SCIENTIFIC ABSTRACT MANDELSHTAM, S.L. - MANDELSHTAM, S.L.
Document Type:
Collection:
Document Number (FOIA) /ESDN (CREST):
CIA-RDP86-00513R001032110020-1
Release Decision:
RIF
Original Classification:
S
Document Page Count:
100
Document Creation Date:
November 2, 2016
Document Release Date:
March 13, 2001
Sequence Number:
20
Case Number:
Publication Date:
December 31, 1967
Content Type:
SCIENTIFIC ABSTRACT
File:
Attachment | Size |
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CIA-RDP86-00513R001032110020-1.pdf | 5.34 MB |
Body:
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IAM&WU"id (WOra Lak). 19M* Sv (S), tn. n LI.11.1 ;11 IN.
methed described dependa on a visual of the hit-
AJ 5697 A.. Zn 4811 A.. and Mn 4824 A.. with neighbouring li&% of inrials
arbit-harv taltertassuandard. cit. JfgS7114A.. Fe4W)A. I'lwaccumy
obtained in 6-8%,. 12) A new method is guggreed inv(4ving ril
interptvtotion. whkb w (az has been cant only in a4ropfi"im PrIh:I"LnIVh"Kl
consists in a sop-wim reduction of the inlenRity of each v@evtw lint, and thr
Lomparison oil their intensities with simi6rkv nAum-4 Jim% ofAmorsts tAken
us standards. A suitable reducIng plate is prepared consisfing of & IUArI4
platc coatt-cl with a photographic cmulsion film, which luts 6"-n rrutov" frx-na
atootographic t"te after dvvvt:,ping ot@ it a photograph ofthe spark s1wrtrum
u Mektron. Pbot%raphsare kenusingda .levent exposures and the plAte is
moved each time by aa amount equal to the width of the alit of tht- s1wetru-
am W A reducing plate with 10 steps is thus obtaintJ and valibralcil ush)g
malli4eiso(ditlervat vactals with kstown intensity ratioa. By Coo . tj
W-ftsit" of Uwe of the element to be atintatw with the luterwily Tanciod,
Pletnent, the value of 4 1 The any given line an bc int"V.Lated. Using L
tog I curve obtained with &Hoy& conWiting a known protortion of the metal.
the nwtal in the unknown alloy can be determined with an &-@y of 9 to%.
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Iflulliplier and an ovdUadraph the ripple appeanne In
Ihe light -introolt y mcillogrant In each cycle of a dincham.
, It
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k
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USEWPhysics
Spectral Lima
Spectrum Analysis
Jul 47
"Factors Affecting the Intensity of Spectral Lines in i'lames during Spectrum Analysia,"
11. G. Aleksoyeva, S. L. Mwdelldhham, Physics Laboratory imeni P. M. Lebedev, Academy
of Sciences of the USSRp 16 pp
"Zhur Takh Fixn Vol XVII, No 7
Discusses work conducted to investigate larious tin compounds, the effect on the
intensity of the lines separated in volatile compoundsp the conditions for disassociation
of salts which are introduced and the formation of new mobecules in the flames, and
approxi'at6-?Z"@culations for the degree of disassociation for various comp=4j, -
The author attempts to explain the intensity of the spectral lines on the basis of the
data obtained ftom the experiments.
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fimt. V, G. AirkwIrviiiatuf .4 L. XLukIvW-jttav,. I
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f1k. 7b9-&J(I04-,?,m
F- - rhetwd. Phys. W S.S 0 1
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-I t1w, 1-14M. mt,132021 A. lim, -
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fIW CK$tcr ..Iw, whrrv 'd lite M. 16001. Li f"Al",
K 4t44. aml '11WO A - lit- at the viine tell,,,.
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o (Sa IAk)", Li =70% K 2110% Tj 2.C)'). in dc,"ermulcut
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As& ILA bI?AtkUAk(KAL LITIRAITtAll CLWIVICATION
44 AV Ali;
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n ICA V
ABRAMSON, I.S.; GIGICHKORI. U.N.; DRABKINA, S.I.; K&HMISHTAK. S.L.
Canal of the spark discharge. Mmr.sksp.i toor.fiz. 17 ne.10:862-867 147.
(MLRA 6.7)
1. Fizicheskiy institut im. P.N.Lebedeva Akadsmii Sauk SM.
(Electric spark)
Utchaalam of electiUm erosion of a mow. I
Mandcl'shLun a,@d S. M. R4Likil kAcad. lws. C .1; N It
riri4s, AW-- vask S.S.S.N., Str. Fis 13, "49 i4
11949).- Froshm of vircti-les, -peeWly ist @ -fulvmw4
SPAfk di%CbAf&C. 1@ CUILlidcMi to IW a @-ldarV J-n-
and attributed t,j the tucch. artion of ructal vApm jr"
torches") for-tted by the dixharge or Itigh C.n, mostly
the cathode and er-mling the anodr. Allawc.d.the
;;;" it revered. Tests were tuade with a spark div-
charge between steel rull" beariviv in air. The spark
meW was in&pendcr.. of the sixe of the gap. At im.11
Maps the esuslost was high Quid the anode w,is more ertmird;
at biggerr Cups the enuton was less and streng" ott the
catbG&. A conical cathode with a shirp point euu*,@l a
higher destruction of the anode than a round cathode
Electrodes of Ve. Al. Mg, Cu were inv",ogstrd; Cu
caused the high"t destruction on the 0 le,PW I
r tore let,
A quattz plate introduced to as to shlefrtl@l 1"
without disturbing the discharge prevents erosion ctim@
pletely. To prewnt the spreatling of the "torches" one
or both clectroles were enclosed in cilpillades and the jets
directed on a 'ted plate cauting high erosion. In thew,
conditions at lugh c.d .the jets were unstable but becAme
stable upon introduetion o( a self-induction coil. Stable
)ct-- do not cause cruskm. acritical "lilt. speed of at least 2
krim./sec. bein&: required. Immersion in a liquid incye,w,
erosion protiobty because of a channeling of the -torchts
S. Pak-r
to steel$ -3-
f=TU O'll Mko"vT7 Its sq@t I t
Nfeth(A I.
A 4.&m1cr*fafv4 condenser. charged to 16 kv. through a
kenoum. d1wharges thmo a 4 min. regulating gap which
an atm. Q(2&-aOcc.o(C(h. Averit oflOd6dtargesis
used per analysk; the sample 6 moved between discharges
because of local impoverishawat of thie steel in Ali. Methful
I I: Samples am kept In 35 cc. of CCN aW excited by an
wdinded low-voltsce Intermittent am with a 110 mkro-
farad power condenser charged to = v. Both the series
regulating gap and the analytical gap are 0.35 mm. wide.
Exposures am short (- 0.5 we.) In order to avnkl UWW IM-
poverMment In N. The Intensity ratio of N 11 3%5.0 to
the adJacent backgmad Is plotted a 4 function of N con-
tent (ddd. chemically). The limit of detection Is -0.(W%
N by both methods- av, deviations for ON
8
ranged fmm 6 to 20k of the amt. presentocts C. Feldman
Ifiroadenfas of tPectral lines under the calm at 1wa and
datmo, 9@ L. MAMIel'slistaill and N N &AMAV (11 %
lAx-dev My%. losr, - Ar-of SH V S S R , lifirst-cm I
Asir. Fllipd. Perri. Fil. 20, 323-fl(IJIM-10 C(iff-11A All.
drilvvil fut the Allplic-Abdity Of 10116jOKI Mid 14 -tAtkti.-.11
4VII!Jkleralk-115 CofliniM CtM",lcr3jsotJ% jfr Apillsedble if
the little of the colli-skism r is much %litnict IhAli lite 111C.111
little C elApsing between cullisioJL3. With r - p.r. %Ixrfv
J, - failius of the effective cross sccl ion for the kollision, r
relative @Clocitr of the collitlitis plitticlei. 41111 0 -
vp'rN. whm A - no. of electrons or lons, cc . lite vrit,rum
licaniscs rOP"V At I. File spectral line% with linvar StArk
effccf, 0 - an/r. where a - Stark cortm fur the given line.
And for lincs with q"frutic effect. J, - (rO, ' r)",, hrittv
the critrrl@s R. - rla'.Virl < I and R,' - r'jN :.r -C 1,
corresponding criteru fur the Applicability of
UUk*1 %146*61-Al C0111MICfAUM) Are. tell' R.' -
V >. I And N" - ON, r @1' I @ '111C rou'l. Ali'l if
Arr rclaird to the wfills. A miff /I (it lite filli-Al jild she
quAdratic Stark effects (Ah - Ah' and Ah - PEI, re,l. .
where E - clec. field strength) by a - 2.7 X 101 A A' And
d - 0.38 BlAs. In an clec. arc At 5M)"K., for quadratic
litics, the criteria are. fur broadening by cIrctrosi ctilli%icJit.
R'. - 3 x 104 0 -C I anti ft.' - 7 X 10' 1 :1, 1. 4 ild for
Intudenina by ims coll6kni. R.' - I X til"it -jb- I Anti
R.' - 2 X 10*0 > 1. Cousparisort will% vxpti. dju fiw
lines with quAdratk Stark c1lect shows the applicability ut
the collision criteria R.'. Essm. of Ilse abi. birmuteninst
shows that P-r lines with p - I X 11) 11 - I X 11) - it i,
thic litAbily to Collis"Is With r1crtitm. For 1111r, lih
low" 0. lite Itile tit Start; Nodairlsois williar. firalitible.
IsheIVAI 1111 lilies 141111 Wilber 0. 11.11W.Ii-Al lillmdriMlig MAY
become istnificint. In tire east: of IlAe@ -till lus-r StAtk
cffcct, "Illision sold Ptatistical bruatfelling plAy role% to
" Thon
Approx. lite sarise extent. N
OM
USSR/Ani*m Sol" Itadiat ton, Felp, 52
=.ve,T@@ Works @on ~the".IUV*Stigiktion,~Lof.~.'SlioLr~twave
tliravibiet Radiation of the Sun" S. L.
@"6#9pekh riz nue V03. xLVI, .10 2, PP 145-1.7,SL
results of investigation* oarrie&,O@t
ii. 4*4iii years on the study of almorwave ultra'-
@V# 'at radiation of the Sun vith the aid of,@Vr2
rdem,ts. Those reaitlts are IncompUtp And
q. I I t, I I don
xypi,*Ix,*,,,,,@. -and"ametims ft*Vo
x are givem
@:21OT3
Udiatim, I Ma Ile
(Contd)
S. SWovskiy, 111z la-ymkoy Actron Obser 4,
1949i -.1. R. Metal I and A. B. Severnyy, '"D.ok
Aklauk SSSRII 80, 867, 1951; translation iutO
RussiI&A, 1-11 of M. Uldwyer's I'Rei@lts and Problum
@.ae.,iOAw Inventigat ion" -(Foreign Lit PrefiB) XP840ws
1%0). Acknowledges co=sel of A. B. Severn",Wd
1. S. @SbkjoVskjy.
20IT3
E-4
J-
777
42 4.
RM11 @ox
'
41
to rint4f6l wvid-ttmp-4:'-'-
man
tf"@k lon;z4t-' lide
tht-
-
'
-
'
d:
iWi
f
d
f:
'5!;J
71 N
jqq:
c7-
bu
nr
Q
Allimith vW-dramil, warc clmdu-ted with.smar @,7113.
-----------
air,
76 -taindd-.- i re I Aoift,
.4pectra lin ts
@pa dia on.-moo Vera,
1, '- H I fl N \) '.-') 11.
KIBISOV. G.I., kandidat khimicheskikh nauk; STMN, Kh.T@.. kandidat
fizikomatematicheskikh nauk; YMMM-KOBETSKATA, T.O., saadahiy
nauchrU7 sotrudnik; MANDFLISHTAM, S.L., doktor fiziko-matena-
tichaskikh nauk, redlOW redaktor; SOKOWVA.
T.F., tekhnicheskiy redaktor.
[Spectrum analysis; annotated list of Soviet works on spectrum
analysis, 1931-19501 Spektrallnyi anal1z; annotirovannyi
ukazatell sovetakikh rabot po spektral'nomu analizy, 1931--1950.
14oskva, 1955. 181 p. (MLRA 8:12)
1. Akadsmiya nau SSSR. Komissiya po spektroskopii.
(Bibliography-Spectrum analysis)
K&Un'SHTAH,3.L.; SMODREV,N.K.
Applicability of Kirchoff law to the emission of gaseous dis-
charge plarama. Izv. AR SSSR Ser. fIz. 19 no.1:11-14 ja-F 155.
(KWA 8: 9)
1. Fisicheskiv institut imeni P.N.Lebedeva Akademil nauk SSSR
(Spectrum analysis) (Soectrometer)
HAORL I SHTAH 4, L, - T MO, 1. P.
I
Additional data onthe photoelectric investigation of spark
channell spectra. Izv. AN SSSR. Ser. fiz. 19 no.1:60-61 Ja-
F '55. MRA 8:9)
1. Fizicheskiy institut ineal P.N.Lebedeva, Alrademit nauk SSSR
(Spectrum analysis) (Spectrometer)
WAR
MA@U-,LSHTAY--, S. --5
"Spec trum -Ex- i tat ion in Spark a pa-,er 'it --@
- r@
111ternational Spectroscopica! Armterlam, 14-1` May
Academy of Sciences of the UF35R, Moscow.
Trans lat ion -D 13 , I "'
a
Ic, cc - )v
le:
MDELISHM, S., 14oscov.
"Gross Stability of Toroid. Discharges by Comparison with Vortez Theory)"
a paper Bubmitted ot the Third IntorattlJonul Conference on Ionizotion
Phen@meno in Gases, 11-15 Jun 57, vellice.
30:B-3,087,49F
MkOEL'SHTAM, S.L.; CHULADOVSKIT, V.M.
The Tentb All-Union Conference on Spectroscopy and its
Applications. Opt. I spektr. 2 no.l*.143 Ja 157. (MLRA 10:2)
(Lvov--Spectrum analysis--Congresses)
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AUTHOR. Mandel'shtam, S.L., Doctor of Physical-Mathematical 30-8-9/37
Sciences,
Striganov, A.R. , Doctor of Ph@sical-MathemAtical Sciences
TITLE: A SMosium on Spectrography at Chicago (Simpozium Po
speTliro@kopjj_@v__@hl_kag6)
FMIODICAL: Vestnik Akademii Nauk SSSR, 1957, Vol. 27, Nr 8, pp.6o-62 (USSR)
sium (29.April - 1 Xay). More than half of the reports was de-
voted to the variou problems concerning the practical applica-
tion of the emission spectral analysis; the corresponding de-
vices and exhibits were demonstrated. The works on the deter-
mination of P, S, C in steel were of special interest. In his
report N. Launami (' S@zedeft ') p4nted out the possibility
to determine P in steels by means of a quantometer. E. Lushera
(Switzerland) dealt with the prdblem of the immediate re-
gistering in the ultraviolet of the vacuum. Special interest
was caused by the reports on the application of the method of
trsn mission in spectroanalysis which was applied for the first
ABSTPJ_CT: The authors of this report attended the above mentioned sympo-
Card 1/2
AVAUAOLE:
A Symposium on Spectrography at Chicago
time in the LM 4nd Taganov) . ThE
paper reported on "The spectral analysis according tc
Evaporation Method" and "Graduation Graphics for the
an Isotope Spectral Analysis". It is remarkable that
spectral analysis the American collegues mainly apply
photoelectric method.
Library of Congress
30-"137
author of this
the
Gaze of
for
the
Cara 2/2
AUTHOR WMEVSHTAN, S.L., YEFREMOV, A.I. 53-lb-ii/i8
TITLE -Miie-stigati@na of the Short-Wave Ultraviolet Radiation of the Sun
(Issledovaniya korotkovolnovogo ulltravioletogo izluchenlya solntsa.
Russian)
FMIODICAL Uspekhi Fiz. Nauk, 1957, Vol 63, Ur lbi pp 163 - 160 (U.S.S.R.)
ABSTRACT The present paper gives a short report on recent results obtained by
experimental and theoretical work on the short-wave radiation of the
sun which were published since the first survey given of this topie
(S*L. MANDELSHTAM, Uspekhi Fiz. Nauk, Vol 46, p, 145 (1952)). The author
further "gesta that experiments be carried out by mearis of arttficial
earth satellites.
The radiation of the photosphere: The authors describe the paper by H.
CLEARMAN'IAstrophys. J. Vol 117, p 29 (1953) as the most important in
this fie" Above all the presence of various elements in the sun is
discussed, something is also said on molecular bonds. According to the
authors' opinion this paper by Clearman does not contain any essentially
new results. Other papers (among them theoretical ones) are then dis-
cussed.
The radiation of the chrmosphere was investigated by the spectral ana-
lyals of light by means of spectrographs. Photoelectric receivers with
Card 1/4 separation of a narrow spectral region were also used. By special systems
53-1b-11/18
Investigations of the Short-Wave Ultraviolet Radiation of the Sun
the optical axis of the spectrograph could be oriented to the sun, Ythile
the rocket covered the upper part of its orbit. In this manner the re-
corded spectrum could be farther advanced into the short-wave region.
Various papers on this problem are discussed.
The radiation of the corona was investigated in earlier as well as in
more recent works by means of photoelectric receivers, i.e. photon coun-
ters which separate narrow spectral regions by filters. The papers on
this problem are discussed in short,
The variations of radiation and the experiments carried out @Z means of
artificial earS satellites; The results given in the preceding articles
indicate the existence O=Very considerable variations of intensity of
the line L a emitted by the chromosphere and of the roentgen region of
the spectrum emitted by the corona. These variationsare doubtlessly con-
nected with physical processes taking place in the chromosphere and in
the corona of the sun. These variations of the intensity of short-wave
ultraviolet ionizing radiation of the sun cause considerable perturba-
tions in the terrestrial atmosphore (disturbance of radio communication,
magnetic storms etc.). The attempt vras recently made to connect these
Card 2/4 variations with solar eruptions.
53-1-b-ii/18
Jnvestigations of the Short-Wave Ultraviolet Radiation of the Sun
The international geophysical year just coincides with the 1.1 years'
period of maximum solar activity, which is very favorable for the in-
vestigations of the variations of the intensity of short-wave solar ra-
diation. Artificial earth satellites should be well suited for this pur-
pose, Experiments planned in the USA are mentioned. In the U.S.S.R. the
measurements of solar radiation will be begun in the roentgen region of
the spectrum. The individual spectral regions will be separated by fil-
ters. The radiation currents will be measured by a single receiver. The
block system of an apparatus for the recording of the roentgen region
of the solar spectruin is illustrated by a drawing. Multipliers of be-
ryllium bronze will be used as radiation receivers for secondary elec-
trons. In front of the receiver are placed filters consisting of alu-
minum, beryllium, and polyethylene filters of various thicknesses. The
calc4ated transmission curves of various filters are illustrated by a
diagram and discussed. Every other two filters are changed in series.
In the disk with the filters there are also normal holes through which
the radiation directly impinges on to the photocathode. The signals
(voltage pulses) coming from the receiver impinge on to a counting and
recording radiotechnical system. At the output of this system continous
Card 3/4 voltages develop proportional to the counting speed of the pulses. The
Investigations of the Short-Wave Ultraviolet Radiation of the Sun
following stage in the investigations with earth satellites consists
of the determination of the line spectra of the chromosphere and the
corona of the sun. (With 33 illustrations, 5 tables).
AWOCIATMN Not given
MWENTED BY
SUBMITTED
AVA-11ABIX Library of Congress
Card 4/4
14) A@ A::E7
5 3-2- V9
AUTHOR: Mandel'slitain, S.L.
TITLE: A Short Sketch of the Life and Activities of G.S. Landsberg,
Academician ( Kratkiy oci;erk zhizni 1 deyatel'-
nosti Akademika G.S. Landsberga)
PERIODICAL: Uspekhi Fiz Nauk, 1957, Vol. 63, Nr 2 , pi 20@c) (USSR)
ABSTRACT: The course of the life of Gri,-Ior 3amuilovich Landaberg was
lacking spectacular events, as it often happens in the case of
eminent scientists, but the more brilbart wa3 his scientific
career. The development of spectral analysis in the Soviet
Union is closely connected with the name of Landsberg. Landsber_K
was born in V31ogda on January 22nd , 1890, he was the son of an
official of the State Forest Service. He commenced his studies
at the Mathematical-Physical Faculty of the Moscow University
in 1908, and he left it with an excellent diplome. He published
his first scientific paper on very hi.--h resistancesin 1-,-,15
Later on, he was called to the arms. From 1916 to 1Q@20 he lec-
tured at the Agricul--tural Inotitute in Omsk and after his re-
turn to Moscow fie became a collaborator at the Institute for
Card 1/3 Physics and Biophysics. 1923 he was appointed assistant and later
53-2-3/9
A Short Sketch of the Life and Activities of G*S, Tandaberg, AcademiciaiL
an lecturer at the Institute for Theoretical Physics of the Moscow
University. From 1q23 to 1931 he was professor at the Second
Moscow University, (which is now the Pedagogical Institute).
Landsberg's work was strongly influenced by Mandel'shtam in the
years from 1925. Numerous investigations of Rayleigh's scatter-
ing (releyevskoye rasoeyaniye) were conducted by Landsberg and
his students in these years. Landsberg and hiandel'shtam examined
theoretically the combination scat,eriDg and, in 1930, they dis-
covered t@a fine structure of the Rayleigh line (liniya Rayleigh).
They discovered the selective scattering light in 1931. 1932
Landaberg was appointed corresponding member af the Academy of
Science of the USSR. He recognized, above all others, the pos-
aiLbilities of spectral analysis for purposes of material exa-
mination, and he received the Stalin prize for investigations
dealing with the same subject. At the beginning of the war, in
1941, Landsberg supervised the erection of emer.-ency installa-
tion of the Physical Institute of the Academy of Science of the
USSR in Kazan'. 1946 he became an acting member of the Academy
of Science of the USSR. He was one of the organizers of the new
Physical-Technical Faculty of the Moscow Univer3ity. There are
Card 2/3 2 figures.
8(2) PHASE I BOOK EXPLOITATION SOV/1855
Soveshchaniye po elektricheskim. kontaktam. Moscow. 1956.
Elektricheskiye kontakty; trudy soveshchaniya (Electrical Contacts; Transactions
of the Conference) Moscowl Gosenergoizdat, 1958. 303 p. 4,150 copies printed.
Editorial board: B.S. Sotskov (Reap. Ed.), V.V. Usov, R.S. Kuznetsov, I.Ye.
Dekabrun, and Z.S. Kirillova; Ed.: I.Ye. Dekabrun; Tech. Ed.: K.P. Voronin.
PURPOSE: This collection of ar@icles is intended for engineers and technicians
designing, developing and operating electrical apparatus and is concerned with
electric contact materials. It may also be useful in scientificy-esearch in-
stitutes and laboratories.
COVERAGE:' This book comprises reports delivered at the Electric Contacts Conference
held in Moscow in Novembertl956. These papers cover physical processes occurring
during connecting or disconnecting, methods of designing and testing electric
contacts, production and characteristics of contact materials. During this con-
ference of the Institut nvtomatiki telemekhaniki AN SSSR (Institute of Automation
and Telemechanics, Academy of Sciences, USSR) participants approved periodic
conferences of physicists, metallurgists, chemists and apparatus design specialists
to discuss problems of electric contacts, which are the components of electric
Card l/ 3.1
Electrical Gontacts (Cont.)
apparatus primarily
d-c control systems.
have still not been
the reports.
TABLE OF CONTENTS:
Foreword
SOV/1855
influencing the reliability of electric systems, especially
Their physical, thermal, mechanical and chemical processes
well analyzed. References are given at the end of most of
I. PHYSICAL PROCESSES
Kragellskiy, I.V. (Institut mashinostroyeniya AN SSSR - Machine-Building In-
stitute., Academy of SciencesUSSR) Contact Area of Rough Surfaces
According to the author, ideal smooth surfaces of mica protrusions measure
20 A. on the beat quartz crystal 100 A, on highly polished metal surfaces
0-05 - 0.1 mi@ron, and on rough metal surfaces 100-200 microns. Moreover,
the machined surfaces usually have.a wavy structure. The author has de-
voted his paper to finding methods of calculating the actual area of con-
tact of surfaces. After a detailed *,heoretical and practical analysis he
derives formulas for practical us6 by designers. There are 6 references,
of which 5 are Soviet and I English.
Card 2/ 1.1
7
7
E1;_*ctrical Contacts (Cont.)
SOV/1855
Mandel'shtam S.L.. Sukhodrev, N.K. and Shabanskiy, V.P. (Fizicheskiy inBtitut
- Institute of Physics, Acndemy of Sciences, US33) Processes Occui-ring
on Electrodes During an Arc Discharge 25
This article is an abridged version of the report delivered at the 10th
Spectroscopy Symposium. It was printed in full in the transactions of
this symposium. It is based on the results of research carried out by
the authors at the Institute of Physics. The authors found that pro-
cesses of arc discharge are different for the plate and cathode. Pho-
tographs of spots, left after the discharge show a different structure,
the plate sport being much larger than the cathode are.
Zolotykh, B.N. (Tsuilelektrom, Academy of Sciences, USSR) Dynamics of the
Process of*Electric Erosion of Metals by Electric Pulse Discuarge 27
The author explains briefly the theoretical fundamentals of this pheno-
menon and discusses in detail its basic regularities, the additivity law,
the relation between erosion volume and spark energy, the relation be-
tween erosion volume and thermal constants of metals,, the polarity of
electric erosion and its relation to pulse duration. He reports results
of exper@mental investigation of the formation of Spots 3nd indentations
on electrode surfaces caused by single pulse discharge. He refers to G.V.
Gusev and A.S. Zingerman and thank A.I. Kruglov, Zh.Ye. Gryazunova and I.P.
Korobova.
Card 3/ 1.1
@j) N ). E L T 6 PV), -,), L -
AUTHOR: Ukholin, S. A., Candidate of P.Vcical-.@Iat@-.e-at_,oal 3C-2-35/49
Sciences
TITLE: New Studies in the Field of Spectroscopy (I@Iovyye raooty
~ oblasti spektroskopii). Conference in voscow (Soveshchaniye
~ Moskve)
PERIODICAL: Vestnik A-kademii Nauk SSSR, 1958. lir 2, pp. 107-107
(USSR)
A13STRACT: The llt11 All Union Conference for Spectroscopy was held from
December 2 to December 10, 1@157 in 11oscow. The tc)T-,-!-,s were
particular problems-oT and que9tionz of lumin-
escence. About 600 representatives of' scientifir! research in-
3titutes of the A-S USSR and the acaclemies of t,-.e union repu-
blics, of the branch institutes and the universities of 36
cities of the country took part. mong -the j@uests there were
scientists frora China, Roumani&, 'ftqroslavia, the German Demo-
cratic Republic, the German Federal Republic, the USA, Ene-
land, and France. In 7 f-eneral mectines and 12 3e,,,tjr)na1 meet-
ings 132 reports were heard and discutised. They -.reated the
theoretical and experimental determination of' the atom con-
Card 1/2 stants, the spectroscopy of the plasma, of the crystals and
New Stud:Les n the Field of Spectroscopy. '@C -2- 3C/4 9
Conference in "'luscow
of the transition stages, the investicationof intermolecular
interactions, and the investiFation of the conversion of the
electzic energy and spectroscopy of the staCes of molecular
oscillation. The opening speech was held by S. L. Mandell
shtaw., Chairman of the Comission for Spectroscopy. S. E.
Prish reported on Soviet spectroscopy during the last 40
years, and A. F. Prikhotlko reported on the inveetigation of
molecular crystals especially at low temj@erat,-res. There
were also many discus3ions.
AVAILABLE: Library of Co.,.,gress
1. Spectroscopy-Applications 2. Lxmtinescence
Card 2/2
HOMISIMM, S.L.; SMODMW, N.K.; SHAMNSKIT, V.P.
Processes on spark-discharge electrodes. Fiz.sbor. no.4:148-
154 '58. (MM 12:5)
1. Fizicheakiy institut imeni P-N-Lebedeva AN SSSR.
(Alectric spark) (Mlectrodes)
WING, N.A.; MAIMEL'SHM, S.L.
Broadening and shift.of spectrum lines in the plasm of a
g%s discharge. Fix.abor. no.4:305-307 158. (KM 12:5)
1. Fizicheskiy institut imeni P.M.Lebedeva AN SSSR.
(spectrum analysis) (Electric discharges through gases)
BALANDIU, V.11.; IWMELISHTAM. S.L.
Possibility of an l.-rzing the composition of a metal in an
are furnace without taking a sample. Fiz.sbor. no.4:387-
388 '58. (MIRA 12:5)
1. Fizicheskiy institut Imeni P.N.Lebedeva AN 353R.
(Metals--Spectra)
iUTHOR- Mandel' dAampS. L. SOV/48-22-6-1/28
TITLE: Opening Address (Vsi@$iltellnoye slovo)
PERIODICAL: Izvestiya Akademii nauk SSSR, Seriya fizicheakaya, 1958, Vol,, 22,
Nr 6, pp. 647-649 (USSR)
ABSTRACT: This speech was made on the occasion of the opening of the
XI. All-Union Congress on Spectroscopy, which took place imme-
diately after the October festivities (during the first days of
November 1957) at Moscow. The author mentions that under Soviet
rule important discoveries were made in this field in the USSR,
above all in the field of atomic and molecular spectroscopy, by
Vavilov and Cherenkov. Further, the works by D.S.Rozhdestvenskiy,
S.I.Vavilov, G.S.Igmdsberg, V.A.Fok, A.N.Terenin and
V.N.Kondrat'yev, which deal with this field, are mentioned. The
author further points out that applied spectroscopy is particu-
lar2y well developed in the USSR, and that it is being used in
various mys for research work and production control. The
author spoke a few words in connection with the decease of
G.S.Landsberg, Member, Academy of Sciences, USSR and former head of
Card 113 the coumission for spectroscopy, which took piace Inis year.
Opening Address
SOV/48-22-6-i/28
The author further telIz that th,3 last congress on spectroscopy,
which took place at Llvov was attended by 1600 delegates, 910
that 300 lectures were delivered. The excessive number of dele-
gates and the great number of subjects to be dealt with by
lectures were disadvantages which caused the organisers of the
congress to convene such meetings every year, but, on4 for one
particular field of spectroscopy. Thus, it is intended this year
to deal only with the physiml problems of spectroscopy, and that
problems of applied spectroscopy will form the sole subject of
the XII. meeting. The author is, however, of the opinion, that
recently a "dangerous tendencyl, has been developing in the USSR
with a view of forming two graaW of "spectroscopists": The
"atomists" and the "molec-alists". For the convenience of the
delegates it was decided that on forenoovz lectures of a general
character will be held, while speoia-I leotureB will figure on
the afterroon program. Finally, the author stresses the impor-
tance of maintaining contact with other countries, and he
mentions the names of foreign scientists who attended the congress
Card 213 to which they had been invited-. Professor Badareu (Roumania),
Opening Address
SOV/48-22-6-i/28
Professor Bartell a (German Federal Republic), Professor and Mrs.
Grillot (Griyo) France), Professor Lokhte-Khol'tgreven (German.
Federal Republic@ :Professor Ritchl' (German Democratic Republic),
Professor Thompson (England), Professor 'Yanke (German Democratic
ReNblic), Professor Khadzhi (Yugoslavia), Professor
Cbzhou-Tun-Tsin (Chinese Peolple's Republic), Professor Dike
(USA) , and Professor Lecade (France).
1. Spectroscopy--USSR 2. Scientific personnel--Performance
Card 313
AUTHORS: Vaynshteyn, L. A., Koloahnikov, V. G., SOV/48-22-6-20/28
Mazing, M. A. , Mandell shtam, S. L.
Sobel' , I.
TITLE: On the Broadening and Displacement of Spectral Lines in a Highly
Ionized P18RmA (Ob ushirenii i advige spek-trallnykh liniy v
vysokoionizovannoy plawne)
PERIODICAL: Izvestiya. Akademii nauk SSSR, Seriya fizicheakaya, 1958, Vol, 22,
Nr 6, pp. 718-719 (USSR)
ABSTRACT: The investigation of the breadth and shape of spectral lines dn,"
not characterize the excitation of atoms with sufficient accumoy,
and therefore an investigation of the breadth and the displacement
of the lines is more advantageous for determining the causes of
these phenomena. The principal cause of the broadening and dis-
placement of spectral lines in a highly ionized plasma is its in-
teraction with charged particles. For lines with quadratic Stark
effect the impact theory of broadening results in the following
expressions for the brea4th of lines and their displacement:
11,4C 213 1 3 9 $8C2/3 ,113,YF
' 4 v 4
Card 113 where Cj+ denotes the constant of the quadratic Stark effect,
On the Broadening and Displacement of Spectral SOV/48-22-6-20/28
Lines in a High2y Ionized Plasma
v - 7elooity, dr- the density of the excited particles. Herefrom
it follows that the ratio between the breadth and the displacement
of 04- 7 and of Is irdepend ent and equal to, f / 4 = ! -1 6, In the
case of interaction of a different kind, as e.g. according to the
equation by Van der Vaal rlZ@ = 2,8. The task to be carried
out by the presen-t paper AS to find a correct explanation of the
interaction batween radiating atoms and charged particles, i. e.
the applioabili@y of the aforem@.ntioned r- formula ?r-th respect
to the lines with quadx-.Uo Stark effect, As objects the 1@.nes
Ar II, which are excited in the channel of the spark dischargeo
were selected. Measurements of breadths and displacements of lines
were carried o1A photographically. Results are given by a table,
By checking these resulta waa found that those obtained by ex-
periment contradioteJ theoretical results oomple4ualy. This is ex-
plained by the fact that ihe initial expression for the Pisplace-
ment of the frequency of the atom oscillator A W = 04/e, where
R denotes the distance to the exciting electron, is not applicable
Card 213 in thia case because the eiectrona playing the pr1nnipa.". part in
On the Broadening and Displacement of Spectral SOV/48-22-6.-2D/28
Lines in a Highly Ionized Plasma
the broadening of the lines form a Weisskopf radius that is too
small. The field formed by the electrons turns out to be so
strong on this occasion that the Stark effect ceases to be
quadratic and goes over to linearity. There is no reason to be-
lieve that the field changes slowly and is quasistatic as is
alleged by a well-known theory. The problem is still being dis-
cussed. There are i table and 3 references, 2 of which ara Sovist.
ASSOCIATION: Fixicheakiy institut im. P. N. Lebedeva. Akademii naiA SSSR
Mysics Instit-ate imeni. P. N. Lebedev,,AS USSR)
1. Spectroscopy 2. Electron gas--Spectra 3. Perturbation
theory
Card 3/3
2,1(3), 2o.(7) SOV/ 51-6-6-21/34
AUTRORS. Sukhodrev, N.K. and Yandellshtam, S.L.
TITL3- On the Temperature of Electrode Vapours in a Spark Discharge
(0 temperature parov elektrodov v lakrovom ratryads)
PERIODIC&LsOptika i spektroakopiya, 1969P Vol 6, Wr 6, pp 723-728 (USSR)
ABSTRACT: Vapour temperatLires in a spark are usually assumed to be equal to electron
temperatures of atoms and ions of the vapour. Electron temperature can
be determined from the relative Intensity of two or more spectral lines,
provided atoms are distributed in excited levels according to Boltunann's
lam. Earlier measurements (Rags 2. 20) yielded valuaa -10 OOOOK for
temperatures of electrode vapours in electric sparks; these values refer
to colder (crater) parts of vapour clouds ( tlflameG"). The Fresent paper
discuss as deter"ination of temperatures in hotter parts of vapour
clouds. Al III, Sn IV and SI IV lines were used (Table 1). Aluminium,
tin and silicon were used because their atoms have sufficiently high
ionization and excitation pot,:mtials to allow determination of temperatures
above 10 OOOOK. A glass spectrograph ISP-51 -was used for Al III lines
(visible region) and a quartz spectrograph ISP-22 was used for Sn IV and
Si IV lines (ultraviolet region). The apparatus used is shown in Fig 1.
The imge of a spark Sl vas focused on a spectrograph slit via
an intermediate slit d., a concave mirror 02 and a rotating piane
Card 1/3
On the Temperature of Electrode Vapours in a Spark Discharge
SOV/51-6-6-2/34
mirror M10 The latter wan rotated at 1-3 MIR/se c producing a time
scan (display) of the spark on a recording film in the spectrograph.
The time resolution of the spark spectra ranged from NO.04 to 0.1 lisec.
Sparks wore synchronized with rotation of MI by means of a device, shown
at the bottom of Fig 1, which ensured tK%t a sparV. at Sl was produced
when the image of 31 was focused at the apectrograph slit. The spark
discharge circuit parameters were: C = 0.01-1 IS, L = 2-3000 IiH. The
voltage across the spark gap Sl was 15 1cV and the distance between
electrodes was 2.5 mm. A record of a spectrum obtrtined between tin
electrodes is shown in Fig 21 it contains Sn IV, Sn 1, 11 11 and 0 11 lines.
The results are given in Tables 2-6. Table 2 refers to sparks between
tin electrodes (Sn IV lines). The results of Table 3 (Sn IV lines) were
obtained with one tin and one copper electrode. Table 4 gives temperatures
deduced from Sn IV and N 11 lines - Table 5 gives the results obtained
vith one aluminium or l0y@-Al bronze electrode (Al III lines). Table 6
gives temperatures deduced from experiments with "silumin" electrodes
containing 10% Si (Si IV lines). The temperatures deduced from Sn 1V
lines were -26 OOOOK, from Al III lines they were 30 OOOOK and from
Card 2/3 Si IV lines they -were 35 OOOOK. BorAuse of high scatter of the result3
On the Temperature of Electrode Vapours in a Spark Discharge SCri/51-6-6-2/,14
it was impossible to say whether the differences between these three
sotq of temperatures were due to a definitue cause or accidental. Since
the spark-channel temperature, deduced from N II and N III lines, is
-35 OOOOK, the results obtained suggest that tin, all=inium and silicon
vapours were heated and excited in the spark channel itself. Acknowladg-
ments are made to L.P. tialyavkin and V.K. Bardin for their help in
experimental viorV. There are 3 figures, 6 tables and 13 references ,
6 of which are Soviet, ^4 English, 1 German and 4 international.
SUBMITTED: July 8, 1958
ca rd 3/ 3
"IT DfORS Tsichay, N.S. and ,iandellshtam, S.L. SOV/51-7-2-2/34
TITLE: On the Influences which -iffect the Intensity of Lines in the Fiame
6pectram kO vliyaniyakh na intensivnost, speictrallnykh linly v
spektre plameni)
PERIODICAL: Opti;ca i spoirtroskopiya, 1959, Vol 7, Nr 2, pp 141-151 (USSR)
BS TRAC T
Card 1/3
The authors studied chano-as in the intensities of the lines in the
flame soectra of sodium and strontium when the forul of the compound used
to introduce the element vas altered and the changes which occurred on
introduction of compounds of other elements. To find the reasons for
these changes it is necessary to investigate the vkriations produced
in the density of free sodium or strontium atoins in the flame and the
variations in zhe conditions of excitation of these atoms. rho method of
anomalous discersion was used to ..@easure the Consities of atoms in the
flame. The apparatus used is shovrn schematically in Fig la; it is
based on D.S. Rozhdostvanskiyls interfarometer. To measure the densities
of atoms at v@-rious distances from the axis of ar, acetylene flame
(1 in Fig la) the interference fringes were localized at the contra of
the flame parallel to its axis. By means of three plane mirrors 2, 3, 4
and a lens 5,the flame and the interference fringes were projected on to
SOV/51-7-2) '2/114
On the Inf luences whi ch Af feet the Intans ity of Lines in the Fla--a Z pe ctr.=
a spectrograph slit 6, at right angles to the latter. A three-prism
spectrograph ISP-51 was used. Solutions of the compounds amploye'd 7?.nre
injected into the flame by moans of an atomizer of the usual type. The
f1a.me diameter was 11 mm when Na, K or JAg were introduced into It,
9 ian for Li and 7 mm when Sr, Ca and Ba were used. The densities of
atoms were measured at a height of 15 mm above the blue part of tkv@ flame.
The experiment consisted of aleasuring the displacement of the int,4rfaranc6
fringes near an absorption line of the element studied . The zhaL@,5 la
the refractive index of the flame -which produced this displacement -_9
related directly to the atom density N by Selhieierls fonaula. rho
displaceinent of the interference fringes was ueasured with a microscope
with an error of 15Y.- -'part from the atom density X which vias F_ mear,
across the flame, the authors determined also the distribution of --tans
across the flame by measuring the displacement of the interference
fringes at various distances from the centre of the flame. The aut '-:orc
recorded also photographically the intensities of the atomic lines and
they measured the flame temperature (using self-reversal of the lines).
First the authors studied the effect of the comoound which -.,jas used to
oard 2/3 introduce sodimi or strontium. Sodium atoms we@e introduced In the form
of NaGl, Na2CO,3 and Na2SO4, and strontium atoms were introduced as
SOV/51-7-2-2/34
On the Influences which Affect the Intensity of Lines in the Flame Spectrum
SrC12 and Sr(NO3)2. Displacement of the central interference fringe
was meAsured at distances of 1.5 and 2.6 1 from a sodium line at 5890
and at a distance of 0.52 A from a strontium line at 4607 A. Secondly
the affect Of MgC12, GaC12, SrC12 and BaCl.? on the density of sodium
atoms in the flame and the of fact of NaCl ari CaG12 on the density of
strontium atoms In the flame were Investigated. The authors measured
the displacement of the central interference rinc, at a distance of
1.3 1 from a sodium line at 5890 A and at a distance of 0.52 A from a
strontium line at 4607 A. The results (Figs 2-7) show that the changes
in the intensities of sodium and strontium lines,under conditions
discussed above, are due to simultaneous effect of two factors -
(1) a change in the free atom density in the flame due to a change in
the rate of supply of the solution and (2) a change in the conditions
of excitation due to a change in the flame temperature. This conclusion
is confirmed by theoretical calculations. There are 8 figures and
16 references, 5 of which are Soviet, 5 English, I German, I Dutch,
2 Swedish and 2 others.
SUMUTTED: September 9, 1958
Card 3/3
22(9),24,M PHASE I BOOK EXPLADriATTO' so",
Akadeadya nauk 33SR. Fizichoskly LnStitut
lasledovanlys po ek3pertment&llnoy t tcoretlcnes@oy ftzike; fabOmt-
(studi::)on Experimental and Theoretical Physics; Collection of
Artict Roacowt lzd-vo AN SSSRj 1959. 304 p. Errata slip
injp&rt*d. 2,300 copies printed.
Ed. Fabelinsidy I Doctor or Physic aIC&nd Rathematica:
nCX,;;L 0 is H a.
Zda *f Publ hing us . A. L. hernyak and V. a. tmrKgmu%,
T*ch. Zd.& Tu. V. ftylins. Commission for Publishing the Collection
i.=r7)Qf tIlIg.,il. SammuilovLch Landaborg. 1. Ye. Team
(C .Academician; M. A. LeontOvIch, headetatclan;
F. L. Uzhulin, Doctor or Physical and mathematical sciences;
3. 1. Randel'ahtam, Doctor or Physical and Withematical Sciences;
1. L. Fabelinsidy, Doctor or Physical and Pt%thematical Scianzel%;
F. 3. Landabarg-Baryshanakaya, Candidate of Physical and Math-
O&ACical Sciences., and 0. P. Motulavich (Secretary), Candidate of LA
p1tysical and Math*mAtIcAl sciences.
PURMUt This book to Intended for physicists and roaaamnerm
engwa. in the study of electromagnetic radiations and their role
_131-v"fitighting the sti-4cture and composition of' materials.
COV12LUM. The collection contains 30 articles which review
Investigations In spectroscopy, monies, molecular optics, soul
cond:umtor physics, nuclear physics, and other branches of
physics. The Introductory Chapter gives a biographical prortl
of 0. 5. Landaberg, Professor and Read of the Department of
Optics of the Division of Phyalcal Technology at Moscow Uni-
versity, and reviews his work In Rayleigh scactertng, coutbat
9IL"S. spectral Analysis or metals, *to. No personalities am
amnotiontd. nortren.es &ceomp&ny_e.h article.
Bazhulln. P. A., y__L_J1LjzshLv. and M. N. Suahchinakl The
Work of G. S. LandBbOra UT-the Field or molecular i;*.trC.cCWrT
-__WrCAiCa_. T_'j_..and Inv*stigntlon of Trans-
ro-ruatio. ;AcOssed In an Activated Diacharge Generator Ope .-
tin& Under Conditions of Low Am Currents 27
1. R. Kuznet-
a ro-.3-MM-cy- I
.Orlc DLalkyl-
Cnl0h*X&no an the ftsIs Of & Combined Scattering Spectrum 43
Andrayev, M. X StAnding Sound Waves of [Arr
Amplitude 53
_ Investigation of Cho
ti..P A_@@C!.A_ I- Sgw@1gmkAjq,
101:11,1-n
psi ture r Idth Of Cce;blned Scattering Lines to TOM- 56
ftdIV__A-ftbrUZLnt. A Radius With Magativo
arc
?
t
l
.
c
en 62
V. V. Nuclear Tr "neitions in Nonaph*r1cal Iduclal 71
0. Optical Properties Of Substance, Lio the
'S
.1 80
3. Vdvllov and A. P. Shotov. The Question of
-
-
-
-
-A
w-r
tr
a7a
o
.
miconucX
t
d
rw 95
Vul't r
3
"O%Methoft or Increasing the Effectiveness
r
,,.
The ocouples
100
and A.
L. 50
ttering of Light Near
G=, V
r
'60 Transition of the So Ond Type and the
:
CrAtIcAl Curl@ Point 104
1"kOvich, M. A. Irradiation or an Elastic Wall Vibrating
Under thi A@tlon of 3t&tlatic4lly Dlatrib.ted Forces 117
LAVIZ. M. The vt=lng or Light by a Cloud
L21
t nd
V_0_ The
l
1
1
BrOsdaning
ano 1
o
1
,HNO tral LiEe_j _6? a-04a
,ft
@
Discharge n Planma
l 128
M&iy*h*v. V- 1, end V. N. XurUp. Investigation of the Hydro-
-
'
9421 b0fi
ff
in SubatVKian Wh@se mqI&oulQ8 Contain Two Hydroxyl
134
"702
AVMRSj Grane-kLy, T.L. Lkty..cv ..V. and
TrMS i Report a the Second All-U.Icu C-of-r-UG- -A G&O
sloctroMa -
1
PRUTGOICAL. Radlotokhalka I olaktroalka, 2959, Vol 4. Ur 3, 1
vp Wig - X35a (USSIO
AOSTRAM The conference$ v*. organised by the Ac.3c.033R. the
.4 Ministry of 111ghor 19dc.tion -4 State
G" Density During
TAOQXAW tb
ABA,
-
:.
the Dynamic Oper I.. of . Di herg (.*. p 1306 f
?
"a Journal).A.V. Xedcapasav The Nat@o of a Str
atod
Positivo Coltuan..
.. XP_.j, ..,. -The Th.." of Probe. for
. @
aoures
Pr
.
t positive Colu,nu of a niacharge
'
:
:Th,
-
N=.. R
t
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UsIx-Eaupawa - 41",tuonc* of the Processes or the
tion of the Negative Ions on Their Concentration
In the C'cIna*'
.
d
b an ng
a ma O&CLIlations d -.a
w
:
if! =.r Pl
YU,L. Klimantovich - "Bn*rsy Lost by Charged PArti-l.- C.r
MWTE-- ---Fr-tho 0 1 B
=6 atTon Bel I tions In pl.... (rb. L.Ut..Lr
pdta"Z)o Bad aThe Tb*oz@of Mon-lic,ear Flax" Ov4LIlatlonsft,
at
= An A
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Discharge on the Material or the llect-desm. .
A@ &MJ:. X -F.MAttcft of Light
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@
the journal).
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FLOW Co.. V 1233 of the Journal).
To paper by L.M. b*T`- and S.A. T.kl..hw .."Ider.d
th: Approximate nothod. for dot_.L.L.S the
of tows, at the rdL.tL*.
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he Ptrl Ll... In G. _di. h-g.
(Logland) - -The XL-tL.. of 91-t-a Colli.tcna
to th HY4@-C-A 10
X..Lt
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P
240) SOV/48-23-8-18/25
AUTHORS: Mandellshtam, S. L., Mazing, M. A.
TITLE: Widening and Shift of Spectral Lines in the Plasma of Gas Dis-
charge
PERIODICAL: Izvestiya Akademii nauk SSSR. Seriya fizicheskaya, 1959,
Vol 23, Nr 8, PP 1017-1020 (USSR)
ABSTRACT: In the present paper the widening of spectral lines with
quadratic Stark effect due to charged particles is investi-
gated. The equations (1) for the width and shift of the lines
are described. To compare theory with experimental results, the
dependence of width and shift on the constant of the quadratic
Stark effect and the ratio of width to shift are investigated.
The results show remarkable disagreement with the theory by
Weisskopf and Lindholm. Analysis of this disagreement resulted
in the development of an unsteady theory of the widening of
lines. According to the assumptions of the theory, a smaller
effect of the collision of electrons with atoms as well as in-
elastic collision of electrons with atoms are taken into ac-
count. For this theory, the nonuimensional parameter 0 is given
Card 1/2 by formula (2), which characterizes the width and shift of
SOV/48-23-8-18/25
Widening and Shift of Spectral Lines in the Plasma of Gas Discharge
lines. The ratio of width to shift depends on this parameter.
Figure 1 shows a comparison of theoretical values - calculated
by the unsteady theory - to experimental results. Good agree-
ment could be obtained. It was found that this theory permits
the determination of electron density from the width and shift
of lines. Table 4 compares electron densities calculated by
the steady and unsteady method. There are 1 figure, 4 tables,
and 2 references, 1 of which is Soviet.
ASSOCIATION: Fizicheskiy institut im. P. N. Lebedeva Akademii nauk SSSR
(Physics Institute imeni P. N. Lebedev of the Academy of
Sciences, USSR)
Card 2/2
24(7)
AUTHOR: MLndel'shtam, S. L.
TITLE: in-.-rol..'v@tury @;pea-!i@ --',ic I 'J".
@i: ..-pectro3cclyy
PERIOIDICAL. Izvestizya Akadem.-' au---:k SS311. JorAja .`.zicheoka
Vol 23, Nr 99 pp o14-!o96 (uSsa@
AMTRA"' !--I h- S:-"-J"--1 -C'-.! "-,3
auri t"@-- t cv@ 1-2t1'.
;--,f' spflctxos@@-OD to
Y "
spectru-1. "') -2 t7aatel. Whezre-"@, duriri@-. roc
years, concen'tration could 1@o only up t@, a @@on
of jo-4 - 10-6%, a -jurvey givar. ty L. V. 114-pj-9 in form :)f
lecture showed that t,,day conct--ntrations may De ,Je-
t-.rminad withJn the rarga of '*0"- 0 - wh@rh are cf im-
pGrtance e.g. for semicondQctor grin g. It was srated
aith satisfaction that So@riet sper;tr@,e7@,-,py perf.-Irmed pioneer
work ir, the courae of ra-@er-@ ,-Fa7.3 wi@h respv@,it -,- ti,e deter-
minatior. of gases di8eolved in me7@,!- In Sovi2c*,
industry photoele.-.tri@,ai merh@.;-!e are at Tras-,@n- ;c be
introduced irt@; spe,-@t:ra',- ona@3,7113. an,i rh,.* importar"e -@f these
Card 1/13 methods f--,r automatlDn is pointe@' out. Employment of these
oil
methods in the Ameri@Url LIIUrA,%,,M i:--distry is given an exam.-
pie, and it fs ;;oInted thet the J-@,eiopmant :f phctoeleo-
@rica'- methods in X-:ray @Jpe,,+@al inp*.y@,fo s-@all !Aaves mu@.h
to be desired. I. B. BCr-,-fEk1y ga-.-.- a -f th.;; problem.
A considera'@Ie number -of deal-! with an-alysig methxds
with the
as
for powdered npecimans an@ rar6 C
ph_ysi@@al Irasso cf spe-t-al azna@y@,-'P. At,.-mic s e -- ti L analysis
is cconsidered to lj,@ ar. indiapenden-t :f with a
vvell de--re-`,pee the:>ry, aad -'@! the
mclecular spectzai analy,@.t@q '.5 1.9
thati in contraat tr. :)ri---y -:ae Partial
problems are sc!-:P@ ir this F-)-, ':.f :Intro-
methods in The -,f ti;@ cl,ez' :a" -a-,er3
b
.Y V. M. Chulanovsk@.@,, P. A. Br:zl.ui @k- a r. 61', Fjush,-.MnskJy,
and by B. S.Neparo@rst are e @-T lz';@cj7tan@@a. Ton.
pape,-,sieal w1kth paramagnatic awi resonances,
and in r;onnecticn with the f Iw7,)rIe-3zenrFj f3pe(;tral
analyses the soiEintietf; F. 1). Klem-@ri*,, S, V. Shpr, skly, and
A. F. Prikh-@,t'kc. axe Laent':ned. P. P. him-
self with apec,troscopic poIr-rAzat--c.;@ %:id T- A. Tumerman
Card 2/3 dealt with the a2plication .:f in bic-
SOV/46-23 -9-1/57
tz-c@duatcjry Speech al.- the Tvelft*a
I-onferense = Speatrr-s2opy
chemistry and biology. The instruments IKS-'4 SP-1., DFS-112..
and others, which are produced by the Soviet industry for
molecular analyses, are menti-oned. The scientists S. A. Borovik,
?.Iember of the Commission for Spectroscopy., I. A. Shoshin,
who is also a member of this commission, and V, S. Mlliyanchuk
are mentioned, who have died i3iniDe the last confererce, and
honorable mention is also made of G. S. Landsberg7 the former
initiator and chairman of these conf6rences.
Card 515
3 11-2 171
,UTUOR3, B.t;l:" B. U.. VI.*gr.d4%mA. X..
0. . !t@@
VTVTLUPI- & 1*1@tria Stylamster With Tt-jul Coctr-I Of the V--lti-a
1. Lin.. of the Sp..tr-
r raw b
'959,
&kadMti Mak 33SR. (3-R@& fisich-kal-. 1959,
Vol 23, Mr 9. Vp 11$0 - 1112 USS
AMRACT, Iy replacing the gla-e-disParejan Optical . Iat- by . qcs@t-
(TIA 1) or diffraction orti cal ,at. . (FL4 2). th. -,.go at
applicability of %be M-1-typ~ StyLoMeter May be .... id-bir
extended. "p-lally it, by Samoa at an .1--tron-optical can-
v.rter. the Invi.11blo lines cret h @,I:p trus czy b:.d:,t..'..d;.
,:a
Two -rivots of the type rW a, re jap*4 and t t I by t
4o"I %bL, vvrt*r Operates with An sntic*ny-sai-cathodol
"'! "as a,
th dw, an u,-%ransmiwil. I.do.. .. that . 'i.-I
sets,vittlOn 2f the NP00trUAR,Ithin the as I..8-h rsng. at
6000-24on X 1. possible. II"r.* i ad*; ".. the a*.". at
rmystia them* two L. which the hitting at the
$Va. russ with - p"t to the o.tl.t lit i brosht.,b0:1 by
car& 1/2 rotating the dispersion system. Th. line intensity , t as
,"t-ant, to comparable to that of In*trum-te,
of which has 6 14-Ith a the spectrum
4 tf 2oo-3go J. Was, of
.b: linew by 80400 Of he -1-rtar to describ
4 S-4 rOr both Lutr .. n,g # ,my of tb.
teri.tio reat"Os is lirga. Th. focal
'bi ,11 di-t-Q-- Of the mirror
of the collimator are 6a. and 75-
the r:f=,..tLQ. 1.41. (qcurts prism) in Ong of the
is 60 . 0 rams L..t--t.
grating 110-- path* 4"fr"O"O' 9"ti-4 at the other ban 6oo
r millimeter. Th. j.oi_.-&ptj_j mrmag_ect
asks. it Posigible in *be-". the fl.. details r .,Ii..t.d
.Pact
arm d this 4-'1-- is said 1. h...
a gr t
C"d 212
21(7) SOV/56-36-4-66/70
AUTHORS: Mazing, M. A., Mandel'shtamr, IQ. L.
TITLE: On the Widening of Spectral Lines in a Highly Ionized Plasma
(Ob ushirenii spektrallnykh liniy v saillno ionizovannoy plazme)
PERIODICAL: Zhurnal ekuperimentallnoy i teoreticheskoy fiziki, 1959, Vol 36,
Jr 4, pp 1329-1331 (USSio
ABSTHACT: Already in earlier papers the authors measured width and shift
of spectral lines in spark discharges (Ref 1); here a short
introductory report is given about this problem and also about
the theoretical connections between line width, shift, and the
plasma parameters. The authors carried out much more accurate
measurements of the line width y and the shift L of 50 Ar II -
lines as well as of some He I -lines in the plasma of a spark
discharge in argon and helium. Experimental data: U - 14 kv,
C = 0,02 F, L - 10 H, T - 30 - 40000 0K, electron concentra-
tion -,-,1017 CM3. The spectra were photographed by means of a
upectrograph with a dispersion of 21/mm. The accuracy of meaour-
ing line width amounted to 5 - lOdlo, the smallest still record-
Card 1/2 able shift was - 0.03 1. The results obtained from measuring
SOV/56-36-4-66/70
On the Widening of Spectral Lines in a Highly Ionized Plasma
ASSOCIATION:
SUBMITTED:
Card 2/2
4579,4 5,1 0.45
4460.4 3.8 0,66
4598,8 8.4 2 7
3561,0 12 5@O
3559,5 13 5.6
4474.8 15 7.6
There are 1 figure, I table, and 6 references,
Soviet.
6 Ar 11 -lines are shown by a table; they are typical of this
kind of measurements.
- 0 -11 -1 - 11 -1
", A 10 , sec 10 sec Y/6
11@5
5 S
3,1
2.4
2 3
1.9
3 of which are
Fi7.icheskiy inatitut im. P, N. Lebedeva Akademii nauk
(Phy3ics Institute imeni P. N- Lebedev of the Academy of :@cien-
oeu, USSR)
February 12, 1959
240) SOV/56-37-2-4/56
AUTHORS: Lebedev, S. V., Mandal_Lz@ -S.L-, Rodin, G. M.
TITLE: On the Short-wave Radiation of a Vacuum Spark
PERIODICAL: Zhurnal eksperimentallnoy i teoreticheskoy fiziki, 1959,
Vol 37, Nr 20), PP 349-354 (USSR)
ABSTRACT: The spectra of the highly ionized atoms in a spark discharge are
in the ultraviolet range and in the range of soft X-ray radia-
tion; it was investigated down to 6 1 (Ref 1). In this case the
excitation energy amounts to 2000 ev. In the present paper the
authors give results obtained from investigating these spectra
within the range ),< 6 1, as well as an evaluation of the dis-
charge temperatures by means of a spectroscopic method. (Anal-
ogous temperature measurements have already been carried out by
Aki;aov and Malkov (Ref 2).) The measuring method is first brief-
ly described (iron electrode - one plate and one cylinder, dis-
tance 4 mm; initial pressure in the discharge chamber 1.10-5= Hg;
current source: condenser 3.3 @(F, 40 kv, 1.511H, O.2Q3 ,
- 4.8-10 4a; absorption of the longer-wave radiation by
1
Card 1/3 max
On the Short-wave Radiation of a Vacuum Spark SOV/56-37-2-4/56
beryllium filters; recording: photomultiplier FEU-25 and cathode
ray oscillograph. Total sensitivity of the FEU: 10 a/lumen;
filter dimensions: thickness 0.25 mm, diameter 18 mm; scintil-
lators: tetraphenyl-butadiene in polystyrene and CsI(Tl),
5 mm thick . The results are given in form of characteristic
oscillograme. Three series of measurements were carried out
under various conditions and by using the two above-mentioned
scintillators, and the latter are described in detail. The sec-
ond part of the paper deals with temperature evaluation. The
value obtained for electron temperature in the case of a spark
discharge in a vacuum was found to amount to 2.1o5 OK. These
evaluations agree with measurements. Figure 5 shows the temper-
ature dependence of the intensity of the lines of multiple
charged ions for an electron concentration ne - 10 18 electron/GM3;
the curves from Al V to Al X are given. The Position of the
curves shows to what extent temperature evaluation depends on
ionization - the curves shift with increasing ionization towards
higher temperatures; to the here mentioned temperature of
Card 2/3 2.105 OK there corresponds the Al VII peak. There follows a
On tho Short-wave Radiation of a Vacuum Spark SOV/56-37-2-4/56
short discussion of the excitation mechanism, which m1ght ex-
plain the spectral composition of the observed radiation.
There are 5 figures, 1 table, and 8 references, 4 of which are
Soviet.
ASSOCIATION: Fizicheskiy institut im. P. N. Lebedeva Akademii nauk SSSR
(Physics Institute imeni P. N. Lebedev of the Academy of
Sciences, USSR)
SUBMITTED: March 3, 1959
Card 3/3
S/560/-61/000/010/002/016
D299/D302
AUTHORS: Mandel'shtam, S. L , Tindo, I. P., VoronIko,
-YU-. 'K., Shurygin, A. I., and Vasillyev, B. N@
2ITLE: Study of solar X-radiation, 1. 'Geophysical-
rocket measurements
SOURCE; Akademiya nauk SSSR. Iskusstvennyye sputniki
Zemli. no. 10. Moscow, 1961, 12-21
TEXT: This is the first of 3 investigations on X-radiation
in the range below 10 R carried out by research rockets and the
2nd and 3rd Sputniks. Provisional results of these measurements
were set forth in brief in an earlier study. Experimental
method: The measurements described in the present article were
carried out during the flight of 2 research rockets. The urime
object of the measurements was to accumulate experimental data
and to develop a method for subsequent measurements by means of
Card(1/5
S/560/61/000/010/002/016
Study of solar... D299/D302
earth-satellites. As detectors, photon counters were used, as
these are more sensitive in the spectral range --@ 10 R than
vacuum photomultipliers, The sensor unit was placed on the in-
strument container which turned automatically towards the sun.
Special precautions were taken to ensure that no corpuscular
radiation should interfere with the measurements. In the first
launching, the sensor unit incorporated 2 similar counters
directed towards the sun; one of the counters had a inagnetic
shield, and the other had none, In the second launching, both
counters hag magnetic shields.. but the second counter was at an
angle of 15 towards the sun, recording non-solar radiation only,
Standard counters of type C 5 T 9 @SBT-9) viere used, The charac-
teristics of the counters are described. The cojn6ing rate @vas
calculated from the telemetered data, The 2 rockets were
launched on July 21, 1959, in the morning and evening respective-
ly. On that day, the solar activity was intense, Results: A
figure shows the dependence of the counting rate on altitude.
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A considerable X-ray flow was recorded from altitudes of 95 km
up. Owing to the stability of orientation of the container Y/ith
respect to the sun, it was unnecessary to make allowance for the
angular dependence of counter efficiency. From the counting-
rate data, the energy distribution and the magnitude of the
energy flux outside the atmosphere were calculated. The data
processing was based on the expression m inci @__ Mvert (z)
where mincl is the mass of an inclined air-column of 1 CM2
cross-section lying between the apparatus and the sun, m vert-_
the mass of a vertical column e@ual to -the atmospheric pressure
at the given altitude, and (@ Z) is determined by the zenith
angle of the sun z, A figure shows the counting rate as a
function of mincl* Assuming the spectral region under investi-
gation to be continuous, it is possible to construct the photon-
distribution curve by means of the counting-rate curves, the mass
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coefficients of absorption of air, and the spectral-sensitivity
curve of the counters, A figure shows the photon-distribution
curves as a function of wavelength. The energy distribution in
the morning and evening launchings was found to differ by a fac-
tor of 3. It is difficult to ascertain whether this difference
is real. The main source for the continuous radiation is elec-
tron bremostrahlung in the field of hydrogen and helium ions,
The obtained electron temperature considerably exceeded the
value of T e,--1 + 3 x 10 6 oK obtained in subsequent inveat:Lga--
tions by space-ships, A comparison of measurements condiicted by
Friedman (in 1953) during a minimum-period of solar activity
with the authors' measurements (in December 1960, by space-ship)
after a maximum-phase showed that the temperature and intensity
of radiation are greatiy dependent on the phase of the sun cycle,,
As the above-described rocket investigations were carried out
for very low positions of the sun above the horizon (in contra-
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distinction to Friedman's investigations), further systematic
measurements are required. In ensuing articles, the results of
measurements carried out on the 2nd and 3rd Sputnike will be
given, as well as a description of the electronic equipment,
There are 11 figures and 20 references: 8 Soviet-bloc and 12 non-
Soviet-bloc, The 4 most recent references to the English-language
publications read as follows: G. Elwert, J. Geophys. Res., 66,
391, 1961; H. Friedman, Trans. Intern. Astr. Un., 10, 706, 1960,
Cambridge Univ. Press; T. A. Chubb, H. Friedman, R. W. Kreplin,
J. Geophys. Res., 65, 1831, 1960; R. W. Champion, R. A. Minzner,
Plan.. and Space Science, 1, 259, 1959.
SUBMITTED: May 17, 1961
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3 . i'V5 0 _7032/El14
g, -1, /00
AUTHORS: Mandel'shtam. S.L., Tindo, I.P., Voron1ko, Yu.K.,
----------- - -7-
Vasillyev, B.N. and Shury.-in, A.I.
TITLE; Studies of solar X-ray emission. II
SOURCE: Akademiya nauk SSSR, Iskusstvennyye sputniki Zemli.
no.11. Moscow, 1961. Rezul'taty nauchnylch
I-ssledovaniy, provedennykh vo vremya poletov vtorogo
i tretlyego kosmicheskikh korabley-sputnikov, 3-14
TEXT: In a previous paper @Ref.l: Iskusstvennyye sputniki
Zemli, no.10, Izd-vo AN SSSR, 1961, p.12) the authors reported
MGasurements of the intensity of solar X-ray emission below 10
which were carried out with the aid of geophysical rockets. In
the present paper they report the corresponding results obtained
with the second and third Soviet spaceships on August 19-20 and
December 1-2, 1960. The aim of the measurements was to investi-
gate the intensity over an extended period of time(of the order
of a day or twol. Preliminary results have been given by the
authors in another paper (Ref.2: Dokl. AN SSSR, 14o, 1058, 1961).
The second spaceship carried six end-window photon counters
(15 m@&Lcm2 beryllium foils) with an oxygen-neon quenching mixture.
Card (1/ %)
,* 5/.160/6//a0e7/0/0/,0-V 2 /10" 4
Studies of solar X-ray emission.Il S/56o/61/ooo/oll/001/012
E032/E5i4
These counters were developed under the direction of 1. A. Prager
and S. M_ Perellman. The counters had a sensitivity of between
0.1 and 0.2 pulses/photon in the wavelength range 3-7.5 A. The
counters were mounted so that their axes were oriented along six
directions at equal angles to each other' the field of view of
each counter was 450. The telemetric record showing the counting
rate as a function of time is reproduced. It is estimated that
the flux of radiation in the range 2-10 A, which was recorded
durin the flare of August 19 (15 hr 33 min) was of the order of
-5 -2 -2 -1
7-10 - 1.5-10 erg cm sec The apparatus mounted on the
third spaceship was somewhat modified. Three types of probes were
employed so that tbp solar radiation below 10 4 could be
continuously monitoredtogether with interference due to radiation-
belt particles. The main detectors were two parallel-connected
C6 T-q (SBT-9) counters with mica windows (1.6 nig cm-2) and
located in a lead screen 1 mm thick. The counters were supplied
by solar batteries. In addition, there were two "control-
counters" which were mounted at right angles to the direction of
the sun. A tantalum plate was placed in front of the counter
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Studies of solar X-ray emission.II S/560/61/000/011/001/012
E032/F,5i4
windows and served as a target for the radiation-belt particles.
The counters were practically insensitive to solar X-ray radiation.
A third pair of counters was mounted on the outersurface of the
third spaceship. These counters were similar to those carried
by the second spaceship. The aim was to estimate the spectral
energy distribution by comparing the indications of the beryllium
and the mica counters. The telemetric record obtained with t
aid of the third spaceship is reproduced. It 4 is estimated t@at
the flux of radiation below 10 A was 2.5 .10- erg cm-2 sec-
Moreover, the intensity of radiation in this spectral region
remained constant within +20% during the observations. This was
due to the fact that on December 1-2, 1960 the sun was very
quiet and there was only one flare (importance 1+). The question
of the flux and the energy of the particles recorded in these
experiments is being examined at the present time. There are
10 figures and 2 tables.
SUBMITTED: June 26, 1961
Card 3/3
MAMELISHTAI-4, S.L.; NEDLER, V.V.
Sensitivity of emission spectrum analysis. OptA spektr. 10
no.3-.390-397 Mr 161. WIRA 14:8)
(Spectrum analysis)
-KOLMHUMOV9 V.G.; MZINGj M.A.; MMELISHTAM, S.L.0- MARASANGV, Yu*Po
Using a Fabry and Perot etalon for the study of line widths
in pulse discharge spectra. OptA spektr. 1.1 no-4-556-558 0
16L, (MIRA 1010)
(Electric discharges) (Scintillation spectrometry)
BAZHULINO P.A.;IfA LISHTAM, S.L.; STRIGANOV, A.R.
Conference on op$4co and spectroscopy,. Vest. AN SSSR 31 no.2:91-
@2 F 161. (MIRA 14:2)
(Optics-Congresses)