SCIENTIFIC ABSTRACT MIROSHNICHENKO, I. V. - MIROSHNICHENKO, L. S.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001134530006-8
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: January 3, 2017
• Document Release Date: June 21, 2000
• Sequence Number: 6
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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MIRCSIMICHENKo, I.V.i LARIN, G.M.1 MAKAROV, S.F.; ViDEM-1, A.F.
Electron paramagnetii resonance iretnod ef BLuJvinq, a fT?i--
radinal of hexafluorodimet-hy, nitropen ey'de.
6 tio.51776-777 S-0 4~~. ~ '41 R.A 18 . ~:, ",
1. Institut rbsh,.hpy , neorgunicheakoy khimii '-wrt N. 1.
Kurnakova AN S~ZR. Mftrn' ' l,iric r .

MIRMHNICHE31KO, I.Ya.
Our work experience in the mechanization of production pr,)cesses.
Kons.i ov.prom. 16 no.5:13-15 My '61. (MI?A 14:5)
1. Dubnovskiy ovoshci,.eaushillno-konseiLvsiyy kambinat.
(Dubno-Carining industry-Equipment and supplies)

Nil "tiosmucallyo , -. G.
. , Inst. 11 tw-C Sci. im T.F. Lenraft, Leninfrad,
Ybr., Lat. Flant FY)-sjclcgi Va
"Corbohydrate Yetabolisr. in WYeats linder Conditions of
Insufficient Soil Moisture," Do:,. Ali', 32, No. 1, 1941; "Exchanpe of Carlo~,ydrates
in Summer Wheats in the Earing Phase urvier Conditicn.,,, of Sofl DrouE~.t (TYe
Prot-lem of the Physiolo(Ty of the Critical Period In Cereals)," itid., 50, Nr,
194-; "The Influence of Ethyl Alcohol ort the Growth and hoot Formation of klants,"
ibid., 60, No. 1, 104F; "Implantinf? of Slips under the Influence of Water
Extraction fro- the Leaves," itid., No. R, 194P

FA 51T41
~/Wmftclm Wmat 21 MW
Wdletne, Cartab"Iratee
63kchazigs of Carbohydrates in Summer Whftte In the
Swing Phase under Conditions of Soil Mvught (Prob
of the Physiology of the Critical Period In Csreala),,fl
K ' - Wrotbn1ohemko, Lab Plant P48101, TAnInarad
U
al Sci most immi Isegraft, 511 pp
"D* Aked Nauk ff=, Nova. Ser" Vol LIX, So 9
ftwente date collected as result of studies of two
typee of sumAr ftest. Determines monosaccharlde,
amachaross., starch, and smIcellmloss, In the roots,
step leaves, and bee", Subadtted by1eadmician
ff. A. Nsksimov, 24 Jan 19h8.

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426-84",;). In such cipts.. in which tan ctiertul nutri-
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at 0.25-41.6% conco " only it root growth stimulattif vi
plant cuttings but the bome W roof-forruAlkin mi- in-
creamrs. Coatings 'd 'WOR fraswra V-11 for 5 d"Ya ki
sq. a1c. (2.b. I.b. and 0.6%) showed highest no. cid roots
at the loom conens, , although 2.51, "n at- .;wnutrd goo
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ITSSR (600)
01"owth of Plstnt8
"Affect if the Root Systatm on the Growth of Stems" Dok1 . AN, SSSR
No 6, 1952
Rail. ?2 Jan 52
SO: MonthlX Liit of Russien AcaessionR, Library Of Cngregs, Sept rber 1952, UNCL
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USSR/17_h-_-'j lhyzid~cgy - &~WtOand D~Velqnent
H44
Abe Jm"! I Reforat Zhur - Blols No 16, 25 Aug 1957j 68979
Author I MiMahni mhu%*RA_K 10*
Title I The Root Formatton of Stalk Graftings In Plants Under
the Influence of Ethyl Alcohol and Aqueous Extracts.
Orig Pub Ucho Zaps Kurskogo goo* pod* in-tal 1954t 3, ee-iol
Abstract The treatment of beans willow and geranim outtings by
ethYl alcohol (0*25-1,,B%) stlmrlated root form. atono It
is aeswee that siopholp like gro-.tn substanoeop increa-
ses the flow of nutrient mater:~al.: 4--a the base of"tho
graft, Aqaeoug eftraots from the 3-;aves of beans; gera-
aim, and retle rtimulated the rooting of bean cuttings.
A high cornantrnt!on extract from geraniun leaves sated
as an 2.4#-D* The weakeL--~ aotion was prodUced
by ex"-Irni.`3 Prm ~4ilowy leaves, whi-,h the author explains
by the ?rfjaenaq of tannin@@ In the opinion of the authort
the substances present in the extracts are analogous to
Oard 1 /P

MIROSHNICHENKOI K.G.
Effect of the removal after various length$ of time of the growing
point of the main shoot on tillering in wheat and barley. Uch.zap.
lurak.gov.pedi.inst. no.4:5-19 157. (KrRA 12:4)
1. Is kafedry biologii (sav. - prof. NeR. Geller) Kmrskogo goeu-
daretvannogo podagogicheakago instituta.
(Wheat) (1krlay)

I-ILIOSHNICHMIKO, K.G.
Formation of rooto in fiprout,-) under I.: 'c- of J,..c phynidIc-
gically active substancen. Uch. zai . Ku--s :. -~S. pe-.. inot. no.1-1.
98-109 '58. (1-11 A 1i,-.1
(corn Naize)-Fertilizers and :i-inurus) (--oto (Botany))

I
.4110SHI! CIMIKO, K.G.
Ef:ect of 2,~- on sor..e 7ovt:. I.rocoq ies in w c-it mil baxlet. "c'...
zap. Kursk. gos. pe6. inst. no.11:11C-124 '53. (.". 1, ~, 14: 1)
1. Kafedra biologii Kurokogo Oojud,-xrstvenno!--v 2oda-aGicLeo -o -o Inst!'. -.ta.
(Barley) Mcat) ('), 4-j)

"'ITLE:
On t ~.c Ir !'Ivence of 2 , 4-1) Upon tt;,~ F-.r--
-)n f
(0 v1iyLnii 2,4-D na for~airovanije .-r.- oy j o j , i,
IR I D I U Do 1: 1 a,,,' -Ai naul-, SSSR, Vol 12~, '.r
p ; 135,, - 1558 (,-,SiR) -.111 17
A L STR -h T One of t.,.e wecific reactions of t'e r-)-t s-.,s'e-. of -.,,r- ~3
Plan t 3 U;'011 t.-,e act I on of t e 2 c- 1 r,-
(2,.;-D' cQv-2i ~l !3i-.il~r s-C.st '~e3 17 t r, t
t, e lnr i- a. :,rowth, of tl,,i c ~ e-: -tn -m,~ .-s m- 7-~.
-i;A a defor. ation of tne nair roots 'Re~[; I a
in tne ir-zser t a,,er ~: tu~ ied the i -:f,':,e ce of I f'
ce.r.*r-.ttic,rs oft e iodium salt oftne a:~ woll E
(as J1,B'v, heterca~;xi n , and riolj'Ll eni.:- or t
o f t:i-~ -~ -.i z e s,:, ei a of t ~.e " Vu r .: ne z hn- T
of t1'.L- cuolli --s wnr,~ i7c-ersei in ~orrcz,-~ - 4i-
nit ercce Ii:. 24 hours a t t--,

0 :if -1 u,~r)ri c.)-centration of I -i '
t c :-_~: :-,
Tr..-
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-"e
Ca M 2 v,) 1 u -a o' t~.e ruot3 in the ~,-:-,e of seeili!~ -n r,',,,

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PRESE.-;TED
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et I T~rVS2,)- !',Y
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MIROSMIICHEMO, K.G.-, BUYANMVA. R.V.
Disturbances in the vernalization process of winter wheat. Bot. zhur.
45 no.11:1653-1656 N 160. (KIRA 13:11)
1. Kurskiy, gosudaretvennyy pedagogicheakiy institut.
(Wheat) (Vernalization)

MIROSIHNICHENKC, K,r,. , 'j w I
Effmct of Lrron Fin,, r-' iir, t ;-x . n r,,, I ro gyr - ~.' r ;ir,,' - ;~" c ' " 1-- --
carrol,.%, 11-h , Zdp , F.U- lk j?oS p("1 . ', r~-ql- . 1.6 - _" -'- , ~ I , f , ". .
,p --H A 1". 4. !
I. V a f (!,I ri ~,-- fir' k ' - ~,m~ir itv --n p! -,-I. -" , '~
Inn'Itat 1.

,"Jlj~ L ~ ' ~ !%I ~' 17 7._' : ' 'C , K .
-) I ~ .1
Kti t e I 11, , li),rLi I ini-
Ll ec I ro-meellir. ici., . - r,:: , int- 7,,.c 1; -.P. : r 5 1 , ', r ~ 1 e r 1- 5. i-iui . - , ., . , - . . . I
11 1 ~'.
~~ of 1 us-5ipm iccessions , ~ iu-.ry L,,' ress , "ecer:.,-e" . ", . , :.c" 5s,;: le(l.

4
1 MC SIPT T~ li-Ell- ~ 9~ . P .
*
Techno!G~-,,
,)ur exmrience in golvinf, the r)r(-)bl(lr of !n(,renqlnp t.he i)rryluctivity r,r
)'oskva, Qnanle' 11)51.
','onthl- List of Russian Accesqi,-,n.9, I lbray-y of Conrresq, April unclassiflo,l.

MIROSI*IIMMNKO, K. P.
Reduction of subsidiary time Moskva Profizdat, 1952. 60 p.
(Novatory sotsialisticheakogo proizvodstva) (54-18329)
TJU60,M59

MIROSHRICHMO, Klimentty Petrovich, inzh.; RUBIN, H., red.: MOLCHAHOVA, T.,
- - - - - - ~ - timit.-red. I . I ~ - -- , 1
(Reduction of setup, mnn, and down time in plants] Sokrashchenle
vopomogetellnogo vremeni na proizvodetva. Odesskoe obl.izd-vo,
1958 57 p. (YERA 12:2)
Nachine-shop practice) (Time atudy)

PME I 99OK EXPLOITATTON BOV/3579
Ki-x-Ehnicaenk-, FItmently Petr-,vich
Nolrayu tekhniku - na sluzhbu semiletki (New Technique to Serve the Seven Tear
Plan) (Odessa] Odesskoye knizhno-ye izd-vo, 1959. 54 p. 2,,000 copies printed.
Ed.- K. Rubin; Tech. Ed.: T. Molchanova.
PURP06S., This booklet Is Intended for the general reader.
COVERAGE: The booklet deale with new machinery and devices built in the Odessa
industrial region and with advanced processing methods in the machine industry.
The principles of cybernetics and newly developed techniques in industrial
operations am discussed. No personalities are mentioned. There w.-e no
references.
TAM OP (70YMM:
Solving the Problem of Technical Progress
4
Card 1/2

I New Techni.que to Serve the Se-ven Year Plan WQ /,5579
Advanced Technology -.- Viants of the Se-mlet gconmm 3 (7)
Kust Signi-ficant b7end tn Techniral Flr-~,jrreaiq 41
Crestore of New Technique 47
AVATLA=: Library "t C~ngrees (TA5.ic)
Card 2/2 VK/Mas
6-29-60

MIROSDUCIENKO, K. T. and Bukreyev, 11. V
.1 Preseace of Giu~athione tn Healthy Stieep rind Its ~:!.ang,-
BnIce I ios is
Tr. In-Ta Veterinarii Kazakh. Fll.. VALKIJ;I:_, ~1.,
Author studied the pathogrenesis -)f truce.Linsis and arrled
chemica- Investigations f I.he )1' nen'T'hy T114d Isellsed !;'Ilev; Wl'".
respect ot giut.athlonc and 4*,,s ~rnctl.,_)ns. A:i Inerf!ase ' t~~c qmrjur.'
oxidized giutathilone was -)b3erved
(?,Zhl,.iG-L. lie ,, ZRY I i5'))
SO :Sum-No 118.7. 1,1 jall 5(j

i7l . .I , * , , . .- .

KIROMMICHINNO, L.A.
skarns or central Kazakhstan. Jzv.Aff razakh.&M.Ser.geol. no.20:
115-125 '55. (NLRA 9-8)
(Kazakhstan--Ore deposits)

MIROSHNICHMKO, L.A.
---
Ore-bearing capacity of Central Ksz&khst&n skarns of different
uet&llogente epochs. Izv.AI Uzakh.SSR.Ser.geol. no.21:29-40 '55.
(KLRA 9:8)
(Kaz&khatan--Gre deposits)

MIROSH3111,Hl'.1iKO, ~.A.
Lr)(-.Pt ton if qk~rn It ~ ' -
S SR . S e r . g,~4 n ' . ri r . - - . -.,' - - " - ~
(KnZ A ktl --Skurrs )
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LYAPICHEV, G.F.: MIROStUTICHEMO
~ L.A.
1 -1 - -
Joint scientific conmiesion an the developeent of m1neral
of central Kazakhstan. IZ7. AN Kazakh. SS11. Ser. geol. nc.2:1~1 !~'
'59. (MIRA 1i:2)
(Kazakhetan-MI non nnd mineral r-jources)

MIROSHNICIMIZO. L.A.
Microbiological principals involved in the use of mineral fertil!zers
in Irkutsk Province. Izv. Slb. otd. AN SSSH no.6:112-119 159.
( 1AIU. 12 : 12
I.Irkutskijr godudarstvennyy universitet.
(Irkutsk Province--Fertilizers and manures)

MIROSIDUCHENK0. L.A.. kand.gool.-mineral.nuuk
Joint scientific geasion on metal logenet ic ani prognootic
maps. Vest.AN Kazakh.SSH 19 nn.!:96-IDO Ja '59.
(MIRA 12-1)
(Genjoa-kaps)

HIROS194ICHENKO, L.A.; SOKOLOV, G.Ya.
Effect of various cultivation practices an microbiological proceseel
in turf-carbonaceous soils. Trudy Inst. mikrobiol. no.71196-204
160, 041RA 14:4)
1. Irkutakiy gosudarstvennyy universitet imeni A.A.Zhdanova,
kafedra fiziologii i mikrobiologii, Bayandayevskaya*aellskokhozyay-
stvennaya opy-tnayn stanteiya.
(SOIL MIQRQ- ORGANISMS) (TILLAGE)
I

MHOSHNICHENKO L.A.
Effect of prolonged cultivation on microbiological procespea In
gray forest soils of Irkutsk Province. Trudy Inst. mikroblol.
no.7t239-248 160. (MLA 14:4)
1. Irkutskiy gosudarstvennyy universitet Imeni. A.A.Zhdancrva, kafedra
fiziologii 1. mikrobiologii.
(IhKUTSK PROVINCE-SOIL 141 C 40-ORGO ISMS) (TILLAGE)

3/051/61/000/OUI/OGI/005
A161/A129
AUTHORSt giroshnichenko, L.A., Candidate of Geologic~il and Mineralo-
gical Science; Veleshina, T.A.
TITLEs Selenium and tellurium in polymetal deposits of Central
Kazakhstan
PERIODICALt Vestnik Akademii nauk Kdzakhskoy SSR, no. 1, 1961, 15-21
TEXT: The work presents preliminary information on the results of
wide-scale explorations started in 1955-1957. The explorations'purpose was
mainly to determine the minerals collecting selenium and tellurium and the
regularities of their distribution in different genetic types and forma-
tions. The data for this preliminary information was gathered from the
authorst own collections and from the Geological Museum of the AS KazSSR,
as well as from single samples from the galenites of the Dzhezkizgan
(collected by T.A. Satpayeva) and Gul'shad deposits (Y.S. Gazizova). The
presence of selenium and tellurium in Kazakhstan has jr~jctically not been
studied before, though data on other rare earth elements (Indium, gallium,
etc.) exist in some works. The authors gathered data from 271 deposits in
Card 1/4

S/C
Selenium and tellurium ... A161/A129
all, belonging to the foilowing ore formation3i lead-zinc skarn form~itlon
with copper and bismuth; lead-zinc skArn; lead-zinc 4uartz veins; birite
with predominant lead content; metasomatic with predominant lead content,
and lead zinc. Galenite from other formations was also studied for compari-
son, viz.,from copper, tungsten, molybdenum and P,,old deposits. A lihoto-
colorimetric determination method (developed by staffers of IGN AS KazSSR
T A. Valeqhina and I.I. Gekht) was uqed for selenium as it cannot be reveal-
ei oy the common spectral analysis. ~Abstractorls notei No data concerning
the method are given]. The investigated minerals were mainly four very
common sulfide types: galenite, sphalerite, pyrite and chalcopyrite. Some
behavior peculiarities of selenium and tellurium were noted which are
possibly indirect indicatiuna of the laws of their formation, but the ubatjr-
vatione do not confirm the view of the majority of Kazakhstan explorers
supposing isomorphism of tellurium and 3elenium with sulfur. They were
spread unevenly in the studied sulfides. Individual microscopic inclusicns
may be supposed, but their determination is not possible at the time being.
Natural tellurium compounds are known in single deposits (Kyzylespe), viz., r
tetradymite in sulfide ores, and montanite (earth crusts on tetradymite).
The authors investigated galenites spectroscopically and noted that nigh
Card 2/4

3/0 5 1/61/000/301
Selenium and tellurium A161/AI29
concentrations of silver and bismuth were always accumpanied with increased
concentrations of selenium and tellurium. This may be a confirmation of
N.D. Sindeyeva'a view (who is specialist of the mineralogy ind geochemi3try
of selenium and tellurium) who points uut in her works that the two elemerU
tend to form independent minerals in microscopic volumes (about 4b ~4ra
known). The highest concontratiun fuund in the expluratiun was o.u) -
0.08% in oulfidea (by micruchemical determination). Conclusionst 1) the
major accumulations of Se and Te are in skarn deposits of lead-zinc ore
with copper and bismuth. Polymetal.'ic deposits with higher Se and Te con-
tent belong to the early and late Variscean epoch; no higher concentrations
are present in Caledonian deposits; 2) all deposits with higher Se and Te
content are situated at definite ore centers: Akchagyl, Karagayla, Baty-
staus and Berkara; 3) the mAjor collector cf Se and Te or their compounds
with bismuth and silver is galenite of skarn deposits with lead-zinc,
copper and bismuth mineralization. Se and Te are rire in sphalerites,
pyrites and chalcopyrites; in pyrrhotines and Arsenopyrite3 they -%re absent;
in separate minerals of the oxidization zone increased Se tLnd Te contents
are mainly present in deposits where th" primary sulfiles ;iru o?nriched with
Se and Tei 4) TQ~ p-edominates over Se in the ma,~Iurity ~,f galenite samples,
Card 5/4

Ij ~ -~l " ~' -
S/131/61/~ 0/ --1,
Selenium and tellurium A16l/A129
in the mean proportion of l12; no abrupt viriAtions in So and To ccntent
with depth was ob3erved; they ire present in gulenite of i certain ItIP031t
type throughout, in variAticns that do not depend on the depth of sampling;
5) the authors are inclined to explain the higher Se and To cuncentritiGn
in sulfides (particularly in galenites) by the pr-3sence of miorcsccpic
inclusions of natural comicunds of Se und Te with bismuth (predominantly
for tellurium) and silver (for 3elenium) and only insignificant influence
of their isomorphism with sulfur.
Card 4/4

'JHC I. , rl , .1 1~ ~,Xe- ~ ~ 'iV , Yli A.; A ) A, M 'I , ~UFk SHN I AMEN- t , L A.
Slibn,irf -,r-o m- I ii- z r, -; I r. ent.-q I K a z"nsf.-in . lz-.r. All
r~r, , , 1~ , Z I . I ~IdPA I C : I
II -- ia'~ r.r, t 1(j,,./ , SI.r,ir , ril j

-MlROSRNICHEMKO, L.A.
New data on the distribution of indium I-n the ore deposio of
central Kazakhstan. Trudy Inst.geol.nauk AN Kazakh.SSR 6tl7o-
180 162. (MIRA 16s6)
(Kazakhstan-Inditm)

SHCURBA G.N. , Juktur go(ilogo-mineralogii-i;f~L;K"kii ntiux; U , '-!~ ..N.KOP L.A.)
I . I I - -
kana. r-auk
Endogenic ore forma*,ions of Siber,a ar.-. ..ne war Bast. "-s*,. AN
Kazakh. SSII. ~k~ n. .7:85-Ft3 .-I '~-,4~ (M-RA "':Ill

r I,
a: I MO th W P
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ouruy'rive v

L rptlor, Spec
at50
Infrared 1419)
p part Z~,.jr.ob- (1411ti
series- ,,tbenes.
yrrolYl -netbel"
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ip astituted
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dipyr
eel. ")v
P't,a)

HIROSIMICHMO, L.D.; TEVSTIGIILYEVA. R.P.; PRMBRAZHMISKIY. N.A.
lafrared absorption spectra and structure of some deriv&tlves
of P-diketones. Zhur.ob.khim. 30 no.e:2533-2536 Ag 160.
(MUU 13:8)
1. MoskDvskiy institut tonko7 khimlchebtko7 tekhnologii.
(Ketones --Spectra)

M1110STWICHMO. L.D.: FILAPPOT70H. To.I.; TUSTIGNITE7A, R.P.; FRDQMUZIMI-
SKIY. N.A.
Prototropic rearrangement In the lipyrr7loethene series. Dokl. AN
SSSr 134 no.5:1100-1103 0 160. (MMi 13:10)
1. Moskovskiy institut tonkoy khimicheskiy W-hnologii im. N.V.
Lomonosova. Precistavleno akadenikom AjR.Nesmeyanovym.
(Methene)

ZOTCHIK, IN.V.; IAIROSMICILM, L.D.; )Tl&.IMIEYEV:I, R.P.; . 'AIDBPL'.: 11-1 I:S',-IY,
11,A.
~;tudy of the Claisen condensa-ion of esters of levulinic acid and
their conversion products. Zhur.ob.khim. 32 rc,.9:2623-2628 S 16;~.
(MIP"'. 11 : a )
1. Mockovskiy institut torJ-.oy khimicheskoy tekhnclogii imeni
M.V. bomonosova.
(Levu-linic acid) (Claisen condensation)

','i ro s h n i
?rutotrUUi~
ao e m. r~,~
~'7
-,T3rtant naturil
~n tso clipyrry1methenes that
cif tliese substances can Liv-- il,.
,Dne -,.roui, of mesosubstitut~;
V
i ;rr
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Curu 112

troi. i c ree, roupto~ i
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recroupin, .9 9e
i; c~. *.ro~hc tome t ri c t it
~ic~r. takeq nlace at FA cert;,.
ures
j
f

GHOKASOVA, Ye.M.; YEAKUMAISHVILI, G.S.; HIRUSHNICIIENKO, L.D.
On the two products of aminomethylation of cyclohexyl methyl eton6.
Zhur.ob.khim. 33 no-01244-1U6 Ap 163. OUi--A 16:5~
1. Moskovskly institut tonkoy khimicheskoy tekhnologii imeni
M.V.14monosova.
(Ketone) (Aminomethylation)

~4-~ ~7'
-','ACCMICK-% NR
"AUMORVIlt]
77,
tion an, the ~-Cocanlw series
'602
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W
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iiij~ ",4ire.-AAWW~ td 'refine, their absoltAbe, 'oonfigurations
14 9.
tlxi,~ oil jo
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two -I;-! Woludad:1, iii, an Ints'imoloo-ular'
lbvvr,9906_':I~~d` - ~~i6li b riie~ .,dimm upoll dilu:tion. of Ah6 abluti. ,; anal 6govas V-
+
biopins Othir "Ifeatur, es~ of the adamtJon x*trw 6f
reg ML: id of* the (;-Off I":
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' /- / .
BUDILOV, L. 1. DOWNP V. 1. TVANnv, Y-. V. KOU4EYET!, f, M11403'al
Flar,- and the Propagation of Solar Cosmic Rays in Interplanetary 1pef
-F,:,rL submitted for the 8th Intl. Conf. on Cosmic Rays (IMP), Jaipur India.
2-i4 Dec 1963

ACCUSSION NHs AP4013"8 3/0203/6h/00h/001/0168/0170
AUTHORSt Dorman,, L. I.; 14iroshnichenkox L, I*
TITLE: The dependence of the diffusion coefficient of solar cosmic rays on their
energy
SOURCEs Oeomagnetizm i aeronomiya, v. 4, no. 1, 1964s 166-170
TOPIC TAGS: cosmic ray, solar cosmic ray, diffusion coefficient, solar particlej
scatterin.o. uniform distribution, scatterine center, magnetic cloud, magnetic
inhomogeneity, heavy nucleus, magnetic field, proton
ABSTWTi The authors started from an equation for isotropic spherical diffusion
as a first approximation for propagation of solar particles in interplanetw7
space. They found an expression to define the density of solar cos Mic rays on
tho earth. For a maximum value, this expression is written t max a R /6d, where
is the radius of the earth's orbit about the sun and d is the diffusion coefficient
(a function of the kinetic energy of the particle; its possible dependence on
distance to the sun is neglected), It is noted that in making calculations by
this formula scattering is significant only for protons and for uniform distribu-
tion of scattering centers in the solar system. Consideration of inhomogeneities
Card 1/2

ACCM1014 NRt A?4013146
in the distribution of mapetio clouds and of their movement in interplanetary
space leads to the conclusion that the diffusion coefficient and scattering depend
on the distance from the sun and that the timain uhich the majdw- Is achieved
depends on the velocity of the magnetic inhorweeneity. It is noted si conclusion
that the method based on using the indicated formla contains the basic possibility
of distinguishing streams of solar protons from streams of heavier nuclei, because
of the lover velocities of nuclei with z > 1 in any interplanetary magnetic field
(approximately half in a nonrelativistic field) than protons having the same
hardness factor. Orig. art. has3 2 fiLives and 8 formulas.
A3SOCIATIO14.- Inatitut semnogo magnetiama, iono.4fery* i rasprostrananiya radiovoln
AN SSSR (Institute of Terrestrial Mat;netism, Ionosphere, and Propagation of &iAio
Waves AN SSSR)
SUMurLD, WuO63 DVE ACQt O2Mar64 ENCLe 00
SUB COJEt AS, PH No Rr~? SOVt 004 OTHERs 003
Card 2/2

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MIROSHNICHENKO, L.I.
School on cosmic physics at Alma-Ata. Vest. AN SSSR 34 no.5:
139-141 Pq 164. (~G RA Y, 16 11,

ACCESSION NR: AP4033779 S/0026/64/000/004/0109/olii-'
AUTHOR: Hiroshnichenko, L. I.
TITLE: First All-Union School of Saace Phyficists
SOURCE: Priroda','no.4, 1964, iog-ill
TOPIC TAGS: space physics, astronomy, superstar, radio gaLtxy, radio emission,
gravitational collapse, Galaxy, interstellar space, solar physics, solar flare,
magnetic field, magnetosphere, solar corpuscular stream
ABSTRACT: The First All-Union School of Space Physicists was held during the
period 22 January-7 February 1964 and was attended by 50 Young scientists from 16
observatories and physics institutes of the USSR; the school was held in Alma-
Ata at the observatory of the Astrophysical Institute of the Academy of Sciences
of the Kazakh SSR. I. S. Sbklovskiy discussed superstars and the origin of radio
galaxies. Great interest was evoked by a report of discovery of objects of
variable radiation in the optical range with small linear dimensions in compiLrison
with galaxies. This discove5y appears to confirm the postulated existence of
superstars with a mass of 10 -10 solar masses and the tbaory of gravitational
Card 1/3

ACCESSION NR: AP4033779
collapse. The latter theory was advanced In the 1930's when it became clear
that the degenerate gas within a star could not withstand the pressure of the
outer layers, thus leading to a process of catastrophic compression (gravi-
tational collapse). Gravitational collapse possibly to only a catalyst, leading
to powerful electromagnetic mechanisms of acceleration of particles and emission
of radio waves. The possibility that cosmic rays escape from the Galaxy as a re-
sult of an increase in the diffusion coefficient with an increase in particle
energy was discussed. Among the topics discussed were solar X- and W-radiation,
the mechanism of chromospheric flares, solar radio emission, solar magnetic fields
and generation of low-energy cosmic rays on the sun. The latter problem is of
importance for predicting solar flare activity and estimating the radiation dan-
ger in interplanetary space. Special attention was given to Interaction between
a solar corpuscular stream and the earth's magnetosphere. It In important to
know the mechanism of this energy transfer; It is assumed by some that the trans-
fer is by shock waves arising in the earth's magnetosphere at the time of inter-
action with the nonuniform -go tic field of a stream. About one-third of the
reports dealt with cosmic ray variations. It was noted that cosmic rays my
~_Card 213
_A"

ACCESSION NR: AP4033779
accu=ulate in interplanetary space and in certain cases collectively overcome
magnetic fields vith a strength up to 10-" gauss. Orig. art. bag: 1 figure.
ASSOCIATION: Institut zemnogo magnettzma I radistaii AN SSSH (I
Terrestrial Magnetism and Radiation, AC3dEMY Of Sciences atitute of.
SUBMITrED: 00 DRME ACQ; 07May64 EXCL; 00
SUB CODE: AS NO REF SOV: 000 OTHM: 000
-3/3

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1964-,~:135' 6
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t: -to -'iL'-' Otto tha editor 0
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7,7077-, ~,77 ~ -7. 1, .7
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L 2o473-66 FBD/
I ACC NRa AP6012060
SOURCE CODEt
AUTHOR: Miroshnichenko.-L. 1.
ORG: none
TITLE: The youngest source of cosmic radiq_3Mypg.
SOURCE: Zemlya i vaelennaya, no. 6, 1965t 15
TOPIC TAGS: star, variable star,, stellar radiation
&/684/65/000/006/0015/001,5
ABSTRACT: This article is a detailed discussion of the radio source 1934-63. T1"i-8
object was investigated by Prof. jA-a&_1hklovskiy in 1965, who computed the secular
change of the flux and the radio emission spectrum. 7his information was reported
in Astronomicheskiy Zhurnal (Astronomical Journal), Vol. XLII, No. 1, 1965).
Shklovskiy believes that the age of the source is scarcely more than 100 years. The
indications are that the linear and angular dimensions of the source are varying
rather rapidly. He also believes that the source represents an extremely early stage
in the development of quasars appearing after explosions of enormous intensity. The
absence of optical radiation in sources of this type probably can be attributed to
light absorption in the expanding, very dense gas envelope ejected together with
relativistic particles at the time of the explosion. When in the course of expansion
of the envelope it becomes sufficiently thin, the optical radiation of the central
region begins to pass through it and the quasar 'ecomes observable. Orig. art. has:
11 figures. IJPRS)
SUB CODE: 03 / SUBM DATE: none

7- 7
-the:, tri
Pa.x.turf
nuidber
,,tr%jk~- ol
be c a U~ sif
AN -.SSSR
Vaves a
-6116
77
'Ojj
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-4

:~
4OL3 77

77

L 2o464-66 . E!v7ft)!FCC!WA(h) GW
ACC NRt SOURCE C ~/6-~/bod-~/o65 /69lo
AP6012057
f AUTHOR: Dorman, L& Is; Hiroshnichanko, L, I*
j3
ORG: Institute of Terrestrial Ma tism, tho~ n a mid ~~o Wave Propagatio
jq-q~!&~r
TITIE: Determination of the duration of emission of solar cosmic rmp from the gone-
ration region I
it SOURCE: Goomagnetitm i aeronamiya, v- 5. no- 5. 1965, 910-913
TOPIC TAGS: cosmic ray, solar radiation, solar corona, solar chromosphere
ABSTaACT; A diffusion model usually is used in the investigation of the
propagation of solar cosmc rays in interplanetary space. Me density
change of solar particles in cpaco and ch6go with time is described
approximetely by a nonhomogeneous equation of the parabolic type. A
solution is easily obtaiqcd. Source density is thle quantity of particles I
emitted from the source (from the region of generation) in a unit time
and Ln general is a function of ~,kin and t. It is determined by the
character of generation of particles on the sun and their propagation
in '%'he solar corona and 6upercorona. At present there is no detailed
information on the character of the dependence of f on 6 kin and t W
is source density);'it is only knoum that f (Skins, t) rapidly attains
a maximim after the onset of a chromospheric flare and then drops off
steeply approximately exponentially. In-the-case ofjow energies
Card 1/2 mc: 523.165

L
mk.%. "m
kin, t) can be dram out considerably in time, which is partly
responsible for the considerable lag of low-energy particles. Expres-
sions are derived for approximatuLng f. Since recent data indicate the
possibility of accumulation of low-onorgy solar particles in inter-
planetary space in years of high solar activity, the authors have in-
vestigated the nonhomogeneous parabolic diffusion model equation in'
combination with their proposed expression for f for, the case when
emission occurs uniformly over a finite interval of time. With an in-
crease of T (emission period) the maximum of the density curve is dis-
placed in the direction of larger values to The density increase occurs i
quite sr.-,oothly and the decrease after the maximum. is quite steep. When
t :>, T the density decrease conforms to the diffusion law It-372; this
is applicable to an instantaneous source. In the case of prolonged
anxission density increases to a ra-ximum, more slowly and then begins to
decrease much more rapidly. The results make it possible to use the
temporal variation of intensity change of solar cosmic rays to determine
the duration of their mission from the region of generation. They also
show that for study of the duration of emission of solar cosmic rays it
is most important to have detailed measurements of the particle flux no *ar
the increase maximum, where the influence of T is manifested most strongly.
The authors thank Yet A. Kornitgkajg, To L. Yjazdkows, To N. Utkina~ya, and Do I*
Fishchuk for canryi-ng out the calculations OrIgo arto hai-s7-figures. 8 foiiiUs
wA 1 tabie. Ij_PRsT
SUB CODEt 03 04 / SUEN DAM 29Wo64 / (RIG W: 004 / orH pzFt ool

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:,.' ~;! - i~ : -- ~, -4", `..!;'~., ~ - 2 - .~ ~,.,--.; - II. : .1 ~' ~~ ;: -.1, ~.-, .",''-, ;~r.. ~- - - '. A : ~ , - -;, , . ,
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i!2

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4,

'
bii~W Liire~eilts. Of 'Solar
pr6tid by 68
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-
.
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ary patiq
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.
,
Oan_j 0", 9, _AW ge-.`miikhetiz6&-dloudir of,aolir,viattei~. This lco'nclusiod
f t11'.
"simb bd.'_thd~~, ypdt6a o. ~.. e, so-caU6d"fore~(ae''os"megnitio fields 6Avocated by.
Occcir~~! to~ `-4~ ormat ong move.from sun to,
2000.~ ~p' nd
it:w f m ... dr peco Their
e4A h- w h-;'Tq P
.
the, eijg;j._':Solar!'_T'Rrt
movewht do6 a noV, ai 6 a' t-.
propa~
-
6o'cuifpd'on::the nohhomogei4itiesk

Ider6t,"stat
p~.pons
.
_b ui;:IdstiWV
A=Iift' ai, G- ma- ionod arr,- -.,,rasprostraneniy~w radiovcria
and Radio Wtva
.
a a

EMDU
60 AL
SUB OD
-
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EWT(1))
ACC MAs Ap 5*026223
/F-WA (h) GW
SOUWX CCDZ:
AUTHOR: Doman, L. 1. ', MI rosbuicheako. 16,
ORO: none
UW0048/65/029/010/1810/1812
37
TITIZ: Solar cosmic rays from the flare of 28 September 1961 and the properties of
Interplanetary space (Report. All-Union Conference on Cosmic Ray Physics hold at
Apatity 24-31 August 1904)--
SCUWZ: An SSSR. Izvestlya, Serly4 fixicheskaya, v.29 no.10, 1965, 1820-1812
TOPIC TAGS: cosmic ray?~polsr flaryVphysical diffusion, Interplanetary space,non-
homogeneous magnetic field
N2/
ABSTRACT: The measurements with Explorer -12 of the cosmic ray intensity during the
28 Sept. 1961 Solar flare were compared with the predictions of the authorts diffu-
sion theory Of cosmic ray propagation (Geomagnetlam I aeronomlymo 50 No.3,337 (1965).
Agreement could he obtained by assuming that the particles began to be emitted when
the x-ray burst reached Its maximum some 15 minutes after the onset of the solar flare
The scattering mean free path was almost Independent of particle energy for energies
from 10 to 600 MoV, and was approximately 7.5 x loll coo The differential mission
spectrum was found to be 5.6 x 1034 g-2 protons/MoV. where It Is the kinetic energy.
A lower limit of 5 x 10-6 G was found for the strength of the magnetic field Inhome-
Card

L 6944-66
ACC NR' AP 5026223
geneltles. If one asst a on the basis of measurements with Karl3er 2 that the
strength of the magnetic field Inhomagenelties Is 10-4 0 one finds that a linear dl-
mension of such an Inhonogeneity is approximately 4 x 1010 cm, which Is about half tile
distance between the Inhonogeneitles. OrIg. art. ham: 8 fomulas,
SUB CCOX: AA/ SUBM IDATX: CO/Oat 63 ORIG. W: 001 OM RW; 001
I CWd--WX

I ~ I
,I . ., .

I~MOSIINICFENKO, L.I. (Ho.Akva)
San as a "broom" fcr C(13rdr; rays. Priroda 54 .3 1(-~.
,, '1"A -13:,-
k 4- 1

L 39895-,",6 9qT 1)/3WA (h)/P~C GWI -2
-- (- --- Lr)
ACC NR, 018097 1,011RCE COM TTR/0203/66/006/002/0215/0222
AUTHOR: Dorman, L. I.; Miroshnichen o, L. 1.
ORG: Institute of Terrestrial Magnetism, Ionosphere and Radio Wave YropngutltT~A A-"'K
(Institut zemnogo magnetizma, ionosfery i rnsprostraneniya radiovoln)
TITLY: Method for determining the spectrum of solar cosmic rays In the high-enerFy
region
SCURCE- Geomagnetizm i aeronomiya, v. 6, no. 2, 1966, '',,,-222
TOPIC TAGS: cosmic ray, conmic ray shower, cosmic ray measurnment. solnr raliaticn,
ion.'zation chamber, solar spectrum
-ii~lt.':ThiG paper presents the results of computations of the integral
A ij-
m~iitipiicity of generation for a neutron monitor and an iorLizatinn
'rhmiber. The computations for the neutmn monitor were made usinr t-111P
latitude effect of the neutron component At sea level. The interral
mult,lplicity of generation for the ionization chuTiber was co.ipited w.
the basis of the latit.wle effect, of the bur!3t of 23 February 1956. On
the basis of the compaited generation multi pliciti ea the with-,ro detf-r
mined the spectrum of solar cosmic rays at the boundary of t-o
for the burst of 23 February 1956 in the reglon of rigiditle-, 1-15 ilt!).
orig. art. hWb,- 11 Ngnirev 9wi -"I forTmilas. Z.',P
, I I r-, ~tj
n4 ;)A
'nn~)5/ 0,qJCj HEY: r)()~/ F-T! '-FF:
--C.,d I i -

AC C A. 7- 7 3
T I T L.-:
Cc, 1 Cray,
1-5
7r
~y
2-1 Yzy-1)
'L) L L
t-on of
Gf t'heir
C~u t 0 C.~,--CL-vjl~r ~X, .-Ii) ~,O '--.0 Of
a S&rt-c-~ - ". 1. ~~:,Q.-,Cntcd a
ti~n of cox--ic ray vax-.atiorx wlhlcti ta;~cz. account
Cord 1/2

ACC NR~
f 0
effCCL3 of Cif,`u3,Jon, ~_n pax-.icula.:.
L.-yez-r, 27-day ari. variat-ons. -,-.o
i3 essentic~!~ 0:, -_a SJZC Cf the
"-tion 1;-. . -
region, d=~.A'.-.;sic),-. coefficie:%-. and wrind.G
-iat ~hc -~odula-~- ;~ro.:.cs3 can be cc,-..3_'dc.-,zI
ca--a of v.
3tationa.:-.f 110:- P_'-t_*C_'03 a. high ri~-Jkdity and utLh a suf-
ficilently %,''us of t'.io dif.'L_,; rci;_,on 'zbour, 1W z,3'~ronoz-1cal
"t3). 3~_-Ico tau r~jffusion coefficient t.-)o nor..-clativistic ragion
-is oz3cnt_:.-__'y dcpcndant on the hardnen.3 par.1cloo the amplit,~11-.Ia
-.-cilI bo for paxticles with difforo.-.t. charges. S. N. Vornov
o'd of '.-e o.' the intcnsity of lo-,.,-cncr7 cos. c r s or,
-,,jr L! ay
solar ac.~.v.4t-r and dz;-.znce to the sun. ray intensity c.-1 an~, e a
irr, ci;ularlj -~he cycle of solar activ_:ty and corrclates ,r-th tno
,,,up in aun5;~O-. , ~bor (th4z conclasion wzr, d.---,,m on the t~asis of
nur
3trutospheric MO,15urcmenta). -,no exi,tence o.7 a razial grad!.ent of
co_-_Jc rays ii. space c-a-I bu ma~;~,-ed by tempora:-y intcrs-_'ty
aria, r -
_,,13 ','.-ie measurement pe.-iod. 3. !-. __,~Ii3 presented pro3ent.-
d,~Y ideas or. tnc _~..-ucturc ;-rd -..c G. Ye.
Aocnarvv 6avc on ne-trino a;-.Ci noted the
b,-egA' in t'no co---,ic ray spectrum ~_r, t %o reZion of energies IG15-
10 aV can be attributed to the interact-4on of nc,-trinozi and protons
of superhigh energies. V. L. Ginz1burg =pna~-Zlod 'no need for work
in the field3 of ;:-ray and gamma-ray astronomy. ~,~
LJPRS: 39,10
-Card-21-2

MLROSHRICHMO, L.P.
Blolog7 of vild fodder vetches under cultivation. Ukr.bot.zhur. 17
no.2:43-" 16o. (MIRA 13:11)
1. TSentralInaya Slaellaikovakaya selektatonno-issledovatel'skaya
stantelya Tsesoynznogo nauchno-ionledovateliskogo InstItuta kukuruzy.
(vetch)

BORZTAK. P.G. [Borz1aJsv P.H.J; MfROSHVICHMO, L.S. [Mrroshrqchenko. L.S.];
SARM,-D.G. CSarbei. O.HAT-
Photoelectron emission of germanium and silicon In the amorphous
and crystalline states. Uirr.fiz.zhur. 4 no.4:521,-525 JI-Ag
'59. (KRA 13-4)
1. Institut fiziki AN USSR.
(Germatum) (Silicon) (Photoolectricity)

81778
0
S/181 601OG21021'2210"
B006XB067
AUTHORS: Borzyak, P G.., Miroshnichenko, L. S., Sarbey, 0 G
'Y I --- )11 1/1
TITLEt Photoelectronic Emis6ion of Germanium and-Silicon In the
Amorphous and Crystalline Statsf,
PERIODICAL: Fizika tverdogo tela, 1960, Vol. 2, No. z, pp. 414-z/18
TF-M The germanium and silicon sam;les examined by the authors were
produced by vaporizing films onto metallic backings. The germanium films
were sputtered onto tungsten backings, cold as well as at T c 450 0C.
Electron diffraction Ptudies showed that the films sputtered at room
temperature were amorphous, and crystalline at increased temper,sture
An investigation of the contact potential differences between the
amorphous ftnd crystalline films produced under otherwise equal conditions
showed that the thermoelectronic work function of the latter was some
ton electronvolts smailer than that of the former, Fig. I shows '-he change
of the work function Aq(t) with time of simultaneously sputtered BaCl for
crystalline (Curve 1) and amorphous (Curve 2) films- The values of the
primary photoelectronic work function of crystalline germanium films are
Card 1/3 V~'

81778
Photoelectroni~3 Emission of Germanium and Sili- S/1 81 C02 --,'221()
con ir. the Amorphous rind Crystalline States BOC)6/BG6'-i
lower than those of amorphous ones Experiments were also made with
morocrystalline p- and n-type germanium samples The preparation Df
these samTles is deacrited; the Ture surfaces of the single-crystal
samples were obtained in such an evacuated tute as shown in Fie 2
Fig 3 shows the spectral characteristics of the photoele~tronic (-7:s
sion of three crystalline germanium samples with reduced work
Curve I refers to high-resl3ta,-.ce single-crystal germanium, Curv,
n-type Ge single crystals with 3 ohm c~m, qnd Curve 2. to a cryst4lilr.E
film Fig. 4 gives a comparison of th,~ :;pectral characteristics Df
amorrhous and crystalline germanium Similar investigations were ~jlso
-ade with sillcor, The a-i-orphoas fi3ms were c1tained by sputterinF orto
* h,icking at room Lempr.,rpiture, th,a crystalline ones were -Atained from
* p-type sinele crystal in high ,,~r-aum The spectral charFicteristirs of
these samples are also 9r.,,wn in Fig. 4 For comparison, this diatr~.Lrr.
shows the characterig'1--s of the ;ipectral. sensitivity of W - Bao
photocathode2 hrid tw(, ',s,O"b sarriples In contrazt to anorphous ttrmaniurr,
3rystalline -Orwj it weak miriimu~r ,n the short-wave rut;4 r. 0.1
correqp,nir to ttip -~;ix~- .,r. ,f thtj -~.arar*eri2tic if U.P
'ard

P,-1 7 P
Photoe'lectronic Emian1--- of ",,~rmani~m and Sill- c./ I P~ /'6 2/2
-on I n 'he Amori-nc ua qrjd Cr.vr~ ~ -%4 11 no S tat~s BGC , P~-, - 7
re f I t3c cri (if cry,-, t ti~ II r.,~ rm,iz, i ,,.r A.Tci rj hcluv, P aaq I e.1 do no t u v-r Klive
O.ir maxlm~im 5irrc- JI tic;,l i~,7orpt!-)n ir; silicor is weaker t1,,,r ir
6ermanium, the p~.otoo' ectron,~c sensit.-jity of silicor. is also lower
Such a parallel cannot ~~? ob:7~,rved in a com,--irison of germaniu-,r iir.d
'a Sb In -onclusion , the t,--ithr vs t hurl':, ProC4,s: L N Narledciv fcz- Iri,
rr4parati - --f tl.e S. Ye 3 and A N
K-iasni i fnr t- f ~.- .,,rTrF,niUM 3infle crystaln, 4r~ ~ N1
K L1L i n the ~!ond--ictirin Of the electron diffraction studiegPhere
are 4 fiEures and 4 refer~n-vsi 5 S,)viet ~:&nd I Amerloan
A'JSCCIATI,-N: In-titut 'izlkl AN Klyev (Institute of Physicq of-'he
itS UkrSSP
5"BN;1 TTED! Apri I 5r)
Card 3/

BIDULYA, P.N.; SFUL'TE, G.Tu.; PEL110i, V.N.j HLADOVA, A.A;; SHERSTYUK,
A.A.; HIROSUNICHMXO L.S.
Nonmetallic inclusions In malleable cast iron. Lit proizv. no.l:
25-27 Ja '61. ~ MIRA 14,' 1)
(Cast iron-Defe.ets) (Nonmetallic materials)

17, ~- f 7S- 24919
:?
o r 7. ~i alk i r !~ r r
T IT:- p t i --i I , r or e r t i - -, r, i
F --R 1 F i z i ~- % I v- r 4 -) w(, t -: ~, , v
T -.'XT: %I,- Z~ ? I t he i r, t erm- t d C,
thorou,v,,ly Y.e--etofore, ta-
tric ~jnd optic4l proterti-f-. 't
were prerared i n d i f f,~rs~r t ways r "I Ti L r 1~
initial substiinceg had '-epr~ su,-.T i -d
neorg,!nic~eql~oy khimit AN TJS:~P'~ I ri- t
AS Ukr7)SR) by V. P. Zosimovich. T t. e r r.
rreDared in three di f ferer t ways were t
vioualy (FT', aid
0 p t i c a I con.9tants: t e e F1 .9 r I'M o-!
r!oeff jCertq r,f I jo~,,J.t r,f r j r
'.'ard 4

249 9
r t i c ~i I . r,) r P r t i e s o e
of Fir. C,~-A! "F-4 ~ spec., trc- rot--):ret P. z
254 - 17F~ m~k sr-er tral r-Ir ~re , h I - ~ . Y.,
t~.e ~5C - 1 ' ' C~ m~4 runge ~.n
> I K t
we re usod ~or diffe-P, e r;, i r,,., A
light scattering -&~is i
the exTerimen* s w a s c; ~ t t i, v
o f s e I f - a t s o r p t i o r~
ir.terferer-e method. F i m
t~ e sel f-atqorT-.t i on rAo!,. -,r. !.p r-i
tric const:int Fit hi f A,
R,ramp R f hv I IFht fil tr t 'V
n - aj e r .9 o r~A '~,e ', i -r.t ~i r- e
eml a .9 i on w i t h S F - 4 1 vlcf)- 2 P .:p -
a ri: r, -) f t k, p t e npK- PRX-4 tI.H
ci.romator was detpi T,: r.- i ~ y : ehr.9
were measured by a d-c ua I ; f r
co- pn red wi t h t h se o f '~a Z b re ,i
Card 214

;~q "q
optical rror.-ertlo~.q ir I ---.e 'r
I~a rat., t s - i t i c
to to
A F,
f f i
a
ffin
~40 to
"he data for Na,St -,r,- r -n F
laboratory ap. i e aL;* !.or.-
of t r e i r i ;r 'a -e~:
duc-d ~,Y i s t t. e r: c~ r. -a.,
Ye,i e I ' s or, re -i eri o r t,
Sove!-~ loc ~i,d v. 'L
"ard '. 4

24919
Tt i c
T-uhliratio~s read ai Ii , vv V/~
P . 3 r 1 i e , e r t ~i r as r.
E I ec tr P!.-. .9c -td
AT I
rev i n
-,t rd

22909
S/109A 1/0u6/004/024/025
C?I E 140/E 135
AUTHOR: Miroahnichenko, L.S.
TITLE, Photoelectronic emission of LaBA
PERIODICALi Radiotekhnika i elektronika, Vol.6, Nu.4i, 1961,
P. 673
TEXTj The results given in this paper have been presented at
the All-Union Conference on Cathode Electronics, Moscow, 1959.
The author studied the photoemission characterimtics of specimems
with various surface states. The specimens were inside sealed
tubes, heating was by electron bombardment to a temperature of
1200 OC for a duration of about 20 hours. The results are plotted
in the figure. Curve 1 applies to specimens with the surface in
the initial state and placed for a long per .0d in an atmosphere of
residual gases with a pressure of about 10-A mm Hg. Curves 2 and 3
apply to surfaces which have been purified to different degrees
(by heating to about 1100 OC) (dashed line curves represent the
results of Lafferty, Ref-3). The work function values determined
by the method of Fauler were respectively 3.55, 2.89 and 2.77 eV.
Optimal coatings of the initial surfaces with molecules of
Card 1/ 3

?909
s/ lo ()/6 1 ~006 /00 4 A 24 /0 2 5
Photoelectronic emission of LnFJ6 E1160/L135
barium oxide leads to a shift in the spectral chara-teristics to
the positions of the curves 11, 21 and 3' and to changes in the
work function values: 2.07, 2.12 and 2.24 eV, Stirfaces that
have been most purified showed the smallest optimal reduction in
the work function, 0.53 eV, which is very small compared to the
reduction of the work function of ordinary metals (tungsten, gold,
tantalum, etc). Results obtained with GdB6 specimens contradict
data given in the literature; the spectral characteristic for the
surface in the purified state is shown by the dashed line curve,
The work function is appr~,ximately 4.6 eV as compared to 2.1 eV
quoted by G.V. Samsonov (Ref.1). By means of BaO the work function
of the specimen was redaced to slightly over 2 eV
Acknowledgements are expressed to P.G. Borzyak, G.V. Samsonov and
Yu.B. Paderno for their assistance.
There are 1 figure and 4 referencest 2 Soviet and 2 English.
ASSOCIATIONi Institut fiziki AN USSR
(Institute of Physics, Ukr.SSR)
SUBMITTED: November 9, 1960
Card 2/3