SCIENTIFIC ABSTRACT V.P. DOKUCHAYEV - O.D. DOKUCHAYEVA

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000410720019-7
• Release Decision: RIF
• Original Classification: S
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• Document Creation Date: November 2, 2016
• Document Release Date: June 13, 2000
• Sequence Number: 19
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

06514
SOV/141-58-1-4/14
On the Theory of Motion of Ionospheric Irregularities
follows that Eqs (23) and (24) are acceptable solutions.
The final velocity ratios obtained are given by Eqs (30)and
(31), where k is the ratio of the electron concentration
in the surrounding medium to the electron concentration in
the cylinder ' and G is given by Eq (16). A discussion of
these equations leads to the conclusion that in the region
of the D-layer and the lower part of the E-layer the ionized
gas moves with the velocity of the wind, Drift vel 'ties
'K 1 -4
are lower than the wind velocity by a factor of 10- or 10
In the F-layer the velocity of uniformly ionized masses is
appreciably different from the velocity of the wind. The
difference is approximately 10% of the latter velocity.
The transverse component of the drift velocity falls off
very rapidly. Polarization corrections are also shown to
be very small compared with drift velocities. Acknowledge-

06514
SOV/141-58-1-4/14
On the Theory of Motion of Ionospheric Irregularities
ments are made to Prof. V. L. Ginzburg and B. N. Gershman
for a number of valuable suggestions and interest respect-
ively. There are 15 references, of which 6 are Soviet and
9 are English.
ASSOCIATION: Gorlkovskiy gosudarstvennyy univerBitet (Gorlkiy State
University)
SUBMITTED: October 5, 1957.
Card 6/6

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14(10); 3(5) 1Y PHASE I BOOK EXPLOITATION SOV/2843
Soveshchanlye po ratsionallnym sposobam fundamentostroyeniya na
vechnomerzlykh gruntakh
Trudy... (Transactions of the Conference on Efficient Methods ~of
Building.,Foundations on Permafrost Soils) Moscow, Gosstroyizdat,
1959. 131 P. Errata slip inserted. 1,200 copies printed.
Ed. of Publishing House; N. M. Borshchevskaya; Tech. Ed.t Ye. L.
Temkina. I
PURPOSE: This book is intended for construction ongineers, indus-
trial planners and builders. %
COVERAGE: This book contains reports originally read in Vorkuta in
1958 on experience gained in planning and building foundations
in permafrost regions of the USSR. The reports were prepared
for publication in the NIIOSP (Scientific Research Institute
for the Study of Foundations and Underground Structures). The
tntroduction was Wtitten by Professor V. G. Bulychev. No
references are given.
Card 1/4

Transactions of the Conference (Cont.) sov/2843
TABLE OF CONTENTS:
Foreword 3
Kiselev, M. F. Basic Principles of Designing Natural
Foundations and BuildinE; Substructures on Frozen Ground 6
Suvorov, B. T. Experience In the Construction of Buildings
and Structures on Thawing Ground 18
Ushkalov, V. P. Computing the Bases of Foundations on
Thaw-14ng Ground According to the Limiting Conditions 27
_D_QkuahAyev,_Y._.P. Experience In Designing Foundations
in Northern Permafrost Regions 37
Bakanin, V. P. Construction Conditions and the Exploi-
tation of Mining Enterprises In the Pechora Coal Basin 47
Card 2/4

80120
S/141/59/002/06/001/024,
AUMORS: Gershman, and Dokuchayev, f?M/E314
TITLE: On the Theory of Formation of Ionospheric Irregularities
in the F-layer \-?
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1959t Vol 2, Nr 6, pp 843 - 847 (USSR)
ABSTRACT: An analysis of recent papers (Refs 1-3) shows that one
of the most difficult problems in the theory of the
ionosphere is the theoretical interpretation of the origin
of irregula-rities in the F-layer. In the present paper
the authors are concerned with the mechanism originally
put forward by Martyn in Ref 4 and later analysed in detail
by Dagg (Ref 5). In their papers, Martyn and Dagg have
only formulated the above hypothesis but have not given
any quantitative estimates. The present authors start with
the microscopic equation for the electric field E given
by Eq (1), where j is the total microscopic current.
This equation is written down for the'case when:
div E e ON N 0
e
Cardl/5

S/141P, 'O:L'Y4o6/oOl/024
2032/Z31-14
On the Theory of Formation of Ionospheric Irregularities in the
F-layer
where -e is the electronic charge ajud
N and N I are the-concentrations of electrons
and tons , respectively.
The latter condition Is satisfied for a quasi-neutral
plasma, in which case N e W Ni . The current I is
related to the field E Vy -the generalised Ohm's law
wh1ch, fcr quasi-stati;T pro .'c,ess-ear-may'be written in the
form given by Eq (2), where h is a unit vector-in the
direction of the field H 0 , ;ihich'is the ma4;imeotic field
due to the-Rarth.- Since in thd general case the medium
is in motion, Eq (2) includes not the field R but the
fl:eld El . defined by Ect. (3), where =EA= [jH,,j/c and
v is the velocity of.the medium. In Eq (2) o~, d and
d are,the longiiudixia:~*and transverse conductivities
a:no the Hall qonductivity, respectively, and are given
by Eq In Eq (4) 9 is the effective number of
Card2/5

S/l41/59/oo2/o6/ool/o24
E012/fJJ4
On the Theory of Formation of Ionospher 0 egularities in the
F-layer
collisions between electrons and other particles,
Vi are the number of collisions for ions, w H and A H
are the gyro-frequencies for electrons and ions, m and
M are the mass of electrons and ions and N 13 N e = N,
Eq (1) can be written in the form given by Eqs (5), (6)
and (7) if Eq.(2) is taken into account and the
coordinate axes are defined as follows. The x-axis is
directed towards the geomagnetic equatorg the Y-axis
is eastwise,.and the z-axis Is taken vertically upwards.
In these coibTdinates the Earth's magnetic field can be
written in the form:
H = H h H cos i-- H sin k
__o 0- 0 XA 0 ka
These equations are applied to the case which is found
to hold in the Ionosphere above 130 km. In that regiou
it may be assumed that d,= 0 and d 'D and d I are
Card3/5 ' given by Eq (8). Moreover, -ji > -aH a The discussion

80120
S/141/59/002/o6/001/024
ffl24 4
On the Theory of Formation of lonospher PAQuIarities in the
P-layer
is then specialized to the case of )Lac 900. and )L =L 0
Under these conditlons,,and using the above apprcximationsl
the appropriate equations for the electric-field components
are given by Eqs (9) and (10), from which it follows that
it is necessary to solve two types of partial differential
equations, I.e* those given by Rqs (11) and (12). The
solution. is sought.in the form given by Eq (13), where
k canin genera3, be complex. Substituting Eq (13) into
Eqs (11) and (12), Eqs (14) and (15) are obtained,and
using the substitution x = exp(z/z 0 ) in Eq (14) and
X = exp(-Z/Z 0) In Eq (15), the solutions given by Eqs (16)
and (17) are obtained, where H (1,2) are the Hankel
V
functions of the first and second kind.and the other
symbols are defined at the top of p 84~. When the
boundary conditions are taken into account,and it Is
assumed that the fields are generated in the E-layer
Card4/5 L-(

On the Theory of Formation of
F-layer
80120
S/141/59/002/o6/001/024
110g2j8~14
Ionospherl r egularities in the
without any discontinuities and fast changes In the
properties of the medium, the final form-of the solutions
is given by Eqs (18) and (19). These equations are
used to show, using the data reported by Martyn in Ref 6,
that only the transport of large-scale irregularities In
the electric field is possible. It is concluded that
the Ma-rtyn-Dagg mechanism can explain the formation of
more-or-less regular motibus In the F-layer but Is
IncApable of ensuring the formation in this layer of
irregularities on the :3cale of the order of 2 - 4 km.
There are 7 references, 5 of which are English and
2 Soviet.
ASSOCIATION: Nauchno-issledovatellskiy radiofizicheskiy institut
pri Gor1kovskom univerattetR,(Selentlflc-research Radio-
physical Institute of Gorlkiy University)
SUBMITTED: July 13, 1959
Card 5/5

69413
s/141/60/003/01/004/020
E032/E414
AUTHOR., Dokuchayev, V.P.
TITLE: ~i~ffusion in =eteor Trails NI/
PERIODICAL%Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1960, Vol 3, Nr 1, PP 50-56 (USSR)
ABSTRACT: It is well known that when meteroic particles pass
through the upper atmosphere (at an altitude of about
80 to 120 km) clouds of enhanced ionization having
approximate cylindrical form are produced. These
ionized columns disappear as a result of diffusion,
recombination, turbulent mixing and a number of other
factors. It has been established that diffusion is the
most important. It is assumed that the diffusion of
charged particles in meteor trails is of ambipolar
character and can be anisotropic because of the presence
of the earth's magnetic field. In order to calculate
the diffusion coefficients, the author uses the quasi-
hydrodynamic equations which describe the motion of
Card 1/4 charged particles in a weakly ionized plasma (Ref 8) q1"

69413
s/i4l/60/003/01/004/020
E032/E414
Diffusion in Meteor Trails
and which are given by Eq 3 and 4. Neglecting terms
containing time derivatives, it is easy to show from
these two equations that the electron and ion current
densities are given by Eq (5) and (6) respectively.
Starting these equations, it is shown that the diffusion
coefficients in the direction parallel and perpendicular
to the magnetic field are given by Eq (15) and (16)
where a is the conductivity and e and i refer to
the electrons and the ions respectively; N is the
charge density and x is Boltzmanngs constant. It may
be concluded from this formula that the diffusion
coefficients, both parallel and perpendicular to the
magnetic field, are determined by the charged particles
with the lowest mobility. If one assumes that the
product of the particle mass and the effective number of
collisions with air molecules is much greater for the
ions than for the electrons, then the diffusion
coefficients are given by the simpler equations (17) and
Card 2/4 (18), where w = eHO/mc. From this expression for V

69413
s/i4i/60/003/01/004/020
E032/E414
Diffusion in Meteor Trails
the diffusion coefficient D
.L it may be deduced that
the criterion according to which the magnetic field
has an appreciable effect on the process of ambipolar
diffusion is given by Eq (19) where *%) is the collision
frequency. If the condition given by Eq (19) is
satisfied, D11 becomes greater than D1 , ie the
process becomes anisotropic. It is also shown that the
ratio of the linear dimensions of irregularities in the
electron concentration in the ionosphere in directions
perpendicular and parallel to the magnetic fieldt are
equal to the square root of the ratio of the corresponding
diffusion coefficients. Thus, the study of the effect
of the earth's magnetic field on the diffusion process in
meteor trails is closely connected with the problem of
anisotropy of small-scale irregularities in the ionosphere.
It is just in the region where ionized meteor trails are
formed (90 and 120 km) that the transition takes place
from isotropic to anisotropic diffusion. Above 110 km.
the-anisotropy due to the magnetic field is quite
Card 3/4 strong. However, Eq (17) and (18) are quite general

69413
s/14i/60/003/oi/oo4/o2o
E032/E4i4
Diffusion in Meteor Trails
and apply to the transition region. The present theory
is in agreement with the results of Greenhow and
Neufeldt (Ref 12). Acknowledgements are made to
B.N.Gershman for constant interest and discussion of
results, There are 1 figure and 12 references, 2 of
which are Soviet, 1 a translation from English and
9 English,
ASSOCIATION&Nauchno-issledovatellskiy radiofizicheskiy institut pri
Gor1kovskom universitete (Scientific Research
Radlo-Physical Institute of the Gor7kiy unlveFg-ity)
SUBMITTED: January 29, 1959
Card 4/4

60670
WQ/141/60/003/02/004/025
E032/E314
AUTHOR: Dokuchayev, V.P.
TITLE; On the Scattering of Radio Waves by Long-lived Ionized
Meteor Trails
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1960, Vol 3, Nr 2m. pp 199)- 207 (USSR)
ABSTRACT: Two hypotheses have been advanced as to the mechanism
whereby radio waves are scattered from trails"*'Wl-th high
electron concentration. The first of these is due to
Herlofson (Ref 2) and was developed in detail by Kaiser
and Closs in Ref 3. It assumes that a trail having a high
electron concentration scatters6radio wavessin a way
similar to the scattering of such waves by a metallic
cylinder. According to the second hypothesis put forward
by Booker and Cohen (Ref 4), there are small-scale electron
density irregularities in the region of the trail which
appear as a result of turbulent motion in the surrounding
medium. According to this'mechanism the scattering of
radio waves by the statistical irregularities has a non-
coherent character. It is shown in the present paper that
Cardl/3 during most of their lifetime the trails scatter radio L/

80870
s/l41/6o/oO3/O2/oo4/O25
n ed Ionized Meteor Trails
On the Scattering of Radio Waves E93E~Ejjjiv
waves similarly to a metallic cylinder (Herlofson and
Kaiser theory). The non-coherent scattering mechanism
theory put forward by Booker and Cohen does not agree with
experimental data on the t1me-distribution of reflections.
This is the case both in sporadic meteors and meteors in
streams. The turbuleit diffuaion mechanism leads to a rapid
disappearance of tracks even with a very high initial
electron density which is indicated by experimental data
and is easily understood on the basis of physical consid-
erations. An increase in the diffusion coefficient should
lead to a rapid disappearance of the trail and should
reduce rather than increasethe number of long-lived trails and
the reflections from them. Moreover, there are days when
ionospheric stations indicate the absence of strong
turbulent flow in the E layer of the ionosphere.
According to Booker's hypothesis there should be a reduction
in the number of long reflections from meteor trails during
such days. However, such a strong correlation between these
two phenomena does not appear to have been established.
Card2/3 The paper is concluded with an attempt to explain the fadin

80870
5/141/60/003/02/004/025
E03
On the Scattering ofRadio Waves by Long-MRPIonized Meteor Trails
of the reflected signal amplitude in terms of the Kaiser-
Closs mechanism. It is shown that the fading is due to the
diffraction of radio waves by strongly-ionized meteor trails.
Acknowledgment is made to B.N. Gershman for reading the
manuscript of the present paper.
There are 5 figures and 16 references, of which 4 are
Soviet, 11 English and 1 is. Swedish.
ASSOCIATION: Nauchno-issledovatellskiy radiofizicheskiy institut
pri Gor1kovskom universitete (Scientific-research ka'dio-
physics Institute of Gortkiy University)
SUBMITTED: September 10, 1959
Card3/5

86865
S/141/60/003/005/020/026
E032/E3l4
AUTHOR-.
TITLE: The Effect of Geomagnetic Disturbances on the Drift
of Ionis s in the Upper Atmosphere
PERIODICAL: Izve tiya v-ysshlkh uchebnykh zavedeniy,
' tiya
, ~ia
Radioflz a, 1960, Vol- 3, No. 5, Pp- 901 - 903
's exp
TEXTs Fig. I shows.expertmental data on the correlation
between drift velo ties In various regions of the Ionosphere
t 1e,
turJ31
and gecmagnetic. di turbance's. This figure gives plots of the
drift velocity V ~,-Un:m see) as a function of the mean
p
j amplitude of the gecUha~~etic disturbances. These experimental
results are plotted for three regions, namely, the E-layer,
the F-layer and the R-layer (the latter causes fluctuations
In the intensity of the emission of radio stars). The relation
-'is linear in each of th ese three regions. The slopes of the
straight lines increase with altitude of the layer. Finally,
- ~--i -
:tfie'Interceptis .- on the Vp axis also increase with the
altitude of the layer. These experimental results can be
simply explained on the basis of the relation betweeJx geomagnetic
Card 1/4

86865
s/141/60/003/005/020/026
B032/B314
The Effect of Geomagnetic Disturbances on the Drift of Ionised
Gas in the Upper.Atmosphere
disturbances and the drift velocitt 5 It is well Imown that
geomagnetic disturbances are due to teraction between solar
corpuscular streams'and the outer atmosphere (exosphere)
(Refs- 5-7) . Low-Ti;queney disturbances in the exosphere,
having a quast-period greater than 10 see are of a magneto-
hydrodynamic character. These disturbances are propagated
into the underlyIng x-eglons of the atmosphereand into the
ionosphexa,by diffusion of electromagnetic wavesand on reach�ng
the Earth's surface give rise to variations in the geomagnetic
field. On the other hand, It is also known that an electric
field gives rise to the drift of the ionised gas in the Iono-
sphere. Thus, solar corpuscular streams excite magnetohydro-
dynamic disturbances in the exosphere which are propagated
through the ionosphere in the form of electromagnetic waves and
produce variations in the geomagnetic and electric fields on the
EarthOs surface. Electric fields associated with these
disturbanc'es give rise to the drift of the ionised gas when

86865
S/141/60/003/005/020/o26
E032/z314
The Effect of Geomagnetic Disturbances onthe Drift of Ionised
Gas in the Upper Atmosphere
they are propagated through the ionosphere. It is shown that
the relation between the drift velocity and the mean amplitude
of disturbances in the magnetic field is of the formt
V H?" o h
(5)
p c 1~im Ho
p
where H0 is the Earth's magnetic field,
orL is the electrical. conductivity of the medium in a
direction perpendicular to H
0
Pp is the ton density in the plasma,
NJ. is the number of collisions between ions and
:LM molecules. and
W is the angular .' frequency of the electromagnetic
Card 3/4 field.

86865
S/141/60/003/005/02o/o26
E032/E314
The Effect of Geomagnetic Disturbances on the Drift of Ionised
Gas in the Upper Atmosphere
This formula is in good agreement with the experimental results
for the E-region.
There are I figure and 10 references: 2 Japanese (in English),
5 English and 3 Soviet.
ASSOCIATION; Nauchno-issledovatellskiy radiofizicheskiy
institut prl Gor4kovskom universItete
(Scientific Research Radiophysics Institute
of Gorlkiy University)
SUBMITTED: June 23, 196o
Card 4/4

AUTHOR: Dol".ii:.,:x.
TITLL: ot' an lunl,~ed Mletc,~ov I'vaLl
PERIODICAL: Astronomiche3kiy zhurmul, 1960, Vol Nr, 1,
Po
A13STRACT: When a "burninir" imeteur p~wticle mo,;es in t-he upper
Ltom,,- fpoai this pai-ticle evaporate, become
!of I i'r,,ed, and toget'hel, with elect-ow', fol'in a cloud of
'Im.l.,ii-neUtV.al plasim). The atithor consider-, cases In,
0
whicti. the meteot- tL.ack makes an larq-,Ie of' more than 70
wiltii vespect to the vertical and in whlch the coeffi-
cient of diffugion, D, the voloctty, V, zlnd the ene-r1gy
in the trail, Q do riot chanire with altitude. if
only meteors below, 100-1kin altitude are considered,
theri the pt-ocess of' difTuston may be i-e,~-arded as Iso-
L.~
ti,opic If N is the con cent mA ion of' the plasim" it) 011~,
Caild 1/- L -,;
ant! ,; Is the coovdInat'E: a1anir the t-aj~L-101'y, then

Foriiiation ol' an Ionized Meteov Trail
'18 0 15
S 0 V I - 15 1
tit Z > 11t
A' (0, -It) (10)
at Z <
Th!:3 Indicates that In the Immedicate vicinity o'L the
meteor the concentration of' the Ionized gas Is much
greater than in the atmosphere avound it; fuPthermore,
the Concent rat loll III i'vont of' the meteov dec-1-cases
exponentially, but in the trail behind the meteor it
decreases much inove gradually. The "ounning, echo"
observed by radar results from difTerences in dispel,-
sions, in par-ts of' the troll: neLlr the flyinc; meteor
the concentvation may exceed the critical value
necessary fov the radlo wave veflection, but in other
pavt.s It 13 smaller than thlis, v:Aue. The -~Uthol- r--e-
jects i;he theory of' W,.-KInley :-nd Millman who explaill
thio efTec"t. by 21) incvc,)~;e IIII t-he 1',nd lat 1011 at thf~
e:q)ense ol' the ultr:aviolet. v~i(JJAA.on. Theve are 9
ref(-'Pences, b Soviet, '1*1 Uj-'Y I U.S. The U.S. and U.K.

1~ormation of an -Ionized Meteor Trail
ASSOCIATION:
SUBMITTED:
8015
_7 -7
OV /3 -12, "1 -1-15/31
references ace: L. A. Manning, j. Geoph. Res., 63,
181 (1958); T. R. Kaiser, R. L. Closs, Phil. Mag.,
43, 336 (1952 ; Dz W. R. McKinley, P,'M. Millman, Proc.
I.R.E., 37, 3R (1949)~
Scientific-Research Radlopl~yslcal Institute at the
Gor1ky-University (NaucYt~o-l-,~,sledovatellsl~ly radio-
fizicheskiy inst1tut pri Gor1kovskom un-te)
March 50, 1959
Card 3/3

83192
A-1
S/056/60/039/002/029/044
B006/BO56
AUTHOR: Dokuchayev, V. P.
TITLE, The Growth of Rapetohydrodynamic Waves in a Plasma Flo%
Moving Through an Ionized Gas
PERIODICAL: Zhurnal sksperimentalvnoy i teoreticheskoy fiziki, 1960,
Vol. 39j No. 2(8), pp. 413-415
TEXT: The author investigatle magnetohydrodynamic waves propagating in a
plasma moving at a velocity V through a gas at rest, which is completely
ionize al risi-neutr6l. ThR gas is assumed to be in an external magnetic
field The"formation of high-frequency electromagnetic waves 4,1
in the mO;ti8n o? electron and-ion currents in a plasma has repeatedly been
investigated. Here, the conditions are determined under which magnetohydro-
dynamic waves increasing with time (as a consequence o 'f which the system
becomes unstable) are formed in the system current - plasma at rest. Pro-
oesding from the system ofthe linearized equations (1) - (6), which do-
scribes the electrodynamic processes of the system investigated, the au-
thor obtains the dispersion equation (7) for plane electromagnetic waves
Card 1/3

83192
The Growth of Magnotohydrodynamic Waves in a 3/056/60/039/002/029/044
Plasma Flow Moving Through an Ionized Gas B006/BO56
propagating in the direction of current, i.e., in the direction of the
asgnstio lines of force of the R field. The sign + in (7) corresponds to
the ordinary,, and the sign - to The extraordinary wave. The author then
investigates the ordinary hydrodynamic approximation - the case of very
low frequencies (CO> 1
are determined, and various regions of perturbations are outlined (see
Fig. 1). An interpetation of the dependence between the drag coefficient
on the Mach number is presented, and a calculation of the energy of

ACC NR. AP7001993
emission of sound waves by the force source at M > I Is included. lk,ke
author hopes that this method of force sources may be useful for ol~,,Iaining
both rigotous and approximate solutions of problems of mechanical oolid
bodies-fluid medium inte'ractions. 'Orig. art. has: 3 figures and 39 'formulas.
SUB CODE: 20/ SUBM DATE: 06Sep65/ ORIG REF: Oll/ OTH REF: 006
ATD PRESS: 5111

DDKUCUYEVI V. V.1 Candidate Tech Sci (dime) -- "Computation of the depth of
foundations in permfrost". Leningrad, 1959. 17 PP (Min Transportation USSR,
Leningrad Order of Lenin Inst of Railroad TTansport Egnineers im Acad V. N.
Obrazteov), 150 copies (KL, No 24, 1959, 136)

DOKUCHAYEV9 ~.V.
calculating the depth,of
grounds. Trudy'Gos.inst.
no.6:3-28 159.
(Foundations)
buildin 'toundations in permafrost
9
po proek. mor. pro. i sudorem. pred,
(MIRA 14:3)
(Prozen ground)

PUUMYE-Vp -Vladimir Vladimirovich, kand. takhn.nauk; SIPIDIN,
V.P., kan 0 na ~ nauchnyy red.; KOSTANDOV, A.I.,
red.izd-va: PUL4KINA,,-Ye.A., takhn. red. I w- I - - I
(Foundations and footings OR Permafrost]-Oonovaniia i funds-
menty na vechnomerzlykh gruntakh. Leai^ngr'-*d, Gosatro112dit,
1963. 194 p. (MIRA 16:5)
(Foundations) (Frozen g '
roxind)

A&035375 BOOK DITATMN S/
Venis Tu (candidate of Technical Golemsh DokudbaMs V, Vq Moms
N. F. iDootor of Technical Sciences)
Buildings and structures In. the szLreme Northl a handbook (Maniya I somzbeniya
na Kraynem Severej vWaroobnoye posoblye)# LeninVads Goastroyisdats-W3p
(At bead
h9o p, illus,s biblio, Irrata slip innowtedo 5#000 copies printed.
of titles Lenmoruiiproyekt).
'TOPIC TAGSs civil engineeringp constructions highways paroafrosts commmicatlAm
lines water plant
PURPOSE AND COVERAGEs The book presents handbook data necess=7 for plamings do-
signing, and construction of conamitiess civil and industrial buildings and their
structural elements In the northern regions of the country and also gives data for
designing engineering links& higbwayss water plantss commication Unasj, an4,elec-
trical transmission linee* The book contains the technical-economic indicators
and hanM=k materials necessary to select design parameterso The book In Intended
for enginsers-planners and constrwUm vorkwao
CWj

.AIM4035375
TABLE OF CONTENS [abrLdgedll
Foreword - 3
Introduction -- 5
Part I. Planning., Construction., and Public Welfare of Settlements
Ch, L Features of planning and construction of settlements 19.
Ch, n, Engineering preparation of the territory 47
Ch, In, Snow proteation of settlements mm 64
Ch.,IV. Municipal and town highways - 86
Part II. Civil and industrial buildings and structv"s
Ch, V. of buildings
Space-planning and structures 103
Ch. VI. Heating of enclosed structures - 248
Ch, Vn. Planning load-bearing structures - 176
undations 236
71s Designing buildings on melting fo
Ch. VI1
Part IM Foundations
01
Ch. IX*. Structural at son - 256
Ch, XG, Use of PIM&MMOU Win tamdations 279
'Ch* X1, PlAnning 1mindations on pwmaftvot bass -- 299
Ch. XII. Deaigni~g foundation@ an bases Q-W 345
e I
Card 2/3

Ch, XIM Designing foundations on saltei givund and under equipment 385
Paq IV. Sanitation-technical comiAmication and equipient, Conuunication, lines
nd electrical trpnemission
Ch,~Vo Features of sanitatioip-technical communication - 396
Cho calculation of networks and equipment In permafrost.
Thermo-toohnioal
soil -. h25
Ch. XVI, Water olants - h33
Ch. XVTI.' Features of the design and construction of Ounping stations AVA
and cleaning equipment
Ch. XMI, Communication lines and electricity transmission 459
kppendix - 473
Bibliogranby .4M
SUB CODES NZ M&X&Ms OPD*c6) IR Ur SOVs 056-
OTHMt 000 DA72 AOQs 26APr64
Cwd 313

MAZUROV, Grigoriy Petrovich; DOKUCHAY V.V.p kand. tekhn. naLk,
-- - --.-
nauchn. red.
(Physical and mechanical properties of frozen ground;
methods of determining and employing them in calculationsl
Fiziko-mekhanicheskie svoistva merzlykh gruntov; metody
opredeleniia i ispolIzovaniia v raschetakh. Leningrad,
Stroiizdat, 1964. 164 p. (MIRA 17:12)

21(6) SOV/89-6-1-13/33
AUTHORS: Dokuohavev, Ya. 11., Osipov, 1. S.
TITLE: Determination of Specific a-Activity aild the 11alf-Life of U233
(Opredeleniye udellnoy a-aktivnosti i perioda poluraepada U 233)
PERIODICAL: Atomnaya energiya, 1959, Vol 6, Nr 1, PP 73-73 (USSR)
ABSTRACT: The specific activity of 5 uranium samples was determined.
The isotope composition, which was measured mass-spectroscopi-
cally, fluctuated in the case of individual samples between
U232 4.10- 3 percentage by weight
U233 93.28 up to 95.24 percentage by weight
U234 2.25 up to 2.36 (� 0.07) percentage by weight
U235 4-' 0.1 percentage by weight
U 2-46 up to 4.38 (+ 0.07) percentage by weight.
A nitric acid solution is produced from each uranium sample.
Card 1/2 From each of these solutions 30 preparations having a diameter

SOV/89-6-1-13/33
Determination of Specific a-Activity and the 11alf-Life of U233
of 10.� 0.5 mm was made. The basis material is not given.
The preparations were measured by two pulse ionization chambers
with a small solid angle. From the multiplicity of me~Sye-
ments it follows that the specific activity of 1 ~g U
corresponds to 20.950 + 100 a-decays. To this specific 4
a-activity there corres-ponds a half-life of (16.20' + 0.08).10
years. This result is in good agreement with the dja Given
by references I and 2. There are 2 references.
SUBMITTED: September 20, 1950
Card 2/2

21(8)
AUTHORz Dokuchayev, Ya. P. SOV/89-6-1-14/33
239
TITLEz Determination of the Specific c(-Aotivities of Pu and
Pu 240 (Oprodeleniye udellnoy c(-aktivnosti Pu 239 1 Pu 240
PERIODICAL: Atomnaya energiya, 1959, Vol 6, Nr 1, Pp 74 - 74 (USSR)
ABSTRACTs The specific 4-activity of Pu 239 and Pu 240 was determined
from 12 plutonium samples the isotopic compositions of which
were within the following limitsi
Pu 239 91.26 to 99.11 percentage by weight
Pu 240 (0.87�0.06) to (7-57tO-lO)percentage by weight
Pu 241 (1-M-3)-10- 2 to (1.04�0.05) percentage by weight
Pu 238 (1.62tO.10) to (1-75+0-05).10- 2 percentage by weight
242 257
'Pu + Np , 0.01 to 0.1 percentage by weight
A solution was produced from each of these samples. From
each solution 25 preparations were produced by weighing. The
activity of the preparations was determined by parallel
Card 1/2 measuring (after drying and hardening of the precipitation)

Determination of the Specific c(-Activities of SOV/89-6-1-14/33
Fu 239 and Fu 240
in two ionization chambers with a small solid angle. Each
preparation was measured for 90 minutes in each chamber.
The specific activity of Fu 239 +Pu 240 was determined from the
difference between the measured activity and the activity
PU 238+An 241+PU 241.
1'Ag PU 239 has 136,2OOt2OO c(-decays / min., which corresponds
to a half life of 24,39Ot3O years.
1 'Ag PU 240 has 500,OOOt4,000 c(-deoays / min., which
corresponds to a half-life of 6,62Ot5O years. The half-lives
obtained agree well with the data given by references 4 and
5. There are 5 references.
SUBMITTEDt September 20, 1958
Card 2/2

DOKUCHAYEV, Yuriy Aleksandrovich; TITOV, G.S., Geroy Sovetakogo
S-o-yuza, letchik-koemon-wit SSSR, red.; BYKOV, V., red.;
LESHCHINSKAYA, G., tekhn. red.
(Going to the stars] Idushchie k zvezdam. Moskva, Molodaia
gvardiia, 1963. 106 p. (MIRA 16:5)
l.Spetsiallnyy korrespondent agentstva pechati "Novosti"
(for Dokuchayev).
(Astronauts)

Goihg to the
Starsh.-serzh. no.9s4-5
(Astronautics)

DC*'.MRYrVA, A. ~,. (11ccm Etarz)
OCKLICHAYEVA, A. V. (14LCii ENcrz) -- "TECHNOLOI-ICAL VROULDIS' OF TRACTOR FLc' SVE'- 2~1 VAR ~2,
MOSCOW 111ST or MIECHANIZATION AND ELE:CTRIF$CATIOI1 or AwtICULTVRE Y. If.
(D15SE11TATION rOR THE DcrRcE CT CANOICATr it., TEcHwCAL SCI NCE I
E E:,
SO: VECHERNAYA M~OSKVA, IANUARY-DtCEMDER 19r"

SVIRSWHRTMY. Bromislay Stanislarovich; ABIEKOV, M.S., red.; ANTONOVSKIT,
B.N., red.-; BIDNTAXWAt A.V.,,'red.; GIAUO, V.G., i-ed.;.GORMJT3.
P Z i red L Ted.; 7ILMM, A.V., red.; KISXW,
.--A.B., i9do KCNMTI
r ed:- tvm Mff, X.A., -red.-, KONWSUP,
V.A.: red.: KWANOIV, A.i.9 IN, X.D"s, red.; 7M. No3o,
v red.; PMAT
red.; NEW, B.Ta., red.; XUMOVA. N.N., tekhn. red.; GMIKOVA,
Z.D., tekhn. red, I
[Utilization of tractorn and machinery] Akepluatataiia mashinno'-
traktornogo Parka. Izd.3., perer. Xoskva, Goo. izd-vo sellkhow.
lit-27, 1958. 660 p. (xiu 11:10)
(Agricultural machinery)

DOLZMIKOV, Andrey Tim-O'&A- P
itch, dotsent'-kand.tekhn.nauk; ABDREW,
Nikola'y Ilikolayetvich,p. doteont; DOKUCHAYVVA, �gusta Paramonavas,
doteent; _K=0f;-Mi~'n '1~nvlovlch, st-a-r-sEry '~re~oaava- M617-ITSMT.
Ivan Ivanovich, dotsent; PARAMZIN, Ivan Ivanovich, dotsent;
TROFIMOV, Vladimir Ivanovich, dotsent; BMZOVSKAYA, A.L., red.;
KRYUKOV, V.L., red.; RAKOV, S.I., tekhn.red.
(Reference manual for young agricultural machinery operators]
Spravochnik molodogo meklianizatora Bollskogo khoziniatva. Moskva,
Voss. uchabno-pedagog.izd-vo Trudrazervindat, 1959. 694 p.
(MIRA 12:12)
1. Prepodavateli Moskovskogo institUta makhanizataii i elektri-
filmteii sel'skogo khozyaystva (for Dolzhenkov, Andreyev, Dokuchayeva,
K0210V, Kiselev, Paramzin, Trofimov).
(Agricultural machinery-Maintenance and repair)

DOKUCHA'YEVA, A.P., dotsent
Effect of the condition of plowshares on the quelity and economic
aspects of plowing. Trudy 141MESKH 6:179-188 159. (MIRA 14:5)
(Flows)

ANDREYEV, N.N., dots.1 ACHKASOV, K.A.p st. prepodavateD; DOLZHENKOVp
A.T., dots.; DOKUCHAYEVA A.P., dots.j KISELEV, I.I., dots.;
KOZLOV, I.P.; at. prepodavatell; TROFIMOV, V.I., dots.1
PESTRYAKOV, A.I., nauohnyy red.; SHALYT, N.A., red.,- TOKER,
A.M., tekhn. red.
[Manual for the young agricultural machinery operator) Spra-
vochnik molodogo mekhanizatora sellskogo khoziaistva. Pod red.
A.T.Dolzhankova. Izd.2., ispr. i dop. Moskva, Proftekhizdat,
1963. 653 p. (MIRA 16:6)
1. Fakulltet makhanizatsii Moskovskoy akademil im. K.A.
Timiryazeva (for all except Pestryakov, Shalyt, Toker).
(Agricultural machinery)

DOUG noyna kande tekhn. nauk; GUZUNOVA., N.I.,,
red. - IV 2 A*Ssp khno red,
[High production use of machines and tractors) Vysokoproizvo-
ditellnoe ispoltzovanie mashinno-traktornogo parka. Moskva.,
Izd-VO "Znanie," 1961. 38 p..(Narodnyi universitet kulltury:
Sel'sko-kho2iaistvanMi fakulitet,, no.18) (MIU150)
(Agricultural machinery-Produotion standards)
(Tractors-Production standards)

STARUNv Y.R,; DUDAVSKlYp I.Ye.; DAVYDOVs I.P.; KOLESNIKp M.I.;
RYAZANTSEV9 V.D.; SAMOnMv I.G.; DOKUCHA3ZVA9, I.N.
Dressing chrome iron ores from the Kimpersaiski deposits by
magnetic separation. Ogneuproy 25 no. 3:108-U4 160.
(13:10)
1. Zaporozhakiy ogneupornyy zavod (for Starung DudavskiyP DavydovP
Kolesniks, Ryazantsev). 2. Institut "Makhanobrehermet" (for Samo~~-
lovp Dokuchayeva).
(Ore dressing) (Magnetic separation of ores)

?RAS I BOON ZVWrTATIGN SUV/4984
International symposium on macromolocular chemistry. .Moscow,
2960.
Xe-h-13marodn simpozium po aikrosolokulyarnor kbi-IL SSSR,
Noskva# IV-18 y& 1960 g.; doklady I avtoreferaty.
SektmLya III. rZaternational Symposium an X3cromolecular
Chemistry Hold In Moscow. June 14-18, 1960; Papers and
3ammarles) Section 111. (Moscow, Izd-vo AN 3S3R, 1960]
469 F. 55,000 copies printed.
TocjL. Zd.: 11. 3. Kashina.
SponsorIng Agencys Tho.International Union or Pure and ApplIed
Cbmmlstr7. Commission an Macroaclecular Chemistry.
PURPM: -This book to intend6d for chemists Interested In poly-
marizatloo reactlona And the synthesis of high molecular
eampounds.
CCVZR=s This Is 500 tIOU III Of a 21'atIvolume work contain-
Ing Pape" cc aacromolocular chemistry. The articles In
general deal with the kinetics or polymerization reactions,
the 8ynth0mLX Or special-purpose polymers, e.g., Ion ex-
change resins, semiconductor materials, *to., methods or cat-
17-1 9 POIYa*rlz&tL*n reactions, properties and chemical
Interactions Of high sole"lar naterlals, and the effects or
TOKOOM f%ctO" cc POITmerIzation and the degradation of
high molecular compounds. In p*rsona.1.1ties art mentLoned.
Reffti-ences given follow the articles.
and j_jL=Z&d_ (Poland). Chlorination or
Phowl-Formaldehydo Regina 27

1
(Ruzania).
1
'
1
h
4
folyvlnyl Alcohol
y
12
", PYI FLU.
'
34
Zjob-jo. A. T2- a- T., Cordnn, Ye- N~
.1
a (USSR1.
I
1
and
1
I
&;X.
Z
C
g
-_Atudy or. the versions of PolyearbonatIp 44
Dyamd2kIn. B. A , X* 3. Pol'dshtern. and Z-A-ZalZapaza (USSR).
-
Chevacal. Interact
Ion and-X veanism of -he AotivatIng Action
of Vulcanization AoeleratorS

gsuz. r. __Vo-b'Zeva, and M~ P~
Fin . &-E
-
1-
Hazer* or suirur-le Acid and Pollviny
73

"
d 0. Ttj rzg'- (Hungary). The Inter-
ff2
'
1
T
b
ff
-
;
ac
A
n
Nn.:
&nd Polyvinyl Chloride 79
A
a
0;
Zh;
ti
USSR). The 46~
mle4odu4tor Proper as
XLk"v-1-A., and CbemLcal Properties
of RLPolar Ion-Excliango Resins
93
jgakftk~l~ I.j. and J. Morawlea (Poland). Effeqt of the Struc.
turs OLf organic ARN-0-T-c-c-P-0-un-do on the Properties of AnIon
-A45hjknpAesin* From Po2ystyrtne
SAIdAd-tt-K-K. (U3SX). The Problem of the Effect or the
- ro
5Vr-ucVQrv of -nites on Ion -Exchange-ftoe *esea Between
lonitas and Electrolyte Solutions 10T
Bps-r4L_.L, A., --LU&0=X. and
__t,2Arjmj_ (USSR).
JF-_ _
.CtIon-afid Proportion of Some Aromatic Polymers 115
P. L*eev -3 S. B.
Wstranskma. Y4
#d0.., j&O WRY. Chemical
Conversions Of soluble Copolymers of Styrene 124
Poland). Thermal Stability of Strongly Basic
Mi. k.-, Real
no 146 40

RUDDIANOV, JQuD.; 3)OXWH&IMVA, N.Y.
A large aneurysm of the descending aort& simalating a hydated cyst
of the left lung. Xhirurgila no.12:66-67 DI 55. '%NLRL 9--7)
1. Is kliniki fakalltatakoy khirurgii (say.-prof. G.K.Kinte)
Samarkandskogg meditsinskogo InstItuta.
(AORTIC-ANJUNISM, differ- diag.
echinococcosis of
(,;JIM$ dies
sohinococcosis. differ. divig.. from aortic aneurysm)
(IGEIINOCWGWIS
lung, differ. diag, fron aortic aneurysu)

RAXHKANOV,lh.D. (Uzb.SSR., Samarkand, ul. Ksyl-Davat, d.6); DOWCHAUVA, N.Y.
Multiple cartilaginous exostosim. Yest.khir. 77 no.9:120-122 S '56.
(MIRA 9:11)
1. Is fakal'tatskoy khirurgicheekoy kliniki (i.oosav. - dots. V.7,
Medvedkov) Samarkandskogo meditainskogo instituta im. I.P.Paviova.
(EXOSTOSIS, NUI&IPIA, case reports
cartilaginous.)

a
DOKUCHAYEVA, Ii. F. Ca d Med Sci -- (dies) "X-Ray Picture of the
", ta~ j
Osseous System 4%gftg eat Burns. (Clinical-er-Ray Parallels)."
Samarkand, 1957. 20 pp 22 cm. (Samarkand State Medical Inst im
Academician I. P. Pavlov), 200 copies (KL, 28-57, 111-112)
- 34 -

DOKUCHAYEVA, N.F., kand. med. nauk; SHAKIROV, M.Sh., kand. med. nauk
Data of X-ray investigations following neurotomy of irradiated
animals. Nauch. trudy SamMI 22%49-57 163. (MIRA 17:9)
1. Iz kafedry fakulltetskoy khirurgii i kafc-dry rentgenologii
i meditsinskoy radiologii Samarkandskogo meditsinskogo instituta.

RAIUiMANOV, Eh.D.., dotsent;,.DOKUCHAYEVA, N.F.,, kand.med.nauk
Anomaly of the urinary tract simulating actite appendicitis.
Vept.khir. no.l.-134-136'63. (MIRA 16:7)
1. Iz kliniki fakulltetskoy kWurgii (zav.-prof. F.M. Golu~) i
kafedry rentgenologii i, radiologii (zav.-dotsent G.S.Kuznetsov)
Sams kandskogo meditsinskogo instituta imeni akademika I.P.Pavlova
(rektor - dotsent N.N.Khaitov).
(URINARY ORGANS--ABNORMITIES AND DEFORMITIES)
(APPENDIGITIS)

D.
USSR/Astronomy - Nebulae
May/Jun 49
"Int6p,ral Photographic Astral Dimensions of Certain Planetary Mists," L. N. Radlova,
0. V. Kats, 0. D. Dokuchavev,, State Astr Inst imeni P. K. Shternberg, 1~ pp
"Astron Zhurl Vol XXVI, No 3
Discusses southern planetary mists photographed in 1947 by L. N. Radlova and 0. V. Kats
at-Abar.tuman Astrophys Ubs. Photographing was done with an 8-inch camera (one meter
length) and a Schmidt nonaberration camera (D-36 cm, P-62 cm). Gives table of names of
mists, their coordinates for the year 1900, angular diameters, etc.
58/49T4

to
E-I
C-1
USSR/Astronomy Absorption Coeffi- Sep/Octo'52'
cient
,Problem'of Reality of Stellar Model With Con-
stant Coef?icients of Absorption," A. 0. Mase-
vich,.O. D. Dokubhayeva, State Astr Inst imeni
.Shternberg
"Astron Zhur"', Vol 29, No 5YPP 526-531
Analyzes mass-luminosity7radius relations by vari-11
ous scientists.'- Concludes that a model of a
purely s~cattering star does not correspond to re
amity pjvwin~the casb of highest tole., es, in
cbem compn. Absorption by electrons inIstars of by,.
drpgen and helium will, always - play an impo-rtant role,
-king the discussed model unreal. A model with-,
60,hst absorption - 6oeff may be considered only as a6
tbeoretical limitifig case.
0
234T56

vUKuCK,kYEVA, 0. 1).
mase of Urion nebula, qstron.

DO, 11C I U11111 F, IrA0111).
6Vi
USSR/Aii:- fuie Nebula
a ronomy Tan/reb 53
"Determinati6n of Mass of the Diffuse Nebula of
Orion,",' O.D.. Do.kuchayeva, State Astron Inst imeni
Shternberg
"Astron Zhur" Vol 30, No 1, pp 76-79
States results of mass determination of Orion
nebula using V. A. Ambartsumyan's method (Ucbebrdk
Teoreticheskoy Astrofiziki, 19391.' Work is per-
formed according to project of State Astron Inst
imeni Shternberg. Obtains for mass of nebula
around 166itime's mass of Sun. Indebted to Prof
.B.A. Vorontsov-Vellyaminov. Received 9 Apr 52.
246T43

DOKUCHAYEVAj 0. D.
t'Study of Characteristics of B Type Stars With Emission Lines
in the Speattrum." Cand Pbys-Math Sci, Moscow State Uj State
Astronomical Inst imeni Shternbergs Moscow, 1954. (RZMfftr, Noy 54)
Survey of Scientific and Technical Dissertations Defended at USSR
Higher Educational Institutions (3-1)
SO: Sum. No-521, 2 Jun 55

VORONTSOT-VILITAKINOV. B.A.;_DOKUCHAYNA, O.D.; YEMMDV, Tu.I.;
KOZARENKO, B. 1. : Y-WWWA.77~1r,-KOSWAKOVA, Te.B. ; LDZIIISKIT, A. X.;
MANOVA, G.A.; TSITSIN, P.A.; SHAROT, A.S.
Observations of Arend-Roland's comet (1956 h). Astron.tsir.
no.180:2-4 Vq 157. (MHA 13:4)
1. GosudarBtvenn~7 astronomicheakiy institut im. F.K.Shernberga,
Moskva.
(Comets--1956)

DOKUCHAMA, O.D.
The final luminosity curve of 3M GemiDorum. Per.zvezdv 12 n0-5:358-
363 N 158. (KIPA 13:9)
1. Goaudarstvenny7 astromonichookiy institut im.Shternberga.
(stars, NOW)

DOKUCHAYITAo O.D.
Determining the spectrophotometric temperature and the Balmer aerie
decrement of AG Pegasi (1952). Per.zvezdy 12 no-5:372-373*N 158-
(IMU 13:9)
1. GosudarstvenW astronomicheakiy inatitut im. Shternberga, Moskva.
(Stars, Variable)

XMWIN,
H 14-Y&711,~ 6) J>-
S.G.; KOYBASYUK, L.D.; DAGAIW, M*M.; ROZIMBLIUM, N.D.; TMRCHENKO,
I.F.(Irkutsk); KATIRIN; A.A.:(Irkutsk); KONSTANTINOVA, T.G. (Irkutsk);
=='A, T.A. (Irkutsk)-. XMIN, G.T. (Irkutsk); SAIONOTA, Z.G.,
(Irkatsk)-, COW , L.I. (Iiimtoj); CMWWt*N.S (Irkiitak);
MWIDWICHO To.Ge'; 3MMM9 T.A.1 TAKHMMTA, N.;, (Lsning~!d);
P=YA~ WeB*,j_pq1VMj3 AL O*D*; KATAW, L.A.; KLTAKOTKO, K.A.;
PARUJaO, P.P. SHCNi6fNi3VX6 A, I.S.; KIMICH, 1&'G*;.
RTABOT, TV.-I.; SHCHIMOT, T.P.-, IV.G.~ NART7NOT, D.Tse;
FIDINSKIT, T.T.; TORONTSOT-73LITAKINOT, B.A.; ZIMMI, P.Tu.;
SAMIN '1*74., red.1 AMMOT, M.,
j P*-I,, oty,red,-, I - IN,
tekhn.red,
[.Astronomical calendar] Astranosiohnskii kalendar. [A yearbook;
Takable section for 19591 Sshsgodaik.' raremennaia obast', 1959.
Re'd.kellegliai P~1. Bakalix i dr. Moskva, Gos.isd-ve hziko-
mstom.lit-ry, 1958 370 pe (Yeseciusnoo astr9nomo-goodesioboskes,
obshchastvo, no.Ui (MIRA 12:2)
1e G~sudarstvonzoys astronome-goodesighe keys obehohostvo (for Wagin,
lovbasyuk. Momidevich). 2. Hoskovskoye itasieniy* Vassoyuznogo astre-
zome-goodesioheeksgo obehohsotva (for Dmgay*vl Rosonblraj?, Bronshtelt,
Pereva).
(Astronomy-Toorbooks)

o v" Li (I.- H AA b
~.q PHASE I BOOK EXPLOITATION SOV13651
Vsesoyuznoye astronomo-geodezicheskoye obshchestvo
Astronomicheskiy kalendarl 1960 (Astronomical Calendar, 1960) Moscow,
Fizmatgiz, 1959. 351 p. (Series: Its: Yezhegodnik; peremennaya
chast', vyp. 63) 7,200 copies printed.
Ed.: I.Ye. Rakhlin; Tech. Ed.: S.N. Akhlamov; Editorial Board: P.I.
Bakulin (Resp. Ed.), M.M. Dagayev, S.G. Kulagin, A.G. Masevich, P.P.
Parenago.
PURPOSE: The book is intended for astronomers and geophysicists and
physioists interested in astronomical phenomena.
COVERAGE: This yearbook on astronomy was compiled by a number of Soviet
scientists specializing in several different branches of astronomy.
The following persons participated in the work: L.D. Kovbasyuk, who
wrote the chapters on ephemerides of the Sun and Moon; M.M. Dagayev,
the chapters on planets, eclipses, physical coordinates of the Sun,
koon, Mrs, and Jupiter, and the satellites of Jupiter and Saturn;
V.S. Lazarevskiy,the chapters on ephemerides and heliocentric longitudes
,of planets; Ye.G. Demidov, the chapters on occultation of stars and '
planets by the Mponj observations of Polaris and computation of coor-
Card 1/6

Astronomical Calendar, 1960
SOV/3651
dinates of stars; V.A. Bronshten, the chapters on comets; N.S. Yakhon-
tova, sections on minor planets; and N.B. Perova, the chapters on
variable stars. The appendixes contain articles on recent develop-
mbnts and events in astronomy such as the launching of the first Soviet
space rocket, the 10th Congress of the International Astronomical
Association,held in Moscow in August 1958, developments in a4ronomy
in 1958 during the IGY. There are 385 references, all Soviet.
TABLE OF CONTENTS:
Editor's Note
PART I. EPHEMERIDES
Explanations on the Ephemetides
Ephemerides of the Sun and the Moon
Planets
Card 2,6
5
7
;:,*6
40

Astronomical Calendar, 1960
SOV/3651
Eclipses 66
Opcultations of Stars and Planets by the Moon 90
Physical Coordinates of Sun, Moon, Mars, and Jupiter 103
4tellites of Jupiter 112
Satellites of Saturn
Comats
134
135
Minor Planets 136
Variable Stars
On the Observation of Polaris
137
148
Card 3/6

Astronomical Calendar, 196o SOV/3653-
On-the Computation of Coordinates of Stars 158
PART II. APPENDIXES
Developments in Astronomy in 1958 .162
Shcherbina-S&moylova, I.S. The.Sun 162
'Dokuchayeva,O.D. The Stars and Nebulae 180
Bronshten, V.A. The Moon and the Planets 205
Bronshten, V.A. The Comets 218
Arsen~1yevi-V,V. The Firat,-!Soviet Sg6aq Rocket 220
The 10th Congress of the International Astronokic Association 237
Card 4/6

Astronomical Calendar, 1960 SOV3 6 51
Frank-Kamenetskiy, D.A. Discussion on the Origin of Elements 237
Leykin, G.A. Symposium on the Herzsprung-Russel Diagram 240
Shcheglov, P.V. Electron Telescopes 247
Bton8hteh,3.A.~~i The~ Fifth Asbeih~iy. of ',the Speblal.-Committbe on the Intibrr-`
national Geophysical Year 252
Masevich, A.G. Visit to Observatories in the United States 262
Semakin, N.K. The People's Observatory of the Plant imeni Likhachev 284
Sakharovskiy, L.T. "Eternal" Calendar with TILble of Lunar Phases 292
Perell, Y~i.G- 350th Anniversary of Galileo's Discoveries With the Tele-
scope 308
Card 5/6

Astronomical Calendar, 1960 SOV/3651
Perell, Yu.G. Anniversaries in Soviet and World Astronomy in 1960 313
Bibliography (compiled by Yu.G. Perell) 330
AVAILABLE: Library of Congress
Card 6/6 TM/lsb
6-23-60

30)
AUTHOR: Dokuohayeva,0,-D. SOV/33-36-3-10/29
- --------------------
TITLE: Determination of the Mass of the Orion Nebula From Photographs
in the Red Light
PERIODICAL: Astronomioheskiy zhurnal,1959,Vol 36,Nr 3,Pp 461-467 (USSR)
ABSTRACT: The paper contains an estimation of the radiation E nx 0 f the
Orion nebula in Hcin ergs/cm 2 see in a unit solid angle. Four
photographs of the nebula (with red filter) were used which were
taken by the author in 1954 in GAISh with a 25-cm telescope and
by G.A.Manova in 1955 in the Astrophysical Observatory AS Xaz.
SSR with a 50-0M telescope. The calculations are carried out for
the concentric domains of the nebula (extent: 55,',,2601,and 430.0-
The En7C"lues everalze& over the whole measured surfaces are:
2 -3 2
2-23-10- ,2-26-10"3 v 5-o6-io ergs/cm see. The mass = and
the mean electron densities" ni were calculatea un&er the
following assumptions : a) the nebula is spherical, b) the
nebula is flat. For a): n1 - 1-3-103 9 4-7,10 29 3-7,10 2; masses -
16, 57t 96 in solar unities. In the case b) the masses are 1.5-2
Card 1/2 times smaller. The results show a good agreement with the data

Determination of the Mass of the Orion Nebula SOV133-36-3-10129
From Photographs in the Red Ligot
of other observers. The author mentions G.A.Shayn, V.F.Gaze,
V.A.Ambartsumyan, P.P.Parenago, S.B.Pikellner, A.A.Nikitin. The
author thanks Professor B.A.Vorontsov-Vellyaminov, Academician
V.G.Fesenkovt D.A.Rozhkovskiy, and Z.V.Koryagina.
There are 16 references, 10 of which are Soviet, 1 English,
I French, and. 4 American.
ASSOCIATION:Gosudarstvennyy astronomicheskiy institut imeni P.K.Shternberga
(State Astronomical Institute imeni P.K.Shternberg)
SUBMITTED: June 17, 1958
Card 2/2

DOWGUYNTA, O.D.
A presumed variable star iu the Pleiades. Astron.tsir.
U0,200313 * 159* (MIRA 1332)
1, Gosudaretvanz.V "tronomicheakiy institut im. PA.
Shternberga, Moskva iStars, Variable)