SCIENTIFIC ABSTRACT FELGELSON l. P - FEYGELSON, YE.M.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000412930002-0
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 23, 2000
• Sequence Number: 2
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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c7dechragrommom .1 wit Ifted fAke (19"-
Sea, i: 100). N. S.- Xufwkov, k
C0011W. rend. d
litwilm that likke
in tell takes avvr a perW of yeacs vin be woord"I
tZroulm ilk the Ifif -4 the P-1011111-k-W 9-111y
The
t"Ib0djo filst locolowd in 1902 by P. It. Schoute, ,06
camp". at thm mat takes me be simplified b!r owitcting (wity .00
own in MCI. MaCto awl
4, M#W)., Witto 11.0 moo illoo facuth twatKopprit. aml trmt-~
t
11A blood
md Outdo as addid. vwL
obtahmol, Torkkit'give a Aw-dimenAmull figure fur the
dimvam of state. This "n be repmWitted $2 a Complex
it PFO)KIWW In annual cyclic curves givilte tinic, trinp..
flea Mwels. MIT matio. . a twojmtlm dkwmms AIMIX 5,
&U.S. via 6 Paints, fiv each cm1m. Tbc "Ok rurv"
tolo4ahmood* this way am miled cycWhrmullorsons. 'llwy
and me Trull I Ald in woockLog. aidt votinn and in de-
o4pdm welt-produttivo, cwwTW..vl-* It 9 v. Of
free
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A
Boton Is the saft lakes of the ManUablek Peninsula. -04
U. Felpi'son and A. A. KoAttvaikova. Byall. last.
1-7 - KUM. Referal. ZAMr. 2. No. 4. .0
00 ,I ~iiU; b.i;4tan't In the salt Lakes of the Man-
2% to 01115% (cakd. ~00
~00 will, varies fmm O-W.
a ! . B0&). In ibe-Karab
4 wu Gulf the lialliD, content Is
PHS" of the total salt mattat. and In the Caspian Ses
M
1.28R. the IU(h content In Ke water is only 0.005%
the total salt. The ItillOs salts dimolve bi pure water 6490
-tatnuchs-al desree: than ]6fgCfandJ%Isf.A. Them- a
0 0 13 lit fore, it would be "pected that under tht: con(litions of the =00
nit lakes the 11,110i salts will be deposited before NI&CI.
Goo
so '3 This was im the case, except In the like Kn=oc. where
'aCl.
true* of INB(h wem found fit layers of NIt Is can.
eluded that MSS04 way inactsee the soly. at the bortates
and that II&BO# Is covacd. in the mother J14u
:011 i 1%9.,Id
17in
evapa. of the soins.
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Goo
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00
is 200
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sdulblllty of NasN 000 Co., in saturated NO
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sduckmis 46 36* is 4ru Pao
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0 a adubaity in pm dil. WASO's at 0 is < in pum H 0
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AM.07 exists, in H as the Dt&-
At 80* X
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Into " dvesbydra* Mob, An Ore. the ;roe
e in saturated X&O bmwea with increasing
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Avir. 1940,
19". No. 10, 340; 1A
Joe jo No. 4. ZI.-Tbe visaiiX" I" t1w MmPrl- I lilt WtOu take
.00
bit
009 llwats C11111191111 If, yvt sm Ctil
~01 the sk, L41matic fulms IWWS ObstgVel %illudialwitia
xentpri. .- oaLvmwwrvW In d
C01,114derabir varistkas% In L
and wet yun; C*SU~ UAR -0.10. M SO. 2AM-4-t1k Ma-
i0o a 'Ch W 0A;-OX slid
N(ACA 1 Ittlop. t Wine varied ("Nil
0 of 0.1 to 29.1'. Tile it onto lumis oted., MSS04:1,19-
). Itilisup JIM 9moo
00,3 old the lifixte pax" th sh f =t
NaC1 in WISIA.61111,10 lis A* 1-( ';ol)rr. The brine
1xilains "lax. suits. of 1, sild k1slivs at thr end ill 1 tic 000
'sea evnpri. period. Par M Is lite Autunul l3wil. I- 2,IA,% aof
(ill September) isad lite winter mail. V.fzj% (hk )&"Italy).
0 The min. UsClcontentinApirill b 6MI andfulkcvniher
~00% 9.185L For UAW,, the max. 6 01% In September
1 0 0
end I tain. % in Aprd and Dmmbcr, The brine goo
rewirvoirs tlKxttd be Sled In the autumn. Mirabilhe
Atintsf be culim-ted Io januar yand Ftbrinity. W. R. it, 400
doo
,it
:10
tio
A111111-SLA &"A'-LVNCAL 1111111101611112 CLAUIPOCATM Ctoo
lissova "it 04T dad, ItIPW wwlflv woo
quinewel NI&ASI am Of" Lit
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No
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.
.
.
.
,
~
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t = ~04
rate a
1. lake brims will Investittated; 2.0-2W
ut 2D. 34. 20, At. 30. 33 and 110% being were evopil.
.00
umkr Salwal Clowlims from 1"wh with an arm Gf
w4~ vm~ and a btine layer depth of 15,,m, The
V"Owk wtv wirittleell dady out dield. ithilin lievii added its -00
iho oddiwal wt. Air i" anowitch tiollthw-ft vv-
kwily suid dk*vSkm o1 or~" lk hw4fily and .90

4 CUM". and depth of the beine larer we obagr%Td. rbl:
"'Vilipa. coeff. for the Wwn take bgfim Is 0,42.

000 IVA. evapa. of the brims isixup; in Ausust at 46 It-
occurs in &-obvr
Gift Justaidity of the air and thin. graph
00 L1 atild4%hunildity. fit May'awcond that. of evap". is
oboerved. us the tviativc huniklity of the sk dmireaws to

v
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ng
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ow ptm .1) "ball pulmVIAq cialiq -Pxms 041 I"aq P&ACM
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ASS-ILA OCTALLU04K&L L"IftAltiNt CLA11WICUMN
Ad. M~tft.
am, d.( goo
Ott -4
CP a It 0 a a a it it it It it-T, oil 1. 1 1 64 0 00 a I Ar a 4
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AMC #Re# !~LL f4L

Synthesis of fisdonitc. 1. It. rvlgvl'~ V. F.
vit.4kil awl T. V. KoflAkkIlk wad. to.
V. R. S. S, 22, 242-31MM)tln

a '0, in Sq. sl4n. at 35* theTt Wat
ion of borax and AlsS
a synthetic indefite corresImmling to 2NIgO.-
cwthothm"hic' 011ficullY 11111161
'
:0 with tht asslit 2 1* nftr W. mraight voinclim
txwAlvr. itp. xT. Lig, and basing it, I.&I!,
anti w. IM) A)tt,
00
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(is
Occarow, of boron in sall lakes of Aral-KWima -00
7 ~jm .1. G. ValywAku and A. G.
foe Ir j( cmijV. pixd. amd. lei. V. H. S. S. 22. 20
j(HIAlf(in.finglish)~An examu. of 14 *Attlpk. of salt
takv briam found in Kazakh, Turkinvo and Utbek S. S.
40 RepUblics sbowed %0r contvnl~ ;It. 1- WE) 9- mine-I
fee

to mWuc) ranging from OJT1 it, !tir% ;!I umple- show
Values greater than 1.0, (kmKv Avrt* -41110
400

,3 9

A=00
cool
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00 COO
000

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F mid otber wasksto It.wo pas" to cossmAmd a coca-
_i~
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at
MS"tams. ia Is mW dm, sm1mr dmps to a m1n,
_Owd coo
'a d" kkodl. ]n'ton
04) Lsk rdpi'mm aw .400
040.3 $a, 3w.
Chu. 11kile
Of 'w
S&O
Oil .00
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boo.
boo
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slow $11,16149A %saw 64"am.
S4111-012 .4 A 143664 .1. 040 cut wirn,", 6111,11 Ott O%V M
S AV 00 AS to, 41 ; i I
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0 6 4 0 0 0 0 0 0 0 0 -11 mc
Id to k 12 a 14 is J11, v on )0 '110, )1~3111 ids Jill to it to it ow 41 4d a 0
1-4 1 4 - A- o
JR-L A L-1-
100 A 04
A* 00
(1410clietilikell ladlestlean for the ficesoncot at barittes
I ll~ FOO',o-w 6-.tj, 4.wj I,at .,f 1-~ 8 1-00
rho tAu" 11,11#s, it, 0
lia, the valar DAM for the %Vt)fl4l w"n, Far Wtrw, ft..m
V
wiotm 4fi%Ir4-1* the value-1 are givell. l1ral-Ftlit.ticgiult, -00
so*
0 -of the littler (it. WOO, tMIN). Masipbliti1w jwnict-111J.
Karalwa'O remi.m. 2.tkl; Tefirlkar rrgimi, 2. Id, A 0 0
~TjkarrruLy~h drivretititi, *21~w; a
;c ttl4ki rettiall, Is.L"N' %
goo
With Vallw bor file rsotio# kistruld lw 41 p%mol illilk-4tuttl 14
l"Wate IC(XFqi#4 its file friliml, r-O 0
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47P C~j

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4600600000000400111-0-410f#
0 4
0
0 A i Unditigroutild wattin of gas-patrobroat dirp"Its Of the
L A41ady AaJ.
0 Sarstor district. %&IL-
00 ridergruiand waterti
10
Naok S.S.S.N. 59, _I
00 were observed in the whole stratittraphic complex front
jurassictoMvoitian. They are Na sulfav orcarbortAte'
so waters. or brines.conig. hf4CJs and Caal, or, NaCI anti
00 A '~-CAXI The Wt cotitent Incireases reSdArlY With the
00 a! de th,r)l the watr 4muting horiloni. Missing froin 0.4 to
Tr 0 its tile first group. and Imn 52 to 19.4l,; in the
00 Whirs. Tile Cact, [gill" are Inct Italy in tile productive
00 callitalitcrous and DrVulliall In tile Cenozoic
slightly sulty, dcrivitil froin
fresh
the
or
waters are
horizons
00 sands and sandstones, Hr. 1, D. and K tire Prestut only
in SISIX"inAle Unit%.; cvvn It the country rocks tire of t
00 InArine origin, the totA suln of, the mincrAl mAterial Is
00 %1 not above 0 Al" A wood Tirol. com Iv% conligisk-A tile
0 0 V i%rdinients. ci"iel~y' liftlestolIC4. down to t9c'middle c4thim-
iferous, The waters dcrived [ruin thew horizons art! ex-
clusivtly of the CaCJj type. In contrast to the first zone,
00 the salts could not have been derived (Tom leaching out the
k. but by ructatnurphic, procv_ws in the
~:=12-iherwks. The waters show a type trunsitlooggi
to the twines coatig. up to 2.21% sAlts. l"roleutu and
000000000000000
W-D- Is V a 4; -a-43 -*-a
t A,& k 9 A
Middle NVOI11411, tile witer-briiring hiWilOol aff(I'VI,iting
with Mineral oil anti hydrocartma, jr,,"~ c&wor of 1he
brines tire nearly sal,l. with N
'XI in the MviaiLin, with
remarkable antis. 1)( 1. fir, it. Under the -Ant
coudititnis in these florizo,ij. the wjItc,.,Irc inn emulsion.
like state of mist. with mincral oil anti hydrocarbon p%C4:
the brines have a hjgfj if. anti vis
~cojty. I hey no, sJuggishly
ever' Its fxjr(ml% country rocks. A detail"I t4ble of the
W. Vito
00:11 hydiocarbort gases are absent, but the limestone% contain
The third zone, contS.
bitimaltious material up to 1%.
CaCls brines. exclusively. comprises the Middle Carbon-
i4i I md*tncnts of the 26losmylan Ditsin down to the
:A,l crous I
Fi_
I AS..lLA SITALLURGICAL LITERATURE CLASSIMAT"
Wi-l
-00
-00
-00
*00
.00
soo
Izo 0
0
-%*
YCOO
.1
100
UO 0
we 0
;V Its
1 nee
300
too
moo
9
Nar U t% &I No is?
0 0 to IF 0 IF ORK lWit Ifit Ku~ Ill V13.I
000-0600.90006 00060000400
10 Is ~O a 0 0 0 0 0 0 0 0 0 0 0 9 0 0 0 0 0 0 0 `10
:

KC[
and ceeffis.; nf mdamorght-milo;'. K., wd~~Wlrcso'
and JCjtx -Cxffs; of'K
(Nvt. % IC/wt, %, z saits).106. Varying fcom 1.10 t6
-ing from 0.0 to-10.9. wtd cwffs_*aI B contt~mt, Km '(Wt.
% B4000. '/o Z s4t3M' flunix 047 to';Jig un
A" givta for nil 62C takes, =M9 the qlautity Nacjlz
."UPAble for tile dewtopmot elf S34t Indust IL-0-

SHORNIKOV, B-Ya.; MGEL'SCN, LB-,
Methods of developing c6AMITNTf"helds. Yeft.khox.34 no.11:47-
48 X 156* (MJAA 10:1)
(Volga Valley-Oil fields)

V, C L 50~'J)
IARIONOVA,, O.R. FXYGIL SON
Using mineral hydrogen sulfide solution for edge water drive,
Neft. khoz, 35.uo,8:4&-5O Ag 157, (NIU 10:11)
(Oil'field flooding) (Hydrogen sulfide)
MOM

3M FUSS I BOOK ZXPLOXTATION 3OV/1827

VASSOYUM7 Manabno-lavlodovatellakly goologeresvedochn" jeaftyansy 6N
Q~
dedleglys, I morta-gazonasnoott 7ugo-wostoshay- rayonow Rualkoy It
s aboralk statey (Geology and OIL and Gas bmarIng
1a
l
r='
1
1
.
.
Uties or the Southeastern Rsglom or the Russian
Platform; Collection or Articles) Lealograd, - 43*atopto dat.
190. 242 9. Xrrsta slip Inserted. 1.200 copies printed.

and
Reap. 54.r U.S. Eventovs Xd*.v X.3. Dwsht&r, X.3. 1191na, H
l
S.A. 3&khnovakl7l Toch..Zd.s A.S. YasbeharxhlAskayal SzolutIve
Sd.S X.T. NUMOV.
nRPQ321 This book I& Intended for petroleum exploration goologlets,
partioulawly these interested in tba RUSSI&A platform a"&.
COURAM Tbose articles, originally read at a meeting of the
Solontifte and Teaftleal Counall of Kinistry of the Petroleum
Industry (1953). discuss the pelagic structux- of IM2 soutb-
Card 2/5
-dastara Pans of the Russian platform, tbA planning or expi tory
ors
&Ad Prg$P*Gtlzg vOrkv and Special problem& In gooobealstr7.
Studios are &1wed at realizing the e1.1 and gas potential
arOa. V-.IGAZ. ZL&
MSvvdkz Trust, Samtovo4ft', Kasakhotanneftv. and Grotnerts
OontrLbutod to the work. Go references are given.
CONVINTS8
Geology and OIL and "a Zearlv4 (Cent.) 3OV/%ft7
folubyatnik&v, V.D. (Neaess*d). Results of the Ortentatloo and
Itzplaratory Drilling in Central Preftavicas-yo 1203

loses. I.3. Forecasting the Oll-bearing PessIbIlLtles
Z
% ~I&W-Platform by Hydrochealeal Findings 218
Sam MAN
-*'KL*allgof, 3.X. Rydrochowleal 3tudloo in the Stall"radskays
Oblast# 116
Dollar, TOA. Some Geeabooleal Works In the Lawer P*volzblye 231
T.G. The ftlooat*loglsal FAthod
in Stratlgraph7 1134
~Svftrlkov. Tu.A. The Problem of the Tectonle AstwrO Of the
Sete-Targoalmakaya Klghlands
7
Seayukov* T.K. techniques In the Zxplorstlon of DevonLan
::
0
OIL Deposits of the 3talLagradaka7z Oblast-
AVALIABISt t4brary or Congress
Card 5^

FZYGILISON, I.B.,; CABRIELYAN, A.G.; SINUGOVSKIT, I.M.
Distribution'of satu*ration' pressure in ~ the B' lVer of the
Zhirnovsk oil field.,Neft.khoz--.37 noo,3:47-49 - Mr 159.
OdRA 12:5)
(Stalingrad Province-Oil reservoir engineering)

FRYGMISON, I.B.
Selecting absorptive horizons for sewage disposal; a topic for
discussion. Neft.khoz. 38 no.8:29-33 Ag 160. (MU 13: 8)
(sewage)
IN

FEYGELISON I.B.
Basic water resources for edge wpter flooding in Saratov and Stalin-
grad Provinces, Trudy VNIGNI no,.MI94405 160. (MM 14:4)
L Nizhne-Volzbekiy filial Vaesoy uzz ogo nauchno-isoledovatelinkogo
geologo-razvedoohnogo.neftyanogo instit-ata.
(Volga Valley--OU field flooding)

AGAPOVAy G.D.; kEYGE-L'SON, I-B*
Geological characteristics of oil and gas Pools of the Rvet
stage (layer'D~S) of the Stepnovskoye field. Gaol. nefti i
_3
gaza 6 no.6:3 Z3 Je .162. (IMU 15:6)
1. Nizhne-Volzhskiy nauchno-issledovatellskiy instittrt
geologJA i geofiziki.
(Saratov Province- Patroleum geolo6)
(Saratov Province-Gas., Natural-Geology)

gin
2
f6

inzh., redo; pBVZMM, A.S.-O red. izd-va; TOMM, A.M.,, tokhn.
redo'
[Manual of consolidated indiIces of the coot of planning and research]
-Spravochnik ukr6pnennykh pokazatelei stoimosti proekbrqkh I Isiyake,-
tellskikh rabots' VVIditsia v doistvie a 1 ianvaria 1958 go Pt.8.
Dkterprises of the petroleum industry] Rredpriiatiia neftianol vre;-
myshlennosti, 1958, 28.p. ~oqkva, Goo, izd-vo lit-ry po strolt:1 arkhit.
(MIRL 11:8)
1. Russia (19~j- UA.S.R.) Goondaretvennyy komitet'po delam
stroitelletva.'
(Petroleum industry)

MGEL'4Q&_&A,,_st&rshiy nauchnyy sotrudalk
Something new in the very old, Izobr.i rate. no.7;
16-19 ji 16o. o6MA 13:8)
1. TseeoyuzWy nauchno-issledovatellskiy institut zerna
produktov yego perarabotki.
(Grain handli machinery-Technological innovations)
Icereial products)

/5, OA
F GELSON, S.
F JEG
Obledenenie samoletov i*bo.rlba a nim. (Grazhdanskaia aviastsiia~ 1940,
no.1, p.8-10, illus.)
Title tr.: Icing of aircraft and the fight against it.
TL504.G7 1940
SO: Aeronautical Sciences and Aviation in the Soviet Union, Library of
Congress~ 1955-

IiEYGELtSON, -a-i- I-.,:En-gr -- ------ Cand-.--Tech.- -Sci.--
Dissertation: "Protection of Airplanes Against Icing." Moscow Order of Lenin Aviation
'alnst imeni Sergo Ordzhonikidze, 9 Jun 47,
SO: Vechernyaya Moskva, Jun, 1947 (Project #17836)

FZYGELI'SON, T.S.
h e
Simple met od.for stabliching the imdependence of statistics.
Vest. LGV 19 no.13tl57-158 164 (MIR& 17s8)
wa
1103 M IN t ~4
ME " -,--R!5M4

FjYGELISON, Yakav Llvovichj-PMTERP Mikhail Semdnovich; ZAYTS:,;Vp Viktor
lvazovlcwtV�~Xi~INSK"At IsIer inshor red,'-j GVIRTS, V.L., tekbn.
red,
[Making sectional'. imid-a13py.;,die03,. OVA I,zgotovleniia sosUvMkh
tverdoop~~kh obtampov. _ nimpadvI961. 20 p. (LeninpadSkii
Dom natobbo.-tekbnicheskoi propagan#. Obien peredovym opytom.
Seriial MAhanicbeskiia obrabotka netallov to 2) (KML 14:7)
.(Dies (Metalworking)j

PETROVA, L.V.,- FEYGELISCN*p Ye*M*
Role of radiation In the buildup of clouds. Izv. AN SSSR Ser.
geofiz. no.8:1247-1252 Ag '64 (K= 17:8)
1. Institut fiziki, atmosfery AN SSSR.
R

FEYGELI.SON, Ye'sm.
Speptraltflectio '.of radiatimby,cla ..Trudy GGO no.4166:
n udq
:L28~-~3 '64i,
(MIM i7: I I)

7:19GEL SON, Ye. M. CAUJO PRYSICOMAITH SCI.
Dissertation: "Distribution of Nmperaturri of the Earth's Atmosphere by altitude
during Radiant aAd VerUcal Turbulent Ifeat Exchange."
18 May 49
Ueophysic Inst. Acad Sci..USSR.
SO Vecheryaya' Moskva
Sum 71

piopbysics lapse Ratt JU/Aug 50~
Turbulence,
Distribution of Temperature of the
ti~thls Atmosphere in the. Presence of Radiation
.iiA.'Vertical Turbulent Rest Exchange," Ye. M. Fey-
04tson, Geophys Inst,.Acad Sci USSR
'41z, Nauk SSSR, Ser Geograf i Geofiz" Vol XIV,
Ak
0
44, PP 359-382
~Solves approximately equations of radiation beat
e=bange, considering turbulent heat conductivity..
Satablishes that equations which take diffuse na-
2
turt, of radiation into account yield considerably
i64T4o
UM'/Geopbysics lapse Rate Jul/Aug 50
(Contd)
hi,gber temperatures at.all,levels than the solu-
TaLon of the Scbvartzschild -equation. , Evaluates
b~ti~al thickness'of the,.atmosphere from adsorp-
and isdiat
Uiw: spectrum of. vater vupor. lion energy.
dalcu'lates temperature distribution and.flow~ of.
iaditstion energy vith height. L Gives for=la:.re-
lati-h# effective radiation vith temperature and
liumi4iity at the earth's surface. Submitted
L. S. Leybenzon.
2246v 49 by Acad
164T40

I WE f
IRE 1=191.1 wlmoaomummi,
M -M Al
NO

li-llc;.--, A
00 PP
IWA,
wo

. ~ I -:. ! --- ~i~' I- ~ - - - - !-- ~ I-- -- , - '- - ': -.-- - , ---- 1--.- 1
-r - .- -,II -Y-A! ~-- I - C - Z, I - - ~:' IL~ 7-'t .- -1 -- - ~ . - . - - -

L .`~~ -~;:.- .. - ,
~
c5i, !ffil 1 M IMIS Rillill-R, li~.~-,,~-;-i' .. . -.1

-- . I - .1
, - -1
Z-
t,-- 7:.--
E---W
K~ :3
M

"rid ba t-th la
"s-7 "M,
ha
Asi
6i.
Z.-
tcF, wat6r -vii-por ard7-
soi
--.2

SR/Geophysi cs Heat exchange in the atmosphere FD-1785
Card 1/1 Pub 45-7/18
Author Feygellson, Ye. M.'

Title Taking into ac.count, selective absorption in the theory of radiant beat-ex-
change in,theatmosphere

P(iriodical Izv- AN SSSR, Ser. geofiz.- 249-26o., may-jun l955
Abstract The.author,investigates-'i6tUant heat-ex Ichange of long-wavelength radiation
in the terrestrial atmosphere under the,assumption of the divis.-Jon of the
absorption spectrum of water vapor into regions of small, medium and large
values of the coefficients. He clarifies separately the role of large Co-
efficients in the upper layers of the atmosphere. He thanks Ye. S. KuznetE;ov.
Kupetsov, 'bistribution of the temperature of the
Your references:
Ye. S.
,
,
atmosphere along the vertical under radiant equilibrium," Trudy Instituta
teoretich. geofiziki, 1, 1946; Ye. M.:Feygellson, "Absorptive properties of,
'water vapor.an.d.carbon dioxide in the atmosphere," Izv. AN SSSR, Ser. geofiz.
No 1, 1955; K. Yao Kondratlyev,'Peirence dlinnovolnovogG izlucheniya v atmos-~
fere (Transfer of long-wave radiation in the atmosphere), GITTL, Moscow-
Leningrad, 1950-'
Institution: Geophysical Ifistitute,:Academy of.Sciences USSR
~Submitted March 20,11954

IN

Ar I
60-37-3/7
AUTHOR: Feygellson, Ye. M.
TITLE: The Effect of Clouds on the Thermal Equilibria in the
Atmosphere (Vliyaniye oblakov na teplovoy rezhim
atmosk.ery)
PERIODICAL: Trudy Geofizicheskogo instituta Akademii nauk SSSR,
1956, Nr 37(164), pp. 62-88 (USSR)
ABSTRACT: The author examines the transfer of long-wave radiation
in an atmosphere containing a homogeneous horizontal
layer of clouds of finite thiakness and computes the
distribution of temperature in such an atmosphere when
a state of radiative equilibrium exists outside the
cloudy layer. The dispersion and absorption of long-
wave radiation in clouds with variants, the character-
istics of solar radiation penetration in a cloudy at-
mosphere, and the selective character of the absorption
spectra of vapor outside the clouds are considered.
There are 2 tables, 7 figures, and 7 references, all
USSR.
AVAILABLE: Library of Congress
Card 1/1

FM=09, X M.- , KOGAN,- G. Y.- p MALIWIICR, M. S.

IFF-Y GE C 8 0
3(7) PWWZ I.B.OOK MWITATION sov/i6b
Akademiya riadk SSSR. :XmItift po ge9det'll'i geofizike.
Teziby dokl6dov'na, XX Generallnoy, wembl4e Mezhdwmrodnogo ge6dazicheakogo
I geo-fizi6he'skogo aoyuzia. Mtzhdune,~odiaya assotsiatsiya, meterologii,
(Ab6~ricts'of Reports at the 11th General'Maembly' of the International
Uni6n of-Geodesy ~nd Geophysics. The International Association of Meteorologyj
Mosrowil 1957-'~ -38.P* /Pir"l texts in Rtissian ~nd English or Freicli/
1,500 copies printed. No additional contributors mentioned.
PURPOSE: This booklet ~,s Intended for metebro Sts.
yogi
COVERAGE; These reports cover variew- subjects in the field'of meteoroloao AwLM
the specific sodivisions discu46ed are: the fitat balance of the Earth's surftce
jet strpams, t;rsnsteAnce of heat, radiation, electric coagulatton o~ cloud perti-m
cles., turbulent diffusion, 61oud studies,'and others. AbstraAs' of all the arti-'.
clefs areItranslitedinto either,Freiich'or En~lish.There are n .o references given.

SOV/3-6115
tue
it
its ~~Oj .
the
sit
-Of
st",
t-fou Jet
roxims", Catte
3.1sollo Oaspe
i(Ouu I - ";
e 14
-te ease ous
the zc~,Atl
'VIch, sm--yor -f C--
-lut 0
TLes
sets., e*a tiie Ptm&c'svhere
on
of Val
test.
the
wrt'leles 24,
Tro -f
on
Cal CPS Ivilst~ ola
t Diff'ol
28-
of
PTO . I - tractuve
gie'ro
Aes -A'A. -on to
n,
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a
C$bUISUO" f Ce Of t1le
stite
The
Tversuoy t JIL-d"
~aeu

24(4) PHASE I BOOK EXPLOITATION SOV/2545
Feygellson Ye. M., M. S. Malkevich, S. Ya. Kogan, T. D. Koron-
afo-v-a-, 77ZT-Glazova, and M. A. Kuznetsova
Ras&t Yarkosti sveta v.atmosfera pri anizotropnom rasseyanii,
eh. 1 (Computation of Light Intensity in the Atmosphere In
a Case of Anisotropic Scattering, Pt. 1) Moscow, Izd-vo
AN SSSR, 1958. 101 p. '(Series: Mademiya nauk SSSR. Insti-
tut fizilci atmosfery, Trudy, nrl) Errata slip inserted.
2,000 copies printed,
Ed.: G. V. Rozenberg, Doctor of Physical and Mathematical
-Sciences, Ed. 6f Publishing House: V. I. Rydnik.-
PURPOSE: This book is intended*tor physicists and scientists
engaged in the study of atmospheric cpp~im
COVERAGE: This wc(rk contains the results of computation on the
intensity of light,soattered anisotropically in the atmosphere
under various physical parameters and functions of scattering.
The solution of integro-differential equations of the theory
of radiative transfer in an anisotropically sdatterikig medium
Card 1/4

Computation (Cont-.) SOV/2545
was obtained by the method of successive approximations.
The work wqs-carried out by the staff members of the.La.bor-.
ato*. of--Atmospheric Optics within the Ina titute of Physics
of the Atmosphere, Academy of Sciences, USSR. No personalities
.are mentioned.' There.are 23 references;' 14 Sov.'Let, 4 English,
4 German, and 1 French.
TABLE OF CONTENTS:
Introduction 3
Ch. I. Mathematical Solution of the Problem 5
1. Statement of the problem. Derivation of basic rela-
tionships 5
2. The zero-approximation
.3. Selection of the-first approximation 11:
4. Computation of subBequenit approximations 13
5. Accounting for the albedo of the underlying surface 15
Ch. II. Processing Observation Data 19
Card 2/4

Compu tation (Co'nt.) SOV/2545
1. Review of Observation materials 19
2. Utiltzation:of experimental data 22
3. Processing seattering functions ~24
~
4. Change from"optical thickness to the geopietrical height 25
-
Ch. I II. Computation Results and oertain Conclusions 27
1. Convergence of the series and of successive approxima-
tions 27
2. Relation between the intensity of scattered radiation
and the solar altitude, transpareny of the atmosphere'
and the form of the scattering function 29
3. Light reflection from the Earth's surface 42
4. -The flux scattered'radiation 43
.5. - comparison with a case of i3otropic scattering .48
6. Significance of multiple scattering .50
7. Explanation of the tables -52
Table.I 56
Table 11 97
Table 111 .98
Card 3/4

Computation (Cont.)
Table IV
Table V
Bibliography
AVAILABLE: Librau of Congress
Card 4/4
SOV/2545
99
99
100
MM/jb
.11-2-59.

SOV/49 -58-10-7/15
AUTHOR: Feygel'son. Ye
TITLE- n erpreting Observations of S B i ess (Ob interp-
0 ky rightn
retatsii nablyudeniy yarkdsti neba)
FERIODICAL:'Izvestiya Akademii Nauk SSSR, seriya geofizicheskaya,
1958, Nr 10, pp 1222 1233 (USSR)
ABSTRACT: Observations~on the brightness of scattered light. are
used extensively to determine the scattering propertiesof
the atmosphere (Ref.1). The present article tries to ex-
plain the following points in interpreting the observational
theory: 1) what information on the scatterin.- function Ican
be obtained from bric;,,htness.measurements based on the theory
of single scattering 2) to what degree multiple scattering
can be imnored, 3) how accurate a correction fo.r multiple
can be made, using Ye. V. Pyaskovsk,,~y-a-Fesenkovals
method. The propagation of light in the Earth's atmosphere
can be described by an equation of the form:
C16S 9' 01 T;- r) 1 I(T; ~rl y (,r;r;rt dwI I(r; r)
41r
S
+ ex,0, (T -0. sec y: (-r; r
0-
Card 1/7

SOV/49 -58-10-7/15
On Interpreting Observations of Sky Brightness
Here T.- is the optical thickness of the atmosphere
T., cr (z) dz
0
,.vhere cr(z) is the scatterin- coefficient. I(t;r) is the
0
intensity of radiation at a height z in a direction r
(at an anc-le 9 to the vertical and an azimuthal angle
L3 C3
y is the relative scattering function and r' is the
direction of propagation of scattered light. The scattering
function depends-on cos(r, r') = cos O(P The atmospheric
boundary conditions are given by Eq.(4) where q is the
albedo of the Earth's surface and -F (-r5 , F -r) are the
1 2(
integral functions of I(T-, r) shown. lvllultiple scattering,
r3
is represented in Eq.(l) by the first term: if this is
neglected Eq-(5) results, which, using the boundary condit-
ions Eq.(4) gives Eq.(6) ior a level T = 0 This can acrain-
be re-expressed in the forms Eqs-M, (8) if y(t7 (p) does
Card 2/7

On
Card.
"MI
SOV/49 -58--10-7/15
Interpreting Observations.of Sky Brightness
not depend on height. As is shown in Ref.21 the scattering
function of a real atmosphere chanv-,es 6onsiderably,-with
height. Hence, thevalue of y calculated from. Eqs.(?) or
(8) is called the relative scattering function averaged over
the whole atmos here I A more realistic average is that de-
fined in Eq.(103; which transforms Eqs.(6) to the form (1 1),
(12). Using the averaged scattering functions Eqs.(9) and
(10), some information can be obtained on the change of
y(t, (p) with height for a given sky brightness at the
Earth's surface. The atmosphere is assumed to consist of n
layers in each of which y is constant. Eqs.(g) and (10)
are then written in the form Eqs.(13) and (14). If measure-
ments are.made of.the sky briGhtness at sufficiently small
time intervals for n points (9k14)k ) and the resultant
val,aes substituted in Eqs_.(13) and (14), n equations are
-b-taired. to determine the scattering functions for the n
layers with (p - (p 0 . The system of equations has the form
%(17). Localization.of the layers requires a Imowledge of
a z). The role of multiple scattering is considered in re-
lation to the data given in Ref.3. The results are related
3/7 to an idealized two-layer model. The calculated brightness

SOV/49'-58-10-7/15
On Tnterpreting Observations of Sky Brightness
is expressed in the~form:
B(T; r) BI(T;.r) + BII(T; r) where B I is the.
brightness due to first order scattering and BII due to
higher order scatterings. Table I gives values for 10OB11/.B
when T - 0 1 and Fig.1 shows the scattering indices for the
two layers. Table I shows that the part played by multiple
scattering incteases with T*~. The'effect of multiple
scattering is indicated even better in the case represented
by Table 2. Thi 's gives the scattering function as defined
in Eq.(14) for a 'two-layered atmosphe;e (dotted line in Fig.1)
together with the relativj brightness 'T(O,, r). Table 2 does
not show the change in 6B due to change in y or (p - this
is represented in Table 3. This latter table indicates
smaller values-of 6B than Table 2 and shows there is a
value of yo for which 6BN(07~1 (00 0 . Table 4 gives
Card 4/7

sov/49-58-10-7/15
On Interpreting Observations of SIU Brightness
the diminution m multiple scattering with height. The
relative bri-htness 13(", r) and reloative scattering function
y(T) are those of the model atmosphere curve 2 in Fig.l.
Table 5 gives the change in correction due to multiple
scatterin.a more accurately. The method of estimating the
effect of multiple scattering worked out by Ye V. Pjaskovs-
kaya-Fesenkova can be put very simply for 9 =~' . Writing
down Eq.(19) with the notations (20) (21) and (22) it is
foundthat the substitution BII = a~7 - T4) can be made in
Eq.(25) to give Eq.(26) (c.f. Ref.3). Table 6 gives values
of BI, as a function of 0 and y for various values of
tAF ~ and 9 . Table ~ is taken from Ref.0 and gives values
of the brightness B(O,c, for 'the values of rl given
in the first column, corresponding to the lower layer.
(r = 1.3 in the upper layer). Values of y(g) calculated
from.zq.~14) and y(T) by:Piaskovskaya-Fesenkovals method
are also given together with T 7 which can be considered
as the optical thickness corrected for multiple scattering.
The following conclusions are drawn: (1) Single scatterin-
0
formulaq can be used for determining the scattering function
Card 5/7 when 0.15 with an error -410-15964 (2) Eq. (7) does not

SOV/49 -58-10-7/15
On Interpretin- Observations-of Sky Brightness
0 0
have a physical .-I,nterpretation - it cannot be-used for def-
ining the scatterin~function averaged over the whole atmos-
Dhere. (3) For -r* 0.2 , the brightness curve measured at
ihe Earth's surface differs considerably from the average
relative scattering index owing to multiple scattering. In
this case, the part played by multiple scattering is consid-
erably larger for directions (p>900 than for q< 900 .
(4) The ef feet of multiple scattering diminishes with height.
CM,
At heights of 7-10 km the single scattering theory can.be
used for T*-=zO.4 with greater accuracy than for T-*-='0.2
in the surface layers. (5) Condition (23) is approximately
fulfilled in the angular interval 300 W/2
(H thickness' of cloud,,9 polar angle of direction r).
Since the water,vapoux in the cloud is st8l rated, the
function (5) can be defined, where ?~ (z, t,.i, Eo =-6.lmb
_saturation elasticity of water vapour at 0 0C, a =.7.5,
b 2 2
RW =.._460m/sec -deg gas constant, t*
Card 2/5

SOV/49-59-6-6/21
The Radiation Cooling.of Stratus-CloijA
temperature in degrees-0 (index 1 -atmosphere, index:O
cloud). These conditions are applied in Eq (6) for the
atmosphere above the cloud. The coefficient of damping
for drops of 6.265 11 radius is taken from Ref L~, as illu5-
trated in Fig.1, continuous line (the dotted line - data
from Ref 5). This coefficient is calculated from Bq (7)
Where a. - mean damping coefficient (Eq 8). The cal.ou-
lation shows that av,,% given in Fig 1. can be substi-
tuted by' av 1000 - 1500 am 2/g. Then the value of A
will be obtained with an accuracy of 3%~ Thus Eqs (1) and
(2) can be adjusted as Eq (9). Also, taking into account
the thickness of the cloud,(Eq (10)), and the mass of a
vertical column of water vapour in the atmoss here above
the cloud, (Eq (11)1 the - f inal form of Eqs (l and (2) can,
be written as E s (13) to (17). Fig 2 gives the values of.
ffi(T) and 13(TI - As an example, the following are
given: !o -, 2730 , Bo 0.146 cal./c2min') 0
= 4.9 x 10-6g/CM3 5 p =.1.3 x 10-3 g/OM3 9 cp = 0.24
Card 3/5 cal/g deg,, to 24 hours? Mv 1100 CM2/g aw - 1 CM2/g,

SOY/49-59-6-6/21
The Radiation Cooling of Stratus Cloud
01= 0.51X.10 -6 S/cM3 , then the values a(0) 0.117.,
a(1) '. 13.19 b -0-398 x 10 -2 are calculated from Eq (17)
for L -at, 590 cal/S. The formulae (13) and (14) can be ob-
tained as the.dimensionless equations (18) to 1:24), wh,ire
R(,rI t) is the function of temperature (Fig 3). Table 1
illustrates the values of
T (0) (0)(T
(T I ti) and ?v(T-1 Y
at different-points,of the cloud. Table 2 gives the above
values for the top boundary of the cloud for 6t =0.5 h
Table 3 gives the density~of the d-vops (second column) and
its upward'rate of fluctuation (third column) for three
types of cloud (first column): rain-cloud, cumulus-stratus,
Card 4/5

MGZLISON. Ye.M.; MALKNICH, H.S.
Calculation of light intensity and haziness coefficients in
anisotropic scatterirg. Trudy Iab.aeromet- 707-44 159-
(MIRA 1311)
1. Institut fixiki atnos'fery AN SSSR.
(Photogisphy, Aerial) (Atmospheric transparency)

SOV49-50/-9-2?:/25
AUTHOR: Mastrov, V. G. and.Feygellson, Ye. M.
e on ----and-Atmo spheric Optics
TITLE: Conferenc the Acujn~metry
PERIODICAL: Izvestiya Akademii nauk SSSR, Seriya geofizic.heskaya
1959, Nr.9,.pp 1435-1436 (USSR)
ABSTRACT: The Conference was convened in Leningrad on January 28
to February 4, 1959, by the Commission of Physics
of the Atmosphere', Academy of Sciences,USSR,the Leningrad
State University and Central Geophysical Observatory.
Altogether 102 papers were presented. The separate
sessions were devoted to: radiation, sky luminosity
and polarisation, reflective properties of the
foundations surfaces., transition of atmospheric
radiation, methods of actionometric. measurements and
radiation in industry. L. G. MakhGtkin spoke on new'
characteristics of the atmospheric turbulence; T. G.
Berlyand described the distribution of solar radiation
on the Earth; N. T. OhernigovsklyIT. T. Rusin, T. V.
Kirillova, M. S. Marshunova, B. M. Gal'perin and M. K.
Gavrilova-dealt with investigations of radiation in the
Arctic and Antartic; G. N. Faraponova, Yu. I.
Rabinovich, V. 1. Myukhyur and G. P. Gushellin discussed
Card 1/3 the decreasing of sunlight at 6 to 7 km high;
L-X

ISOV/49-59-9-23/25
Conference on the Actinometry and Atmospheric Optics
0. D. Bartenlyeva spoke on the determination of the
indicatrix: of light diffusion in ground surface layer
of the atmosphere (apart-maximum at 0 and 1800 an
additional maximum 130 to 1450, corresponding to the
rainbow, was defined); B. A. Chayanov described an
automatic photometer with a range of 25 km; G. V.
Rozenberg dealt with investigations of the angular
diffusion of polarised light in the ground surface at-
mosphere; Ye. M. Feygellson consi&ered the cooling of
cloud tops and its effect on precipitations. The other
papers and their authors were as follows: K. Ya.
Kondratlyev - Carbon oxide in the atmosphere; I. N.
Minin - Trar-sfer of radiation affected by refraction;
Yu. D. Yanishevskiy - Pyrheliometer as a radiation
counter; V. S. Atroshenko and 0. A. Avaste - Gn the
Sobolev transfer equation in optics,; K. S. Lyalikov.-,
L. B. Krasil'shchikov , N. Ye. Tet-f-Urkaryants,
N. I. Goys,, K. Ya. Kondratlyev , Z. F. Mironova,~
Card 2/3 and L. P. Dayevc.'- Determination of Albedo and
spectral luminosity; M. S. Malkevich - Reflecting

SOV/49-59-9--23/25
Conference on the Actinometry and Atmospheric Optics
properties of the ground surface in. rela-IL-lion -'U-o light
diffusion,j-n the atmosphere; V. G. Kastrov - Errors in
determininE; the absorption of solar.radiation'in the
atmosphere. The Conference approved the formation of a
special corrimission for the revision of thermin-ology.
The addresEes of two members of the commission are 63-ven.
Card 3/3

--,~ I
wv~

PKM I BOOK MWITATION SW15019
Georgiyevskiy, Yu. S., A. Ya. Driving, N. V.. Zolotavina, G. V. Rozenberg,
Ye. M. Feygellson and V. S. Khazanov
Prozbektornyy luch v atmoefere; iseledovaniya po atmosfernoy optike
(SeareliligWRLy in the AtaoipbIerej InvestigiLtions in Atmospheric Optics)
Moscow, Izd-vo AN a=,,: 1960. 243 p., Irrata slip inserted. 1,600 copies
printed.
Sponsoring Agency: Akade" nauk SM. Institut fiziki atmoofery.
(Titlepage): G. V. BDzenberg, Professor; Ed. of Publishing House: N. L.
I!elesninj Tech. Ed.: I., F. Koval'slo,*%.
P=)=: This book is intended for geophysicists cpncerned with searchlight
vo~nding of the atmosphere and questions in atmospheric optics.
COVERRO: The book reports oa.jee-ent'invistia"ions of-the effect of SAMOspheric
conditions on the visibility of distant objects illuminated by a searchlight,
and the utilization of a searchlight beam for investigations in atmospheric
crptics. The authors limit themselves to that side of the problem directly
Card~_

Searchlight fty in the Atmosphere (Coat.) SOV/5019
connected with atmo c conditions, but give a sufficiently detailed re-
spheri
viev of present-day data on the optical properties of the atmospherat. At-
tention is-concentrated. on'studies made by the authors and their colleagues
9.t the I"oratoriya atmoofernoy optiki Instituta fiziki atmosfer7 Alzademil
rauk SM (Laboratory of Atmospheric Optics of the Iastitute of Phpico of
1he ktmc,~,phere AR USSR). No personalities sa-e mentioned. There art 173
zeferences r 100 Soviet., 38Rn"hj 25 Gerumn., and 10 French.
TAMZ'OF CONNINTS:
Preface 3,
Ch. 1. Problem of Forecasting Visibility, and Searchlight Sounding'of the
Atmosphere ( G. Ve Rozenberg) 5
l.Problem of forecastIng the vlsiblLtty of distwit, objects illumin-
ated by & searchlight 5
2.0ptteal characteristics of the atmosphere and the problem of
measuring them 10
3.11roblem *0f,sounding the atmosphere with & searchlight 14
4-History ofthe ,development.of. the searchlight method of sound-
ing,the atmosphere 1T
5-Problems-of method 26
carcp/:6,

Searchlight My in the Atmaphere (Cont.) MV/50,19
Mundnation, by
scattered Ught of a searchlight
156
A. TI I mmination Outside the MY 156
b. -t Usti an OnAhe am of' the M"blight bean 15T:.
4. Visible contrast 'Of ob.41ect
Muminated by a sear .159

5. .
an ght sounding. of t4m atmosphere
Theory- Of GO
16k
fte_L QZtremdty of tbe dbeervation'tas at &Vertnz* and the
equation of 16k
b
Ways of solving equetIon of searchlight soanding 167
6. ;
)eteridnation of compoments of scattering matrix ITO
Ch. V. (~mntitwtlve Analysis of ~Zffect ot Various, Factors on Intensity
of Scattered Light, of -a ~ Searchlight (Ye. IL - Pbylpl son) 1T5
1. -Solution' of transfer. eqmation In the Mai _OfscLivffr6_T_USht
of &L searchlight 175
2. Intensity of singly scattered ligtt of a searchl.1ght; method
of cooputation 179.
3. Gemetric ccmfondty 284.
4. -Dependence of the -Intensity of singly scattered Ught of
seinhught an the optical properties of the atumpbere 190

1A

bealthlijbt WY in the AtMoMpbere (Cont.) WV/5019

r
. Effect of distrIbution of light intensi-kir of march-
5
light 197
6. Visible contzeAt of object illuminated by a searchlight '199
7. XatIzatIons of doubly scattered light Of a searclillght
ch. V11. fterlsental Verification of the 5wory ad Ban Results of
Searchlight Soundint of, the Maosphere 1 209
f visible Intensity of scattered 1:Eght of a
."archlight and comparisonylth +A* theory, (A* TA. Driving
S, V. ZCIO+AL*IDAS.G. V. Rosenberg) 209
2. C;.n;;a7t according to experizental data of aft object illminated.
by a Searchlight (A.'Ta. DriVing, N. V. ZolotavirAs 0. V.
~.Hozenberg), 219
3,. Aerosol structure of+.he atmosphere (As 7a. Driving, N. V.
zolotavinO 224
4., Chameteristice of atmospheric aerosol according to data from
,searchlight a TS. ftiving) 232
5., Concludin ~re (.00 Y. Rosenberg) 2~7
Bibliography 2*
AVAnARIXt Llbrary~of Congress JA/dw's/,%1
Caig �t6 5.2-61

S/o4g/60/000/02/013/022
~EOWE414
Alrj,'HOR t Feael-la n. Xq. M.
The Ef f ec+ ok'Turlmlenc e on the'Radiation Cooling of
Clouds IV
PERIODICAL:Izve stiya Akademii nauk SSSR, Seriya geofizicheskaya,
1960, Nr 2,. p-p 299-308.(USSR)
ABSTRACT% It is to be,expected,that weak turbulent mixing, which
was neglected~in the previous paper by the present
author (Ref 1),would tend to reduce radiation cooling
since the latter takes place in a very thin layer (Ref 1).
The-present paper is therefore concerned with the
extension of the-model-discussed in Ref I to the case
which.includes turbulent heat transfer. The latter
effect is estimated Approximately It is found that the
turbulent mixing coefficient D icm2/sec), which
charac erizes the tur ulent heat-transfer, lies between
2 x 10t and -50 x lot CM2/sec. For such values'of D,
the radiation cooling-near the cloud boundary is shown
to be of the order of 0.1 to 1.70 per half-hour. Pure
radiation Icooling.under these -conditions is 60/hal.f-hour.
Card 1,12 Simple calculations show that turbulent mixing

s/049/60/000/02/013/022
E032/E414
-The-Effect of Turbulenceon the Radiation Cooling of Clouds
considerably weakens the radiation cooling process for
the:upper parts of the,:cloud.and leads to an increase in
the thickness of the cooling layer. The numerical
calculations are summarized in Tables 1 to 3, in which
the symbols are said to be defined in the previous paper
(Ref 1). There.are 1 figure, 4 tables and
6 references,.5 of which are Soviet and 1 English,
ASSOCIATION3 Akademiya nauk SSSR Institut fizikl atmosfery
(Academy of Sciences USSR, Institute of Physics of' the
Atmosphere)
SUBMIIVED: February 24, 1959
Card 2/2

ATROBEEN900 V.Sep- GLAZOVAS 4#4.j VALKEVIGHp K*8ej.XMQP-LSONj. Te4,-M"-.
prini"li uobastiyej'XD1# E...' studentka; TONASHOVA, L., studentka;
ROZE GIG., prof.., d6ktor fiz.-mdtam,nauk, o 'tv.red.;
PENKINAS N*V*., redizd-va; BUSHKOVAO L.A*,, tekhnered.
[Calculation of light Intensity in the atmosphereduring
anisotro scattering.. Part 2] Ranchet :Larkosti aveta v
PIC
atmonfere pri anizotropnom raeBe at' 2. Mookvaj
idemiia nauk
Izd-vo Akad.nauk MR., 1962* -222 ps S&91R.
Institut fisiki atmosfery. Trudy.. no*3). [MICROFILM) (MIRL 15:8)
1. XbskovBkiy gosudarstvenrWy universitet (f,6r Kim, Tomagihova).
(Light-.Scattering) (Atmosphere)

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2
NR: "4043909 8/0049/64/06#08/12A,1/125
AUTHOR: Petrom, L* V*;'Feygelloon, Ye 'M
t, Ij 7.!
TITIH: Role ct radiatim in cloud development
SOURCE: AN as
an. IzvestiYa.-'seriya goorizicheakeya, no. 8,, 3.9641,: 324,7-1252.,
b
TOPICSWS: cloud physics, atmospheric:ftsica, atmospheric radiatl.oa,.ataa6;he'ri6'*L'-4L,~
cagwave radiation, cloud fomation, temperature inversion
ABSTRACT: In investigations of the origin and development of nonc(mve6tive
it ie custanary to consider heat exchange and moisture exchange in the atMOSPbGre"'I
-brought' about'by vertical movements
turbulent mixing, and
-phase trawfaimatidis
of water* This.paper differs in that, in addition to these factors, the authors
e
also take Into accouat th heat flux associated with the transfer of longyave
radlation aud, the role of the latter' :Lu cloud -farmatloa. The method uned In soly-
ing this problem vu praDmec
I by: L. V, Matveyev and. was deacribed Jh an earlier.
Paper by Ye.M. Veysellson (Xzv.'All aSSR, ger..geofizo,, no. 19Q). -------
This article.,."
gives ame numerical results showing the influence of a racliation heat flux on,.
the variatica in the liquid vater.coatedt of a olovids Comp4tatiomig made with-'].:,.,.-.,..---,.
1/3.

wassion nR.- AP043909,
a "Ural-l't electronio ocmputer, revealed that a cloud develops upward under the'
Influence of radiation cooling. It vas also found that the contribution to
-water content from radi
ation decreanes with an increase in the velocity of 48-
cending movement. ~In this case the -role of vertical movements as the principal
factor in cloud formation is manife(sted. With an iatenoification ct vertical
Z:the,other factors iq lessened. In th
movements the relative importance a a canter. -
of a cloud the effect of.radiation is less, than that of turbulence). bAt it is not
negligible in. cotaparizon vith the latter. In the upper part of a claud, the role
of radiation transfer Is the dcminant.9ne. The generally-acce~teamechanism Of
formation of,stratus clouds,taking into account vertical movemento and turbulent,
transport of beat and moisture, is thus shown to be incanplete. This result,-,
IM, Ser.
confirms the concluxion Previously drawn by Peygellson (Izv,, AN SSI
no. 6. 1950 and no- 7.. 196o) that radiation has a decisive effect lcm, the fm-ma-
of the upper layers of a cloud. Tile conditions imposed in theae carller
studies (liquid vater-content does not decreaze*,in the'direction or the upper
-3:
boundary) made'it possible to investigate directly the thermal effect. of radia.
tioup isee., the develolmenit: of A temperature inversions In this new study the
I formulatim of.ithe 1wob Is awh 'that'the..Uquld water -content & a develqping,~; 1-~
lem
Card

~7:

AP1,043909
AC(,'ESSXON HR

Cloud decreases rapidly in the direction'ofthe upper botmdary, Under this ecd-

cur, Orlg* art..
'dition no inversion of radiation origin will oc
.has: 27 fomiUm
and 5 tables*

Akademlyuntiuk SSSR Inatitite of
BOCIATIM Inatitut Mild atnoofery*
S.
A
,
0f,.Sciences SWR)
ca, Academy -
Atnoopheria Physi
.
,
,L:' 00
SUB CCDE:t SS
P suamlmm 14sep63.

001
NO MW SOVI

3;1V

ACCESMON M. AP4041568
AUTHOR: :00 It 0. M.
TITLE Optical properties of clouds
-A
SOURCE: Kosmicheskiye 1s9ledo"nii~&,.Y,' 2, no. 3, 1964, 455-461
TOPIC TAGS: cloud, atmospheric optics, meteorology, meteorological.sitellite, cloud
optics, cloud albedo
'ABSTRACT: This article is a brief review of studies of cloud opt!cs made at the Institute of
Atmospherio Physics by Ye. M. Feygellson, L. M. Romanava, and'A V. Rozenburg; original
sources are cited In the bibliography. Principal attention in tbe review is given to theoretical
work On the transport of radiation in clouds, determining the laws of reflection tind txans
sion of radiation by clouds, without taking Into account the influence of the atmoetphere out-.-
side clouds. Ia.these studies the following conclusions were cb-awn. 1. In the visible part
Pf the spectrum the scattered light of haze considerably distorts the light passiq; from the
cloud to the upper bcundary of the atmosphere. 2. The 141bi of haze over clouda Is not de
penderat on wavelengih; this Is true of cloud albedo as well. It therefore is impossible to
Card 1/3

A
ACCE SSION NR: AP4"16611
count on distinguishAng clouds situated at identical levels on the basis of a chaq,,e of the SPWJ
tial dependence of their brightness. 3. Im-lying clouds can be brighter than high-lying
~Clouds due to the gp3ater thickness and scattiering capacity of -the first. . Therefore it also Is
doubtful if cloud levels can be distinguished on the basis of differences in their- brightness.
4,, The angular distribution of the light reflected from a cloud is relatively uniform except in
region of azimuthal angles 1350-< 1800. In the latter case, in the event of low solar
-'altitudes there is a rapid increase of brightness in the direction of -the horizon. It scarcely
swill tie possible to make use of this peculiarity, since it also Is characteristic of snow and
latmoopheric haze. 5. A difference pf albedo at the center 0. 76X4) and on the wing of
:the oxygen absorption band canAntroduce an error of the order of 10-20% into determination 77%.:i",
;of the optical thicknOSS of the 'atmosphere over the cloud. 6. An opaque cloud can be con-.,
isidered a black body
with an error of 5-10% In the spectral ran
I . ge (4 9:!t X itr 7A4 and
40~ ). Li the atmospheric window, of transparency (8,q IZ44 this error is.
15-25% These conclusions, important In the field of satellite meteorology, are followed by'.
:a. listing of what the author feels are highly Important unsolved problems In atplo~p
herio
opticis. Orig. art. hant 3 formulas 9 figuna mW I tablo._