SCIENTIFIC ABSTRACT NOVIKOV, I.D. - NOVIKOV, I.I.
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CIA-RDP86-00513R001137420020-1
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S
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100
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Publication Date:
December 31, 1967
Content Type:
SCIENTIFIC ABSTRACT
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ACCESSION NR: AP40129b2 S/0020/64/154/004/0809/OE111
AUTHORS: Doroshkevich, A.G.; Novikov, I.D.
TITLE: The average radiation density in the metagalaxy, and aome
problems of relativistic cosmology
SOURCE: AN SSSR. Doklady*, v. 154, no. 4, 19b4, &*-811
TOPIC TAGS: electromagnetic radiation, spectral distribution,
cosmology, astrophysics, metagalaxy, Euclidean space, empty space,
metagalactic expansion, intergalactic dust, atmospheric noises,
metric space, diffuse matter
ABSTRACT: A comparison of the calculations with the observations
of the electromagnetic radiation In the metagalaxy would facilitate
the definition of the nature of galactic evolution, provide Infor-
mation on the state of the matter In the early stages of metagalac-
tic expansion as well as possible data on the processes occurring
In interstellar and intergalactic apace. Experiments in this field,
however, are complicated y such factors as galactic dispersion, the
Card
ACCESSION NR: AP4012962
differenve between metric and Euclidean space and the presence of
diffuse matter in InDergalactic space. The experiment under consid-
eration was based on the assumption that the intergalactic medium Is
completely transparent. The presence of diffuse matter alone does
not in any way affect the Isotropic radiation field. An analysis
of the observation data on the relative distribution of various
types of galaxies within the stellar population shows that Dhe
energy distribution per unit of volume in the metagalactic radia-
tion spectrum can be approximated in the optical and Infrared re-
gions by the sum of two Planck curves with a temperature of T,
10,0000K (type I of stellar population) and T2= 5,OOOOK (type
II stellar population), and with an equal integral intensity at the
present time. No reliable data on the evolution of the galaxies are
as yet available. "The authors are profoundly grateful to Prof. S.
B. Pikellner for hie valuable advice, and Acad. Ya. B. Zelldovich
for his numerous discussions of the project." OrIg. art. hass 2
figures.
Card 21A~~
Acassica NR. Ap4o34533 S/0020/64/155/005/1033/1()36
1AMHOR: Zelldovicb,, Yae Be (Academician); Novikovp I., Do
TITIE: Radiation of Gravitational Waves by Bodies Moving in the field of a
'Collapsing Star.
SOURCE: AN SSSR. Doklady*,, v. 155, no- 5s 1964, 1033-1036
'TOPIC TAGS: gravitational wave, collapsing star, general theory of relativity,
gravitation theory,, gravitational radiation friction, astronomy
ABSTRACT: In the present camwnication, the author considers the radiation of
gravitational waves by a body of -11 mans m moving in a spherical field of a
large mass, the effect of this radiation on the motion of m, and the porazible
observable effects. The gravitational radiation friction provides a force acting
on the body. This is the result of inte~wtion of mass m with its owa gramita-
tional field# which is proportional. to a 0 whereas the interaction with the
i
external field is proportional to me Thus, the radiation of gravitational waves
,introduces a correction to tha motion of a body in an extenul. gravitational field*
Calculation showu that as a result of gravitational. radiatloa# the system may
I-Card
L 12914-65 EW(I )/EWG(-.,)/EEC(t Pe-5/Pae-2 GW
~ACCESSION NR: AP4047318 S/0020/64/158/004ifOS11/0314
AUTUOR: Kelfdovich. Ya. B. (Academician); Novikov, L D.
-TIT-LE: Estimating tho mass of a superstar
SOURCE- ANSMR. Dok7,,Wy*,v.-158,no. 4, 1964, 811-814
TOPIC Uosi supetstari steiiw mass, staUar spectrum
ABSTRACT: - Analysis of obsorved data-concernlng superstars of the 3C 273 typo-Indleatoo
that t1w, continuous spectrum of tbese objects In the optical region in omittod ky a'contTal
budy w;rtli dimensiona on t1jo order of 2. 101G cm, %vidle the emission 11nes arise in the
Outur envelope measming sevoral parsecs or more. 11ic generation of thn light [low takes
place, in all Ilk(Alhood, in We Innermast region of the central body, referred to -by the
authors of 114r, wLiclc as the nucleus. They axbitrarily call the plasma s%irrounftn- this
nucleus the -"atmosphuro". The forces actimr on flic plasnia of the atmosphere al..e con-
Bid(irad for tJ-,e purpot;G- of estimating tho mass of the superstar, A fundamental assump-
tion, Is biat Vie forco of gravity Is lWanecd by ffic force of 11glit: pressure. 'nio baBle value
In tbis Jine of reasoning Is the total radiation flow. For X 273 O)c authors have adopted a
value of qe = 3.5-1025 erg/cm2- see for the energy flow at the surfaco of the Eartli. Ile
red slifft X 1/.A2 1. 158 when It 100 km/sec! MPs corresponds to a diatence of "A 5. 108
Card
L 11.M4_65
ACCESSION'NR-. AP4047318
'K
MPS, giving a total flow for the ob)ect of 4:tRJq, -.2 10" qpr/cL Tho auftrS In-
dicate that the hypothesis to the effect t1hat the light pressure in the atmosphere of the super-
star is balanced by the force of avity leads to an estimation of the mass of the nucleus of
the superstar on the order of 10wrM. Moreover, they show that in the outer parts of the
atmosphere, where the light pressure is fundamentally determined by phololonizailon
processes and not IW scat-Wring on electrons, radfation forcos Increaso sharply, 1he balance
is disruptiad and the external parts of the atmosphere are oJectiul outward, As a rossiblo
mechanism for the generation of the energy of the superstar, the authors point to the
accretion of atmospheric matter Into the small circumference of the coUapsed nucleus.
The mt1ty of Incident matter, necessary to provide the light flow observed, Is about
ryea~. This mechanism is said to be self-regulaUng. Orig. arf. ham 6 formulae.
3 M
ASSOCIATION; None
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:ACCESSION M 05004841 S/0269/64/0OO/012/Vo76/oo76
.SOURCE.- Ref. zh. Antronomi3rat Otdo vyp., Aba. 12-51.620
1AUTHOM Novikov, L D,
of energy release during the collapse of a quasar
CITED SOURCEs Astron# tairkulyar, no. 290, apr 8, 1964, 1-5
:TOPIC TAGS.* asar, gravitational collapse, gravItational ener 'electrottagnetic
g7
rrAintion energy, bydrcoagnetic wave
'TMMATIONt The last stages of collapse of a quasar are accompanied by a strong
fjncreave of the magnetictieldo The ckange in the field during the twoceso of
;'compression leads to'eleatremagnetic radiation. The total amount of radiated
:energy is determined by the expression
M,
'R
Card 1/2
L 38565-65
:ACCESSION fiRt AR5004841
km, d/R, d mean
vhere R gravitational radius, equal to 3MIMa / etic mo-
t en M - 100 M(b and the field inten ity-d ing
imentga R - radius of the stir. Wb
the last stages of the collapse is H su 109 G. the radiated energy is 0 ;; x 110,15%
erg. The radiation is producedin the case vhen the den3ity N of the Plasma Our-
rounding the star satisfies the condition
01RI > 2nW.
;vheree electron charge.' In the opposite caaeg a hydromagnstic wswe is pro-
duce-1. E# Kotok,
~GIM COM CP AA MCM 00
2/2
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NOVIKOV, I.D.
Delay of the explosion of a part of the Friedman unirerse
and superstars. Astron. zhur. 4.1 no.6:l(y75-1083 N-D '64
(MIRA Ml)
N')V I K~"-'
SWA KOV So
meruine as --r r~(,a
thpin' Surnociel 'Tiy,~, nar
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L 5444..66 T.'4T(1)/EWP(m)/T IJP(c) G11-1
ACCESSION VH: APW19230 up/oo%/65/049/001/0170/0181
AUTHOR: DorqshkTdqjit--A# G.; ZQVA hP--Y%-qj3j NOVINU& X, Df
Gravitational col:~~Ge Of aaymmetricai and rotating masses
SOMCE: Zhurnal eksperimentaltnoy I teoreticheakoy fizikip V. 490, no* 1, 1965v
170-181
TOPIC TAGS: gravitation, stellar evolution, ramagc=v gravitation effect, griLvitar-
tion field
ABSTRACT: The theory of stars contracting without limit, hitherto developed for a
simple model of a spherical body., is extended In this article to include non-
spherical and asymmetrical stars. It Is proved rigorously that the characteristic
pattern of gravitational self-closing is valid also for the general case. Morcoverp
collapse of a non-rotating body leads to damping (proportiora.1 to the reciprocal of
the time) of the quadrupole and higher field moments as seen by an external observer.
The variation of a rotating body Is shown to be different. The changer. in the
metricp connected with the rotation of the local inertial frame,, are shown to tend
to a nonvanishing constant value., but otherwise the collApce remains qualitatively
the same os In the spherical case. Static nonspherical solutlens of Einstein's
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ACCESSXOH HR: APW19230
equations are investigated and the properties of the SchwarzachilA surface are ana-
].~rzed for the case of static fleld with axial symmetry., e. rotating body with an ex-
ternal fieldp a Schwarzachild sphere in an external quadrupole fieldj, and the cal-
:lapse of a perturbed sphericaL dust cloud., Orige art. has: I figure and 20 form-
lag.
iASSOCIATION: none
sumaTTED: iLftec&
,e
Im BEF Ml 006
IML: 00 M CODE: GP# AA
OTM: 910
Car, 2/2
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AC=109 NR9 AM1%O9 vR/dO53/65/066/003/04kT/0"6
525 + 530-12651-51
AUIMORt Z*Vdovichp Uo B.;-Novikay
A I* D.
Tr=t RelAtivistic astropEysics. rX.
t' aOUWZ: Uspekht fizicheakikh nauk, Y. 86p no. 3j, 1,96% 4kT-536
TOPIC TAGS: astropWices radio astranoWs, stellar evalutioup cosmogotW
AMTRACT: The first part of the article was published in Uapekhi fiticheakikh
nauk v. (V4-,9 577P 196k# and dealt with the conditions under which stars go over t
the neutron or collapsed (cooled) state. The present part Is a review of the
literature up to the end of 1964s deals with the dbsemtio=L properties of star:,
that are on the "Me of collapse or neutronizationt and analyzes in detail how a
star can either mold or reach the allte of collapse. Somw problems concerning
quasars# for Vh1ch there Is no complete theory as yet# are expounded. The section
headings aret IG Introductione 2o Equilibrius of a auperwassive Aare 3. Xqui-
librium of a rotating star with r a 4/5. ke The possible occurrence of a super-
vassive stare 51, Evolution of supermassive stars. 6. Evolution of stars of medium
muse To Notion of trial particles and M4#rt re" In a SchwarzachUd fiald.
S. Radiation of grwwItationaL wev it, 9e Collapse of rotating star. 10. Collapae
of nonspberleaL boOre Ile Does rapid rotatlon Interfere with collapee of it. St"41
cacj 2/2
L 2009-66
Acewszow nRc AP5G166og
12* Comparison with abservationse 13. Accretion of g" by neutr= and cooled starse
1111rowtoft i ---
Magnetia arid ~.W~c phenomenso 15. quasars ("xuperstare")
16. ent theory of quasars. ITe The anticallapgo IWpotbealse ;MdIxI
Literature. Ortgo, art, has e IT figures wid 1W farsdas.
AwocrMOINt now
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KOVIKOVP I.D.
Mechanism of energy release during the collapse of superBtars.
Astron. tair, no.290sl-5 Ap 164. (MIRA l8slO)
1. Otdeleniye prikladnoy matematiki Hatematicheakogo instituta
imeni Steklova AN SSSR.
_2 76-66 F-4T(l)
ACC NRs 11,146olo4W
SOURICE CODE: MV0386/66/003/(Y-,',~'0223/02zt*
AUTHOR: Novikov, I. D.
ORG: Division of Applied Fathematicat L41~.h
Acad.crq-,o.f ((rtdclenlye prikladnoy matematIM Matematichealtogo ini;t
Akademii nauk
TITLE: Change of relativistic collapse Into anti-collapse and kinematics of a charge
sphere
SWRCE: Zhurnal eksperintentallnoy I teoreticheskoy Miki. Pialm v redaktaiyu.
PrIlozhenlye,p v. 3,, no- 5, 1966, 223-227
'~_Yl_
TOPIC TAGS: co~2 ~go ~, gravitation field, gravitation effect
ABS,rMCT: The author shows that a collapsing star, on reaching the Schwarzachild
radius) and going beyond It, may reverse its motion and expand from under the
Schwarzachild sphere, but Into another external region (which is Euclidian at in-
finity) with the same properties as the first external region end situated in the
absolute future relative to it. This is demonstrated for a sphere of charged dust
in a strictly spherical geometry. The change from contraction to expansion within
the Schwarschild sphere occurs without the matter going through infinite density
(except for the particle in the center). The sphere is assumed to be uniformly
charged and the charge did not become redistributed during the course of the collapse.!
The contraction gives wey to expansion not simultaneously, but beginning at the edge
GV
G-V
2
L
ACC t4R, AP6=44o
of the sphere and moving toward the center. This is demonstrated bZ inver-t1gating
separately the motlon of a point on the surface of -the sphere and internal points
under the combined influence of the masses and charges acting on the particle in
question. OrIg. art. has: 1 figure.
SUB CODE: 20j. 03/ SUM DATE: 24jan66/ oRiG RF.F: ooV ow Rw: oo3
L 44706-ff cE11VT ( IGj
ACC-NR.-AP6-031342 SOURCE CODE: UP,/03%/66/0o4/oo
AUTHOR: Zel*dovich, Ya. B.; Novikav, I.-D.
ORG: none
Z7'
TITLE: Charge asymmetry and entropy of a hot Universe
SOURCE: Zh. eksper. I teoret. fiz. Pialma v redaktslyu. Prilozhenlye Y. 4, no. 3.
1966, 1.17-120
N't
TOPIC TAGS: cosmo, stellar evolution, entropy, gravitation effect
ABSTRACT: The authors offer a natural explanation of the small charge asymmetry of
the Universe at high density, which is deduced from recent measurements of the cosmic i
background of radio emission at wavelengths 20, 7, 3, and 0.25 em, which have con-
firmed the theory of the hot Universe. The dimensionless entropy (per baryon, in a
system of units where the Boltzmann constant is k = 1), amounts to approximately 109.
This means that there are approximately 1043 quanta of electromagnetic radiation per
b&rjon,and approximately as many electrons and muonic neutrinos. The almost-charge-,
syrmetrical atate becomes rational if it In assumed thall a phane when matter was cam,
pressed existed at t < 0. In this phase (at t - -1020 see) there were no antibaryom
at all, and only baryons existed (nucleons, ordinary nuclei, ions, and atoms). The
average density at this instant was 10-30 g/CM3. It is further azm=ed that up to
that instant there was released an energy of the order of E - 10ye erg/g as a result.-
of nuclear reactions or gravitational processes. During the course of contmation,
Card 1/2
L 44706-66
XCC NR,
this energy (which initially could be in the form of optical quanta and high-energy
neutrinos) should be tr2nsformed into equilibrium forms; the presented value of E e;~'-
sures the necessary entropy. In this case the occurrence of baryon-antibaryon pairs
and the surprising almost- charge- symmetrical state are already a natural consequence-
of the known laws of physics. Consequently, during the expansion phase there exists-
the same high specific entropy and almost complete charge symmetry at high densities.
In particular, it follows from this that cyclAc evolution with an infinite number 0:9
contraction and expansion cycles does not agree with the finite value of the entropy
S at the present time. This quantity, which is fundamental for cosmology, may POS ..
sibly be expressed in terms of a combination of atomic and gravitational quantities.
The expression for 3 differs from the outwardly analogous formulaz of Eddington, Dirac~
and others in the fact that S is a local quantity and the expression has been derived
logically, from a consideration of physical processes during the course of the evolu-
.tion. It can be concluded on this basis that the Universe is 100% charge-aymimetrical,i
with the exception of a short high-denaity period, when it in almost symmetrical for
natural reasons. The authors thank B. P. Konstantinav and A. D. Bakharoy for discus-
:sion that led to the formulation of the -probletm-considered in this note. Orig. art.
!has: 1 formula.
.SUB CODE: 2o/ Sum DATE: 2jun66/ ORIG REF: oo4/ 07H RM 005
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-25
ACC NR: AP6027542 SOURCE CODE: UR/0384/66/000/003/0011/0013
AUTHOR: Novikov, I. D. (Candidate of physico-mathenatical sciences)
ORG: none
TITLE: The discovery of primary radio f-requency radiation frcm the metagalaxy
SOURCE: Zemlya i vselennaya, no. 3, 1966, 11-13
TOPIC TAGS: radio astronomy, galactic radiation, metagalaxy, space research
&B,137FAC7: -ine author explains why the general radiation from -space on the 7.5 cm wave-
length is significant in our understanding of the evolution of the universe. In the
reglon of lower radio frequencies (wavelengths greater than 3 cm), the principal radia-
t1on is not produced by stars and cosmic dust but rather by non-thermal processes in
our galaxy and in other galaxies, particularly in radiogalaxies. The possibility ez-
.st5 that intergalactic space contains quanta which originate not in galaxies but, ra-
t4cr 1.0 billion years ago before the galaxies existed. At that time, the densit-I of
matter was not less than the nuclear density and this density decreased as the metaga-
laxy expanded. According to the "hot" model of outer space, the temperature 10 billion
years ago was very high and the density of radiation exceeded the density of matter.
After a long period of time, after matter expanded to its modern state and galaxies and
stars were formed, the primary radiation still remained. At the present tirne, the den--
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ACC NR, AP6027542
sity of primary radiation in accordance with the "hot" model is much less than the der-
sity of matter while the radiation temperature is only 1-100K. In 1965 it was report-
ed that the American radioastronomers observed radiation at a wavelength of 7.5 cm as
predicted. This corresponds to a modern temperature of 3.50K for primary radiation.
Thus the conclusion is confirmed that matter in the far past (10 billion years ago) was
in a dense state and was at a very high temperature. If future radio frequency obser-
vations confirm this discovery, the scientists will obtain Interesting information con-
cerning the far distant epoch which determined the modem state of the metagalaxy.
Orig. art. has: 2 figures, I photograph.
,SUB CODE: 03/ SUBM DATE: none
ACC N ~' A116035556 SOURCE CODE: UR/0269/66/000/010/0076/007G--
AUTHOR: Zelldovicli, Ya. B. ; Novikov, 1. D. ; Syunyayev, R. A.
TITLE: Methods of investigation and the cosmological importance of He in the
intergalactic matter
SOURCE: Ref. zh. Astronomiya, Abs. 10.51.572
REF SO'(;RCE: Astron. tsirkulyar, no. 371, apr. 27, 1966, 1-3
TOPIC TAGS: helium, model, star cluster, intergalactic helium, cosmological
model, (piasar spectrum
ABSTRACT: An investigation of intergalactic lie would make it possible to
determine tile degree of isotropy in-the expansion of the metagalaxy in its early
stages and the present density of intergalactic matter. Observation of tile follow-
1119 phenornena is suggested: 1) light absorption in quasar spectra by intergalactic
Ile remaining in its basic state; 2) absorption lines of neutral lie in source spectra.-
located beyond the cluster of galaxies; 3) neutral lie radiation lines located in
clusters of galaxies; 4) He3 observations by radio methods. The presence of
intergalactic He, which, according to the "hot" cosmological model, represents
i_Cc.,d_ - 1/ 2 UDC:52301
ACC NR- ARG03555G
r*--J 3016 of the gas which has riot passed the stellar state, increases the rate ol
intergalactic gas cooling and changes the conditions of its ionization. Bibliography
has 6 titles. A. Zasov. [Translation of abstract] [DW) i
SUB CODE: 03/
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Novikov, 1. D.
17, Cortraction to oxj~nzion. and
pl.-,Y:3-,Cal Ch arac tics durin'; contract~,Or,
S 0 ~-,, C v. no. 911-C)18
TOKC TA33. Coz;.-._IoCy, astrol;"aysics, evolution
A337RACT: of otol'Lar c',-.an;,,c from ro--, zivirtlc gravitational contract-Ion,
or to in eLz;o of 3"r~; L;Tuil-lor t~rioir
JraV4_~ation:,I -d_-,IL discu.3~;Lid. In thu of a charged sr~.oro, infinite
clu,nsity clooL; not havo bo a'-iainn by xcopt for t~-io particle ir, the
icenter o f t,- o .3 for au :-, " ` -
2 C.-.:~ng(j tc, occar. dan~,`ty of mz_ttor in
de-~or7."4_ncjd by t*:-,o tor.-, 10 ~~ C-~M4 C ~_- T-11c of 1-'7ht, jr, i5 tho and
c'-IarL:u. Tho rasu.1'65 o.-'-, '-ned t,no charj(,d model ::Iould irdLcato the
natu-r-D of ~n tu.,10 1,01,--L. of tho Change from ra_Iat;.vist_'c Contraction
~o o: a neutral zt-ar, L---tabillity of spherical Contraction
and possi'--le procGsaec; at _u,_(~r hi-h dcns_-_iaL over 1093 Lm/cm). or, c."ango
from Contraction to ox-par,51on are c~.-:,aus5c_d for comoloGical models. "ZaG author
Cord I UX; 523.11
ACC INR. 0 33: ! 6 !
th--n'-s *.-'-,. . Z. Zolldovicli for mary st~mula',-4-11r- d.'5c .-i~,ions . 11 Orig. art. ha.:; ; 4
f~zurQ~ Lxlfa Q,
SUB COLZ: Oll/ SUE" LATZ: OweD6~/ * GR:~, GIC/ Ozi Rus 009
~ Card 2/
NOVIKOV, Illya Dmitriyevich; KONDYUKOVA, P.D., red.; AVDaEVA, V.A.,
fe-MF. - -re&-. - -
(Efficient organizers of the masse3]Boevye orpnizatory m3s;
iz opyta partiinoi raboty. Mo3kva, Sovetskain Aossiia, 1962.
63 p. (MIRA 15:11)
1. Sakretarl Partiynogo korAtetij zavodr, "Sarp i ro1ot",:'oscoIj(for
Novikov). 2. Chlen partiynogo komiteta zavoda "Serp i r,olot" MOSCOW
(for Ryzhkov). (Moscow--Stool induntry)
(Com.-unist Party of the Soviet Union-Party wor'c)
NOV:KOV) :.F.
Iz kafedry
rEeiiit,ginskogc, in.-A 7
b o I I n I f, sy lme y t-y i,a n L
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STAROSTIN, Petr Fedorovich; NOVIKOV, I.I., red.
[Selecting optimum structi4res of rubber seaIings, V:;bor
optimalInykh konstruktsli rezinovykh uplotnenii. Lenin-
grad, 1964. 13 P. (MIRA 18:4)
w ri I \ r\ C' 1, 1 - I -
1. VALUEV, I. V., NOVIRO'l, 1.1.
2. USSR (6oo)
4. Grinding and Polishing
7. Machine for lapping priamatic grooves, Ston. I Instr. 211 No. 2
1953
9. Monthl List of Russian Accessions, Library of Congress, . May Uncl.
- j
USSR/Miscellaneous Machinery
CarE t 1/1
'Authors V Movikov, 1. 1.
Title Application of combined multi-blade cutters
Periodiftl Stan 1, inatri, 3, 33 35, Mar 1954
Abstract A detailed description of combined multi-blade cutters used in machining
various articles. Diagrams are included.
Institution :
Submitted :
!;v it L.:
i UM/ Engineering - Machine tools
end 1/1
ARUwm Novikcrw,, 1. 1. and Akimov, N. H.
Title t k highly-efficient device for rolling semi-finished components with
complicated profiles.
Periodical, j Stan. i rndtr.j Ed. 6, 33 - 34, June 1954
Abstract t The employees of the machine construction industry in cooperation with
the scientific institute, designed and built a device for rolling semi-
finished components with complicated profiles on a turret lathe. Dear-
cription of tha above device, is presented. Diagrams; illustration.
Institution
Submitted
NOVIKOVO I.I.; KALININ. H.A.-
Attachment for cutting blanks for Woodruff keys. Stan. I instr. 28
no.10-'38 0 157. (KIM 10:11)
(Grinding mchines-Attachments)
AUTHOF: No4lk-oQ. 1,1,
TITLE- eads w1th LI ~e fc,-, Ttird f,,epa:u,-,rj, , f
(GOl-,VkI pia ap-t~m,:hlm tsentrom (Ilya kni
.I)braL-.-,, ~*, -t iy)
PERIODIL;AL: St-3r,,ci Ins, (ument 19'--8, Nr ~i, 35 k'' Li3R)
ABSTRACT! 6evoraj 'ype- )I.Trep-3finLrIg, tocis are
de s -- j be- , hoi~-s of 0mm d-,ameter in
shee" a maridrel *w"th a mcurited ~r(lw.,-, catter arid
a _i-., ~ --ni-nS in needle bearingS i~3 in
r ii, c) I e sA 15or i rig head w 1 t L I nterc hangeabl e
atA i it r .3 r --, a-'s,-. carrying iv
L 0 a 1 0
ni F The aiya-:tatia torl bits move
w. th f,,ermanent
J L 7r j r j e ,,)no -~i ', on ~:- en J , a nd a
-1.,ve n -e ;~t -i~- n both types r,17 trepannifig drill
h ea Tn e _- w n I Y n i -Itter ma7 b,-) -LntapTal or provided
with ~art:'If c(it*,nw, r.or,"n InSeT~.R, T~i,~i-e ar- I fit~ures.
Card 1/1
--.mWvlxov I'l,
MillIng hft&4o un"d for vuschinins, alumirium rilloya. :;ttLri.1 Instr.
?9 no. 11138 11 '511. OfIIIA 11111)
(14111ine, ruichines)
NOVIKOV. I.I., Inzh.
Hermetica!17 sealed joints of distant rings of an assonbled piston
for a nonlubricated compressor. EhIm. msh. no.6-32-31 ?~-D 159.
(MI-iA 13:3)
(compressors)
- -.A. C")
s F"'4 (' 0/0 (" 0 /o /0 G fi ;~ 0 1
IT 11()~" 140q A'~ I A! '0
AUTHOR:
TITLE: C.,::,,-,TjtjAt I ~)n c ttj.- f - cf I r-. cut,~d -,1 Stor, ri -'1"75
PERIODICAL: Khimicf~eskcye z12-z6
7EXT: t~.~- jurp--~j,~, -f -raphite cum-ore.3jor
rinC~ -nist ~,f tl,rt- ~~r,3 with re6ard
r .. , '
to rnet"I'l ~tijt~'ri L 1, ye~.- , P. 11, -
R~f I N a k ~'.n ti-jk -.y ty,i I I P ten L-r-, i Ai j,,. .,.-o po.' i tpkh,-,- cheskogo
2 !~:3 k V N R,.:" i Avt~*raktornyye dvi6atf.',1
Au * em 1 ai~ r'~ T r~,: n o ~j S e I z, ~ur'~!i3ha, 3 N. , yu-
h, iia , A. 3 2 n s t r t j j t lokomohi Iya (Theory
,1,~L3ign afct - a I - -, i I a t the lq'-2~, cannot be applied
to non-lutr~cut'2j jiqtr~n r"nf-') Th,! fri -ti -,r. 'orr:- is ralculated accordine
to Formula T K - , ,P u-ij;m',n6 that th'? (,u0 (-r. rlr,6 .1'all3 from pl to
P2 Fcr:es effeztive the inner s--irface -f ge67-,-?rt are shown in Fi-
g-dre 2 Calc'jla': Cr..3 3hc,-.-,, that the force which preases the 3e6zment to the
c-,,'.*.'r;der Ires t,Gt if--~end on the rir,~; Hav~.no: chta-.ned the va,,-;e
C a r I
20163
q I C, C c' 0 2
Coal put at I ur; C1 fr i ('r' 1~f' A'G .'+, A'G
, t i C o r, 3 4 3 tn ,o fz - r i n - 3
T the f rj,
tale' cylinder j'rQ33'_;re and the :'ricti~n lcj.; are cal,~-_Ilated Tests were car-
ried out at constant _~rcjslire on U C37,j)reJ3or erjjji~ped
with a f-,y1tn1t?r cf 10 =-i diameter (D piston strokp 160 mm, (S), rotation
apeed 300 rpr.,. (n) All Piston parto w1 th tho ,xceptlon of rings and sprirjA
were made of sta,nleso steel, Piston rln~;s (h - '0 t = 6 am) consisted
of three jeL.'T.4~rts preojed to the -~ylind~,-r hi a flat sprint; at 0.6 kg,/aq cm
preus,;r. . P:,3ton rin,r5 -s;-re made a. ord, !1c lo -a L;-ecial methcd developed by
LhF, authcr R- f 9 - P c, r j hn e vy ~, r ~ o, ~ t 3 a , ra t 7, t A~- -i L; h c h i y P lt,e z u ma zk i ( P i 3 t on
riri6s Wrrkii,.t., w,. th,_~ut lubricants) , Loriin~,,radL;Viy dom nauchnoy-t(Ahnicheikoy
r c pa6a ndy s i y a "Mcd e rr.1 z ai ,y a , a,,, t z, ma t . z a t. j ; y a I r em on t o bo rud o van iy a"
n c" 4, 19~oj a (D) 6ra~~.Ite wa3 t'(%r -~Igtoni and s,,ip;ort rin~_;S. The
fri-tion "er- :'f :omj~resaor Nu~i -,(~a3ur,d ty a %ew method which is
briefly descr'ted. Rint,:j wer t-inod on tl-ie -rirq;rf?sjcr for 90 hra. During
the firit 30 ~r5 therp was a constant pre_--s,zr~ of 10 kg/sq cm inside the
Outon A brief _1C-!3cr,,jt1(_)n of the n(,*hod and condi'lon5 'la given, Fit7are 6
shows an elustir cyl~nier support u.3,A for kirio:tir tejtL1 carr.ed cut at con-
stant pressure wi th air ~'unj-.d into the container by a lubr-cated compre.33or.
It was later that the kinet,.-~ c,)eff-_-_,~nt had increass~i d.-k-
Card 2/~
3/1 F34/60/000/006/0061/01 2
Coi-inutation of the friction of ... 101 //"11 ~0
to the presence of lubricant'-- in Friction force and friction
losDe3 can be calculated and IL~a a'. con3tant and
approxi!.iativc at LIt(!--?ut-,.n,,- T!~(- fric'.ion of nioton rin,:o CLU.,3,-.(,,
. ;, r -~ o:v ii
by aj ,)reS:3UrU dUQ!3 no,. depon.,! o:'. Can. be cale"11 tod e!%-
~ir!cally ...... ("r0:) in cm. "he fric-
at i
tion force and durLbility on force P e of o p r in co 'lib o t r -~~ c -
tei-13 notes desi(:naticr, e -J:-, -_i tran:,,lat"on fron thc Ru.,3jian
(upruGoat.1)7 . Thio dependcnc~, ii; particularly evidont at low precoureo.
One 'r:glsq cm of elaitic force cauiej th, friction a3 6-7 kdoq Cm L-I'a!3.
The value PY should riot exu,,~ed 0.1 - 0.11 cm, particularly a3 there were
ca~;eo of ring3 operatInj 7Plutalova, L. A. - Ref.
Anti friktoionnyye L;mazk-' ~A.Pt~-frictllon ma-
Jal.q operatinf, ~ait!.~ 11 z d a t , 1 "' 5 7 1 -Overall fr4 C -
ter UUrI C arlt~; r,
tion inoitle pioton `:izit: Ili(, )I--jU-,,e dro-) rather than on the
distribution of pre. ure on piolon ririC~'j. ':Ii(-- productlun mothod of onn1I
,;rLL-)h-Jt(.! rin,~~,- with interchan,-,~-,'Dic, J-~Ipjnti3 ;)roved jatinfactory and 3uited
for industrial pur.)ote~;. Th-re are 0 f 1 La,'~ ? ref erences: 1 ',',orman and
a 20"riet.
Card 3/5
S/18 60/000/006/008/Cl2
Computation of the friction off... A104YAl 70
Ndl~
P,
41~
Fi,-,~ire 2:
DiaL;ram of foraes actine on inner
jurface of 3conont
Card 0
3'1/10-1/60/000/006/000/012
. 0 -, " " I -:r,
C',).'~:putati(jn of frict."Or, (,f ... A. . .-
71"7kire ():
Zlu.ittc cylinder support
Card 5/5
4-A
-0 () 7- >-
NOVIKOV, I.I., inzh.
Effect of ras pressure on the performance 3f the 7raphite piEton
rinp. Kh~m. mash. no.4:20-24 Jl-Ag '61. (KIRA 14:6)
(Piston rinf_rs)
L 4.i7a:-ja_
17
11-~iGkv 1-'.PR1/T-2/V4P(b)
A~XGSSSMIINR: A.P5010899 UR/0286/65/OW/007/0087/0083
AUTHOR.% NqVikqKs 1. 1.
TITLE: Gra hits Riston rinj~/Class 2'j, No. 169733
S~UfCz-,: DyuUetenl izobrateniy i tovarnykh znakovp no L 1965s 87-88
TOPIC TAGS: piston ring, graphite, po_mpr~q~sor
ABSTWT: This Author Cortific -ate proserts a graphite piston ring, as- for instance
for compressors working without lubrication. The ring has one or several looks.
To facilitate the constraction md to extend tho longevity of the ring, the looks
ara mtido in the form of rough cracks formed in the ring by.zubjecting it to a
machanicaliy applied force.
ASSOC'MI014i, Uningrad-gUy filial nauchno-isslodavatellakogo in3tituta
k-himichaskogo mashinostroyeaiya (LaninTrad Branch of the Seientific Research
bitut a--of-Chopic al-Yaabip-a-C onsti-uotiqn)
SUBIMMD: 201W64 DMOL; CO So COM Iz
No PEip Sov, 000 OTHM 1 000
Card
.66-- W(AVEWP(OZE
Ke -&pSOZ898Z SOURCE CODS: UR1014916510001004/0131/0133
Novi
AUTHOR: Navikovj, 1. 1,,; ks re so
ORG: Moscow Institute of Steel and Alloys,Non-Ver ous, Rare, and Radioactive Metals
tavetnykh,
redKIM L tedLoaktivafth metallov)
TITLE: Effect of straining rate on the plasticity of aluminum alloys in solid-liquid
state
SOURCE: IVUZ. Tsvetnaya metallurgiya, no. 4, t965, 131-133
TOPIC TAGS: strain, elongation, aluminum alloy, tensile test, plasticity, liquid
state, soLidus
ABSMCT: The effect of straining rate an the temperature dependence of relative
elongation in solid-liquid state was investigated for alloys with variations Ln,,The
thickness of liquid intergr4nular layers. Binary Al Rllovi with 1.5 and 6.5% Cu-*ks
well as with 0.6 and 5% SiPgreatly differing In the amounts of liquid phase in the
lower part of the crystal-Dizatim Itage, were selected for the investigation. The al-
loy specimens were annealed for 2qthr at temperatures of 0.9 a.p. Tensile tests In
the melting range (on heating specimens from solid state) were performed at deform-
ation rates of 8 and 80 antwin, Findings: an transition across the solidus to the
UDC: 669.715
ACC W, A25028982
~'j
region of solid-ligul state relative elongation either abruptly falls to a fraction
of a percent or rmains unchanged or slLghtLy increases over some te"Wrature range
(in the brittleness range), whereupon, with increasing temperature, it continually
increases. If the liquid phase to abundant &ad its intergradular layers are suffi-
ciently thick, the straining rate greatly affects the degree of relative a
'~Ongation.
The Al alloy with 5% Sit with its considerable amount of autectict is chs4actorized
by extremely thick liquid intergranular layers throughout the btittlenessiliange, and
hence in this case the straining rate greatly affects elongation (increase in strain-
ing rate from 8 to 80 molkin reduces relative elongation from 0.7 to 0.2%). By con-
trast the annealed Al alloy with 0.6% Si and the alloy with 1.5% Cu. which contain
no eutectLc, contain an extremely small amount of Uquid phase in the brittleness
interval and hence for them the straining rate does not affect plasticity. It is in-
teresting that so long an the Al alloy with 5.6% Cu contains little liquid in the
brittleness interval(at up to PsM*C), the straining rate does not affect elongation.
once the temperature is raised above this limit, however, the amount of liquid increa-
ses and elongation increases with decreasing straLning rate. In addition to tensile
tests in the melting range, tests in the crystatlization range, with cooling of spe-
cimens from liquid state, were performed. The resulting pattern of the effect of
straining rate on plasticity was the same. For example. for the At alloy with 5% Si
conversion to straining rates of 5 and 2 mm/min caused a further increase In elonga-
tion within the brittleness range. Thus, a change in straining rate markedly influen-
2/3
-- L- I,35,-19-66
I ACC Nits APS029962 I
0 j
Ices the leval of relative elongation to the brittleness range. if the liquid Later-
I
igranular layers are sufficiently thick. Grfg~* art. has: 2 figures. I
SUB COOS: 11, 13. 20/ WM DOLTS: 26Apr64/ ORIC RU: 006/ OTH Iff: 003
MOVIKOV, I.I., dotsent.
HistoloCical structure of mile sperm. Nauch.bi,il I,~n.un.no.2l:.?-'
26 148. (YL.V. 10: 3)
1. ]Wedr& darvinizma.
(Asses and mules) (Spermatozoa)
NOVIKOV, I.I., dotsent.
Htstologi,~&I structure of togates of hybrids obtained b:7 ~,roisslng
tha AslaticwIld ass with horses and asses. Rauch.blul.Len.un.
no.21:26-28 '48. (MIRA 10:3)
1. Kafedra darvinitma.
(Asses and -Tulea) (Testicle)
1. T.
movirow, I.I.
Zffect of Intervaristal blood tranafuaion on the color of fur
of rabbits. Uch.csp.len.un. no.165:215-216 153. (KERL 7:7)
1. laboratorlys b1ologit ravvitlya 4hivotnykh kafedry darvinizma.
(Rabbits) (Blood--Transfusion)
IZTKO'i', T. T.
NOVIXOW, I.I.
fleteratransplantation of overtes. Uch.rap.Lon.un. mo. 165:209-214
'53. (MLRA 7:7)
1. Labaratortys biolegii razvltlya shivotnykh komfedry darvinitma.
(Transplantation (Physiology)) (Ovaries-Transpl&ntatten)
11OVIKOV, I.I.
Changes in the DIMentation of Himalayan rabbits rewilting
from the transfnaion of blood of a different breed. Z~nir.
ob.biol. 20 no.):214-215 14Y-Jo '59. (KIRA 12:8)
1. Leningradskiy gowuiaratvenW universitet im. A.A.Zhdanova.
(IMBITS) (BIA)OD-TIMSFUSIO11) (COLOR OF ANIMALS)
.!~OVjKQV,_j_van_jymoxic.h; GOROBETS, A.M., kand. biolog. nauk, nauchrVy
red.; VOROBIYEV, G.S., red. izd-va; CRJRDZMr-,VA, A.M., tekhn.
red.
[Is everyting expedient in living nature?]Vse li toolesoobraz-
no v zhivoi pr1rode. Leningrad, Vses. ob-vo pa raspr. polit. i
nauchn. znanii RSFSR, 1961. 59 p. (MIRA 15:12)
(Zoology-Ecology)
NOVIKOV. I.I., kand.iskusstvovedeni7a. arkhttaktor.
Experimental construction of apartment houses made of
large silicate blocks. Opyt stroi. no.8:33-52 '57. (14IRA 11:1)
(Apartment houses)
(silicates)
(Precast concrete construction)
NOVIKOV, Ivan Ivnnovich; CIMR14OV, Te., red.; YK,10ROVA, I., tekhn.red.
(Tiling] Plitochnye raboty. 14ook-va, Kosk.rnbochii. 1958.
30 P. (MIRA 13:1)
. V11
1. Brii:adir plitochnikov 82-go npotaiiiliziroviinlogo upmvltinl.
trasta "14osotdoIRtroy" No.2 Glnvmosatroya.
(Tile construction)
IIDVIKOV. I.I.. kqnd.Iskuastvovedsnt7a arkh.
planning in pnople's 4amcractes. Op7t stmi. no.14:
3-65 158. OGRA 11:10)
(Sbrope. Rastern-City planning)
- NOV.IKOV. 1.I., Imnd.iskusstovovedeniya arkh.
Constructing houses iising effective building materials. Owt. strol.
no.19:51-86 '58. (KIRA 12: 1)
(Silicates) (Building blocks)
NOVIKOV. I.L. kand.isk-uontv.nauk, arkhitektor: SKOROV, B.M., kand.
tokhn.nalik, red.; 140ROZOVA, G.V., red.izd-va; RUDAKOVA.
S.L. tekhn.red.
[City building in foreign countries (France, the Netherlands,
Belgium. Austria. and the German federal Republic] Iz
praktikt Irradastrottalletwi za rubachom (Prantatin. Gollandiia.
Bologlia, Avotrita i FRG). Moskva. Goo.izd-vo lit-ry po ntrolt..
arkhit.i stroit.matArialam, 1959. 73 P. (Opyt stroitel.stva,
no.25) (MIRA 13:2)
(Europe, Western--City planning)
,,-.DGV A.P., * - i ~ . '. 1. , ... I, :!C)l
0
9
PI i,~ I -,. I :,uil,lin, - --,, I " ~ . t :-,- * n *( r, -~ C! -, : -
( , ;, 1, 1, -, t - ),, - 31: '1- '~' '- ( , 1, , '. :
(c . It I-J.", , , ( p , c;- 3 " 0 ~ n, ..
,. , . , .
1. i.
"Arterial Blood Supply of' the Pons Varolii of the Human 13raiij."
!-'os(~ow 3tate !~:edical Inst. irf-iii 1. V. "talin. "o.-~c-wy I I . ~ !J ~:spr-
tation for the Lef~me of Cwi(J,clate hi :e-(;ical ,riencc)
So: Kni7hnaya Intopis', 7o. 2 7, 2 Jii'-,,, ~951
U M / Humrn -nd ,niiarl i,orp:,.olovy (Norrarl -rd p., 010 -3'
t-h
Cardiovascular 3-steri.
r ( 01
Abs Jour Ref Rilur ~- r~iol.' 1:0 21, f958p rlo 97085
,,uthor i lJovikol',
Inst : 2nd I;oscc,,4 'I.edicpl Inctitute
Title : Blood &up.ly of the Pons V-rolii fror. ..rtrries.
Orip Plob : TJch. z-p. L1-: ) osk. mod. in-t, 1257, 14, -~2-95
,,bstr:,ct - It wns s1-invin on le prepnr-ti.nns of t'., c-~rt`,,rum
by Yn~Ahods of momntiry pol,' chronic injection of .,essels
~nd by pr~_prrrticn, that from th,. dors,-! surf-cc, of the
b:-,s:-l rrt(.ry, 5-8 nedim -rterk-s b- in, which ent-r
the su'-,st--nc(1-- of U~c. oons v-rolii lon .-It~_rn~-l border
of th,, sl)lcus b.-sil-rin -nd nt:n-Ar-t_- throu.-l- t~_ ontir,~
m:,ss of 41- onn up to rV ventric1c. In t z rupion of
districUtIon, 10!urc nrc pyrnmid-1 tr-cts, 1-_ mclki of
the ponn itsclf, tho inturn,-1 p-rt of t,-,oi nx_dJ,.-1 1-~mnlscus,
tho posterior --ongituciJi.A. f~!txiciilus, Vic nucleus :,nd
Ccrd 1/2
NOVIKOVI I.I.
Do-relopment of the innervation of the co=rr, carotid arter7 In man.
Top.morf.perlf.merv.sist. no.4:159-178 15P. (KIRA 13:5)
(CAROTID ARTERY-IMMUTION)
"0v-,- -.-
N I 1 1, - -,,, zind -ei L~ci - ( , ii, -- -, , De ve - .7~7ne -- t o ~* * r - -. --v - - !
j )/- 4,.,. ~~ rq , It I- 'IJ-14-0-
0, -ve:,sels xx L;lQ I (---dl 4amit-. 1,
1L. pp ("i"Isk t,; t,f' 1.0d ~ - F ., ( -,, - , , , I ,.
I
- bji -
GOUTB, D.m.; AAVROS'YRV, A.P.; LZONYM, T. .
KIMIRAN, F.B. ..-_ I - _, A.~ ~_, ;-ORWVA. B. L. ;
Formation of new sensory paths In the pelvic organs. Dokl.AM
BSSR 3 no.3:121-125 Mr '59. 04IRA 12: 8)
(Viscera--Innervation)
HOVIKOV, I.I.
"'he right subc1avian artery as a highly sensitive reflexogeai.- zone.
7drav. Belor. 5 n0-3:50-52 Mr '59. (XIIA 12:7)
1. 1z, kafedry normllnoy anatomil (caveduyushchiy - prof. D.K.
Golub) 14inskogo ieditsinskogo, inatituta.
(SUBCIA71" ARTIRT-INNTUATIO11)
MOVIKOV. 1.1.
Role of the superior cerebellar arteries In the blood 9upply of the
pone varolii. Zhur.nevr. I psikh- 59 no.8:944-9146 159. (HIRA 12:12)
1. Irafedra normllnoy anatomit (Eav. - prof. 7.N. Ternovskiv) II
Konkovalcogo meditsinskogo instituta.
(PONS blood supply)
(CYMELLUM blood supply)
110VIKOV, I.-I.-
Innervation of Botallo's duct in human embryos and fetuses. Vop.
morr. perif. nerv. sist. no.5tl9-30 160. (MIJU 14:3)
(DUCTUS ARTERIOSUS-021ERVAT ION) (FETUS)
(FETUS)
I-IA43HALKOVICH, D.B. P polkovnik meditsinskoy sluzhby; SAGiallIKO, N.L. , podpolkcvnik
meditsinskoy sluzhby; BELOUSOV, G.G., podpolkovnik meditsinalcoy sluzhby;
ImIKOV, 1. 1. -mayor meditainf3koy sluzhby; FUVAIN, M.A., myor
.___m6JlT_u_Eikoy sluzhb~
Organization of work at a receiving and sorting section of a thera-
peutic ho3pital. Voen.-med. zhur. no.6:15-17 Je 161. (14IRA 14:8)
(IIOSPITAIZ) (RADIATION SICIUIES.9)
SUPRON, L.F., dots., otv. red.; A.~INCHIN, N.I., prof., red.;
GELIDERG, S.I., prof., red.; KLEPATSYJY, B.I., prof., red.;
LIBERWIl , G.Ya. , prof. , red.; NOVIKOV I I. , kanLi. med.nauk
red.; RAZWOVICII, A.P., assistefit, red.
[Abstracts of the reports of the Fourth Scientific Session
on the Problem: Physiology, Morphology and Ppthology of the
Cardiovascular System] Tezisy dokladov Nauchnoi sessii po
probleme: Fiziologlia, morfologiia i patologiia serdechno-
sosudistoi sistemy. Grodno, Grodnenskii mod. in-t, 1962. 20? p.
(M IRA 17: 10)
1. Nauchnaya sessiya po probleme: Fiziologiya, morfologiya i
patologiya serdechno-sosudistoy sistemy, 4th, 1962. 2. Zave-
duyushchiy kafedroy patologicheskoy fiziologii Grodenskogo me-
ditsinskogo instituta (for Supron). 3. Zaveduyushchiy kafedroy
normallnoy fiziologii Grodenskogo meditsinskogo instituts. (for
krinchin). 4. Kafedra normallnoy anatomii Grodenskogo meditsin-
skogo instituta (for Novikov). 5.Zaveduyushchiy kafedroy mikro-
biologii Grodenskogo meditsinskogo instituta (for Gellberg).
6. Zaveduyushchiy kaffedroy obahchey khirurgii Grodenskogo medi-
tsinskogo instituta (for Klepatskiy). 7. Zaveduyushchiy kafed-
roy nervnykh bolezney Grodenskogo meditsinskogo instituta (for
Liberzon). 8. Kafedra biokhimii Grodenskogo meditsinskogo in-
stituta (for Razumovich).
NOVIKOV.9 I.I.
Irmervation of the subc1mr1u, ll-n 'Icp. w-r-f*
perifo nervo sist* no,6:143-152163. 0-mu 16:10)
(SUBCIAVIAII ARMY - 1',IEII,-I,!.TIO";)
NOVIKOV f i.l.
Arteriovenu3 ara3tcmo3,,.,q In thin i;,_iI of tnu, nilryin
artery. Arkh. anat., gi3t. i emix. 45 no.7:10,.r*107 I e 63.
(YI li.A IV: j.,
L Knfodra normtdInoy anatumii (zav. - prof'. A.11. Gaouzov)
Grorininkogo meditDinskogo inotituta i kafodra normallnoy anatomii
(zav.- akIL-InMik AV BSSP nr-'. D.11. GnIub) Kins~-,n
'-'-)it_ Adros avtora: Grwinc), ulAso Onosricr, 1, ',',enitsinqkty-I
institut, ka-fedra normall noy anatorn"I.
'1-: 'U
n n
r In re
u: 41
A, ri 4;";u rmu,~
GOLUB, D.M.; AHVROSIIEV, A.P.; LEONTYUK, A.S.; NOVIKOV, I.I.; ORLOVA, B.L.;
MIRWIt F.B*
Data on the formation of new afferent pathways in the urinar-f bladder
and large intestine. Arkh. anat. gist.i embr. 38 no.1:3-19 Ja 160.
(MICA 13:7)
1. Kafedra anatomii cheloveka Nav. - prof.D.14.Golub) Minskogo
meditsinskogo instituta i laboratorii morfologii Instituta fiziologii
Alcademii nauk BSSR. Adres avtorov: Minsk, Universitetskaya ai., 2,
14editsinskiy institut. Kafedra anatomii cheloveka.
(BLADDER-INITERVATION) (INTESTMS-INTIEWATION)
WIV 1 i. W.: ,
~,~v of blor-d v (I as c 8 of Fuj r :,,,w n 2rf,.r!
t, I ar r t La ~ ~X, n C. a C, t, r. e , k e I riomal and eype.-
i! m b!- 49 no 8
P- r"'I 11 t ~ C', na rkh a na t 19 t
'Y. v l1," 7 A~i '1,)'v
A -Y I K l:Wl g~, s),-, -ir q7~lrl i2C Mp~l n,,j i., r
r. e r 1 1%) 1')
IF A,
01 Ad A,
,
it .11 th" IAt-lat
A,
ISO -00
00
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NsFertation: "On Certain Themodynale RevularitJpr of ths? Rftal (Nonconce"title)
ProcesFes o2 Gas and Vapor FlawG.ll Po-:ei- En -inecrJnr- Inf3t., 1!-reni ('~. M. Krzt-.iz.-a,.c,,S!a7,
Acad. Scl. USFR, 19 Jun h7.
So: Ilechei-nZaya Voskva, Jun, 190 (Projcct #17P3()
UL
,~, A
L. ucavwc&sw-
It Id
topwis 5-1,97% i'm don ad VW
I-ow). mammal comolknit. == Isufto.
I%". Mr. RW. Review*4 to UlsAAi Fit. me*&
Itu ).
sc M I ).
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Atsmucilwimi, I In Ruixian I 1 1. Nuvlkl)v. th".,mig
00 J'viLA*w*r*CaLt's.Ak (Ji)urnal ,f T.,chnical Physicsi.
Y. 18, Har 194.4, p. 345 164
00
A formula is tirrived which inves the average
041111 .3 dlamct~r. .( th., droto Comporivim with rapirri
mental data sh,,** t e oxtr~m. a--urarv ,f Ow
00 00
formula. 09
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00009000000000000000:01000*00000*0*0000000oeoo
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Ker 1948
Thermodynamics
Stem
"Adiabatic Indicator of Saturated and Damp Stem,"
t. 1. Novikov, Naval, Acad Shipbuilding and Armanent
Iment A. N. Krylov, 3 pp
"Dck Akad Nauk SSSR, Nava Ser" Vol Mr, No 8
1 a - I+ L.J-- 1-1
Gives Mrasaian for value of the adlqbatlc indica-
tor as
TAJ.7T42
dood. for both a constant gas and for damp steam.
glaborates, an-thia equation. Su ml~tpdby_Academl-
*U= M. V. Kirpicher, 17 Jan Ign. '
FA 517'05
21 Nor 19W
Shock Waves
016clatenco of Rarefaction Shook Wexesp* 1. 1. NOVIkOTSi
UT Mad 6111pbuilding and Armment imml A. 5. Irrylov,
2 pp
69ok Mad Namk SSM, Nova Bar" Val LIX, So 9
Vb - 1114 r- G
SmIkWo research loads to coacItAlon that In ==qat
of water steam at near critical pr"sures It In therw
dynamically possible to have formation of rarefactIon
shock waves. Analogma conoluslon vill hold also fW
aller nubstances.
ft, - -- - 51M
lvuvlF.r,,v, 1. 1.
27601. N)VTKOV, 1. 1. Cl skachkakh uplotneniya, voenikayuchshikh Fri neravn-ve-
snykh khimicheskikh prevrasbehiyakh v sverkhzvukovim potZke raza. zhurnal
tekhn. fiziki, 1949, vyp. 9, s. 1053-55
SO: Knizhaya Letopis, Vil. 1, 1955
NOVIKOV, 1. 1. PA 46/49TIO7
(MR/Physics im 49
Gas Dynamics
Gas flow
I-Polytropi c Prorqmsom in Grae; Flow, " 1 . 1. Norikor,
5 PP
"Zhur rekb 1?i z x u, No 'D
Sbovs tho P,117t-OPir procasses are impossible In g&j;
flerva in whAch thti rhbtkga In state of a maring gas
satleflee thij p-,r- . const, where the irAox
of polytropy rA s,-~rn,9t, In ganeral does not equal the
a4isbatic In-lei cp Sutmitte4 U Jun 48
46/49TIOT
Z3
V-1
t--
_:4
04
*'- ZAAI * A:) ~ -00
(wha A, - wje, w, aid w, mV ps Vgeft MW .06
*6 0. 00d 01 dW so-COOd crkkd 0 - 1, be(OM W4 =60
4ACI d* -dd- d-se. S*KiOM > I
000 Na an dw uppa F ri of dw cww~ WWO _am
-- I U
~ : 06
00 .3 O On k9 lower bnw
Vw bwer bra
1
.
conewcn& 10 Am- ch-4" Q( wwvmmm a
goo
tht WSLW 4VP,' iAL WO llb,,* pMCbWo Wea
(,W No 0( 16C "m - -crewov,& to vim. ,**
cks"- of C-A&ct'^ dks WAW Wn to viddin go*
so dw4P Of 0000(ugi= dwftdclild by ,Vww,,,c -.00
2 md-dwo Vccd. The Elua OMW,,,m a,,Om
COO
*0 t 40f --WY rfgm ttbc OcdxLgFY wft by UnV
001 k
cd dwzw- -Jym U*Y am dwandrsamcat, 104a
powdAe~
F LAcXk4.%
Igoe
a*
w
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r
a* WOO
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u
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0 4 0 0 0 4 a 0 a o
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. . .1 1 - I . -
I
y
I
I
VUKALOVICH, Hikhall Petrovich; NOVIKOV, Ivan Ivanovich; AORYUSHCUNKO,
A. I., redaktor; FRIDKII, A. 1., tekhnicheskly redaktor.
[Technical thermodyTAmics] Tsichnicheskain temodinamika. Izd.
2-oo, porer. Hoakvu, Gos.enorg.izd-vo 1W. 136 p. (KLRA 9:1)
(ThermndynanicB)
NOVI KO V~
AID P - 2573
Subject USSR/Engineering
Card 1/1 Pub. 110-a - 12/16
Author Novikov, 1. 1., Doc. Tech. Scl., Prof.
Title Thermodynamic theory of thQ regenerative cycles of
h1gh-preosure oterim power un1t3
Periodical Teploenergetika, 8, 51-5L, Ag 19715
Abstract A theoretical and mathematical analysis of the regener-
ative cycles for feed water determining the temperature
by the optimal effective power factor of the unit. Two
Russian references, 1951-1953.
Institution Moscow Engineering and Physics Institute
Submitted No date
MOVIKOV.I.I., professor
Internationad scientific cooperation on the peaceful use of atomic
energy (at the Geneva Conference) Vest.AS SSSR 25 no.9:47-61 S'55.
(Geneva--Atomic power--Congresses) (HLRA 8:12)
'"KI) V
0
V /
USER/ Cheiristry Physical chemistry
Card VI Pub. .22 - 23/47
Authors I No Ivikov, I.. I.,
Title. --OWMAMOMMO:
Two type-j of phase diagrams with conLTuently- melting chemical compounds
Periodical. i Dok. AN SSSH 100/6., 1119-1121, Feb 21, 1955
Abstraot I Two basic types ofp~ase diigr-ams theoretically formulated on the basis of
geometrical themodynmics are described. The basic differences between
the two phase diagrams is that in one case th~ compounds, melt congruently
in the distectic point and in the intermediate point in the other case.
The phase diagrara with compounds congruently melting in the intermediate
point was found to be the independent type wMch reflects the real phase
conversions. Three USSR references (1935-1947). Diagram.
Inatitut:~on *00.0
Presented by Academician A. A. Sochyars September 218 1954
H-,v,,;tc-j Nti~:Iear Erigineering and flower, C-~~
Abe* Journal: Ro=f-rat Ze.-jr - Fizi j
_ka, 11r, 12, -,956, )1~14l
A ut hrj r
InBt I t
Title: K