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    .4IUI4.SA News~" 'National Aeronautics andSpace AdministrationWashington. D.C 20546AC 202 755-8370

    Fe Release IMMEDIATE

    Press Kit Project Atmosphere Explorer-EPej6g,,q5 WyO' 757'*0

    ContentsGENERAL RELEASE ................... ........... *. 1-6ATMOSPHERE EXPLORER SCIENCE INSTRUMENTS........... 7-8AE-E MISSION FACTS AT A GLANCE .................... 9LAUNCH VEHICLE .......................... *....... .10-ilLAUNCH OPERATIONS.... ............................... O..**. 11MAJOR AE-E/DELTA FLIGHT EVENTS.................... 12AE-E/DELTA TEAM ............ 13-14

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    National Aeronautics andSpace AdministrationWashinaton. D.C 20546AC 202 755-8370

    For ReleaseNicholas Panagakos IMMEDIATEHeadquarters, Washington, D.C.(Phone: 202/755-3680)Joe McRobertsGoddard Space Flight Center, Greenbelt, Md.(Phone: 301/982-4955)

    RELEASE NO: 75-290

    SATELLITE TO MEASURE EQUATORIAL OZONE LAYER

    The third in a series of maneuverable, unmannedspacecraft will be launched by NASA this month to studythe upper atmosphere, including Earth's protective ozonelayer above the Equator.

    Atmosphere Explorer E will be launched aboard aDelta rocket from Cape Canaveral, Fla., about Nov. 18.

    Linked through a sophisticated ground computer withscientists in widely scattered parts of the country, AE-Ecarries 12 scientific instruments designed to return in-formation on the Earth's heat balance and energy con-version mechanisms, as well as the flow of heat or energyfrom one hemisphere to the other.

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    The AE-E satellite (Explorer 55 in orbit) also carriesan instrument to measure Earth's ozone layer between 20degrees north and south. Called a backscatter ultravioletspectrometer (BUV), it was added to the spacecraft's payloadlast spring as part of NASA's continuing program to mea-sure the atmospheric distribution of ozone on a globalbasis.

    Information returned by this instrument in conjunc-tion with the others could represent a major step inunderstanding the interaction of upper atmosphereconstituents with solar ultraviolet light and the re-sulting impact on the ozone layer.

    Originally carried on Nimbus-4, a NASA weatherresearch satellite launched into polar orbit fhst theWestern Test Range in 1970, the BUV instrumentation hasbeen measuring the global ozone distribution ever since.As a result, the world's largest data base on atmosphericozone has been gathered by Nimbus, and detailed analysisof the data is currently underway.

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    NASA's Goddard Space Flight Center, Greenbelt, Md.,has management responsibility for the Nimbus and AEseries of spacecraft, as well as the Delta launchvehicle that places them in orbit. RCA Corp., Princeton,N.J., is AE spacecraft prime contractor and McDonnellDouglas Corp., Huntington Beach, Calif., builds theDelta.

    Goddard's Dr. Donald Heath, Principal Investigatoron the BUV instrument, says: "This is a typical exampleof space technology developed in the past being put touse to solve problems of today. In 1970 we knew ozonemeasurement was necessary, but until scientists began tobecome alarmed about the possible depletion of the ozonelayer some 22-25 kilometers (13-15 miles) above us, wewere not aware of the critical necessity to understandwhat is happening there.

    The only way you can get at the problem, that is,measure ozone on a global, seasonal and solar-cyclebasis, is by satellite. Satellite data gathering hasbeen going on for 5-*1/2 ycrs and should continue throughseveral 11-year solar cycles and beyond, to get an ideaof the magnitude of the problem or determine if indeedthere is a problem."

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    Dr. Heath says we will probably have an understandingof important trends on which we can base some decisionshere on Earth, such as whether to ban the widespread use ofaerosol cans using chlorofluoromethanes (CFM), commonly knownby the trade name "Freon." CFMs expelled from aerosolcans slowly, over a period of about 10 years, work theirway up to the ozone layer where sunlight and resultingchemical reactions are believed to cause it to destroyozone.

    AE-E will look at the ozone content in the equatorialregion in conjunction with its sister satellite, AE-D,which is dipping into the atmosphere to sample nitricoxide, one of the controlling agents oL ozone productionand depletion. AE-D was launched in early October 1975.

    The new spacecraft will measure changes in ozone dis-tribution and provide new information on the horizontalscale of the structure in the ozone fields at different al-titudes in the stratosphere over the equator. It also willprovide an opportunity to evaluate the long-term accuracy ofthe Nimbus-4 BUV instrument by comparing newly-calibratedequipment with that launched in 1970. In addition, it willfill the gap between Nimbus-4 and Nimbus-G, scheduled forlaunch in 1978. Nimbus-4, wiLh a design lifetime of onlyone year, cannot be counted ci1 to operate until 1978.

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    AE's low perigee, dipping into the atmosphere at timesto an altitude of some 130 km (80 mi.), will return valuableinformation on changes in the total ozone field. Thisincludes the vertical ozone distribution between 22 km (13mi.) and 50 km (31 mi.) as well as changes in relation tocomposition, structure and dynamics of the entire upper

    atmosphere.

    The spacecraft's initial apogee will be 3000 km(1875 mi.) with a period of 118 minutes and an inclina-tion of 20 degrees.

    The main energy input to the atmosphere is known tocome from the absorption of solar ultraviolet radiation,but a substantial portion also comes from the solar wind(a mass of ionized gas flowing out of the Sun) interactingwith the atmosphere in the polar regions. An immediateconsequence of this interaction can be seen in the aurorae,whose bands of light consume more energy than is used bythe entire United States.

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    The magnitude and variability of this high latitudeheat source which causes worldwide radio blackouts duringgeomagnetic storms is poorly understood. An importantobjective of this mission is to investigate these processesand mechanisms. The 12 instruments aboard AE-E will mea-sure particle fluxes, airglow intensities, plasma densi-ties and temperatures, and neutral densities, temperaturesand compositions at the low altitudes where energy dissipationoccurs as well as solar ultraviolet radiation.

    The spacecraft design, making use of existing techno-logy, is relatively inexpensive. Prime contract custs forall three spacecraft are expected to total about $24 million.

    The AE satellite is a 16-sided polyhedron, 135 centi-meters (53.2 inches) in diameter and 115 cm (45 in.)high. It weighs 720 kilograms (1587 pounds), including107 kg (237 lbs.) of instrumentation.

    Overall program direction is the responsibility ofNASA's Office of Space Science, Washington, D.C., withGoddard providing the spacecraft and rocket manage-ment. Launch operations have been assigned to Kennedy SpaceCenter Unmanned Launch Operations Directorate. RCA Corpora-tion, Princeton, N.J., is the spacecraft prime contractor,and McDonnell-Douglas Corp., Huntington Beach, Calif.,builds the launch vehicle.(END OF GENERAL RELEASE; BACKGROUND INFORMATION FOLLOWS)

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    -7-ATMOSPHERE EXPLORER SCIENCE INSTRUMENTS

    Cylindrical Electrostatic Probes Measure electron tempera-(L. H. Brace and R. F. Theis, GSFC ture and ion and electronand A. Dalgarno, Harvard College concentrations in the orbi-Observatory) tal path of the spacecraft.Atmospheric Density Accelerometer Determine density of the(K. S. W. Champion and F. A. Marcos neutral atmosphere byAir Force Cambridge Research Labs) measurement of satellitedeceleration due to aero-dynamic drag.

    Photoelectron Spectrometer Measure the low energy(J. P. Doering, Johns Hopkins flux and energy distribu-University, and C. 0. Bostrom and tion in the thermosphereJ. C. Armstrong, APL) by means of two electro-static deflection-type elec-

    tron spectrometers.

    Positive Ion Mass Spectrometer Measure the concentrations(BIMS) of thermal positive ions(H. C. Briton, GSFC) and identify major andminor species.

    Airglow PhotometerMeasure the airglow emis-

    (P. B. Hays and G. Carignan, sions for dayglow, nightglowUniversity of Michigan; G. G. and aurora borealisShepherd, York University,Canada, and J. C. G. Walker,Yale University)Solar Extreme Ultraviolet Measure the solar extremeSpectrophotometer (H. E. ultraviolet radiation andHinteregger, D, E. Bedo and and the monochromatic opti-J. E. Manson, Air Force cal depths of the Earth'sCambridge Research Labs) atmosphere.

    Open Source Neucral MassMeasure the densities of

    Spectrometer (A. 0. Nier, various neutral atmosphericW. E. Potter, D. R. Hickman gases, particularly atomicand K. Mauersberger, Univer- oxygen.sity of Minnesota)Neutral Atmosphere Composition Measure concentrations(D. T. Pelz and C. A. Reber, and distributions of neu-GSFC, and G. R. Carignan, tral gas constituents ofUniversity of Michigan' the thermosphere.

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    -8-Neutral Temperature (N W. Spencer Measure atmospheric kineticand H. Niemann, GSFC and G. R. temperature by determiningCarignan, University of Michigan) the response of a mass spec-trometer and baffle tuned

    to neutral nitrogen (N2)in a spherical chamber.Backscatter Ultraviolet Spectro- Measure atmospheric distri-meter (Donald F. Heath, GSFC) bution. f ozone.Planar Ion Trap (RPA) (W. B. Hanson, Measure ion-temperature andand D. R. Zuccaro, University of concentration: DetermineTexas1Dallas) velocity of plasma flow.Solar Extreme Ultraviolet Broad-band photometric measure-Photometer (ESUM) ments of the solar extreme(D. F. Heath and J. Osantowski, ultraviolet irradiance.GSFC) Emphasis on high spectroradio-metric accuracy and long

    term variability of the Sunin EUV.

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    AE-E MISSION FACTS AT A GLANCE

    Launch: From Cape Canaveral, Fla.Launch Vehicle: Two stage Delta with ninesolid fuel strap-on motors.Orbit: Apogee: 3000 kilometers(1875 miles)

    Perigee: 157 kilometers(97 miles)Period: 118 minutesInclination: 20 degrees

    Operating Lifetime: At least one yearSpacecraft Weight: 720 kilograms (1587 pounds)Structure: Drum-shaped (16-sided

    polyhedron),135 centimeters(53.2 inches) in diameterand 115 centimeters (45inches) high. Consists oftwo shills, inner and outer,with solar cells, telemetryantennas and viewing portson outer shell. Inner shellholds 12 scientific instru-ments. 107 kilograms,(237pounds), electronic packages,attitude control system,hydrazine thruster subsystem.

    Power System: Solar cells on exterior ofspacecraft, redundant nickelcadmium batteries. Provides120 watts of power duringnormal operation.

    CQmmunications and Data Handling: Telemetry, tracking andcommand and control and theantennas.

    Telemetry: Pulse-coded Modulation (PCM)Tracking and Data Acquisition; Stations of the Space

    Tracking and Data Network(STDN) operated by GSFC.

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    LAUNCH VEHICLE

    The two-stage Delta 2910 launch vehicle will be usedfor this 117th Delta payload. The vehicle has an overalllength of approximately 35 meters (116 feet) and a maximumbody diameter of 2.48 m (8 ft.). The nominal launch weiqhtis about 130,000 kilograms (290,000 pounds), including thenine booster thrust-augmentation solid motors.

    The first stage is a McDonnell Douglas Astronautics Co.modified Thor booster incorporating nine strap-on Thiokolsolid fuel rocket motors. The booster is powered by an RS-27engine using liquid oxygen and liquid hydrocarbon

    propellants.The main engine is gimbal-mounted to provide pitch and yaw con-trol from liftoff to main engine cutoff (MECO). Two liquidpropellant vernier engines provide roll control throughout firststage operation and pitch and yaw control from MECO to firststage separation.

    The second stage is powered by a TRIW-TR 201 liquid fuelpressure fed engine which is also gimbal-mounted to providepitch and yaw control through second stage burn. A nitrogengas system using eight fixed nozzles provides roll controlduring powered and coast flight as well as pitch and yaw con-trol after second stage cutoff. Two fixed nozzles, fed by thepropellant tank helium pressurization

    system, provide retro-thrust after spacecraft separation.

    The Atmosphere Explorer spacecraft will be attached tothe Delta second stage by means of a standard fitting whichincorporates the separation system.

    The Delta fairing which is attached to the forward faceof the second stage is 560 centimeters (224 inches) long and162.5 cm (65 in.) in diameter. This fairing, which protectsthe spacecraft from aerodynamic heating during the boost flight,is jettisoned as soon as the vehicle leaves the atmosphereshortly after second stage ignition.An all-inertial guidance system consisting of an inertialsensor package and digital guidance computer controls thevehicle and sequence of operations from liftoff to spacecraftseparation. The sensor package provides vehicle attitude andacceleration information to the guidance computer. The guidancecomputer generates vehicle steering commands to each stage tocorrect trajectory deviations by comparing computed positionand velocity against prestored values.

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    -1 1-In addition, the guidance computations perform thefunctions of timing and staging as well as issuing pre-programmed command attitude rates during the open loop andcoast guidance phases.After second stage burnout, the vehicle will be re-oriented so that the spacecraft spin axis is normal to theorbit plane. The desired orbital spin rate will be achievedby rolling the vehicle prior to spacecraft separation.

    LAUNCH OPERATIJNS

    The Kennedy Space Center's Unmanned Launch OperationsDirectorate plays a key role in the preparation and launch ofthe two-stage, thrust-augmented Delta rocket carrying Atmos-phere Explorer-E.Delta 317 will be launched from Pad B at Complex 17,Cape Canaveral.The Delta 117 booster was erected on Pad B and four ofthe nine strap-on solid motors were mated Oct. 22. The remain-ing five solid rocket motors were mated with the booster Oct. 23.The second stage was erected Oct. 24.The AE-E spacecraft arrived at Cape Canaveral Oct. 28and was placed in Hangar S for checkout and prelaunch prepara-tions, The spacecraft was mated with Delta 117 Nov. 7 and thepayload fairing which will protect AE-E during its flightthrough the atmosphere was placed atop the rocket and space-craft several days prior to launch.

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    MAJOR AE-E/DELTA FLIGHT EVENTS

    EVENT TIME ALTITUDE VELOCITYMin./Sec. Kilometers/Miles Ft./Sec.

    Liftoff 0:00 0 0 0Six Solid Motors 0:38 6.0 3.7 2,209Burnout

    Three Solid Motors 0:39 6.4 4 2,210Ignite

    Three Solid Motors 1:18 22 14 3,783Burnout

    Jettison Nine Motor 1:27 26 16 4,074Casings

    Main Engine Cutoff 3:48 100 62 18,234(MECO)

    Stage I/II Separation 3:56 105 65 18,271

    Stage II Ignition 4:01 108 67 18,254Jettison Fairing 4:36 126 78 18,948Stage II First 7:49 158 98 25,628Cutoff (SECO)

    Second Stage Restart 23:50 157 97.5 25,621Second Stage Cutoff 25:12 158 98.2 27,828Stage II/Spacecraft 3^:20 432 268 27,051Separation

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    AE-E/DELTA TEAM

    NASA HeadquartersDr. Noel W. Hinners Associate Adminis tra torfor Space Science

    Dr. Alois W. Schardt Director, Physicsand Astronomy

    Frank W. Gaetano AE Program Manager

    Dr. E. R. SchmerlingAE Program Scientist

    Joseph B. Mahon Director, Launch Vehicleand Propulsion Program

    I. T. Gillam IV Small Launch Vehiclesand InternationalPrograms Manager

    P. T. Eaton Delta Program Manager

    Robert R. Stephens Tracking and Data AnalysisProgram Manager

    Goddard Space Flight Center

    Dr. John F. Clark DirectorDr. Robert S. Cooper Deputy Director

    Robert N. Lindley Director of Projects

    David W. Grimes Project Manager

    Robert C. Weaver Deputy Project Manager,Technical

    John A. Underwood Deputy Project Manager,Resources

    Nelson W. Spencer Project Scientist

    Richard E. Donnelly Experiment Manager

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    David J. Haykin Mission Operations Director

    Robert Baumann Associate Director ofProjects for Delta

    Robert Goss Chief, Mission Integrationand Analysis

    George D. Baker Chief, Mission Integration

    Francis J. Lawrence Mission Integration Engineer

    Tecwyn Roberts Director of Networks

    Albert Ferris Director of Mission andData Operations

    Ed Lowe Network Support Manager

    Roger V. Tetrick Mission Support Manager

    Seaton B. Norman Communications Engineer

    Kennedy Space CenterLee R. Scherer DirectorJohn J. Neilon Director, Unmanned LaunchOperations

    Hugh A. Weston, Jr. Manager, Delta LaunchOperations

    Wayne McCall Chief Engineer, DeltaOperations

    John J. Bunn Spacecraft Coordinator

    ContractorsRCA Corp., Astro-Electronics AE-E SpacecraftDivisionHightstown, N.J.McDonnell Douglas Astronautics Delta Launch VehicleHuntington Beach, Calif.

    i000 November 6, 1975