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Collezione Per Genova
1958-1978: 20 anni di sperimentazioni spaziali in Occidente La collezione copre il ventennio 1958-1978 che è stato particolarmente importante nella storia della esplorazio- ne spaziale, in quanto ha posto le basi delle conoscenze tecnico-scientifiche necessarie per andare nello spa- zio in sicurezza e per imparare ad utilizzare le grandi potenzialità offerte dallo spazio per varie esigenze civili e militari. Nel clima di guerra fredda, lo spazio è stato fin dai primi tempi, utilizzato dagli Americani per tenere sotto con- trollo l’avversario e le sue dotazioni militari, in risposta ad analoghe misure adottate dai Sovietici. Per preparare le missioni umane nello spazio, era indispensabile raccogliere dati e conoscenze sull’alta atmo- sfera e sulle radiazioni che si incontrano nello spazio che circonda la Terra. Dopo la sfida lanciata da Kennedy, gli Americani dovettero anche prepararsi allo sbarco dell’uomo sulla Luna ed intensificarono gli sforzi per conoscere l’ambiente lunare. Fin dai primi anni, le sonde automatiche fecero compiere progressi giganteschi alla conoscenza del sistema solare. Ben presto si imparò ad utilizzare i satelliti per la comunicazione intercontinentale e il supporto alla navigazio- ne, per le previsioni meteorologiche, per l’osservazione della Terra. La Collezione testimonia anche i primi tentativi delle nuove “potenze spaziali” che si avvicinano al nuovo mon- do dei satelliti, che inizialmente erano monopolio delle due Superpotenze URSS e USA. L’Italia, con San Mar- co, diventò il terzo Paese al mondo a lanciare un proprio satellite e allestì a Malindi la prima base equatoriale, che fu largamente utilizzata dalla NASA. Alla fine degli anni ’60 anche l’Europa entrò attivamente nell’arena spaziale, lanciando i propri satelliti scientifici e di telecomunicazione dalla propria base equatoriale di Kourou. -
Satellite Situation Report
NASA Office of Public Affairs Satellite Situation Report VOLUME 17 NUMBER 6 DECEMBER 31, 1977 (NASA-TM-793t5) SATELLITE SITUATION~ BEPORT, N8-17131 VOLUME 17, NO. 6 (NASA) 114 F HC A06/mF A01 CSCL 05B Unclas G3/15 05059 Goddard Space Flight Center Greenbelt, Maryland NOTICE .THIS DOCUMENT HAS'BEEN REPRODUCED FROM THE BEST COPY FURNISHED US BY THE SPONSORING AGENCY. ALTHOUGH IT IS RECOGNIZED THAT CERTAIN PORTIONS' ARE ILLEGIBLE, IT IS BEING RELEASED IN THE INTEREST OF MAKING AVAILABLE AS MUCH INFORMATION AS POSSIBLE. OFFICE OF PUBLIC AFFAIRS GCDDARD SPACE FLIGHT CENTER NATIONAL AERONAUTICS AND SPACE ADMINISTRATION VOLUME 17 NO. 6 DECEMBER 31, 1977 SATELLITE SITUATION REPORT THIS REPORT IS PUBLIShED AND DISTRIBUTED BY THE OFFICE OF PUBLIC AFFAIRS, GSFC. GODPH DRgP2 FE I T ERETAO5MUJS E SMITHSONIAN ASTRCPHYSICAL OBSERVATORY. SPACEFLIGHT TRACKING AND DATA NETWORK. NOTE: The Satellite Situation Report dated October 31, 1977, contained an entry in the "Objects Decayed Within the Reporting Period" that 1977 042P, object number 10349, decayed on September 21, 1977. That entry was in error. The object is still in orbit. SPACE OBJECTS BOX SCORE OBJECTS IN ORBIT DECAYED OBJECTS AUSTRALIA I I CANACA 8 0 ESA 4 0 ESRO 1 9 FRANCE 54 26 FRANCE/FRG 2 0 FRG 9 3 INCIA 1 0 INDONESIA 2 0 INTERNATIONAL TELECOM- MUNICATIONS SATELLITE ORGANIZATION (ITSO) 22 0 ITALY 1 4 JAPAN 27 0 NATC 4 0 NETHERLANDS 0 4 PRC 6 14 SPAIN 1 0 UK 11 4 US 2928 1523 USSR 1439 4456 TOTAL 4E21 6044 INTER- CBJECTS IN ORIT NATIONAL CATALOG PERIOD INCLI- APOGEE PERIGEE TQANSMITTTNG DESIGNATION NAME NUMBER SOURCE LAUNCH MINUTES NATION KM. -
ARIEL – 13Th Appleton Space Conference PLANETS ARE UBIQUITOUS
Background image credit NASA ARIEL – 13th Appleton Space Conference PLANETS ARE UBIQUITOUS OUR GALAXY IS MADE OF GAS, STARS & PLANETS There are at least as many planets as stars Cassan et al, 2012; Batalha et al., 2015; ARIEL – 13th Appleton Space Conference 2 EXOPLANETS TODAY: HUGE DIVERSITY 3700+ PLANETS, 2700 PLANETARY SYSTEMS KNOWN IN OUR GALAXY ARIEL – 13th Appleton Space Conference 3 HUGE DIVERSITY: WHY? FORMATION & EVOLUTION PROCESSES? MIGRATION? INTERACTION WITH STAR? Accretion Gaseous planets form here Interaction with star Planet migration Ices, dust, gas ARIEL – 13th Appleton Space Conference 4 STAR & PLANET FORMATION/EVOLUTION WHAT WE KNOW: CONSTRAINTS FROM OBSERVATIONS – HERSCHEL, ALMA, SOLAR SYSTEM Measured elements in Solar system ? Image credit ESA-Herschel, ALMA (ESO/NAOJ/NRAO), Marty et al, 2016; André, 2012; ARIEL – 13th Appleton Space Conference 5 THE SUN’S PLANETS ARE COLD SOME KEY O, C, N, S MOLECULES ARE NOT IN GAS FORM T ~ 150 K Image credit NASA Juno mission, NASA Galileo ARIEL – 13th Appleton Space Conference 6 WARM/HOT EXOPLANETS O, C, N, S (TI, VO, SI) MOLECULES ARE IN GAS FORM Atmospheric pressure 0.01Bar H2O gas CO2 gas CO gas CH4 gas HCN gas TiO gas T ~ 500-2500 K Condensates VO gas H2S gas 1 Bar Gases from interior ARIEL – 13th Appleton Space Conference 7 CHEMICAL MEASUREMENTS TODAY SPECTROSCOPIC OBSERVATIONS WITH CURRENT INSTRUMENTS (HUBBLE, SPITZER,SPHERE,GPI) • Precision of 20 ppm can be reached today by Hubble-WFC3 • Current data are sparse, instruments not absolutely calibrated • ~ 40 planets analysed -
Water, Energy, and Biogeochemical Model (WEBMOD), User’S Manual, Version 1
Water, Energy, and Biogeochemical Model (WEBMOD), User’s Manual, Version 1 Chapter 35 of Section B, Surface Water, of Book 6, Modeling Techniques Techniques and Methods 6–B35 U.S. Department of the Interior U.S. Geological Survey A B C D E F G H I Front Cover. Forested upland watersheds of the Water, Energy, and Biogeochemical Budget Program (A, F, H, I ) and agricultural watersheds of the National Water Quality Assessment Agricultural Chemical Transport Studies (B, C, D, E, G). A, Luquillo, Puerto Rico; B, Mustang River, California; C, Maple Creek, Nebraska; D, DR2 Drain, Washington; E, Morgan Creek, Maryland; F, Panola Mountain, Georgia; G, Sugar Creek, Indiana; H, Trout Lake, Wisconsin; I, Sleepers River, Vermont. Back Cover. Loch Vale watershed, Rocky Mountain National Park, Colorado. Photograph by Austin Seeback, U.S. Geological Survey (Flickr, U.S. Geological Survey, public domain). Water, Energy, and Biogeochemical Model (WEBMOD), User’s Manual, Version 1 By Richard M.T. Webb and David L. Parkhurst Chapter 35 of Section B, Surface Water Book 6, Modeling Techniques Techniques and Methods 6–B35 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior SALLY JEWELL, Secretary U.S. Geological Survey Suzette M. Kimball, Director U.S. Geological Survey, Reston, Virginia: 2017 For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment—visit http://www.usgs.gov or call 1–888–ASK–USGS. For an overview of USGS information products, including maps, imagery, and publications, visit http://store.usgs.gov. -
Table of Artificial Satellites Launched Between 1 January and 31 December 1967
This electronic version (PDF) was scanned by the International Telecommunication Union (ITU) Library & Archives Service from an original paper document in the ITU Library & Archives collections. La présente version électronique (PDF) a été numérisée par le Service de la bibliothèque et des archives de l'Union internationale des télécommunications (UIT) à partir d'un document papier original des collections de ce service. Esta versión electrónica (PDF) ha sido escaneada por el Servicio de Biblioteca y Archivos de la Unión Internacional de Telecomunicaciones (UIT) a partir de un documento impreso original de las colecciones del Servicio de Biblioteca y Archivos de la UIT. (ITU) ﻟﻼﺗﺼﺎﻻﺕ ﺍﻟﺪﻭﻟﻲ ﺍﻻﺗﺤﺎﺩ ﻓﻲ ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﺃﺟﺮﺍﻩ ﺍﻟﻀﻮﺋﻲ ﺑﺎﻟﻤﺴﺢ ﺗﺼﻮﻳﺮ ﻧﺘﺎﺝ (PDF) ﺍﻹﻟﻜﺘﺮﻭﻧﻴﺔ ﺍﻟﻨﺴﺨﺔ ﻫﺬﻩ .ﻭﺍﻟﻤﺤﻔﻮﻇﺎﺕ ﺍﻟﻤﻜﺘﺒﺔ ﻗﺴﻢ ﻓﻲ ﺍﻟﻤﺘﻮﻓﺮﺓ ﺍﻟﻮﺛﺎﺋﻖ ﺿﻤﻦ ﺃﺻﻠﻴﺔ ﻭﺭﻗﻴﺔ ﻭﺛﻴﻘﺔ ﻣﻦ ﻧﻘﻼ ً◌ 此电子版(PDF版本)由国际电信联盟(ITU)图书馆和档案室利用存于该处的纸质文件扫描提供。 Настоящий электронный вариант (PDF) был подготовлен в библиотечно-архивной службе Международного союза электросвязи путем сканирования исходного документа в бумажной форме из библиотечно-архивной службы МСЭ. © International Telecommunication Union HIS list of artificial satellites launched in 1967 was prepared from information provided by TTelecommunication Administrations, the Com m ittee on Space Research (COSPAR), the Goddard Space Flight Center (GSFC), the United States National Aeronautics and Space Administration (NASA), the International Fre quency Registration Board (IFRB), one of the fo ur permanent organs o f the ITU, and from details published in the specialized press. For decayed satellites the data concerning the orbit parameters are those immediately after launching. For the others, still in orbit, the orbit parameters are those reported on 31 De cember 1967 by GSFC. -
Desind Finding
NATIONAL AIR AND SPACE ARCHIVES Herbert Stephen Desind Collection Accession No. 1997-0014 NASM 9A00657 National Air and Space Museum Smithsonian Institution Washington, DC Brian D. Nicklas © Smithsonian Institution, 2003 NASM Archives Desind Collection 1997-0014 Herbert Stephen Desind Collection 109 Cubic Feet, 305 Boxes Biographical Note Herbert Stephen Desind was a Washington, DC area native born on January 15, 1945, raised in Silver Spring, Maryland and educated at the University of Maryland. He obtained his BA degree in Communications at Maryland in 1967, and began working in the local public schools as a science teacher. At the time of his death, in October 1992, he was a high school teacher and a freelance writer/lecturer on spaceflight. Desind also was an avid model rocketeer, specializing in using the Estes Cineroc, a model rocket with an 8mm movie camera mounted in the nose. To many members of the National Association of Rocketry (NAR), he was known as “Mr. Cineroc.” His extensive requests worldwide for information and photographs of rocketry programs even led to a visit from FBI agents who asked him about the nature of his activities. Mr. Desind used the collection to support his writings in NAR publications, and his building scale model rockets for NAR competitions. Desind also used the material in the classroom, and in promoting model rocket clubs to foster an interest in spaceflight among his students. Desind entered the NASA Teacher in Space program in 1985, but it is not clear how far along his submission rose in the selection process. He was not a semi-finalist, although he had a strong application. -
Artificial Earth Satellites Designed and Fabricated by the Johns Hopkins University Applied Physics Laboratory
SDO-1600 lCL 7 (Revised) tQ SARTIFICIAL EARTH SATELLITES DESIGNED AND FABRICATED 9 by I THE JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY I __CD C-:) PREPARED i LJJby THE SPACE DEPARTMENT -ow w - THE JOHNS HOPKINS UNIVERSITY 0 APPLIED PHYSICS LABORATORY Johns Hopkins Road, Laurel, Maryland 20810 Operating under Contract N00024 78-C-5384 with the Department of the Navv Approved for public release; distributiort uni mited. 7 9 0 3 2 2, 0 74 Unclassified PLEASE FOLD BACK IF NOT NEEDED : FOR BIBLIOGRAPHIC PURPOSES SECURITY CLASSIFICATION OF THIS PAGE REPORT DOCUMENTATION PAGE ER 2. GOVT ACCESSION NO 3. RECIPIENT'S CATALOG NUMBER 4._ TITLE (and, TYR- ,E, . COVERED / Artificial Earth Satellites Designed and Fabricated / Status Xept* L959 to date by The Johns Hopkins University Applied Physics Laboratory. U*. t APL/JHU SDO-1600 7. AUTHOR(s) 8. CONTRACTOR GRANT NUMBER($) Space Department N00024-=78-C-5384 9. PERFORMING ORGANIZATION NAME & ADDRESS 10. PROGRAM ELEMENT, PROJECT. TASK AREA & WORK UNIT NUMBERS The Johns Hopkins University Applied Physics Laboratory Task Y22 Johns Hopkins Road Laurel, Maryland 20810 11.CONTROLLING OFFICE NAME & ADDRESS 12.R Naval Plant Representative Office Julp 078 Johns Hopkins Road 13. NUMBER OF PAGES MyLaurel,rland 20810 235 14. MONITORING AGENCY NAME & ADDRESS , -. 15. SECURITY CLASS. (of this report) Naval Plant Representative Office j Unclassified - Johns Hopkins Road f" . Laurel, Maryland 20810 r ' 15a. SCHEDULEDECLASSIFICATION/DOWNGRADING 16 DISTRIBUTION STATEMENT (of th,s Report) Approved for public release; distribution N/A unlimited 17. DISTRIBUTION STATEMENT (of the abstrat entered in Block 20. of tifferent from Report) N/A 18. -
Survey of New Solar Results
SURVEY OF NEW SOLAR RESULTS R.TOUSEY E. O. Hulburt Center for Space Research, U.S. Naval Research Laboratory, Washington, D.C., U.S.A. Abstract. Following a brief historical review, new observations of the sun in the wavelength range 3000 to 20 A are surveyed for the period since about 1958. Vehicles employed have been sounding rockets, the OSO (Orbiting Solar Observatories), balloons for the window 2300-1900 A and for k > 2700 A, and small orbiting observatories such as Solrad, for XUV solar monitoring. Advances have been made in spectral resolution, using echelle gratings and also Fabry-Perot interferometers. Much progress has been made towards increased spatial resolution, to obtain spectra of specific solar features and to analyse the chromosphere and corona. Methods employed include spectrographs that are stigmatic, or that have a stabilized solar image projected onto the slit; slitless objective-type spectrographs; and observations during a total eclipse. Spectra have been obtained of a solar flare, showing its form and intensity in the emission lines between 171 and 630 A. From OSO 4-6 many XUV spectroheliograms and spectra have been obtained over the range 300 to 1350 A, with spatial resolution 35 < 35 arc sec in OSO 6. Photographic XUV spectroheliograms have provided solar images with spatial resolution as great as 3 arc sec in some cases. Although much effort has been spent to increase the accuracy of XUV intensity measurements, a great deal remains to be done before the requirements of solar physics theory are satisfied. Line identification, however, is proceeding well, although more laboratory spectroscopy is needed. -
ESRO SP-72 European Space Research Organisation
ESRO SP-72 I. Proc. ESRO-GRI ESRO SP-72 I. Proc ESRO-GRI European Space Research Organisation Colloquium March 1971 European Space Research Organisation Colloquium March 1971 COLLOQUIUM ON WAVE-PARTICLE INTER II. ESRO SP-72 COLLOQUIUM ON WAVE-PARTICLE INTER II. ESRO SP-72 ACTIONS IN THE MAGNETOSPHERE HI. Texts in English ACTIONS IN THE MAGNETOSPHERE III. Texts in English September 1971 September 1971 iv + 284 pages iv + 284 pages The Colloquium on wave-particle interactions in the magnetosphere held in The Colloquium on wave-particle interactions in the magnetosphere held in Orleans (March 17-19,1971) intended to review the outstanding problems still unsolved Orleans (March 17-19, 1971) intended to review the outstanding problems still unsolved in this field : in this field : — large-scale dynamics of the magnetosphere; — large-scale dynamics of the magnetosphere; — distribution of 'Oasma parameters; — distribution of plasma parameters; — decoupling of n..gnetospheric from ionospheric plasma; — decoupling of magnetospheric from ionospheric plasma; — acceleration and convection mechanisms; — acceleration and convection mechanisms; — substorms; — substorms; — polar wind..., — polar wind..., as well as the theoretical and experimental work needed to solve these problems in the as well as the theoretical and experimental work needed to solve these problems in the light of previous experiments (rocket launchings in auroral zone, Ariel 3 satellite...) light of previous experiments (rocket launchings in auroral zone, Ariel 3 satellite...) and of technical achievements (onboard computers, new sensors...). and of technical achievements (onboard computers, new sensors...). Ensuing discussions attempted to define types of missions which could be carried Ensuing discussions attempted to define types of missions which could be carried out in the future by the Small Scientific Satellites now being considered by ESRO. -
Solar Radiation (SOLRAD) Satellite Summary Table As of 26 March 2004
Solar Radiation (SOLRAD) Satellite Summary Table as of 26 March 2004 Satellite Name Launch Date Transmitter(s) Vanguard 3 18 September 1959 108.00 Mc/s 30 mW FM/PM IRIG 2, 3, 4 & 5 Explorer 7 13 October 1959 19.9915 Mc/s 660 mW FM/AM IRIG 2, 3, 4 & 5 Solrad Dummy 13 April 1960 Inert Test Article Sun Ray 1 22 June 1960 108.00 Mc/s 40 mW FM/AM IRIG Ch 4 & Ch 5 Sun Ray 2 30 November 1960 (Failure) 108.00 Mc/s 40 mW FM/AM IRIG Ch 4 & Ch 5 here Sun Ray 3 29 June 1961 (Partial failure) 108.00 Mc/s Sun Ray 4 24 January 1962 (Failure) 108.09 Mc/s 100 mW FM/AM Sun Ray 4B 26 April 1962 (Failure) 108.00 Mc/s 100 mW FM/AM 20 inch sp Sun Ray 5 Not Launched Sun Ray 6 15 June 1963 136.890 MHz 100 mW FM/AM SolRad 7A 11 January 1964 136.887 MHz 100 mW FM/AM IRIG Ch 3 to 8 SolRad 7B 9 March 1965 136.800 MHz 100 mW FM/AM IRIG Ch 3 to 8 SolRad 8 19 November 1965 137.41 MHz 1W Stored data playback Explorer 30 136.44 MHz 100mW 24 inch sphere Solar Explorer A 136.53 MHz 100mW SolRad 9 5 March 1968 136.41 MHz 500 mW Stored data playback Explorer 37 136.52 MHz 150 mW Primary RT FM/AM IRIG 3 to 8 Solar Explorer B 137.59 MHz 150 mW RT FM/AM IRIG 3 to 7, 12 PCM SolRad 10 8 July 1971 136.38 MHz 250 mW 5W on cmd TM2 - PCM/PM or Stored Data or Stellrad on cmd Explorer 44 137.71 MHz 250 mW TM1 - PAM/PCM/FM/PM RT analog (chs 4-8, COSPAR Ch 7) Solar Explorer-C and digital PCM (ch 12) SolRad 11A & 14 March 1976 137.44 MHz 5W (11A), 136.53 MHz 5W (11B) SolRad 11B 102.4 bps PCM/BiØ-L/PM convolutional encoded (R=½, k=7) Early X-ray missions Name Vanguard 3 Launch Date 1959 September 18.22 UTC SAO ID 1959 ? (Eta) COSPAR ID 1959-07A Catalog No. -
<> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA
1 SATELITES ARTIFICIALES. Capítulo 5º Subcap. 10 <> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA TIERRA. Esta es una relación cronológica de todos los lanzamientos de satélites artificiales de nuestro planeta, con independencia de su éxito o fracaso, tanto en el disparo como en órbita. Significa pues que muchos de ellos no han alcanzado el espacio y fueron destruidos. Se señala en primer lugar (a la izquierda) su nombre, seguido de la fecha del lanzamiento, el país al que pertenece el satélite (que puede ser otro distinto al que lo lanza) y el tipo de satélite; este último aspecto podría no corresponderse en exactitud dado que algunos son de finalidad múltiple. En los lanzamientos múltiples, cada satélite figura separado (salvo en los casos de fracaso, en que no llegan a separarse) pero naturalmente en la misma fecha y juntos. NO ESTÁN incluidos los llevados en vuelos tripulados, si bien se citan en el programa de satélites correspondiente y en el capítulo de “Cronología general de lanzamientos”. .SATÉLITE Fecha País Tipo SPUTNIK F1 15.05.1957 URSS Experimental o tecnológico SPUTNIK F2 21.08.1957 URSS Experimental o tecnológico SPUTNIK 01 04.10.1957 URSS Experimental o tecnológico SPUTNIK 02 03.11.1957 URSS Científico VANGUARD-1A 06.12.1957 USA Experimental o tecnológico EXPLORER 01 31.01.1958 USA Científico VANGUARD-1B 05.02.1958 USA Experimental o tecnológico EXPLORER 02 05.03.1958 USA Científico VANGUARD-1 17.03.1958 USA Experimental o tecnológico EXPLORER 03 26.03.1958 USA Científico SPUTNIK D1 27.04.1958 URSS Geodésico VANGUARD-2A -
A Digital Elevation Model of Miranda's Youngest Corona
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2543.pdf A DIGITAL ELEVATION MODEL OF MIRANDA’S YOUNGEST CORONA, INVERNESS. C. B. Beddingfield1,2; E. J. Leonard3, C. M. Elder3, T. A. Nordheim3, R. J. Cartwright1, C. Cochrane3, L. Regoli4, and D. Atkinson3. ([email protected]) 1SETI Institute, 2NASA Ames Research Center, 3Jet Propulsion Laboratory, California Institute of Technology, 4John Hopkins University Applied Physics Laboratory, MD Background: Miranda is the innermost and ~4.34°), which is notably higher than that of the other smallest of the classical Uranian satellites, with a classical moons (i < 0.13°) [12]. ~470-km-mean-diameter [1]. This satellite has a In our ongoing work, we are investigating geologically complex and highly deformed surface, Inverness Corona, the youngest corona on Miranda highlighted by regions of tectonically resurfaced [13], to improve our understanding of the most recent terrain with low crater densities, termed “coronae” and geologic activity on this moon, and how this activity a large system of normal fault scarps up to 8 km in might be linked to endogenic processes, such as height making up the “Global Rift System,” present tectonism and cryovolcanism [e.g. 4]. Although within the cratered terrain (Figure 1) [2,3]. Verona Voyager 2 only imaged approximately half of Rupes, the 340 Degree Chasma, and the South Pole Miranda’s surface, the full spatial extent of Inverness Tangent Chasma are part of the Global Rift System Corona was captured during the flyby, unlike Arden [3], along with numerous smaller scale faults and and Elsinore Coronae, which were only partially fractures across the cratered terrain.