SCIENTIFIC ABSTRACT SMAIL[ ]EGOVIC, F. - SMALC, A.
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December 31, 1967
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SCIENTIFIC ABSTRACT
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I
5MAIUEGUVIG, ,;rsthulah, dr inz., prof., (Sarajovo,, Vuka Karadzica 123)
Realization of tho dosign, and determination of geometric *Is-
mentos for tho conatruction of a hyperboloid cooling tower*
Tehnika Jug 18 no.9t3upp1*:Gradevin&rstvo 17 no.9tI641-1647
S 163.
1. Vioa geodstuka akala, Sarajevo.
@ 11 1 1 11 11 . I
1@ 1. . !@; q ,I
i: , . , ..0 , ; , , , @, -, , ,I 'W - .-*
F,i,;! ;nellt fc- ,I .- "... @ - @ @ @. r. @ z " - -- . n - ? , - .:.x. I @ *. - 1 :- @@, " : .- r h t @ -, -, n
st-nt)t3. "rud-, @ '8 1 @,@
I - ; * I .- I " - - ; - -1 1
Z
( (m r F-" 1 ? -. @j ,
JAl.-USKEVICIUS,Z., prof'.; S,"IILYS,A., med, me kande
Ileart massage. Sveik. apsaug. 8 ro.400-24 Ap'63-
1. Kauro Valst. Mediciros irititutas.
Ar
SMAILYS,A., med.m.kand.
Unfavorable effect of the transfUBion of c1trated blood on
cardiac activity. Sveiks apeaugs 8 no.2948 F*63,
lo Kauno Medicinos instituto hospitalines chirurgljos katedrao
I.rl @@
iELLEH, Ji.-I; -
S,:ilants as a Of
ix-, lir ingi ,.;troj iyr -1-11 1".. , i,, @@/ .0
1, Ilarnd! Irit-lonal Fn4erpr.n@--, Zall(A (j. Cpska Lipa.
SMAJIC, N.; D090'JiSiXp P.
Mechanism of sintering ferrous oxides. p. 241.
'i
HI'DARSKo*MET LURSI'1 ZBURNA. (Ljubljana. Univerza. Fakulteta za
rudarstvo, metalurgijo in kemijsko tehnologijo. Oddelek Aa rudarstvo
in metalurgijo) Ljubljana, Yugoslavias No. 3, P@58-
Montlily List of East European Accessions (EEAI) LC) Vol. 8. no. 6.
June 1959.
Uncl.
SMAJIC, rl.
"Atlas of defects in casting." 2d ed. Prepared by the Sub-
Committee T. S. 9 of the Technical Council. Heview,@d by N,
Smajic. Rud met zbor no.1:53-54 162.
SMAJIC) N.
NHonequi.Iibj%L= thermodynimico" by Donald D. Pitts.
Reviewed by N. Sma4ic. Rud met sbor no.3:299 162.
SMAJIC, N.
*Mathematical methods for engineers and technologists"
by P.I. Romanovski (Romanovskiy, Pavel Ignatl7evichl.
Reviewed by N. Smajic. Rud met sbor no.3:291-292
,62.
SMA.TIC, B.
"14etallurgical. principles for engineers. Tjo controlp
manufacture., manipulation#end use of metalsO by J.G.
Tweeddale. Reviewed by N. SMjic. Rud met zbor no@3:292
162.
Z. dr. @rx., r!oce-t Mlubljana), Ni i-,, ,b'
-K, Ec
V
hral-rila of the IrMienc) of physical raramoters, of nrapl@-s c-,, ',,hr@
I Fhad met zbor no.2;l6l-L74 '61.
vailic of thi constant
1, @,t@v,-trtrpnt of Virlyip, ard Wjtfkllurgl of the FacultY of NrAtLrul
S-lr;rc@n,; nr,i T,:-thnoloqj of the University in Ljullljnnn, LjAljana,
A--.koz--,,ava 2.1; inenbar of @Altorlal Commit-tne, "'Aimiarsko-motalueski
nnel YOallurpri (.@uartnrlylr (for Dobrvisek)
2. It-stitut., Ljubljara, Lop! pot '-I (for Irajii-l',
Quantitative detcriWaaflon of activity of pe sid bey cv.
I to method. Usick Kr6wcgY&ki and a
Md., Lablia, Poland), A(laza. @Aa:r:m
it, 41-*C 957); d. Sptycr. C-4. 47, M9w.-A method
for the assay of pep6in (1) is described vt hich Is based on the
diffusion of I on agas-casain gels. The diame. of wnto of
dimted protein szo directly proportional to the cookut of 1.
The latter Is obtained graphically from a calibration curve.
A.Yeragettror: *4%ottotall. presenceoltinnidgeirtats
Interferes. The proteoblic activitr of gastric @Uiccs wits
. - 'r r, ff-,= I
INOWSKI, i)ustaw; !;HAJKIIT'IICZ. ludwik
Bullaus m,:iph7aema. in the course of at&,-))qlococca1 -pneumonia. Poleki
tygod. lek. 13 no.52:2124-2128 29 Dec 58.
1. (Z I Kliniki Chorob Wewnetrznych; kierownik; prof. dr ced. M. Nedra i
z Zakladu Rxidiologil A. M. w Lablinie; kierownik: prof. dr med. L
Skorzynski). Adres: Lublin, i Klin. Chor. Wewn.
(WPJIYS@ft, PLUXOURY, case reports
bullous. assoc, with micrococcal bronchopneumonia (Pol))
(13ROTICHOPITEMIOIIIA, case reports
micrococcal. assoc. with bullous emphysema (Pol))
(MICROCCOCCAL PIMTIONS, compl.
bullous emphysema assoc. with micrococcal bronchopneumonia
(Pol))
KRYNSKI, Marian; SMJKI.EWICZ, Iudwik
A case of gastric besoar. Polski tygod.lek.15 no.6:229-230 8
7 160.
1. Z 11 Kliniki Chirargiczuej A.M. v lublinie; kierownikz prof.
dr.med. I%Iiks Simbiazewski i z Zaklada ladiologii A.M. v Iublillie;
kierownik; prof.dr.sed. lazinlers Skorsynaki,
(BIZOARS case reports)
KOROLKO, Andrzej; SNAJYJ@-VIOZV Ludwik
A case of abscess of the anterior mediastin= following dental
infection. Folski tygod. Ick. 16 no.49:1899-1901 4 D 161.
1. Z I Kliniki Chorob Wewnotrznych A.M. w Lublinie; kierownik: prof
dr med. 1-fieczyslaw Kedra i a Zakladu Radiologii A.M. w Lublinie;
kierownik: z-ca prof. dr med. Kazimierz Skorzynaki.
(I-LDIASTINUM dis) (ABSCESS etiol) (TEETH dia)
Lud%-jk i@,r.Lt KLA."tUT, Nazi-
Klxnxkt@, !,
J@ r .I ld q 11 @3 I 'i (' P! A - "@ ',#' Y.,i 2. 1 r@74j J3
1, ift u t a 1.@ "Y , Ink I Z-('& Raa to 1 0 1 rv,@@ QI Tj 4n t
Dr. Nlit.17i:i .31 ho th a t 'Cho A'4 oi. i e r. n a
YEA@-@,,Jlj Jcadorry! in Lublia
cin i ve Lek t- r stc Vo i S:- 3 , !:I- J
2'.n@,Pltsh ,iimmary recetifted.1 Syw;? too s
diagco.,sis of Uhr syndromi &.ro dcogr:r1barl. ?:)A-
t bll it 3 t i f@ Ln 1: y w uwi t od i n o n I y o n j c A s o. Star.Oard tr-jar-
q,@-iit -n,,4 tnred u -,;t@ of I hlj t dirl no t ('im In i sh I t3 tin Irk r,-!^-
M,w. t . 'tlletr.@ tire e, rs)fxrao@@nj, of *hlw) 5 arin P01--sk. anl
arm.
I
in ne c- t
r 19 t -.m d I
Z 7;@kl.-du Raililog' I Akndamli Meiy.@u,t` w lublln-
(YIer@:unlk: cfr@c. dr. me-i.
11 :`AV I tirl, I N I". tin", 1 !'a -,2 o@ I -?@' I e, Ak,-detrn I I Me@ I y
( @ I e rt. .4,11 P. - p :l,-. f . 14 r . m c d . St.1-Imn.-burg).
FLORKIEWICZ Pen ryk; ._ LudIvrik
Pancreatic calelficatlan. Pol. tyg. lek. 20 no,5jl8l-182 1 F165.
1. Z I KlInAl Chorob Wewnetrznych Akademli Medynnej w Lublinle
(klercwnlkt prof. dr. mad. Mieczyulaw Kedru) i z Zakladu Rad-jo-
logli, Akademii Medyaznej v Lublinle (klerownik: doc. dr. mei.
Kazlmlerz Skorzyrnki).
HYSAKOWSKAI Helena; Eugeni-anz; SREDNICI@A, Etinuta; @;tardsllaw;
CYGAN, Edward; ROZrISKA, Marla; SMAJKM-WICZ, ladw1k
Renults of examinations of students 18 months after thp conclumllon
of chenoprophylaxis. Gralica 33 no.7:601-604 Jl 165.
1. Z' Katediy Ftizjatril AM w Lublinie (KlerowniAl: doc. dr.
H. Mysqkowska) i z Akademickiej Poradni Przeciwgx-uzliczej w
Lublinie (Kierownik: lek. E. Pletron).
OA
R-MmOttot bpUbes for W aldtodos. AAMI
Po prdfAmW me)., Sb"ik 04., BrxO 1037MT@Mftb.
1954).-Brusbes for collectors, commutator$, 404 other
dec. machines used In t4h attitudes present qx@dal prob-
Icins owing to the tendency of the brush to break down Into
a fine powder under lowered prtswres. ItisshownbQwsuch
brushes can be prepd. by the aid of powder Tetallurgffrom a
inixt., the main ingredients of whIEF&R-ri"WC, and a
contact film must be applied to those brushes, which contains
as essential ingredient Mo,%. 47 refereacm. W. 3@-
Distrt Wd
S@@ NOVOIIIY@ V.
Te,-*,i cal equipment of a short-circuit testing station. p. 9.
(Czechoslovak Heavy Industry. No. 5, 1957. Prague, Czechoslovakia)
SO: Monthly List of East European Accessions (EFAL) LC, Vol. 6, no. 10, October, 1957. Uncl.
A. KA-ITY. J. "Off"
S 14A j t "- RJ r il, J.
Ile tiicds cf ccntrc-@ a -,.d meas-.rine, @t, s . r,v--ci.-c,. ft ,,s, :;. @- . 2:4.
(Czechoslovak Heavy Industry. No. 5, 1957. Prague, Czechoslovakia)
SO: Monthly List of East European Accessions (EEAL) LC, Vol. 6, no. 10, October 1957. Uncl.
I
SMAK, Yu.; KRUSHEVSKIT, A.
Observations of CO Lacert". Per. zvezdy 10 no.51329-330
155. (KLU 9: 9)
1'. Ptlial Varshavskoy observatorit w Ostrovike.
(Stars, Variable)
31-!A@v j.
"Ihe Perpendicular distribution of InterstplIar calcixn in relation to the
area of the ralaxy.';
7t. 15 (Posten'r Astronomll) Vol. 6, no. 1, Jan./Mar. 1956
Krakow, Poland
SO: Monthly Index of East European Accessions (ELAI) LC. Vol. 7, no. 4,
April 1958
j% F. is
...
"Photometric stiviies of the younvest constellations."
P. 1? (Fosteny Agtronomii) Vol. 6, no. 1, Jan./Mar. 1956
Krakow, Poland
30. Monthly Index of East European Accessions (EW) LC. Vol. 7, no. 4.
April 115P
-s I - y"
34 1 1@ I
"The classification of non-stable stars of the T Tauri type."
P. 22 (Poste-y AstronomiJ) Vol. 6, no. 1, Jan./Mar. 1956
Krakow, Poland
SO: Monthly Index of East European Accessions (EIKAI) LC. Vol. 7, no. 4,
April lq58
?I wr=.i
Warsaw). AaaAskan. Warm
now b-A-1runats of ths of
ISO sun of kw" the d., D, In am. of Ca im/'
cc. of Interstellar space, wos caled., the observed fntaWtke
)mkg corrected for growth effects.
U
SMAKP J.
Occasional observations of eclipsing variables. Acta astronom
9 no.1:52 159.
1. Astronomical Observatory.. University, Warsaw, and Institute
of Astronomy, Polish Academy of Sciencesp Warsaw.
'n c er, j, rom,
lis,@ of Accpr@ion (FIFF,,I) LC, Vol. I), no. 1, Jen. 19i.O.
Uncl.
@k cf _udle.,
K t F, r(. n or K :-r kc-,-r, - olp nd.
C-1r"u ali i
Pnnlcn T) LC, Vol. no. 1, i2n.
Nroio-rr cc
6vic
LAV , jf,@-,
T 1! r. I l'o,3tel y aAronorn
I'l., t)LF-,rt of @ :,i, i ';j:- 1 ",@ r,!- ITI
p - '. !, I ")'.I - @ , - -
696@,i4
2, //1.?, //,fV)
AUTHOR: Smak, J6zef (Warszawa)
TITLE: Life of the Sun. I
P/011/60/031/008/002/002
B 11 5/B217
PERIODICAL: Urania, v. 31, no. 6. 1960, 230-235
TEXT: The author of the present paper reminds the reader that coal, which
we owe to the Sun, and the Sun itself, are two main sources of energy. The
potential menace to human life would be the Sun's extinction on the one
hand, and an increase of the solar energy, on the other. An attempt is made
here to outline the Sun's life in past and future, and to draw resulting V@
conclusions for life on the Earth. It is pointed out that all numerical
data on stellar evolution are based upon the physical data on the efficacy,
the extent, and the rate of atomic reactions which are known to form the
energy source of the stars and the principal cause of their evolution. For
the energy production of the Sun, the proton cycle is written and the mass
loss connected therewith is explained. Thus, the solar mass is consumed
uninterruptedly at a rate of 4 million tons each secondt Within one billion
of years, however, this will amount to merely the 6.6-10-14th part of the
Card 1/3
89684
P/01 1/60/031/0G8/002/002
Life of the Sun. I BI 15/ B217
Sun's mass. Since the atomic reactions take place chiefly in the Sun's
interior, the Sun will contain always less hydroe-en and alway.9 more helium
in the course of time. The problem as to whether the hydrogen deficien@:y
and the helium excess in the interior of the stars will be balanced by the
mixitif; of matter in the couree of time cannot be answered directly. Ac-
cording to an estimation, however, this problem has no practical importance.
The second problem, the stability of the solar mass, is the subject of sev-
eral theories. The Soviet astrophysicists Fesenkov and Masevich have set
up an evolution theory of stars, according to which all stars lose their
matter which in the interior undergoes a complete mixing process. The
latter assumption is at present considered to be wrong. The first point
as well, the effect of corpuscular radiation. can be neglected, since
estimations based both on solar observations and on geophysical data-prove
that compared with the total mass, the Sun suffers a merely inconsiderable
loss. The same holds true for other stars as well.. It is only at the stage
of the red (,,iants that the loss of mass becomes important, &.4 their loss of
mutter is noticeable. By its assumption of the mass remaining unchanged
the evolution theory reproduces the actual stellar state best, whereas ctber
Card 2/3
89684
Life of tile Sun. I
P/011/60/031/008/002/002
B115/B217
theories are not able to explain certain facts. On the strength of the fore-
going arid with reference to S. Piotrowski's paper on the stellar structure,
the author has developed his theory on the evolution of the Sun. Age "zero"
was the moment when temperature and density in the shrinking protosun were
sufficient to release the nuclear reaction. This was the beGinning of a
new enercy source. From then on the Sun became luminous due to a modifica-
tion of its chemical interior, involving changes of its other physical
properties as well Theorists are now faced by the task of calculating the
rate of the growth of heterogeneity in the Sun's interior on the strength of
the physical data and of then designing a model of such a heterogeneous ball.
A number of models illustrating the growing heterogeneity could, when com-
pared to one another, represent the changes of the chemical composition and
the physical parameters (brightness, extents effective temperature) at dif-
ferent moments of the existence of the Sun. The author then repeats his
opinion. that tile evolution theory. although still young, is to be regarded
as tile safest and the most accurate of all theories of modern astrophysics.
A Judgment of the Sun's future on the basis of this theory will be as safe as
on tile basis of experimental. data. J. Gadomski and S. Piotrowski are men-
tioned. There is 1 fiilure.
Card 3/3
MkK, J. -
Close binaries I; on the physical nature of R CMa stars. Acta
astronom 11 no.3:171-179 161.
1. Astronomical Observatory, University, Warsaw and Institute of
Astronomy, Polish Academy of Sciences, Warsaw.
S1269163o(000100410101030
AOOI/AIOI
AUTHOR: Smak, J.
T1=1-: A repeated discussion of the relationship P - (B-V) for variable
stars of the RR Lyrae type in the globular star cluster M3
PIMIODICAL: Referativnyy zhurnal, Astronomiya, no. 4, 1963, 32, abstract
4.51-301 ("Post9py as.tron.", 1962, v. 10, no. 1,87, Polish)
=T-. The values of pulsation constin t q were calculated for two subtypes
of RR Lyrae variable stars, ab and c. The results of calculations warranted the
following conclusions: 1) the observed values of qab and % agree with the
values obtained from the models which are the best in the physical and evolu-
tionary sense; 2) the Qab/q. ratio does not confirm a conjecture by M. Schwarz-
schild that subtype a stars are pulsating in the first overtone.
W. Wihniewski
[Abstracter's note: Complete translation]
Card 1/1
SMAK, J.
The theoretical period frequency function for the classic
Cepheida. Postepy astronom 10 no.2:151-155 162.
SMAKP J.
The internal structure of the components of close binary
systems of the R Canis Major type. Postepy astronom 10
no,2;15@4510' '62,
SMAK I J.
The evolutionary significance of the subgiants in the cloBe
birary systems. Postepy astronom 10 no.2:156-14,8 162.
SMAK, J.
On the shortcomings of the application of the Schott
UG 2 filter for photometry UBV. Postepy astronom 10
no.3.-253-256 162.
SMAry 4!- -
Close binaries. II. Act& astronom 12 no.1:28-54 162.
1. Astronomical Observatory, University, Warsaw, and Institute of
Astronomy, Polish Academy of Sciences, Warsaw.
SM, J.
A theoretical period frequency function of classical Cepheids.
Acts. astr4nom 12 no.2s93-101 162.
1. Astronomical Observatory, Warsav University, and Astronomical
Institute, Polish Academy of Sciences, WarBav.
SM, Jozef
It . - " -.
lAminocities and colors of the Cepheida. Poetepy astronom 11
no.2:105-122 163.
SMAK, J.
Age of the oldest stella.- c1iisters. Postepy astronom n nc.4s
293-299 163,
GR2XDZIELSKI, StanlIslawi SMle,,
Birth and death of stars, ''szechswiat no.10:225-229 0 163.
.-. f-Ro, K @J .
. I
I'tio@,oe-lectric arid observations o' varlable
postf-lif @stroncm 12 no.'1:22-28 164 .
1,:,ng-pprlod st,irs. w
SMAK, J.
Objects of 3C 48 type. Foatepy q9tronom 12 no.3.212-215
164.
GRIGORYAN, K.A.j S-Mt Yu.M.
Polarization observations of stars in clusters KGC 22 and NGC 2264.
Soob.Biur.obser. no.28:3-7 160. %IRA 140)
1. Byurakanskaya astrofizicheskaya observatoriya Akademii nauk
Armyanskoy SSR i Inslitut aotronomii Pollskoy Akademft-ommJ6
(StAre-Clusters)
oNN:004100414100#04 0 #*$ 6
0 0
1 4 It to A, I, Ij a J1 is I t A A u to W a III, sol o., L-.141"to
00 -6, to
00 .00
Ole
.00
:0 Ic The djuretk effect of NovmUm. A 5-" nd N. -00
0 R.,,uhrv* S,,W. Vfuiwb*Yf ZAN
41MIS.-Me"Win, which k4l RUNISIN
19J9
1
zeaft
C"
,
.
,
.
:0 a IfS prepn., when ued in the treatment of beert diwase
r4tweWly. Pf(kluc" it moderate diuresill Whkb S. and it.
00
I
cc.
a regard *4 beneficW. The Wimum dow Is
G
f
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oore
16
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300
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Sf1ALktWCSCfil. ILIfflI&T6019 Ct&%iWKAT.C%
* I.. I ta
too
6 0 o 0 0 Ogg 0
0 0 see 0 0 0 0 0 0 9 0 0 0 0 0 0 0
.0 0-0 0 0 0 0 0 4 0 0 0 4 q 0 e q q!O 0 0 0 0
SKAUYNV,,A.S., kaml.med.nauk; FAR&WHEV, I.D.
Hemolytic jamndice with hemoglobinuria. Aserb.med.shur.
no.3:79-81 Mr '59. (NO& 12:6)
1. Iz -%im&aitBkoy gorodskoy bol'nitay (glavvrach - Sh.Z.Huradov).
(JAMIDICE) (H),,1140GLOBIMMIA)
SMAKATIM, A. S.
Comparative evaluation of methods for the treatment of peptic
ulcer. Aserb.zed.shur. no.1:72-75 Ja 160. (NIU 13:5)
OWPIC Uw1w)
RUSIYA, Zaur; MURTSILAVA, Gigla; SMAKHARAD27., Kukurl; MIKAYA, Zurab;
SIRADZE, Bondo; AVAZASHVILI,-au-g-uui--Pi-tTsr~HALkSHVILI, Favle,-
TATUASHVILI, Anzor
Search goes on. gov. profsoiusy IS no.5tl6-18 Mr 162.
(MIRA 15:3)
1. Zavod "Elaktroavtomatio, g. Tbilisi.
(Tifl-ts--Labor and laboring classes)
1 17- 1957- '-3305 D
Translation from: Referativnyy zhurnal, Metallurgiya, 1957, Nr i-,, p 64 (USSR)
AUTHOR: Smakhtin, L. A@
TITLE: The Measurement of the Partial Vapor Pressures of Gold, Silver,
and Copper in Solid Solutions A-P and A-S (Izmereniye
part,iial'nykh davleniy para zolota, serebra i medi %- tverdykh
rastvorakh A-P i A-S)
ABSTRACT: Bibliographic entry on the Author's dissertation for the degree
of Candidate of Chemical Sciences. presented to the MGU (Moscow
State University), Moscow, 1957.
ASSOCIATION: MGU (Moscow State University)
1. Gold-Vapor prczsure-l@'c@rsurwent 2. Copper-Wpor pressure-
@Icl surm:ent 3. Silver-7. por prcssure--.k'ecsurcment
Card 1/1
i4liasulomtnt at ?&"I P:@&auie f u mi, I ca4
, I
NI Y-t-
Atfl@
"er-"! t the @pt, lu,
.!Ic t.
7 /4
'hoporov, !). Ia. ,
.2 f"m
'r . 71. , 5r-tUt In, L. A. , C
L Y - I ev , 11 .I
T-ive:@ti. -,@tion Imto th@,, Tier-iodyn--..-nioc, of '3oll@! 3obitions
-)f "tol", 'Zil-fer' and COP7'er I po tr--r-,odinomil-e
tl!-'-@rd r-.-1.vnrov zolota s serebrom I medlyu. 1)
'Ir 2
lq5@;, Vol '3,
34"
-':7 T T
B--c lioc the components of solid colutions h-.-,ve such In
v@,,por preE-,ure irvel-ti.-a-tiono of th,? thermo-
-in,
.1, azlic prc@portius of such rolutionn by measure--en+ of the
il-firtial presmire are very diffricililt. Thece m--asure---:its could
be facilitated by the noe of r@idioactivc inotopes. In this
ifa@:er data are Civen for the v@por preroure of --olid Au, AG,
@ind Cu, since the literature data for the pres3ure of saturated
vinor of these -etils are very contradictory. eure m-@Aals
r.,., io-optive i.,:otopes Aulgig 110 64
@ml t-e 1 9 Ag , and Cu
-aere nsod. Th,@ va!,,or pren@7ure wfi@, measured unirg the effuLion
:--ethod of 7nudsen and -in ri j
p:ro,,)r-iate .i@p@lratus (P-*.:; 1'. T'.,.e
C'!@'i 11/3 effWllon prolucod from --iolybder,um. From the experi-
ion !@A,-) tl-.,-@ T.ur-cly- @-icf- of Sol id
f 1 agreement.
n: (-,,- are in
(Douninr-
v - .-ivc;@ 1,y Downing, Edw;@rds and Heriek
E,1varda)(Ref 1.2) are too hit;h and thoe by Ilarteck are too
lata for li-,u-,'d Cu are tho@-e .-iven by
T,,t,:-c :;re 4 fi-vireo, 3 tabless, an! 12 references,
2 (@f are Sovi-,A.
'T
universitet im. 7j@. V. Lomonozova
j@,-.tc Vniv!-,rsity i-ncrd ',.*. V. Lorono-ov)
july 9, '@@--17
5M, 18(6) SOV/76-335-3-15/41
AUTHUS. Nesmayaiov, An. N., Smakhtin, L. A., Lebedev, V. I.
TITLE; Inventiaation of the Thermodynamics of Solid Solutions of
Gold With Silver and Gopper.11 (Iasledovaniye po termodina-
mike tyerdykh rastvorov zolota s serebrom i modlyu. II)
PERIODICAL: Zhurnal fizichoskoy khimii, 1959, Vol 33, Nr 3,
pp 599 - 6o6 (US.@'R)
ABSTRACT: In a previous paper (Ref 1) investigations were carried out
on the pressuro of saturated vapors of solid Au, Ag, and Cu
198 110 64
by means of radioactive isotopes Au 2 .119 , and Cu
according to the Knudsen method. In the present paper ex-
perimental results are described concernint; the partial
pressures of gold, silver and copper in solid solutions. The
experimental data (Tables 1,2) were worked out according to
the method of the least squares and represented as straight
lines Ig P i - A + B/T. The activities in the case of 1250
and 1111 K were calculated from the equations for the pressure
Card 1/3 of the saturated vapors of the pure metals and the partial
Investigation of the Thermodynamics of Solid Solutions SOV/76-37-3-15/41
of Gold With Silver and Copper.II
pressures in the case of Au, Ag, and Cu in the alloys
Au-Ag and Au-Cu. By means of the experimentally obtained
values of the activity coefficients (Tables 112) and the
equation according to Gibbs-Duliem both activity coefficients
in the concentration range of from 0,2 N i to O's Ni were
calculated according to the method of successive approxima-
tions at graphic integration. Equationa on the relation bet-
ween the activities of the componeits of the alloys and the
temperature in form of linear functions lg a I - 1/T were
calculated from the values of the activity coefficients for
the two above-mentioned temperatures (Tables 3,4); herefrom
several thermodynamic partial and integral functions of
solid solutions (Tables 5v6) were derived. The majority of
the results obtained is in good agreement with the publication
data. On comparing the experimental results obtained with the
approximations of the theory of solid solutions only a quali-
tative agreement was to be observed which means a limit@d
applicability of these approximations. The observed excess
Card 2/3 entropy of mixing is considered to be due to the Yariation
InvestiCation of ti-ie 'I"i.ermodynamics of Solid Solw.-ions --:Gvi'7'-- 151,41
F-@ I II
of Gold 'With Sil7er arid Cou-,ler,II
of the oocillation frequency of th., atom:@ in the crystal
lattice on the tra;Isition metal --) alloy. There are 4 figures,
8 tables, and 16 references, 4 of -ahich are Soviet.
ASS6CIATION: Igoskov3kiy gosudar3tvennyy universitet imeni Lt. V. Lomonosova
(Moscow State University imeni M. V. Lomonosov)
July 9, 1957
Card 3/3@
S/CA2/60/026/0?-/001/035
BO*,5/BO66
AUTHORS
TITLE:
Rakovskiy,. E. Ye., Smakhtin, L. A., and Yakovlev, Yu. V.
Determinaticn of Microimp-jritiea in ffl h@purity
by Aleans of Radioactivation Analyaig-W
Anti ony_0
PERIODICAL. Zavodskaya laboratoriya, !960, Vcl. 26, No. Ili pp. 1199-1200
TEXT; The radioactivation analysis of antimony according t-,, A. Kulak
14
(Ref. 4) cannct be applied to determine impuritte-i in ight elements. The
authors describe such a method for the de'@ermirati 'cn of phosphorus,
chromium, manganese, copper '. zinc. galliim., and arsenic impurities in
high-purity samples of antimony. The method -.onsisted cf a iompar:sci
with standard samples. The sample and the standard were Pxpcsed tc a
neutron flux (8.7-1012 n/,.m2-sec,) for 20-48 h. The elements to be
determined were divided into two groups, i.e. Mn.. Cr, Zn anl Ga on "he
(,ne hand. and P, Cu, and As on the cther. Tc ana:yze the former F-,rojp,
*he sample is dissolvel in aqua regfa af*er irradiaticn. evaporated
antimony i3 precipitated with H2S. the sol,itj.on is evaporatel tn, lrynes3
Card 1/5
Determination of Llioroimpurities in S/032/60/026/01'/'001/035
High-purity Antimony by Means of BO-,9/BO66
Radioactivation Analysis
taken up in hydro?7hlorts acid, and the resulting solutien :0 passel thrctk;h
jar with the Dcwec '1-X8 anion exch3nger whif.-h ab-gorbs Ga and Zn. r,:i
is then eluted with '-? ff HC1, Zn with water. Mn and Cr wh!.@h are net
absorbei by tho ex,^.hanget are precipitated wl*b H23 in amru@rl:a-,al medi,-,m
as sulfids and hydroxide, respectively, -and finvil!y tsol-:1teij; Un in the
form cf MnNH4PO4, and Cr as barium chrcmate. In the test for Cu, P., and
Ai, after dissolution :f the irradiated sample As is isolated atl arsenin
bromid;-@ Cu is separated as CuCHS '. and the phosphare ':a is,.1ated as
magneiijin ammcnium P11C3phare al"ter pur-.fication on the K'Y-? (KU-2) ca---7.
exT:hanger. The test samples a3 well as the standard samplaes werp
m-3asured by meang Irf a CO 2E? (SI-2B) Geiger cc-.inter with a-i -i,:@curaiy r@f
abotA The following dele7mlnaticn acouracies were fc@.nd:
11 9; 6
I. '. 0% Mn 3.5@-O-O% Cu, < 8-10"% Zn, 4,10--% As-