SCIENTIFIC ABSTRACT MONIN, A. S. - MONIN, I. F.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001135110019-9
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: March 13, 2001
• Sequence Number: 19
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

SOV/4-') -5,9-10-11/15
Q,;V~~ Cr 74val t -.n ClIart-cturiGI. "'T At-l-iti-
1 i C ,, I " f f ft; t, f -, 't 0 1. ua o f tg, ~ e o D n o n& T.Ic!:-,c
charac tf~r F,, NAll on
?r u + V
e
ZAXICI. 11%1:3 th'~ id-m of the avurz;Lsad kizlf~tic ener,711 1.)f L:,.Lc
unlu M;In7, J., )-Z3') and tl-2e
definiti)n of E' i;,,G.(5) ~tad (6).reault (the zecond is
the ener,-_V b,-IaTic+-- for tHr-- Sev-
cral arc nw; nide. Fir.;t tlv~ ri;"Iit hand
,qilep- of )rc conssider,--.
t
au
Tiii~rdt tlll~ei field ol tliu- --,ul 3- 'u ions
ul und V I L, c.~n3ifl,~rad t.-o b-~~ i6utro,-.i,,. Uf,-Inr.- theoe
upi,roximatl5no (T), (5) and (6) c-in bt? rawritten in the
Card 3/4

%e Am-oal4ulaUm W Z-.mal (4irculnt.i~)a Ch,iract,~rir,,tic5 )f th,~. itni"(1-
(7) Tar, pre6.,iurc- in the macroc,)-,-),)nmt can be found
frcri can be used for tl,,,-- -,tate
of tti:~ for a pr,)IonL;cd period. There are no
figur,3s and 2 ref,.,rmces; 1 of the referencer, is Swiet and
I ia Enzlirh.
L3.101"U'llION: k_-a_e.,Aj-, ntauk. 3jjR, InstiLut fizi'-.i at,io~;fery
(Aeade:~.f -)f Sclences, U&'33R,, ln.,-titate -)f At~"),3-hcric
iUb!.lJTZi;D:
CeLrd 4/4

""GV/ 49-58-11-9/1&
AUTIHORS.: yggjaL A. S. and Obukhov, k. 'U.
TITTA: awl I Amplitude Atwor-pharic Veriations ejA AdapUtion of Meteorologic&l
FieUU, (Ikalyye kolebanlya ataostery i acaptatciya
aeteorologicheskikh poley)
FERIODICAL: Izvestiya Akedenii Kauk SSSR, seriya, Geofizichaskaya,
1958, Nr 11, pp 1360-1573 (USSR)
ABSMC-LI: The movements of the air masses can be classified as
slow (synoptic) and fact (waves). Tbo fact processes
havinf, a small. amplitude possess a character of short
waves.. Thereltore, in order to deter:aine the Gtatic and
Keostrophic properties, a problea of chort waves in the
atmosphere Fhould be solved. The fast movements oriGinate
when cnequilibriu= of static and geostrophic conditions
are disturbed. The waves are produced which apread into
the au rzounding air massea caucin6 them to adjust their
weteorological fieldG. Therefore, in order to establieft
the general equilibri= of thLr air aasees, these vhort
waves of the fact aotion chould be determined (filtered
off). In order Lo describe the short v.Eves
A 6 it, - - is obtained. From the last three
Card 1/5 rt

5DV/ 45-58-11-9/18
Sa&U AnpUtudi Atmospherv: Taxi&#Uons &rA Adaptation of Ne-Uorological FialAs
equations of (;i) the, fins.-il exprecsions (~) are derived la
the fora raost euitable for further analysis when (10)
are included together witli the condition (11), The
equations (Q.) z~r(i ~--pplied Ju Lhe -iz:ojul6jons (12), therefore,
the parameters of j~eoetrop'L-Sic wind (1~) can be included.
The solution-,of (9) will be stable only if (14) to (16)
are catirfied. If the initial parameters (10) are not
related to (14), then the. solutionr-. (9) cran be ehown as
a sun of tho statle condi-,ion, i.e. furv~tioa 0 and
the unstable coridition tiven by (1'7). 1hereforg. th-Jr.
can be eolved b:;~, mt--an- Gf the eguation (19) and the
matrix (C"-'0) whc~a the (~qua-tion (18) is ir.troduced. The
final eoluLion, can be chowm. as (Z-'1), (2L) and (2;), The
invariant (2-5) represents the poteatial eddy (RefG I and 4.)
It should', be noted that frGM the third End fifth equations
of (9) the equation:
~b (P - c2e)
ST
is obtained which can be transformed into an invariant (24)
Card 21�'

i(7) ' ' SOT/2o-122-1-15/44
A-'r-'TORS: KGnin, A. S., 0bukhov, A. K-t Corrteponding Member,
IlVdeur-t* 9 ienceg, U93R
TITLE: The Main Types of the Notions of a Baraclinic Ataosphere in
the Field of the Coriolis Power (Oanoynyya tipy dvlzheniy
baroklinnoy atmoafery v pole sily Koriolisa)
PERIODICAL: Doklady Akademii nauk 555R, 1958, Tol 122, gr 1, PP 5a-61
(UgBR)
ABSTRACT: This paper gives a classification of the main types of the
(horizontai vortex mo-
dynamic processes In the at=osphert
i
tions, gravitation waves and acoun a waves) on the basis
of the solution of the problem of the small vibrations of
a baroclinic atmosphere for sufficiently general aaau--ptions.
In this way, the filtering activity of the quasistatic ap-
proximation may be explained. The authors first give the
system of the equations for the dynamics of the atnoaphere.
.he state of relative rest in chosen as the "main state"
of the atnonThere. Some quantities for the characterization
of the excited state of the atmosphere are then defined.
Card 1/4, Lineariting the equations of the atnoaphere dynamics (i.e.

SOV/2o-122-1-15/44
1"he Vain TyFes of the Kotione of a Baroclinic Atrasphere in the Field of
the Coriolis rower
by eliminating the square terme)f a new system of equations
Is deduced. This system (like the initial system) is of the
fifth order with renimet to time, and it describes approximate-
I.T the evolution of the perturbations. The boundary condi-
tions for the coordinate z are then given. For the solution
of the Cauchy (Koshi) problem, 5 Initial conii%lonx are ne-
ceemary. The abGve-mentioned aystem of equationshis a family
of steady solutions which depends on one arbitrary function
q, (X,Y,r) of the coordinates. TLeae ateady-stste solutionm
&r1- horizontal and have no diverganceef the forciulae of the
geoatrophic wind and the equations of atatica ray be applied
to them. The above-mentionad system of equations has an in-
variant - a function which may be linearly expressed by the
initial characteristics of the field. nle order of the system
%nd the number of the independent characteristics of the
field may be diminished by 2. The wave solutions are scatter-
ad "without leaving a trace". (If the characteristics of the
wave field in the initial instant of time are different from
Card 2/k Eero within a certain finite region, they will approach taro

SOT/2a-122-1-15/44
The Main Types of the Motions of a Baroalinic AtcosPhere in the Field of
the Coriolis Power
for t -&-oi. The initial field may be given as a sum of a
steady component and of a wave component. Tho aithors then
anaume that the initial characteriotics of the rield satis-
fy certain conditions (which are given in this paper) every-
where, with exception of a finite reeiano The various char-
acteristics may be given independently. In the course of
timer the disturbing wave is geattered and the characteristics
of the field approach the steady-state type In any finite
region. This ia the adaption process of the fields in the
atmosphere. Yor an isothermal atmospherat the colution may
be found as a superposition of the correapondirg partial
solutions of the corresponding differential eqtation. The
waves of hirher frequencies are called acoustic: waves, the
waves of lower frequencies - Cravitation waves. The adaption
of the atmosphere to the quacistatic state takos soae cinutes.
There are 5 references, 4 cf which are Soviet*
Card 3/4

NCb tho 81-41 Itr of Turbuls=~ in the Pre"we of a Mm, Vertical Tempsmturv
*Iljrtul*w* la M3*ar rlow with BtabiUtyj,*
yressute& at the iuti. symposim om rluu Y&chmniea in fhe ronmbers,
Itbaft? Virw York, 9-* JU 59
runt. of Pbpioe of the Atumphav" Moscow.

AUT=t Popov, L. r.
TrrUt rnternation&L Congrags of Geophygioiats
(Nesbduna.rodnaya Asseablej%; geofinikov)
PMOIMCALg :KeUwrologiy& L gidrologiya, 1959, Nr 4, RP 74-77 NWR)
LMTRACT t Fm JUIY' 1, 195T to Doccaber 31, 1958, investigations of our
planet were carried out by sclenti-tff of 65 countries unier the
rrogram: of the Lntem&tion&l Geophysic&l Year (IGr). The 5tIL
Congress of the Special COM:-"tt*O On the International GeophyBic&I
Year from July 29r to AuSust 9, 1958. in Mosjor was dedicated to the
execution of' these, measures. A. abort survey of this Congress iv
given. here.-The ouggestion by A. A, Zolotukhin cn a world-wide
organization of evaluations of meteorological data of the IGT in
form of synoptic daily world maps, maps of the toutbern and
northern hemispherej, and of vertical sections cf the atmosphere,
was discussed,, Tht Study Group, of VatooroloeT atzried out the
following works or, numerical method& of weather forecasts
(conducted by r. A, Mel', Corresponding Itembez- of the AS USSR),
on luzinous night clouds (conducted by Pr ofessor V. V. Sbaronor),
Card -1/5 or4 meteorology in the Antarctic (conducted by ProfAavor B. L.

rnternatiovaL Congrars of Geophysicists S0T/5a-5?-4-I!,'21
Dzerdzeyeveldy). V 0, Obukhov, Corresponding Ife2ber of the
AS USSR, and_A, ;1,'~crin (Voscow-) delivered & report, on the
theory of the &d~uatmant of'quasiatatic and quasigoostrophic
conditions in the &tmosphere for & linear case, and Pnt forward
the results of & number cf' irvestiEaticns ir, this direction.
1. A, Kibell, Corresponding Uember of tha. IZ USSIT, and T. P.
Wokov (Moscow), ruporte4 on the forecasts of teareratura =
the e&rth's surface with help of hydrodynamic matUds, and for
the first time put forward a ocherne for the: solution of the
quasi static -quasi6ostrophi c system of equations for the forecast
in consideration of the turbulent heat conductivity. N. 1.
Dulayev and G. I., K&rchuk (Moecov) put forward & new iteration
method for the solution of finite difference oquations typical
for the tasks of the numerical short-tamed foro~iast, Professor
V. 1. Tudin, (Leningrad) sug(-Iratel so%e alterations oLl the forecast
equations, thus reducing theareaof irfluenoa a=si4ored in the
forecast. He pointed out the necessity of thorou_.-:hly testing the
nethodff worked oat by many investigators (K. To. Kochin and
A. k. Dorodnitsyr) for the consideration of the influence, of the
card ?'/3 non-adiabatiz factors and of I&rie mountain ranges. 0. G. Krichak

InlArnational Congress of Coophysiciate SOV/560-53-4-19121
(USSR) delivered a report on 7The Characteristics of the
Circulation in the Ozosphere Over the Antarctic and the
Relationship of This Ciroulation With the Processes on the
Southern Hemisphere".
card W

6(-303
3.17100 SOV/49-59-:.1-1/28
MHORS: Kaylia-Borok, V. I., and *
ERinj A. S.
TITLK: Kagneto-e! last ie Waves and the Boundary of Sm*th Core
FZRIODICAL: Izvestiya Akademii nauk SSSR Seriya. geof:.'zicheakaya,
1959, Ur 11, pp, 1529-1541 (USSR5
kBSTRACT: The authors describe results of their inveetiKations of
the. dispersion,, damping, polarization, and origin of
magneto-elastic waves, The d&mpin6 of waves with an
increase of the field strength attains a certain
maximum value from wh~oh it grad&lly tends to 0. Two
types of waves can occur in a strong field: slow waves
with a velocity between the transverse and I)ngitudinal
elastic waves, and fast waves with a velocity
proportional to H An, intense mechanical vLbration
can only be causeg*by slow waves. ' The charazteristics
or the latter, being similar to longitudinal or
transverse waves, depen(I on, the direction of their
propagation and are not affected by the. initLal pulse. Th-
observed range, of velocities or seismic waves in a
stratum Dw can be explained by a linear increase of
the gradient k40 and by a decrease of uff (see table)
due to compensation by the magnetic field. rhe
existence of transverse waves in the core can be
112 explained by a. presence of the aagnetic field

1~ 6 ~ "i j
SuV1149-59 - 11 -1 /C28
Maaji~,-to-elastic Waves and the Boundary of Earth Core
urdessthero in a layer 20 to 80 km, thick at i h3 surface
with an increased resistance (to - 0.4 x IG- s~a) or 10
there is it radial field with a strength - .10 to 10
oersted. jLn increase of the pWue velocity v of
longitudinal and transverse (dashed lines) wares is
illustrated in Fig 1, where the numbers on cul,ves
denote a Equared strength of the f ield 4~- Yi(; 2 shows
the polarization of vibration in a weak field. FiiL
illustrate4s the phase velocity, of vibrationsir. a
strong ficild. Fig 4 gives the coefficients of' dampin6
with distence in a weak field whure the magnitudes of
e -K IL xw/a , e-K It xw/a deteraine damplng with a distance
x of longitudinal and transverse waves respectively.
Thanks are conveyed to G. S. Golitayn, V. A. Kalinin and
R. Khayd for their assistance. There are 4 figures, I
tabl% and. 12 references, 6 of which are Soviet and 6
Laglish.
4030CIATION: Akademiya nauk SSSR Institut; fiziki Zemli 4:Acadeay
of SciencesUSSR,' Instit~ta of Oiysicil of Sart~j)
SJB2I."IT'IL'..,,1D- March 26, 1959

5M
AUTHOR o Nonill, L. S.
-MOMWOOM
TMEo Atma4pheric Diffusion (Ltmosfernmya diffutlya)
PERrUDICALt Vapekhi fisichaskikh nauk, 1959, Tol 67, lir 1. pp 119-150
(USSO
&BSTRLCTt This article is an 'expanded version of d lecture deliver-
act by the wthar in Oxfor& (EnglaM) in August 1958 at the
Ir.tarnational Sjzposium on atmospheric diffusion and air
contamination. The author investigated all problems connected
with the distribution &M propagation of impurities of
industrial origta as well as with ralionative particles. If*
first discusses the factors influencing atmospheric diffusion
such as contamination sources, meteorological conditions, the
nature and the properties of tha impurities themselves, and
Interaction with the surface of the earth (or thnt of water).
Purthert the specific characteristic featunw,of turbulent
ditfusion are dealt witht and also the analogy between diffun-
ion Lt the field of microturbulonce and molecular 41ffusion.
Also -t samtempirical equation describing turbulent diffusion
is gi-ren; its solution is derived and discuased. The statisti-
Card 1/2 cal tr4tatment of turbulent diffusion Is further 41scussed.

Ltmospherio Diffusion
SOV/55-67-t-6/12
Moreover, the author speaks about the influence exercised by
thermel stratification of tho air upon turbulent diffusion,
which hK* keen inyoxtigatod recently by the author htmaelf an
well so by L. W. Ohukhov (Refs 16-15) and tya-feral Amertann
research workers. L further chapter of the &rticle deKle with
consideration of the finite velocity of turbulent diffusion.
rinal1r, diffusion in the macrosaopio turbulence field to
discaused (A. AG Obukhov, L. N. Kolmogorov, Refs 30,51) and
the erpected development of the theory of turbulent diffusion
It, diticuased. Lpart from those &trendy n&med, the following
$*Tie!; authors are mentioneds D. L. L&ykhtman6 V. A. Fok,
G. Shalefthorskly, S. 1. Darydow, To. S. Lyapin. and
X. D. Millionshchikov. There are 38 references, 19 of which
are Soviet.
Card 2/2

hfonin, I..
Un the 'Lh(,or:- of
~K tcorli 1r)!-n11v)-izotrornr,,v
7-)k1p,!y A17.r-!Qmii
ricuk. '533.1, 1,51), Vol. 1~;,.-,
(7, ~'2(!fn 1, -,) lntr:~f7linc,q tl,.~, n3'~ 'icn of the
': r")," I cme -i , -T ~ t n h r m n .,e r:,- i - t - r, t f n r t h,~
damlopumt; of the, theory of '-1r'iu1 ~ nt --otj,.)n!7 of n 1A,!-,14 rnd for the
dynn-min
in :-iv~vn
!.ut this fam%l~ 'tt"rr'. ot"'l- of t'.-Ic
th-~~ lonni-isotropi- not.
;-(-niratcly. 7hF-1
-.innr,~r af doduning of loc-l-irotropir
p---mitn f, 7or- of the
renult-i, rrvi rtl5o th,7 fir-1w7tion, of n,!t7 Tn thri
pr-sc-it
!,ni thorc-for:~ P17o
dariotea t1vN Nftrj7! --n0,1 of
u 'ho

In tho -Aftaory of
)f ti,,e lil-,ii-! in. ni
r,uVv)r then iari n.m. uir,- n, % j. )n
IlliQne distributiom; tln not '~-rrl n-l til-
t;
of the liq,2itl pr rt iclv tlicy inv irinnt wi V7
respect to ortho~-on-tl of tho initi-il
coor(linates x, nnd -rith roin:~~,t tr) Aonc the
timoi axia. In the -present prtr,~,r, tho r uthor inv,3oti;rates
the values of v, PnA P - P Only In a fix.:!I innti-it. of ti-ic.
In this case, the nbove-mqntion;~d distributior.5 r!c n-it d~r,n~
on ti-ii. First, th, loaal-is-~trinlc fi,!~ nf tt- -:-Jo!)t';~-
u.(r) nn4 then th- 7rutual ;trw~Vir-1
.tinl prsssim~ -re investigoted. 'Alin ::~ 1w;l:
;at-na hy step. Finally Ue m.untion
.4 'r)
6Y:aL A~ A
r IE
thir, oquntlun -111th rcapoct t,)
in. r-mul,-r ttt znro) th:.!

-f I to foun 1. v denotes thc-~
FE the rat(% of d-tanInntion of th,~ -.t -' t T! 1 c 7.
struct'iral f%nittor-
0 ~IA of f i1.,:;, ,r, ! :-.r~conl or~pr. i n
'Or. ~'Oj I
57
La vqry convqninnt for thf, doductt-,n of
P,~umtions which connect the totr-actural funct,-~n
lical-tw)tropic turbulence. Ther., !,r(-
ithich nre 3oviet.
U I it%l I Cj:f fnatitut fiziki atmoctfary Akreemii nru!c fln 11,111, 1,
the Physics of the Atmosphere or the kcaicm,y of 1-illn'.
USSR)
'.:7~., ...irember 2 ',, lln)fl, by A. IN. Kolmogorov,
~;'JT.'3'4!TT.'-,:): December 1"), Ilo5,9
fl I
V7,-r 1 3/3

mcpsia., A4 0. (MOB cmw~
"Da the, Turbulent Motion In a Gravitational Field of Honconstaat Te=pemtjre,"
report presentect at the First AU-Union Congress on Theoretical aryl Appliea
Aechani,.-s, Moacow, 27 -Tan - 3 Feb 1960.

90111, A.S.; OBUXHDV, A.K.
Principal types of nations of a baroclin.10 atmosphere in the f LGIA
of ute Corialit fare*,,- abetract. Ulcproblez4teor. u3.l:Z7 t6O.
CHIRL L3:8)
(Atmosphere)

S/049/60/000/01/024/0.'!7
920119191
AUTHORSt KazanskiZ:, L.B , and Moninp, A.S.
TITLIt Turbulence Lbove the--Eowest Layer F the &fAoRnhQa-YV
PERIODICLL.t Izvestiya. kkademii nauk SSSR., Beriya geofizicheskayat
196oj~ mo it pp 165-168
TIM The &uthors discuss the stitionary turbulence in the
lower layers of the atmosphere, assuming uniformityalong the
horizontal direction. Theproblem. was to find the distri'Jution wilt-h
height of the wind velocity componentaq temperature a,)d s,)ma.
characteristics of turbulence, especially the turbulence L'mixing)
coeffiUient K. The analysio.was based on the experimental material
obtaiaed by an American &arophysical expedition in. 1953- reported in
& book by Lettau. and David-son (Ref 3). IrL spite of the very careful
organization of measuremorkto during this expedition, indiTidual
results were, not very, reliable. Gonsequently the authors limit
themselves to several typical cases (Figs, 1-2), Among, the results
reported are the following conclusionst 1) Coriolis forces reduce
the turbulence (mixing) coefficient, i.e. they tend to stibilize
turbulence; and 2) under turbulent conditions the changes of the
wind direction in the lowest hundred metres of the atmosphere amount
Card 1/2 V/

5/049/60/000/01/024/027
9201/1191
Turbulence Above the Lowext Layer of the Ltmosphero
to only asyeral degree&.
Thor* are 2 figures, 1 table and 6 reforenoest Soviet and
1 English.
"socu=Offt Aktdemiya nauk.BSSRI rastitut fiziki ttmosfery
(institute -of Physics of the Umosphers, Academy of
aciences uum,
SUBMITTED.- may 8 1 19~59
Card V2

I C 41--- 2 C' I
VR: 1~onino A. S.
TiTLZ: LaCran-lan chsracteristic3 Df turbulence
.-MODMU: Doklady Akmde::Ai nauk SSS2, v. 154, no. 2, 1,60,
In tLe introduction, the author explains wh. '!~O f,;,-,ct4 ;n-
enterin,; into ecLuation
ztnj~ YJ T(n' M, (41M1),
for the velocity ot liquid particle3 in t-arbulent diffunon c~a-,
a: ra-.dor, fuacticna: the,,,, are statistically stable. it is t-,,n
Taylor (Przc. Lard. 1!ath. Sao., 20, 1 6 (1021) was the firct. ~.o t 7 U C,--
La-ran-r-iQn c~mracteriatic3 of small-acale turc%i!cnc-z into
fOMU1L-. to ex:)reas the dioperrsicn of llquld -~-,rtial
L&L-.rani:1an velocity correlation fur.,:tlona. Lz , ho-me" Or , zn a kl~: 01
caaes atm,:iapheric turbuloace cmnnet Le re-arle! as & a-za.1*-sc:al-~, t - r,
oal;~ local hydrodynamic characteristics be rei.;arde! as
0 1/4

characteriaticc
stable. T he author introduce
h
s 6
.e inertial S wh"*
h
c
Ocit~'
;
T'e coo
d
r
, ,
-,
inates of thi- SYstem
are
y x - x
-,
,-
v
- t - t
.
,
o
0
0. These relative coordinat
ez arc-,
1 and 7 be Sufficientl
y
IC3
f 10-4 -In the atudy of Probability 1'str!but'
I
*~
r c f
A 0:1 Of
I
'O CC
t is asaurned, in accor, 4anc-2
n)- 4, (1,D41)), thMt i'l th
e ca
sc- of
t depend on t
, x & ei v
0 0 but cnl~' c,-,
t!
t ;rb-ulenc
~
e c
nercy, ani th.e kine=atlc visconit
y.
f (Y. V. v I YO (Y
V
r
V
) (
d
'
'
.
Ys,
v
t
f, (vA i YO
(5)
(YO Y1. Vj T
-
(y
o
Y1
y1r, V - Vt. Z)
*
-
a
e --
:1vent for the probability 1istr1l
I
ution aril th
1 rcb
a
tieze oo~?rdjnatec
(6
.
.
) chows t!-e invariance of v-0
tOn "Uth r
esi~ect to Galilean trar
r
a
- C
t(, use the abovemention
d
e
refere-ce -r t
etc-~~ S
bu
a
, ,
zt e.", S.
uh c h
M
,
,
0 v e z a 2 3 r.,- vr j t h c (3 -. "'ain liqu4d -, icl
'- 1
art
C:
rd 2/
~
r
-00. 1 n t 1.
4

characteristlcZ Bic-4 32C1
th? lo~!al ta~,-rar.Clcn character--'-.t,-~.., a-.,i tho
rticle: ir. the :;yste= S~). !~'Pre, are the ~uc,. t
(t + 't t +
0 a 0 0 0
,uld ra rt i ~c I e sIn 32with cufficion'l., ar. 1
of local isc-tropy, the
probability, dens- f;)r 6T - T(I
~'Qr 1 1, the dependence of (15) on 'v ir, nep_-I"Cible, an-d thi!; ri~' t,,~~ can
lie represented In the form
(6 f, v 11.) . (a,['6
Y-14Q, (Liatll. - 1) - (14)
C ve,
In 4b',,e last geation, the author (;iviz a differential eq-.,m*4.an
Card 3/4

S/020/6C/l 3,j1CO 21C r '/,C2
.LiCranCia,n characteristics ...
+ 0.
tLat describes the Impurity transfer by moved :,articles in an lnc~_-T re:zi-Cle
1'.'quid. UsinG a fixed initial distribution, he obtains
S (X, t) p (X. t I X4, (a) so (KC) dX4,
fcr the -volume concentration. This intecral foms the baois of V..C th~cr:j
of turbulent diffusion. For-mula
z (Y. T) M j p (yl r i VI) so (yt) dyl.
c, rrecraondln,.~ to ( 17) Is derived for the relative dlffuoi cn in t, c r-l'.
S, stem S air~lllar for.-.iila bold.- for
ere ar~, 5 references: 2 Soviet-bloc and 3 non-Scviet-bicc.
nUSCOLT"I 10'7: Inatitut '.izi;.i atzosfory AlKadenil n,~u% SSS? (Tnctit-itc: :f
?hyaics of the Atnosphere, Acr~demy of
ZD jl.)ril 7, 10,60, by A. N. Fol-mocorcv,
jU'F'1TTED: APril 7. vU
rd

Empirical dat3 on turbuleace Ir. the surface laxer of' the atmoa2here.
report ffubmitted for tba Intl. Symposium on FwAawftal Problem in
Turlbulence wA their relatiom to geophysics, IUCG wA IUM, HarseillAff,,
rrRnce, 4-9 Sept 1961.

Preogrure variations in a compressible stmospbers. rzy. Alf 55S.R.
Ser. geofix,.no*4:602-612 Ap 161. OIDA 14-- 3
(Amoophoric prossure
(We&ther foi

KOARSKIT, A*B.vw MONIN, k.S.
DInamic interaction otthe atmosphere and, t" earth's surface.
Izv.AK SM.ftr.g9:TIz. no.5:786-7E* PV 161. (KIRA 14t4)
1. Akadealya, nauk SWI, Inatitut fizi-ki at-tosfery.
(Atmospheric turbulence.) (Friction)

Swe chamt-Tictics -r c;-mi scattirire in a turx-lent
atrow.-h-cm, Akust, z4ur. I ro.4:457-,.1+63- 161. 14:10)
Tnvtitut. ct-,c,3r r:.- 1,011-ma.
(.*.*--..:.- 1,,,-ric turLrulenco)
(cic-,md)

AMIRI ks.
Ttwbulonce "atr= in a tb4rmiLUy inhamogeneous atwophere.
rar, AX SM. Ser, goofis, aa-30974W Kr 162. (KIRk 15W
1, AN SM, Inatitut fisiki ttmoofory.,
(A.twephoric: turbulence)

MONIS. A. S.
We of u=ellabIs forecaste, rimAK SWR.Ser.geofix. ua,2tZlS-
228; LF t62, (MIRL 15t2)
lo Lwtitut fftiki &tmoafery AN SWL
(W"ther forecaatimgl

MWARINOV, A.Ye. I FLIMMMU, B.30 t .Y It., A~S., dolctor fit.mat. mmkf
- ZUBAKOVO V.D.I kand. takhn. nauk, retsenzent,,
re tsensent,
IVANUSBOt N.D.0, red.; SNZSHMOVt A.L., tekhn. red.
[Kethods of &WAstical oequential analynis ancl their applic-4ttion
in. radio engineering] Mstoclq OAtistichaskogo posledovatellnoga ana,-
liza. L ikhradiotekhnichaskie prilozhaniia. Yoakva, Imd-va 'Sovet-
sko4 redio,2 1962. 352 P. (YIU 15z6)
(Hat6matical statistics) (Radio engineering)

S/506/62/000/004/001/001
9032/F,314
AUTHQUI HuninA_Ax*S,,-
TITt,Et On the r4tructure of' the wind velocity and temperature
fields in the near-ground Layer or air
501A(C~F, Akademiya nauk SSSR. Institut Ciziki atmonfery. Trudy.
n0d 4. t962. Atmosrernaya turbuLentnostl- 5 - 20
TEAT: This in a review paper concerned with existinK theoreti-
cal. and emptricaL data on the structure of these fields. Particu-
lar attention is paid to those quantities which can be measured
directly. The subject matter to considered under the following
headings: 1) definition of the near-ground Layer; 2) pamnible
moanttremetit P 13) stability of average vaLtses-, It ) xtructurat
charneterinticx; %I rrozen-in turbtilence, 6) turbttLence
spectrum.; 7) similarity theory for atmospKaric turbutence-,
8) similarity theory for the nenr-ground layer of air; 9) stmi-
larity of mean pro t'i t ex; 10 determination of the "external
parameters" v and q or ttio nimilarity theory for the near-
grotind layer- 11 simtlarity of Inilmations; 12) similarity or
time f4pectra; 13) similnrity theory for the inertial spectrum
4ntarval and t4) strticttirat and spectral. functions in the
ar 10-

S/506/62/000/00/ool/oo5
On the qtructure of' w.3 z/ ~.5 14
inertial. interval. The near-ground layer is defined as extending
to a height of a Few ten% of metres above the Earth surUace in
which the Coriolix force can lie neglected and the followinr,
condition-4 are inntislArd- a) the local tc-rrain im planc, nnd tho
tinderlyinq --turt".%ce, i.- sufficiently homoXeneoun so that the wind
veloctty nnd temriernttire fields are -4tatintically uniform in the V
horizontal direction and b) there are no sudden changes in weather
,o that the wind velocity and temperature fields are statistically
time-tnderendent wittrin time intervals in which the natural diurnal
variation in the weather is not very itoticeable. The statistical,
characteristice of meteorological. fieldm are then Independent of
horizontal coordinates of time and nre
functions or the height z anLy. Most at' tne Int'orntation revLowed
is theoretical but no sj)ecific references are quoted.
Card -'1/2

MKIN, A.S.
Use Of etatiatical methods in weather forecasting. Meteor. L
cidrol. no.70-10 JI 162, (MrRA 15t6)
(StAtiatical weather forecasting)

ay, Y30
11, 1
3 _,04 2
S/040/62/026/002/014/025
D299/D301.
AUTHOR: Uonint A*So 01[oscovf)
TITLE: On the LaGrangian equations in incompressible viscous
fluid hydrodynamics
YzRIODICAM Prikladnaya matematika I mekhanikat vo 26p no. 20
1962t 320 - 327
TEXT: The Lagranglan equations for an incompressible fluid are de-
rived In a form which Is free of the shortcominas of W.J. Piereonla
formulation (see references); Pierson's method leads to a disturbaza-
ce of the continuity conditions. The Lagrangian formulation is par-
ticularly suitable ror the statistical desqripvion of turbulent mo-
tions@ After tranarorrzationar one obtains the oo=plete syste= of
equations in Lagrangian variables:
I v:2 r
5 f > 0 >!7 (1-5)
C
I+ V UV. V. IV, V-41/0411 +1VIE" (VI Ell at1/dt7iT-s
and V. P %P (1-8)
Card 1/4 + [Ell V. Ml. V. at~ latil) ---------

3/040/62/026/002/014/025
On the Lagrangian equations in ... D299/D301
The Lagranglan form of equations ia compared with the Havier-Stokes
equations; thust the viacous forces are described (in the LaGran-
giarx equations) by nonlinear terms of the 5-th order in tip whereas
in the Navier-Stokes equations the inertial forces are described by
second 'order terms (in ui). Some particular cases are considered,
which the Lagran ian equations are simplified, (plane flow and
plane-parallel flow5. For the complzte statistical description of
turbulance# Ea Kopf's method is usad (Re-'* 9: Statistical hydrome-
c'ia.nics and functional calculusp J. Rat. Mech. Anal.g 1952t 1, 87).
Ihis method has the advantage of reducing the problcm to the solu-
tion of linear equations* Furtherr the Lagrangian equations are de-
rived in covariant form. Therebyt the unknown functions are the
contravariant velocity componentsc
L 6-,, axi 84 M 614
. -, W V _. (3-1)
0t F~; 't, Ut 8XIX
The continuity equation anrl- the equations of motion are
Card 2/4
0
6-4)

S/040/62/026/002/014/025
On the La&rangian equations in D299/D301
and dvi I i ia ap
0t + v 71 Ix v 9 ail,+ j?0v (3-5)
where the last term contains the
(3.5) aro used to describe small
its atate of rest. The quantities
(3-5) are linearizedg yielding
dvi 6P +
0t . I
ox
velocity Laplacian. ::'qG. (3-4) a--,d
flyetuations, of the fluid abouto
v are considered s=all,, and
).!~,vi.
(3-6)
advantace of the above method of lineariz..tion (as conplared to
eierson's nethod), consists in the fact that It does not becoi,,,c ne-
cesa-ry to linearize Zqe (3.1)t whan using Zqs. (3.4) and (3-6);
r.ence the continuity equation remains exact. There are 9 references:
3 Soviet-bloo and 6 non-Soviet-bloc. The 4 most recent references
to the Lnglish-language publications read as follo-as: G.K. 3atche-
lor* U=all-acale variation of convected quantities lil,e temperatuZe
in turbulent fluid. Part I.# J. of Fluid Reche 1959t 1.10. 5P Pe lt
113; GaKe Batchelorp I.D. llivells,, A.A6 Townsend,, Small-scale varia-~
Card 3/4-

S/040/62/026/002/014/025
On the Lagrangian equations In D299/D301
tion of convected quantitieG like te=perature in turbulent -rluid#
Part II.0 Jo of I'luid, P:ech., 1959, v. 5t p. 1, 134; G.K. 3atchelor,
The effect of hocoi;eneous turbulence on material li.nea and surfaces
Proc. Roye Soc. A.# 1952, 213, 349; 19.J. Pierson, On the transfor-
m-.tion of the Navier-Stokes equations into Lagrangia_n form with se-
lected linear solutions, Rep. at the Intern. Symposium on turbulen-
ce# JUGG and IYUJ4, 1961, Sept. L'arseille.
Aj:;001A,TI0&1%': Institut fiziki at=osfery AN SSSR (Institute of Phycies
of the Atmosphere of the AS USSR)
SMUTTED: December 22, 1961
Card 4/4

M011111, A. 8., and TSVANG, L. R.,
"Oil ntructure of turbulence in the law trapospheree"
Repart, bo be submitted for the 13tt, Gener&L Azaembly, Intl. Union of' Oeodesy
and Geophysics (IUM), Berkeley Calif., 1-9-3i. Aug 63

MMKO &.5.
P*eical mchanisa of the long-razWe %mather chaMas. )htaor.i
gidrol, no,8t43-46 Ag 163, (ta?-( 16 c 10)
1. Institut fitiki atmaerery AN SSSR.

TAGWK, A.M.
Laws governing small-size turbulent actions of liquids and geseff.
Usp. mat. nauk 19 no.503-114 S-0 163. (MIRA, 16t121

7
mn,,frg, A,S,
. Clizatologr of' ~aat balance.
S-0 163.
law. AM S.M. Ser. geog. na.505-110
(WLRk 16tU))

P d ~A &j~N
A.a. (noncow)
""!srn probl=z of the VI-Aeory of turtraknce".
re-Ort. presented at the 2nd kll-Union Congress on Theoritical und Applied
Sechanics,, Moscow,, 29 -tan - 5 Fab 64.

ACC9$SrCff 10ts AKM590 8/0040/64/(eO/002/0319/0325
AUTHORs Xoning, A. S. _10now)
TITTZI Solution *f a turbulence problem by the wthod of perturtwtion theory
SOURCII Priklodnik" retemattka L riakhanikap v# 28, no, 2, IMP .`119-325
TOPIC TAM t turbulence, perturbation- theoryp turbulent motionf wtmdoa, foroo,
characteristic faitationalt velocity fields scalar product, mathmitical expectation#
probability distribution., Fourier transforia.
ABSTRAM The author uses the characteristic functional descriptt-on. of the
statistical properties of turbulent wtion of an Incompressible -rAuid,, The random
fiWA of exterior forces is assuined-given and statistically-etatiOD117 in timel to
it corresponds a statisticslly~-stationary velocity field* The dwactoriatic
fww--tioml.& of thass two fields will be the soluUou of
D'
+ hit M
VO) to . I
(w k. AeD, Oe. 8) DM'(k - k" 9) A
C.d

ACICESSICK XRt AP4027590
wharom is the Vi$QWUrVftffI9Untp DS (kjt.) and, D (k*t) art operators of
gj
'variational differontlation Ia aj(kot)-and gj(k9t), and-wherv repeated indices
'denote sussmation,, sub4iect to the condition
A (0; g.(k. t)1 G Ig (2)
uhare G is the given characteristic functional of the field of exterior forces*
Finding of such a solution makes it possible to Riv a complete statistical
description of stationary turbulence* 34uation Zl)'Gis solved by the method of the
theorjr of perturbationse As the field of exterior forcess the author uss a
solenoidal, Gaussian, stationax7p homogeneous, and isotropic random field vith ser*
oxpoctation, Orige artt bass 4 ficures and 23 formulas.
ASSOCIATIONt institut fisiii stwerery* Ax swit (rostituts or "ics of, the
Atr.osphernj AN SWR)
SUBIMMEDj OqD*c63 DATZ ACQt 28Apr64 JXCLs 00
SUB 06M M, Al NO a" SOVS 000 t 003
card

4L
ACCPSIM Mt AP403WoU SIbOkPIG4WCOO3IO3P~
qAVMIOt KaUsedahj; X4, 161 Want A* &*,I, 1*0016ars, 0. To
TI=t The three Unetwional struaturs, of & radiation f LeM at a vouraw of
astoorolao"L information
WMXt AN =4 Isre 3srs pofixes) no* It 1964s, 39444T
'TOM TAWt artificial satellite#, weatbw forecastiagg, radiation fi*M,, tropo'.
i *pherv. *tratospbwa
:AWMCTt The authorff, MY* poDAed out the, Jxport4m# of world-wide ~beerv-stic=
Jn order to, make satisfactory weather predictionst arA they have found the use, of
,artificial satellites for collecting meteorological. data to offer both econovT
geographic distribrution. of observational. point# e, But, though the) amount. and
universalitr of the, information is increased, tbel type: of' information Liff, qualitse-
'ti.vsIr altered, The sing!* source of infLormation (for thaL !war layvre of' the)
I
atmospherig-4he troposphere &i4 stratosphere) is electrical radiatica of variow,
,wavelengtho reflected or, asitted b7 the earthts slOrfe" " tha surrounding atno-
!apheret S##v*UU.T this, yroblem, becomes a, matter, of spectral anslpix of radiak4lon
card

ACCmiou HRi ApImMi
1
~bein& lost by the planqt, The authors describe the connection between structure Of
:& radiatiom field and wtsorologiagl and other processes that have acme effect on
the radiatioc- field,, They describe the inhomogonsitiog of various scales in the
radiation Cield andL outline, the,, ptWsizal origin of th*s* inhomogensitias as wall so,
the contribution they make in the recorded stream. of radistiono They propose a
method for computing atmospheric distortioa when recording the, structure of the)
'underlAng suface,, and they Aso, furnish definite; roootaxendati.7na, for a method of
lobserving the radiation field from &rtificia.L eatellitewt This involves prLnoip&Uy*
a hamispherioal receiver turned toward the earth azA a device VUIx the proper solid
;angle or viewe Origw. arte, hast 5 figures and 16, foradaa.,
'A=IkTMKt Akademiya, nauk WSR Institut, Mild &Uwsfwy* (AaadeV of Saimices
SSMf Instituto of Pbrai"', of the ItAospbars))
t 2Wun63 DATS, ACQt 2YApr,64, EML t 001
KO) W, Myt 007 t M

V.J:4F otv. rod.; XULLIONZ;HCHKOV, M.D.,, ftktwe;41k,, red.;
bWrXII;, red.; B1,OK.HWTZV, D.I.,, red.; GRELIENKO,
B.V.,, ekade.-Jk, red.; WYCHROV, V.N., rt-d.; KELM511, M.V.f
0-ader-R. red.; KERILLIAL, V.A.. akademik, red.;
V.V.,, red.; Andrgy,gargayovich,, prof., doktor fiz.-
matem. nauk, red. (1W1); NMEMIM, AX.,, akademik, red.;
PARINg V.V.,, red.; 1F.A., OrAdernlk, red.; SEMOV,
N.N.v akademik, red.; YOK, V.A.p akademiko red.; EM-ISUVO
G.F.j, akademik# red.; ENGELIGWAUT, V.A.,, akademik,, red.;
KRMIEVA, G., red.; BALAZIN)VA, A., redv; BERG,A.1. $akademike red.
[Science and mar.~ind, 19(v.; simple and precioe information
nbout the principal develoFmuntr in world cciencel 1,muka i
cholovechostvop 1964.1 dostulno I toctmo o glavnom v m1ro-
vol nauke. Yaskva, 1zd-vo "Znanle,O 19(W.. 424 p.
(MIRA lstl)
1. Deystvitellrqy chlen AION S.ST. (for Dlokh1n,4FAr1iTM;, Chlen-
korrespondent AIN' SSSP. (for Blo?htntsev). 3. Akai(mmiya nauk
SSSR Ukr*aj (far Gnedenko).

T_
r
&P 50c, 05
A t4
OF: emw pl, oprT th
TAn" 14 orf-111--ace
r, u r
!41.vnn vc
~.,ulfomdty; 3) boti7oncal
-ttt PAIO-Xticnir a K. %I

17

av~rv or,
R -113 C C!'D F

MI(Iff. K'S.
ffonunlform t-mperature conditions In the &tv,,o3-,h#,r1c t)nwomry
layer. 1tv. AN SSSR. Fiz. ntr-. I okpann 1 no.5:49f'-500
Py 16 5. (KIPA 19:8)
1. Instit-it fi,-iki atmv,sfory AN SS.M.

All t f.,
ki k, e
min, ra t t i r P,
FVT.-""
FC7 var !I,. t

Af, rva, j -n thel 3~--.jcyrf t r -t
j, it1 1,1 i I q
T 1
Ll" t z ik i a tr.~~ 1, - A~idlc .10 it f ik T eif thp,
n s~
Atlv~4;4,o rp , A , i

f i
ACC
AP6010839 SOURCE COM UP/0421/66/000/001/0037/0043
Al;'AHOM Monin, At S.CtAo%ow) 4'
'iORG: none,
ITLE: Turbulent heat transfer in a field of Arobimadea forces
OURCEr AN 333R, Izveatiya, Madhanika zh1dkosti i gaza,, no, 1g 1966#
337-43
~
TOPIC TAGSt turbulent heat transfart Archimedes foraet gea flow
ABSTHACTt The artialft analyzea the dependence or the pulsations or the
temperature and or thaturbulant hGat rlux on the nature or the
stratification or a gas located in a field of'Archimades forces , It bad
been established earlier that in a gas there is not only a temperature
stratification 9 (z), but also, a velocity profile u(s).,, The article)
starts with a mathematical consideration of the stability of the
stratification of a gas, The mathematical treatment is based on the
following expressiont
here Ri. Is. the Richardson numberg g is the force of gravityl, and e, is
card

34-
L 297 46
ACC N" AP601-0839
'the so-called potential temperature. It then proceeds to consider
Itempersture) pulsations with neutral stratification and the conneetion
'between turbulent heat riux and tho temperature gradient, The article
concludes, with alengthy reviev of the work of other author& In this
1rield (referred to the bibliogrsphy)# Orig, art, heat 8 formulae and
tavle,
SUB GODEt .20/ SUBM DATEt 04Nbv65/ ORIG REFt 01,~/ vcK REVt 006,

29270." -Mrr~ljj~Lx, (20
ACC Nt, APWI9345 SWRCR CODE:
AUTHM koltenikovaj Ve #1 V
of t4e AtVa efery
_phere.AX MR-(Institut f1siki-atso
AN =R1
TITIAs Uar-,to-"ar variability of meteOrOI-291cgl elements
3CUMt -AN SM. Isvestiya. Mika atmoofery i okeana, v. :1, no. 2. 1966v 113-120
TOPiC TAGSt atrios
-pheric temperature# atmospheric thermodynamles
AMTRAM The authors formilate the problem of comWison of the intra-az~,
*r=&I, 3iw-to-yeaw arA secuinr variability of meteorological alwientst
.It is ;Ovtulated Mat for most of the weather elements the relation
~between theme forms of variabi1ity is apprwdmately identical. Ey the
_ana1Y8i8 of factual data it is demonstrated that the ratio of theL year-
to-year to intra,-umual variabilit7 in the radiant heat flux at the
euthwai mwfacs is aporoximateV. equal to the eimilar ratio for tempera
'ait.- hast 4 fi~-sev 3 formulas'''and 1 table, [C M91
G IMF: 004 M REF: 001
SUB COM, 04 SUEN DLTEI 'L7Sep65 ORI
C."

,A
L CW,186t~..Z I ---SLr-T-
ACC NRv fj A 6i,'dd766i16W6fij76ii6i
SOURCE COD
AUTHOR-- Koleanikovx, V. Ni nnfn- A- M-
ORG: Institute of Physies of the Atm
Slphere, AcadeME of Sclenoogr WSR (Akademiya na
%SR InstItut TiziM atinoafery)
TITLE: The year-to-year var,,abUity of meteorological elements
SOURCE: AN SWR. Izvestlya, Mika atmogfery I okcana, v. 2, no. 2, 1966. 113-IZO
TOPIC TAGS: meteorologic observation. meteorology, variation. periodic function
ABSTRACT: The authors, while studying the time variations of meteorological elements
(temperature, wind velocity, pressure, cloudiness, etc.). discovered in ibem components
with it great variety of periods, from fractions of a second to tens of millenta. The entire
spectrum of fluctuation periods Is arbitrarily divided into nine classes. On the basta; of an
analysis of those periods , the authors 11ormulate tho problem of comparing the month-to-
month, year-to-year, and secular variability of meteorological elements. A hypothesis pro-
posed states that for a majority of vmather elements the relationship between the types of
variability to approximately identical. It is. shown, by means of proocouing real dAta4 that
I Z UDC: 561.606.3-651.683,

L 061RE-~c5-45"T
ACC NRs AP6019510
0
the rolationship of the; nionth-to-month, and year-to-year variability in a radiation beat flux
at the, surface of the Earth, Ig appro)dmately equal to the corresponding relationship for tem-
perature. . Orig. ext. has: 1 table rnd 4 figures.
SUB CODE: 08/ SUBM DATE: 17SeP66/ ORIG REF-. 004/ , OTH REF: OOL
2/2

AC1- N;,k~ At,7()~54;60
(Doctor of p:Vuiconathomtical (;0ionc-0a)
C.".3t nona
,Ar,L;c Roaults arA prospoato of Soviet oca' m_r
ST,r,',C-P: AAN SIS2. Vestrdk, no. 3, 1966, 39-43
T
40?10 TAGS: acoanoZraphic roroarch facility. ocoanographio uh1p/Vqyoykov ocoano-
p-~apldc ship, Shokallaidy oceano(praphic ship
4iST,-NW: Tho Prosont status of 5ovict ocaano,-rap!V ir. roviawoi. 'I-* 13ad-
ing resaarch institute is; the Institute of Ocoanology., which has a staff
of about ltOOO,, including 20 doctors and 105 candidates of science. Half
worlk in Moscow$ and the others in divisions at Golandzhik, Vl,-Ld1voatok,,
and Kaliningrads Basic inyestigations in marino'physics and chemistr7
are made br the Harina Hydrophysical Institute of the AcadeV of Sciencas
UkrSSIZ. An entire research city is being constructed at Savastopolt.
Tzportr-%t wrk in ocoanologr iis done by- specialists at, Moscow,, Loningrad
and Far Eaatem Universities and at the Leningrad f4rdromoteorologicz2
Institute& Hoot reawoh vessels &re under the control of the AU-Union
Scientific Research Institute of Fiahories and Oceanographr, and its
ak and
duqhtor institutes on We AtUatic and FaclXic Oceans,, at. Hurmam
Card
3 C%3 X9-

815460
APTO
on the Black Sea, Sea of Azov and Caspian Saaa. For wca:kple, the scope
041 the Pacific Ocean division# T324-70, extends in both hemispherea, froza
'the Arctic to Antarctica* 7ha work or the State Oceanographic Instituto
and the Arctic and Antarctic Scientiric Research Inatituto is i=r,,m
:Ln the Arctic and in Antar--tica. Tae Far Eastern Hydromoteorological
Scientific Research Institute has the major vessels "Voyeykav" arA
115hokallskl,y4l. -the Vdnistry of the 121fary makes no oceanographic atudica
of its o~wn, depending on the, other agencies. Some of the prolilems of
ocewiagraphic research aramentioned,, and a few details am given coa-
ceraing Individual agoneies and activities,, but the) article does not-,
juatiry tho general title given it; tho article is too briar to give
any ovorall. picture of tho status of oceanograp~q in, the USSRO, 41 might
rather b# aaUed.aa 'lint roduction!t to.thia. topi*$, fm-ast 3?. 0
SUB CCDZt 06 1 sm DAM c none

ACC Wit
SOUCE CODE't UR!0Z13t66f006!0061L093111099
AUTHORt tbntnl A. Sot Bogorvvt Y. Go
ORG t none
%ITLZ.p Wentleth annivarsary of the Institute of Oceanology of the 4CAdomy
of sciances MS!t
SOUR~& OkeanoloSlyas Yo 6w not 6t 1966w 1093-1099
TOPIC TAWt eeewwgraphy, easowgraphic research 9settleys oceanographEn
personneL
SUB, coolt 08
ABSTRAM
The article cited below Is an, extensive wmcizrizatlon of'the
work of the 1hatitute of oce=oloey during the last Wenty yezra, the
most important, permaUties Wi* havo, participated in its activities,
a progressive year-by-year accoant, of the broadening or its fteld of
operations, its cooperation with. other agencies# its participation in
International pro&r=3,,, its wrpeditions and research vessels end the
-outstL-iding advances it. has contributed in the'field of,oceanolazT.
.Or particular interest is L ligting of all the institutets. e*editions,
th.40-4tas, ~hevesseU,ueeds t4e reopn~- involved &rA the- nr_--e of
UDct 00~,16051.46'
.7 y
ly.

ACC NR-, A.P7013695
,the chief or the expedition. 'The specialistsof the institute have
Iproduced more than 2A00 articles and 60 bookso. Thi transactlons of
..the institute now constitute 80 volumes, Its msociatos have defended
10 dDOtoral dissertations and 16 candidate's dissertations,, "Ino Fresont,
director Is Andray Sorgeyevich H=in. 7here are two branches; - the
Pacific Ocean Divisions, in Vladivostok,,, and the Kalini:ngrad Divisiont
in the city of the same. name# both founded in 1961*, The institute has.
& new, laboratory in Moscow,, has recently obtained the 6,800-ton rescarch,
vessel "Akademik Kurchatov"# and is sche&1ed. to receive &.muabar- v:
research vissols in the 09ming years.#.' Orig. art.. hast. L tablas
4LJFRS t 39,9ty
Cwj 2/1

Ar-C Wk-
f Monogrripft UR[
Monin, Andrey SSrgey -t, Akiva Molseyevich
Si&h; Yaglon
Statistical hydromechanics. tuvbulence mechanics (Staiisticheskaya g(dromekhanika;
mekhanika turbulentnostO pt. 1. Moscow, Izd-vol "Nauka!', 65. 063(t p. f1lus..
biblio. 7, 000 copiett printed
TOPIC TAGS: turbulent flow, laninar flow, hydrodynaaics, probability, aiail#rLtr
theory, fluid mechankcs, correlation function, Reynolds equation
PURPOSE ANM COVERAGE: This Is the first or two volumes on the theory of
turbulent flow In liquids and gases. Specifically, the authors are concerned with
the statistical properties of ense-mbles of currents characterized by macra-
scopically similar conditions. 3asic information to given on equationa In
hydromechanics and their simplest corollaries and the genesis of turbulence and,
hydrodynamic instability, Including elements in the theory, of nonlinear instabilit:3
The following are discussed at 1rariorus lengths: the theoryof probability; the
UDC: 53 2. 507

NRc Am7OU476
theory of random fields; application of the concepts of dimensionality and
similitude to turbulent flow In conduits, canals and boundary layers and to free
turbulent flow; basic concepts In the semiempirical theory of turbulence;
application of the theory of similitude to turbulence in a medium stratified
vertically with respect to, density; Lagrargian. characteristics of turbulence;
and the theory of turbulent diffusion. The book is. intended for specialists in
hydromechanics and theoretical physics. The authors express, their thanks to
A. M., Obukhov, " A. Dikly, Ye. A. Ifovikov, V. 1. Tatarskiy, A. S. Gurvich,
L. R. Tevang (the latter two for their assistance. on the subject of atmospheric
turbulenc*), and G. S. Golitsytu
TABLE OF CONTENT (abridgedl
Foreword -- T
Introduction -- 9,
Ch. 1. Laminar and turbulent motions -- 36
Ch. 2. Kathematical methods of docribiniturbulence. Averege values and
correlatfon Nnctions -- 16 2
cd, 2/3

Ono!
ACC NIv
LAr^s
Ch. 3. Reynolds equationg.and the semiempirical theory, of turbulence 215
Ch. 4. Turbulence in a thermally stratified medium -- 358
Ch. 5. Part(cle, motion in the turbulent flow -- 460
lAterature -- 603
SVB, CODEt 20 ISUBM DATE: IODec641 ORIGREF,-, 1241
OTH REF: 541

~UHIN, G.G., uchiteV.
, -C,". ~
* ,
OrgRafting the wart of atudtinta, im the cottoctive faru orchard.
301. y shkolo no-4:52-56 JI-AC (58. (KIRA, ligg)
1. Cbornnkaya srodtWarm ahkola Chernskogo rayona Tullskor oblasti,
(Cherx*-rmEt culture--Stu4r and teaching)

IALAYAIMS, A K. glaYT" red.; ARRANTAN, A -A., rel.; UmUWUIT, r.D., rad,,~
DOKMY. A.T.. red.-. ZASADTGH. B.I., red.: LVTOA*. U.A., red..
LITSHIT8. I.r.; LMRII, V.A.: MAXID., Z.X.f.2X!O"Ir,."4-SU)CHIIKO,.
Y.A.- TWGHLIXT, A.T.; SMILDIR, L.S.; TSOUWTt G#Pes rfA.;
LMHIKOVs IraGa, rsdj94-va-, PROZOROTMCATA, T.L., takha.red.
[Naterials and equipment us-dd in the cost industry; a harAbook]
gaterialr L oborudavania, pricaniaerqe v ugollnot prowphlennostt;
spravochni1c. Koskya, UgIstakhttdat. Vol.?. (Nquipmentl Oboraxiovemie.
?t,3- 1957. 655 P. (KIU UQ)
(Coal nines and mining-lquipwnt and supplies)

XALYTICOT, te.P., in&h. j: KC911, G. 1. , insh. - FUMY, A. r., inth.
monsolonam
Rev typo of coal ginet. ShAkht. stroi. no.12:11-16 D IS?.
(KIRA 11:1)
(Coal mines and wining)

DUCHNEV, V.K.p prof., doktor tekLr.. nauki KAMINg R.I., doteent; KORABIXV,
A.A.g kand. tekbn. nauk;- Mal 2,1.s indi.; BELYAYEVt V..S.t kna.
tekbm. nauk; Y,-u%XLTLUVp V-.Ye,#-Iinzb.; LLELS=;KOp V.D., in&.j
ILISHT=t A.K., kand. taklmamiuk; GKIZSXUL, K.Y.v k". tekha nax,
KODISECRABOYt: K.A. 0 kard. ",ekhn.nalak; DOWOVOLSq=j, Y.Y., kand.
tekhn. muki KLUWMV#. A,,GI, 5nshe; VOllOPAMp A#Ysr. proGr doktor
tokbn,: nwk; LIDIN, G.D,t prof.r dokt*r tekbn.naukl TOPCMTEVf, A.V.F;
prof.r MNWIKOVp V.1.9 kand, tokbn.mutkl, KUZINICEt, I.A., kand.
takhn. rAuk;. LETTES9. Z.M.j Insh.1 SrSOTEVA, V.A.,# kand. tekhnL, amakf
KELAMp Z.H., kand. tekhn.nauk; CEWAVXBI K.Kt. in2h.1
KARPIUNICHv M.Sh.r. inzh.j Mlrul'QVt L.G.9, inab.1 BOGOTOLtSKIrg,
R.Kb.t Sush.1 FROLOVT A.G., dokt= tekhn.naak; KWOSTOVp F.K.fi
inzh.l BAGASMt K.K.t k&nd. tekhr.. nauk,' KAMINSHY, I.K., insh.1
P".TROVICHI, T.I., inzb.; ZHUKOVt V.V.t red. izd-va;, I.43AILINA, L.K.p,
takhu. red.1 PROZOROVSKAIA, V.Ls-j takbn& red,
(Mining engineerat hw)dbookISpravocbnik g9mogainshenera.
Moskya#. Goa.mucbno-tekbn. isd-vo, lit;-rr pa Como= delu, 1960.
(KIKA 14 t 1)
(Xining engineering-Handbookirf, mamuals, ate.)

DYMIKO. Tef nn Ylsd imiroyi chi. 1; hl, _ T Liu OVSKIT,
Alaksandr Kakarovich; SUOTICK, P.O., otr.r~4.r CMHOTSKAUv
T.P., r*djtd-va; PROZOMMATA, T,L.-t tekhns-rodpl. SKMTAR,
B.T*,, takhA.rod.
, Ed"nAsrd preatiose for ulne construction astimateaj Swtuala
d6kwwntattila dlis, stroitelOatya shakht. Koskya. Ckmaauchno-
takha.iad-va lit-rr po gornorm 4&1u, 1960. 352 p.
(Kining enginwiaC) (KIRA 13:9)

0.1.1 KAUIZV,,re.R.;'-IZY(;ZO)rj F.B.
Basis of a method for faster calculation of sionoUtIde
tuiderground aonstructlons, for workings having a ltalv cross
Peotion. Trudr TSKIPodsomehakhtstrola no.W57-17E, *620
(Mine timbering),

G PIK'
UT-~,'A/AstrcpnoW Spectrohellograpb 1951
"Lipw-ctrobiliograph of the Crimean Astrophysical
Ob;,-~-rvatory," Gz. A. Kmin, A. B. Severnyy
"1,:, Xryniihoy Astrofi% Obser" Vol 7, PP 113-1.7
%~valuatc~~ various types of epectrohellograph-;.
De -
,cribe.; the spectroheliovXaph constructeI in the
(.zrln.~-an ~'.fftrophyv Obs. It ia lo--ated in thc t-.)-~;er
-,r ) ~'!-'Lnch reflector, has grating and prion,
nnl *"an ~Oapted to cinematography. However, fte.1-
ztrtl-s, photograpbs by this eq~Llpment Gho-ired
dl~-,.al errors and tl-k-- parts hail to be -31'usted,
c'-28TIO2

r,-? r
~q
T.
nw-
T.
7 1~
r,i
r r i-,
!I r r,-1 nc rf,. 1i -1-

S/71-2/62/028/000/014/020
E01O/E4O1
AUTHORS: ~Eartynchuk, N.A., Honin, G.A.
TITLE:: A device ror printing solar magnetic tield maps
SOURCE: Akademiya, nauk SSSR. Krymskaya astrofIzichaskaym
observatoriya. lzvestiYa-, v-28. 1962. 271-276
TZKT: The Krymskays. astrofizichaskaya, observatoriya (Crimean
Astrophysical Observatory) designed a. device for printing solar
m~-xgnetlc fie.1d maps. The device represents an attachment to the
electron potentiometer Dnn-og (EPP-09) used for recording
longitudinal and transverse components of the solar magnetic field
with a solar magnetograph. The signals are recorded not in the
form of curves but in the form of numbers sh(nring directly the
strength and polarity of.a field on the section of the solar
surface investigated, which eliminates the necessity of processing
the maps. The attachment prints: maps with black numbers from
C to 20 for one polarity and with red numbers, also from 0 to 20,
for the. opposite polarity of magnetic- fields. The pointe with
the Bame numbers,.indicating the magnetic field strength, are
connected by the curved lines, isogausses, and the map is then.
completed, The printing of numbers is performed by a printing
Card 1/2!

5/712/62/028/000/oi4/020
A device for printing ... EOIO/Z401
wheel having 40 grooves with inserted stamph provided with
.engraved figures., A two-color tape is used to print black and
red figures, in dependence on polarity of a field. The tape iB
lifted or lowered by an electromagnet functioning from contacts
1 ..
.actuated by the printing wheel. The article contains a detailed
description or the mechanical and electrical parts of the device
and its operation. There are 3 speeds of the motion or a
carriage which produces a line on the magnetic field map: 1.4,
2.8 and 5.6 nim/see, A change in speed results in changing the
w_ip scale along the line in the ratio 1:2:4. The device was
constructed in 1960 and'in July 1961 after adjustment, was put
into regular operation.. There are figures.
SUBMITTEDi December 23, 1961.
Card 2/2

OR/Oa9VhyvI4S lkr/AVr 52
jVvb1*n of Lwastigation of rlgw* of Geold by
Gmvimetric Method," .1.7. Monin, Inst of Geol
of Useful Minerals, Acad Sci Vral SSR
*I% Ak Wauk OSSR, Bar Geofiz" go 2, PP 3845
ftinti out scue difficulties in the choice of
fox la for investigation of the Earth's figure.
Presents and analyzes a fonrala by W.K. Kigal
(cf. Collection of L'yov Polytech lust, -rheory
of Simultaneous Determination of IFigure and Di-
mansions of the Earth," 1949), facilitating investi-
ption of terrestrial figure by gruvinstric method
10A Allowir 02w to avoid the** diffla"Itiss. Be
--jolv0d PI oil, 216rya

xcxixr~ I. F.
ODeMidation or Ca7t-invuts- and Deformation or the Geoid*u Cand Tech Sci,. Ltvoy,,,
Polyl.echnic last,, Min, Righer Zdacation UMJ: Llvor,, 1954. (KL No 5, J= 55)
&xr"y of Scivitifia " Technical Dissertations Defended at USSR Higher
IducatWul Institutione (12)
Sot Sm. 94. 556t 24 J= 55

Koff is. I.r.
, 4~- -
Koveseat of the earth's axLg and char4ea La its "ead, of rotatica
amiA-A by denvdation. Dokl. All SSM 105 na.2:260-263 155.
(XLU 9:3)
t. Wvovakiy p*lit4khxLteh&&ki3,r inatItut. Pr*40arleno aWealkow
T.T. ShuloyklArw.
(Urth-latation) (Chemical denudation)

50)
AUTHOR: X=LD4.x~F0j Docent,, Candidate of soir/I 54-59-6-6/i9
Technical Sciences
TITLE: Solution of the Stokes Problemo/in.a. Particular Gaut
PaaODICAL: Isysetiya vyeshikh uchobnykh sayedeniy. Geodaz4a, i
aerofotoe"yeaka, t959, Nr 6.,., PP 59-64 (ussa)
037RACT0. rat problem of Stokes (Rof 1) deals with findinj; the potential
of gravit 1.)6zdL the force of gravity itself both orL a given,
surface and in the entire cuter space on. the strength of' the,
given closed outside level surface, of' mass, and. of angular
velocity of planetary rotation. Hero, the solution of this
problem is given for the case in which the center of gravity
of the ref*r*now surface does not coincide: with the center of
mass of the earth., The simplest cases are investiCated here,
namelyp those of a sphere and,of aepheroid., Forcula. (6) is
derived, in the case of the sphere, for tKe force of' gravity
&t the level spherej thus. the problem of' Stokee appears to
be solved. as rej;azda the sphere. Formulas (10) and (16): are
derived for the spheroid., By their aid. it is ponsibli to
determine the potential of gravity and. the force of gravity
Card I/z at the level ellipsoid,, the center of which does not coincide

Solution of the Stoke& Problem in a Particular Case SO'rft54-5?-6-6/19
with the center of mass of the earth. Roferonce is made to
the following papers! M.9. Molodniskiy (Ref 3), ad D.T.
Zagrabin. (Rof 5). There are 5 Soviet references.
ASSOCUTION: WyovskLy politekhniaheskiy inatitut (L'yor Polytechnic
- rnstituts;
SUMITTED: April 6, 1559
Card. 2/2

too a fto Y/, //6 ?1 / 3 21) ~12
AUTHOR: Yonin, 1. F.
IV
TITLE: The Theory of the Gravitationa ~ Field of the Regulated
Earth
PRRIODICALs Izvenviya wyashikh uchabnykh zav#denty. Oeolerlya i
atrofotos"yemka, 1960, No. 5, Pp. 57-61
TEXT: The formulas of M. S. Molodenskiy (Ref. 1) for the relationship
between the geold heights and the deflections from the vertical, the
formula of I. S. Volodenskiy (Rof. 1) and V. L. Magnitakiy (Ref. 4)
rotciprocal to the formula. of Toning-Keineav: (for the relationdhip betweftn
the deflections from the vertical ani the gravity anomalies), a.! the
formula of V. A. 11agnitakLy (Ref. 2) and W. A. Kolodenskly (Ref: 1) reci-
procal to the formula c-f Stokes (for the relationship between the geoid VZ1
heights and the gravity anomalies) were obtained for a special casi-We-re
theriference surface Is a level spheroid whose center coincides w"th
the center cf inertia. N. K. Ulgall (Ref. 6) studied the tieory of the
figure of the earth from a new angle. He auggested to use s reference
Card 1/ 5

86(ju
The Theory of the ('gravitational !*,1213 ~-f 54/60/OJO/O-~ 3/C',14/00;-,-/XX
the Regulated Earth B012/BO54
surface whose center coincidea with the t.-reatrial center of
This makes It possible to solve various taska without using the normal
fielil. In this case. it is also possible to obtain relations tetween the
characteristics of the gravitational field of the geoid. The formulae
analogous to Stakes' and Vening-LEeintez, formulas had already betn ob-
taine4 by N. K. Kigall (Ref. 61 and T. K. Chalyuk (Ref. 11), respectively.
In the present paper, the author obtains the formulas reciprocal to
Stokes' and Vening-Keinosz, formulas, as well as the formula of Kallandro,
and the formula for the second radial derivation
Ia2W
2. . W is the gravitational potential on the sphere with the radius R.
q to the radius vector. It to assumed that the reference surfece is not
a level aphers. Two cases are dealt with: 1) The center of the reference
surfac* notneidts with tho ttrrestrial center of Inertia, ant 2) it loen
not coincide. The, origin of coordinates is assumed in the center of the
tdhare, and"the axial direction is assumed as usual. The acciracy of the
formulms derived here Is nearly equal to that of Stokes, formula since
the prosuppos It ions for the derivation were the same. The coorlinates
Card 215

The Tboory of the Gra v it -I Gij-j UJ D04/1ju,j/ za,
the Rtgulatod Varth 13~,',12/~054
of the terrestrial center of Inertia --i the!3* formulas can t
by the method of It. K. Migall (Rof. 6) or from the spherical hatrmoni,-
of the first order 4evelopei for g, vith the use of data by 1. D.
Zhongolovich. The formulas obtained can be used in geology, terrestrial
glob* physics, and geodesy. For case 1), the author obtains formula (8)
reciprocal to Stakegi f0MUIR;
9M + !S 5-jo 4 70 4) 2R 5-02R cos'~ then formula (11)
9 r 2 it ff r5 d5 R 3 2 -
reciprocal to Venirg4einesz, formula: g R 4. gm af (R 1 )dS
9M fo 2KR ar 2 2r
1 2 ff r
4 4 i(A'R - 14) R cos'~ , Kallandro's formula (14):
1 If A (i -, I )dS, and formulas (16) for the wicond radiml
17 ar r 2
R
derivati on,
2
Card 5/5

66u u?
A.L
The Theery of the aravitationrtl
the Regulat-0 Earth B012/BOCA
2 4gl-w 6g 2w0
a I . - - 0 4~3 2z- 52 a g-gc dS. For
)02 R R 2 R2 5 2z ff r5
,cmae 2) the author obtains formul% (20) reciprocal to 5tokos, formula;
grA
t dS + + 4) 2 &,)2RcCG2
21 r5 R R 2. + 3 Ca2 (r coal,
2 2 2
Z,.!3inL,\ Cos (v + y ani formula (21) rec,procal t~ Vening-
e
9
m ff 21 (R I 'WO 2 2
Lleintar; formuln: g R )ej + 2vR 6r r2 2r + R
2 2 4 3 63 2 Y2).
6j R