SCIENTIFIC ABSTRACT VINOGRADOV, A.P. - VINOGRADOV, A.S.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001859910010-7
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: September 1, 2001
• Sequence Number: 10
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

AFP11ASIYEV) G.D., otv. red.; WANOVI prof., ram, otv& red.;
SHGBRBAKOV) D.I.) akademik, red.; FOLKA11OV, A.A., akademik
red.[deceased]; STARIK, I.Ye., redaktor
_ADOV.# A.P., akademik, red.; GERLING, E.K., prof.,
red.; PEKARSKAYA, T.B... kana. geois-winero nauk) rod.;
BORSUK, A.M., red.izd-va,- SIMKINA, G.S.) tekhn. red.
[Transactions of the Ilth session of the Commission on the
Determination of the Absolute Age of Geological Formations,
May 12-27, 1963) Trudy odinnadt:jatoi sessii... ; 12-27 mais,
1963 g. Moskva.. Izd-vo AN SSSRy 1963. 390 p.
(MIRA 17:4)
1. Akademiya nauk SSSR. Komissiya po opredeleniyu absolyut-
nogo vozrasta geologicheskikh formatsly. 2. Chlen-korrespon-
dent AN SSSR (for Afanaslyev~ Starik).

VlW)GR#llX!V,_&.X., akademik, otv. red.; BARANOV, V.I., red.; BAF611KOV,
V. L., red.; Bk~US, A.A., red.; VALYASHY0, M.G., red.;
GZRASIMOVSKIY, V.I., red.; KGR711INSKIY, D.S., red.; hOWN,
A.B., red.; TUGARINOV, A.I., red.; KHITAROV, N.I., red.j
SHCHERBINA, V.V., red.; TARASOV, L.S,, rod. izd-va; DOROKHINA,
I.N.P tekhri. red.
(Chemistry of the earth's crust]Khimila zemnoi kory; trudy.
Moskva, lzd-vo Aknd.nauk. VoLL, 1963. 430 P. (MIRA 16:3)
1. Geokhimicheskaya konferentsiya, poavyashchennaya stoletiyu
so dnya rozhdeniya akademika V.I.Vernadskogo, Moscow,i963.
(Geochemistry)

VINOGRADOVS A.P.
V.I.Vernadskii; IDOth ahniversary of his birth. GeokhimLiia
no.3tl95-198 Yx 1630 - (KRA 16:9)
(Vernadskii, Vladimir Ivanoviohl 1863-1945)
',~O

VINOGRADOV, A*P*
Biogeochemical provinces and their role'in the organic evolution.
Ge6khimiia no-3:199-213 Mr 163* (KMA 16:9)
1. Vernadsky Institute of Geochemistry and Analytical Chemistryp
Academy of Sciences, U.S.S.R. Moscow.
biogeochemietry)

I
VINOGRADOV,,
Development of V.I.Vernadskii's theories. Pochvovedenie no.S:
1-10 Ag 163. (MIFLA 16s9)
1. Institut geokbimii i analitichaskoy khimii imeni Vernadskogo.

JL 18369-63 EWT(1)/19WF(q)/WT(w)/F!CG (w)/BDS/EW-2/ZS(v) gM/ASP/ESD-
.3
ACCUSSYM NR: AP3005213 Pe-4 WH/GW S/0007/63/000/608/6715/&20
-AUTHORS: Virioizr)dov, A. P.; Vdovy* nX G. P. -70.
Tlq.TE: Diaywnd In stony meteorites
SOURCE: M SSSR.1eokhimiya, no. 8, 1963, 715-72D
TOPIC TAGS: diamond, meteorite
ABSTRACT: Studier; of.meteorites with M gh carbon content confirmed the presence of
diamonds in the moteorites Novy*y Urey and Coalpqra and uncovered diamonds in the i
meteorites DyAlpw, and Ghuhnra. Small portions o" thesa meteorites were ground,
cleaned of their orgAnic (biturdnous) contents, and then troated with noua regia,
I 'greJns. no hnrdness of
.F, EC104 and HCl. The residue consisted of 0-3-0.9-mm
these Frrdrs exceeded 9g, rod their fluorfmcence in ultraviolet licht was greenish.
X-ray analyses of the residue proved the presence of diAmonds. The compositions
and structures of thn four meteorites (three ureilites and one chorkdrite) pre dis-
evssed. The authors attribute the formntion of both graphite and dismonds.to
strPsaes irrosed on enrbonnceous Inclusions durirg collisions of asteroids. Orig.
srt. has, 2 tables and 5 photographs.
,card 1/2

L 18369-63
ACCESSM) FR: AP'1005213
-*SOGTA'.TTCK,: Institut ccokhmimii i annlitic~eskoy khiirdi im. V. 1. Vernadsirogo
INT SOM., Moscow ('Institute of Geochemistry arA Analytioal Chemistryt AN SSSR)
SUBMITTED: 29,MnY(,3 DATE ACQ- Z7Aug63 RIM 00
f--UB CCDE: AS) EL NO PV SOV: 004 OTBFR: 010
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VINOGRADOVY A.P., akademik
V.I.Vemadakii's scientific legacy. Vest. AN SSSR 33 no.3:91-96
Mr 163. (MIRA 160)
(Vernadskii, Vladimir Ivanovioh, 1863-1945)

VINOOMOV; A. P. , akademik
Dating of events of the remote past; symposium hold at Ithans.
Vast. AN SM 33 no.6:84-86 je 163. (KIRA 16:7)
(Qeolog~cal time)

L 12278-63 -vdr(i)/BDs/Es(~L)/ES(J)/ES(c)/M(k) AFM/ASD. Pb-4*
A/DD-.-.
ACCESSION 11M AP30005Z7 S/0020/63/150/002/0411/0413 6
ova, M. V.1
AUTHOR: Vinogradov, A. P. (Academician); ~~in,'V. M.; qM~Sk
Zakharova',~~t-.~-,i-.-]-,-Rroroz7w*y.- 1_W_,Kb
-:---,TITLE i --.Oxygen of --photosynt
hesis and phosphates-
'SOURCEt All SSSR. Doklady v..150s no. 2, 1963P 411-413
:TOPIC TAGS: -photosynthesis oxygen and phosphatebt andocellular water,
!phosphorylation processy Elodea canadensis
~ABSTRACT: This btudy investigated the propcsal by Roux (C, R.j Vol. 251, no. 18j,
1925, 1960) that the oxygen during photosynthesis is formed from the hydroxyl
~radicalv of phosphate ions. M*as==ont of tagged 0 sW 18 in ondocellular water
:and in 'Who oxygen given off by Elodea canadansis in solutions of H sub 2 0 sup 18,,
iKH sub 2 PO,sub 4 sup 18, or Kh sub 2 P sup 32 0 sub 4 suP 18 showed that the
photosynthesis oxygen comas only from water and not from phosphate ions. That
phosphate ions do not enter into th* photolysis (as oppoood to pbosphorylation
process) was further confirmed by analysis of taeged phosphorus in the plants.
"In conclusionp we express thanks to N.-14. Nazarov and K. G. Semenyuk for
-;assistance in this work." ,Orig. art. has: 2 tables.
ASSOCI, tic Chemistry, Academy of Sciences
&TION: Inst. of Geoebamistry and Analy
Card J/Aj

L 24414-6c~ ~-'~T1 V F3 F c, /P c~/P 14 /P,7 - 4
ACCESSION NH: AT5002636 5/0000/64/0021/000/0005/0021
AIMHOR. V1nogN_qdqv,_!~. F
TiTtE: The gag cycle of Lite earth
SOURCE: Geakhimicheskaya konferentsiya KhLmiya zemnoy kory. Moscow, 1964.
Kh im 41 ya zemnoy kory (Cherxistry of the earth'~s crtjsL); trudy konferentsti, v. 2.
Moscow. Izd-vo Nauka, 1964, 5-21
ff-nnn here. -degasification, eartb mantli
4BSTRACT* The author proceeds from the --concept-diat-degis
war, the main -nechinism leading to the formationj in the ea~tl~q
field, of a gascous envelope which was stable but variable in time. The gas
sources exalmined were: the highly volatiLe fractions (mainly water vapor) of the
mantlo, gases and vnj)rjra of cosmic origin, ganes from radioactive (Jecay, gases
from cheiiiical and bfocheinlcj~ rc-action!;, --j-id gases- of exogenous origin, i.e.,
meLeorlLe!', and c,-,~:mic dus, ;',pLic1eF .Th;~, varth's --1LtnoGj)her0 Is analyred 'orlth
respect to Lts gains and io7sc~s owing to, for example, cosmic and radioger~ic
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L 21+414-65
ACCESSION NR: AT3002636
contributiong, fract0nation, and outcropping of gases on the one hand and dissi-
pation and chemical and biological ptocesses on the other. As regards the
character of degasification, the author postulates that the bulk of the vapors
and gases of the earth's atmosphere orIginated through degasification of Lhe highly
volatile frections of the mantle, which brought to the surface of the earth about
content of each gap or vapor. The gases that contri-
)Mpletely Ltansformed the atmosphere, changed the salt
were due e---
an
quence-vl--
app-i-a-rancii - 6 f - a tab le-quant 1 -oxtg-en as--a--consc~quence-*
tirely to Che-- t
photosynthesis. &s a result of oxidation, W, C*114, and 13 disappeared ram Uie
atmosphei7c and hydrosphere, an ozone screen was formed, and the content of N2
increased in the atmosphere owing to oyidation of 14113- Plantq began to extract
the C02 from the atmosphere. -Ine composition of sea water changed oup to a r hange
in the cdf bonate- bicarbonate buffer and sulfate formed through oxidation of S,
HZS? and other compounds. A diagraw of the nain stages in the evolution of the
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L 24414-65
ACCESSION VR: AT5002636
atmosphere is shown in tabular form (see Table I of the Enclosure). Orig.
art. has. 10 tables.
ASSOCIATION: Institut Peokhimii i anal iticheskov khimit Irn. V. 1. Vernadskogo
All SSSR (Geochemistry and analytical cheritstry institute, AN SSSR)
SUIR-11TTED: 22Sep64 ENCL: Q1 SUB CODE: ESD LS
140 REF SOV: 012 OTHER. 031
Card A

L 24414-65
ACCESSION NR: AT5002636
ENCWSURE: 01
Table 1. Diagram of the Main Stages in the Evolution of
the Atmosphere
Surface temperature Componition of the aunosLhere
of earth Main
Components Secondaa components
100 H20 N2v N113, B(OH)31 CO, C02, CH4, HC!,
HF, inert gases, etc.
100 142 C021 CO, CF41 02, inert oases
10-20 02, N2 Ar, C02, etc.
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. ............................
14

AMMSION NRt AP4034717 s/boo7/64/000/005/0395/03,
:AUTHORS: Vinogradoys As F.; Vdovy*kint G. Pei Marov, I* N.
TITLE: Free radicals in the Mighei meteorite
SOURCM Geokhimiya,, no. 5. 1964P 395-398
TOPIC TAGS: electron paramagnetic resonancep meteorite, chondriteg organic radical!
'ABSTRACT: The Mighei chondrite fell in the vicinity of Odessa in 1689s It has been
~previously analyzed chemically, and carbonaceous matter has been determined. The
~present authors have made electron paramagnetic resonance studies on the meteorite
~to determine the structure of this carbonaceous material,, and they have found free
,organic radicals to be present. The spectrum showed hyperfine structure con'e-
.sponding to a complex type of free organic radical. EPR studies were made on otheri
!substances, such as ozokerite,, gilsonite, rock salt, and graphite, butonly coal
showed a similar structure to that observed in the meteorite. It was established
:that the radicals are primary constituents and are not due to the chemical procesaw,
used in treating the meteorite during its analysis hnd the extraction of carbons
Cc]rj 1/2

ACCESSION NR: Ap4o34717
IThe authors conclude that the free radicals were formed either during the evolution~
,of matter before formation of the meteorite or were formed in the meteorite before.,
-it reached the earth. The existence of such radicals must
modify our opinion of
the evolution of matter. Their presence is confirmation of earlier views that
;,simpler organic compoundar chiefly through the radical reactions of polymerization'
;,gave rise to more complex*forms* Orig. art. has& I figure ani 1 table.
ASSOCIATION: Institut geokhimii-i analiticheskoy khimil ime Vo L Vernadskogo AN
SSSR.. Moscow (Institute of Geochemistry and Analytical GhemistryAK SSSR)
ISUBMITTEDs 24Feb64 DATE Ad
Qt 2CKay64 ENCLt 00
,SUB COM ESj, AA NO "REP SOVI 005
OTHERs 00T
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VIN(Xj'RA-nOV A.P.; GRINPIKO L,H,
-.1- -1--~-I..- -1 P
-,L
Effect of enclosing rocks on the isotopic composition of sulfur in ore
sulfides. Geokhlmiia no.6-491~490 Je '64. (YTIRA 18:7)
1. Institut geokhimli I analiticheskoy khImii imeni Vernadskogo AN
SSSR i TSentrallnyy nauchno-issledovatellskly gornorazvedochnyy in-
stitut radkikh, rasseyannykh I blagorodnykh wtallov (TSNIGRI), MosVva.

ACCESSION NRs AP042628 S/0007/64/000/007/0587/06M
AUTHORSt vinagradov, A. Pq Zadoroahny*yp 1. K*
TITLEs Inert gases in stony meteorites
-SOURCEs Geokhimiyap no. 78 1"40 567-6m
'TOPIC TAGS: meteoritep inert gas, age determination/ MV 23 02 maas spectrometer
ABSTRACTi Twenty-one chondrites, three carbon-bearing chondritesj, and one
.achondrite were examined for their contents of He. Me# and A. The gases were ex-
tracted by, heating, the aamples in a molybdenum crucible at 1700C for 30 min- San-
plas were crushed and given preliminary degassing treatment at 150C for three houraq,
-Isotopic analysis wa-3 made on an KV 23-02 1800 mass spoctrometer. The resolving
power of 1~he 5etup w4n greater than 2000. Measuring errors were computed to be,
12-3% for jje4 and 7% for No and A, Most of the stony meteorites contain inert gases'
that may be attributed to three different originst primary, cosmogenicl and radio-
~genic. It, is possible that some A may be of atmospheric origin as woll (adsorption).
Most 6f the inveatigated meteorites contain A and heavier inert gases, but less
corlmonly containHe or Ne. The content, and isotopic composition of Inert, gases
from radioactive decay depend on the.intensity and energy spectrum of cosmic
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i
ACCESSION NRt AP4042628
I I ..
Tadiation, on the duration of irradiations on the shielding effect, and on the
chemical composition of the meteorite. The average isotopic ratios among decay
.products are 0.92 * 0.02 for Me 21/Ne22 P 5.4 + 1 for 1103/NO21, and 8 + 1 for NAAr3~
Yariation in the Zcond ratio is due chiefly-to cosmic radiation, ?Fo grouping of
iradiation ages was.observed# but about, 73% of the determinations gave values less
Uan 109106 years. Determinations of radiogenic age from He are generally smaller
than those from K-Ap probably because of relative losses through heating of the
.meteoritesp but some are larger. The values range from 0,5 to 4.5-109 years. No
,express our sincere thanks to L. G. Kvash and Ye. L. Krinov for supplying meteorite:
;samples aiA making possible the completion of this work.* Orig. art. hast 7
!figures and 3 tablese
ASSOCIATION: Institut geokhimii i analiticheskoy khimii imo Ve Is Vernadskogo AN I
,SSSRs Moscow (Institute of Geochemistry and Analytical Chemistry,, AN SSSR)
:suBmITTEi)i U4xay64 ENCLs 00, '1
SUB ODDE: AAj NP NO REF SM 007 OTHERt 0341-
Card 2

ACCEMION IiRs AP4045065 5/0001/64/ooo/bo9/o643/0846
AUTHORSt Vinogradow, A. P.; Vdovy*kinj Go Fe
TITLEt High-molecular orgaido subatanhe in earbonaceous ohondrites
souRcE, aeommiya, no. 9, 19a, 643-%8.
TOPIC TAGSi meteoritej, or1pnic derivatives electron paramagnetic resonance,
electron diffractions infrared spectroscopys ardaiatic. hidrocarbon
ABsTRACTs The authors investigated the high-awlecular organic mater'. I of
several carbonaceous chondrites by Inrrared spectroscopy, x-ray studies, electron
diffraction., electron paramagnetic resonance spectroscopyj and other methodso
The infrared absorption spectrum of the Higei meteorite shown a number of bandes
the one at 1080-3-175 c**"'L is due to the C-H bond (aromatic) j a weaker band at
i44o eel is due to a der Off group of carbomyl or alcohol; a-strong band
with maximum at 1660 W1 corro"nds to C-0 oscillation in the carboxyl groups
but could be related to adn' se oscillation in the aromatic groups Elemental
analysis of the Stara" SoVidkino meteorite ahowe 17*16% C, 5.47% Hs 2.5% Cls
and 74-79% O+S+N, Via lAgi-062ecular arganio material in carbonaceous chondritoo
is thus food to hm higky condweed &romUo structures Free organic molecules
Y2
--- --- ------ - --

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ACCESMON Mitt AP4045065
have been doteeted in the carbonaceous inclusiona of tho Burgayli iron meteorite .1
and in the Staroye BoriBkinoq Cold Bokkevold, and Groan@" carbonaceous chondrites.
Those molecUlea "a localised in the Higei and Groznaya netooritoaj, but not in the.
other two. Coanic rays were apparently responsible for the development of complex,
IWdrocarbone from simpler form of the prometeorite substance, Orig. art* hass
2 figures and I table.
AMCIATION: Institut gookbinii i analitichenkoy khimJi in. V. L Vernadskogo
AN SSSRs HDecow (Lwtituts of Oeochewistr7 and Andlyti"I Chemietr7j, AN SSSR)
WBM1T=)t 08ju3.64 EWL 1 00;
SUB CMIS AAO OG RD MW SOVt OW OTHMt 005':

[J."T-114OV, V.I.
r the -,re of tLe Shcr--.5u
j' fur aril -~arbll 'r
5 t (lTzt*Vls;un;~ C6c.',.lilml Ij
/MIRA 18s8)
arali tic~i--iski-y ~J-Jmli Imen! V.1.1lernadakego
AN S-,"SRO Kc, s k va .

..VIINOG.RCOV., A.P.1 KROPUTOVA, 0.1.; USTINOV, V.I.
Possible sources of carbon in natural diamonds according to C12/C13
isotope data. Gookhimlia no.61643-651 A 165. (MIRA 180)
1. Institut geolchimit i analitlebeskoy khimii imeni. Vernadskogo AN SSSR,
Moskva.

FATGit~&f6li IMR: AP5018369
UP/0007/65/000/007/0779/0790
t Vinc,~7,,-qd v I A
T T
7- n~
SuWeGg: uew-j-1mya, no. t, ivb5, vf~--tQc
TOPIC TAGSi zone melting, earth mantle, differentiation
On tl-ic '-,is
U gl'P .9 pi-evi~j ;s'-,l propos"ei rien; that cdl:lferen-
~~7 m i r-L~ -L-i r z n
n, U-LT,-lng-pvin-r, nirve is consiaeral)ly hip
per than the
rAj aj)~jt j C C Uy--.r~! and ',:i i fj i, fld 11 P t e!4 t W
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TINCIGRAT01 j, '- _,-,I-ad,3rlk
.=I~~
'i!,zld~ prob2pmz 'T t'-,-- scl.ence-11 --e-sults of the 22d session
of th~ lritemat!~~naj. Corigimris. 'feat.All SSSR 35 no.8*.1,3.-66
Ag 165. (141RA 18:8)

NkLIVKIN, V.D.; RONOV, A.B.; KHAIN~ V.Ye.: 4701OV. B.S.; DOPIRACHEV,
S.M.; TIKHI!r, V.N.; POWER, V.M., FORSH, N.N.j LYUTKEVICE,
Te.M.; SLAVI11, V.I.; SAZONOV, N.T.; SAZONOVA, I.G.;
SHUTSKAYA, Ye.K.; KRASNOV, I.I.; KALEX)VA, G.N.; VINOCRADOV,
A.P., glav. red.; ~, I ~
[Histor7 of the geological development of the Russian PLat-
form and its marginal Irtoriia geologicheskogo razvitiia
Rusokoi, platformy i ee obramleniia. Moskva# Nedraq 1964.
251 P. - [Mapaj Karty. 981. (MIRA 18W

17:
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48340-65 _7
ACCESSION NR: AP5009498
-Central Asia were discussed at three interrelated geographic symposia hold in
--:-Tash.kent,,- Ashldia,-_d~j --and at -A!=-At--.- The f irst-dealt with the- geographical
aspects of Irrigation in Cantral Asia- the second with the problems of desert
conquest and U-,; ouI141rr ',h,3 K~~ru Kun :.anal: tho '.Iiird with the reiT12.1a'._-)r
-A' .71 m.. ier Y '~2 I a A n -.r,t -3
ltie,,~i of watnr ~.ranjplra~.Ion by d_ifferent typon of veget tion. F. F. Day
I -,a
-or qs-)U--~'zaF.. n-
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~L ItR34o-65
ACCESSION NR: AP5009498
9olian sands, and deltalc Jep,.)sits of this rar~ion. R. 1. Varentsov doscribed
~pacts in southeas~.o--.~ tc)pi- ~qs liscus,3F)-i ~7rea ter
pr oz-
d e ta i kvr ~7' X, T3-rfm*.a,--;, 'i -a Li.
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ACCESSION"UR3 AP5009-498
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IhIloGRADOV, A.!,.; IMOHIFOV, A-1.
PT'e-GLY-.brIkn nf Ue 063tPrn part of the Baltic
Shield busud mi- datirg. Trudy Lab. geol.
dol.,.am. 11c.19.7181-204 sr,4, (MIRA 17:8)

F S F'~ I F 3-7
AGG= 10N INK: AF501CY~66 6R/0007/65/000/W4/0387/0389
AUTHORSt Vinogradovp A. P.; Vdovykin, G. P,t Popovp N. H
TITLE: Investigation of carbortaccous matter in misteoritea*by microdiffraction
with ultrahigh velocity electrons
SOURCE: Geokhlmiya, no. 4, 1965, 367-389
TOPIC TAGS: diffraction analysis, electron, electron microscopy, meteorite,
carbon compound
'ABSTRACT- The authors have investigated the structure of the high-molecular
la~rbonaceoua matter in the ator
xy moteorites (carbor-,ceous chondrites) Mighei,
Cold Bokkaveld, and Staroye, Boriskinno, the diamond-bearing achondrite-ureinte
Yovy Urei, and the c-arboraceouB inclusions of the iron meteorite Burgavli. The
ln-79pt~vatlnns vere -nda with a olact~ron microscope having an
-he en-irKy was Kov ano, *~rn v-3vF)-
Lorwath 0.016 1. Allowable thic~_-ess of Ibe, test mterial wlLn Lhis sotup was
3 bc-_i t 1 jj_ , ft nd the &I crod c t I on s 43 j! oc t !-I ty rfinjed up to 0. 05 1.k . I t NMB
',hat tre zp-rberacp,~Tus 'z ~~hor(fr!'_as of
-~rkanlc
str%ic'-urs.
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-1, 4F3337-65
ACCES31011 NR: AP5010666
Extremely fine inclusions of finely dispersed black carbon were also detected,
showing traces of graphiti7at'~on. In th6 Novy Urei meteorite, organic polym~era
are present, bu'~ -raphl-le -41.amc7.~ thFi princilpal car~)onaceous matter.
Ks~k car!D-r. qn-A a7;? alao preperit. I':' *~ne Purgavli
-no a~'-1:.rg
L-P-.e
mp-*.'-er *-I-,e
*--e i3lla-~~-7~ ~--y %ne
bUt -~: ~,)e WtOC'r'-',138 %nEIMBO'~79,9. 7-ey ~c neat -nit *-nJo Jevelo-,mient,
however. Orig. art. has. 4 flgUreS,
A&AKIATION: Institut geokhimii i araliticheskoy khimil im. V. I. Veruadakogo
'-P Ge~chemdfstry ancl Amal7tical 0hp
zs-SR) Institut
-3:. ~-Z
Geoctam;.a txr,
7 Ali. -3,~ R,
SUBMI=Di 01Feb65 ZNCL: 00 SUB COEE AA, NP
90 REIP SOVe 006 OTHER t 000
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L '294-15-55
ACCESSTON NR: AP~00766'--)

ASSOCT-ATTON:' ltnsibllltut mealdhLmii 1 -analitichaskoy, khindl I=.
~-iocchem!sstr-y and
N-R REF SOV: -12
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NEMODRUK, Aleksandr Andreyevich; KARALOVA, Zinaidu KonstunLlnovna;
VINOGRADOV A P akademik., glav. red.; FAIZY, P.N., red.j
d.
(Analytical chemistry of boron (010,811 )) Analiticheskaia.
khimila bora ( 5 B10,811 ). Moskva, Nauka, 1964. 282 p.
(MIRA 17:11)

VINOGRADOV,, A.P.,, akademik; SADOVSKIY, M.A.; AKWSDSAFIN, U.M., akademik;
I.P., akademik; YANSHIN, A.L.., akademik; SHCHERBAKOV,
D.I., akademik; PEYVE, A.V... akademik; ZAYTSEV, L.P., kand.fiz.-
matem.nauk; OVCHINNIKOV, I.M.
Develnpment of earth sciences in Central Asia and Kazakhstan;
results of the out-of-town session of the Department of Earth
Sciences. Vest.AN SSSR 35 no.31128-150 Mr 165.
1834)
1. Chlen-korrespondent All SSSR (for Sadovskiy),
SSR (for Akhmedsafin).
(MIRA
2. AN Kazakhakoy

,VINOGRADOV., A.P.; KORZHINSKIY, D.S.; SMIHNUV, V.I.; SHCHFI(BAKOV, D.I.;
-1- - -'jVff)'LN'YAN, 'I.Kh.; VINOGRADOV, V.I.; VOLtFSOH, F.I.; GENKI-1, A.D.;
DANCHFV, V.I., LUKIN, L.I.; OZEROV.11, N.A.; FERTELIMAN, A.I.; REYHARSKIY,
V.I.; SMORCHKOV, I.Ya.; FFODOTIEV, K.M.; SHOWN, T.N.; SHIPULIN, F.K.
Aloksandr Aleksandrovich Saukov, 1902-1964; obituary. Geol. rud. mestorozh.
7 no.lsl24-12-5 Ja-F 165. (MIRA 18W

ACCLWI(8 IM: AP4042210 6/0020/64/1"/0D2/0388/0391
AMPOR: Uyushteymp X* Teej Chirkov, V* I ~T* A-.!- P Academician
TITIZ: The structure of x-ray K -lime emitted by titanium in its oxides
(TLOO.85 ;- TILOjL.20)
SOUHCX: AN SWR. Dokl&Wp ve 157,p no, 2p 1964P 388-391
VOPIC TAGS; x ray emission liness, titanLuis mmoxide., x ray spectrum,, fine
:structurv
ABS=Cr-. The purpose of this study vas to investigate the fine structure of
/,/x-ray K I,.$ -line wAtted by titanium in specimens videh correspond to titanium
monoxide composition# X-ray studies vere conducted on six samples of the foLloving!
-campositions: TiOO~8 OF TiO , UO UO ; TLO ej Tio 0 in A--- 3 ,.
0 9 -g(2;tojch~LItrjc 1.1 Isition, -
addition Ti spectrum ra; stuWln 20do'closel czm?i
vhich sim4la to titanium monoxide has the RaCl type structure. The temperature
during studies yas 80 - 100 C, The results oQxperhmte an shown in Figures 1
jand 2 of the enclosures The position of K(I band in-tbe titanium spectrum In
Mm; M consUL The greatest differvaces Jn thb
iall- id an remedw, essentially

ACOSSICS XR-. AAOh2210
structure of ium In lower oxidesp corresponding to different
K
intervala of Cho are associated with the differeuce of the relative
4& authors express their gratitude to S. M. Airy
intensity of band components,
'-jwA Ya. V. Vaoillyev for preparation of specimens and Le L Perevalova for the belpt
with the experimental part". Orige art. has: 4 fiVuve md 1 table.
ASSOCMICK: Institut neorgicbeakoy khIml L Sibirskogo *Wleniya Akadev&i nw*
MR (Ltstitute, of Inorganic Mmaistry Riberian BrMch - Academy of ftiences
SUBQTM): 28ftb(A =CL. 02
006
so MW 9MI
Sim cow

ACCZWICN NRI AP404= WCMURXI Ol
KpwmL~5jw lawAs ot Ti, In lower oxides
Fig. 1. The structure Of Us lat
Imental cur"s).
daid 3/4

AOGZSSICN XRs Aphoh2M WCUMMI 02
Ail,
T'llpt,
TLDIXW Two*
ir
IF
%
20 JO so zu 40 is is
TtOLOU Wt178 TIOU91
V,
za JU JV JO .78 zy ju is
rig* 2, M e structure of X&c- emission band of Ti, in its oxides after removal
ackSwund f to the same scale (according
of the b rom Kp, line and after-reduction
a Indicate components of
to the Integni Intwwity of Kp, -line). Dotted-line
the bande
card

_Y~ItQG ; KONDRATIYEV, MI.;
WOV,-A..F,.,),akademikj otv. red.,
akademik, red.; ALIMARE, I.P., reod.; BAK11, N.A., drkt-,r
khim. nauk,, red.; NEMASOVA, G.A., kand. kh1m. nauk, red.
[Isotopes and radiation in chemistry; transactions] lza-
topy i izlucheniia v khim-11; trudy. Moskvaq Izd-vo AN
SSSR, '195~3- 380 P. (MIRA 18.6)
1. Vsesoyuznaya nauchno-tekhnicheskaya konferentsiya po
primeneniyu radicaktivmykh 4L stabillnykh izotopov i lzlu-
cheniy v narodnom khozyaystve i nauke. 2d, Moscow, 1957.
2. Chlen-korrespondent Pll SSSR (for Alimarln).

I t.1- ,
MVSKAYA, Soft~R l,loiseievr,.a, dckTor- 1-Aul. Dit"',ID'VA, lat"yana
Vasillyevpal kan4l. blo2. nauk; VINCGRADOV, A.r,.,,
otv. red. I
(Geochemisti-j of organle matterl Gcokhirriia organtche::kogo
veshchestva. Eoekvay Naukri, 19~4. 314 ii. (INIPA 18- 1.)

-1110V
,,amuil Vladirdrovicb;
YELINSOU)
PI-01'.. retsenzent r
V.1.9 . .. -1 ea
Vjj,,OC.P.ADG'I akademlf~p 6-
of zirconiul" lo(
[Analytical chemistry oniia i gafniia. "~`Kval
che-.kaia. klilidia tsirk KI 1~ it
239 P.

L 34096-66 EWT(J) M
ACC NR: AP6008803 SOURCE CODE: UR/0007/65/000/011/1275/1312
AUTHOR: Vinngrndnv- A_
Im. V. 1. Vernadakiy, AN SSSR,
ORG:
Moscow (Institut geokhimii i analiticheskoy kh1mii AN SSSR)
TITLE: The substance of meteorites pe
SOURCE: Geokhimiya, no. 11, 1965, 1275-1312
TOPIC TAGS: meteorite, mineral, cosmic ray effect
ABSTRACT: This comprehensive review of the literature on the composition of meteorites
consists of the following sections: composition and classification of meteorites, fraction-
ation of the chemical composition of meteorites, products of cosmic Irradiation of meteor-
ites, a discussion of the extent to which the composition of meteorites reflccts the compo-
sition of the meteorite belt, the origin of meteorites, and the problems of cosmochemiBtry
of the immediate future. The distribution of brecciated forms and polymorphous alterations
in meteoritic matter to indicative of collision and agglomeration of heterogeneous matter
Card 1/2 UDC: 550.4:552.6:551.12

L 34096-66
ACC NR- AP6008803
resulting in the formation of different meteorites, Molecules containing Mg, Fe, and other
meta- and orthosilicates, the feldspar structure, etc. are the major components of the
silicate portion of the composition of meteorites. Iron-nickel alloys and to a lesser extent
trollite, chromite, phosphides, carbides, etc. form an independent phase. Since the
number of minerals constituting meteorites is approximately 50, while there are about
5000 minerals on earth, the chemical fractionation of meteoritic matter must be different
from the magmatic differentiation of the earth's crustal matter. The main composition of
chondrites, achnodrites, iron-stony and iron meteorites is considered with special empha-
sis on the content of cosmic radiation products, I. e. , neutral gases and long-lived
Isotopes. On the basis of statistics it Is postulated that the composition of meteorites
fallen and found on earth Is not representative and apparently does not reflect the true
composition of the matter of the meteorite belt of the solar system. Orig art. has: 18
figures and 16 tables.
SUB CODE- 03 / SUBM DATE: 06Aug65 ORIG REF: 033 OTH REF: 124
Card 2/2 V111b

L*04702-67
ACC NRt
FSS-2/LWT0)/EWTW/FCC f~'JiT/TT/GW
~P~628010 . . I SOURCE COUE:
AUTHOR: VinogEadov, A.-PL; Surkov, Yu. A.; Chernov, G. M.; KArnozov. F. F.;
,Nazarkind,f~"
ORG: Institute of Geochemistry and Analytical Chemistry im._V. I. Vernadski
AN SSSR, Moscow (Instilut-geo i ana ticheskoy i
TITLE: Measurement A~a-radiation of the lunar s face by the Luna-10 spaceship
(Paper presented at the Seventh CUSFAR Neeti-a-g-Eeld in Vienna in May 19661
SOURCE: Geokhimiya, no. 8, 1966, 891-899
TOPIC TAGS: radiation measurement, gamma radiationp moon, lunar probe,
scintillation spectrcmater
ABSTRACT: The spaceship Lumn-a-1100, placed into a selenocentric orbit'on 3 April
1.966, was equipped with a 32-channel scintillation spectr9me-terTo investi-
gate the intensity -and spectral composition A y-radiation-eirnitted from the
Y'
lunar. surface. The absence of an atmospherW-_-3WT1-c-Wnt1 ~ dense to absorb
Y
Y-rays makes it possible for a spaceship in lunar orbit to register Y-radiation.
However, the counting rate measured from an orbiting spaceship decreases
as a result-of a -decrease in- the solid angle subtended by the visible surface

L 04702-67
,~C(~R -A ~80D~-
of the Moon, which was 0. 9'9 at periselene and 0. 46v at aposelene in the
initial orbit.
It is known that the content of natural radioactive elements (U, Th, K40
in terrestrial rocks decreases from acidic to basic to ultrabasic rocks and
that the decrease covers a range of several orders of magnitude. Therefore,
it was expected that it would be possible to determine the type of rocks
present in the lunar surface from the relative content of U, Th, and K
established from the the -tray spectrum. In conducting the experiments, the
fact that the level of Y-radiation from natural radioactive elem6nts can -
be lower than the level of Y-radiation produced during the interaction Of
primar cosmic particles (primarily protons) with the lunar surface was taken
-- Y - - . . --I
into account by analyzing the characteristic Y-rays emitted during the
interaction.
%s- tnunentalion
The measurements were made with a scintillation spectrometer
consisting of aax 4-cm Nal(TO cylindrical crystal Y-ray detector -with an
FEU-16 photomultiplier and a pulse-height analyzer. To eliminate the back-
Card.

L 04702-67
ACC NRt
ground from charged particles, the NaI(71) crystal was enclosed in a container
of a thin plastic scintillator. The pulses generated by charged particles were,
registered by the NaI(TI) crystal and the plastic scintillator and were then
separated from the pulses generated by Y-rays which went practically
unregistered by the plastic scintillator.
The scintillation spectrometer recorded Y-ray spectra in the energy
ranges between 0. 3--~-3.1 and 0.15-~-l. 5 Mev. The switching of energy ranges
was performed by ground command. The detector and the analyzer of the
spectrometer wem 1cpated in a hermetically sealed compartment under a shell
1 g/cm 2thick.
Eae~impn!Lal j!esHIts
Six Y-ray spectra in the energy range 0. 3-3.1 Mev were obtained during
t4,e first month of operation of Luna 10. In addition, the integrated intensity
(it Y-radiation in the same energy range Was obtained at approximately
points.. The measurements were conducted over relatively wide surface
01areas covering the continents and the seas on both the light and the dark
sides of the Moon.. The height and the approximate selenographic coordinates
Card 3/15

L 04702-67
ACC NRs AP6028010
of the regions above which, the spectra were measured are given in Table 1.
Table 1. The Height Above the Lunar Surface and the Selenocentric
rnnvMna+~Pa nf thp RezinnR Abnva Which Measurements Were-Made
No. of

spec- Date and time

of measurement er,fe
i~h
bo e
Selenogra. hic
latitude YDeg
) Selenogrq~hic

longitude (Deg)
trum surface Start End Start 1 End
1 5AIr 19 h 26 m 350 +70 +62 185 _
228
2 5 Aly 20 h 11 m 600 -22 -4o 272 279
3 Bppr 4 h'45 m 700 -.47 -63 253 273
4- 9AJpr lh 37 m 600 -53 -64 25'2 2.72
5 appr 12 h 45 m 6oo +30 [phone]
6 21 tir 13 h 56 m 1000 -58 -45 208 220
Fig. I (ourve i) shows one of the primary y-ray-spectra fgPectrum No. 3
in Table 1), taken above the dark side of theMoon. The background due to
Card 4/15

1, 04/02-6Y
-AdCkft
H
-0
V .Y
Energy (Mev)
~ig. 1. Gama-ray spectra obtained by Luna 10 while
in orbit around the Moon and along the trajectory of
the flight from the earth to the Moon
'15

L 04702-67
1 - y-ray spectrum of the lunar rocks together with
the background; 2 - y-ray spectrum of the background
due to interaction of cosmic rays with the material of
Luna 10 corrected for the screening by the Moon; 3 and
4 - same spectra as those given by 1 and 2, respectively,
recalculated to represent measurements which would be
taken at the surface of the Moon. The errors shown are
root-mean-square errors.
interaction of cosmic rays with the substance of Luna 10, taking the screen-
ing by the moon into account, is also shown in.Fig, 1 (curve 2).
Compared to the counting rate of y-rays measured along the flight
trajectory, the counting rate in orbit around the Moon increased by 30-40%.
As a result of the screening effect of the Moon, th.e background due to
irradiation of the spaceship by cosmic particles near the Moon decreases
and is equal to about 78-89% of the background encountered along the trajec-
tory of the flight. The background spectrum was measured during the flight
Card

_-Acc NR,'_AP6028o1a
of Luna 10 toward the Moon at a distance of about 230, 000 km from the Earth.
'The principal part of the Y -ray background registered is associated with
.inelastic Interactions of charged particles with the substance of Luna 10 and
is not primary cosmic Y-radiation. The natural radioactivity was small due
to the small amounts of K, Th, and U present in the spaceship. There were
no radioactive sources aboard the Luna 10. Fig. I also shows curves cal-
culated so as to represent measurements that would be obtained directly at
the surface of the Moon. Curve 3 in Fig. I shows the Y-ray spectrum at
the lunar surfac6 together with the background due to irradiation of the space-
.ship, while curve 4 in Fig. 1 shows the background alone.
Fig. 2 (curve 1) shows the spectrum of Y-radiation of lunar rocks
(after subtraction of the background) obtained by Lunar 10 while in orbit.
7his curve represents the difference between spectra represented by curves
.1 and 2 of Fig. 1. Fig. 2 shows that the lunar x-ray spectrum differs con-
oiderably from the spectrum of Y-radiation emitted by the surface of the
Earth [not shown], the shape of which is primarily determined by the content
of natural radioactive elements in the rocks. A distinguishing feature of the
lunar *f -ray spectrum is its relatively flat slope and large number of
Ca,d 7/15

-AcCrA- --AP6a6Oib--'-'-- V
0-51 Annihilation peak
IF Fig. 2. Gamma-ray spectrum 6r lunar'-
It rocks obtained by LUna 10 while in
,u 4~ 0~~j orbit around the Moon
I Y-ray spectrum of lunar rocks with,
the background substracted from the
curve; 2 - y-ray spectrum associated
j with the interaction of cosmic rays
0
U t, with lunar rocks (prompt y-radiation
0 and decay of cosmogenic isotopes),
x 101 3 - spectrum of y-radiation associated,
with decay of natural radioactive
elements K, Th, and U contained in
2 lunar rocks.
b0
93
.A
1.77
0 121-2,$j
I f
Energy-Nev)
Card
- j, 5- U- ---AL-A

L 04702-0
ACC NR, AP6028010
hard Y-rays with energies in excess of 1. 5 Mev while the spectrum of natural
radioactive elements is characterized by a steep slope at higher energies
and the absence of -i-rays with energies greater than 2. 62 Mev. This shows
that most Y-radiation from the lunar surface is not associated with the.
40
natural radioactivity of U, Th, and K but is the result of the interaction of
cosmic rays with the lunar substance and the decay of cosmogenic isotopes.
Table 2 shows ihe characteristic Y-rays identified from the lunar.
Y-ray spectra-and the principal nuclear reactions involving the probable
constituent elements of lunar'rocks. It can be seen from Table 2 that 0,
Si, Al, and Mg are likely the most widely distributed elements in lunar.
rocks.
Table 2. Energies of Gamma Rays Identified From the Lunar
Gamma-Rav Sueetra
ergy

M
(Mev) Principal Nuclear Reactions Causing Emission of
Characteristic Gamma-Rays
0,811
APT (pj,'j) A127, Sisd (p.2p-,) A127. FeAd (P,P'I) Feld
1,0t All? pp,.j),%l24. Si26 (p,2pity) AM
1,37 N1,131 (P.,)") Mg24, All' (p,pl-.) Mg24, SPI (P.Piy) Mg"
*
1,78 p.%-.) Ne'O. All' p.2pT) Mgt$. Sill (P,P,T) Sill
(r.
2.31
.2,02
011 kj,.,.,.pa*.) N14. Mg" (ppq) AlgI2, Mgls (p.2py) Na2s, Alt? (p.piny) Mg1l
ardq&S ------------- W.J

L 04702-67 ,
FA_CC_ NRt AP6028010
Since the lunar surface is exposed to constant interaction with cosmic
rays, all of the cosmogenic radioisotopes should be in radioactive equilibrium.
Therefore, both long-lived and short-lived radioisotopes should be radio-
active, and their content should be proportional to the effective cross sec-
tion for their production. Calculations show that the main contribution to
'Y-ray emission is made by the decay of the following cosmogenic isotopes:
0 14 (T 7 2 se c, E = 2. 31 Mev), 0 19 (T 27 sec, E = 1. 37 Mev),
Y 22 Y
.F20 10. sec, E Y = 1. 63 Me-;), Na (A/2 = 2. 6 hr, E 1. 28 Mev),
Na2 (Tj = 15 hr, E Y =1.37Mevand2.76Mev). These raJioisotopes are
formed with a considerable yield in nuclear reactions involving the same
rock-f orming elements: Mg, Al, and Si.
The peak at 0. 51 Mev, which is especially pronounced in the lunar
Y -ray spectra measured in the energy range 0. 15-1. 5 Mev, is produced
by Y-radiation emitted during annihilation. -
Analysis of the results shows that the Y-radiation intensity corrected
for the difference in height is practically constant above the different regions
of the lunar surface (intensities did not differ by more than 4076). This can
probably be attributed to the fact that the main source of Y-rays is cosmic
radiation. A preliminary analysis shows that the total dose rate of
Lqq~,_d 10/15

L 04702-67
'-Acc
y-radiation above the lunar surface is somewhat higher than the do'se rate
above the rocks of the Earth' s crust. The dose rate of Y-radiation
em itted by the.lunar surface is roughly 1. 5-2 times-grqater than that emitted
by terrestrial granites (14 Pr/h).
An evaluation of the natural radioactivity and the concentration of
natural radioactive el4ments can be made by substracting the effect of
Y -radiation produced in the ineraction of cosmic rays with lunar rocks
from the overall lunar *-ray spectrum. Although the exact shape of the Y-ray
s ectrum induced by cosmic rays is unknown, approximate results can be
ottained by using the shape of the spectrum obtained along the Right trajec-
tory of Luna 10 from the Earth to the Moon. Curve 2 in Fig. 4 shows the
sppctrum. of Y-radiation from the Moon produced by cosmic rays, determined,
by~combining the Y-ray spectra obtained along the flight trajectory with the
Y-ray spectrum of the lunar rbcks in the energy range exceeding 2 Mev (the
contribution of the natural Isotopes is almost zero). This approximation is
justified only if the t-ray spectra induced by cosmic rays in the spaceship
and in the lunar rocks have the same shape and differ only in intensity. This
Assumption was demonstrated to be jUstified by both theoretical calculations
'and modeling experiments performed by the authors. The validity of this

ACCAM-7ATOZ801-07-
assumption follows from the fact that the spaceship and its components were
made of light alloys of Si, Al, and Mg with very little Fe, I. e., the dominant
elements in the composition of rocks. Curve 3 in Fig. 2, obtained by sub-
tracting curve 2 from curve 1, shows the-y-ray spectrum produced by,the
decay of natural radioactive elements. Fig. 2 shows that 9016 of the Intensity
of gamma radiation emitted by lunar rocks is produced by radioactivity
:induced by cosmic rays and no more than 101o by decay of K, Th, and U.
Prior to the flight the Y-spectrometer aboard the spaceship was pre-
calibrated using samples with a measured amount of K, Th, and U and also
with rock samples containing different amounts of these elements. Ibis
procedure made It possible to calculate the Y-ray spectra, which should be
obtained by the orbiting spaceship, emitted by rocks with different amounts
of natural radioactive elements (it was assumed that the radiation produced'
.by cosmic rays is absent). Fig. 3 shows such spectra which would be
'obtained at a height of 350 km with the b~ackground'subtracted from the
,Spectrum. The hatched areas correspond to range of concentrations of
radioactive elements for given types of rockv The average values of con-
centrations of K, Th, and U were taken from a paper by A. P. Vinogradov
(Geokhimi a, no.. 7, 1962).
y
Card 12/15

L-04702-67
ACC NRj AP6028010
Comparison of the lunar -(-ray spedtra with those of terrestrial rocks
.with a known content of K, Th, and U shows that at least in the.regions of
the Moon'over which measurements were conducted there are no rocks on
the lunar surface; or at a depth not exceeding 27 cm, containing the same
amouht of K, Th, and U as do the acidic terrestrial rocks, such.as gran-
ites. The intensity of y-radiation due to natural radioactivity (Fig. 2,
curve 3) tends to indicate the presence of basic rocks such as ba~alts.
However, at the pres6nt time it is impossible to exclude the possibility that
the concentration of natural radoactive elements was estimated a -bit too high.
It is interesting to note that tektites, which have almost the same composi-
t4on and amounts of U, Th, and K as acidic rocks, cannot be Qf lunar origin.
Conclusions
The main results obtained from the measurements of the intensity
~,qod spectral composition of -r-radiation by the Luna 10 can be summarized
follows.-
1. The overall level of Y-radiation of the lunar surface slightly exceeds that
of the Earth. Preliminary results show that the intensity of 'Y-radiation of

L 04702-67-
ACC NR, AN
LGard
_P
Cd
;-4
b0 101
0
10
Fig. 3. The y-ray spectra of lunar rocks
which would be observed by a spaceship in
granites orbit around the Moon. The spectrum was
calculated from the y-ray spectra of
natural radioactive elements on the assump-
tion that the relative contents of K, Th,
and U in lunar rocks correspond to those
occurring in the most important terrestrial
/~S/
L rocks.
LhS
ultrab
rocks
Energy. of y-rqs (Mev)

1, 04707-6/
__ - kP6028016
ACC NR,
the surface of the Moon is 20-30 0 r1h.
2. About 90% of the 7-rays emitted by the surface of the Moon Is produced
during interaction of cosmic rays with lunar substance (prompt Y-rays and
decays of cosmogenic isotopes).
3. The basic rock-forming elements of the lunar surface are believed to be
0, Mg, Al, and St.
4. No differe.nce was noted in intensity of y -rays emitted by different re-
gions of the lunar surface including the seas and the continents (variation of
intensity did not exceed 4076).
5. The decay of K, Th, and U in lunar rocks does not contribute more than
1076 to t'he total -Y-ray emission of the lunar surface.
6. Comparison of the intensity of -y-radiation from the decay of natural
radioactive elements K, Th, and U with the results obtained by a calibrated
instrument from terrestrial rocks.'shows that the concentration of radioactive.
elements in lunar rocks is close to that of basic terrestrial rocks and differs
,greatly from acidic rocks. However, it can not be posiUvely stated that the
lunar surface contains no ultrabasic (meteoritic) substance. At the present
time an attempt is being made to determine the relative content of 0, Mg, Al,
and Si in lunar rocks from the available Y-ray spectra produced in interac-
tions with cosmic rays. Orig. art. has: 3 figures and 3 tables. [FS3: v. 2, no. 103
SUB CoDE.: 22 SUBM DATE: 24Jun66 / ORIG RU : 002
Ca!d 15/15

ACC NRj AP7005449 SOURC3 COD~_:_ U-q/oo~o/66/i7o/oo3/o561/o~%4-_
jVJ7ATO:t; Vinor;radov, A. P. (Academician); Surkov, Yu. A.; Chornov, G. RA10
W-.G: and Analytical Chemistry in. V9 1. VornadrMy, MI SSS11:
(Institut gook-hirdi i analitichaskoy Idiiaii All S33111)
i TIM: Lwestigations of the intensity and spectral composition of lunar ea=
radiation on the automatic station "Luna-1011
SO =,S: AN SSSR. Dolda4y, v. 170, no- 3, 1966, 361-564
TOPIC VMS: rarama apectsrum, gamma spectrometer, scintillation spoctromotor,
bromsstrahlung, cosrao radiation, moson, lunar satellite. photozoultiplior/Luna-lo
lunar satellite, F'U-16 photomItiplior
A33MML: IQ=-1011 cm-ried a scintillation ga=a spectrometer with a detector of
Y-radiation; this was a Nal(TI) crystal measuring 30 x 1#0 m, connected to a 7,z*,U-16---1
phottomilUplier, and a pulse amplitude* analyzer. The instrument made it possible
to wasure the spectruzi of It-radiation against a background of charged partic1c's.
!-1he instrument recorded the spectrum of 'r-radiation in Uro ranges: fron 0*'3 to-3.1
KaV and from 0.15 to 1-5 Mfov. During the first nonth of operation of "Luna-logo it
'was possible to obtain 6 spectra ofY-radiation in the energy range from 0o3 to 3-1
VIeV. In addition, at approximato2y 15 poirVta the intensity of Y-radiation was mea-
Isured in this same range of energies. The measurements covered rather ortensivo area-.
of the surface, :Including both the "continentill and 11ceas" on both the visiblo and
Ifar sides. Analysis of the form of the lunar Y-spectra. revealed that they differ

ACC NR, A?7005449
considerably from the spectra of terrestrial Y-~P.--~Lntion. whose form is doterzdned
for the most part by the content of natural radioactivu olnmnts in rock. For tho
moon the graater part of the -r-radiation is that arising du~r~q; 41--toraction of coszdcI
4:kie przLnu.L
rays with lunar matter and from the decay of cosmogenic rad~oiuMopog6 ,,1.22, and
contribution is from the follotring cosmogenic isotopes*. 014,
Table 1 gives the onorgy of gamma rays identified in the Linar gamma spectrum. Tn
addition to nuclear reactions leading to the omission of charaqtoristic Y-quanta
(instantannouslf-radiation and the decay of coamogenic isotopes) there is some con-
tribution from processes of the decay of 7c'mosons and the brensatrahlung of olec-
trons and protons. Preliminary data indicate that the total intensity of prma
radiation on the lunar surface exeeodu the intensity over-the rocks of the earlth's
crust by 1.5-2 times and changes little from or* part of the lunar surface to another.l.
About 90% of the gamma radiation of lunar rocks can be attributed to the effect Of
cosmic rays and not zore than 10% is due to the decay of K, Th. and U. Orig. art.
bas: 1 figure and 1 table, DPiW: 38.67Z7
SUB CODS3 22, 3.8, 20 / SM DATEs . 23JUn66 OM RUt 003
L

ACC NRs AP603lo62 SOURCE CODE: UR/0007/66/000/009/1106/1109
AUTHOR! Vinogradov, A. P.; Vdovykin, G. P.; Karyakin, A. V.; Zubrilina, M. Ye.
ORG: Institute of Geochemistry and Analytical Chemistry im. V. 1. Vernadskiy,
AN SSSR, ~bscaw (Inatitut geokhimii i analiticheskoy khimii AN SSSR)
TITLE: Investigation of the organic compounds and diamonds of the Novyy Urey
meteorite by infrared absorption spectroscopy
SOURCE: Geokhimiya, no. 9, 1966, no6-ilog
TOPIC TAGS: meteoritics, diamond, istrx9re-d abso tion spectroscopy, organic
compound, meteorite / 19 T"ImAtTli a,-Af
ABSTRACT: The organic compounds and diamonds of the Novyy Urey meteorite, which
fell in the Gor'kiy oblast' in 1886, are investigated by means of infrared absorption
spectroscopy. The Novyy Urey meteorite, like the Goalpara meteorite with which it is
compared, is an ureilite. Specimens were examined with the UR-10 quartz spectrograph
The organic compounds were extracted with chloroform, while the diamonds were ex-
tracted by fusing the meteorite powder with Na202. The presence of the CH and CH
groups was positively confirmed, while the presence of C-N-H groups was t 3 ought
possible. The organic matter was represented by paraffin hydrocarbons. In the
infrared spectrum of the diamond fraction, absorption bands appeared at 500 'Cm_1 end
especially at 900-1300 cm7l. - These absorption bands are characteristic of type-I

ACC NR, AP6031062.
,diamonds containing and admixture of nitrogen in their crystal lattice. 7be presence
of nitrogen in the diamonds of the Novyy Urey meteorite is thought to suggest a
genetic raltionship between ureilite diamonds and the carbonaceous matter in chon-
drites. The nitrogen, most probably, was captured by the dip-nds during crystalli-
zation resulting from a collosion with asteroids. Orig. art. has: 3 figures. [DMI
SUB CODE: 03/ SUBM DATE: 21Apr66/ OTH REF: 002
Card 2/2

ACC
SOURCE CODEt UR/0007/66/000/008/0891/0899
'AUT11ORt Vino&radoV, A. Pe; Chernov. G. M.; Kirnozov, F.
Nazarkina, G. 0.
.y and Analytical Chemist
ORGt rY ime V. I* VernadsklZp
-AS SSSR- MtqqK,(rnstItut gookbimil ImIFANMSR)
TITIZ: Measurements of gnma radiation of the lunar surface by the space
station Luna-lo,0
SOURM Geol(himlyat no. 8,, 19660 891-899
70PIC TAGS: Gamma specermi, lunar satellite, enrth crust, lunar surface,, lunar'
radiation / Luna-10 lunar satellite
ABSTRACT:
Lu
During its first month or operation the lunar satellite 11 na
VYI obtained six Dpoctra or gamma radiation in the energy range from
PJ to 3-1 MeV- In additiono at about 15 points it measured the total
.'intensity or gamma radiation in.the namo energy rango.'~Tho measurements,
covered extensive areas of -the surface of both tho uead and continents
'on both aides of the moon. it was found that tho general level of g
radiation of lunar rocka.approachas the level-of gamma7radiation over.
the rocks of the earth's crust,, somewhat excooding the latter* The pr*-.
liminary estimate or gamma radiation for the lunar surface is 20-30 P
curies. The principal. contribution to lunar gama radiation is from
processes of interaction of comic rays with lunar matter (inatantineous,
g==& radiation and the decay or isotopes), About 90% of the total
lunai~,.gamma radiation can be attributed_j4o. these p~rocessee Ana4sis

.CC NRi Ai'7005118
makes it possible to identii~r in the lunar spectru'm photopeaka from
amma quanta emitted at the time of interaction between cosmic parti-I
.cles and the principal rock-forming elements of the lunar surface
-00 Ylge Al, Si, as well as gamma quanta emitted during the deiay of
cosmogenic isotopes. (The possibility of dotermining the relative
content of these elements now is being studied.) Results of measure-
ments over different regions of the lunar 3urface, including the aeaz
-and continentsPdid ncV, reveal an appreciable difference in the intens-!
lity,of g=na radiation over those regions (intensity variations do not
exceed 40%). In the total intensity of gar.= radiation of lunar rocks
the percentage of radiation caused by decay of K, Th and U is approxi-
mately 10%. Comparison of the intensity of gamma radiation from decay:
.of the natural radioactive elements K,, Th and U with the results of
calibration of the instrument against terrestrial rocks makes it poe-
sible to ascribe to lunar rocks concentrations of radioactive elements
close to terrestrial rocks of basic composition (such &a basalts)*
The OA&UAicate that. +.heir^ %rq no. a"na of - rocks with conoontrations
of radioactive alemonts such'as terrestr141 aranitesp and especially none
vlth ors centration f K9 Th and Ue Orig. arte hams 3 figures wA 3
tables, MPBSs 3894:60~0
SUB CODEs 03922,20 SUBm DATEI 24Jun66 ORIG REFt 002

ACr, NR, Ap7002296
SOURCE
CODES
UR/0020/66/168/004/0900/0903
AUTNORS Y~qqgrad0V,_A.__R.; J?qy1rts*_A.,-L.; 1~~b4lnaj, E.- I.
.~I~stltute of Gcochemistr and Analytical Chomistry,im. V. 1. Vernadl~kix___
AN SSS.R.(Institut gookhimit i analiticheskoy khImil AN SSSR)
I=S, C14 the time of the Tunguska Catastrophe ,
concentration in the atmosphere at
and antimatter
'~tOURCE: AN SSSR. Doklady, v. 168, no. 4, 1966, 900-903
.-MDPIQ!TAGSt meteorite* antimatter Tanguska meteorite
A ",!K4.wl :o
Cowan, Atlury and Libby analyzed a number of hypotheses on the
claiJ, the explosion of the Tunguska meteorite; they concluded that the
,,~,qyLtima'tter hypothesis most satisfactorily explained all the accompanying
'6`~Siib'Aa;~', If antirdatter*, in fact, was responsible, there should have been
p
0 -
an ass6~ia~'ted increase of radioactive carbon. Accordingly, this paper de-
.sclr~-bei qn~-investigation for determination of C14 in tree rings in the im-
le iatdc-Ire'a of the Tunguska explosion (60 km to the south of the epicenter).
Thp 140-year-old tree was cut in 1961. The growing season for the tree was
tsuAlltliat any increase of C14 would be reflected in the tree ring for 1908.
Other'rings also were studied 1885-1890.(qs.a control),,1894. 1901, 1907,
UDCi.-550.4----

00,2-2-96
i913. All other' *fa tors- whfc~ -could _aZio'unt-f o~' indreases,
c
7 ]1:908,,,.;,.9q9, 1910,
.ior variations of C14 content were taken into account. No evidence was found
which would justify the assertion that the so-called Tunguska"
,41,basis Is
jp~ jt~
wiks, related__kq _the_pe etration of antimatter into the earth
:&tas~qbphe n
OrIg. art. has: 3 f I
-gures.- 6iRSs 3793977
20903 SUBM DATEs 23)kr66 ORIG RErs We,/ on RZF, 008
I CWd 2/2

ACC NR: A.'7007599 SOURCE CODZ: UlU0293/66/004/006/0571/0379
AUT'10q: -Vnogradov, A. P.; Surkov, Yu. A.; Chornov, G. M.; YIrnozov, F. F.;
TITLE: Preliminary results of neasurements of gamma radiation of the
lunar surface onithe space station "Luna-1011
SOURCE: lZosmichaskiye Issledovaniya, v. 4, no. 6, 1966, 871-879
TOPIC TAGS: lunar satellitet gamma spectramater, cosmic radiation
SUB CODE: 22, 20,18
ABSTRACT: Experi'mentol Inve5tigations of the Intensity and spectral
componsition of gamma radiation of lunar rocks made using a gamma spectro-
meter carried aboard the automatic station "Luna-101, demonstrated that:
1) The general level of ga-=a radiation of lunar rocks approaches the
level of gwi= radiation over rocks of the earth's crust, somewhat
exceeding the latter. According to a preliminary estimate, the intensity
of the gamra radiation at the lunar surface Is 20-30,AjR/hour. 2) The
principal contribution to lunar gamma radiation is from processes of the
Interaction of cosmic rays w1zh lunar matter (instantaneous gamma radiation
and the decay of cosmo.ffonic isotopes). About 90% of the total lunar gamma
radiation can be attributed to these processes. 3) Analysis made It
possible to identify in the lunar apact-rum photopeaks from Camma quanta
emitted during the interaction of cosmic particles with the principal
rock- f ormi ngy elements of the lunar surface -- Oj 11gs Al, Si -- and
gamma quanta emitted during the decay of cosmogenic isotopes. 4) Tho
results of mcasurcments over different rozions of tho lunar surfaces,
IncludInG the ragionz ia-` the lunar fleon.11-inents" and Seas" did not mako
Card 1 2 LTM 629.195.3!523.36
094-Iff 115-WXY --

ACC.NR:AP7007599
possible detection of an appreciable difference in the level of intensity of
garna radiation over these regions (the changes of intensity do not ex-
ceed 40%). 5) In the total intensity of ganna radiation of lunar rocks
the porcenta.-o of radiation caused by the decay of X, Th and U is not
greater than 10%. 6)Comparlson of the intensity of gamma radiation from the
decay of natural radioactive elements X, Th and U with the results of
Instrumient calibration.against terrestrial rocks makes it possible to
ascribe to lunar rocks concentrations of radioactive elements close to
terrestrial rocks of basic compositi6n of the basalt typo. The
collected drata. make It possible to exclude for those regions of the lunar
surface whore the measure-ments'Mro made the existenco of rocks with a
content oA4 the radioactive elements X, Th and U such as In terrestrial
acidic rocks (granites)'and ospocially rocks with oro concentrAtions of
thoso elements. Orig. art* hast 3 tables and 3 figures. Linst 39,71 7a
ORG: none
,Ca.rd 2/2

ACC NR; Ai,700.5879 SOURCE CODE':
Airl*iOF: %Iinogradov, A. P. (Academician)
C-
Gccc-.e.%,,.Ica1 probleMis of developaPnt~ of the ocean
S T ;~z C, 7 :36-. Vestnik, no. 9, 1966, 93-97
AN
.LoPIC TAGS: geochemistry, oceanographic conference
:,U3 COD!, :06
of % report by Acadoinician A. 1'. Vinogradov,
prc3c:-.ted at. the Intcrnat-Jon.L1 Oceanographic Con."rons in Moscow, now
has been publio~cd. In this papcr he con5ldered the General dcvclop-
of the occa;,,, with nccoo3axy consideration of the evolution and
diffc.-entiation of the dccp la,,el-s of I[Ihe earth. As part of thlo
P-110cess ne P,35tuiatcs the. as a result of degasification the outpour-
inc- of basa-I's al,~,rays brouj[~-it 1.~o the surface an average of 7,1. by aeight
of, Juven-LIC ,.are-, --n. the forn of water vapor or In a liquid state. H'a
also pos-_Ulatz~s the ratio between the mass of ejected basalt, ".-al"er
14ttle Jn geological time. He contends that the nain
cn=gos
,,.-nss of -iater -.ust have arrived at the earth's -surface in the process of
-Por---tion, and devolopmeat of the continents and only a minor part of it
in thic zrocca~; of formation of the basaltic oceanic crust* This con-
cl:,sion, paradoxical at first glanco, suEz-eata that the change,of the
voltune of water in the occan and chango of its level was determined pri-
marily by development of the continents. Orig. art. has: 2 fig,-4res.
rjpjS:
L 318,9371
.-Card UDC: 551-.4k: __550-A-

~- ---
" 1 *. 7 . " .1 1-:,- 1 i. :'I , ".
B;It i q , I.. I.. t I I -, U, - ~LLL- - . , ; jj
teather
Classification of hard leather. Leg. prom.,
No. 3t 1952.
Monthly List of Russian kccessions, Library of
Congress, June 1952. Unclassified

1. VINOGRADOV A-p-
2. USSR (600)
4. Leather Industry Standards
7. Units of measurement for heavy leather. Leg.prom. no. 12, 1952
Monthly Lists of Russian Accessions Library of Congress, tEchj 19531 Unclassfied.

V % tf 0 CrRhDO V, ~j - P -
ZTBIN, Yu.P., doktor takhnichaskikh nauk, professor; STESHEY. I.1., retsenzent;
vrll~ ~y A.F., retsenzent.
[Technology of footwear] Takhnologila obuyi. Moskva. Goo. nauchno-tokhn.
izd-vo KinisterstTa. prouqehlennykh tovarov shirokogo potreblenlla Sm,
193-3- " (KLRA 7%6)
(Shoo industry)

ZYBIN, Yuriy Petrovich. doktor tekhnichookikh nauk, professor; STIMY,
I.I.. reteenzent; VIVD2F-I&A-.P--, ratoenzent; HINAYWA, T.M.
redaktor; manEM. 1,. =a., tekhnicheskly redaktor.
(Technology of footwear) Tekhnologlim obuyi. Moskva, Gos.nauchno-
tekhn.izd-vo Minieterstva prosyshlonnykb tovarov shirokogo po-
treblentia SSSR,,Pt. 2, 1955. 446 p. NLRA 8:10)
(Shoo indnetry)

VINOGRAWV, A.P.
Unit for coating electrode packages with paraffin, Mashinc-
stroitell no.4:38-39 AV 160. (MIU 13:6)
(Protective coatings)

TINOGRADOV Aleksandr PetMIch; KEDRII, Yevgeniy Alekseyevich;
MITDOV, Baris Fedorovich; SERMYEV, M.Ye.,, zaal. doyatelt
nauki, prof., doktor iekbn. nauk,, retwnmtj BUIAUDV, U.V.,
prof., doktor tekbn, ftauk, retmenzentj PLATIMOV, K.M.9 kand,
tekhn. nauk, re tsenzent; SMTSOVA, T.P... inzhoo retsenzent;
MUMNIME, D.S., inzh... rateenzent; YEGORKIN, N.I., Prof.)
doktor tekhn. nauk. retsenzent;
, MASIIKOV, A.11., kand. Dellkhoz.
naukp retsenzent! ARKHANGELISKIZ,,N.At. prof.j red.;BDRIBOVA,
Q-A,O%ra4*3 GROMOVp A.S., tekbne r9d*
(Leatber goods., shoes, furs and pelts] Kozhavenno-obuvmye,
pushno-mekhovye i ovehirmo-shubWe tovary. Pod red. N.A.Ar-
khanggllsko6p. Mosk7a, Goo. izd-vo torg. lit-ry., 2962. 536 p.
(Boots and Ihoes) ~(Fur) (HMOs and skins) (MRA 15:3)

~

1) is W is 16 of to " a
A J4 a J6 n jopp
tI oll Vil mks U1. Uhl o
A A L - 8 'A 0 It P I I V I A I J I I M 4 CC LV U 4 0 6
v
lt4o

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CUPOIJ141IMMO O"MUMS, A. 1'. VIN(WINANW. &0" 111^ Ao i. V, 40- .00
KrIalkins sumAg tusullos. of top gm of the lim uf furl, It" of -00
inetal by lottraing and vol. of bL-Lot are discuswd. In ctionpari-m with 144~ufurttacc .049
cuke. Portual tattallurgical coke for cupolit furnaces should Ile ax strosig treviumisically,
o -bmld coutam Iem 3 and "It awl Amid be Im portmo. (kTmn metallurgotal C"kc -00
ct"Itaitso all av. Of ms% tized C. Whitt the Uktaiinian coke corttainsonly 9117;. Farnsulas
i
.00
art g
ven Itw finding "nud comumption Ad coke of given ctmalm oml givrit cmidi-
00 tiuna 0 atutiting; for deig. coke cAmmiumption fiv bloviing-in the rul..U. snot rclat"m

00 Imliarru ClAr m1mumptitm In genesit) and duralison IA o1wraling jlrr~ill J4 rulmils. 011
the ha*is t4 cullula tuelting data it is "ta6fihr-I that ram".ike m"m-mv itt co,ke cim
ousupt"i musd excessive incitritsc in InIrmity of tunrlting with inctra- 4 co-kr c,di-
S%

Ixi Is lead its rittv i e laws of ntr(al due to Imirtims S 1. %1
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if r-"05RAIDICT --And ro; Fnv-, cvich --- , - ---
p I .. I . -
(,-in C77
". -1 . " 174 )
Callbrntion of Metil rolls. Khqr'kov, lolluchno-tekhm. izi-vo "krninfp 1951. L ... ~ -
COJIFItIon of the originil -s determined from the ME: 244 P.
Microfilm TS-5

VINOGRADCV, Ati(Irei FRvicvIchi, !F75-
Groove desiEning of rollers. 2. !zd. eninjrrni, Go!7. nnuchno-tek-n. izi-vo lit-r-,, Pc
chernoi i tsvetnoi metsilurp-Ji, 1950. 34-11 p. (51-"-55971
1,
T3340.V5 1950

M60'306V j, k OPO
Aiithcr. :Iinogradov, A. 11.
Title: T-io cztllbration of rallere. (We-Iibrijv'xn Trak:,!'&k-?;rh valkcv.)
City: Leningrrcl
P-abllshsr, State Soientific %nd Techrical Publication portaintlac t-.-)
the crude and chromium metrJ lurgy
Date lq~jo
Avallablej L!"Miry of Congra:3
Zource; 11onthly Lf:A of Rass-.an Kcc*6ctona, Vol. 14, 17c). 1, P. ---g.

TIMOGRADOV, A.P.
Device for boring cylindLrical holes. Xashinostroltell
no.6:25 Ja 160. (MM 13.8)
(Drilling and boring machinez7)

VIN,,IGRADOV,, A.S.
The density hypotheals for Diricblet I-series. ';iv. kY ~-~3R,
Ser. mat. 29 no.40011-934 165. (P.-o

so
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16
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no 11W rtu'l year t-Arly Ill floe -pling Iml atirt file nirlimpor
st 11W Almost all.1 ilt%l 4% file cheirr twittivi 1,, tenth thr"noth
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VINOGRADOV, A.S., master; OSMINNIKOV, A.M., 8188arl
Recommendations on the maintenance of the distribution panel board
of the ChSl electric locomotive* Elek. i topl.tiaga no.8:36
Ag 163. (KRA 160)
1. Depo Moskva-SortirovoA Wae
(Czechoilovakia-Electrio locomotives)

VII-IOGRADCYV A.S., dotsent. AVANESOVA, V.Ya (Kazaal)
Primary cancer of th4'gillbladder. Kaz.med.zhur.no.3t
83-84 Itr-Je 163. t (~MIA 16:9)
(GALLBIADDEB--GANCER)

-e Jcb;-GFMHE-
BAIZKOV, Vladimir MikhaylovichjSIEQWUDU,-Alekoandr $ ma=y
NOVICH, Samuil Yefimovich; BOGUTSKIY, N.V., otv. red.; ABRAFIOVp V.I.,
red. izd-vaj LOMILINA, L.N., tekhn. red,
[K19 equipment complex for mechanization of coal recovery from thin
steeply dipping beds] Kompleks obbrudovanila K19 dlia mekhanizataii
vyemki uglia iz tonkikh krutopadaiusbabikh plastov. Moskva,, Goo.
nauchno-tekhn.izd-vo lit-ry po gornomu delu, 1961. 135 P.
(MIRA 14:9)
(Mining machinery)

VINOGRAWV, A.S.,, kand.tokhn.nauk
The PSX-1.0 silo loader# Biul, to kh.-okon. infom Goo o nauch--issl-
inst.nauoh.i tekh.inform. 18 no.lt58-59 Ja 065m. (MIRA 1814)

VINOGRADOV 3, A. [ 5 - 3
Flax
Obtaining high quality flax fiber. Kolkh. proizv., 12, No. 7, 1952.
2
9. Month List of Russian Accessions, Library of Congress, October-195~, Uncl.

- ,
T
,j
VINOGRkWV, A. I agrouom,
Flax. mauka I pored. op. v sellkhoz. 18 no.2;73-74 7 158.
(71am) (mm 1133)

Z.AUSHITZIM, V. Ye., kand. teZ'-.hn. nauk; -RADOV, A.S., kand. tekhn. nauk;
FOGREBITSKIY, R.D., inzh.; MDIIKOVSKIY, V.F., inzY.; YISELFT,
F.P., inzh.
The MN-1 mounted loader for silage. Trakt. i sellkhozmasz.
no.2.-26-28 F 165.
1. Vsesoyuznyy nauchno-issledovatellskiy Institut sellskokhoz-
yaystvennogo mashinostroyeniya (for Mushitsyn, Vinog-ador).
2. Gosudarstvennoye spetsiallnoye konstrL.~torskoye byuro po
sellskokhozyaystvennv'n mashinam, g. Kiyer (for Pograbitskiy,
Min Ikovskiy, Kiselev)-a-

A - , inzh.
Investigating the drying process of grasses. Nauch. trudy VINSM
4%58-87 159. (MIRA 13:11)
(Grasses-Drying)