SCIENTIFIC ABSTRACT NIKOLSKIY, A. YU. - NIKOLSKIY, B. P.

Document Type: 
Document Number (FOIA) /ESDN (CREST): 
CIA-RDP86-00513R001137210012-3
Release Decision: 
RIF
Original Classification: 
S
Document Page Count: 
100
Document Creation Date: 
January 3, 2017
Document Release Date: 
August 1, 2000
Sequence Number: 
12
Case Number: 
Publication Date: 
December 31, 1967
Content Type: 
SCIENTIFIC ABSTRACT
File: 
AttachmentSize
PDF icon CIA-RDP86-00513R001137210012-3.pdf2.69 MB
Body: 
2"10 Tr*lAm (amt.) wr/"Is lmvrwfqmu-. of the VuLuty Of tbo XOfte.. Kbadrut'M# A. D. lcmoide,* of Tuibnima &--iennax, oomenti. imadts of MpletWim tad Lc;pmzA'=om of latraftelug sigh-Speed acludlK of Metals 193L fte luxesticWcm of klgh-spme4 grjAdlng vith pargue grinding *AeU Is d;:x=xW. Advvewcemp vb"l Waj, mad =f1lum xvtr4m" ae tUs tM of grLsdlW apcmtlm a--* 1=1A4444 2W sulbW ZVOOmmuds the &&w2A::e.*d amsL=tviam of grft4jerv aad mbeeU for speeds of 806.90 8/000. M*dMrl Be Ke fCs;m4-SU+^ or %%m~mlcma scitmoes]. assets of ma la- v1stl6stim of Owe-erlese MrIndird With Wlde &tvung ramelm ]JIL fte amtkor dfs=x&*& tba possEbLUtlas a" aftwate4ps of Latra. dkclm ammUrleff grlndbW vItA vIde (800-9W m) ifteels into =as Praftstlam" so restate of expertmem"I OPM with tum typ of ifteel at tho 14PZ Mat am x%s*vt*d. SOCAlort To L (Cand1datle of Teclialftl SclAuceel. ChumcterictIc ffilaftzvs of t~m fto~mma cf Qevt-*L~ Catftldkez 144 fto* dmmmzt~jm feat=-fts cc tbo fr-4-adIft of cAxtj&W as the WO at 6111aste-b-cded ,&oft2Ap t!o fmmt!m OC powdered vaste Instead ce Card k/6 Nola prWons Ooe;. save, Ais dLtp# Md IUw ad --..rrrgu *a of hr.,cukre axIdxtL-c2 Lm discassed. Ow A& -Mialps betvwu taqsrs 4=14C vladi4go prea --w wwass Aeal and sintp ape-idp and pr*4=tIvIW we amtUnad, Bw watbw f"Wafts Isers"Ift proftetivity thrMA& sp"" wA man is- 140101" oaddsUou. 4111vectnve To L EOnWIdau 4c %doleat Salome] to YOMWOO Of UW GCUWUUC ct ntaulm AUwa Me a=tbw lailloe-os the basla owns of 1w prowtivity in Mw grlndlng of titselm &UOYS. no attromus um praftativity to uw cbmdftl afrWty of tit"Im &Uays t* +jw wdwrlaU at Wo pljWft 16001 Md Ww rewItIng emm"Lve upar of t%e *WL ft Laaj~ Aiviv (20-25 tlnos),, hO MOMUNIO tbA WN Of NP04141 pladft on eampositims of the wolamts PC 4 am Fressnaed, Me A* (Nudidsts of Teaj=iua scismass). Oattift AeUds af GrIsdirid Vbvelm @ad Ntibunicall Vwk is arindInc 16X %O reamIts of ezpw.-IvwA&I vwk by the amtb= am pneouU.I. aw vwk Is bow& an a stm4y of se.&I =a ghr"Ive vsmto proftft~ 1u griadIme no Offea". ef trulm Md &MMIng M *Md vow is do. teralwds and tkw -UnffielAe. 6 Is dtri"4 UU coafficlaut ebwgic. tarlms tbw reftntt= of &"rage 6=1m drma Ims In v&4to Cud 516 U4.4.0 pr*iaw off/5918 odogwmd vlt*n Orle-rAl 9M'qM "'AM= io=. An uAlolis aC mehmotool VWk (fwm X roUtl-m dlxp3A*3mut of vark and Aw*l a=fam) &WfM abdfag Is ILLMO Wooozo.44. Ckestowt A* Le (Candl4aU of NehaLcal scl=aesl, lPlnqAhq Qf WAL" owfamis ITL Me eKtbw d1vowwos ttA r*V:AU-lt#,,IA af tho ndcraflaUhIng p. "p a alcrocil"Imbing KtUtmw=t row 4L ljr&.boa, and the *=,act of f1mUkift OC a jammal an the vear cf tin b=wmg. walkhmm p L 2. So= P--~*3ma of FlAx:ibl* arin4ing and ftrfl~c Wstb F*lt Ift"2A 29 fte awtb= desc-ribea a,- &xpj=j==tftj jurtutlgatim of flAxalo "Afug vith f*lt lbeels vith bond" abr":E" powder. fte aosVe- SLUM Of & PffAt* for bufflW Is also dWswSed (T5% cbroodm azldeo 23% suarin, and 4% *u:ic acid). ATAVABUt M-ml:ly of Coagmse Card 6/6 W/PW/GC @-mow 14(10) SO"-'1_08-59-2-8122 AUTHORS: Mineyeva, I.A., Candiate of Technical Sciences; Engineer TITLE; The Influence of the Heating up of Reinforcements on the Strength of Rein- forced Concrete Structures (Vliyaniye nagreva armatury na prochnost' zhelezo- betonnykh konstruktsiy) PERIODICAL: Gidrotekhnicheskoye stroitel'stvo, 1959, Ur 2, P 33-35 (USSR) ABSTRACT: Research on the influence of heating up of reinforcements on the strength and hard- ness of reinforced concrete structures was conducted at the Moskovskiy energeticheskiy institut (the Moscow Institute of Energetics). It was found that the heating up of relnforce- -t t 1, -ft QWAMW e tion currents ] dw Card 112 3 m a m * * ments f ) a considerable UsswdAc of the 14(10) SOV/08-59-2--8/22 The Influence of the Heating up of Reinforcements on the Strength of Rein- forced Concrete Structures hardness of reinforced concrete beams (figure 3). The amount of breaking load for beams with periodic profile reinforce- ments depends little on the temperature of the heating up of the beam (figure 4). There are 3 graphs, 2 diagrams, ? references, 4 of which are Soviet and 3 American. Card 212 SOY/98-89-8-1113a 15(6) AUTHOWs Nikol I SUZLr~~,Yu. t 15agineer, and I.A. t Caadidat* of T*ek- T - _ --Slc&Ylc @aces TtTLZv The Ifff act of Moat on the Mardness and Durability air rerro-Caacrat* we"a PIMUCALe Gidrotekhaichaskoye stroitellatye, 1959, Nr S. Vp 45-46 (UM) ABSTRACTs The &rticle describes tests carried out by the Chair of NydrawLic Construction Work in the M11 (Voscov Power Inatitato)) on the causes and effect on ferro-coacrete of heat (up to 2500C) generated from high-power electric cables (up to 11,000,awp*) installed In the steel fr*Aevork of the concrater they showed that the hardness of farro-concrete, exposed to such heat van considerably, lovered. The experiment was conducted on farro-conerete beans messurinC 150t 200x1, 300mm, reinforced with, in one cast, ULrk 6 atee,10 and in the othert or round rods of Mark 3,steal, of the same dimensions. The asnembly equipment was &Lao made of the saaa, mataritl, consist- ing of 2 6m diameter rods amd a. hoop 4= in diameter &ad lOOM". Card 1/3 long. The compression of the concrete, which was in Llt cases iden- BOY/99-59-8-11/33 The Uf*t.t of float on the (fardness and Durability of rarro-Coserate be"" LULL, was carried out by an 1-21 vibrator? white the durability varied between 150-200 kga/c&4. Conditions of hardening Varied, one group of Lost boom* having been treated In & steam chamber at temperatures of TO-SOOC for 49 hourst the other having been harden- ad under normal. conditions at 16-200C for 98 days. Tho:b*ame wars subjected to. heat in the form of electric currents, of ROO-ItOOO asplit the heat being maintained at the required temperatures for 3 hours. T Lenperaturea Y&rie 9r thebeanx reinforced with Mark 5. steel being heatedupto 80 C and 230OCt while thoso~ with round Mark 3 steel rods were subjected to temperature& of 800C, 1600 C and 2300C. The test& were carried out on a 50 ton universal by- draillic VJM__50L machine, made by them Kharlkov works. Pressure, in the Cam of 2 concentrated weights graded up to 500 kgg, was sp- plied to boam* and continued until they snapped; the results of' the tests on beams retaforced with Mark 6 steel are given itx table 1 and fig.1, and show that the breaking pressure varied only slight- ly when applied to the 2 differentlN treated bettax. rig.1 comparew the graph* of the relative pressure of the 2 kinds of beams (steam- Card 2/3 ad. and cotd-tremted)q, showing that the vmriatiou in the degree of sov/98-sq-S-11/31 The grfect of ffoat, on the ffardness and Durability of Ferro-Concrete Room& sag, which, was greater in the former type than in the letter, par- ticularly at low pressuref decreased && pressure increased. L com- pariaon of figs.Is. and lb shows that the method of hardening has little effect on the degree of gag of bt&mx tested when cold. The graph of the tests on been& reinforced with Mark 3 steel is given in fig.2 and table: 21~ which data shorwa that the durstrility of the beams was considerably lowered even at 1600C, and that this do- crease, roe* iven moretteeply aboyo this temperature; tig.2 shave the relation between sag and pressure and temperature. ConelusLoas drawn from: the experiments are that the shape of the steel rein- forcement, affects, the hardness of concrete; angular steel is more resistant to pressure when, heated, but is unaffected by the method of hardening and testing. Thereare 2 diagrams and 2 tables. Car& 3/3 Illowarr"k.u.6 insh. Matorsdaing the footing also of Occoutrt0lillf 146d" fosafttlems from chartse lawb.54p. KIMM 219J~1-3" 159. (*Wlastlus) (MIK 13,tul INYWRlY, A.M., karJ. to-tUn. iihuk; NIKOLI.-,Eill, A.Yu., 'Anz h. [Vaterlala for tba calculation of precast prestreared elownts for reel =atlon construction) Vaterialy po raschatu sbomykh predvaLritellno mpriazi-annykh kon- atruktaly d1la reliorativriogo stroitellstva. Votkvap Giprovodkhoz, 19C4. 86 p. (VUL4 160) 1. MOSCOW. Weawfuzr*7 proyektrio-Iryakatellukiy i nauchno-issledovatellsklY Inatitut. LY11,111KOV A$P ft.-) A.Yu.9 !rxh.1 S AYRA*fi Y.M., inah.; Maih-reinforceJ cf;r-,-.rnt#i on hUldirg sitei of vatpr dwrelopcont projects. Trady G-!prrvodkhoza no.2603-123 164, (WIRA MO N=la IT._I-A-r DUBMOTSXIT'* Yg.ff. - AMtqpr~ I- Po~tou af dlototte milk. Itabr. v SM 3 uo,2tl2.lfs D 999, (PI Ik oWply) (am 110) MTJR, V.A. LiffiTAUUTA. r.E.g 11KOLIKLY, B.A. Sradicatim of btttag Imeals In ptower amapso 1W.parms. t peruse bat. 26 ms*3047-350 *-J* 157. (NIVA 10:11) 1. Zs noel terse-apidmiologtahemkoy stantelt Moskovsko-Orrushitor theleavAr dorogt (vach. stantatt I.I.Xogllovskiy). (URMS. *mdtantlas tu *J6918 MO) o NIXOLISXIT, S.A.: DUBIMTSKir. re.l. Untrersol Ovault"T cambiaO. Isabr.1 rate. ma.8t" AC t58. Wu 1119) 1. SotrudatkI Tnogoyugwgo muchno-Iseltdovetollgkogo lastituta sUktriflkatelt solleko&O khas M stva. Traro equipment) wir.o.wair., a.-A, CAS-01 mobile distafoating apparatus. ToUrtWUs, 37 50.1tW70 IS 160, (KIA 16t6) 1. ftuddy MerlmsrW vraoh Gosudarstv"Aogo mum&okanstrall"o Institute velerinarpykh preparatov, (I!IsIaf*Loa ad disisfostants-41quipment and mnUfs) I" t r i 113 Jour : Pelf Zhur - Fixika, Ho 2, 195'( llc~ 313C. Author : Alpers, V. V., Barkov, L. H., Geresicove, R. I., GurevIch, I. I., t K. N., Ulkal'skly, H. A.. Tiopor-kows, X.T. Title : Production of kovlr;3-~xonz ~in -he Nuclei of Photographic Ecuslion by 460 Him Protons and Neutrons of 400 Hev Effective Energy. Orig Pub : Zh. eksperia. I tear fiziki, 1956, 3o, no 6, ion-1033 Abstimat The emulatPn-camers procedure uss used to study the production of charged 7r.-:t* sons by 460 Vev protons and by imutrons a.* WO Hev effective energy. Card 1/1 AUIPM, T.To[d*a*"sdjm HARM, L,K.,GZRASIMMA. R.1,; GUMICE, r-lo; KISMUrA, A.P.; KUKKIN, IC.K.kA ! MM. 3. A. I, ~ .. 1 -.-OW1414 pr"Wtt4On Of SIOVr-wsono In photftraphic mlei= ftelat by 60 New pratcme, thureetip. I toorefts. 30 no.6tlOff-1039 go 056. (an 9110) Oftsous) (Nwlear retwtions) SUBJECT USSR / PaTSICS CARD i / 2 PA - 1955 AUTHOR XUDRIII'L.P.0 NIKOWlay.B.A. tion betwe~_W_fa_st Pions and Nuclei. TITLE The Interao PERIODICAL Dokl.Akad.Sauk 1119fasc-4,795-798 (1956) Issued: I / 1957 In the course of this work the results obtained by computing the nonelactic scattering of negative 160 UeV-pions by the nuclei of the photoemulsias are compared with the experiment. On this occasion the assumption concerning in- divIdual meson-nucleon collisions within the nucleus Is accepted as being correct, which is also indicated by the experimental d4t& available concerning the nonelastic scattering of plons by nuclei. Experimental data: The authors used the bundle of negative plons with the energy E. = 188 + 6 KeV emerging from the chamber of the synchrocyclotron of the Institute fo; Nuclear Problems of the Academy of Science In the USSR. This bundle, after passing through a deflecting magnet and a collimator Incided upon an emulsion chamber consisting of layers of 395,;4A- thickness. There are 30 of these layerso The atare found in the emulsion chamber were selooted so that the experimental results obtained relate to E - 160 MeT. Togetherg a to- tal of 1185 act@ of Interaction between such negadve pious and the nuclei of the photoomulsion, among them 323 nonelastic acts of scattering of a charged pionp were found. The acts of scattering of pion@ were Identified by the de- termination of Crain density along the trace. For the 325 nonelastic acts of scattering the energy- and angular distribution of the scattered ne6ative pions Dokl.kkad.Sauk 111, fase-4,795-798 (1956) CARD 2 / 2 PA - 1935 were determined. for the further Interpretation of tLe experlatntal caterial obtained a graph shows the *norjey spectrum of the plons scattered In the angu- lar range from 0 - 90 to 1800; this :p;otrum has the average energy of 64 ! 3 11aV and the half width (30,9 _ ) 99T. Cc utation of the interaction between negat ve 160 MeV pions and the nuclei of the Photo#mulsion was carried out on the assumption that meson-nuoleon collisions In the nucleus develop In a way similar to that of the free nucleons. The results obtained on the baste of the scattering of pions by the nucleons of the nucleus by the computation of the energy- and angular distributions of meson-nucleon collisions within the nucleus do not depend on the particular features of the cross section of the Interaction between a pion and the nucleons of the nucleus. Therefore the potential of interaction between the pion and the nucleus can be evaluated with sufficient accuracy on the basis of the results obtained by the aforementioned nonelastic scattering tests. The conditions upon which such an evaluation Is based are enumerated. For the average Inter- action potential of negative 160 MeV-pions the value V - Eexp - E theor - - (24 + 6) MeT was found. This value agrees with the average potentials of ;he Inteiaction between plons and nuclei which were obtained by experiments concerning the elastic scattering of pions by nuolei. INSTITUTION: NIMOLISKIY, B. A. Cand Phys-Math Sci _- (disa) "Jilre Non.-Elastic Fi Scattering of X-Mesona on.Nuclei." Moe, 195T. 11 pp 20 cm. (Academy of Sciencea USSR), 100 copies (KLj 2T-57't 104) enzj:~ Y % ) I - T - I &UIHOR: Barkov, L. M.j aad ANIAL k" oW Ias, k1h, Ji 120-2-11/37 TITLE: Graphical Method of Determining the Energy and Angles of Dispersion of Two uoving Relativistic 1hrticles. (Grafichaskiy Sposob Opredeleniya Energil i Uglov pri Rasseyanii dvukh Dvizhushchikhaya Relyativistskikh Chastits.) IfSRIODICAL: Pribory i Tekhnika Sksperimenta, 1957, No.2, pp. 40 - 43 (USSR). ABSTRAUT: The interaction between high energy nucleons or Vwsons with nuclei may be regarded as a result of their inter- action with sepainte nucleons in the nucleus (Ref. 1)o The relevant computations are usually carried out using the Monte Carlo method. In the present article a graphical method is given for a rapid determination of the enerCj and of the scattering angles of two moving particles for the case when the characteristics of their interaction are known in the centre of the mass system. The velocity in the cenLre of mass system of two collidin6 parLicius is aeztriainua iroia oiluatioa 1. The magnitude of the resulting momentum arA its angle with direction of Liotion of the incident particle are deter-ained graphicallv using Card 1/3 the instrument shown schematically in figure 1. it 12-72-11/57 Gmphicetl method of oetermin'nS the Energy and Angles of Dispersion of Two Movin6 Relativistic Particles. consists of a rule OA used as an indicator for a protractor. The momentum of the nuclear nucleon is produced along the rule,, while the angle a corresponds to the angle between the direction of motion of this nucleon. and the inci,,'L--nt particle. BG is parallel to 001 and its length represents the momentum of the incident nucleon. The rule OA is then moved so as to coincide with point C (position OAI) and the total momentum and the angle7( are thus found. After determining this angle the parallel and the parpendicula.- components of the momentum of the impinging particle are found using a set-square in the nanner shown in Figure 2. The complete vector dia9mm of the transformation is shown in Fi6pre 5. The method of determining the ener&7 and the scattering an6lo of particles in the laboratory system of co-ordinates is given next; schematic illustrations are shown in Figures 6 and 7. The procedure of findinj~ the maSnitude and direction of the momentum of the scattered particle is again discusrAd in detail, the magnitude of the nomeatum of the scattered particle is eventually determined by the distance OKI Agure 8. The above instru- ment; has been used to evaluate the interaction of 1601!eV Card 213 Yr-mesons with nuclei of photo-emulsions assuming the AdT11GR t XIK0L$SKIJqB.A.v KUDRII,L.P.o ALI-UDZ,S.A. FA - 2058 -'IMM: 12*14016 sGattorine of 160 NOT C-Nefous on rhatocrapkic Smalsion Sualei. (K*uprugas rass*jaalo 160 NOT C-sexasov as jadimok fetoweloil" Russian). PMODICAI: Zhurnal Zkoperimentaltsol I Toorot.lislklp 1957, Vol 529 Ir 1. pp 48-58 (U.S.S.R.) Resolved: 3 / 1957 RovIewed: 4 / 1957 AUTRACTs TkIm work compares tke 4emputatlea of the Laelastis seattering of negative plans of 160 NOT by the nuclei of pkMagraphle walsloa with the experiment. Cosipxtatloa of the LatorsatLea betweea fast piano and tko nucleus, Contra" to analogous gas- putatIone of the lateractlea of fast sualsoas, Offer* tke ad- vantage that In this case the nualosa pact of the Inner amelear cam4ade kas act to to taken late account. lo"t&l ropyltes The authors used a tundle of negative en 5 NOT)-pisam emitted by the Ck4abor of the sys4kra- M eyolotres of the IJAP AN 26SR (- Institute for Nual4ar Prob- Iwo of the Acedeny of sciences of the USSR) and SIM we tolas* of the type F. The *zp*rtaental results obtained rofer to a proton *norgy of ZZ a 162 NOT of tko plans. A total Card of 1165 cases of Interaction between plans of this energy sad PL - 2056 raolaotlo scattering of 160 NOT a -Kesons an Fkatograpkis IhMIGIOR Xuolol. assumptions or* discussed In dotall. Furthermore, the follow- lag facts are layeattgalet more accurately: The r&Me of a pies in the malese, tke salculatlem of tko, soattering of plea* 'by the nucleons of a ameloseq the effects connected with US modification of the potential on the 0644slon of the passage of a plea tiLrough the boundary of a mucloveg the ab- sorption of tke pica* in th* nucleus. J19 good o"oessat of tko theoretical with the experlsontal energy spectr of the pious scattered 'by the auclol of the photographic eaulsion prove@ that the here assumed model deserltem, the Interaction between the plans and the nucleus satisfactorily. ASSNUTION: not given PIXABNM By: go TMS ATAIZAMs Ubc"*y of Congress Card 3/1 AUTROR BARKOV L.H.t NIKOLISKIT B.A. TITM Kous. (8urY#776f-TOrF#rtWWntZl Data) -Russian) (x-nssony Obsor ekeporizentalOnykh danAykh, P&RIODICA.L Uspekhi Fiz. Nsuk 1957, Vol 610 Ir 3, PP 341-398 (USSR) Received: 5/1957 Reviewed: 6/1957 OSTRACT The prevent survey systematizes the most, important, experimental. data on the properties of pions and their interaction with nuel*ons and nuclei. The first part deals with the iateraotion'of pious with nucleons and Is divided into the following sectioust the properties of pion*, the scattering of pious by, nuoltone (phase analysis of this scattering# dependence of the total cross section of this scattering on energy),,, the creation of pion& on the occasion of nualeon-nucleon- collisions, the creation of pious under the influence exercised by 7, -quantv.. Dummiu of first part: The energy dependence. of the cross stations of photoproduotion and. the s"ttering: of' pion* by nucleons have many features in common. The cross sections of both processes attaintheir maxisua W 110 - 120 XeV of the pion# in the at the energy E , CAXV 1/3 Fiona* (Survey of experimental Data) PL - ZG96 masons with different charges the effeats connected with th* action, at the COULM field of the nuclei, the aschanive of tho pro4ustion of.51oas an nuclei. (39 Illustrations and 25 Table ASSOCUTIM.- not gtv**. M I D MMUTUD: AVAILABLN: 1;brazy of Congress. CAU 3/3 "A *tAWY of AvlAsion Showers Caused. by MC)~-Eftergy Cosmic tay Particles," by V. V. Alpers, 1. 1. G-arevich, V. 11.1. Kutu~-.ovm, A. P. V16A=va, B. A. ffikol'okiy, and -1. V. Gurkovar Doklady, denli, Hau14 SWR, Vol U2, No It Jan 57, YP 33-36 ReauLto are C;Lvcn of' ct study oC exploaLon Oioverft caused by high- energy cosmic ray particlem. An cmLlsion ch=b-,r, cont&inin& "MM Type P" t=Lsion, vas exposed for 7 hours in II.V 1955 e. an altitude of 2'1 kilometers. The 29 erploston shovers observed are analyzad. The primary pmrti- cle causing each shover, the number of rclatiActic particle6 per shaver, and t4e anaular distributiou of shovi2r p&rtLclea relativer to the shovor a;(Is are dete-ratined. M XF 4 r OLOWICH, KISHAMA. A.r.-. RIKOWSKIT'. B.A.; GMXGVA, LT. Explosion showers produced by high ontrgr cosmic ray particles. Zhur. *kup. I teor. fis. 34 no.2t265-280 7 159. (KMA 11:4) 1. Abodemlys mauk ISU. (desule rare) Ah < AUTHORS: Guravicb, Z. I., kuturovao V. M., -"Ishakora, 56-2-2/51 A. P. , Mal B. A. , Surkova, L. v TITLX: The Asy=etry in the An,;ular Distribution of p+ Decay Electrona,0beerved In Photographic Emulsions (Aaimostriya uglovoeo ra3predelenlya elektronov p+ -1 e* - -raopada po nablyudenlyan v fotoemullali) PERIODICAL: Zhurnal Eksperimentallnoy I Teoreticheakoy FIzikI, 1950, Vol 34, 11r 2, pp 21,10-205 (USSR) ABSTRACT: An sQulsion chamber of 7 x 4 x I cm conciatinG of 23 layers of an ffkiK,0% photo,xaphic emulsion fron th~- F type wan irradiated with slow positive pione of the G#iQ-1 (Ob"Yedinennyy inatitut yaderrykh lssledovani7 - United Institute for Nuclear Research) synchrocyclotron. The chamber was mounted In r. double maZ;netic screen I-. order to make sure that the scattered magnetic field of the synchrotron did not lead to a precession of the spin of the nyon. In looking throuGh the emulsions after developing those cases were selected where the whole nyon track of the x -.9p-decay Card 1/3 Is situated in a single layer of the emulsion. In this the The Asymmetry in the An~ular Distribution of p+ -0 e+ Decay 56-2-2/51 Slootrons Observed in PhotoCraphic F-iulsiono myon to supposed to come to a standstill after the passaGe through at least 50P of tho surface of the non-developed layer of emulsion. The authora deterzined the angle a between the direction of e2lasion of the myon it. the x -91A- -decay and that of the electron of the p --% e-decay by deter-itnina the anale a between these directions on the emulsion level and the anCle of sitribution 01, P2 reap. of the traces of the nyon, the electron towards the level of emulsion resp.. Furthermore an emulsion chamber of the saLe dimensions was irradiated with slow positive plona. The results of meacurenents cre collected in a table. The ancular distributions determined this way are shown by a diaGrami they do not contradict the thooreticol dependence I + a cosep a - (X/3)(1 - 1), where y denotes the depolarication coefficient of ayona. A relation fer the determination of the optimum value of a in given. The na--netic field (11 ~1100 0) Increases a little the acyraiotry, i.e. it decreasea tLe depolarization of the --jona in the enulcion. "-ut thin effect in not regarded as strictly proved. 7he =ean valus of the parameter a calculuted fro-i the reaulto of thin work Ir Card 2/3 a a -(0,103 t 0,0094). The an"-ular distribution for 13771i& The Asyametry In the An6gular Distribution of p e Afecag 56-2-2/51 glectrons Observed in Photographic Eaulcions ASSOCIATION: SUBUITM: AVAILADLE: -9 decajr processes proceeding from the results of various previous works and from those of the present Investigation In also shown In a diagram. Within the error limits the anaular distribution of the elootrons or the relation I + + a co~4,is aufficioutg where a - -0011 + 0,015)- There are 2 f1gures, 2 tables, and 13 references; I of which Is Slavic. Ag USSR (Akadealya nauk SSSR) August 14, 1957 Library of Con&-rose 1, ftotopaphic eaulatons-Irradiation 2. Xlect4a, -Distribution Card 3/3 t - j A-1 4Y U 2-55/51 AUTHORSe Dobrotsov, ru. P. , Nikolfekiy, B. A. - -- -1 . . ............................., TITLEs The FemokUm If Positive Pions by ffertive Plona (Rozhdenlye x -nozonov e-mazonlat PERIODICALs Zhurnal Zkoporimentallnoy I Tooraticheskoy Fitiki, 1950, Tol, 34, Ur 2# PP 510 - 511 (USSR) ABSTRACTo The prenent work investigated the production of positive pions on the nuclei of a photo-amulsion, under the action of neea- tive pions of an energy of frou 340 + 30 I:ev. The emulsion chamber consisting of 60 emulsion layers of a total thick- noes of 23 am and of a diameter of 100 mm was arranged in a bean of negative 370 190Y plons of the synchrocyclotron of the OMAM (- United Institute for Nuclear Research, Ob" yedinannyy institut yadernykh Issledovanly). The chamber consisted of an HO K~ff -amul2lon ~f th~ P type. On obaorv- ing the emulsion layers the -roe decays were re- corded. Teen the found positive pions were traced to the place of their production. When tracing their Path 56 stars Card 113 caused by negative pion@ were founde In the case of 21 stars 56-2-35/51 Ahe PWW Ion of Pesitive Plons by Negative Pions the emission of a positive pion to accompanied by the enisuion of a second plont which Is IdentIfted from the gradient of granulaor density along Its path. Such cases obviously belon,; tq1the production of positive plons, In the remalnin6 number of the cases no emission of secand pion was noticed but these cases can also be related to the production of a positive pion with submaquent absorption of a negative pion In the nucleus (or with emission of a neutral pion)# The enerCy of the such produced positive pions was determined from their range within the emulsion. The enera of the negative pions (in the stars with 2 pions) was dote--mined from the density of the grain* ,J,'he taking into account ol" the edge effect is shortly discussed. Two diagrams show the energy spectrum and the angular spectrum of the produced positive pions. The spectra of the positive pions with aniwithout enisBion of a second pion from the nucleus are similar to eac1h other. In determining the relative moment& of two pions emitted from the same star no noticeable correlation of the two plona of the final atmte was found. This is# however, only a qua'Atta- Card 2/3 tive final conclusions The cro~3 section of the production The F011MIM of roAtive Plona by :(oCative Plons 56-2-35/51 of slow poottive plons (Ee - 0 to 60 UeT) b7 ne,-,attva pirmn of an enero.1 of from 340 + 30 UeV on a nu$ua.jof t~c photo- -enulsion ii equal to 0;~ (2,1 + 000) .10- c 2. TIncre ,r,~ 2 f1jureat an~ 0 referoncoso 4 of which are Slavic., ASSOCIATIOlls MUSSR (Ahade-,Aya nruk 33311) 3 UIN.'I 7.-ED sOctober 29f 1957 AVAILADLEs Library or Conrreau 1. Pions-FormtIon-Positive 2. Pjan"sgative4ppUcations 3o Pions-ga*rgy spectnn 4,, Plow-AaCmUr sPectrum Card 3/3 kM%A,R DISTRINUTIOU OF ~Amc=' III IUGH-WEMT EM=IVE sfacz is A.P. KIONLkova, 04A. N Vdlxkiy, V.L Feddrov Thit pappr coverx a stud~r or )7 blarst shomrs gentrated by ttigh-energy comic particles 6&0'u ev) in nuclear emulsion. Th-.t main part of these explosive showers hal already been Investigated by the authors in an earlier work. The aiA of this paper is to consi,4r all, arrors (fluctuational ani caused by meagurements) that influenced the angular distribution of show%r particles. This was nacaaaat7 to verify, the, earlier conclusion that the angular distribution of sbowlar particles in the cent m-or-ine rtia sy3tem, in son-!,ntric bac?varJfr (in the lirection, of angles 130-1800)., This conclusion did not aj;rne with thT prudlations of various theori,~s of shower production. The r4Lin effort in this study was to deteimine tb-- orrors that are. possiblq In. deterninin& th-- true direction of the show-r axis, The direction of th%-- primary partial(- may tx- tak---n as t~--~ direction or th~- stjow,,3 r axis t if this is impossiblo, thon the Ji m-ction ot Ot~~ centm, of gravltY4 of tire showr is consilerel to be thm dimetion, of ttxt shower axis., k study has been male, (expirlimentally an,1 by t~.s For* Carlo, metho I) of the, deviation of the dire-ction of th,,,~ llc,?ntm- of gravity' of the shower from that of th-- primary particl-i It has been found teat the ro-lount of rluctutttion in Jetemin~ng s~trw--r axis in 0.17~~ 1). which corresponds to an error or ZCP in IstomininE tha direction of the shower axis in the cents r-o f-ine rtia system. An evaluation of widening dw to this arrect shows that the nw-,ber of particles in the interval 00-3CP in t~e center-or-inartia, systom kill ftmini3h, tr.- -' 22C TM- total systematic er.-or in the experim-mtally observed nu:-,ber of' showar particles in th--! interval 00 -)00' In the centar-or-inertial systa-m =ounts to-25~40 The angular distributions oC shower rarticles in thi cantre-of-inartial irystez- have been obtained for 39 showers froot 0:0 to, 1800., The, distributiors indicate an essential anisotropy of shower particleff movinC rather urLtrordT for%(ards ani backwa with respect to the direction of motion of the primary particle, Thus. account of this crror leala to a sym-)--trization of angular dtirtribution in the cent re-of-Ine rtia systeem relative to the angle 0 r 'a /Z. This conciusion is in agree*--at with the data of all otlar laborat4riax that were anal",ad in the pap%r- Report presented at the International CowAc Ray Conference. Koscow. 6-U. July 19W 24(3)0 21(7) SOT/56- 56-4-6VTO AUTHO113s Ali-Zade, S. A., Gurevich, 1. 1., Dobretsov, Yu. P., Rikollskiy, B. A., Surkova, L. 1. TITLE: The Asymmetry of Electron Angular Diotribution inAt+- e 4-Decay in a kat-,neti~ Field of 27000 G (Asicactriya uglovo-go raapredeler,:~w + elektronov si - e -raspada v magnitnom pole 27000 G) PERILIDICAL: Zhurnal eksperimentallnol I teoreticheakoy fiziki, 19jq, Vol 36, Nr 4, pp 1327-1329 (U.;,;R) ABSTPUCTs If anCular distribution is described by the exprenoion F1 '),_ - U . -coo(V,A) char- 47-&N/do - 1-a cosO (a ->,P/3 w & O O acterizes the ratio of the vectorial and poeudovectorial share of interaction in 41 - e-docay; P denotes muon polariration) , it in found that the quantity a depends both on tho ncRGuring neth- ad and on the nature of the depolarized. matter. It attains 4 maximum value of a a 1/3 at cos(A,V) - -1. For NIKFI-R emulsions a was determined as amounting to 0.092 t 0..018, for Ilford G-5 it was 0.14, The icaximwi value attained by a for Craphite Is 0-303 � 0.040. The depoInrizing property of matter may be reduced by applying~- strong magnetic fields, the direction of which co- Card 1/5 incides with muon polarization. The Increase of n brought about + JOY/56-36-4-65/To The Asymmetry of Electron Angular Distribution In ~M - 0 Decay to a Nagnotic Ifteld of 21000 0 by magnetic field can be described by a a a 1 0.5 of 1+(WvaE) 2 a0 donotee the &-value If no dopolarization takes place, AE the energy of fine-structurs, splitting of th*~A-msslc &ton In the IS-stats. An oxporisental checking of this formula in fields of UP to 14000 G showed that by it the dependence a(H) is quall- tativ*ly described. The authors determined a In the 1jr-(A- e- docay In photasmulsions at 5 w 2TOOO 0- a was determined from the ratio a - 20 backward _x forwardW Kbackward+"forward)* Results' For 9 a 0 - 50 &1 - 0.315 +_ 0.026 0 - 150 - 1800 a2 a 0-295 t 0.027. Kean value formation averaged over the directions in which suons fly off gives$ a 3 - 0.305 t 0-019- 'f oreal 0 &V coo@, one ob- tains areal AVO-940 - 0.324 t 0-020- Herefrom It follows that Card 213 OAP - 0.972 0.06, i.e. 1%I with an accuracy of up to a + JOT/56-36-4-65/70 The Asymmetry of Sloctron Angular Distribution In ~A -Decoy In a Kagnetic Field of 27000 0 statistical error of 6% attains Its maximum value and P This Indicates a considerable degree of inaccuracy of the for- mula describing a(H). The authors finally thank B. S. Xeganov and B. V. Sokolov for their help in Irradiating the photoeaul- Sion*, D. K. Samoylovich for developing the saulsion. and fur- ther also V. W. Kutukova, A. M. Alperef and G. V. Plesh1vtseva for their assistance. There are 8 references, 2 of which are Soviet. SUMITTEDs February 1, 1959 Card 3/3 2t (7) AuTion: Gurevichv 1. 1., Qko"I !!~y ~8- A~-- SOV/56-3T-1-56/64 durkovs, Le T. TITLX: Three-Zlectron Decay of the O-Keson (Trokhol*ktrcnnyy raspal P-nozons) PUIODICAL: Zhurnal eke ps risen %zl;no i teoreticheakoy fitiki, 1959, Vol 3T9 Ir I j, pp 318 - 319 u 813 ANTUCT: The anthore of the present "L*ttor to tho 141tor"q whom Investi- SatinC the asymmetry of the angular electron 41stribution of %-+ p -4 e-docay, observed that in one case three relativistic electron* depart from the stopping potnt of the p-seson (or. figure). All three electrons have largo Inclination allles with respect to the emulsion plane# and therefore exact mosettroment of CraLn density w I:jo!afo:#Iblef It was, however, near that for rolativistic part * trey-I Ifer). The recorded part of tho, electron path length: L *I w 455 p# L 02 - 562 p# L 03 . 455 It. The nuon rangs, amounts to R. so 596 p in the case of an average path length of the muou of the a-ott-4scay In a R-51Kri-esulatom Card 1/3 of 602 p. The angles between the electrons: 012 , e.6 9 a15 a ftroe-glectran Decal of the it-K*son aor/56-3T-l -58164 - to.6% 023 a W950# The cage observed cannot be LaUrprotcd as a nuon decor in electron + lowith a transformation of the quantum into electron + positron at the place of decay, becauce in this case the direction of the departure of the particle pairs would hays had to be opposite to the observed direction of flight of the decay tlectronso The explanation* p +-+ e+ + + 0+ + 0- + p + 3; or p+-+ e+ + 9 + w + r with following trans- formation of tho quantum Into a pair would be possible. The case described her*'was observed In connection with the gvaluatLon of about 509000 muon. d4cays. Thus# the uthroo-tlectron" decay probability of the suon. may be estimated at 2.10-5. It the results obtained by other authors are taken Into accountv a probability or io-6 I* obtained. This order of mWitudo to obtained also If a radiation process of second order is ansuat4t emission of a virtual t-quantua accompanying the departure of the electron with follovine transformation Into an *Iactron-po- sitron pair# the pair onor" of which may be estimated as anount- Card 2/3 Three-laoctrom Decay of the g-Kosom SOV/56-37-1-56/64 129 to 15 New* The authors finally thank 1. So Shapiro for Aim- cuselosm. Thore, is I figure. SUBMITTIM: April 17, 1959 card 3/3 24.6900,24.6200o 24.6600024.6510, 16.8ioo AUTHORSt Mlahakova,, TITLE: Angular Showers 76974 sov/56-37-6-i4/55 A. P., Mikol'sklyp B. A. W', aw.., Distribution of Shower Particles in EKplosive Produced by Ifigh-Energy cosmic Ray Particles PERIODTCAL: Zhurnal eksperimental0noy I teoreticheskoy fiziki, 1959, Vol 37, Hr 60 PP 1594-1603 (USSR) ABSTRACT: An Investigation was made of the angular distribution of cosmic particlea in showers with an energy or 1010 - 1013 ev in the center mass system. The data were obtained on the basis or an analysis of 39 cosmic showers recorded In 1956-1957 at the height or 23-27 km. The method of the analysis was described in the first part of this study (cf. I. I. aurevich, A. P. Mishakovat B. A, Mikollskiy, L. V, Surkova, Zhur. eksp. I teoret. fiz..,340 265o 1958). The main Card 1/5 features of the radiation are summ&rized In Table 1. Angular Distribution ift Exp4oaLve Showers Cosmic Ray Particles of Shower Particles 76 9 -14 Produced by High-Energy SOV/56-37-6-14/55 fV 1944 39.8 3. is. tots 2 10 2+3 ~,7 2'.5 2 32.4 :8.9 1.65.1010 A x I - ~;I 35 lo,7 i S.3 4 *03 S.01 4.0 to- 4 p S+2 ~'3 3,23 17,7 13:0 Is,xs 4,7 -toge 5 4 0 (40 1 1 to 20 QU :%1 & Z, 5 0 97 48.3 7 4 St.$ 7 16 5.144001 to's 04 1 8 p + 3+4 . ,-,s , 7.9 . , te *0 . . 0t p 3 to.2.1 to.56 p 3+2 17 5 k, q.G~ 1 MIS 11.9t 2.78-toct to p 5+3 Is &1 1 9: 5.9 $.(* .5.98 ?,12.10" I I p Iz-r7 24 4.26 0, in 0.41 a." $93-1010 12 p 11-4-13 Is 4), *p7 98.0 74.0 86.0 1: 47. to" 3 p 5+3 .17 2.37 z%'o 15.4 20.3 8.2 .1011 14 p 9+7 t4 4.4 13.0 10.0 11.94 2.62-104, Is a 1Z+3 42 R.45 6".-1 0.41, 6.38 Sj .044 16 p f, 0 t to 4 03 14.2 13.1 t3.95 3.88. lot' 17 p 2 I i IS 7:44 't G' , 0 to 6.93 0,6 tow to p 141 12 9.82 5:82 5:6S 5, v sm-up. to it Z+L, 27 1.42 40).5 41's 41.05 20 p 10-1-6 35 0. CF7 9.5.1 9,45 0.49 1.9 -SoAs ,,i At R,, + Ol't -fw.440 We-Ilk &ad 4104, 'reacks is% 064wee. Card r-fj Angular'Distribution of Shower Particles 76974 in Explosive Showers Produced by High-Energy SOV/56-37-6-14/55 Cosmic Ray Particles + 21 a +1 33 I'M 24.0 309 U.45 1.0 4069 a 7+.1 12 5.50 9.00 0:06 9 U 1,74-1011 21 P 1.1.1 20 2,((1 28.2 204 24:3 1, te - to's 24 P ~,& 4 9 0.3ts Iso t09:8 R-4.8 4, ts - to- (14 j 1) t oV2 it) 0 lie 23.6 1, 13. toll f io to -..62 *.0: 3 13:6 (6.9 5.7 toga 1 '.2 to ~,41 10.5 #.Z? 9.48 1.9 .1(01 84-26 87 1;...2 4.6 3.94 4,27 3.64-10KO 2q P W 6 M It,-, 4.9 4,77 4.93 4.&S-069 '01 P lo-f 1 29 5,V 97 to.(Yj 9.97 1,14. t0II 31 0 1+2 4.0 1.31 42:0 X.4 40,2 3,22. to,* 32 4+0 W L"90 t9,4 ts.85 11.62 6,2 Icdl -3 74 37 13.0 4.37 4.25 5.32 5.6 .1010 34 15+7 74 6,93 a,Z4 7.75 8.0 1,27 WO .11% 13+6 2$ 4.08 t2,2 9A t0.62 2.24 016 Gfj 17 Z,(M 16.4 28,2 28,3 1.6 -tots 37 X Fj+ a 31 4.74 tZ.0 toj ti.05 2,".t(00 38 a S 2147 1 +2 40 7a a :0 5:55 6,95 10.3 S. % 10.24 tt,z 10.27 Z.5 .1041 2JA ICOJ ir.-.vshe too M&OW4'. Card 3/5 Angular Distribution of Shower Particles 76974 in Explosive Showers Produced by High-Energy SOV/56-3'r-6-14/55 Cosmic Ray Particles The magnitude of the energy was obtained on the assumption of the syr-unetry In the angular distribution of cosmic particles relative angle Ir/2 according to the relations: C 19 The direction of the particle motion In tte laboratory system ~'was found to be related with thic. direction of motion in the center of inertia system 0 by the following relation: ctg t);- 7, (3) (where fJ Is the velocit of the particle in 'he center of Inertia systemi. ~The analysis 3f th~e data showed that a collision of the primary particle and nucleus leads to a synuretrical angular distribution of the cosmic particles in the center mass system, and that there is no correlation between the angles of the particle pairs in thi shower. 1. 1. GurevIc!h1o Card 4/~ L. M, Barkov, V. 0. Vaks, 0. V. Ryzhova, and AngulaIr Disitribution of Shower Particles 76974 in Explosive Showers Produced by High-Energy sov/56-37-6-14/55 Cosmic Ray Particles V."B. Fedorova made various contributions In the course of this work. The text contains 3 tatles; 4 graphs; and 2 Soviet references. SULIPI.M&D: July 10, 1959 Card 5/5 63587 8/056/60/038/005/020/050 B006/B070 LIDT11013t likollskil,I D. A.t Ulahakov&, A.-P. TITLSt Fluctuations in the Angular Distribution. of Seconlary Particles of Explosive Showers 9 PERIODICALS Zhurnal eksperimentallnoy I toorotichoskol fiziki, 1960, Vol. 38, go. 5, PP, 1507-1511 TEXTs Assuming the "two-center" model of the production of shower particles in high-energy explosive showers, the authors have cilcula.ted. the fluctuations of the angular distribution of shower particlos by the Yonte-Carlo method. In the pronent work, the authors only give th* results of those calculations and a comparison of the theoretical results with tbe.abundant experimental. material. Fig. 1 st,ows charactorintic oxszples of "two-center" angular distritutions of cosmic stower particles observed in the laboratories of Chicago, Bristol, and Warsaw. Fig,, 2 shots th& angular distribution of two particles each of those showers, whiah correspond partly to narrow and partly to wide cones in the labora,tory system. The distributions are givqn by the functioAs Card 1/2 91056/61/040/002/009/041 DII)/324 j'~ ad*t 8. Ato. Curevicht L, 1.~# 11kollskiyf, lojw Ali AUTNORSt -Z . TITLII Asymastrr of' the angular distribution of eltotrons of' ~.o decor in, magnetic fields of'strong,the up to 35,000 as URIODICALt Zhurnal oksperimentallnoy i toorstiahookor fisikil v. 40t, not Zt 196t? 452-4,54 IM Taking into account the multiple *x*hazg* cf electrons in auoaiua T productiont the sechanisa of suca depolarise.tion haw hass. studied La 2' 2- earlier paper& and the equation a &b.0.5/0+x +-T, )j (5) Obtaia*4i. Norat a denotes the aunber of siahangsa with sl*atrons, t the mean life- 4t et tiRO of #K RTA*ai= atom in the Units Aj(ht a 5'"56.10, a Paq Thor* P It the degree of residual polarization of the suoa on stopping La the moderator, &at a Ist the asvam*trjr paranater., The present poper is coa- L,7 cornod with the invostlgation-of the asymm#try of angular dLetributioa Of 2 electrons ofx.t dscay in Salbstio fields up to 35#000 of* and with the *rpianstlon of the function 0(8) in a wide range of at For oarrying out Card 1/4 5/056/61104010021009104,7 keymactry of the angular..* f the exportuentt the phatosavasion chamber* were koakardot with slow f. x+ secant a* that the Ruons war* atopped. in the chaulker. Froa tke events 'at' I-p-e decal such were sele4tedo in which the dirgation of emission of the Suou formed angles of 0-361' and tGO-150 with the direction A decal ware'oonsiler*d, of the, ftgn*ti* fiaU. Only those events of X so"aral which the auou range was greater than or equal to t5 kron, the surface of tho eaultion. In allt a total of IM650 events of x feeftey were reacrial in accordance with those selection rules. The ngl* ketwesiL the direction of onission of the, electron and the direction a of the magnetic fitli was pro4sct*d onto the surface of the sealsioa, and. .LO: the O"Jeatet anal* measure The T&IMO-Of the GOjf as deter- r I ILK(a L mine& frog the equatioat Lx(41 > 94' 1 -5(a