SCIENTIFIC ABSTRACT KHARITONOV, A.T. - KHARITONOV, S.F.
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CIA-RDP86-00513R000721820001-0
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S
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100
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December 31, 1967
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SCIENTIFIC ABSTRACT
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S11381621000101110061008
/0, ~ /075 A051/A126
AUTHOR: Kharitonov, A.T.
TTITLE: Maximum compression deformation of rubber-metal elements
PERI06ICAL: Kauchuk i rezina no. 11, 1962, 24 - ZT.
TM: The author discusses the derivation of quantitative relations of
maximum deformationibr three types of elements tFig. 1): a) a cylinder with
free ends; b) a cylinder with fixed ends; c) an element with "recesses". He
derives equations for the calculation of various parameters. It is concluded
that maximum deformations of compression in elements with "recesses" are higher
than those of right-angled ones. This is the advantage of the elements de-
scribed. There are 5 figures.
ASSOCIATION: Bryanskiy institut transportnogo mashinostroyeniya(Bryanak Insti-
tute of Transport Machine-Bulding)
Q9_1nnft1A_
,T~ ~To,-.A.T.; KRASNOVA, N.A.; VINITSKIY, L.Ye.
Effect of the shape of the side 8urface of rubber-dnd-metal
elements on the force characteristics of the compression.
Kauch. i rez. 22 no.10:38-42 0 163. (MIRA 16:11)
1. Bryanskiy institut, transportnogo rwishinostroyeniya i Vsesoyuznyy
nauchno-insledovateliskiy Institut zheleznodorozhnogo transporta.
A.V.
Inspection carried out by voluntary inspectors. Izm. tekh.
no.9:56 S 164. (MIRA 18:3)
SOV/46_5_~,1_9/34
AUTHORS: Merkulov, L.G. and
TITLE: Theory and Calculation of Composite Concentrators
(Teoriya I raschet sostavnylih kontsentratorov)
PERIODICAL: Akusticheskiy zhurnal, 1959, Vol 5, Nr 2, pp 183-190
(USSR)
ABSTRACT: In an earlier paper (Ref.1) Merkulov discussed simple
ultrasonic concentrators in the form of conical, exponential
and catenoidal horns. Composite concentrators, formed by
joining the rods of constant and variable cross-sections
(Fig.1), are also of interest. Some work has already been
published on composite concentrators (Refs.2,3), but the
lack of a technique of calculation of properties of such
concentrators has impeded their practical application. The
authors remedy this by deriving general expressions for the
condition of resonance, the amplification factor and the
input impedance of composite concentrators. Some cases of
practical importance, shown in Figs.2-9, are dealt with in
detail, and the best forms of concentrators are determined.
The input Impedance characteristics of various concentrators
L;ard 1/3 near the rasonance frequency are sLown in Fig-11. To
Theory and Calculation of Composite Concentrators
6OV/46 -5-2 -9/ 34
verify the theoretical results the authors tested several
concentrators made from steel St.40. The testing technique
was essentially the same as that doscribed in Ref.1, but
6ortain Improvements to it made it possible to measure the
resonance frequency within 0.1% and the amplification
factor to 5-10%. A table on p 189 shows the results
obtained on testing a conical horn with a cylindrical rod,
and an exponential horn, also with a cylindrical rod. 'The
empirical values of the amplification factor ~col.9)
agree with the theoretical values (col.7) within the
experimental error. The empirical resonance frequencies
(col.8) are somewhat lower than the theoretical values
(001.6). A"stepped" concentrator (shown in Fig.8) was
also tested experimentally and the results are shown in Fig.12.
The experimental values of the amplification factor agree
viell with the theoretical values, but the agreement between
the empirical and theoretical resonance curves is somewhat
Doorer (probably because of bending vibrationsi. The
authors studied also three-piece concentratcrs; good agreement
Card 2/3 between the calculated and experimental values of the
SOV/46-5-2-9/.34
Theory and Calculation of Composite Concentrators
amplification factor was obtained, while the empirical
resonance frequency was found to be somewhat lower than
the theoretical value and it depended strongly on the form
of the intermediate piece which joined the two outer parts
of the concentrator ke.g. Fig.9). There are 12 figures,
1 table and 4 references, of which 2 are Soviet, 1 Bnj~lish
and 1 translation of Sngllsh into R=qian~
ASSOCIATION: Leningradakiy elektrotekhnichoskiy institut im. V.I.
Ullyanova (Lenina) (Leningrad Electro-Technical Institute
imeni V.I. Ullyanov (Lenin))
SUBMITTED: April-18, 1956
Card 3/3
;eU241
-55-)
9, 9-00 0 (-a,,(t 106 3) i'l
S/04 61/007/001/012/015
B104YB204
AUTHOR: Kharitonov, A. V.
,.TITLE: A device for measuring the internal friction of solids in the
frequency range of 20 to 400 kc
PERIODICAL: Akustiaheskiy zhurnal, V. 7, no. 1, 1961, 104-lo6
TEXT: The device described was developed at the Laboratorv of Mectroacous-
+ir-- t,-r fl- T-.titiitp mentioned under Association. It is destined for meas-
uring the internal friction and the propagation rates of elastic waves in
solids, Within the frequency range studied, many materials, especially
single crystals, have very low attenuation decrements and the difficulty of
investigating such substances is due to the scattering of the vibration enex-
gy of the test specimen in the structural parts of the apparatus, and to its
radiation into the surrounding medium. By suitable selection of the means
of fastening the test specimen, by suitable excitation and recording methods,
and by placing the test specimen in a container with iarefied air '6 the resid-
ual attenuation decrement of the apparatus could be reduced to 10- . The
block diagram of the entire apparatus is shown in Fig. 1. Test specimen I
is a full cylinder accurately fastened by a wiretriangle. The excitation of
Card 1/3
20241
A device for
S/046/61/007/001/012/015
B104/B204
an odd harmonic longitudinal vibration is effected with the help of a plate
condenser. One of the plates forms the end of the test specimens, whilst
the other plate is the electrode-.2, which is connected to a sound generator
3- In the case of non-metallic test specimens, a silver plate is fastened
to one of the ends. By means of a micrometer screw, the air gap between the
electrodes may be varied between 0-05 and 0.1 mm. The frequency of the
generator was measured by means of a heterodyne frequency meter. In the in
vestigation of non-ferromagnetic test specimens, the recording of vibrations~i
was carried out electrodynamically. In ferromagnetic materials, a ring
made from bariumtitanate was used, which served as receiver of the permanent
radial oscillations. The sensitivity of this method was somewhat lower than
that of the first. The electric signal was amplified by means of a super-
heterodyne 7, and the amplified signal was conveyed to a voltmeter 8 and an
oscilloscopq 9. The entire system was placed into a vacuum chamber
(10- 2 to 10-3 mm. Hg). The measurements were made by two methods. In the
case of internal frictions with q-1> 10-4, the 0-7-width of the resonance
curve was determined. With Q_ 1< 10-4, the attenuation of the fi:',--e*1Vibra-
tions of the test specimen was measured. When awitch.ing off the generator
Card 2/3
~02hl
3/046/61/0077001/012/015
jA device for B104/B2U4
voltage, the decrease of the amplitudes could be observed on the screen. By~
means of this apparatus' the internal friction of aluminum, magnesium, and
',copper was investigated! A certain frequency dependence of internal fric-
ftion, and the least internal friction were mgasured with p6lycrystalline
aluminum of high purity (99 - 990/~) Q-1 10- . There are 3.figures and
4 Soviet-bloc references.
ASSOCIATIOIT: Leningradski- elektrotekhnicheskiy institut im. V. I.
Ul'Zranova (Lefiina) (Lenin&rad Institute of Electrical
Engineering imeni V. I. Ullyanov (Lenin))
SUBMI-TTED: February 23, 1960
Fig.
P7
Card 3/3
no
AUTHORi
TITLE:
PERIODICAL:
1) ~' . 1:. 1) 1.
S/64_6~61/CO7/003/004/004
B104/B201
Kharitonov, A. V.
Ultrasonic torsion concentrators
Akusticheskiy zhurnal, v- 7, no- 3, 1961, 387 - 389
TEXT: It is noted by way of an introduction that interest for conoent.-~Aors
using torsional vibrations has Grovin in racentyears in connectlon -with the
devolopment of trasonic violding tachninues. PAs is oho= in the present
paper, results of an analynis on concentrators operating with longitudinal
vibrations can be used for their calculation. The torsion concentrator is
a3siraed to be a solid rod or a hollow rod with a variable cross section
lonethwiso (coo attached figure), its maximum diameter being considerably
smaller t1uni the wavelength. In this case, the cross sections of the vibrat-
ing rod romain perpendicular to the longitudinal axis of the rod. Under
these premises, the problem can be solved in one-dimonoional approximations
Idz;~..2 2
'Q/~t -lea- dz;.Gl - G(z,t) is the torsionj I I(Z) is the
z
polar moment of inertia, M - M(Z't) is the torque, and 2 is the density of
Card 1/4
~w', 3 ) ",
SIO 4 6J61100 7/0 0 3/00 4/0 0 4
Ultra--onic torsion B104/B201
the rod material. Herefromf one obtains the differential equation
2 2 2
d G,/dz + d-T dP + kig - OP whore kt =,A;/cl; and a is the velocity of.
= dz t
transversal waves in the rod. A comparison with the differential equation
d 2 2 dIr' du 2
u/dz + = + kja 0 for the longitudinal displacement in a rod
Sdz z
of variable thickness shows the agroement of all calculative expressions
obtained from the two differential equations. FInally, the author examings
the form of a rod in which the torsional waves (or longitudinal waves) propag.-
ata at2a velocity that is indopendent of
A d I I dT. 2
~n - const holds for a rod of this kind* One then
-'I d-2 4i2 z
obtains for the rod shape:
Card 2/4
re
26398
9/046/61/007/003/004/004
Ultrasonic toraion as* B104/B201
2
-.0
1((Cz+D)
2 2
I(Z) (Ce!" + Do- z) > 0
2 2
(Ccosbz + Dsinbz) ;J3 < :. 01' IS jb.
The first case is charac~e'rized by the absence of a diapersi6n; t6 second
case ddnplays a negative diaparsion, and the third ca6e.a positive dispersior.
of tho wave velocities. There are 1 figure and 6 Soviet references.
ASSOCIATION: Leningradakiy elektrotekhnicheskiy inatitut im. V. If,
Ullyanova, (Lenina) (Leningrad-Institute of Electrical
Engineering imeni V. I. Ullyanov (Lenin))
SUBMITTEDi March 27, 1961
Card 3/ 4
:31
3/046/63/009/ool/014/026
B100186
A UT 1101? Kharitonov A V-
TIT LE s The dep(ndence of internal friction in metals on the amplitudes
of vibration
PEI'%IC~DICAIJ: Akusticheskiy zhurnal, v. 9, no. 1, 1965, 60 - 87
T;:,,,,T :f.,. Gi-anato. and K. LUcke (J. Appl. 11hys., 1956, 27, 6. 583 593;
7, 769 - 605) developed o dislocation theory of intornal friction based on
the dl.;IocaLion modul of J. S. Koehler (Imporfactiona in nearly perfect
cr,istalo. N. Y-9 1952, 1). 197)- Here this thoory 'n completed by a cal-
of the dep~,ndence of logarithmic decrement of damping, on the am-
plitudr.:3 of vibrition. The following arisumptions are mudoz (1) in the
Polycry.-tallille nample a act of slip sy3teff,3 is oriented ohaotioallyj
(2) dislocations are distributed uniformly betwoon all slip systems. The
logarithmic devremenL of damping (6(a) - A(Eu), whQro u is the deformation
ai;iplitude) ia represented in the form
Card 1/5
Do(-, depui.6c.-nce of internal friction ...
CO Ito
A (U) C (U) U',
2) Y,
M-0
P2
(m + 3) D~ A- mDn_l B,
C- Zrn I
B,
0 0 a
,-/04,A3/0Qq/,OU1/014/026
B100166
I Co +1
- ---1
18 C,
1,33 C,
1,47 G, 40,00its
1,60 C, -0,00012
./2
D, sin3(p (sin ip - 1)"dp.
0
In a comparison between this result and experimental data it. is shown that
the theory of Granato and LUcke doea not give a real dependence of the
decrement of damping on the amplitudes. Granato and LUcke assumed a random
distribution of the point defects along the diGlocations. Here it is shown
that elastic interactions between the point defects force them to spread
alon- the dislocations so th3t lattice distortions produced by dislocations
are reduced to a minimum. There are 4 figures.
ASSOCIATIONs Leningradakiy k;lektrotekhnicheakiy institut im. V. 1.
Ullyanova (Lenina) (Leningrad Electrotechnical Institute'
Card 2/3 imeni V..I. Ullyanov (Lenin))
KHARITONOV, A.V.
Training metr-logtfits for the factories of Central Chernozem Economio
Region. Izmstekh. no.608 Jo 164. (MIRA 17:12)
KHARITONOV, A.T.
-
ObserVations of minor planets at the Institute of Astrophysics of
the Academy of Sciences of the Kazakh S,S.R. Astron.tair.no.172:4-
5 Ag 156. (MLRA 10:1)
t -
(Plapets, Minor)
MOROZ, V.I.; KHAJRITONOV, A.Y.
Photoelectric photometry of areas on Mara' surface. Astron.tair
no.174%4-6 N 156, (MLRA 10:31
1e Astrofimicheskiy institut AN KazSSR.
(Mare (Planet))
) A. V .
KHARITMOV A,
,:.
Spec t rophot ometr Ic tempernture of two peculirir stqrs near Orion
nebula [with summary in English]. Izv.Aatrofiz.inst. AN Kazakh.SSR
5 no-7:17-20 '57. (MRA 10:7)
(Stars--Tecrperature)
KHILRITONOV, k.y.
Photoelectric observations of AB Aurigae. Per.zvozdy 12
no.2:148-149 N '57. (MIRK 13:4)
1. Astrofizicheakiy institut AW SSSR, ~Klma-Ata.
(Stars, Variable)
MOROZ, V. I,; MARITON
Pbotoolectric photometry of regiona on Rare' surface [with summr7
in Hnglish]. Astron, shur, 34 no,6:903-920 N-D 157, (MIRA 1W)
1. Antrofisicheekiy institut AN XhzM
(Yare (Planet))
BOYKO. P-N-; KHARITONOV. A.T.
Polarization observations of Arend-Roland's comet. A9tron. tair.
no.181:6-8 Je 157. (MIRA 13:3)
l.Astrofizicheskiy inatitut AN XazSSR.
(Comet'3-1956)
AUTHORa Ro,~,.hi:ovaUy, ).A., Matyagin, V.3). and
33-35-3-17/27
Kharlton~;V
TITLEs The Experiences of the Photographic Observations of the
Artificial Satellites With the Aid of the Yeninciis Tniosco,.-c
of Mahautov (Opyt fotograficheakikh nablyudeni~ iskussi,~,,rcrry"'-
sputnikov zemli pri pomoshchi meniskovogo telesl:opa
PERIODICA4 The observatory of t.ho A.,itrophysical Institute of the Academy
of Sciences of th( Kazal~h SSR-InAlma Ata tested and developed
different methods for the photographic observation of arti-
ficial satellites. In particular an improvemont of the ob-
servations with a meniscus telescope of Makautov (D - 50 Cm
F = 120 am) was aimed at. The observations of the second nput-
nik proved that the application of this telescope to the pur-
poses mentioned above is also possible under unfavorable con-
ditions. For the synchronization of the moments of motion of
the sputnik with the cV.onometer an oscillating plane-parallel
glass plate (12)(12 cm , thickness 8 mm) was used which was
plit before the correcting lense of the telescope. (A similar
nuaratus was already applied by R. TrUmpler [ief 31 ). The
exactness of the measurements amounted to + 21, for the de-
Card 1/2 termination of the ~:ocrdinates and + 0,001 see for the time.
PERIODICAL41. Astr)n zhM. 35, no. 3, P. 479-85 1-58
The BY-perien,,,es of the Photographic Observations of 33-35-3-17/27
the Artificial Satellites With the Aid of ths Meniscus Telescope of
I.ak.,3utolt
The calculations were carried out by L.N. Tulenkova accor,]--*Tlg
to th~'j mothcd of Deych L-Rof 51. From January 22 to February 411
6 photoGraphs of the accond sputnii Niere taken.- . The
"iiors think that the riethod would be essentially improv-~:C-,,
if the correcting lence, not the plate, Vere made to oscillatc.
There are 3 figuresv 1 table, and 5 references, 4 of which
are Soviet, and 1 German.
A,'~:;6CIA-;.'ION! AstrofizLr;heskly institut Akademii nauk Kaz SSR (Astro-
physical. Institute of the Academy of Sciences of the Kaz SSR)
SUBLTITTEDt March 21, 1958
Card 212
7, r
U T 71, -1 , 11. -11 1, 1. '--, 17, 1. i t G n ovC j f,C
TI M To .. ... ".0-r-11 3-pl!-
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or, Uioir i-v;, f t!
ol,:7erva!.,orY o~
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f
2ail, ra above
:7,ea 12 ic from -~_lma-_~,.ta. --2he scicntific worl:
-3 4
0 F 4 C~S tU t 0 is, ca-rr;cd oii" un' r the i r,:, 4 C,,~j
_'_cade-ici.-in V.G. _-TeF~enkov. carri,-r of
U-
s-inutelik- ,-,-ar, o' so,nrc,l 4-" _ od,,)
u__ U,
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of of t,:1,~
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m , cwts. In tho colir :;~ of eacl~, 1-11f f;;-Cmm~l tile
plal;c, L7, in one of t:)e oute-- t"-2
r
of mcj%in-
the r mi,nik dr "M Unl'Iterrunted,
rack on tho pi,-~'urc. v,-h)(--n t'ic plate
traui.-4fers, fro!:~the one out.-c- Lo Lh2 0~'Iler,
tracl: of Vie .~,putnik
of t'if~ slu-ars, art3 t~ Ie
fli,--hu tlirw-1-11 Ole 0~- t7l~')
~j - 1; C- 'e,
1c LIVO ?0,.:,
tho i~rac,!r i.-, (-,~Aaj-n!-,,J as an
Thc:,,, are ,,--n in Ulic no~~atuivo t;'.o
of 1,1[w cor!~--,-,pondin~ to L-1-lem can ea-2.1.-- be by
-in to an -"'hiS
_-;S T,:]o!-"i1fic--,,ti(--Jn c~f To
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',,atch t-11it: J
o1AAn a mare r.rcci,so re-istr,,,itio?l of tll-
t-r-an.,
~,ec
)o by f!rl
W' sv., n.- -,:CIO%,'
I) 1--e i-, L ',; t- ed L 'liecifl- 41
-of the C;,:-; in'f
up 1,e 0.0005 de--ree:,. Bly me!,um,, 01, tll,'
authon~ obUaincd about 10 "hotc,-ra- of
~jjmtnik 11, 6 of 'jj-,,ulu-nik III =1(1 1:"Orc! than 110n no
rocket-carrier of Sputnik III. Th;_-re are
-C"'I I TIOTT: institut Aka-lemii nau!!:
S S) R(,'.strop'llysical InsLitute of t'ie S
lard 4/4
3.9000
78010,
501~ 9/31
AUTHORS: Dzhasybekova, E. K., KaZachevokly, V. M., Kharitonov, A. V.
TITLE: A Determination of the Albedo of' the Earth.
PERIODICAL: Astronomicheskiy zhurnal, Vol 37, Nr 1, PP 131-134
(USSR)
ABSTRACT: This work was undertalwn upon the recommendation of
Academician V. G. Fesenkov. The earth-shine of the
moon was observed between September 29, 1957 and
August 21, 1958. The problem consists In comparing
the brightness of the portion of' the moon's surface
illuminated by the sun with the earth-shine. Taking
into account the "phase" of the earth for an observer
on the moon, one can compute the average spherical
albedo of the earth. The theory and the method of ob-
servation were described in 1955 by the second of the
three authors. The instrw-nent consists essentially of
two objectives, which bring into the field of an eye-
piece both the sunlit and the earth-shine portions of'
Card 1/3 the inoon; a cat's-eye diaphragrn in front of' 'Uhe first
A De termina t loll of- the Albedo ~8w' 9
of the Earth S C, V/3 3 - 13,Y - I - 19/3 1
lens equalizes visually the brightness of thr-. two
images. The mean wave length of' the visual mocn
light is found to be equal to 5,640 A, and the
polarization of the moon's light about 10%. The
ratio of the light intensity reduced by the diaphragm
during the observations to that of the fuil opening
is 0.0057. A table gives the observed values of the
earth's albedo for 17 observations 'together with the
geographical coordinates of' the moon for each date.
The average value'of the earth's albedo is equal to
0.391 + 0.014. Previous values found by various
observers between 1914 and 1953 vary from 0.29
(A. Danjon) to 0.56 (F. Very). Whether there are any
variations with the seasons or with the 11-year period
of solar activity remains imdecided. The authors
thank Z. V. Karyagina for help in observing and com-
puting. There is I figure; 3 tables; and 12 refer-
ences, 8 Soviet, 2 French and 2 U.S. The U.S. ref-
Card 2/3 erences are: H. Russel., Astrophys. j., h3, (1916);
A Determination of' the Albedo
J
of the Earth
0 ~7
ASSOCIATION-
SUBMITTEDg
F. Very, Astrophys, Obs
_, Nr I
Astrophysical Institute of the Azademy of' Scletices
of Kazakh SSR (Astrof'izichesi~iy Ins-IT-.ut, AN KrazSSF-L)
June 1, 1959
Card 3/3
.. K11RITOROV, A.V.
-11 --- - . i,--11-11. 4-. -
Blootrophotometric observation of the variable AD Aurigae.
Izv,Astrofiz.inst.AN Kazakh,BSR 9S29-31 160,
(KIRA 13:5)
(Stars, Variable)
lQu,llITOli-Ov,-Aa--
Determining the night coefficient of transpurancy. Izv.
Astrofiz.inut.All Kazakh.SSR 9:53-55 l6o. (KIM 13:5)
(Atmoapheric tranaparency)
808
S/026/60%OO/04/036/070
(3 -S -C) D048/DO06
AUTHORS: Kazachevskiy, V-M.; Kharitonov, A.V. (Alma-Ata)
11=000".777Z777.
TITLE: The Earth's Reflectivity
PERIODICAL: Priroda', 1960, Nr 4, pp 95-96 (USSR)
ABSTRACT. This is an account of the reflectivity of the Eart
and other planets in relation to the spherl al albedo.
The albedo of some parts of the surface ofliars was
determined from photoelectric observations male- by
V.I. Moroz and-A.V. Kharitonov in 1956. Academician
V.G.-Ye's-ZeEkov, 01 tne As~rophysical Institute of the
A13 YazSSR, proposed that the spherical albedo of tHe
______Ta_rEh sbnuld he redetermined in connection with IGY.
Among those who took part in this work were E.K.
Dzhaszbekova Z.V. Karyagina, VJ1. Kazachevski7 and
Miaritonov. ]Xhe reflections from the positive
eage of tne kioon\~nd dust light went through two dif-
Card 1/3 ferent optical c annels whereby the rays from the
808Xi
S102( 000/04/036/070
D048/DO06
The Earth's Reflectivity
positive edge were greatly weakened by the reflection
from the two unsilvered glass surfaces, the prism
and the plate. The reflections then reached the
ocular along with the unweakened rays from the dust
light in such a way that the observer at 'the same
time could see the crescent of the Moon and the outer
side of the dust light pertaining to the Moon's outer
edge. With the aid of extensible "cat's eye" dia-
phragm fixed in the optical channel for crescent
rays, the observer was able to regulate the visible
brightness of the crescent and that of the dust light.
From observations carried out over a period of nearly
two years (1957-58), the mean alb-ido value of 0.39
Card 2/3 was obtained.,
21200
S/503/61/01.L/000/001/003
E. o32/ E3 14
0 6 1., 116 e,,V L
AUTHOR: Kharitonov. -A.K.
TITLE: A Photo-electric Stellar Spectrophotometer for
a 50 cm Reflector
PERIODICAL: Alcademiya nauk Kazakhskoy SSR. Astrofizicheskiv
institut. Izvestiya. v. 11. Alma-Ata, 1961p
pp. 54 - 63
TEXT: The spectrophotometer was designed for investigations
of the continuous spectra of stars and is mounted on the 50 cm
reflector of the Astrofizicheskiy institut AN KazSSR
(Astrophysics Institute of the AS KazSSR). The mechanical
design and assembly was carried out at the workshops of the
Institute by M.S. Semenov with the assistance of F.T. Lyuts.
First recordings were obtained in May, 1959, and since then
various modifications have been introduced.' The optical
arrangement of the device is illustrated schematically in
Fig. 1, in which A is the section in the plane of the
declination circle and 6 is the section through the
Card 1/6
V/I\
21200
S/503/61/011/000/001/003
A Photo-electric .... E032/E314
perpendicular plane. The main mirror of the Cassegrain
reflector is 50 cm in diameter and the auxiliary one is
14 cm in diameter. The equivalent focal length is 12 m
and the image of the star is formed at the point marked 3 -
The exit slit is mounted in this position and the plane
containing the slit makes an angle of 67.50 with the optical
axis of the telescope, the slit itself lying in the plane
of the declination circle. The apparatus also includes an
eyepiece attachment 4 . The plane mirror 5 is introduced
in order to reduce the dimensions of the monochromator in the
direction of the axis of the telescope. This mirror reflects
the light through 900 to the telescope axis onto a spherical
collimating mirror 6 (focal. lonsth 50 cm). The parnIlel
beam produced by this mirror is directed onto the diffraction
grating 7, and,finally,the spectrum is focused by the
mirror 8 onto the exit slit 9 . The mirrors 6 and 8
are used in the off-axis position, which gives rise to
astigmatism but this is said to be unimportant in the study
Card 2/6
21200
S/503/61/011/000/001/003
A Photo-electric .... E032/E314
The plane parallel thin glass plate 13 reflects about
8-locio' of the light incident upon it onto the photomultiplier
and a record is made of t-'-,e ratio of the signals from
9.1 and ZN/ . This can be used to compensate for random
YI Sr 11
changes in the image of the star on the slit. All the
absolute measurements are carried out with a wide entrance
slit (3 - 4 mm), in which case the monochromator, in fact,
becomes a slitless one so that the latter effect is not of
great importance. Fluctuations associated with stellar
flicker are reduced by using a large time constant (0.4 -
0.6 see). The rate of scanning normally employed is
8-3 X/sec. The amplifier is of the form described by
Kuprevich in Ref. 14. The results obtained with this instru-
ment are summarised as follows. Continuous spectra between
3600 and 5900 A can be studied when antimony-caesium
photocathodes are e niplo y e d. In this region the
spectrophotometer can be used to observe 6 M stars.
Card 4/6
23200
S/503/61/011/ooo/ool/oo3
A "hoto-clectric .... L'032/r,31/,
(The ',
(VEJ) photomultiRlier was lased with tile fastcst
s
stars ; dark current T x 10 A, sensitivity 0.4 A/,-Il at
300 V usi-,17, special photomultipEel's with a 10117 I,nvc limit'
t 3
_300 A (I'labotilova and ;~ollul'c"110. - Ref. "10, Lhe ran-'-C call
ho n.--tencicd to 6 600 A. lit the ro(I region the -.)on '~.-I;rnt in,-
ot: c rc' tile instrument falls to 3.5 Ti ijt.~,trumcnt
for the determination of equivalent widths cf strong
olntodt lines, o.r,. Balmcr lines .1,11 t;ic spectra of early
L;tars all(! the 1-1 and K lines in type G stars, etc. riz.
--hows the spectrum of aLyr in tLin violet and ultraviolet
rer.-ion. This record was obtained in the third order using
.111 e,-'Jt slit 'o' 0.5 =a and tile Ic-(
(-,~S-6) filter. At the
tirie, the spectrophotomcter is being used to investij;atc
the encr,(-y distribution in t1he 's-)cctrum of a number of bright
stars in absolute Ninits. There are 4 figures and 211
references: 14 Soviet and 10 noli-Soviet.
The following Soviet personalities are also mentioned:
P. 1". Dobronravin, V. B. Nikonov ;%nd V. 1. Moroz.
Cnrd 5/6
A Plioto-clectric ....
Fig. 1:
Card 6/6
- T-I
21200
3/505/61/011/000/001/co,
C052/E314
ri-
Rl
EILIRITONOV, A~V,
Methods and sow resulto of studying -the energy distriimtion
in Aellar spectra in absolute unite. Izv,Ajtrofiz.inL;t.AN
Kaz6kh,SSR 12:27-36 161. (MIPU't 14:12)
(Stars-Spectra)
~ 2 31 31 2
S/033/61/038/001/015/019
916 E032/E5111
AUTHOR: Kharitonov, A.V.
TITLE: A Study of the Temp6`rature Dependence of the
Luminescence of a Phosphor Excited by P-Radiation
PERIODICAL: Astronomicheskiy zhurnal, 1961, Vol-38, No.1, pp.164-
166
TEXT: The apparatus employed in the present work is
illustrated schematically in Fig.l. Type UC-5 (BS-5) phosphor,
incorporating Sr90 as the ratioactive exciting agent, was employed.
The phosphor 1 was located inside an aluminium double-walled
container which was kept at the required temperature by passing
water through the gap between tne walls,or by filling it with a
mixture of salt and snow. One end of the container was covered
with a glass plate 2. The phosphor was "viewed" through this
glass window by the photomultiplier located inside the container 5.
Standard phosphors were attached to the moveable rod 6 so that
they could be presented to the photomultiplier when required. The
signal from the photomultiplier was amplified using an amplifier
described by V. 1. Moroz in Ref-3 and was recorded with the aid of
Card 1/4
89332
S/033/61/038/ooi/015/019
E032/E5i4
A Study of the Temperature Dependence of the Luminescence of a
Phosphor Excited by P-Radiation
the )MI- 09 (EPP-09) potentiometer. Fig.2 shows the dependence
of the luminescence of the phosphor BS-5 as a function of the
temperature in the range -8 to +48*C. The luminescence decrenses
almost linearly, the decrease being 0.60 per deg. The use of
various filters showed that the blue and red regions of the spec-
trum are the most sensitive to temperature changes. while the green
region (4900-5800 A) remains practically unaffected. Thus, on
heating from 8 to 440C the intensity in the region 4200 to 4900 A
decreases by 37%, while in the region 4900 to 5800 A the decrease
was 4%. The corresponding figures for the regions 5700 to
6100 A and above 6000 A were 20% and 22%, respectively. Thus, the
temperature changes affect not only the intensity of the
luminescence emitted by this phosphor but also the energy distri-
bution in its spectrum. The apparatus was also used to investi-
gate the a-particle excited luminescence in the a-CA-IJA (SPD)
(type 3(Z)) phosphor. The reduction in luminescence in the latter
case was found to be lower (0.17% per deg.). The above phosphors
Card 2/4
89332
S/033/61/038/001/015/019
E032/E514
A Study of the Temperature Dependence of the Luminescence of a
Phosphor Excited by P-Radiation
were prepared in the laboratory of Professor V. L. Levshin at the
FIAN im. P. N. Lebedeva(Physics Institute, AS imeni P. N. Lebedev).
There are 2 figures and 3 Soviet references.
ASSOCIATION% Astrofizicheakiy institut Akademii nauk KazSSR
(Astrophysical Institute, Academy of Sciences
KazSSR)
SUBMITTED: June 14, 1960
Card 3/4
t- el X- U -tr -t-
KHARITONOT, A.V.
Distribution of energy in the spectra of C- Lyrae, -( Aqullae and
Ophiuchi given in absolute units. Astron.tsir. no.222%20-23
mq 161. (KUU 15W
1. Astrofizicheskiy institut AN KazSM.
(Stars, Variable-Spectra)
KMRITONOV, A.V.
Energy distrib-ition in the spectrum of Lyrae In abeolute
units. Izv.Astrofix.inst.AU Ka-lrb.SSR 15t52-62 162.
(MBU 16:1)
(Stars, Variable--Speutt~a)
GLAGOLEVSKIYI Yu.V.; KHARITONOV, A.V.
Operation, analysis, and some improvements in the design of a photo-
electric.spectrophotometer. Vest.AN Kazakh.SSR 19 no.lOt67-75 0 163.
(MIRA 17%1)
A ~ Tiic~ a I -Khari-tonov, ;,.Y.
TITLEs Concerning the nocturna.
parency in the
'r ft
stitut ut me A~5 Kazakh GS-
SOURM Akademiya nauk Kazakhakoy SSR. Astrofiziches-
kiy in-stitut. Trudy. ,r. 5. 1962. Rasseyaniye
i polar4zatsiya S-"Pta v
material./ 51-ovesnenaniya ~t,
polyarizatsii svet~ v 7
The results given in the pr,~F,?nt Ta-er rel*ate
*o the study of the energy distributior, in s-,ectra
%-qrious stare for the pur;>- ~~e*.*:!47
C al-e 7,~, 7
were coz.d~tFd ~Y tLen .S
t:-. 'r.D ti;elec trio recording
I
--incy coefficient vaa deterrnit.e, --j e.
ar-(I 1,12
~Ma and ZkLyr were observed (as
,'re stars jDri ar;d jAkri (as aaccz-,dinF star-,
over a period of 8 summer-autumn ragritu of were pro c e s s ed.
The wavelength region of 670C to A
f a r.1 67h t a W ee C
~.,j t rfli,spa re nc y dd no t re ma. r.
aue tc '.re remc,;~
n(; wnich star's in the evening, ~n r - Dr:
ir. daytime. 7hc
r,:,~-tts rjf obser,.ration are
(,i'/FCr,(w) LFF T C IJPI,'~-'
a~us..In, V. L. and Yharitonov, A.. V.
Solution of the-stability proble" by iteration
'arnal vjchis]-itellnoy i mat mat chc-slkoy f4zi'-, v. 3,
no. 2, 1963, 361-1164
Ine dixect Rauss-Hurvritz methol for studies of the stz~hillt:, of dif-
U U
r~:-,t4 a' e,: ations and systairs of such equal tions is sometLraes ex-,rerzaly sens-i ve
errom. The authors prezent -,n c S- 3
Pa-
-Y
Y C
er 7, a'- Dd3 for -,`e
nd
Rep
_7,
w~s
7 L. 3
ca-c'--
7.-.e n,.-%'Der of iteratJ-o:-Ls -,Des :-~,:t, 3-1 tne ,cin. om-
e order of the matrix, but iz detc=inad by the locatior. of t1ne roots
~axd 1/2
L 12741-63
a st ability ...
o4 the initial polynomial, in particulaar of those close ,,) the f zcis. Af-
a gnaz-y
tIr C--7ae -445cussions of the case of pl=e =-aziaary rco-,,s, t:~e-
-,-,h-~n the me-thod fai'ls to -=cduce a
cf -,he polynom,-Inl 'o:-
for, - 4 -
na~.:~enad --'-..e in-
--he authors thank S. A. Avramenko and ot-er ma=-oars conductinE-, the
seaLnar for the evaluation of 'the paper and useful re.Tarks.
5, 19'
b2
Caxd 2/2
KHARITONOV, A.V.
Extra-galactic spectrophotometric standards; energy distribution
in the spectra of selected stare in CGS units. Astron.zhur. 40
no.2039-350 Mr-Ap 163. (MRA 16:3)
1. Institut astrofiziki AN KazSSR.
(Stars--Spectra)
KARYAGINAp Z.V.; HARITONOV, A.V,
Determining the stallar jdagnitude of the sun in three-color
systems on the basis of"absoluto spectrophotomotric observationa.
AstroNzhur* . 40 no.6tll23-1125 N-D 163. (MIRA 16:11)
1. Astrofizichaskiy Institut AN Kaz3SR.
KARTAGINA, Z.V.; KHARITONOV, A#V#
Use of standards in spectrophotometric observations. Energy
distribution in the spectrum of Persei in the region
3200-30300 1 in abooluto units. Izv. AN Kazakh. SSR. Ser. fiz.-unt.
nauk no.1:32-42 163. (MIRA 17:4)
MTA-'~TIONOV, A.7.
f;eteradring the Bpectral abDGrption faotrx for h spharical concave
rdrror. Izv. AN Kazakh. SIxR. -",er. fiz,mat.nauk na.1:713-82 163.
(MRA 17W
KWITONOVj A,V.
Night spectral transparency in the region aV the Aitrophysic&l
Institute of the-Academy of Soiencea of-the Kazakh Z.S.R, Trudy
Aatrofiz.inst.AN Kazakh.SSR 3:183-187 162. (MIRA 16:11
KARYACNILP %V.~ Ydlikf(IIONOV~ A.V.
Fnergy distribation In the epce.,tra or 17 st,-,rs erprcsr,~-3 I-r,
ab3olute anorgy uni". lav. AN Kaznxh. SS.R. Sar. fit.-mat.
nauk no.3310-27 S-D 164. (MIFA -17,12)
KHARITONOV, AoVo
Energy distrihitioi in the spectra of four stars expressed
in absolute energy units. Izv. AN Kazakh. SSR. Ser. fiz.-
mat. nauk noJR28-32 S-D 164. (~UIRA 17;12)
WYAGINA, Z.V.1 KHARITONOV A.V.
Study on the UBV photometric system# Astron,zhure 4.2 no*21377-385
Mr-Ap 165. (HIRA l8s4)
1. Institut astrofiziki AN KaZSSR.
ACC NRs AT60328iIt,
SOURCE CODE':-PO/0000/6-6/000/~0001002110028
AUTHOA:' KhaFitonov, A. V. (Leningrad)
ORG': Leninjr~d Electrotechnical Institute im. V. 1. Ullyanov (Lenini, (Lenin-
gradskly elektr6tekhnicheskiy Institut)
TITLE: Dislocation theory of amplitude-dependent internal friction in crystalline
media
SOURCE: Conf~rence on Acoustics of Solid Media. Warsaw, 1964. Proceedings.
Warsaw, PWN.1 19660 21-28
TOPIC TAGS: polycrystal, crystal lattice dislocation, crystal vibration, single
crystal, aluminum crystal, copper crystal, dislocation theory, internal friction
ABSTRACT: A inew dislocation theory on the dependence of internal friction in
crystalline media on amplitude has been developed on the basis of the Kochler
model. The theory examines not only the longitudinal exponential distribution of
dislocation segments, bui also the case of an arbitrary distribution. It is shown
that in such conditions only one pair of adjacent dislocations can logically be con-
'sidered to participate' In each separation. Since there are relatively few separated
Pkc NR'-AT6'03-28'-I I
points, it is not'very probable that a flow separation would occur in the range of
stresses, examined in this theory. A theoretical analysis of the theory includes cal-
culation of separation probability, of mean energy lost during separation, of energy
loss per unit volume of the crystal during the period of vibrations, and of the
damping constant. The theory to shown to forecast the quadratic dependence of the
damping constant on vibration amplitude. The deduction is confirmed by experi-
mental study of amplitude-dependent interval friction in polycrystal aluminur
copper single crystals, and iodium carbide single crystals. Data obtained from
.earlier resear,64 (A.' V. Kharitonov, Akusticheskiy zhurn., 9, (19~3), 80-87)
are presented to illustrate the agreement of the theory with experimental results.
Orig. art..has: 4.figures and 7 formulas. [Based on author's abstract) JGC]
SUB CODE: 20/STIBM DATE:
14Jun65/ORIG REF: 002/OTH REF: 007/
212
ACCESSION NR: AP3013579 S/00-M,/6-3/000/010/0067/0075
AUTIHORS; Glagolovokiy, Yu. V.; Kharitonov, A. V.
TITLE: Operating experience with, investigation of, and some improvements to
the photoelectric spoctrophotometer
SOURCE: M XazSSR Vestnik,, no. 10, 1963, 67-75
TOPIC TAGS: stellar spectrophotometer, photoelectric spectrophotometer,
photoelectric stellar spoctrophotometer, spectrophotomotor design, star spoctro-
photometer, pfiotoolectric recording 3
ABSTIUCT: Several improvements and changes made, recently on a stellar spectro-
photometer and photoelectric recorder, built by A. V. IMaritonov (Izv.
Astrofizichockogo instituta AN KazSSR, 11, 54, 1961), have been described. The
diffraction lattice rotation of the scannGr has been changed. A new kinematic
nochanism is introduced for ",he lattice rotation, powered by a reversible RD-09
rotor. With the forward advance of the screw rod connected to the motor shaft.,
the anaular rotation rate of the lattice can be mado to vary. By means of this
mechanism'changes in the dispersion, the prosence-of, dj8/dt and cos. inhomogonotio;
are shown to be completoly compensated for (see Pig. I on the Enclosure). Also, the
-Cord 113, - 1. -- -----
ACCESSION NR: AP3013579
electrometric amplifier circuit has been modifiod with the use of a new amplifier
system called "Kaktus.11 The filament current for the first lamp is increased to
improve the amplifier gain without loss of stability. The now circuit contains a
inuiti-alkaline photocatho0a photomultiplier -rEU-38. Decreasing of pho~ozotric
errors connected with guiding at various wavelengths is reported. These errors
9
involve a rraximun of 7.31% at A= 32G0 R to a minimum of 1. 0% at A = 4221 it. The
penetration capability of the instrument is set at stars of magnitude 6F - 6' .2.
The various characteristics of this spectrophotometer are then compared with
those reported by J. E. Geake and W. L. Wilcock (Monthly Notices Roy. Astom. Soc.
116, 5, 561, 1956), W. Lillier (Publ. Astron. Soc. Pacif. 69, 4,11, 511, 1957),
and P. Guerin (Ann. Astro~hyaiquo, 22, 6p 63-1 - 1959). Orig. art. has: 6 figures,
4 formulas, and 2 tables.
ASSOCIATION: none
S7'LJB.',1IT-1-`;'D: 00
DATE ACQ: 2711ov63
ENCL: 01
SUB CODE: OP
NO REF SOV: 009
OTHM: 003
Card 2/3
ACCESSION NR: AP3013579
.69
i
I
ENCLOSURE: 01
Pig. 1. Scanning speed and dispersion changes bn recorder.
b
Card 313
FILATOV, F.I.; KOLPASIINIKOV, A.I.; Prinimali uchastiye: PWAPOI, P.I.;
YEW-ULOVP A.M.; TOLMACHEV, fl.Ya.; rJURITUNOV, A,Ya.
Determination of residual stresses in the brake drums of airplane
wheels. Zav.lab. 28 no.2:223.,221+ 162. 01-URA 15:3)
(Airplane---Brakes) (Strains and stresses)
KHARITONOV, A.Ye., inzhener.
Experience In the production of concrete pipes. Biul.stroi.tekh. 10
no.10:13-15 )4,v 153.
(KLRA 6:8)
(Pipe, Concrete)
i "I, 1"I" rip I"
. .. ~- , ~ k- 0 ~ ~ i ,. ;~ I Ul R . I, T k)l I OV ,D . ii .-
. -,-, : " ~. -- -~- 11,
Rt~fflllllf,lrig tLe an.!Ie -;C f% c~ -; I m.41~3 -
. c. j. , L)~ I . I
n ~ -t- !-I llf-,-f~l
r,
T ru,,.i y 1. F J ro. 24-Cj 1 -2- R) I ~, " I il,!!l'-,'k R.?)
ACC .jR.: Monograph UR/
' V. M., B. A.
a henko. 14. Kh. - Kostin A. K. Mel'nikov G. V. Ri~tr~o Kharitonov,
D
Theory of internal combustion -ngtdW(Teoriya dvigateley vnkitrennogo 9goraniya)
140S cow, Mq!~E-Inosili6yenl~i,-'( 1965. 459 p. illus., biblio. Textbook for
students specializing in Internal combustion engines at inatitutions of higher K-"
learning. Errata Aip inserted. 16,000 coplen printed.
TOPIC TAGS: internal combustion engine, carburization, engine combustion system,
engine performance characteristic, engitte exhaust system
PURPOSE tuND COVERAGE: Ibis book Is published as a textbook for students ip higher
technical educational institutions and can also be used as a handbook for engine-
design engineers wid their tochoical staffs. It gives an analysis of the internal
combustion engLne and Its applications, from agricultural equipmcnt (stationary
and mobille) through automotive and mnrin,! Uqe". A thorouF3111 dc~~crij,tfon of Lutbo-
superchargers and engine power rating is included. Fuel and cooling systems and
their characteristic-9 are also discussed. This book was prepared by tile internal-
facility of Lbe LeningK.L(j P2 ~chnic,31. InstitiiLp !-r;~ 11. 1.
Kalintri. The authoro apj)ear In the followitij; ordor: 11. A. Kharin'tovich, chapters 1_
and IX; G. V. HeVnIkov, chapLers It and VII (E.xcept -3tibliciding 4 and 5 tit chapter
~Ji. D'yachenko, chapters III aad VI (E%cept 4 In chnpter-V1)-...
V.-M. j1evro';' ChnPt'--r0jV al V Except cubhe'adIng I and chvpter v):
I in V11; D. P. P 'gachev,
A. 1.'.. VosLin, chapEers V111, X, and rjublicading 4
subheading 1 and 4 in chapter Vf Yii. IN. T-.,,1kov',- gubhoidlilp, 5 In rhnpter V11.
Card .:.1/3 UDC: 621.43.001(075.8)
IL (if.,
ACC NRi AM6 00 104 8
TABLE OF CONTENTS [abridged):
,Introduction -- 3
Basic notations -- 5
1. Working principle and working cycles of internal combustion engines 7
ll. Ideal and theoretical cycles -- 32
III. Working cycle of the internal combustion engine -- 79
IV. Process of intake, exhausting, and scavenging in two-cycle engines- 134
V. Carburetion process - 191
VI. Fundamentals of the combustion process theory in engines 250
VII. Engine supercharging - 279.
VIII. Heat transfer in engines, and the combustion intensity of the working
cylinder -- 321
IX. Engine performance and characteris tics -- 356
Card 2/3
.. I I I --- 0
ACC NRi
406
X. Automatic coatrol of internal combtLqtion engines
Appendix 455
References 456
SUB OODE: 21/ SUBM DATE: l6jul65/ ORIG REF: 0261
Card 313
KHARITCHOV, B.D.
Toctionics of the Vollsk Khvalynak region of the Volga Valley.
1xv.AN SSSR.Ser.geol.21 no,10:107-109 0 156. (KLRA 10:1)
1. Upravlenive proyektirovanipt soorutheniy i ifteledovaniy stroitell-
stva gicirotakhnichaskikh soorusheniy Hinisterstva alektrostantsiy
SSSR, Xuybyahevokiy filial.
(Volga Vallay-Geology, Structural)
AUr_' MOR t KHARITONMB.D. PA - 3175
_-L~s 2eRFo-mena as Conno,cted YrL+h Proc--.35es of Rliver-Bed
TITLE: I
Formation. (0 avyazi opo1zn:-,.-rykh yavl,~-r_V a protseseami formirovaniye,
rusla. rek, Russian)
PERIODICAL: Doklady Akademii Nauk SSSR, 1957, Vol '!3, lir 3, PP 671,-673
(U.S.S.R.)
ABSTRACT: With respect to conditions of the lanislidi ax-.as in the asutml
Volga district two basic types m!xy be distinguishid along the high
r1ght banks of the river Volgw.
1.) The ur-bank, which is se-parated f rom the bed of the river by the
deposits of the terraces looatea above the manh, ax,0 sometimes
alao'by the marah itself.
2.) The river bed is immediately beside the bank.
With respect to landslides the followIng axaaA can in thiz o"a be
distinguished:
1.i Such as are covered by "aoti-ire" land,!tlides.
2. Such an are covered by landslides which have been stopped, and
3. Such as shw no landslide-.like fornations arb am detectable
only by boring.
The order of "PI'e's" sections an the ri-gor Volga. an3 sandbanks is
also responsible for the order in whict, stctioa% with active
Cari 1/2
PA -- 3 175
Landslide Phenomena as Connected with F~roceages Of RiynZlk,Bffd
Formation.
landsli4es and such where IaMslide,% ha':r,, bein stopped follow onq
another. Gradually, these -P143" an3 ,5anYbuak3 shift farther in t'tA
direction of the flow of the river If the xlver be-] ia fair
straight. .17
Consequently, seOtiOnz maxked by lw-4ilides will &13O
tend in a downstream direction, wheresa :L
,1 th,
Rowever, as soom as upper parta janes- d_,
Will gr"ulllY stop , .41 '.
CcMitiOnB 00nn'30ted with the
formation Of & "PUS" Occur againp landalijes will again set
(2 Illustr&tiom and 3 Slavic Referencei). in.
ASSOCIATICK: Not given
PRESENTED BY: N-U-STRAKHOV, Member of the AcadeaW, on 25.10.1956
SUBMITTED: 1.6.1956
AVAIIABLE: Library of Congress
Carl 212
KHARITONOV, B.D.
Method Of classifying reservoir banks according to their design.
Geog.sbor. no.10:189-192 158. (MIRk 12:1)
(Reservoirs)
3(0) SOV120-123-2-33150
AUTHOR: Kharitonov, B. D.
TITLE: The Origin of Towpaths on River Banks (0 prichine formirovaniya
bechevnikov na beregakh rek)
PERIODICAL: Doklady Akademii nauk SSSR, 1958, Vol 123, Nr 2, PP 350-352
(USSR)
ABSTRACT% One of the characteristic elements of the banks of larger
rivers is the towpath, a small strip of land, which is slightly
inclined towards the river and flooded during high water. The
upper part of the towpath gives way to a one to few dozen meter
.high steep bank; this then breaks to a flatter slope which
eventually merges with the level high ground. Usually the
steep bank is ascribed to the work of erosion kRef 2). From
this it would follow that the towpath itself i. a site of in-
tensive arosionj however, such an assumption contradicts actu-
ality. From an analysis of collected facts, it is seen that the
towpaths are best formed an slopes which have had a long his-
tory of development (Fig 1, A). Such slopes are mostly of bed-
rock. Banks which are of unconsolidated river gravels have only
Card 1/3 rudimentary towpaths or none at all (Fig 1, B). This fact and
The Origin of Towpaths on River Banks SOV/20-123-2-39/faw
others indicate that the formation of the towpath and the
steep slope above is due to the action of breakers, which is
significantly great along large rivers. The poor development
of towpaths along the edge of flood plains and the strong
development on bedrock 18 simply explained; towpathe can only
develop fully where normal bank undercutting is less intensive
than vrave*erasion; otherwise the towpath is dest~,oyed by under-
cutting. Thus an indispensable condition for towpath formation
is a retardation of erosion and such a condition is found only
along banks which are of solid rock, which to be sure, though
resistant to a flowing river, are not resistant to waves. The
best'conditions occur along cliffs or rock-like cliffs, where
the towpaths reach their highest development. Where the bank
is protected,by river accumulations, i.e. sandbanks (Ref 6),
the wave ero7sive force is spent on these bars and the river
banks are not eroded. At place3 where the slope of the bar is
slight, narrow wave-out terraces develop, mostly during fall
storms. There are 2 figures and 6 Soviet references.
ASSOCIATION: Kuybyshevskiy filial Vsesoyuznogo proyektno-izyskatel'skogo i
Card 213 nauchno-issledovatellskogo instituta "Gidroproyekt" im. S. Ya.
I The Origin of Towpaths on River Banks SOV/20-123-2-39/50
Zhuka (KuybyBhev Branch of the All-Union Planning and Pros-
pecting Scientific Research Institute "Gidroproyekt" imeni
S. Ya. Zhuk)
PRESENTED; June 18, 1956, by 1. P. Gerasimov, Academician
USSR
SUBMITTED: June 15, 1958
Card 3/3
PETROV, Ye.G., kand.sql'-skokhoz.nauk; KHARITONOV, B.D., inzh.; VANFYAN,
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(Irrigation)
, -7 T~ i l :' ; I " - 7 , - :. I
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.- - , . -'. , , I - . ,, - -1-1 .1 ': . L - ~ , ~ - ~ .
9. Monthly List of Bussian Accessions, Library of Congress, -1951; Uncl.
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~
- I
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-.-- KH ATRIT OJW,-B~
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KEILRLT01
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. --inzh.,..-
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--- KHARITOMOV,-.B.K., inzh.
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1909-1962)
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I
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KWITONOV, D.
-
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1, Glavnyy Inshener fabriki remonta obuvi# Saratov.
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XHARITONOVV D.-F.,
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