidisciplinary area of research and can be divided into three areas: solar-terrestrial or Sun–Earth relations, solar-systems exploration and astrophysics. Though space science grew out of the rocket research which followed the end of World War II, the early investigations which began in 1946 concentrated on studies of the Earth’s atmosphere, solar radiation and cosmic rays from space. It was in 1958 that launch of Ex- plorer I and subsequent discovery of Van Allen belts which brought the scientific research in space sciences on to the list of other branches of physical and astrophysical sciences. These earlier flights of Pioneer I and subsequent series which laid the foundation of area of space plasma physics which as we now know has become a highly developed multidis- ciplinary area of research to understand the Sun–Earth or solar-terrestrial relations. -
Geological Survey Research 1961 Synopsis of Geologic and Hydrologic Results
Geological Survey Research 1961 Synopsis of Geologic and Hydrologic Results GEOLOGICAL SURVEY PROFESSIONAL PAPER 424-A Geological Survey Research 1961 THOMAS B. NOLAN, Director GEOLOGICAL SURVEY PROFESSIONAL PAPER 424 A synopsis ofgeologic and hydrologic results, accompanied by short papers in the geologic and hydrologic sciences. Published separately as chapters A, B, C, and D UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1961 FOEEWOED The Geological Survey is engaged in many different kinds of investigations in the fields of geology and hydrology. These investigations may be grouped into several broad, inter related categories as follows: (a) Economic geology, including engineering geology (b) Eegional geologic mapping, including detailed mapping and stratigraphic studies (c) Eesource and topical studies (d) Ground-water studies (e) Surface-water studies (f) Quality-of-water studies (g) Field and laboratory research on geologic and hydrologic processes and principles. The Geological Survey also carries on investigations in its fields of competence for other Fed eral agencies that do not have the required specialized staffs or scientific facilities. Nearly all the Geological Survey's activities yield new data and principles of value in the development or application of the geologic and hydrologic sciences. The purpose of this report, which consists of 4 chapters, is to present as promptly as possible findings that have come to the fore during the fiscal year 1961 the 12 months ending June 30, 1961. The present volume, chapter A, is a synopsis of the highlights of recent findings of scientific and economic interest. Some of these findings have been published or placed on open file during the year; some are presented in chapters B, C, and D ; still others have not been pub lished previously. -
Deep Space Chronicle Deep Space Chronicle: a Chronology of Deep Space and Planetary Probes, 1958–2000 | Asifa
dsc_cover (Converted)-1 8/6/02 10:33 AM Page 1 Deep Space Chronicle Deep Space Chronicle: A Chronology ofDeep Space and Planetary Probes, 1958–2000 |Asif A.Siddiqi National Aeronautics and Space Administration NASA SP-2002-4524 A Chronology of Deep Space and Planetary Probes 1958–2000 Asif A. Siddiqi NASA SP-2002-4524 Monographs in Aerospace History Number 24 dsc_cover (Converted)-1 8/6/02 10:33 AM Page 2 Cover photo: A montage of planetary images taken by Mariner 10, the Mars Global Surveyor Orbiter, Voyager 1, and Voyager 2, all managed by the Jet Propulsion Laboratory in Pasadena, California. Included (from top to bottom) are images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets (Mercury, Venus, Earth and its Moon, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) are roughly to scale to each other. NASA SP-2002-4524 Deep Space Chronicle A Chronology of Deep Space and Planetary Probes 1958–2000 ASIF A. SIDDIQI Monographs in Aerospace History Number 24 June 2002 National Aeronautics and Space Administration Office of External Relations NASA History Office Washington, DC 20546-0001 Library of Congress Cataloging-in-Publication Data Siddiqi, Asif A., 1966 Deep space chronicle: a chronology of deep space and planetary probes, 1958-2000 / by Asif A. Siddiqi. p.cm. – (Monographs in aerospace history; no. 24) (NASA SP; 2002-4524) Includes bibliographical references and index. 1. Space flight—History—20th century. I. Title. II. Series. III. NASA SP; 4524 TL 790.S53 2002 629.4’1’0904—dc21 2001044012 Table of Contents Foreword by Roger D. -
FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER SPECTROSCOPY of the O Vi RESONANCE DOUBLET in SAND 2 (WO) Paul A
The Astrophysical Journal, 538:L51±L55, 2000 July 20 q 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A. FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER SPECTROSCOPY OF THE O vi RESONANCE DOUBLET IN SAND 2 (WO) Paul A. Crowther,1 A. W. Fullerton,2,3 D. J. Hillier,4 K. Brownsberger,5 L. Dessart,1,6 A. J. Willis,1 O. De Marco,1 M. J. Barlow,1 J. B. Hutchings,7 D. L. Massa,8 D. C. Morton,7 and G. Sonneborn9 Received 2000 March 17; accepted 2000 June 8; published 2000 July 14 ABSTRACT We present Far Ultraviolet Spectroscopic Explorer spectroscopy of Sand 2, an LMC WO-type Wolf-Rayet star, revealing the O vi resonance P Cygni doublet at 1032±1038 AÊ . These data are combined with Hubble Space Telescope Faint Object Spectrograph ultraviolet and Mount Stromlo 2.3 m optical spectroscopy and analyzed using a spherical, non-LTE, line-blanketed code. Our study reveals exceptional stellar parameters: T¤ » 21 Ç 25 21 150,000 K,v` = 4100 km s , log (L/L,,) = 5.3 , andM=1 # 10 M yr , if we adopt a volume ®lling factor » 5 » 10.10 of 10%. Elemental abundances ofC/He 0.7 0.2 and O/He 0.1520.05 by number qualitatively support pre- vious recombination line studies. We con®rm that Sand 2 is more chemically enriched in carbon than LMC WC stars and that it is expected to undergo a supernova explosion within the next5 # 10 4 yr. Subject headings: stars: evolution Ð stars: individual (Sand 2) Ð stars: Wolf-Rayet 1. -
Mission Overview the Pioneer Mission Set the Stage for U.S. Space
Mission Overview The Pioneer mission set the stage for U.S. space exploration. Pioneer 1 was the first manmade object to escape the Earth's gravitational field. Later Pioneer 4 was the first spacecraft to fly to the moon, Pioneer 10 was the first to Jupiter, Pioneer 11 was the first to Saturn and Pioneer 12 was the first U.S. spacecraft to orbit another planet, Venus. The following table summarizes the Pioneer spacecraft and scientific objectives of the Pioneer mission. Name Launch Mission Status (as of 1998) ----------------------------------------------------------------- Pioneer 1 1958-10-11 Moon Reached altitude of 72765 miles Pioneer 2 1958-11-08 Moon Reached altitude of 963 miles Pioneer 3 1958-12-02 Moon Reached altitude of 63580 miles Pioneer 4 1959-03-03 Moon Passed by moon into solar orbit Pioneer 5 1960-03-11 Solar Orbit Entered solar orbit Pioneer 6 1965-12-16 Solar Orbit Still operating Pioneer 7 1966-08-17 Solar Orbit Still operating Pioneer 8 1967-12-13 Solar Orbit Still operating Pioneer 9 1967-11-08 Solar Orbit Signal lost in 1983 Pioneer E 1969-08-07 Solar Orbit Launch failure Pioneer10 1972-03-02 Jupiter Communication terminated 1998 Pioneer11 1972-03-02 Jupiter/Saturn Communication terminated 1997 Pioneer12 1978-05-20 Venus Entered Venus atmos. 1992-10-08 The focus of this document is on Pioneer Venus (12), the last spacecraft in a mission of firsts in space exploration. Probe Separation: Pioneer Venus separated into two spacecraft on Aug 8, 1978: an Orbiter (PVO) and a Multiprobe. The latter was separated into five separate vehicles near Venus. -
New Observational Results on the Colliding Wind WR+O Binary WR 30A
Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies Proceedings IAU Symposium No. 193, @1999 IAU K.A. van der Hucht, G. Koenigsberger & P.R.J. Eenens, eds. New observational results on the colliding wind WR+O binary WR 30a Eric Gosset", Pierre Royer I, Gregor Rauw", Jean Manfroid", and Jean-Marie Vreux Institut d'Astrophysique et de Geophsisique, Unioersite de Liege, avenue de Cointe, 5, B-4000 Liege, Belgium 1. Introduction WR 30a (MS 4) was first suspected as a possible Wolf-Rayet star by McConnell & Sanduleak (1970) during a deep objective-prism survey performed around the Carina Nebula region. From subsequent studies, the spectrum turned out to be composite, with a WR component classified W04 (or alternatively WC4, W05 and WC3) and an 0 component classified 04. Niemela (1995) reported the first, and up-to-now unique, radial velocity study for that star. She noticed large variations of C IV A4658 from night to night, suggesting that WR 30a might be a short period binary. A plot of the C IV emission-line velocities versus the He II absorption ones clearly indicates that they are exhibiting opposite binary motions. The apparent velocity amplitudes imply a rather low mass ratio Mwo 4/Mo4 == 0.15, although the radial velocities of the C IV line could be distorted due to line-profile variations. In the present paper, we confirm the binary nature of WR 30a and propose, for the first time, a value for the orbital period of the system: P == 4.62 days. Other orbital parameters are also derived and discussed. -
Pioneer Data-Processing Equipment
https://ntrs.nasa.gov/search.jsp?R=19730009155 2020-03-23T07:26:19+00:00Z 'THE INTERPLANETARY 'PIONEERS VOLUME II: SYSTEM DESIGN AND DEVELOPMENT (NASA-SP-279-Vol-2) THE INTERPLANETARY PIONEERS. VOLUME 2: SYSTEM DESIGN AND DEVELOPMENT (NASA) 312 p MF. $0.95; SOD HC$2.5 N73-1788 CSCL 22C. N"' 73' 111/3 Unclas 62187 m0 I- U~~ NASA SP-279 THE INTERPLANETARY PIONEERS VOLUME II: SYSTEM DESIGN AND DEVELOPMENT by William R. Corliss Scientific and Technical Information Office 1972 NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Washington, D.C. For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402 Price $2.50 Stock Number 3300-0452 Library of Congress Catalog Card Number 74-176234 Foreword SOME EXPLORATORY ENTERPRISES start with fanfare and end with a quiet burial; some start with hardly a notice, yet end up significantly ad- vancing mankind's knowledge. The Interplanetary Pioneers more closely fit the latter description. When the National Aeronautics and Space Administration started the program a decade ago it received little public attention. Yet the four spacecraft, designated Pioneers 6, 7, 8, and 9, have faithfully lived up to their name as defined by Webster, "to discover or explore in advance of others." These pioneering spacecraft were the first to systematically orbit the Sun at widely separated points in space, collecting information on conditions far from the Earth's disturbing influence. From them we have learned much about space, the solar wind, and the fluc- tuating bursts of cosmic radiation of both solar and galactic origin. -
Callimachi Cyrenaei Hymni Cum Latina Interpretatione a Viro Cl. Ant
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