Report on Phase Two of 1990 Ossa Data Census
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The Highly Structured Outer Solar Corona
The Astrophysical Journal, 862:18 (18pp), 2018 July 20 https://doi.org/10.3847/1538-4357/aac8e3 © 2018. The American Astronomical Society. The Highly Structured Outer Solar Corona C. E. DeForest1 , R. A. Howard2 , M. Velli3 , N. Viall4 , and A. Vourlidas5,6 1 Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, USA; [email protected] 2 Naval Research Laboratory, Washington, DC, USA 3 University of California, Los Angeles, CA, USA 4 NASA/Goddard Space Flight Center, Greenbelt, MD, USA 5 Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA Received 2018 March 6; revised 2018 April 28; accepted 2018 May 22; published 2018 July 18 Abstract We report on the observation of fine-scale structure in the outer corona at solar maximum, using deep-exposure campaign data from the Solar Terrestrial Relations Observatory-A (STEREO-A)/COR2 coronagraph coupled with postprocessing to further reduce noise and thereby improve effective spatial resolution. The processed images reveal radial structure with high density contrast at all observable scales down to the optical limit of the instrument, giving the corona a “woodgrain” appearance. Inferred density varies by an order of magnitude on spatial scales of 50 Mm and follows an f −1 spatial spectrum. The variations belie the notion of a smooth outer corona. They are inconsistent with a well-defined “Alfvén surface,” indicating instead a more nuanced “Alfvén zone”—a broad trans-Alfvénic region rather than a simple boundary. Intermittent compact structures are also present at all observable scales, forming a size spectrum with the familiar “Sheeley blobs” at the large-scale end. -
CR-/3017S B ORBITING SOLAR OBSERVATORY FINAL REPORT
4: it W::: 050-7 ~AS ACR-/3017s B ORBITING SOLAR OBSERVATORY FINAL REPORT N C) U2a ~ 0mU 4~~~~~~~~~~~~~~~~~~~~~~~~~~~~~-4' W 10 ~~~~~~ -7 Ol C",.1-a -9- ---- o ' ocl '.-l Q) o QU2i~WL4cO 1-a . ), 3xr N~~~~~~~~~~~~~~~. .~ tjir~ V I ed F7. 3 wUii rH1 _.1- ~~z,~~OULECORD r~ BALBOTESRSERHCRPRTO o~~~~~USDAY FBL OPRTO BOULDER, COLRAD I~ ~..... LDER-'COLOR.DO '-01 OSO-7 ORBITING SOLAR OBSERVATORY PROGRAM FINAL REPORT F72-01 December 31, 1972 PREPARED BY APPROVED BY OSO Program Staff J. O. Simpson Director, OSO Programs BALL BROTHERS RESEARCH CORPORATION SUBSIDIARY OF BALL CORPORATION BOULDER, COLORADO F72-01 PREFACE During the 1950's rapid progress was made in solar physics and in instrument and space hardware technology, using rocket and balloon flights that, although of brief duration, provided a view of the sun free from the obscuring atmosphere. The significance of data from these flights confirmed the often-asserted value of long-term observations from a spacecraft in advancing our knowledge of the sun's behavior. Thus, the first of NASA's space platforms designed for long-term observations of the universe from above the atmosphere was planned, and the Orbiting Solar Observatory program started in 1959. Solar physics data return began with the launch of OSO-1 in March of 1962. OSO-2 and OSO-3 were launched in 1965, OSO-4 and OS0-5 in 1967, OSO-6 in 1969, and the most recent, OSO-7/, was launched on September 29, 1971. All seven OSO's have been highly successful both in scientific data return and in per- formance of the engineering systems. -
Information Summaries
TIROS 8 12/21/63 Delta-22 TIROS-H (A-53) 17B S National Aeronautics and TIROS 9 1/22/65 Delta-28 TIROS-I (A-54) 17A S Space Administration TIROS Operational 2TIROS 10 7/1/65 Delta-32 OT-1 17B S John F. Kennedy Space Center 2ESSA 1 2/3/66 Delta-36 OT-3 (TOS) 17A S Information Summaries 2 2 ESSA 2 2/28/66 Delta-37 OT-2 (TOS) 17B S 2ESSA 3 10/2/66 2Delta-41 TOS-A 1SLC-2E S PMS 031 (KSC) OSO (Orbiting Solar Observatories) Lunar and Planetary 2ESSA 4 1/26/67 2Delta-45 TOS-B 1SLC-2E S June 1999 OSO 1 3/7/62 Delta-8 OSO-A (S-16) 17A S 2ESSA 5 4/20/67 2Delta-48 TOS-C 1SLC-2E S OSO 2 2/3/65 Delta-29 OSO-B2 (S-17) 17B S Mission Launch Launch Payload Launch 2ESSA 6 11/10/67 2Delta-54 TOS-D 1SLC-2E S OSO 8/25/65 Delta-33 OSO-C 17B U Name Date Vehicle Code Pad Results 2ESSA 7 8/16/68 2Delta-58 TOS-E 1SLC-2E S OSO 3 3/8/67 Delta-46 OSO-E1 17A S 2ESSA 8 12/15/68 2Delta-62 TOS-F 1SLC-2E S OSO 4 10/18/67 Delta-53 OSO-D 17B S PIONEER (Lunar) 2ESSA 9 2/26/69 2Delta-67 TOS-G 17B S OSO 5 1/22/69 Delta-64 OSO-F 17B S Pioneer 1 10/11/58 Thor-Able-1 –– 17A U Major NASA 2 1 OSO 6/PAC 8/9/69 Delta-72 OSO-G/PAC 17A S Pioneer 2 11/8/58 Thor-Able-2 –– 17A U IMPROVED TIROS OPERATIONAL 2 1 OSO 7/TETR 3 9/29/71 Delta-85 OSO-H/TETR-D 17A S Pioneer 3 12/6/58 Juno II AM-11 –– 5 U 3ITOS 1/OSCAR 5 1/23/70 2Delta-76 1TIROS-M/OSCAR 1SLC-2W S 2 OSO 8 6/21/75 Delta-112 OSO-1 17B S Pioneer 4 3/3/59 Juno II AM-14 –– 5 S 3NOAA 1 12/11/70 2Delta-81 ITOS-A 1SLC-2W S Launches Pioneer 11/26/59 Atlas-Able-1 –– 14 U 3ITOS 10/21/71 2Delta-86 ITOS-B 1SLC-2E U OGO (Orbiting Geophysical -
OSO 20M Telescope Handbook
OSO 20m Telescope Handbook Onsala Space Observatory August 31, 2016 The latest version of this handbook can be found here. Original version by Lars E.B. Johansson. Latest revisions by A.O.H.Olofsson and E. De Beck. Table of Contents Contents2 List of Figures5 List of Tables6 1 Introduction7 1 Quick system overview..........................7 2 Observing.................................8 3 Staff....................................9 4 Communication..............................9 2 Technical description 10 1 The telescope............................... 10 2 Receivers / frontends........................... 10 2.1 3 mm: 85 – 116 GHz........................ 11 2.2 4 mm: 67 – 87 GHz........................ 12 2.3 100 GHz receiver......................... 12 3 Spectrometers / backends........................ 14 4 Telescope and instrument control system................ 15 3 Spectral-line observations 16 1 Observing modes............................. 16 1.1 Beam switching.......................... 16 1.2 Position switching......................... 17 1.3 Frequency switching....................... 17 1.4 Mapping.............................. 17 2 Calibration................................ 18 3 Pointing strategy............................. 18 4 Velocity systems.............................. 18 5 Time estimates.............................. 19 6 Atmospheric transmission........................ 20 4 Data 22 1 Backups, retrieval and transfer...................... 22 2 File names................................. 22 2 OSO 20 m Telescope Handbook Table -
A Journey of Exploration to the Polar Regions of a Star: Probing the Solar
Experimental Astronomy manuscript No. (will be inserted by the editor) A journey of exploration to the polar regions of a star: probing the solar poles and the heliosphere from high helio-latitude Louise Harra · Vincenzo Andretta · Thierry Appourchaux · Fr´ed´eric Baudin · Luis Bellot-Rubio · Aaron C. Birch · Patrick Boumier · Robert H. Cameron · Matts Carlsson · Thierry Corbard · Jackie Davies · Andrew Fazakerley · Silvano Fineschi · Wolfgang Finsterle · Laurent Gizon · Richard Harrison · Donald M. Hassler · John Leibacher · Paulett Liewer · Malcolm Macdonald · Milan Maksimovic · Neil Murphy · Giampiero Naletto · Giuseppina Nigro · Christopher Owen · Valent´ın Mart´ınez-Pillet · Pierre Rochus · Marco Romoli · Takashi Sekii · Daniele Spadaro · Astrid Veronig · W. Schmutz Received: date / Accepted: date L. Harra PMOD/WRC, Dorfstrasse 33, CH-7260 Davos Dorf and ETH-Z¨urich, Z¨urich, Switzerland E-mail: [email protected]; ORCID: 0000-0001-9457-6200 V. Andretta INAF, Osservatorio Astronomico di Capodimonte, Naples, Italy E-mail: vin- [email protected]; ORCID: 0000-0003-1962-9741 T. Appourchaux Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: [email protected]; ORCID: 0000-0002-1790-1951 F. Baudin Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: [email protected]; ORCID: 0000-0001-6213-6382 L. Bellot Rubio Inst. de Astrofisica de Andaluc´ıa, Granada Spain A.C. Birch Max-Planck-Institut f¨ur Sonnensystemforschung, 37077 G¨ottingen, Germany; E-mail: arXiv:2104.10876v1 [astro-ph.SR] 22 Apr 2021 [email protected]; ORCID: 0000-0001-6612-3861 P. Boumier Institut d’Astrophysique Spatiale, CNRS, Universit´e Paris–Saclay, France; E-mail: 2 Louise Harra et al. -
Pokroky Kosmické Astronomie
Pokroky matematiky, fyziky a astronomie Marcel Grün; Pavel Koubský Pokroky kosmické astronomie Pokroky matematiky, fyziky a astronomie, Vol. 15 (1970), No. 2, 62--76 Persistent URL: http://dml.cz/dmlcz/138230 Terms of use: © Jednota českých matematiků a fyziků, 1970 Institute of Mathematics of the Academy of Sciences of the Czech Republic provides access to digitized documents strictly for personal use. Each copy of any part of this document must contain these Terms of use. This paper has been digitized, optimized for electronic delivery and stamped with digital signature within the project DML-CZ: The Czech Digital Mathematics Library http://project.dml.cz POKROKY KOSMICKÉ ASTRONOMIE MARCEL GRÚN, PAVEL KOUBSKÝ, Praha Astronomická pozorování konaná ze zemského povrchu jsou znesnadňována přítomností atmosféry, která se chová jako filtr se specifickými vlastnostmi: 1. Je nepropustná pro většinu frekvencí elektromagnetických vln přicházejících z vesmíru (obr. I). 2. Omezuje rozlišovací schopnost v těch oborech, které propouští. Vzhledem k difrakci světla je teoretická rozlišovací schopnost přímoúměrná apertuře (průměru objektivu) a nepřímo- úměrná vlnové délce. To však platí pouze pro ideální podmínky, neboť turbulence atmosféry nedovoluje rozlišit ve viditelném oboru více než 0,1". Obvyklé pozorovací podmínky snižují tuto hodnotu nejméně o řád; třiceticentimetrový dalekohled ve vakuu je po stránce praktické rozlišo vací schopnosti ekvivalentní největším pozemským přístrojům. 3. Pozorování je rušeno existencí vlastního záření atmosféry a přítomností záření rozptýleného v atmosféře. Rozptýlené záření způsobuje, že dosah největších fotografických dalekohledů je nižší, než by odpovídalo optice a citlivosti detektorů. Záření atmosféry je překážkou též při spektrální analýze slabých objektů. Ve zprávě [1] se předpokládá, že třímetrový reflektor na oběž né dráze pointovaný s přesností 0,004" by byl schopen zachytit objekty do 29m, o 2 řády méně jasné než dosud ze Země. -
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. -
Aeronautics and Space Report of the President
Aeronautics and Space Report of the President 1971 Activities NOTE TO READERS: ALL PRINTED PAGES ARE INCLUDED, UNNUMBERED BLANK PAGES DURING SCANNING AND QUALITY CONTROL CHECK HAVE BEEN DELETED Aeronautics and Space Report of the President 197 I Activities i W Executive Office of the President National Aeronautics and Space Council Washington, D.C. 20502 PRESIDENT’S MESSAGE OF TRANSMITTAL To the Congress of the United States: I am pleased to transmit herewith a report of our national progress in aero- nautics and space activities during 1971. This report shows that we have made forward strides toward each of the six objectives which I set forth for a balanced space program in my statement of March 7, 1970. Aided by the improvements we have made in mobility, our explorers on the moon last summer produced new, exciting and useful evidence on the structure and origin of the moon. Several phenomena which they uncovered are now under study. Our unmanned nearby observation of Mars is similarly valuable and significant for the advancement of science. During 1971, we gave added emphasis to aeronautics activities which contribute substantially to improved travel conditions, safety and security, and we gained in- creasing recognition that space and aeronautical research serves in many ways to keep us in the forefront of man’s technological achievements. There can be little doubt that the investments we are now making in explora- tions of the unknown are but a prelude to the accomplishments of mankind in future generations. THEWHITE HOUSE, March 1972 iii Table of Contents Page Page I . Progress Toward U.S. -
9538\Ariel View.Pdf
Cover story.qxd 2/5/07 4:59 pm Page 14 An Ariel view of UK spacecraft It’s 40 years since t was 5 May 1967, just before 12pm, when a satellite was designed by the Space Scout rocket was launched from NASA’s West- Department of the Royal Aircraft Estab- the first UK designed and I ern Test Range in California, witnessed by a lishment (RAE), Farnborough, with group of British scientists and engineers wit- British Aircraft Corporation and GEC as manufactured satellite nessed. The successful launch assured the precious the main industrial contractors. cargo – and the engineers – a place in UK engi- At the time, relatively little was known was launched. How has neering history. about the space environment, although Sitting atop the four stage Scout was Ariel III the RAE did simulate vacuum, radiation – the first entirely UK built satellite and third in and thermal effects on Ariel and its pay- the UK satellite industry an Anglo-American cooperative space research load. Meanwhile, thanks to the RAE’s SkyLark programme to extend atmospheric and ionos- rockets, which had been providing upper atmos- developed? pheric investigations. The small observatory car- phere research data since 1957, many of the test ried five British experiments and a tape recorder payloads used by Ariel had been proved in rocket Vanessa Knivett to obtain data. launch and simply required adaptation. Sputnik 1, the first man made satellite, had Ariel III was approximately 66in high and 30in explores. been launched almost 10 years earlier, on 4 Octo- in diameter. Four booms hinged out from the ber 1957. -
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. -
19710023003.Pdf
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) X-625-71-308 PkEFRlil NASA T1:1 X- ELECTRON AND POSITIVE ION DENSITY ALTITUDE DISTRIBUTIONS IN THE EQUATORIAL Q REGION A. C. AIKIN R. A. GOLDBERG Y. V. SOMAYAJULU Aq ^F q "9,>/ #44#i4 a^F/j/F C-r; AI!riICT 1471 Jp ,32479 Ole °o (ACCESSi JN N MBCR) (THR 0 'i (NASA CR R TMX OR AD NUMBER) (CATEGORY) --- GODDARD SPACE FLIGHT CENTER GREENBELT, MARYLAND - it %0 ELECTRON AND POSITIVE ION DENSITY ALTITUDE DISTRIBUTIONS IN THE EQUATORIAL D REGION by A. C. Aikin R. A. Goldberg • Laboratory for .Planetary Atmospheres NASA/Goddard !7nace Flight Center Greenb?.. , Maryland and Y. V. Somayajulu National Physical Laboratory New Delhi, India ABSTRACT Three simultaneous rocket measurements of P region ionization sources and electron and ion densities have been made in one day. -
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.