(MPD) Thrustor for Space Applications

Total Page:16

File Type:pdf, Size:1020Kb

(MPD) Thrustor for Space Applications XXXX so NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Technical Report 32-1196 A Critical Review of the Magnetop/asmadynamic (MPD) Thrustor for Space Applications Noble M. Nerheim Arnold J. Kelly .__'_ CFSTI PRICE(S) $ __ Hard copy (HC) J_°'_ M_crof_che (MF)___ t {5"- __ ff 653 July 65 JET PROPULSION LABORATORY CALIFORNIA INSTITUTi OF TICHNOLOeY PASADENA, ¢ALePORNIA February 15, 1968 i XXXX-O02 Nb, TIONAL AERONAUTICS AND SPACE ADMINISTRATION Technical Report 32-1196 A Critical Review of the Magnetoplasmadynamic (MPD) Thrustor for Space Applications Noble M. Nerheim Arnold J. Kelly Approvedby: _r D. R. Bartz,ManF/_er Researchand Advanced ConceptsSection JET PROPULSION LABORATORY CALIFORNIA INITITUTE OF TECHNOLOGY PASADENA, CALIFORNIA February 15, 1968 i XXXX-O03 _ m TECHNICAL REPORT32.1196 Copyright © 1968 Jet PropulsionLaboratory California Instituteof Technology Prepared UnderContract No. NAS 7-100 National Aeronautics& :SpaceAdministration -L ¢,' 4 i XXXX-O04 Contents Part h Applicationof the MPD Thrustorto SolarElectricSpaceMissions h Introduction ........................ I U. Purposeof the Survey .................... 2 llh Solar ElectricSpacecraftCharacteristics .............. 2 IV. Requirementsfor a Solar ElectricPropulsionSystemThrustor ...... 3 A. Lifetime......................... 3 B. Performance ....................... 3 C. ThrustLeveland Throttlability................. 4 i I Part II. Scopeof the Survey I. Sources of Information .................... 5 II. A Description of the MPD Thrustor ................ 5 IIh History .......................... 6 Part III. ExistingTechnology I. Early Development ...................... 9 II. Propellant Selection ..................... 10 III. Thrustor Configurations .................... 12 : IV. Test Facilities ........................ 17 _ A. PowerSupplies ...................... 17 B. VacuumSystems...................... 17 V. Test Proceduresand Performance Measurements .......... 18 A. EngineOperatingVariables .................. 18 B. TestProcedures ...................... 20 C. Measurementof OperatingVariables............... 20 JPL TECHNICAL REPORT32.1196 iii I XXXX-O05 Contents (contd) l VI. Environmental Factors .................... 20 A. Entrainment ....................... 21 B. InteractionsWith TestHardware ................ 24 i VII. Experimental Results ..................... 25 A. Performance ....................... 25 B. ThermalEfficiencies .................... 35 C. DiagnosticMeasurements................... 41 i Part IV. Theory _' h Introduction ........................ 49 Ih AElectrom. MPDEngiagnetineOcAcperationcelerationWithMechanismNo ExternaslM.............agneticField ........ 515' B. MPDEngineOperationWith a StrongExternallyApplied ! MagneticField ...................... 54 C. ThrustorOperatingCharacteristics................ 65 III. ElectrothermalAcceleration Processes............... 69 • A. Introduction ....................... 69 B. AnElectrothermalModelfor a Cesium-FedEngine .......... 69 C. AnElectrothermalModelfor Hydrogen .............. 70 IV. Summary ......................... 7i PartV. Discussion h Reliability of Performance Data ................. 73 A. Entrainment ....................... 73 B. InteractionsWith the Vacuuml_,_k Walk. ............. 83 C. VoltageMode Variations................... 83 Ih The Effectof FeedRate on Thrustor Performunce .......... 84 III. Statusof TheoreticalStudies .................. 85 A. Summaryof TheoreticalProblems................ 85 B. AccelerationMechanismsar,d EnergyAdditionProcesses........ 86 iv JPL TECHNICAL aPORT 32-1 I XXXX-O06 Contents (contd) C. CommonAssumptions .................... 88 D. ExperimentalVerificationof Theories............... 91 E. TheRoleof Hall CurrentsinMPDThrustors............. 94 IV. MPD Magnet Systems..................... 95 A. MagnetSystemsUsedWith ExperimentalEngines........... 95 B. FlightConfigurations ................... 95 Part VI. Conclusions I. High ThrustDensity ..................... 99 II. Favorable Current-Voltage Operating Characteristics ........ 99 III. Lifetime .......................... 100 IV. Throttlability ....................... 100 V. ThrustLevel ........................ 100 i VII.Vi. PerformanceSummary ................................................. 100102 References .......................... 102 Tables 1. Somepropertiesof commonlyusedpropellants ........... 11 _ 2. Nomenclatureusedto describevariousefficiencies .......... 12 3. Comparisonof MPDarc jet voltageandthrustfor propellantinjection : throughthe engineand propel!antinjectionoutsidethe engine ...... 21 • 4. Comparisonof thermalefficiencieswith predictedvalues ........ 38 = S. Comparisonof the observedand predictedslopesof the _* voltage--magneticfieldcharacteristics 67 '; 6. Ionizationfractionin theexhaustof thehydrogen-fedX-2C _ MPDengine ....................... 76 "_ 7. Ionizationfractionin theexhaustof the ammonia-_edX.2C ._. MPDengine ....................... 79 _- 8. Estimatedweightsof cylindricalbarmagnetsto produce * the field far MPDthrustors................... 97 ' JPL TECHNICAL REPORT32-1196 v I XXXX-O07 Contents (contd) Figures 1. AVSSDX-2CMPDthrustorusedwith hydrogenand ammonia....... 12 2. Avco-EverettMc_gneticAnnular Arc:(a)Early (1961)configuration usedwith argon and helium and (b)prescnt MAARCused with hydrogen and ammonia .................. 13 3. Early (1964Jmodel of EOShydrogen-fed MPDacce',erator ........ 13 4. EOSH._-Ihydrogen-fedHall currentaccelerator ........... 13 5. Giannlni hydrogen-fedThemo-lonicAccelerator with tungsten-linedanode..................... 13 6. Giannini hydrogen-fed Thermo-lonicAccelerator ........... 14 7. Giannini hydrogen-fedMPDaccelerator .............. 14 8. Low-power(SkW) Gionnini hydrogen-fedaccelerator ......... 14 ! 9. Low-power (10kW) EOSH..-4hydrogen-fed Hall current accelerator .... 14 J i 10. AVSSDX-7CRradiation-cooledMPDthrustorusedwith ammonia 15 11. AVSSDX-7CMPDthrustor usedwith ammonia ............ 1S 12. AVSSDalkali metalMPDthrustorusedwith cesiumand lithium ...... 16 13. AVSSDradiation-cooled alkali metalMPDthrustor .......... 16 14. EOSlithium-fed Hall currentaccelerators ............. 16 15. EOSalkali metal Hall currentaccelerator ............. 16 16. EOSlithium-fed Hall currentaccelerator, Model LAJ-BF.1 ........ 17 17. EOSHall currentaccelerator,Model LAJ-AF-BG-1 .......... 17 18. Giannini lithium-fed MPDthrustor ................ 17 19. Accei_r,_terusedby NASA Langleyfor diagnosticstudieswith argon .... 18 20. PulsedMPDaccelerator investigatedby Lovberg ........... 19 21. Thrustvsinput power of thehydrogen-fueledAVSSDX-2Cengine ..... 23 22. Overall efficiencyvsspecificimpulseof hydrogen-fueledengines ..... 24 23. Overall efficiencyvs specificimpulseof Gianninithrustorsshowing anodethroatdiameter t the effectsof variationsof the and very strongapplied magneticfields ................. 28 24. Overall efficiencyvsspecificimpulseof ummonia.fedengines ...... 30 25. A comparisonof the overallperformanceof water-cooledand radiation-coo_edammonia-fedthrustors .............. 30 26. Overall efficiencyvsspecificimpulseof enginesoperatedwith alkali metalpropellants.................... 32 _J vi JPL TECHNICAL REPORT 32.119 XXXX-O08 Contents (contd) Figures (contd) 27. Overall efficiencyvsspecificimpulseof enginesoperatedwithLi-H2 andLi-N2 bipropellants ................... 33 28. Performanceof miscellaneouspropellants ............. 34 29. Correlationof the thermalefficiencyof the AVSSDhydrogen-fed X-2Cenginewiththe arc voltage ................ 36 30. Anodevoltagevsarc currentfor theX-7C-4engine .......... 37 31. Summaryof thethermalefficienciesvsinputpower,showingthe dependenceonvoltagemodes ................. 38 32. Correlationof the thermalefficiencyof the Gianninithrustorwith thespecificimpulse ..................... 39 33. Correlationof the thermalefficiencyof Gianninithrustorsand oneset of data fromtheAVSSDX-2Cenginewiththeplasmaspecificenthalpy 39 34. Effectof magneticfield strengthonanodepower lossfor sodium and potassium....................... 41 35. Hall-effectsensousedr to measurecurr_ntdensityinexhaustplume .... 42 36. Rogowskicoilusedby Avco-Eve:ttf to measurecurrentloopsinthe exhaustof theMAARC .................... 42 37. Axial and radial distributionsof axial currentdensityand applied magneticfield .................... 43 38. Variationof the cathodetip pressureandthe arc chamberpressure asa functionof the appliedarc current .............. 46 39. Variationof thecathodetip pressureandthearc chamberpressure of the AVSSDengin,,withincreasingappliedfield strength ....... 46 40. Schematicdrawingof theprobe usedto measurethe thrustprofiles inthe MAARCl,xperiments .................. 47 41. Profilesobtainedwith thepu: probe inthe exhaustof the Avco-Everett MAARC operatedon hydrogen ................. 47 42. Schematicdiagramof the pu probe u._edin the MAARC ........ 48 43. Schemahcof an MPDengine .................. 5?. 44. A modelforHall accelerationin an MPDengine ........... 58 45. An analyticalmodelof the magneticswirlmechanism ......... 60 46. One modelof themechanismsproposedfor the EOSALPHA ....... 62 47. Comparisonof thrustsobtainedfromthruststandmeasurementsand thrustdensityprofiles .................... 78 48. Thrustefficiencyvsspecificimpulsefor theAVSSDammonia-fed X-2Cenginefora numberof applied magneticfield strengths ...... 80 JP£ TECHNICAL REPORT32.1194 vii i XXXX-O09 Contenls (contd) Figures (contd) 49. Thru:,tefficiencyvsspecificimpulsefor the AVSSDammonia-fed X-7engine ........................ 81 50. Twoexamplesof the variationinthe performanceof the EOS
Recommended publications
  • Special Presentation by Wassim Jabi, Quentin Jones, Katia
    Special Presentation by Wassim Jabi, Quentin Jones, Katia Passerini, Cristian Borcea, and Theodore Hall, “Fostering Creativity in Ubiquitous Social Computing through Casual and Formal Interactions in Interdisciplinary Design Studios”, Tables 1 This project aims to foster "CreativeIT": using information technology to enhance creativity in design, and applying creative design processes employed in disciplines such as architecture to enhance information technology. One aspect of this project is an interactive touch-screen poster display that enables two-way communication between designers, other team members, and the general public. Poster authors prepare their presentations in the form of web pages and submit the URIs to the display manager. The URIs are placed in an XML poster database on a networked server. The display kiosk software updates its poster list from the XML file periodically, displays the posters in sequence, and places thumbnails in a selection area. Viewers can give feedback on any poster that interests them through graffiti-style interaction with the touch-sensitive display, and e-mail the marked-up poster back to the author. This free-form feedback is a vital part of the creative process. Ikemefuna Chukwuemeka Agbanusi, Senior Student in Mathematics, “Dissecting the Phase Response Curve of a Bursting Neuron”, (advised by Amitabha Bose, advisors Amitabha Bose, Farzan Nadim and Jorge Golowasch), Table 52 We define and analyze the Phase Response Curve (PRC) of an endogenous neuronal oscillator. The PRC measures how an oscillator responds to the timing of stimulus. We utilize a Morris-Leccar type model to reproduce some of the phenomena observed in laboratory experiments on the PD neuron in the Stomatogastric Ganglion of the crab, Cancer borealis.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • Planetary Surfaces
    Chapter 4 PLANETARY SURFACES 4.1 The Absence of Bedrock A striking and obvious observation is that at full Moon, the lunar surface is bright from limb to limb, with only limited darkening toward the edges. Since this effect is not consistent with the intensity of light reflected from a smooth sphere, pre-Apollo observers concluded that the upper surface was porous on a centimeter scale and had the properties of dust. The thickness of the dust layer was a critical question for landing on the surface. The general view was that a layer a few meters thick of rubble and dust from the meteorite bombardment covered the surface. Alternative views called for kilometer thicknesses of fine dust, filling the maria. The unmanned missions, notably Surveyor, resolved questions about the nature and bearing strength of the surface. However, a somewhat surprising feature of the lunar surface was the completeness of the mantle or blanket of debris. Bedrock exposures are extremely rare, the occurrence in the wall of Hadley Rille (Fig. 6.6) being the only one which was observed closely during the Apollo missions. Fragments of rock excavated during meteorite impact are, of course, common, and provided both samples and evidence of co,mpetent rock layers at shallow levels in the mare basins. Freshly exposed surface material (e.g., bright rays from craters such as Tycho) darken with time due mainly to the production of glass during micro- meteorite impacts. Since some magnetic anomalies correlate with unusually bright regions, the solar wind bombardment (which is strongly deflected by the magnetic anomalies) may also be responsible for darkening the surface [I].
    [Show full text]
  • General Index
    General Index Italicized page numbers indicate figures and tables. Color plates are in- cussed; full listings of authors’ works as cited in this volume may be dicated as “pl.” Color plates 1– 40 are in part 1 and plates 41–80 are found in the bibliographical index. in part 2. Authors are listed only when their ideas or works are dis- Aa, Pieter van der (1659–1733), 1338 of military cartography, 971 934 –39; Genoa, 864 –65; Low Coun- Aa River, pl.61, 1523 of nautical charts, 1069, 1424 tries, 1257 Aachen, 1241 printing’s impact on, 607–8 of Dutch hamlets, 1264 Abate, Agostino, 857–58, 864 –65 role of sources in, 66 –67 ecclesiastical subdivisions in, 1090, 1091 Abbeys. See also Cartularies; Monasteries of Russian maps, 1873 of forests, 50 maps: property, 50–51; water system, 43 standards of, 7 German maps in context of, 1224, 1225 plans: juridical uses of, pl.61, 1523–24, studies of, 505–8, 1258 n.53 map consciousness in, 636, 661–62 1525; Wildmore Fen (in psalter), 43– 44 of surveys, 505–8, 708, 1435–36 maps in: cadastral (See Cadastral maps); Abbreviations, 1897, 1899 of town models, 489 central Italy, 909–15; characteristics of, Abreu, Lisuarte de, 1019 Acequia Imperial de Aragón, 507 874 –75, 880 –82; coloring of, 1499, Abruzzi River, 547, 570 Acerra, 951 1588; East-Central Europe, 1806, 1808; Absolutism, 831, 833, 835–36 Ackerman, James S., 427 n.2 England, 50 –51, 1595, 1599, 1603, See also Sovereigns and monarchs Aconcio, Jacopo (d. 1566), 1611 1615, 1629, 1720; France, 1497–1500, Abstraction Acosta, José de (1539–1600), 1235 1501; humanism linked to, 909–10; in- in bird’s-eye views, 688 Acquaviva, Andrea Matteo (d.
    [Show full text]
  • Chester County Marriages Bride Index 1885-1930
    Chester County Marriages Bride Index 1885-1930 Bride's Last Name Bride's First Name Bride's Middle Bride's Date of Birth Bride's Age Groom's First Groom's Last Date of Application Date of Marriage Place of Marriage License # Dabney Ruth 47 Arthur Garner October 16, 1929 West Chester 29675 Dabundo Louise 18 Saverio DiMaio December 10, 1925 West Chester 26115.5 Dadley Fannie K 23 Albert Smith April 12, 1916 Toughkenamon 19118 Dagastina LorenzaFebruary 6, 1889 Michele Mastragiolo March 16, 1908 Norristown 13663 Dagne Eva EJuly 8, 1874 Jesse Downs December 27, 1899 West Chester 7490 Dagostina Philomena 18 Nicholas Tuscano August 2, 1925 Phoenixville 25847 D'Agostino Angelina 28 Gabriele Natale April 19, 1915 Norristown 18401 Dague Anna LSeptember 23, 1884 James Porter December 18, 1907 Parkesburg 13097 Dague CoraNovember 10, 1874 Vernon Powell February 10, 1904 Lionville 10244 Dague Lillie AApril 27, 1873 Frederick Gottier April 7, 1902 West Chester 9034 Dague M KatieJanuary 1, 1872 Charles Gantt April 17, 1900 Downington 7673 Dague Mary J 29 Ralph Young March 5, 1921 Coatesville 22856 Dague Sara Ellen 36 Rees Helms October 4, 1922 Honey Brook 23933 Dague Sarah Emma1858 James Eppihimer January 14, 1886 West Chester 104 Dahl Olga G 23 Claude Prettyman January 24, 1925 West Chester 25559 Dahms Elsie Annie 26 Chester Kirkhoff October 31, 1929 Pottstown 29710 Dailey Agnes1859 John McCarthy January 13, 1886 West Chester 084 Dailey Anna 19 Rhinehart Merkt August 14, 1913 Downingtown 17216 Dailey Anna RApril 29, 1877 18 Thomas Argne January 4, 1896
    [Show full text]
  • General Disclaimer One Or More of the Following Statements May Affect
    https://ntrs.nasa.gov/search.jsp?R=19710025504 2020-03-11T22:36:49+00:00Z View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by NASA Technical Reports Server 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) 6 X t B ICC"m date: July 16, 1971 955 L'Enfant Plaza North, S. W Washington, D. C. 20024 to Distribution B71 07023 from. J. W. Head suhiecf Derivation of Topographic Feature Names in the Apollo 15 Landing Region - Case 340 ABSTRACT The topographic features in the region of the Apollo 15 landing site (Figure 1) are named for a number of philosophers, explorers and scientists (astronomers in particular) representing periods throughout recorded history. It is of particular interest that several of the individuals were responsible for specific discoveries, observations, or inventions which considerably advanced the study and under- standing of the moon (for instance, Hadley designed the first large reflecting telescope; Beer published classic maps and explanations of the moon's surface).
    [Show full text]
  • Wallace Eckert
    Wallace Eckert Nakumbuka Dk Eckert aliniambia, "Siku moja, kila mtu atakuwa na kompyuta kwenye dawati lao." Macho yangu yalifunguka. Hiyo lazima iwe katika miaka mapema ya 1950’s. Aliona mapema. -Eleanor Krawitz Kolchin, mahojiano ya Huffington Post, Februari 2013. Picha: Karibu 1930, Jalada la Columbiana. Wallace John Eckert, 1902-1971. Pamoja na masomo ya kuhitimu huko Columbia, Chuo Kikuu cha Chicago, na Yale, alipokea Ph.D. kutoka Yale mnamo 1931 chini ya Profesa Ernest William Brown (1866-1938), ambaye alitumia kazi yake katika kuendeleza nadharia ya mwongozo wa mwezi. Maarufu zaidi kwa mahesabu ya mzunguko wa mwezi ambayo yaliongoza misheni ya Apollo kwenda kwa mwezi, Eckert alikuwa Profesa wa Sayansi ya Chuo Kikuu cha Columbia kutoka 1926 hadi 1970, mwanzilishi na Mkurugenzi wa Ofisi ya Taasisi ya Taaluma ya Thomas J. Watson katika Chuo Kikuu cha Columbia (1937-40), Mkurugenzi wa Ofisi ya Amerika ya US Naval Observatory Nautical Almanac (1940-45), na mwanzilishi na Mkurugenzi wa Maabara ya Sayansi ya Watson ya Sayansi katika Chuo Kikuu cha Columbia (1945-1966). Kwanza kabisa, na daima ni mtaalam wa nyota, Eckert aliendesha na mara nyingi alisimamia ujenzi wa mashine za kompyuta zenye nguvu kusuluhisha shida katika mechanics ya mbinguni, haswa ili kuhakikisha, kupanua, na kuboresha nadharia ya Brown. Alikuwa mmoja wa kwanza kutumia mashine za kadi za kuchomwa kwa suluhisho la shida tata za kisayansi. Labda kwa maana zaidi, alikuwa wa kwanza kusasisha mchakato wakati, mnamo 1933-34, aliunganisha mahesabu na kompyuta za IBM kadhaa na mzunguko wa vifaa na vifaa vya muundo wake ili kusuluhisha usawa wa aina, njia ambazo baadaye zilibadilishwa na kupanuliwa kwa IBM ya "Aberdeen "Calculator inayoweza kupatikana ya Udhibiti wa Mpangilio, Punch Kuhesabu elektroniki, Calculator ya Kadi iliyopangwa, na SSEC.
    [Show full text]
  • University of Cincinnati
    UNIVERSITY OF CINCINNATI Date:__7/30/07_________________ I, __ MUNISH GUPTA_____________________________________, hereby submit this work as part of the requirements for the degree of: DOCTORATE OF PHILOSOPHY (Ph.D) in: MATERIALS SCIENCE AND ENGINEERING It is entitled: LOW-PRESSURE AND ATMOSPHERIC PRESSURE PLASMA POLYMERIZED SILICA-LIKE FILMS AS PRIMERS FOR ADHESIVE BONDING OF ALUMINUM This work and its defense approved by: Chair: __Dr. F. JAMES BOERIO ___ ______ __Dr. GREGORY BEAUCAGE __ ___ __ __Dr. RODNEY ROSEMAN _____ ___ __Dr. JUDE IROH _ _____________ _______________________________ LOW-PRESSURE AND ATMOSPHERIC PRESSURE PLASMA POLYMERIZED SILICA-LIKE FILMS AS PRIMERS FOR ADHESIVE BONDING OF ALUMINUM A dissertation submitted to the Division of Research and Advanced Studies of the University of Cincinnati in partial fulfillment of the requirements for the degree of DOCTORATE OF PHILOSOPHY (Ph.D) in the Department of Chemical and Material Engineering of the College of Engineering 2007 by Munish Gupta M.S., University of Cincinnati, 2005 B.E., Punjab Technical University, India, 2000 Committee Chair: Dr. F. James Boerio i ABSTRACT Plasma processes, including plasma etching and plasma polymerization, were investigated for the pretreatment of aluminum prior to structural adhesive bonding. Since native oxides of aluminum are unstable in the presence of moisture at elevated temperature, surface engineering processes must usually be applied to aluminum prior to adhesive bonding to produce oxides that are stable. Plasma processes are attractive for surface engineering since they take place in the gas phase and do not produce effluents that are difficult to dispose off. Reactive species that are generated in plasmas have relatively short lifetimes and form inert products.
    [Show full text]
  • DMAAC – February 1973
    LUNAR TOPOGRAPHIC ORTHOPHOTOMAP (LTO) AND LUNAR ORTHOPHOTMAP (LO) SERIES (Published by DMATC) Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Scale: 1:250,000 Projection: Transverse Mercator Sheet Size: 25.5”x 26.5” The Lunar Topographic Orthophotmaps and Lunar Orthophotomaps Series are the first comprehensive and continuous mapping to be accomplished from Apollo Mission 15-17 mapping photographs. This series is also the first major effort to apply recent advances in orthophotography to lunar mapping. Presently developed maps of this series were designed to support initial lunar scientific investigations primarily employing results of Apollo Mission 15-17 data. Individual maps of this series cover 4 degrees of lunar latitude and 5 degrees of lunar longitude consisting of 1/16 of the area of a 1:1,000,000 scale Lunar Astronautical Chart (LAC) (Section 4.2.1). Their apha-numeric identification (example – LTO38B1) consists of the designator LTO for topographic orthophoto editions or LO for orthophoto editions followed by the LAC number in which they fall, followed by an A, B, C or D designator defining the pertinent LAC quadrant and a 1, 2, 3, or 4 designator defining the specific sub-quadrant actually covered. The following designation (250) identifies the sheets as being at 1:250,000 scale. The LTO editions display 100-meter contours, 50-meter supplemental contours and spot elevations in a red overprint to the base, which is lithographed in black and white. LO editions are identical except that all relief information is omitted and selenographic graticule is restricted to border ticks, presenting an umencumbered view of lunar features imaged by the photographic base.
    [Show full text]
  • Appendix I Lunar and Martian Nomenclature
    APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei
    [Show full text]
  • User Guide to 1:250,000 Scale Lunar Maps
    CORE https://ntrs.nasa.gov/search.jsp?R=19750010068Metadata, citation 2020-03-22T22:26:24+00:00Z and similar papers at core.ac.uk Provided by NASA Technical Reports Server USER GUIDE TO 1:250,000 SCALE LUNAR MAPS (NASA-CF-136753) USE? GJIDE TO l:i>,, :LC h75- lu1+3 SCALE LUNAR YAPS (Lumoalcs Feseclrch Ltu., Ottewa (Ontario) .) 24 p KC 53.25 CSCL ,33 'JIACA~S G3/31 11111 DANNY C, KINSLER Lunar Science Instltute 3303 NASA Road $1 Houston, TX 77058 Telephone: 7131488-5200 Cable Address: LUtiSI USER GUIDE TO 1: 250,000 SCALE LUNAR MAPS GENERAL In 1972 the NASA Lunar Programs Office initiated the Apollo Photographic Data Analysis Program. The principal point of this program was a detailed scientific analysis of the orbital and surface experiments data derived from Apollo missions 15, 16, and 17. One of the requirements of this program was the production of detailed photo base maps at a useable scale. NASA in conjunction with the Defense Mapping Agency (DMA) commenced a mapping program in early 1973 that would lead to the production of the necessary maps based on the need for certain areas. This paper is designed to present in outline form the neces- sary background informatiox or users to become familiar with the program. MAP FORMAT * The scale chosen for the project was 1:250,000 . The re- search being done required a scale that Principal Investigators (PI'S) using orbital photography could use, but would also serve PI'S doing surface photographic investigations. Each map sheet covers an area four degrees north/south by five degrees east/west.
    [Show full text]