SCIENTIFIC ABSTRACT KOROBKOV, V. I. - KOROBKOVA, M. P.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000824730009-8
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 14, 2000
• Sequence Number: 9
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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M.5

The Electric Conductivity of the Aqueous Solutions of SOV/20-126-2-28/64
Sodium Hydroxide at High Temperatures
portion of covalent binding in the molecule of sodium
hydroxide. An exact interpretation of the process will be
possible only after a large number of experimental data will
have accumulated. There are 2 figures, 1 table, and 6
references, 5 of which are Soviet.
ASSOCIATION: KharlkoV;3kiy sellskokhozyaystvennyy institut im. V. V. Doku-
chayeva (Khartkov Agricultural Institute imeni V. V. Doku-
chayev
PRESENTED: March 3, 1959, by A. Y. Frumkin, Academician
SUBMITTED: February 99 1959~
Card 3/3

RODNyANSKjy, I.M.; KoFtOBKOV, V.I.; GALINKER, I.S.
Specific volumes of electrolyte solutions at high temperatures.
Zhur.fiz.khim. 36 no.lOt2216-2-219 0 162. (MMA 17%4)
1. Kharlkovskiy sellskokhozyaystvannyy institut imeni Dokuchayeva.

GALINKER I.S.; RODNYANSKIY, I.M.; KORQMOV, V I. - LEKAKH N.B.
.9 -4.L.Z:y .9
Temperature-dependent differences in the thermodynamic pro-
perties of water and electrolyte solutions. Ukr..fiz. zhur. 9
no-4:401-405 Ap 164. (MIRA 17.#8)
1. Sellskokhozyaystvennyy inetitut im. V.V. Dokuchayeva,
KharIkov.

KOROBKOV V I - RODNYANSKII, I.M.
Compressibility of saturated monoatomic alcohols and their aqueous
solutions at 2370C, Izv,vys.ucheb.zav,; khim. i khIm.tekh. 8
no.W14-217 165. (MIRA 1818)
1. Rharlkovskiy sellskokhozyaystvennyy institut imeni, Dokuchayeva,
kafedra obshchey khimii.

LUKIYANOV~ V.B.; KCROBKOV, V I.
Study'of the method of relative measurements of radioactivity by means
of dispersion analysis. Radiokhimiia 7 no.3050-355 165. (MIRA 18:7)

DARAFOV.9 V.I.; DU IB-TYANE j:Tu Id,eh-t Ilan]- KOROBKOV,7 V.I.
G
teochemistry of urmdun and thorlum Jn granite rocks of the Kyzyltau
- massif ?.,,entral Kazitkhstan). Report No.2: Occurrence form of
radloactive element.-i In granite rockso Geokhimlia no.5-,411-419 162.
(MBA- 15-7)
1. Glixtr of gbochendstry and chaLr of ra,,Uachemistry., Moscow State
Tfo-lf rorslty.
(Kyz,vltau Region --- Radioactive substanzes)
(Fyzf,tau Region-Granite)

I cS:
II-,)2 and f9 ~>> f2' where --~ is the
I c
effective number of collisions of electrons with ions and
neutral molecules, and f. is the critical frequency of the
F-laver, then the integral absorption is given by:
2
e N -~ dz (2)
mcf
In this expression N is the electron concentration, z is the
thickness of the absorbing layer, e and m are the charge and
mass of the electron, and c is the velocity of light. it then
follows thatr I/r 2 = (f2 /f 1)2 and hence, finally, the integral
absorption for each of the frequencies is given by:
In (1 02 /1 01 - In (1 2/11
2 2 (3a)
Card 2/7 1 2

21166
S/i4iAo/003/oo6/005/025
E032/Ell4
Results of Measurements of the Absorption of Radio Waves in the
Ionosphere
and r2 = r. (fI/f2)2 (3b)
if 102/Iol does not depend on the galactic coordinates then
changes in ri with time depend only on the ratio of the two
frequencies. In fact, the above intensity ratio is not independent
of the galactic coordinates but t'Ais fact should not lead to large
errors in the absorption measurements. Published data on the
absorption of radio waves in the ionosphere during night hours
shows that the absorption is frequently negligible. If the
intensity ratio 1()2/Iol is determined for these hours, then the
absorption for any other time can be calculated from Eq. (3)-
It may be shown that the optimum frequency range for the above
method differs from the standard method (described by Blum et al.
in Ref.2 and Mitra and Shain in Ref.3) in that it does not require
highly specialized apparatus or prolonged observations. The
present authors have used the above method between August and
Card 317

21166
S/141/60/003/oo6/005/025
EO32/El14
Results of Measurements of the Absorption of Radio Waves in the
ionosphere
December 1959 on 8.6 and 25 Mc/s. The results obtained show that
the absorption has a characteristic maximum at noon each day, and
a minimum at about 4 hrs. In August and September there is also
an additional evening maximum at about 20 hrs. The magnitude of
the noon maximum was found to be 1.1 db in August, 1.15 db in
September, 1.2 db in October and November, and 1.6 db in December
(on 18.6 ",cls throughout). Fig.4 shows the diurnal dependence of
the total absorption (continuous curve) and the absorption in.the
lower layers of the ionosphere (dotted curve) averaged over the
periods 23rd to 31st October-(Fig.4a) and 12th to 15th November
(Fig. 4 6). The reoults obtained by the Radio Astronomical methods
were checked by means, uf the pulse method des-'.ribed by Pigott et al.
(Ref.9). Fix.5 shows the dependence of the czbsorption in the
r-itical frequencies o
P-layer on the c. f the F-luyQr (18.5 Mc/s)
(curve I - 12th to 15th November; curve 11 - 20th to 31st-October-,
curve III - data from Ref.3). Acknowledgements are expressed to
G.G. Getmantsev and V.L. Ginzburg for interest and advice.
Card 4/7

s/i4i/61/004/004/022/024
E032/E314
AUTHORS- Benediktov, Ye.A. and Korobkov,_Yu.S.
TITLE: Absorption of Cosmic Radio-emission During the.
Magnetic Storm on April 1, 1960
PERIODICAL: Izvestiya vysahikh uchebnykh zavedeniy;,
Radiofizikai 1961, Vol. 4-, No. /*,-PP- 763 - 764
TEXT: The present autho *rs report observations of the
intensity of radio-emission on 18.6 and 25 Mc/s. The
curves art--shown in Fig. 1 (the,25 Mc/s record is displaced
in the downward direction relative to the.18.6 Mc/s record).
The broken curves show the approximate lev'els of the undisturbed
signal. The top curve shows the variation in the Earth's
magnetic- field H in the same region. Assuming that the ratio
of the absorption coefficient at these two frequencies is
2 2
W +
2
W2 + 2
r 2 1
Card I

Absorption of Cosmic ....
(Ref- 3 - V.L. Ginzburg -
Pizmatgizl Moscow, 1961),
it is found that r,U8.6
s/14i/ft/oWoO/021/024
E032/E314
Plaiwa-wav* Propagation,
Me/s)/r-2 (25 Me/8) = 1.5 so that
^.V i . 4 x 107 see- I .For a normal ionnnnhar^ +him VAIIIM nP
corresponds to altitudes of the order of 65 - 70 km. During
magnetic disturbances, absorption at such altitudes occurs in
the Polar regions. As can be seen from Fig. 1 there-19 good
correlation between the intensity variation and the magnetic-
field variation. The correlation is less well defined
when the curve obtained in the Leningrad region is used
instead of the magnetic field for the Moscow region. Ackngwlbdg-
ments are expressed to G.G. Getmantsev for assistance in this
work. There are I figure and 6 references: 3 Soviet and
3 non-Soviet. The three English-language references quoted
are: Ref. 4 - W*$H. Campbell, H. Leinbach - J. Geoph. Res.-,
66, 25, 1961; Ref. 5 - S. Ziaudin - Canad. J. Phys., 38 '*
1714, 1960 and Ref. 6 - T. Obayashl, Y. Kahura - J-Radlo7 Res.
Lab. Report Ionosph. and Space, Res. Japan, 14, 1, 1960.
10-01
Card 2//,(,:7

s/141/61/oo4/oo4/O21/O24-
Absorption of Cosmic.* ... ~~IJ32/E314
ASSOCIATION: Nauchno-issledovatellskiy radiofizicheskiy.
institut pri Gor1kovskom universit6te
(Scientific ReSearch Radiophysics Institute
of Gorlkiy University)
SUBMITTED: March 23, 1961
Card 3//~

h2157
S/203/62/002/001/005/019
1023/1223
AUTHORS: Arteml-yeva,G.M., Belikovich,V.V.,, Bonedikto,~.,,Ye.A.,
Yeru!diimov,Z.,*A. ard Korobkov,Yu.S.
TITLE: Measurements of cosinic radioamlssion absorption
during the solar eclipse on Febrnary 15, 1961
PERIODICAL: Geomegnetizm I Aeronomiya, y*2, no.1, 1962, 68-60
TEXT: During tne solar eclipse of February 15, 1961 observations
of the cosmic radioemission were made In Yevpatori7a at the
following frequencies: 25, 18.6 and 13 Mes, and in Gorlkly at
25 and 13 Mes. Such measurements were omjtted during previous
eclipses. The purpose of the prosent measurements is to discover
any decrease In the absorption of cosmic radloomission caused by.
the solar eclipse and to differentiate between the absorption of
.different layers, 'The apparatus used in bq~th,,p~lac~s was identical,
The receiving antenpas consisted of six wav'S*4-14retors. The
ointed t the zenith, and the width
maximurd d4-r-ec-t-1Z am was p . 0
at half power was 300. ~The inoasuroments were aonducted for 10-12
Card 1/3

S/203/62/002/001/005/019
1023/1223
Measurements of cosmic rndioemission...
days, before and after the eclips.e.- Data from the five days, on
which foF2 was not much different from its value on the eclipse
day, were used for further analysis, The variations of the
absorption during the eclipse are presented graphically. In
Gor'kiy at 25114cs no effect was observed within experimental errors.
The maximum decrease of the abaorption is shifted several minutes
with respect to the maximum of rhe eclipse. The lag is near to
the value of relaxat Ion time, I?. the D-layer. In Yevpatori-ya a
second, smaller maximum, lagging by approximately 30 min, was
observed. This me-xi=m is probably connected with changes in the
absorption in the P-la-yer, where the relaxation time is much
longer than in the D-layer. The ratio of the mqximum changes of.
the absorption in Gor'kiy and in Evpatoriva is-approximately equal
to the ratio of the 'Solar zenith angles cosines. The main reason
for the changes In the atsorption are changes In the electron
density In the D-layere There aro 2 figures and 1 table.
Card 2/3
Card 3/3

36965
S/141/62/005/001/012/024
E203/E435
AUTHORS: Korobkov. S., Eydmin, V.Ya.
t__Yu
TITLE: The radiation reaction of a moving charge in a
waveguide filled -with an anisotropic dielectric
PERIODICAL: Izvestiya vysshikh ucb.obnykli zavedeniy. Radiofizika.
V-5, no.1, 1962, 122-127
TEXT: A full mathematical treatment is given of the motion of
an electric charge in a waveguide filled with an anisotropic
dielectric for the case that the axis of symmetry of the crystal
is parallel to the waveguide axis, and also the case when it is
at right angles thereto. Starting from Maxitell's equations
the authors calculate the energy transfers between the particle
and the electromagnetic field. The energy equation-splits into
separate equations: one containing terms due to the rectilinear
component of the particle's motion and the other containing those
due to the oscillatory component. The first equation gives the
Cherenkov effect, the second shows two effects: the first
corresponding to an energy loss by the'particle (normal Doppler
effect) and the second'to an energy, gain (anomalous Doppler effect),
Card 1/2

S/141/62/005/001/012/024
The radiation reaction E203/E435
If the terms giving the energy loss are now equated to zero, the
condition is established under which a growth of oscillations must
take place,
ASSOCIATION: Nauchno-issledovatelliskiy radiofizicheskiy institut
pri Gor1kovskom universitete (Radiophysics Scientific
Research Institute at Gorlkiy Univerzity)
SUBMITTED; June 9, 1961
Card 2/2

t'-hT--,'M't-vE'VA. G.M.; BELIKOVICH, V.V.-- BENEDIKT.CIV, Ye.A.; YERUMaiTI, L.M.;
ITKIIIA9 M.A.;
Resultv of observatkQas of intensity fluctuations of discrete
sources at low frequencies, Goomag. I aer. 3 110-5:835-840 S-
o t63. (MMA 16:11)
1. IIj)diofi--icheskiy institut p! Gorlkov&kom gosudai-stirennom
Universitete.

-P-e
�rm
WrWr (-V)
C C E S CS I I 1 41' IT R AP4
04GZal 02011641004

Radfofizicheskiy institut pri riort~-Ovqkom I-oqud!rat-
Q c TZ a o T) 11 y q c t
ATD PR88S, j L ENCL 00
AA-- NG~'REP S-GVt-- 003 OTHrRi 003
2 2

KOROBKOV, Yu.S.; PISAREVA, V.V.
..............
Some result's of investigations of E layers in the region of the
Pacific Ocean. Geomag. i aer. 4 no.S:866-872 S-0 164. (KRA 17:11)
1. Radiofizicheakiy institut pri Gorlkovskom gosudarstvennom universitete.

7 . . . . . . . . .
2 7~0
L WCO/2.1c EG INIA(h) pq~~k/
-" -csm- ray emission, radio asL-~ono.-,'
T"he C;-1st~ri.bution. spectrurr, Of Sm. n e 3 0
mp-te-" band was not -qh--,,;s that
2-S Oc irterest Ln connection cosmic-ray research and
.-s~--,nnomica- .~nves-
In conif- 1- the use o' th-is fo- ra--,c-
tlga~--icns of the -ionospl-here. Pesullts are reported of the n~easure-
-"e =Pectrum oF dis~r4bul--A -osm4c emission 4r, t',e
0 1, To e-,clude
..c ban,3, made in Septembbe-r a
inFluence of t-he ionosp-ere, ~'-e -ere made
Card

thd7--~&itz d6rfa~-&-re cU
m na 7&f~
nined by the'angle
a center having galactic coordinates 1 98,50 and b
resLA-11--s show that the temperature decreases nearly exponenti ally
a S 4 n, C1 Frequency, the relative intensity is "airiv flat up
,,:o about 1-0 Mc after which it drops off, and the spect-~al index
rises in this Erequency range from about 1.9 to 2.5, its value being
given by a' =~ 2.7 2.1/2)- frequency in megacycles) . n, e
reasons for the drooping nature,of the spedtrum are discussed
briefly. Various factors affecting the accuracy of the results are-
discussed. "The author thanks A. F._-X-arasov for help and
Tseytlin for valuable remarks." Orig. art. has.- 2 figures and 1
Card 2/3

5
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41

_71-7-'-Ii~- 7777~
1. A obt
on pattern on the earthts surfwm waa olAdined.- tfie7-67*C~4
7h e diffra-ati
fcrnula was used for T, the time for irregul-ar chang-es in the Bigrial the
Fraunhauf er region ----
(h +
j
1.0 fih~mdgeneity._ the velocityof the &atc-
aer
7 dtt'e -.'h of the Anhoir
I the 'Phaee sWt'. --to t6:,, inhqi~ thd ~aiiitixde
I- the dbaei~fttt6A6` that'.the
-2 - -
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dndex of fluctuation ia
f cland to be the r - Th---"- a
well correled6d-to Uffusenead: or-. -2 layer., e doe icient-bf

.L 1713-66 EM(l)/FCCAWA(h). GW_
ACCESSION NR: AP5020999 UR/0203/65/005/004JO69810104
550488. 3:550. 30.2 02/-
AUTHOR: Benediktov, Ye. A Korobkov, tis SO Tolmacheva, AL. Vv 0
,TITLE: Anomalous ionization of the lower Wupbue over tomperatelatitudes durial
global geomagnetic storms
SOURCE: Geomagnetizm,i seronotAya, V.: 5, no.. 4# 1965, 698-704
TOPIC TAGS: ionospheric ababrotion,.-tonospheiric inhomogeneity, TMetic atorm,
geomagnetic disturbance radio wave.absorptiow.
ABSTRACT: Anomalous ionization of~the lower i~onoaphere, -causing additional ab-
sorption of radio waves, is observed during gtobal geomagnetic storms over temperatb
geographic latitudes. This paper reports on t%easurements of flareups In radio
wave ionospheric absorption made at, .Zimenki-netar Gorky % - 56 091, 4 - 50021t)
during global geomagnetic stotms on July 15, 1,959, April 1, 1960, and October 28,
1961. The first two storms were registered at: 25 and 18.6 Mc. and the last one
was tracked at 9,13, and 25 Hcby means of cyaphase multi-Aipole antenna systems.
The following findings were made.' 1) Anomalovs absorption& appeariid. in the form of
consecutive absorption bursto lasting from several minutes to several dozen minutes&
Card 113

L 17113-66
ACCE15FLON NR,. AP5020999
.2) ~1hiy appeared.'regularly at the e d
n of the first phase of the magnetic storm
and continued to appear while the storm developed. 3) In the case of the last
two storms, some correlation apparently oxists between the geomagnetic field
variations and the absorption occurrencest. 4) During the same two storms, short
(5 min) fadeouts of cosmic radiation wete observed over periods of several hours
prior to the appearance of.anamalous absorptions.-These fadeouts were not accom-
panied by solar chromospheric flares. 5Y The'ratio-,of absorption-intensitiOs..at
two frequencies.was smaller than.the inve~rse of the ratio of the equ&res,of the
respective frequenc ea. Q.-Humdrous
bursts of solar,_'~radiation. at 18 6'and-,15.-Ne-~-
e'
were-. registered on .-July: 25,, d ih,
tude of the anomalous llr'm _,te"b"i :absarptlbn~ A
q _ Foo 'over -the, hor zon. did
not- exceed~04 ith--"
--i'ib 6.31 iehili-_Ai-zen sorp4on*at the -same: f requency.- eached
2-~_-Ub*':~8) Changes in7thelt_,S_M~ cosai Ici*:ridio wave -intensity, observed: by-; IZMXPM -
at - Krasnaya Pakfira on July~ 7 15, - i9~~ -,led tht, absorption burs ts-ai ~ Ziziewki. -b 8-42
minutes. :-SO At. the. vertical" -#rbbink'~ stat on the reflected sipal was,
during the 'abi6rmai. A sorption.', - Analysis of fonosphatictonow- "L
b
-..i h -th I' -4ou'-L, 42
a owe'~' xatidd-:Occutg*-,--iit'-"tlt'*'to WO
and absorption re ak-shons ow,
a vroximataly~~
to
dii~
Tht._,authoris Cims'-':~Md--~ji _tiii~_Pdiiii4liitWd f Uk~fteedd 0
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L'Oftizitic&.. 4~ihoti
Cad 2/3
-T -F

"i _7 7
'ASSOCIM%jo. ...Yvqwbb~-fsi4
sumanot

L 6522 mm(d)/3wT('1)AS(y)-VFSS4 IT/AST/GW
ACCESSIONMv AP"=55
AVrAMi GoWntsev. Q, muftnwr.-J. AS arkov,.-V. Lty,
I If, unerepovi TY Ir 5
TITIEs The romdto ol'an experimient on_ZI& comminicAtioa via Nlcho 20\Ld the
moon at a frequency of 262.4 wkscyclas betwon the observatories -oF-Jodr*U Nuft.
and Zimanki
SOURCIt lowdebeeklys 159196 malps To 3# so. 4t 190t 616-W
!X
TOPIC TAGSt moon, qata=~ 2gMWaMtj%q6d1c, teltacape, radio
satellite tracking, scientific research ooorclination / io&-*U Bank rszziv-~
scope# XimmuM observatory radio telescope, EESM 2 electronic computer
ABSTRACTs Dm-14 Irebrum7-Harch 1964 the AomduW of Sciences of the Ww, MA
of the Mg,aud the asommi ftet office Deputmt or armat Britain aau&=tW m
expazliment to establish one-W radio oommloation at 162.4 mapayal" w1m the
passive satellite ftobo46 and the now. Xoftm-Q um wed for 34 eammioatim
;wd .........

L 65295-65
ACCESSION URt AP5021255
tests of 1045 mimtes (the time i4erval. pmdtted by Echols orbit), and the
moon was used for 15 toot rum betuee" the Ecto tests. The transmitting equip-
ment at Jodrell Bank and the receiving unit of' the Zimenki Obaervatory are de-
scribed in detail. Echo orbit inrormation fuTnished by HASA, visual observations,
and radio tracking date from fixed stations vere fed to a BES11-2 electronic cal-
Pulator uhich provided proMmmed tracking control. The received signal exhibited
strong fluctuations separable into Wo periods: 1) a 2-2 minute fluctuation as-
sociated with Echo-2 distortion from a sphere and vith tracking errors; 2) a 3-10
second period associated vith amen surface irregularities. The rapid fluctua-
tions varied with each test. Voice Bignials, slaved by a factor of 9, vere bu-ely
intelligible. Telegraph, tAlstyps, and photofacsimile transmission, in general,
were unsatisfactory, but in periods of high signal-to-wiso ratios Irtelligiblo
messages were received. The won transmissions were not as olear but did furnish
scientific information. Unexpected transmission losses Included 3-5 db for polar-
ization losses and 2-2 db for unknm causes. The International cooperation was
excel.lent, with the Soviet submitting a complete report. .Pffera fw furtber co-
operation have been extended. OrIg. art. bass 3 tables, TfIgures, said 4, for-
mulas.
ASSOCIATIONs none
SUMUMD1 18A UCLI 00 SUB OOM i . AA, NG
ND RV BOT1 Oct!

KMGKOVA, N.A.
Review of the OBulletin do psych6loglem; published by a psychology
research group of Paris University. Zhur.nevr. t palkh. 57 no.l:
138-145 157. (MLHA 10:3)
(FUNC11--ftYCHOLMY-MIG)ICALS)

DML'SKATA, Inns, Naumovna- RT)Tlf)BZDRA,#.~Imm-Alekg&rArovna,- BABATA11, N.A.;
red.; KUUIN, K.T., tekhn.red.
[Disability evaluation and employment of schizophrenics] Vrachebno-
trudovala ekspertiza, I trudoustiroistvo bolli7kh shisofrenial.
Moakva. Goa. isd-vo mod. lit-ry, 1958. 70 P. (MIRA 12:1)
(SCHIZOPfflWNIA) (DISABILITY 31TALUkTION)
(MENTALLY RMICAPPKD--IIqPWY14SNT)

MEIZMWr D,Xe,j iKOROBKOVAp S.A.
Glinicalxtudy of mental patients during work activity as a method
of funati6nal diagnosis. Trudy Goso nauch.-isal. psikhobw, imt,
no.20ii3l-138 159. (MIRA 14:1)
le Institut poiWii-stril MWstejZtws-zdravookhrazwniya RSM
(direktor - prof. VA kwlioUrov)i TSentral'W institut ekspertisy
Andosposobn6isti i organiza~tvii truda Invalidov (direktor - prof.
0.1* Sokollnik*~). (KKNTLL ILLNESS) (WORK)

KLMOBKOVA* R.A*
On D. Wechsler's Me&ourement and ap -4sal of adult intelligence.0
Zhur. nerv. i psikh. 61 no. 1:110-: .161. (MIRA 14:4)
1 (INTELLECT)
(MUMUM9 V.)

NOGANS V.M. (Mc)sklm); KOROBKOVAp E.A. (roskva)
Pathopsychological studies in' Its active therapy of
psychoses. Zhur.,nevr. i psikh., 64 no.3%464-467 164.
(WRA 17:5)

EXCERPTA KEDICA See 4 Vol 1215 Med'. Micro. May 59
1302. CONCERNING THE METHODS OF INCREASING THE IMMUNOGENIC
PROPERTIES OF VARIOUS STRAINS OF PLAGUE VACCINE AND THEIR
STABILIZATION (Russian text) - KorobkovA-E--L __ZH. MIKROBIOL.
1957,7 (64-68) Tables I -------
By passage of the vaccine strain through guinea-pig:s the absence of any increase
of virulence was conf Irmed. On the other hand, In f reeze-dried Infected organs the
organisms maintained their immunogenic properties for years, particularly In the
spleen.
KauLen - Moscow
EXCERPTA MEDICA See 4 Vol 12/7 Med. Micro. July 59
2057. THE EFFECT OF GLYCOCOLL ON P. PESTIS, 111. ON THE ORIGIN OF
PLAGUE TOXIN AND ITS SIGNIFICANCE IN ACTIVE IMMUNIZATION
(Russian text) - Korobkova E. 1. - ZH. M11GIOB. EPID. I IMMUNOBIOL.
1957, 11 (143-148) Tamew-5--
P. pestis grown on Hottinger's agar with added glycocoll produces a factor highly
toxic for white mice and rabbits, P. pestis grown on ordinary agar plate Ireated
with glycocoll solution undergoes lysis and toxic products are liberated. Serum of
horses immunized with a live culture contained antitoxins to both toxins. Serum of
rabbits immunized with a killed culture was able to neutralize the lysate-toxin but
no, the toxin produced during growth onglycocoll agar, (native toxln)~ Mice immuniz-
ed with sublethal doses of native toxin were able to withstand Infection with viru-
lent plague bacilli and the toxins. Anatoxin (formolized native toxin) was also able
to Impair Immunit to native toxin and to virulent bacilli. Mice are more suscept-
ible to the toxins tKan guinea-pigs. Live antiplague vaccine incorporating anatoxin
was found much more effective thin the usual vaccine and gave rise to both anti-
bacterial and antitoxic immunity. This opens the way for improvements of the live
accine.

KAXASHOV, Alekisay Ivanovich; qM4TIYZT, Goorgiyyeaorovich; KOROB.K,OVA,,G.,
rea.; Himov, Y., tokt;n.red.
Ntsqnsk. Orel, Orlovskas W2hnim lad-vot 1959. 113 P-
(MIRA 13:5)
(Ntsopsk)

9 0 Ih.Ye.; I[ORC9KOVAg.,.. rod.-, IMMOV, V., takhn.red.
(The present and the past of the Ofokmash" PlantOl
Nostoiashchoo i pronfiloo savodis "Tokmah." Orel, Orlov-
skoe knishnoe izd-vo, 1?59. 136 p. (MIRA 13:2)
(Orel Province-Nachinery industry)

Akademlys. neuk SSSR. Mazhduvcdozetvennyy kazitet Po Provedenlyu
Mezhdunarodnogo goofirlehaskogo gods. III razdal proera=y 1Ws
Ze=oy UnvatIzn I zemuy~b toki.
rorotkoperlodlChaskly" kolebanlys e2sktronagnitnogo polya scull
(ahort-Porlod Oncillations of the 33--th's Electroctapetio
Field) Moscow, Izd-vo AN SSSR, 1961. X14 p. 1,800 eoplez.
printed (Series: Its- 3bornik statcy, no. 3)
Reap. Eda..- A. 0. FAI&ahnlkov. Doctor of Phys to and Rathematicap
and V. A. Troltakayn, CandLdate of Faysicaland Mathomation;
Zd. a to. P. Shchuk-Ina; Toeb. Ed. s Yo. V. Xnkunl.
rURPQS3: ThAs publication In Intended for geophysicists.
MERWRI Title collection of articles, Vubllzbed t7 the Inter-
departmental IGY Co=mlttee or the USSR Xtedemy of Sciences,
treats problems Or goozaaenctism and telluric currents. In-
divIdual articles deal with various (ftort-"r1od. s1sxctic,
ateedy# etc.) oscillation* or the terrestrial electro-mignetle
fields PILrtlcul&rlY In the arctic reS:L4=. NO personalities
are mentioned. Brief J~n&Unh abstrac-.g azc=;Ianj ~c=h article.
References follow individual articles.
TAWX OF CCUTENTSs
Ainnas V 1. Sbort-Porlod Oscillations of the zarth's
1904;m
91b led T V. Some Regularities of the Disturbed Field or
21
M. V., ft. B. Rastrusin. ZA_I~_~okltygcjsUjy.
a.&W. Sl!ghS I Lon. the nwififlia-or-
iiM
Fe!io-d As. llaftoon. in xiddie xAtitudes, 27
Short Period 03cIllationo of the Cie
MOO
Zen cordin; to Observations 3= Irkutsk) 23
22br.ov: RApid Gooolectric and Goomametic -WrIatio _na
a_,M_ 4r, V. 5.
an Lr Heguluxltlez (According to Observatlons 1- A-hkhabal) 35
Traltskayo, V* A* U680 05cillotIona mod Main 000121ation,
In the Arctic and Antartlo 41
P. Preliminary Results of rArth Current Obser-
vilaono In 4dal. Bay 62
Ulkitins X M Preliminary Results or Zarth. Current Obser-
-i&-U.2~n% ~at t '~~-.tvbuz-g Statl.. (Splzsbergen)
Z"va R , P , 0 1 Frobkva, jL_M_FW1Li.a, and V. A.
I. the avia-Ircti. Luring
the 1935-1956 Period 76
Barnukov, 0. M., and K. Tu. Zybin. Wouperpendicularity of the
-Nectors-IT-WE-Z and 0 Variations or the Larth's Rlectromag~
antic Pleld
Troltaksys, V. A., and M. T. Kellnikova- Characteristic
Intervals Of 06cillatic;irs;-D-Oii~Figiiig--O*er a Period (30.1
060), in the 1&rth-s ElectrmagnatIc. P%*ld, and Their ftelatlon-
ablp With Phonoc:sna in the Vppr Atwgpb*r.
bol-shakova 0 V X Yu. 2~rbln, and N 7 MAI %qeva. Some 1`0
Mogul -&-r1t.NAA a ieJ;Avlor of the " ta-jj~d' ' -
in% V*rU&JL caPonent or
Short-Parlod 06cl1latlons or the 000=12SMOtIc Field In & Stab
Rssl-- ( PC le 108
FUSE x B= IZ rTATI(X1 507/5215

37315
S/169/62/000/004/101/103
D290/D302
AUTHORS: Korobkovat G.I., and 011, A.I.
TITLE: Measizements of the Q-index of geomagnetic activity
in the Soviet Arctic observatories
PERIODICAL: Referativnyy zhurnal. Geofizika, no. 4, 1962P 41, ab-
stract 4G238 (V sb. Probl. Arktiki i Antarktiki, Vyp.
9p L., Morskq transportp 1961, 89-92)
TEXT: A statistical study was made of the Q-indices of magnetic
activity at the stations on Dickson island, at cape Chelyuskin, at
Tilzsi bay, and at Uelen during 1958. The authors calculated the
mean-annual diurnal variation, the mean-hourly value (~), the maxi-
mum during each hourly interval (Q )p and the number of hourly
max
intervals during which Q:p-5 (N The diurnal varlations of Q#
Qmax , and XQ agree well among themselves and also x7ith the diurnal
variation of r.. It is shown that the diurnal sum of the Q-indices
(Z Q) ' losely correlated with the sum of tbeplanetary K-indices
Card ~1//l

Alleasuremente of the Q-index of ...
S/169/62/000/004/101/103
D290/D302
(Z Kp); the*correlation.is linear only for low activities (Z K p<
----30). The correlation between the Q-indices andrIj was studied; it
V~
is shown that it is possible to convert values of Q into equivalent
values of rH. [Abstractor's note: Complete translation
Card 2/2
B/561/61/000/009/003/003
D207/D308
AUTHORS: IKorobkovai G.I., and Ollp A-L t'o'the
TITLE.' Q-indices of geomagnetic aotivity according
data from Soviet Arctic observatories
SOURCE: Problemy arktiki i antarktikip no. 9F 1961., 89 92
TEXT: An analysis of the records obtained in 1958 at the Dikson
Island, Ghelyuskin Cape,. Tiksi Bayt and Uelen stations showed that:
1) There is a close correlation between, the hourly values of the
horizontal component of the earth's maIgnetic field r H and the hour-
ly values of Q-indices,. 2).there is little difference between the
hourly Q-values calculated by (a) averaging measurements taken at
15 min. intervals (&), (b) selecting the highest of the Q values
(Q ) in a given hour for every day, or (c) taking the number of
max
Q-indices greater than 5 in a given hour and averaging this number
for a mbnth or a year. The calculation methods (b) and (c) are re-
commended because of their greater convenience. Por stations based
on drifting ice, where Q-indices are difficult to measurev it is
Card-

. KO-RO--BKO-VA, G.I.; OLI, A.I.
I Q-indices of gpolyLgaetic activity according to the data of Soviet
Arabic obsezv * Probl. Arkt. i Antarkt. no.9:89-92 161.
(MMA 15:1)
(Arctic regions-4ULpetismy Terrestrial)

KOROBKOVk, G.I.
Relation of polar magnetic disturbe.nres to the main phase of
magnetic storms. Probl. krkt. i Anllaxkt. no.18:78-86 164.
(MIRA 18:3)

2
S1 16 976'1%00/00 8~0 48/0 53
A006/A101
Nikitina, N.M., Troitakaya, V.A.
AUTHORS: Zubareva E.P1, KoE2bkova,_Q.I
Giant pulsations in Soviet Arctic during 1935 - 1956
PERIODICAL: Referativnyy zhurnal. Oeofizika, no. 8, 1961, 39, abattraot 80262
V-sb.,"Korotkoperiod. kolobanlya alektromagnitn. polya Zemli, no.
~", Moscow, AN SSSR, 1961, 76- 82, English summary)
TEXT: The study of giant pulsations-was 5arried out on the basic of stand-
ard recordings of the magnetic field with 20 nm%/h scanning from data of the fol-
lowing 6 obiervatories.- Dixon, Wellen, Matoohkin Shar, Tiksi, Chelyuskin and
Tikhaya Bay. The greatest number of-giant pulsations was recorded art the Wellen
and Dixon stations. Usually, giant pulsations were observed with T of about 60
and 90 seconds.' For a number of stations T was also about 45,.75 and 135 see,
It is possible that for giant pulsations there are one or two basic perioda,-
whose different harmonies appear differently depending on the local conditions
of the given station. The amplitudes of giant pulsations vary within the limits*
from a few 2`to several tons of T - At Dixon and Wellen giant pulsations arise
mainly during the first half of the day. On Dixon the number of giant pulsations
Card 1/2

29727
S/169/61/000/008/040/053
Giant pulsations.ln Soviet Arctic during 1935-1!)56 Aoo6/Alol
Inoreases-towards the equinox, for the Wellen station seasonal changes are less
marked. -Stmultaneous-giant pulsations on a nudDer of stations are rather seldom,
but some giant pulsationfir were ricorded at the 13ame time at Dixon and Wellen.
Sometimes giant pulsations are exoited'during the day at different but close-
hoursj in the mAjority of such cases they.arisfD first at the stations located
more to -the -easte It is concluded -that giant pulaationa are diaturbancea of the
terrestrial elect-romagnetic field and are typical of polar aurora, zonea. They
damp rapidly Io the north and south of i5ie aurora.
K. Zybin
[Abstraote"ris notei Complete translation]
Card 2/2
Card 112
MSSR/Pharmno,ology. Toxicology. Cholinergic Dr"gs V
Abs Jbur. Ref Zhur-Biol. , No 8, 1958, .4-7546
Abstract atropine. No improvement was noted in 13 of the
patients. Slide effects (dryni?sa in tlie wotith,ro-
duced vision- and others) viere more aDoarent
when I was taken internally. Greater tolerance
by the patients for 1 as compared with atropine
was noted.
Card 2/2

VA L.
Phatometric. method of deterMining peni;&bramacetuneo Izv. AN Turk. SSR.
Sar. fiz.-tekh., khim. I geolb nauk ni).1%54-60 165. (MIRA 180)
1. Instit"t khtmi-i AN Turkzonakoy Ss'R.

SOV/126-7-6-22/24
AUTHORS: Vlasov, V.V. and I.Kaor~b~koy ~**X~
TITLE: Investigations Relatifig'to the Defectoscopy of Railroad
Rails*in Moving Magnetic Fields. 16. Study of the
Possibility of Detecting Defects from Their Reaction on
the Primary Field
PERIODICAL: Fizika metallov i metallovedeniye, 1959, Vol 7, Nr 6,
pp 937-939 (USSR)
ABSTRACT: This is one of a long series of articles on the subject of
detection of rail failures by means of magnetic fields
moving at speeds which are acceptable in normal railroad
operation.
At present the wagon which carries the defectoscopy
apparatus is pulled by means of a separate locomotive.
However, it would be useful to be able to attach the
defectoscopy wagon to any train. This would be possible
only if the test apparatus were not less than 100 mm.
above the rails, which requires increasing the air gap
between the electromagnet and the rail from 10-30 mm to
100 mm and to lift to the same level the search equipment.
Card 1/3 This obviously leads to a considerable drop in the
sensitivity of the defectoscope. The authors considered

SOV/126-7-6-22/24
Investigations Relating to the Defectoscopy of Railroad Rails in
Moving Magnetic Fields. 16. Study of the Possibility of
Detectirg Defects from Their Reaction on the Primary Field
it of interest to study the possibility of detecting
defects from their reaction on the primary field and
particularly from the disturbance of the magnetic flux
in the core of the magnetizing electromagnet. Therefore,
they studied the possibility-of detecting an artificial
defect ofthe type of a transverse crack in the railhead
for various vertical distances from the rail to the
electromagnet, which is used for generating the magnetic
field above the rail, the setarch coil being located
directly on the core of the electromagnet. The
investigations were carried out by using a model, dealt
with in earlier parts of this series of articles,
Refs 2 and 3. A diagrammatic saketch of the model is shown
in Fig 1. For magnetizing the rail model, an
electromagnet was used with a core made of 0.35 tum thick
transformer sheet (30 mm wide, with a packet width of
20 mm). The experiments reirealed that, at least
Card 2/3 extensively developed defects, can be detected in rails

SOV/126-7-6-22/24
Investigations Relating to the Defectoiscopy of R~ilroad Rails in
Moving Magnetic Fields. 16. Study of the Possibility of Detecting
Defects from, Their Reaction on the Primary Field
by means of an electromagnet located 100 mm above the
rail and that the defects can be detected more easily by
means of a coil located on the second (trailing) pole in
the direction of movement than on the first pole (pole S
of Fig 1). The authors recoirinend iniat for solving the
problem the carried out laboratory experiments should be
supplemented by experiments on normal tracks.
There are 3 figures and 3 Soviet references.
ASSOCIATION: Institut fiziki metallov AN SSSR
(Institute of Metal Physics, Ac.Sc. USSR)
SUBMITTED: April 7, 1958
Card 3/3

KOROBKOITA., L. 11.
24043 KOROBKOVA. L. IN. LimPaticliesaye sosudy matuld u kosHd. Trut, Leenlngr.
San.-Gigien..Eled. El-TA, T. 111, 1949, 3. 178-93. - Bib2ilo,gr: 8 Niazv.
SO: Latopis, 110, 32, 19149.

28907
8/170/61/004/011/007/020
B104/B112
AUTHOR:
TITLE: Heat-production rate on the boundaries of vibrational flame
propagation
PERIODICAL: Znzhenerno-fizicheakiy zhurnal, V. 4, no. 11, 1961, 64-67
TEXT: In a previous paper, S. A. Arbukov (Tretlye Vqesoyuznoye soveshchw*
po teorii goreniya, .1, 44, M., 1960) made the assumption that the heat-
production rate Q on the concentration bcundaries of the vibration
excitation ranges of a flame is constant for every fuel. In the p;esent
paper, the author gives an experimental proof of this assumption by
examining the boundaries of vibrational flame propagation of mixtures of
air and carbon monoxide and of oxygen with propane and crude-oil gases.
Measurements were made with an improved tube method (G. A. Barskiy, Ya. B.
Zelldovich, ZhFKh, 2A, 5, 589, 1960) at room temperature and atmospheric
pressure. The assumption q - const is proved by computing' the chemical
reaction rate T, using the theory of flame propagation of Ya. 3.
Zeltdovich and D. A. Frank-Kamenetakiy and measuring the normal component
Card 1 /r or
19-

28907
5/17 61/004/011/007/020
Heat-production rate on the ... B104YEI12
u ~ the flame-propagation velocity. It is shown that Q can be
eut0i'mated from the measured values of uH# Results are given in Tables 1-7-
was calculated from n m
k. rr2 exp(- 3 where r and r are fuel and
T1 RT 1 2
oxygen concentrations. The author thanks 0. A. Tsukhanova (ENIN) for
discussions. There are 7 tables and 7 Soviet references.
I
ASSOCIATION: Aviatsionnyy institutp g. Kazanl (Aviation Inatitutel Kazan')
SU13MITTED: March 1, 1961
Tables 1-3. Mixtures of carbon monoxide with carbon dioxide, oxygen, and
nitrogen.
Legend: (1) N2 impurity; (2) N2 impurity + X2 air*
Card 2/1r

KOROBKOVAq M.P.
Rate of heat liberation on the boundaries of the vibrational propa'-
gation of a flame, Inzh,-fiz,zhur- 4 no.11:64-67 N 161. .
(MIRA 14:10)
1. Aviatsionnyy inatitut, go Kazan's
(Heat of combustion)

ACCESSION NR: ARWA417. 0/044/64/000/ool/BM/BM
SOURCE: RZh. Makhanika, Abe. ID613
AUTHOR: Kordbkova., M. P.
TITLE: Study of the limits.of the vibrational oxtent of the fleme
t
CITED SOURCE: Tr -1-y Voss. nauchno-tekhn- konferentaii.po probl.;.vibratsion. i
pulleatsion. goreniya. M.p.1962,46-51
TOPIC TAGS: coinbuotionj, vibrational combustion
'fWSIATION: The vibrational propagation of the flame during the combustion of
CO-airp propane -oxygen,, and methane-oxygen mixbiree with inert components hu been
studied within horizontal glaas tubes 2-3 and 4.8 ca in diameter. The onset of
oscillations-was determined by car and by the way the flow unfolds. The limits
within .which vibrational combustion occurs depead on the concentration of the com--'
bustive mixture and on the length and diameter of the tube. The results are pre-
sented in a table and 6 graphs. The interpretation of thet experimental results
.(Vibratsionnoye goreniye.. M., Pizmateiz,
follows the theory by B. V. Rauehenbakh
1961). There are 8 references. Yu. S. FWazantsev.
DATE ACQ: 18reb64 MM COM FL ZKCL:- 00
Card 1/1