MSFN Preparing for MM 71

Total Page:16

File Type:pdf, Size:1020Kb

MSFN Preparing for MM 71 Po*i hletw-oeh Pete-on*'’&l C)*du MSFN Preparing For MM 71 ... AN OFFICIAL / PUBLICATION OF.... / The MSFN will support the Mariner USB tracking data. Other prime objec­ Mars 71 (MM 71) launches on May 6 and tives of the experiment will be to prove May 16; the first spacecraft (Mariner-H, the 85-foot station capacity to track NCG-286) is scheduled to precede the effectively in deep space, and to place second spacecraft (Mariner-I, NCG 287) precision frequency standards such as by ten days. The two launches will the GSFC experimental hydrogen masers take place at KSC from the AFETR at several DSN stations to obtain fre­ launch complexes 36A and 36B. quency comparisons with the DSS pri­ mary frequency standards at those sta­ 1The MSFN will provide command, tions. metric, and telemetiy ground support The geodetic experiment will run / to_ the spacecraft and launch vehicle for six months. Each USB station projects, and will conduct a geodetic participating will be used for five or IIP station location experiment to more six tracking periods of one week each. accurately define the coordinates of TECHNICAL “ The MSFN stations that will support iHFB- MSFN USB antennas. 1 INFORMATION this experiment are: ACN, CRO, CYI, The missions present a unique oppor­ BDA, MIL, TEX, GWM, HAW, MAD, BULLETIN tunity to obtain tracking data which can GDS, HSK, and ETC. v r- r~ r~i •*^•"7 1 I be used to generate improved geodetic Unlike the MM-69 planet flyby : J / coordinates for the 30- and 85-foot prime missions, the MM-71 are Mars planet •••THE MANNED SPACE FLIGHT NETWORKt USB tracking stations. The geodetic orbiter missions. The spacecraft will mispositioning of the MSFN stations is provide broad topographic and 1 -" I the major source of error in trajectories thermal coverage, study seasonal Volume 8, Number 3 February 3, 1971 presently being determined from MSFN Continued On Next P nae _______ GODDARD SPACE FLIGHT CENTER LOW-GAIN ANTENNA 1970 Produces Major MANEUVER ENGINE New Findings PROPULSION TANK -2 The United States space program pro­ duced major new scientific findings in SOLAR PANEL -4 1970 as NASA continued its exploration of the moon and beyond. Following up HIGH-GAIN ANTENNA on the historic Apollo 11 and 12 flights, MEDIUM-GAIN ANTENNA scientists reached a number of conclu­ CANOPUS SENSOR sions based on the studies of the lunar CRUISE SUN SENSOR PROPULSION PRESSURIZATION rocks returned to earth and data from TANK -2 automatic recorders left on the moon by TEMPERATURE CONTROL Apollo 12. LOUVERS Among the findings it was noted that: - there is no sign of life, past or present, on the moon. - rocks returned from the moon are older than any found on earth. UV SPECTROMETER - lunar rocks are composed of the ACQUISITION same chemical elements as some found SUN SENSORS -4 NARROW-ANGLE TV on earth, but in unusual proportions. IR INTERFEROMETER SPECTROMETER - and, a new mineral found on the moon has been named Armalcol for the Mariner Mars 71 spacecraft top view. three Apollo 11 astronauts — Arm­ strong, Aldrin and Collins. NASA’sunmanned program also con-, Apollo And Mariner Mars Will Highlight 1971 tributed further to our knowledge of the planets. NASA announced, in May, after a study of enhanced photos taken by Two manned Apollo missions to the scheduled to be crew members on Apollo Mariner spacecraft, that one of Mars’ moon and two unmanned Mariner Mars 15. On this flight, for the first time, two moons, Phobos, appears to be very launches in late spring will highlight an electric lunar roving vehicle will be dark and potato-shaped. NASA’s 1971 space flight program. taken along to extend the expedition’s Another exciting development was the In addition to the Apollo and Mariner range. Scott and Irwin will ride the first positive identification of amino launches, the NASA 1971 space flight Rover, carrying a color TV camera, acids of extraterrestrial (non-earthly) schedule includes a broad range of sci­ over a northern lunar plain cut by the origin. The find, made at NASA’s Ames entific and applications satellites, aer­ Hadley Rille, which is a broad, deep Research Center is probably the first onautical research, and cooperative gorge which runs along the base of the conclusive proof of extraterrestrial space exploration with other countries. 8,000-foot Apennine Mountains. chemical evolution, the chemical pro­ Six months after Apollo 14, on July They will deploy scientific record­ cesses which precede the origin of life. 25, Astronauts David R. Scott, Alfred ers, collect lunar samples, and attempt Continued on Next Page M. Worden, and James B. Irwin are Continued on Next Page Apollo And Mariner Mars Will Highlight 1971 Launches M M 71 Continued From Page One Other launches tentatively scheduled Continued From Page One/ to find evidence on the origin of the for 1971 include: variations in the atmosphere and the strange lunar rilles which resemble the Intelsat (Jan. 25) - a communications surface, and conduct long-term dry river beds found on earth. Samples spacecraft to be orbited for the Inter­ dynamic observations lasting for a may indicate whether water, not yet national Telecommunications Satellite minimum of 90 days. The MM-71 found on the moon, was a factor in its Consortium to supplement its existing missions will vastly increase our formation. satellite network; knowledge of the planet Mars, its The two Mariner Mars T 71 spacecraft NATO-B (Feb. 2) - a communications seasons and atmosphere, and aid in will be launched from Cape Kennedy in satellite which will be operated by the our planning of the first Mars landing May, the second approximately ten North Atlantic Treaty Organization; in 1975—th e Viking mission. days after the launch of the first. Each IMP-I (Feb. 25) - Interplanetary Mon­ will be assigned separate scientific mis­ itoring Platform-I; sions. After injection into orbit around Solrad (February) - a Navy scientific NEW CAMERA USED ON APOLLO 14. Mars in November, they will send back satellite; information via onboard TV cameras ISIS-B (March) - a cooperative Cana- The Apollo 14 astronauts will bring and other instrumentation. dian/NASA scientific satellite mission; back from their lunar expedition some The objective of the project is to ex­ PAET (March) - Planetary Atmosphere of the most revealing photos of the moon plore Mars from orbit long enough to Experiments Test designed to analyze ever taken. Using a modified aerial observe about 70 percent of the planet1 s unknown planetary atmospheres; reconnaissance camera, CMP Stuart A. surface from an altitude of about 1,000 Barium ion cloud (April) - a cooperative Roosa will photograph future candidate m iles, and to record the seasonal chang­ project with West Germany; Apollo landing sites as his spacecraft ing of surface marks such as the wave OSO-H (April) - Orbiting Solar Obser­ swoops within 10 miles of the central of darkening as seen from earth. vatory-H for sun studies; highlands near the crater Descartes. In the NASA aeronautical program, SSS-A (May) - Small Scientific Satel­ The pictures should show the lunar the supercritical wing, a revolutionary lite-A to be launched from the San surface at two or three feet resolution, new airfoil that may be used either to Marco platform off the coast of Kenya; making it possible to recognize boulders permit future subsonic jets to cruise at UK-4 (June) - a cooperative scientific and craters as small as six feet in diam­ substantially higher speeds or to permit satellite project with the United King­ eter. This resolution is 10 times structural weight savings on moderate- dom; greater than that achieved by previous speed aircraft, will receive extensive Intelsat (July-September); Apollo lunar flights. testing in 1971. AFCRL-A (September) - a magnetic storm satellite for the Air Force Cam^ A thin version of the wing has been bridge Research Laboratories; fitted to a Navy F-8 plane at the NASA Intelsat (October-December); Flight Research Center in California, OAO-C (late in the year) - Orbiting and will get its first flight tryout in the Astronomical Observatory C; spring. A thick version of the airfoil, CAS-A (late in the year) - Cooperative fitted to a Navy T2-C, will receive con­ Applications Satellite a cooperative tinued flight tests at the North American American and French meteorological Rockwell aviation facilities in Ohio. studies. 1970 Produces Major New Findings Continued From Page One Einstein’s predictions were right, to Huge hydrogen clouds ‘were discov­ within two to four percent. ered by two NASA satellites. In January, During the year, three meteorologi­ Orbiting Astronomical Observatory-2 cal satellites [Improved TIROS Opera­ found a hydrogen cloud as large as the tional Satellite-1, Nimbus-4 andNOAA- sun surrounding the comet Tago-Sato- 1 (National Oceanic and Atmospheric Kosaka. Another enormous cloud, this Administration) ] were successfully one 10 times larger then the sun, was launched, returning excellent data. located in April by Orbiting Geophysical Three communications satellites Observatory-5 around Comet Bennett. were successfully launched, two for A record amount of data on the 1970 COMSAT, and one for DOD. Mitchell, Shepard, and Roosa stand in front of solar eclipse was gathered in March as The final launch of the year was the Apollo 14 prior to Jan 31 liftoff. a result of a rocket barrage from NA SA1 s Small Astronomy Satellite-A which is Wallops Island station. Scientists are investigating X-ray sources in the ce­ The Technical Information Bulletin is published still analyzing ground and spacecraft lestial sphere. Launched from the San twice monthly by the Manned Flight Operations observations as well as data from the 31 Marco platform in the Indian Ocean off Division for Network personnel only.
Recommended publications
  • AERONET Annual Review
    AERONET Annual Review Colleagues, your AERONET sun and sky scanning network has continued to be a valued resource for basic aerosol research, satellite validation, global and regional aerosol model validation and synergism with field campaigns, in situ and RS observations. Following is my tome on our current state, issues we are facing and plans for the future. 1.0 Introduction and News 2.0 Calibration 3.0 Issues 4.0 Future Developments 5.0 Related Initiatives **Note** Wayne Newcomb, our good friend and primary person responsible for keeping instruments functional network wide and maintaining the swapout rotation through the system among many other things, has made progress in his battle with cancer. After two weeks on life support and multiple surgeries, he’s breathing on his own, talking and is annoyed that he wasn’t able to vote. We’re encouraged by his determination and strength. We need everyone’s help to fill the void left by his absence. We especially need everyone’s support to keep their equipment running in the field. Please see the proactive site manager section under ‘3.0 Issues’. 1.0 Introduction and News I’m very happy to announce the third AERONET workshop and conference to be held in mid August 2009 at or near Hangzhou, China. Although the details will be forthcoming in the months ahead, the plan is for a combined technical and training forum and aerosol science conference that will emphasize surface, airborne and satellite research with several themes. Our host and organizer will be Prof. Jiang Hong of Zhejiang Forestry University and facilitated by Prof.
    [Show full text]
  • Jacques Tiziou Space Collection
    Jacques Tiziou Space Collection Isaac Middleton and Melissa A. N. Keiser 2019 National Air and Space Museum Archives 14390 Air & Space Museum Parkway Chantilly, VA 20151 [email protected] https://airandspace.si.edu/archives Table of Contents Collection Overview ........................................................................................................ 1 Administrative Information .............................................................................................. 1 Biographical / Historical.................................................................................................... 1 Scope and Contents........................................................................................................ 2 Arrangement..................................................................................................................... 2 Names and Subjects ...................................................................................................... 2 Container Listing ............................................................................................................. 4 Series : Files, (bulk 1960-2011)............................................................................... 4 Series : Photography, (bulk 1960-2011)................................................................. 25 Jacques Tiziou Space Collection NASM.2018.0078 Collection Overview Repository: National Air and Space Museum Archives Title: Jacques Tiziou Space Collection Identifier: NASM.2018.0078 Date: (bulk 1960s through
    [Show full text]
  • National Reconnaissance Office Review and Redaction Guide
    NRO Approved for Release 16 Dec 2010 —Tep-nm.T7ymqtmthitmemf- (u) National Reconnaissance Office Review and Redaction Guide For Automatic Declassification Of 25-Year-Old Information Version 1.0 2008 Edition Approved: Scott F. Large Director DECL ON: 25x1, 20590201 DRV FROM: NRO Classification Guide 6.0, 20 May 2005 NRO Approved for Release 16 Dec 2010 (U) Table of Contents (U) Preface (U) Background 1 (U) General Methodology 2 (U) File Series Exemptions 4 (U) Continued Exemption from Declassification 4 1. (U) Reveal Information that Involves the Application of Intelligence Sources and Methods (25X1) 6 1.1 (U) Document Administration 7 1.2 (U) About the National Reconnaissance Program (NRP) 10 1.2.1 (U) Fact of Satellite Reconnaissance 10 1.2.2 (U) National Reconnaissance Program Information 12 1.2.3 (U) Organizational Relationships 16 1.2.3.1. (U) SAF/SS 16 1.2.3.2. (U) SAF/SP (Program A) 18 1.2.3.3. (U) CIA (Program B) 18 1.2.3.4. (U) Navy (Program C) 19 1.2.3.5. (U) CIA/Air Force (Program D) 19 1.2.3.6. (U) Defense Recon Support Program (DRSP/DSRP) 19 1.3 (U) Satellite Imagery (IMINT) Systems 21 1.3.1 (U) Imagery System Information 21 1.3.2 (U) Non-Operational IMINT Systems 25 1.3.3 (U) Current and Future IMINT Operational Systems 32 1.3.4 (U) Meteorological Forecasting 33 1.3.5 (U) IMINT System Ground Operations 34 1.4 (U) Signals Intelligence (SIGINT) Systems 36 1.4.1 (U) Signals Intelligence System Information 36 1.4.2 (U) Non-Operational SIGINT Systems 38 1.4.3 (U) Current and Future SIGINT Operational Systems 40 1.4.4 (U) SIGINT
    [Show full text]
  • 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.
    [Show full text]
  • Table of Artificial Satellites Launched in 1971
    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 A COSMOS-428 1971 57A E 0 COSMOS-429 1971 61A COSMGS-430 1971 62A COSMOS-431 1971 65A APOLLO-14 1971 8A COSMOS-432 1971 66A EOLE 1971 71A OAR-901 1971 67C APOLLO-15 1971 63A COSMOS-433 1971 68A EXPLORER-43 1971 19A CAR-907 1971 67D APOLLO-15 CSUB•SAT 3 1971 63D COSMOS-434 1971 69A EXPLORER-44 1971 58A OREOL-1 1971 119A ARIEL-4 1971 109A COSMOS-435 1971 72A EXPLORER-45 1971 96A OSO- 7 1971 83A COSMOS-436
    [Show full text]
  • Space Test Program
    The Space Congress® Proceedings 1973 (10th) Technology Today and Tomorrow Apr 1st, 8:00 AM Space Test Program Neal T. Anderson Project Officer, HQ SAMSO/Spaee Test Program, Los Angeles, CA 90009 Follow this and additional works at: https://commons.erau.edu/space-congress-proceedings Scholarly Commons Citation Anderson, Neal T., "Space Test Program" (1973). The Space Congress® Proceedings. 4. https://commons.erau.edu/space-congress-proceedings/proceedings-1973-10th/session-6/4 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in The Space Congress® Proceedings by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. SPACE TEST PROGRAM Neal T. Anderson, Capt, USAF Project Officer HQ SAMSO/Spaee Test Program Los Angeles, CA 90009 ABSTRACT The Department of Defense Space Test Program is a certain operational payloads. The only limitation unique organization dedicated to stimulating space- on this charter is that the payloads must not be related technology by providing launch and orbital authorized their own means of spaceflight. The support for research and development payloads. Program was never intended to be a launch agency This paper delineates program management techniques, for the large space programs. past accomplishments, and current activities. The benefit to the DOD is discussed. To achieve this objective a governing philosophy was established which required the Program to: INTRODUCTION • be comprehensive in scope In large measure the military power of the United • select and support the most States depends upon the possession of space systems beneficial payloads which are products of superior technology.
    [Show full text]
  • The Relation Betweeg Solar Cell Flight Performance Data and Materials and Manufacturing Data Report No. 3 Third Quarterly Report
    The Relation BetweeG Solar Cell Flight Performance Data and Materials and Manufacturing Data Report No. 3 Third Quarterly Report Contract No. NASW-1732 Prepared by The CARA Corporation 101 N. 33rd Street Philadelphia, Pennsylvania ’S. R. Pollack, Ph.D. G. R. Zin, P’h.D. Principal Investigator L. A. Girifalco, Ph.D. Staff Scientists ABS TRACT This quarter was spent in acquiring data for the flights chosen for study in the last quarter. Analysis of the environment for the individual flights has begun. This work is progressing with the viewpoint of trying to simplify the environmental specification. The most difficult aspect of the environmental analysis is the speci- fication of the vehicle's thermal history. The vehicles under study are therefore being grouped according to subclassifica- tions based on the nature of the vehicle as the first attempt to find any performance correlations. All of the specific data for the flights under study have been extracted from the literature obtained from the computer searches conducted earlier. These data are incomplete and in- adequate for this study. Examples of the nature of this data were reported in the last quarterly,report and are shown in 8 this report. The data required for this study must be obtained by personal contacts with individuals who have been connected with the various flights. The appropriate individuals to contact have been identified for 75 of the 77 flights included in this study. These people have been and are being contacted to obtain the required data. i Table of Contents Fage I. Introduction 1 11. The Selected Flights and Environment 3 111.
    [Show full text]
  • Table of Contents
    THE CAPE Military Space Operations 1971-1992 by Mark C. Cleary 45th Space Wing History Office Table of Contents Preface Chapter I -USAF Space Organizations and Programs Table of Contents Section 1 - Air Force Systems Command and Subordinate Space Agencies at Cape Canaveral Section 2 - The Creation of Air Force Space Command and Transfer of Air Force Space Resources Section 3 - Defense Department Involvement in the Space Shuttle Section 4 - Air Force Space Launch Vehicles: SCOUT, THOR, ATLAS and TITAN Section 5 - Early Space Shuttle Flights Section 6 - Origins of the TITAN IV Program Section 7 - Development of the ATLAS II and DELTA II Launch Vehicles and the TITAN IV/CENTAUR Upper Stage Section 8 - Space Shuttle Support of Military Payloads Section 9 - U.S. and Soviet Military Space Competition in the 1970s and 1980s Chapter II - TITAN and Shuttle Military Space Operations Section 1 - 6555th Aerospace Test Group Responsibilities Section 2 - Launch Squadron Supervision of Military Space Operations in the 1990s Section 3 - TITAN IV Launch Contractors and Eastern Range Support Contractors Section 4 - Quality Assurance and Payload Processing Agencies Section 5 - TITAN IIIC Military Space Missions after 1970 Section 6 - TITAN 34D Military Space Operations and Facilities at the Cape Section 7 - TITAN IV Program Activation and Completion of the TITAN 34D Program Section 8 - TITAN IV Operations after First Launch Section 9 - Space Shuttle Military Missions Chapter III - Medium and Light Military Space Operations Section 1 - Medium Launch Vehicle and Payload Operations Section 2 - Evolution of the NAVSTAR Global Positioning System and Development of the DELTA II Section 3 - DELTA II Processing and Flight Features Section 4 - NAVSTAR II Global Positioning System Missions Section 5 - Strategic Defense Initiative Missions and the NATO IVA Mission Section 6 - ATLAS/CENTAUR Missions at the Cape Section 7 - Modification of Cape Facilities for ATLAS II/CENTAUR Operations Section 8 - ATLAS II/CENTAUR Missions Section 9 - STARBIRD and RED TIGRESS Operations Section 10 - U.S.
    [Show full text]
  • RADIATIONS FROM21 the SUN 1 -Year Solar Cycle Variation Is
    RADIATIONS FROM21 THE SUN By HERBERT FRIEDMAN E. 0. HULBURT CENTER FOR SPACE RESEARCH, NAVAL RESEARCH LABORATORY, .WASHINGTON, D.C. During the IQSY, the minimum of the solar sunspot cycle was observed, and all solar activity phenomena reached their lowest ebb in mid-1964. The measure of an 1 -year solar cycle variation is different for each activity phenomenon. In inte- grated visible light, characterized by a temperature of about 60000 K, no solar variation is vet clearly measurable. P'henomena produced ill temperature regimes of a few tens of thousands of degrees (solar chromosphere) cycle from maximum to minimum as much as 50 per cent. In the few-hundred-thousand-degree range (quiescent corona), the variations are by factors of .3 to 5. In the active corona, temperatures reach several million degrees and the resulting X-ray emission varies by a factor of 7 at long wavelengths (.50 A) to greater than 500 at short wave- lengths (1-S A). The shortest-wavelength X rays are a major controlling influence on the quality of short-wave radio communication. The IQSY provided an opportunity to establish the quiet background level of solar activity. Against this background it was of particular interest to observe the development of individual disturbances in 1965-66 before the sun became so active that multiple events, occurring in overlapping time sequence, confused the indi- vidual analyses. A solar activity center (CA) develops in all area about one-tenth the solar disk. Its development is accompanied by the transient appearance of sunspots, faculae, plages, flares, surges, prominences, coronal condensations, and the emission of radio bursts, X rays, and solar cosmic rays.
    [Show full text]
  • NASA Is Not Archiving All Potentially Valuable Data
    ‘“L, United States General Acchunting Office \ Report to the Chairman, Committee on Science, Space and Technology, House of Representatives November 1990 SPACE OPERATIONS NASA Is Not Archiving All Potentially Valuable Data GAO/IMTEC-91-3 Information Management and Technology Division B-240427 November 2,199O The Honorable Robert A. Roe Chairman, Committee on Science, Space, and Technology House of Representatives Dear Mr. Chairman: On March 2, 1990, we reported on how well the National Aeronautics and Space Administration (NASA) managed, stored, and archived space science data from past missions. This present report, as agreed with your office, discusses other data management issues, including (1) whether NASA is archiving its most valuable data, and (2) the extent to which a mechanism exists for obtaining input from the scientific community on what types of space science data should be archived. As arranged with your office, unless you publicly announce the contents of this report earlier, we plan no further distribution until 30 days from the date of this letter. We will then give copies to appropriate congressional committees, the Administrator of NASA, and other interested parties upon request. This work was performed under the direction of Samuel W. Howlin, Director for Defense and Security Information Systems, who can be reached at (202) 275-4649. Other major contributors are listed in appendix IX. Sincerely yours, Ralph V. Carlone Assistant Comptroller General Executive Summary The National Aeronautics and Space Administration (NASA) is respon- Purpose sible for space exploration and for managing, archiving, and dissemi- nating space science data. Since 1958, NASA has spent billions on its space science programs and successfully launched over 260 scientific missions.
    [Show full text]
  • NASA, the First 25 Years: 1958-83. a Resource for the Book
    DOCUMENT RESUME ED 252 377 SE 045 294 AUTHOR Thorne, Muriel M., Ed. TITLE NASA, The First 25 Years: 1958-83. A Resource for Teachers. A Curriculum Project. INSTITUTION National Aeronautics and Space Administration, Washington, D.C. REPORT NO EP-182 PUB DATE 83 NOTE 132p.; Some colored photographs may not reproduce clearly. AVAILABLE FROMSuperintendent of Documents, Government Printing Office, Washington, DC 20402. PUB TYPE Books (010) -- Reference Materials - General (130) Historical Materials (060) EDRS PRICE MF01 Plus Postage. PC Not Available from EDRS. DESCRIPTORS Aerospace Education; *Aerospace Technology; Energy; *Federal Programs; International Programs; Satellites (Aerospace); Science History; Secondary Education; *Secondary School Science; *Space Exploration; *Space Sciences IDENTIFIERS *National Aeronautics and Space Administration ABSTRACT This book is designed to serve as a reference base from which teachers can develop classroom concepts and activities related to the National Aeronautics and Space Administration (NASA). The book consists of a prologue, ten chapters, an epilogue, and two appendices. The prologue contains a brief survey of the National Advisory Committee for Aeronautics, NASA's predecessor. The first chapter introduces NASA--the agency, its physical plant, and its mission. Succeeding chapters are devoted to these NASA program areas: aeronautics; applications satellites; energy research; international programs; launch vehicles; space flight; technology utilization; and data systems. Major NASA projects are listed chronologically within each of these program areas. Each chapter concludes with ideas for the classroom. The epilogue offers some perspectives on NASA's first 25 years and a glimpse of the future. Appendices include a record of NASA launches and a list of the NASA educational service offices.
    [Show full text]
  • Explorer Fact Sheet
    NASA Facts National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt, Maryland 20771 FS-1998(10)-018-GSFC EXPLORERS: SEARCHING THE UNIVERSE FORTY YEARS LATER Evolution of the Explorer Missions The First Decade: 1958-1967 From the days of the early explorers like During this period a total of 35 Explorer Christopher Columbus and Magellan, there has missions were successfully launched, leading to always been an inherent desire in humanity to many wonderful discoveries. The mysterious explore his surroundings. From the exploits of saturation of the Explorer 1 radiation counters at those early knowledge seekers, many incredible 600 miles above the Earth’s surface led Professor discoveries were made. So it is fitting and James A. Van Allen to suggest the existence of a understandable that the first spacecraft launched dense belt of radiation around the Earth. This, of by the Army Ballistic Missile Agency on Jan. 31, course, became the now well known Van Allen 1958 was named “Explorer”. Radiation Belt. Since the first mission more than 70 U.S. and cooperative international scientific space missions have been part of the much celebrated Explorer program. Explorer satellites have made impres- sive discoveries: Earth’s magnetosphere and gravity field; the solar wind; micrometeoroids; ultraviolet, cosmic, and X-rays; ionospheric physics; solar plasma; energetic particles; and atmospheric physics. They’ve also investigated air density, radio astronomy, geodesy, and gamma ray astronomy. Some Explorer spacecraft have traveled to other planets, and some have monitored the Sun. The mission of the Explorers Program is to provide frequent flight opportunities for scientific investigations from space.
    [Show full text]