SCIENTIFIC ABSTRACT KUZNETSOV, V. F. - KUZNETSOV, V. G.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000928210003-6
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 20, 2000
• Sequence Number: 3
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

22394
S/12o/61/000/002/004/042
72 42. E032/3114
AUTHORSs Dulint V.A., Kazanokiy, Yu.A., Kuznetsov, Y.F., and
Smirenkinj G.N.
TITLEt A single-crystal, fast neutron scintillation
spectrometer with discrimination against gamma-rays
PERIODICALi Pribory i tokhnika sksperimenta, 1961, No.2, PP-35-41
TEXTs The transformation of the amplitude distribution due
to recoil protons into the neutron energy spectrum in the case of
a small crystal (negligible multiple neutron scattering) for
which the light output depends linearly on the proton enorgyt can
easily be carried out by differentiating the experimental
spectrum. In fact, in the case of stilbone which was used by the
present atithors the relation is not linear and small crystals
cannot be used if an adequate counting efficiency Is to be
obtained. The light output due to recoil protons and the form of
the amplitude distribution due to monoonorgetic neutrons was
investigated using a Vtn do Graaf generator and the T(p,n)He3,
D(d,n)H*3 and T(d,n)Ho reactions. Neutron on rgies in the
following ranges could thus be obtained3 0.375, 4-7.5 and
Card l/ 7
R~
2
M

21394
S/l2o/6l/000/002/Oo4/o42
X032/Z114
A single-crystal, fast neutron scintillation spectrometer with
discrimination against gamma-rays
17-22 Mev respectively, Th amplitude distributions due to
recoil protons for 4,3 and 16.8 Mev neutrons are shown in Fig.l.
The recoil-proton energy distribution F(E) can be obtained from
the amplitude distribution 4~(V) with the aid of the following
relations (V)dV - P(Z)dE,
P(E) 4) [V(Z)l ~ff . F(E) dV
dZ a
The functions V(E) and dV(E)/dE which are necessary to compute'
the neutron spectra are shown in Fig.2. The experimental values
of V(E) are well represented by the Birks theory (Ref.1)
according to which
E E
V(E) "--dE' const dER 3)
S dIS E 1 + kB,dEI'idx
Card 2/ 7 0 0

11394
S/120/61/000/002/004/042
E032/Ell4
A single-crystali fast neutron scintillation spectrometer with
discrimination against gamma-rays
If dE'/dx is expressed in Mev/cm of the range in air then kB turns
out to be 20 cm/Mov, Fig-3 shown the recoil proton spectra for
1.0, 1.8 and 3.6 Mov neutrons. These curves were obtained with a
cylindrical stilbene crystal (30 mm diameter, 15 mm long). The
curves have a hump at the high energy end which is due to multiple
neutron scattering. The latter effect in small for neutron
energies greater than about 2 Mev. It can therefore be neglected
at the higher energies. Fig.4 shows the energy dependence of the
resolution of the aingle-crystal spectrometer. The resolution in
the energy range 1-22 Mev can be described by the formula:
ILS En /En a .20/ '/"E _n%
The efficiency of the spectrometer can be described byt
I - exp, r -j(E n)dj
(En En E
Card 3/ 7

23394
S/l2o/61/000/002/Oo4/o42
E032/E114
A single-crystal, fast neutron scintillation spectrometer with
discrimination against gamma-rays
where 6E in the differentiation stop for the recoil proton
distribution. The efficiency for the above stilbene crystal was
found to be about 3% at 2 Mev and about 0.3% at 10 Mev (the
differentiation stop was taken to be equal to the energy
resolution 4~En)- The discrimination against gamma rays in
based on the differences in the effective scintillation decay
constant for neutrons and gamma rays. The present authors have
used the scheme suggested by Birks and described in detail by
F.D. Brooks in Nucl. Instrum. and Methods, 1959, 4, 151 (Ref-5).
Fig-13 shows neutron spectra for a Po-Be source (curve I -
present results, curves 2 and 3 due to B.G. Whitmore and
W.B. Backer (Ref.71 Phys.Rev., 1950, 78, 799) and J.0. Elliot and
W.I. McGarry and W.R. Faust (Phyn.Rev., 1954, 93, 1348, Ref.8).
It is stated that the overall efficiency for neutrons having an
energy of 2 Mev has been increased to about 10%. The gamma ray
efficiency is lower by a factor of 100. Acknowledgements are
expressed to L.D. Gordeyev, Yu.1. Baranov, V.I. Bol'shov and
Card 4/ 7

S/12o/61/000/002/004/o42
A single-crystal, fast neutron.... E032/E114
Yu.V. Pankratlyev for assistance in this work.
There are 14 figures and references: 2 Soviet and 7 English.
SUBMITTED: June 26 1960
P(
48
1414'.."r ,,
44
0 4S 1 4f2 4S i
Fig- 3
Card 5/7
Fig.

/000
AUTHORSs
TITLEs
21j,06
510091611011100610021014
B102/BI38
Loypunakiyo A. I., Abramov, Ao I., Alekoandrov, Tu. A.,
AnWn,,-.a,I.j Bondarenko, I. I., Gussynov, A. G.,
-14iiiov, V. I., Kazachkovakiy, 0. D.k_.Njj ~netsov, V. F,,
Kuziminov, B. D., Morozov, V. N.,
SallnikoT, 0. A., Smirankin, G. ff., Soldstov, A. S.,
UoaohQv, L. I., Tutkin, M. 0.
Investigation of the $P-5 (BR-5) fast reactor (spatial and
energy distributions of neutrons)
PERIODICALt Atoanaya energiya, v. 11, no. 6, 1961, 498 - 505
TEXTs The fast research reactor BR-5 and its experimental equipment is
described in brief and some of its neutron spectra are given and discussed.
The following date are givens fuel - plutonium oxidel coolant - sodium;
reflector - thin layer of natural uranium plus thick layer of nickels
power - 5000 kw. The reactor has many vertical and horizontal holes for
technical and p1sysioal studies and is well supplied with experimental
equipment. Leypunskiy gave a detailed description of the BR-5 reactor at
Card I/P

211406
910191611011100610021014
Investigation of the... B102/B138
the Second Geneva Conference (1958). Inside the core the neutrons have
energies of more than 100 key which they lose almost completely in passage
through reflector and shield. In the outer layers of the shield, -their
mean energy does not exceed some tons of *v. In the kev range (E,>50 kev)
spectra were measured for the moat important beams and channels. For tb 0
other cases, they were determined from threshold reactions. The soft part
of the spectrum within the reflector was determined from the spatial
distribution of neutrons with E,!A5 ov, recorded with Cold resonance indi-
cators. The total neutron flux was determined only at the points where
the Pu 239 fission cross section was constant. Direct neutron
r,:Pectrum
measurements were carried out in a vertical (0K-70) and a ho antal (B-3)
channel using jHe3+Ar)-filled ionization chamber in the first cane and the
neutron t=naniasica method with n-hexane in the second. The neutron
spectrum of the horizontal channel was also determined by photoemulsions.
From the rates of indicator and fission reactions Au 197(n r). U231(n,f)
PU239(.,f), T032(. 'f)~ No 23(n,r) Cu 63(a,r), and A127(n.,j,) the abrupt
Card 2/s j,

510091611011100610021oli
Investigation of the... h102/B130
drop In neutron energy In the Ni reflector one determined, and the
activity caused by resonance neutrons (E The fast neutron
n ' 4.9 ev).
14
flux (1;
n.>1.4 Mov) in the core center was found to be (2-4 t 0-2)-10
and total flux was (0.2 t 0.3)-1014. Exporlmont4l. results were verified
by energy-group calculations (16 groups). Good agreement bQtveen theory
and experiment was oleo found for the channel spectra. The authors
thank 1). 3. Pinkhaeikt N. N. Ariatorkhov, and the reactor personnel for
assistance. There are 10 figures, 2,tableng and 2 Soviet references,
SUBMITTLI)i August 17, 1961
Table 1. lteso*tion cross sections in the core cer)ter.
Legcnds (i) Renotion'l (2) experimentl (3) a o5joulated, given In barns.
Pigil~- Neutron trannmisolon spectrum (n-hqxeqe) for the horizontal'
channel B-3.
Card 31p'7

L 149~2-6) E:PF(n)-2/SWT(m)/BDS AFFTC/ASD/SSD PU~4 DM
AMEWWNIRI AP3003980 8/0069/63/025/001/00(i4/0066
63
AMORSt Tu. Aeo B=d&r*nkoq 19 191 tuxn*tnov. V Pop Resterov, To
Okolovich, Ve Noo Sm1reukin, 0, No.
TITLE# Number of prompt neutrons and kinetic energy of ft!Mnts a low-numa 11
fission of U sup 235
SOURCEs Atommya energlya, vs 159 not 19 1963t 64-"
TOPIC TAGSi prompt neutrong Vsup 2359 kinetic energy ofiLasion fragment# Fowler
hypothesis
ABW RACT iAccording to Fowler's hypothesing the kinetic energy of the fission
fragment does not depend on the excitation erergy of the splitting atemo from
vhicli it follows that the average number of prompt neutrons (aenopen*) is Im.
creasing linearly with the increase of the energy % of neutrons producing flesione
For large %# this approximately valid,, but may not--be correct for low %* The
present work vas conducted In order to investigate the lover E range In greater
detail. The data sought are Important practicallyp and my he?p to clarify the
nature of tbelLssion channels and the mechanism uhich produces the distribution of
the observed energy. U235 was used targetl the reaction T(p# Alpha) was pro-
1/2
Card

L 14932-63
ACCESSION NHs AP3003980
duced with an electrostatic ginerstoro The correlation between In and agnovano
to presented in three f Igureso The results are discuestdo "ph* authors Givress
their deep appreciation to A. -I. I*Yrwm--kiy for attention and constant Interest
to workp to Le N, Ueachey and V* No, for ftitful discussion of expartmentaf
rewilts, and eratitude to V. 1. Polvehow. Le D. OoEdmyovaa and Up 1, rokhmm
for help with the work and partiallpation in various stages of antunmentso"
Orig. art, haso 3 figuns,.
ASSOCIATIONs none
SUBMTEDs 04Aug62 MR Me 08Aue63 ]MCLs 00
-$"I - -003
Cord 272

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1. s h ow-n zhat 0., 1 ' r a

can opien up at energies iilp to f-yr.,tatircrn anerqy'
2
pLua-uim;u vi an energy gap In the lcvel apectrum of the
I-rans4-Uon nucleus, W Iikewiae explain tha observed decrease
-in the number of a-econdary ftsaion neut-rons neal- 2.2 C"LeV. Other
m, a .1 at a are inte rpreted in
ji I_lt 0[ th(_~Se eSU I ,Is Orlig.
N'? -PET

. - . . ~ - , , : - ,
L. I.; RABOTNOV, N. S.; SMIREIM,70. N.; USACHEV, L. N., CYbninsk
"Effects of energy gap in channel opcctrum on the fission process."
report submitted for Intl Conf on Low & Medium Energies Nuclear Physics)
Paris, 2-8 jul 64.

L,'~Z
D,;japlrig capw~!.ty of a !rt a
'I. Mctlk-~vskly in3litut (-,UTTW3 elt~,(f t Tx. Wri nk
i korrienclovana kmVedroy avtomat.l.Rl' I upravip-ty-uoh h. M, %.s hn

YUKHOV, V.V., inzh.; KII MM4-_V inzh.
4F- p
Automatic device for regulating the voltage of storage batteries.
Elek. eta. 33 no.8t85-86 Ag 162. (NIRA 15t8)
(Voltage regulators) (Storage batteries)

GORBUNOV, Pavel Petrovich; jg%~~ Tladjm4r 2- SrIch. PLATOMOT.
ppo
S.A., red.; MMIKOVA, A.N., takhn.red.
(Radio engineering and its applications] Rediotakhnike i so
primenenis. Nookya, Voon.ixd-vo Y--va obor.5309 1960. 375 p.
(HIRA 1N12)
(Radio, Kilitery)
1-01

KUZNETSOV, V.F., inzh.
I:---'.-.- Modeling the electromechanical turning system of an ESh-50/125
walking excavator, Izv, vys, ucheb, zav.; gor. zhur. 6
no.10:147-154 163. (NIRA 17:2)
1. Moskovskiy institut radioelektroniki i gornoy elektromekhaniki.

NECHAYEVO A.A.1 G014BERGp V.S.j KUZNETSOVp V.F.
Tedhnology of a system for the purification of dril1ing
mud, Trudy KNII N? no,170~-66 162.
Experimental investigation of the hydrooyclone purification
of drilling mud, Ibid.t67-87 (MIRA 170)

KUZNETS , insh.
Tooting of Dr AZhHts 10-3-1,5 bronze hardness. Metalloved. i
terms obr, met, no,8t46 Ag 162. (MIRA 15sllY
. (Brorse-te sting) (Hardne ss--Te sting)

E
KUZZIETSOV, V.F.; rVANTSOV, L.I.
Results of the use of tissue preparatims on the collective and
state farms in the Russian Federation. VeterinarJia 40no.8:9-10
Ag 163. (IffRA 17 110)
1. Zamestitell nachallnika Upravlonlya veterinarii Mi-.1isterstva
proizvodstva i zagotovok sel'skokhozyaystvennykh produktov RS-rSR.

IMU!VXa4p4lj Yo lolfich; ITANOT, K.A., redaktor; TIUIDNOTA, Te.A.
W.Wo-w"w'. ~ , _ ,#qr-l
vsi~i~ ty, iodaktor.
(Navigation] Navigataiia, Moskva. Izd-vo "Morekol transports
1956. 367 pe (Kl-'RA 9:6)
(Navigation)

KMNETSOV. V.G., starshiy inshener.
- I In
Us= a~-'Iieating of the oil vell bottom. Iffaftlanik 2 no.ltl6-17
Ja 157. MR& lOt2)
1. 3-V promysel Neftepromyslovogo upravleniya Mmdyshenneft'.
(Oil wells)

KULIIZTS(YV V.G.; DMCIJEV, V.I.; IUIYAZEV, V.S.
Some problems of the petrography of the old weathered
silpoe of the Zirabulak-Zi"tdinskiye Mountains (western
Uzbekistan), Trudy MINKHiGP no.251334-317 159. (MIRA 15:5)
(Uzbekistan-Weathoring)

XUZUTSOV, V.(L: 11"CIM. V.I.
Litholo&7 of the horlson 12 (lower Albian) in Kagan structures
(western Uzbekistan) WA the paleogeograpby at the tive of its
formation. Trudy NYWHIGP no.27s256-265 160.
(KIR& 13:9)
(Uzbekistan-Rocks. Sedimentary)
(Usbakistan"Faleogeograpby)

KUZNk:TSOV, V.G.
Conditiona governing Ue formation of oil pools In Pashiya
layers of the Bol'ohekinell flexure. Gaol. nefti i gaza 5
no. 3:40-43 Mr 161. (MIRA 14:4)
1. Wentraltnaya nauchno-ioaledovatellskaya laboratoriya treata
Orenburgneft,4;azrazvedka,
(Orenburg Province-Petroleum geology)

BSLOKRYLOVA~ T.G.;,qZZT=4 VjLG,. MOZHAMI N.S.
Oil potential of the Lower Carboniferous of western Orenburg
Provinces Geol. nefti i gaza 6 no.12t/+l-" D 162. (MPU l5tl2)
1. TSentralInaya nauchno-ispledovatel'skaya laboratoriya
tresta Ore:nburgneftegazrazv*Aka.
(Orenburg Province-Petroleum geology)

KUZUETSOV, V.G.
Features of the oil-bearing Lower Carboniferow sediments of
Orenburg Province. Trudy MINKFiGP no.431298-306 163.
(MRA 17:4)

GRACHEVSKIY, M.M.; KHMEZOV, 1821-
Paleogeography of the Bobrikovskii time in the central trans-Volga
region. Dokl. AN SSSR 150 no.lil46-148 Yq 163. (WRA 1616)
1. Pred~tavleno akademikom D.V.Nalivkinym.
(Volga Valley-Paleogeography)

Kul"ITETZIOV7 V.C..
r ~r,
Typen of ventdorlc no
In OrenbLu*g 1r-3vll!(X, nrld AO,~r,(enL reglww. I-ady V14IGNI no.36t
210--218 163. (MIR-A 17:9)

K11"'NETSOV
Oil Mid gfu jx;tun'~.111,1 oc "he 'nf tile Upp-r
Ajv,nilan-huzmai otago, iii OranLniri7 fvvinceo TrrD rise u?hebo
mr.; no"O' I E;az 7 Wflbk 18cZ)
t~azovoy promy-sh-

KIJ21ETSOV V.G.
Simple and effective method for examining feces for helminth
ova. Med. paraz. I paraz. bol. 33 no.12105-108 Ja-F t64
(KIRA 18-.1)

I A UZI '%r CraT E~ 'in ~i I--zf

3 1 IIIC10006166looolooololoolo
ACC NR, AT6o3652z 100
Alri.10M Vikhrovp A* 1.1 Kolomonukiy, A@ Vel SmirennVg L, No Dudkin, Ve Yboi
Kovalay. Yo&J4 Ku4M-tWhJAQh-,
OI.G: none
TrIMS: Principlea of calculating chielding from coamic radiation fp-aper prosontod
at the Conforonce on Problems of Space Hodicino hold in Moscow from 24 to 27 May 1966J.
SOURCO: Konforontuiya po problomam kosmichoolwy modituiny, i966. ProblopV koopdchou-
koy moditairxy. (Problems of space medicine); m~torialy konforontaii, Hoacow, 1966, loc
TOPIC TAGSs apacecraft shielding, radiation protection solar flare, cosmic radiation
biologic effect, radiation shielding
cosmonaut frbn~ high-energy corpuscular
ABSMACT.. The problem of shielding the'
radiations is formulated in the following manner: for given conditions
(trajectory, flight duration, etc.), the main-shielding requirements must
:be determined (type and thickness of material, arrangement of shielding,
;etc. ) in order to protect cosmonauts from irradiation in greater thazi per- I
:rnissible doses with Tninimum additional weight of the shielding. -This
article describes a paper In which: 1) Chief aspects of methods of calcu-
lating. sh~ekdii.~g were examined, 2) Mean tissue doses for monoeneri. "ti
Cord 1/2
ell
N

proton fluxes, for proton spectra from solar flares and the Earth's radia-
tion belts were c&*Iaulated. 3) On the basis of these data sample shieldin
calculations' for some spaceflight trajectories were made. 4) The question
041 the reliability of'radiation protection of a spacecraft was discussed.
At the end of the Ipaper the'main princi plea of designing shielding for-.--,
,140#~d spa i4!ed. 221 ATD hiporC 9)4W
were form,.
SUB cost 06t 180 22 SM Wits 00i*r66
Card --2L2-'

SOURCE COD91 VJV0363/6~/001/007/1027/1038
ACC NRI AP50~29W
AUTHORt Yallseyev, As A Yarembasht Yes I 1_10anetsovt V. Go; Antonova, L, 1,;
Stoyanteovat-:Z. F,
ORGs Institute of General and Inor-Ganic Chemistry Imo N. S. XuriKkko
5 Academy of
Sciences SSSA-';(Insifiti hdiO7 i_iFei_ria_nT4ifii_s_ko7i Wait Akademil nauk SM-R)
TITLEs X ray phase an&lysis of Asthanum tellurides
SOURCEt AN SSSR. levestiya.lNeorganichesklys materialyt vo f. no* 7. 1965S
1027-1038
70PIC TAGS: 6re earth elemen~p'l&thanum compound, tellurldep phase diagram,
crystal chemistry% arystal-lattice parameter
ABSTRACTs Crystallophemical properties of lanthanum tellurides have been studied
,by x-ray phase analysis and differential thermal analysis of the polycry9talline
samples which were synthe;1sed by a technique proviousIr described by the authors
ghe neorgan khimli,,99,8 6'(1964
9 ff. The complete phase diagram of the La-Te
System was established for the first time on the basis of the now data. 110mo-
geneity limits of the six Identified phases were determined. e of the six phas*sp
La2T95, was detected for the first time, The phase Previo~jri dent If led as La4T97
a of
was fowkd to be L&Tel.We Cgetallographic charac risti of all phases were
given.,_The exidtance of the MTO A and ItTO phasesp vhere.-M is a rare earth
element from Ce to Sat Was pre;;W2~~ the growWe of crystallochemical analogy
cewd 1/2 UDC% 546.,6541241s$48.19

AP%222rh
between the rare-earth tellurides of other tnws, Orige art, hast 8 tables mid
5 f Igureso
SUB COM 07 SUIN RAIXI ORIG AWS 006 MR 191PI Oil
Ccwd 212

,cc* R,'Ar6o36526' SOURCE CODEs /M/000/0099/0090
N
AUTHORI Vesolovukiy, Le No; Gribovt Be So; Kuznotsov, Ve Go,* Sakovich, V. Ae
ORG: none
MILE: Heasuremont of absorbed doses of intermediate noutrons ff-apor presented at
the Conference on Problems of Space Ifedioine hold in 11.oscow frovi 24 to 27 Lay 1966J.
SOURCE: Konferentaiya Po Problonam k6amichookoy moditsiny, 1966. Prol)lovV koardeb
1coy m-ditairy, (Problovis of space Wdicino); matorial~y konforontaii, Moscow, 1966,
TOPIC"eAGS: noutron radiation biologic offoct, cosrde radiation biologic effect,
radiation shielding, radiation protection, radiation dosimotry
ABSTRAM: Study of the edectiveness of biological shielding of a nuclear reactor
,showed that the most convenient method of detecting intermediate -energy
neutrons is neutron detection with preliminary moderation. The sensitivity
of such detectors depends on' moderator thickness, and also on the geometry
of the mode rator-de te ctor system as a wfiole. Detectors with isotropic sensi-
-tivity received the most attention, In order to study the angular characteris-
tics of neutron fluxes,'a directional neutron detector with variable moderator
thickness was created for biological shielding. The sensitivity of the de-
tector was investipt.ed with monoenergetic neutrons in the.range 30 kev to

13 Mev. It was found that ~se' of different"moder'~tor thicicn'esse*s peimitsi
measurement both 6f neutron fluxes in the energy range 30 kev-18 Mev,
and of the ph sical and biological dosesproduced by them,/ff. A. No. 22-;-AM
Report 66-3.1J6
suB coDr!,3 o6 suBH DATEt oomay66
Card 2/2
'-W7~

ACC N-R% SOMS CODS-t - E,1666-61661661~ldbdlooq�10100
Au7,,.(n,: Vjkhrov, A. I*; Dudkin, Vs Yoq' K(YvaU'!, Ye. Yo., Kumotoov, V. G.;
Srdronnyy. L. N&
OLIG; nono,
TITI;-,: Evaluation of radiation hazard during a flight to the moon fapor proaontod
at the Conforonco on Problems of Space Hodicine hold in Moscow from 24 to 27 'NaY 1966.1
SOMICO: Konforontsiya po problomam koamichoulcoy mditsirky, i966. ProblorV 1counichou-1
koy rrditainye (Probloma of space modicino); matorialy konforontaii, moscow, 1966, 1
99-100 1
TOPIC TAGS: lunar spaceflightj cosmic radiation biologic effect, radiation dosimotryi
raaiation protection, solar flare, radiation pormissilolo dono
ABSTRACT: During *iunar flight and lunar landing cosmonauts will be exp .osed, to
Ille'Earth's radiation bellk;s, galactic space radiation, corpuscular radiation
from solar flares, and lunar radiation itself. It has been calculated that
during passage through the Earth's radiation belts, which win take approxi-:,
rnately 30 min, the mean tissue dose will not exceed 3-5 rem. On the 11
',30-day lunar flight the dose from galactic 6pace radiation win amount to I
approximately 4-8 rem. Solar flares rej~resent the. greatest radiation.

7
Atc_'Nk,__A'
hazard "Lor lunar -fligl~t. With~ shielding of ^-1 g/cmF the surface"dose- can
reach %, 10 4 rem from a high-intensity flare. If the cosmonaut stays, in a
Yadiation she ~' er during a solar flare, the obtained dose can be lowered to
50 rem or 1(!ss. The probability of an intense solar flare during a period
of maximum solar activity is around 1dja (for a 30-day period). Doses
from galactic space radiation-and corpuscular radiation are determining
factors on the A"unar surface, ~be contribution to the total dose from natural
And induced raWation is no more than several percent. However, doses
Irom galacUc sp-ice radiation and corpuscular radiation on the lunar surface
are two times less than in space, due to shie b the Moon itself.
6_3167
fa. ~A. No. 2z; ATD Report, 6
suB coms o6, 18, 22 / SUB14 DATE& OOM&y66

ACC NRa AP6011361
SOURCE CODE; UR/0206/66/006/002/0336/0342
AMIOR: Kuznetsov, V. G. (Pam
ORG: none
TITLE: Algorithms for finding general solutions to systems of linear Inequalities
SOURCE; Zhurnal vychislitellnoy matematiki I matematicheskoy fiziki, v, 6, no. 2,
1966, 336-342
TOPIC TAGS: algebraic equation, linear equation, linear inequality
A13STRACT: Ai are proposed for solving in a finite number of steps various
systems of linear inequalities with real coefficients. Each successive algorithm es-
sentially reduces to the first, which is an algorithm for a homogeneous system of
rank n. The second is for a system of rank r