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Poblications, Orthe' / , I ·:Jefpro,Pljlsion Laboratory. -, , 1111111111111111111111111111111111111111111111111 111111111111111 , / 3 1176 00134 2360 " , I ! r I ,_ j - I ..,- ) , JP,L BIBq<?-GRAPHY 39-20, NASA-CR-158493 19790014787 /' , ,I i ,1 , //~ I f '- I ; ,-' ; " I \ / ~. /' , \ I I l ) - \ , ,I ' , / ,/ , , ,L / l 1"'-' - '\ / , l , POblications, orthe' / ,i \ \ ' , /' \ I I / - ·:JefPrO,plJlsion Laboratory. / I I _ ,f - ,\....- , "'-"1~978[ ,\I - I' ~\ I /' _,J , , ' J\ ( ------... \ ~ \ '} \ " , \ I "- I -, / I' !, , , I , 1- >' -- \ / / , ," , I I, _J / \ /~- (", \ \ " \ /, , / I I ~ /, t\~ / L '-., \ 1/ , , , \ ' "I '- I: _, - I -' ~ / ~- - --" ! r ' \ -- -- ... -r-" '1 /' r ~-- ~ r.., - ...... - '\ r , r ,II I '- r_ L , ~ - \." j , ,I I I, I > '----;, ':- \ , I \ ~ --1- " ,APf) /" '. (\~ ) ) ./ \ ' -:iI, ,/ F \ r \' \ / ) I ' " \ - / \ ." . - I' , \ /' " \ - I ,=-, \ \ I, I - \ I / \ ' , '/ April 1, ,1979 I '/ ( , - \ \ , \ \ >- /' ,, , -' , J , -/ II 1- I ~ ___ I I National ~Aeronautlcs and co , Space!Admlnlstratlon __ - / ,- - ,/ I \ I - / ,- ,!~~ -Jet' Propulsion Laboratory \ ' J , California Institute of Technglogy ) r Pasadena, Callfornia'- /, r / " , ( \ / , , I , , \ r \ , 1111111111111 II~ 1111111111111111111111111111 NF01291 - / \~l \ ~'- / / - JPL BIBLIOGRAPHY 39-20 Publications of the Jet Propulsion Laboratory 1978 April 1, 1979 National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, California This publication was prepared by the Jet Propulsion Laboratory, California Institute of Technology, under NASA Contract No NAS7-100 Foreword JPL Blbhography 39-20 descnbes and mdexes the externally dlstnbuted techmcal reportmg, released dunng calendar year 1978, that resulted from sCientific and engIneer­ mg work performed, or managed, by the Jet PropulsIOn Laboratory SIX classes of publicatIOns are mcluded' (1) JPL PubhcatlOns (77-, 78-, 79-senes, etc.), In which the informatIOn IS complete for a speCific accomphshment and can be tailored to Wide or hmlted audiences and be presented In an established standard format or special format to meet umque requirements. (2) Articles pubhshed m the open hterature. (3) Articles from the bimonthly Deep Space Network rDSN) Progress Report (42- senes). Each collectiOn of articles In this class of publicatiOn begInmng With 42-20 presents a periodical survey of current accomphshments by the Deep Space Net­ work Formerly, each collectIOn of articles was pubhshed as a separate volume of Techmcal Report 32-1526 (4) Techmcal Reports (32-senes), In which the m(ormatlOn IS complete for a speCific accomphshment and IS Intended for a Wide audience (5) Techmcal Memorandums (33-senes), In which the Information IS complete for a speCific accomphshment but IS Intended for a llffilted audience to satisfy umque reqUirements. (6) Special PublicatIOns (43-senes), m which the mformatlOn IS complete for a speCific accomplishment and IS presented m a special format to emphaSize ItS umque character and directiOn. Effective January 1977, the "JPL Publication" replaced the Technical Report, Technical Memorandum, and SpeCial PublicatIOn. However, the dIscontmued classes may stIll appear In future Issues of the Blbhography If succeeding volumes or reViSions are published In their former senes. The pubhcatlOns are Indexed by (1) author, (2) subject, and (3) pubhcatIon type and number A deSCriptive entry appears under the name of each author of each publication, an abstract IS Included With the entry for the pnmary (first-listed) author JPL personnel can obtam loan copies of formal documents cited from the JPL Library. Personnel of outSide orgamzatlOns can obtam copies or informatIOn regarding availability of documents cited by addressmg a wntten -request to the Technical InformatIOn and Docl1mentatlOn DiVISion, Jet PropulsiOn Laboratory, 4800 Oak Grove Drive, Pasadena, California 91103. 111 Contents Author Index With Abstracts '. 1 Subject Index . , .145 PubHcation Index .178 Author Index With Abstracts ABRAMS, M. J. ferences and, to the first order, suppress albedo differ­ ences due to topography AOO} Evaluation of Landsat MSS vs TM Simulated Data for Distinguishing "Hydrothermal Alteration" The mfluence of atmosphenc scattermg and methods to correct for the scattermg were also studIed Two tech­ M. J. Abrams, A. B. Kahle, D. P. Madura, and nIques were used to correct for atmospherIC effects (1) J. M. Soha dark object subtractIon, (2) normahzatIon by use of ground spectral measurements Of the two, the first tech­ JPl Publication 77·83, March I, 1978 nIque proved to be the most successful for removmg the The object of this study was to sImulate Landsat Follow­ effects of atmospherIC scattermg On (LFO) data to demonstrate the mmeral exploratIon Fmally, a dIgItal mosaIc was produced from two slde­ capabIlity of this prospectIve system for segregating dIf­ lappmg Landsat frames The advantages were that the ferent types of hydrothermal alteratIon and to compare same enhancement algOrIthm can be apphed to both thIS capablhty WIth that of the eXIstIng Landsat system frames, and there IS no seam where the two Images are MultIspectral data were acqUIred for several test sItes Jomed DIsadvantages mcluded the tIme-consummg With the BendIX 24-channel MSDS scanner ThIS instru­ process of domg the mosalCkmg and the fact that the ment had spectral bands closely approxlmatmg those of enhancement algOrIthms may not be optImal for both the LFO The data were geometncally corrected, nOIse scenes, but are a compromise was removed, and resolutIon was degraded to LFO pa­ rameters pnor to further computer processing Contrast AOO3 A Study of Alteration ASSOCiated With Uranium enhancements, band ratIomg, and prmclpal component Occurrences In Sandstone and Its Detection by transformatIons were used to process the SImulated LFO Remote Sensing Methods data for analySIS J. E. Conel, M. J. Abrams, and A. F. H. Goetz For the Red MountaIn, ArIzona, test area, the LFO data allowed IdentIficatIon of SIliCIfied areas, not IdentIfiable JPl Publication 78·66, Vols I and II, August I, WIth Landsat 1 and 2 data. In addItIon, the Improved 1978 LFO resolutIon allowed detectIon of small slhclc out­ For abstract, see Conel, J E crops and of a narrow slhclfied dIke For the Cupnte­ Ralston, Nevada, test area, the LFO spectral bands al­ lowed dlscnmmatIon of argIllIC and opahzed altered ADAMS, M. areas, these could not be spectrally dlScrImmated usmg Landsat 1 and 2 data AdditIon of data from the 1 3- and AOO4 A Statistical, Micromechanlcal Theory of the 2 2-~m regIons allowed better dlscrImmatIons of hy­ Compressive Strength of Brittle Materials drothermal alteratIon types M. Adams and G. Sines AOO2 Computer Image Processlng-GeolQglc Applications J Amer Ceram Soc, Vol 61, No 3-4, pp 126- 131, March-April 1978 M. J. Abrams A general theory of the compressIve strength of brIttle JPl Publication 78·34, June I, 1978 matenals IS presented ThIS theory proposes that faIlure Computer Image processmg of dIgItal data was per­ IS brought about by structural weakenmg from accumu­ formed to support several geologIcal studIes The specIfic lated crack damage whIch increases WIth the stress level goals were to (1) relate the mmeral content to the spec­ The statIstIcs of the flaw dIstrIbutIon and the mechanISm tral reflectance of certain geolOgIC matenals, (2) deter­ of crack InItIatIon and extensIon are important A sample mme the Influence of envIronmental factors, such as calculatIon usmg the theory IS gIven to demonstrate Its atmosphere and vegetation, and (3) Improve Image applicatIon processmg techniques AOOS Crack Extension From Flaws in a Brittle Material For detectIon of spectral dIfferences related to mmeral­ Subjected to Compression ogy we found the technIque of band ratIomg to be the most useful RatIo pIctures exaggerate subtle color dif- M. Adams and G Sines } TectonophysIcs, Vol 49, pp 97-118, 1978 AJELLO, J. M. The mechamsms by which cracks extend from flaws 10 AOO9 An Interpretation of Manner 10 Helium (584 A) bnttle materials subjected to compressive loads are pre­ and Hydrogen (1216 A) Interplanetary EmiSSion sented Although It IS recognized that most geological Observations materials are neither dense nor smgle-phase, this experi­ J M. AIello mental study and analysis are restncted to smgle-phase, dense materials 10 order to proVide a model amenable to Astrophys J. Vol 222, pp 1068-1079, June 15, analysis and expenmental confirmation The flaws which 1978 occur 10 dense, smgle-phase materials are diVided mto three types, each type havmg different charactenstlcs of The Marmer 10 ultraviolet spectrometer measured the crack extensIOn Expenmental shldles of crack extensIOn mterplanetary emissIons of both He(S84 A) and from flaws mtroduced mto blocks of polymethylmethac­ H(1216 A) on January 28, 1974 at time of solar mml­ rylate plastic are deSCribed The shldles show that crack mum The heliocentric distance was 075 AU A first extensIOn from three-<hmenslOnal flaws IS more complex analYSIS of the observations by a Simple model, whICh than two-<limenslOnal theories predict The extensIOn of employs the Copernicus satellite measurement for the velOCity of the mterstellar wmd of 22 ± 3 km s-I. shows secondary cracks may result 10 more damage than that which would be predicted by consldenng only the Pri­ that a Simultaneous measurement of both emissIons re­ mary crack extensIOn treated by current theones The sults m a self-conslstent determmatlon of the phYSical Importance of the dynamiC behaVIOr of flaws which stick properties of the mterstellar
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