SCIENTIFIC ABSTRACT FISHKOVA, L.M. - FISHMAN, A.I.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000413310012-6
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 13, 2000
• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

FISEOVA, L. IAI.
USSR/Geophysics - Night Sky
21 Feb 50
IlInfrared Radiation of the 11orthern lights," S. F. Rodionov, L. M. Fishkova, Fhys Inst.,
Leningrad State U imeni A. A. Zhdanov
I'Dok Ak Nauk SSSRII Vol LXX, No 6, pp 1001-1003
Gives - results of measurements made in liar 49 of intensity of infrared and - green radiation
X'or northern lights of various,forms (diffuse., draperiesp arcs, etc.) and for ordinary
night-sky Iminescence. Measurements revealed radiaticn of northern lights in the
region 9jO00-10, 800 A was 20 -30 times intensity of strong green line (5,577 A).
Comparison with observations made on M Irt El I brus in sumer 1948 showed intensity of night-
sky luminescence at northern latitude (exact latitude rot given) is slightly greater
than at Mt Ellbrus. Submitted 26 Nov 49 by Acad A. A. Lebedev.
-40 PA 165T24

FISHKOVA, L. M.
"Distribution of Brightneis - of Hight-Sky Infrared Radiation over the Celwtial
Arch,* Dokl, AN SWRs 73, No-Is 1950

L -J~i
s7s,x. Ts, X'I it
11W 84ok" rimnlimwit I ,14 Rammi
blund fit d"Trm~ with ri.Int o.-stsp.
be at U071 late%-. t1b.- rataft.4 I at
tiseme 2 estrem temps. were fill, the kAntin fccquerwic.
7W-791. 430. 313. mod 217 CM.", f"P.. 3.1n. 2..'W$. ?~V.
mul 2.16. For W16. between 6 mul 70*. ftw :"*A) an.1 IMI
cut.". row.. 1.47 wW lAg. For "11.0. i of the Stokes
con'Posersts of the 2 timitma XW mul limM ",.-I mtwlnq~j
practically unchanIted between 22 ami 70% The intemity
of Ow undiGplard Um Inernmes vM newly Ixop)nkxwlly
to thr sbo, tems In CA, between ZY21' X. mind
Wt K., the rot 11th 1.11. The change ul d. Ito the
tetup. ft" In rOlpted 16 am% ion antAll lo ammut Pmr
the Sp., dr"" : " the varbiti,mi of i 4 Ott- Stokes mn.
j"Mrsts, old the role of the chance its so I% regligible. In
the tied of It* op. differences olorrie4 (,-r different Ite.
,Tencles wld Im dlfnrnt suberan(vi the elicting lhr,.ly
Y of the Stolim and ajjt~stokfA ertillpoll'.111% ,I
114ments cmid OPPcerl InadeqUAtt. "C jjjjtj.St,)kv, j,"11.
be nwimifed. N.

USSR/Geophysics
Card 1/1 Pub 22 -19/44
Authors s Rodionov, S. F.;-Pavlova, B. N.; Sholokhava, B, D,; and Fishkwmp -L#;..
Title t Yearly variations of infrared radiation cf the night sky
Periodical s Dok. AN SSSR 98/6, 957-960, October 21, 1954
Abstract t The results of experiments with infrared radiation of the night sky,9'
conducted on Mount Elbrud during 1948-3-9!3, ars presented. Four Rassian
references (1948--1951). Graphs.
Inatitution Leningrad State Univers#y im. A. A. Zhd&nov; Mbrus Complex Scientific
Expedition of.thqAcad. of Scs. of the U14GR
Presented by: Academician V. 0. Fesenkov.,*April 19 195k

FISHKOVA, L.K.-. CEWHA q Sh*N.
AnoL.alous sunrises and mmsets in August and Septeuber, 1953.
Astronstair. no.146:18-19 Jr 154. (MM 7:6)
1. Abastumanakaya antrofisichaskeya observatorlya, Gora. Kanobili.
(Stm-Rising and setting)

FISHKOVA, L. M.
Seasonal Variations of the Intensity of Light Sky Luminescence.
Almdemiya Nauk Gruzinskoy SSR. Soobshcherdya, 1.955, V- 16, no. 9, p 681-686.

PISHKOVA, L.M.
----Variations of Intensity of nocturnal sky luminosity in the
near infrared region. Blul. Abast. astrofts. obser. no.19:
3-23 '55. NEaA 9:12)
(Atmosphere, Upper) (Might sky) (Spectrum, Infrared)
I

SOV/169-59-4-4209
Translation from: Referativnyy zhurnal, Geofizika, 1959, Nr 4, P 139 (USSR)
AUTHORS: Megrelishvili, T.G., Fishkovj,_ L.M.
TITLE: On the Investigation of the Upper Atmosphere Glow
PERIODICAL- Mezhdunar. geofiz. god, Inform, by-ul., 1958, Nr 5, pp 43 - 44
ABSTRACT- The authors report on electrophotometri:! and spectrographic
observations of theliglow of the night aid twilight sky, which
were performed by the Abstumanskaya astrofizicheskaya observa-
toriya AN Or-azSSR (Abastumani Astro&sical Obseriatory of the
AS GruzSSR) in accordance with the IGY program. There are
brief descriptions of -the devices with which the aforementioned
investigations were performed. The b6sic purpose of the spectro-
graphic observations during the IGY was the discovery of lines in
the night sky spectrum, belonging to the spectra of the warora
polaris occurring in low latitudes during In-,ense geomagnetic
disturbances, especially in years with maxiffram solar activity.
Card 1/1 Lj. 0

sov/58-59-9-21566
Translaiion from: Referativnyy Zhurnal Fizika, 1959, Nr 9, pp 303 - 304 (USSR)
AUTHORS- Dolidze, M.V., Fishkova, L.M.
TITLE; An Auxiliary Device for the "mF-4" Automatic Recording Microphotometer
PERIODICAL: Abastumanis astropizikur.i observatoria. Bluleteni, Byul. Abastumansk.
astrofiz. observ., 1958, Nr 22, PP 117 - 3.24 (English r6sumQ
ABSTRACT: The attachment is a combination of a photoeleotric-6ptical converter
for transforming optical blackenirgdensities into intensity and a-photo-
electric planimeter. A uniformly illuminated slit of the "UF-l" type
is projected onto a spherical mirror at whose focal point photocell PC2
is located. The mirror of an auxiliary giLlvanometer G2, attached to
photocell PC1 of the microphotometer, senres as one of the elements of
the projecting optical system. The galvanometer of the microphotometer
is used to record the current of PC2. Wedge-shaped diaphragms D, having
the form of the characteristic curves of the given photographic material
for certain wavelengths, are placed in the plane of the spherical mirror.
As the current of PC, varies, galvanometer G 2 deflects the image of the
Card 1/2 slit onto D, which is so set that its narrowest opening corresponds to

sov/58-59-9-21566
An Auxiliary Device for the "MF-4" Automatic Recording Microphotometer
the background of the plate. The necessary angle of deflection of the image of the
slit Is achieved by varying the incandescence of the tube and the width of the slit in
the INF-411. In order to measure the areas, a collimator, consisting of an objective
and a uniformly illuminated round diaphragm, is placed ort the axis of the ray reflected
from the mirror of G2. Diaphragm D is taken down, and Irt its stead a diaphragm is
placed which has the form of the area being measured. Readings of the areas are taken
from the visual dials of the "MF-4". The attachment is used In processing stellar
spectra,
Yu.M. Kutev
Card 2/2

FISHKOVA. L.M.; MARKOVA. G.V.
-
Blectrophotometric observations of low-latitude aurora borealis
of-February 11-12, 1958. in Abastumani. Astron. tair. no.191:
28-29 My 158. (MIRA 11:9)
1. Abastumanskaya astroftsicbeskaya observatoriya AN GruzSSR.
(Auroras)

FISHKOVA, L.; MARKOVA, G.
The R line in the luminescence spoctrDm of the night sky.
Aatron. tair. no.196-.8-9 0 '58. VIRA 12:12)
l.Abastilmanakara astrofizichooksqa observatoriya AN Gruzinsko7 SSR.
Mght o'ky--Spectra)

FISHMVA, L.M.
Checking the transparence constancy of night sky lunineecence.
Meshdunar.geofiz.god no-7:68-69 '59. (KM 132-2)
(Night sky)

88827
Translation from- Referativnyy zhurnal,
P. 57, # 2A470
S/035/61/000/002/012/016
AOO1/AOO1
Astronomlya I Geodeziya, 1961, No. 2,
AUTHORS: Fkabkova, T.-M-, Markova, G.V.
TITLE: Some Results of Electrophotometrical Observations of Emissions of
01, Na, OH and Continuous Background in the Night Sky Glow
PERIODICAL: "Byul. Abastumanak. astrofiz. observ.", 1959, No. 24, pp. 161-173
(Engl. summary)
TEXT: The authors determined absolute intensities of emissionskk5577,
6300, 5890 and continuous background at AX5290, 5730, 6060, and also summary
intensities of infrared bands OH (8,4), (3,0), (9,5) and (4,1) from observational
data for the period from July 1957 to June 1958. 'They present the curves of
daily and seasonal variations in intensity of these emissions. They notothat
daily vAriations of OH intensity have a minimum at mid-night and maximum between
2 and 4 of local time, the maximum of A 5577 leads the maximum of OH by 2-3 hours.
Daily variations In intensities of bands OH and X 5577 have always reverse course.
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88827
S/035/61/000/002/012/016
AOO1/AOO1
Some Results of Electrophotometrical Observations of' Emissions of 01, Na, OH and
Continuous Background in the Night Sky Olow
The mean intensity of continuous background at X 52,cO in the polar zone ~510)
equal:s 2.5 R/A after excluding stellar and zodiacal components which are equal
to 0.4 R/A. Three types of intensity variations of background atX5290 are noted:
1) background variation does not correlate with any emission; 2) background
variation correlates with A 5577; 3) background variation correlates with OH,
mainly at high OH intensities. Seasonal variations of background intensity have
two maxima: major one in January, and minor one in July. It is assumed that con-
tinuous background consists of three components of the proper atmosphere emission
in continuous spectrum; it does not correlate with emissions in bands and lines
and produces January maximum of forbidden molecular bands of scattered Sun's
light. There are 18 references.
N. Shefov
Translator's note: This is the full translation of -the original Russian abstract.
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31 jel
AUTHORSt Fishkova,- L.M.; Markova, O*V.
28839 3/169/61/000/004/020/026
A005/A130
TITLE: Some results of electrophotometric and spectrographic observations
of night-sky glow at Abastumani
PERIODICALt Referativnyy zhurnal. Geofizika, no. 4, 1961, 4o, abstract 4 0 298.
[V sb.t Spektr., elektrofotometr..i radiolokats. issled. polyarn.
siyanly i svecheniya 4ochnogo neba, no. 2 - 3. Moscow, AN SSSR,
1960, 49 - 56 (English summary)]
TEXT: The authors give a brief account of the nxin results of electropho-
tometric observations of diurnal and seasunal variations in the intensities of.
the X 5,577 [011, X 6,300 - 6,364 [011 and Na night-sky emissions, the continuous
emission and the OH bands in the range A 7.9,000 - 10,550 A; the observations
were carried out by the Abastumanskaya Observatoriya All Gruzinskoy SSR (Abastu-
mani Observatory of the Academy of Sciences of the Gruzinskaya SSR) during the
IGY (see ab6tract 4 0 297). In addition, data are givon on variations in the in-
tensity of Hd emission in the glow spectrum of the night sky according to spec-
trographic observations conducted during the same time. A record is presented of
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8/169/61/000/004/020/026
Some results of electrophotometric and .... A005/A130
the night-sky glow spectrum in thl X 3,000 - 4,000 A range showing bands of the
02 Herzberg system, the X 3,qi4 N2 band and three unidontified bands in the 3,700
- 3,800 ~ range.
Author's summary
[Abstracter's note: Complete translation.]
X
Card 2/2

8736o
S/035/60/000/012/018/019
00 ell A001/A001
Translation from: Referativnyy zhurnal, Astronomiya I Geodeziya, 1960, No. 12,
p. 61, # 12345
AUTHORS: _?ishkova, L. M., Markova, G. V.
TITLE: ;On Variations in Intensity of the HOG Line in the Nocturnal Airglow
Spectrum
PERIODICAL: Astron. tsirkulyar, 1960, yanv. 30, No. 208, pp. 14-15
TEXT: Observations of emission % %6562 ia the spectrum of nocturnal air-
glow were continued in 1959. The following preliminary results have been obtained.-
the intensity of Hot, in direction z - 67cN attained the maximum magnitude in June-
August, both in 1958 and 1959; the intensity of HI varies from night to night
analogously to variations of OH band Intensities, but the amplitude of variations
Is twice as small as the amplitude of OH band variation; the ratio of intensity in
direction z = 70 0 to that in direction z = 200 aniounts to 1.73 � 0.14 for Hc~, and
to 2.50 � 0.40 for OH. Attempts are made to explain the peculiarities of varia-
tions of the HQ~intensity. There are 5 referencos. N. P. Kukarkina
Translatorls note: This is the full translation of the original Russian abstract.
Card 1/1

846834
S/020/60/1-34/004/007/023
3, aao ~Iivl, / o 6 4 B019/BO67
AUTHORSj Fishkova, L. M. and Markova, G. V,
TITLEa On Intensity Variations of the 6526 HI Line in the Night
Airglow Spectrum
\V- -:: --- - -
PERIODICAL. Doklady Akademli nauk SSSR, 1960, Vol, 134, No. 4,
PP- 799 - 801
TEXT: From 1958 to 1959 systematic observations of the night airglow
spectrum in the region of from 5400 to 6700 A were made at the observatory
mentioned under the 'Association. The pictures were -,aken on a panchromatic
film by means of a diffraction spectrograph of the typekCff-48 (SP-48) with
a power of 1 s 0.8, a dispersion of approximately 85 L11m, ~-nd an aperture
of 3.5 A. 40 spectra were obtained during moonless nights on the almucantar
at a zenith distance of 67 off. Fig. I graphically shows the seasonal
intensity variations of the Ha line (Curve 1) and, for oompariaon, the
lines P2 with 6554 A of hydroxyl (Curve 2). Curve 3 shows the variations
in the OH band intensity in the region of from 9,400 to '10,550 A. As may be
Card 1/4

On Intensity Variations of the 6526 HI Line S/020/60/134/004/007/023
.in the Night Airglow Spectrum B019/BO67
seen; the Ha lines attain their maximum intensity in July of each year,
the hydroxyl lines have their maximum intensity in November - December.
Emission line 5577 A reaches its maximum intensity in October, and lines
5893 A and 6300 A have their maximum in winter and their minimum in summer.
Thus, the intensity variation of the atomic hydrogen differs from seasonal
variations of other lines. For nine nights the spect:rum was photographed
in the two zenith distances 20 0S and 70 0N and the ratio 1 70 /,20 ' rH was
measured. The similar relations r OF for the hands P 2(6-1), Q(6-1).. and
Q(9-3) were determined. The ratio of the Ha lines, obtained as a mean
value from a large number of measurements was fcund to be 1,73 0,14;
that of hydroxyl was 2.40 + 0.40. The variability of the Ra nn7e
intensity is obviously inffuenced by star and ga.laxy atomic hydrogen
radiation. During the measurements celestial W-,ies emitting the Ha line
did not pass through the telescope field. The 9ummer maximum of the Ha
li.ne intensity cannot be explained by external Influences. The authors
a9sume that the summer maximum of the Ha line intensity is oonnected with
the solar counto4rpoint position which is shifted by 400 from the observa-
tion point in summer. However, rockets measured the Lyman lines at
Card 2/4

---On- Intens-ity---Variations-of-the-6526-HI-Li-re--- ---S/020/"--0/134-/004/007/(Z~23-
in the Night Airglow Spectrum B019/BO67 8-~jv
_3
altitudes of 85 to.120.km as earth's atmosphere e Imission with an albedo'of
0.42. Assuming that an Ha component exists in this emission, the quantity
of Ha emission measured on theearth's surface is about 1/3 of the.total
emission. In the authors' opinion the ratio of the hydroxyl emission agrees :
with the measurement data. According to the au--,hors large amounts of
neutral hydrogen are found up to altitudes of 135 - 120 km, OH up to
7U - 120 km. Furthermore# fluctuations of the ~3olar activity influene e
the intensity of the Ha line. There are I figuxe, 1 table, and
12 referencess 8 Soviet, 2 US, 1 German, and 1 Czech.
ASSOCIATION:, Abastumanskaya astrofizicheskaya observatoriya Akademii nauk
GruzSSR-(Abastumani Astrophysical Observatory of the Academy~
of Sciences Gruzins~aya SSR3
PRESENTEDt may 19, 196o, by A. N. Terenin, Academician
SUBMITTED: May 12, 196o
Card 3/4

50'
40
10
Card 4/4
S/020/60/134/004/007/023
Doig/Bo67
Ta6jviiua I
Da a
ON

Q

51-M VI 1,V5 2,32 3,31 2,68

1-2 VII 1,52 1,77 1,83 2,06
2-3 VII 1.59 2.76 3A) 2,W
13-14 VII t,60 t,87 2.44
2-3 VVI i , sl2i 2, 14 2,14 3,09
21-:0.) VIII tAR
I 3.11) 2.35 3A5
ean

30 --- 11 x 0,70 2,11,
V.1511 r.
'2-3 X11 90 2,41)
--N 111 2,80 2). 1 u
2,30
Ze an
pexl~ 2135 2167 2,30

3,1810
3/169/62/000/004/096/103
D290/D3O2
AUTHORS: Fishkovat L.M.t and Markova, G.V.
TITLE; The OH emission at Abastumar.
PERIODICAL: Referativnyy zhurnal. Geofizikat no. 49 1962, 25-26p
abstract4G149 (V sb. Spektr. elektrofotometr. i radio-
lokats. issled. polyarn. si2raniy i svecheniya nochn.
nebao, no. 6, M.p AN SSSR, 1961p 17-20)
TEXT: 1,1easurements of the nightglow spectra were made at the
Abastuman observatory during the IGY; a_:,n -48 (SP-48) spectrograph
was used. The OH emission between 6100 6700 A was measured. The
rotational temperature (T) of the Oil bands was determined from the
P branch of the (9-3) band, using an equation due to Hill and van
Vleck. The logarithm of the intensity of the (903) band (I) was
plotted a~;ainst 1/T. It was found -that I varied with T only if T:--
~-, 2500K i. e. in winter); I was independent of T if T -.:::: 2500K (i.e.
in summer . The seasonal variations of I and T were measured from
January, 1958 to Septemberp 1959. 1 and T vary appreciably from
night to night, and have similar mean seasonal variations with ma-
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S/169/62/000/004/096/103
The OH emission at Abastuman D290/D302
xima in November-December. T has a distinct winter maximum and sum-
mer minimum. The mean T was 225 � 100K, Emd the mean I was 160 rily-
leighs between January, 1958 and September, 1959. It was observed
that the intensities of the Ha and OH P2 (6-1) emissions were cor-
related. [Abstractorts note: Complete translation].
Card 2/2

DOLIDZE, M.V.; MAZNYY, M.F.;_LISHKOYA L.IL.
Deterinining the zero-point of spectrophotometric temperatures.
Biul.Abast.astrofiz.obser. no.26tl61-167 161. (MM 15:3)
.(Spectrophotometry)

ACCESSION NR: AT3012981 3/2501/62/000/029/0055/0076
AUTHOR: Fishkovap L. H
TITLEt OH rotational temperature ot.the upper atmosphere
SOURCE: Abastumani* Astrofizich, Byul.; no. 29., 1962.
Issledovaniya po programme HGG i mezhdunarod. geofiz. sotrudnichestva, 55-76
TOPIC TAGS3 rotational temperature,, OH rotational tem-oerature, upper atmosphere,,
airglow., OH band intensity., activation energy., geomagnatic disturbance,, aurora,
molecular excitation
ABSTR&CT: This paper is based on spectral observations of airglow in the range
5400-7000 A., made at the Abastumani Astrophysical Observatory during 1958-60.
The OH rotational temperature (TOH) of the upper atmosphere was measured on 106
different nights. The mean value of TOH for Abastumard is 246 + 16K. Seasonal
variations were observed, with a maximum in November-DeoGmber, i minimum in
summer,, and a variation of about 75K. The variations are shown in Fig. 1 on the
,.F4closurea. The mean values of TQH at Abastumani are near those for the sam
periods measured at higher latitudis. For a rotational temperature above 250K,,
Card 115

ACCE=ON NR: AT301461
the dependence of OH band intensity on teVerature, expressed as dependence of
log 3~, on UP R, is approximately linear,, and the ;slope of the averaged straight
line correspo;Ss to an activation energy of 2,2 + 0,8 kcal/mo:Le. ..This reutionship
is shown in Fig, 2 on the Enclosures. The valui-is close to the activation energy
of the 03-H reaction. When the rotational temperature iv below 250K$ -TOH does not
depend on T and this is more suggestive of the 4i;mechanism of OH-molecule
excitation.
0%r rotational temperatures below 270K, the value obtained from the
(9-3) band is the same as that from the (6-1) band, but when the value is above
270Ks the latter is less than the former,, and the difference may be as muoh as
40K, The ratio of intensities for these two bands does not depend on TOH. it
decreased continuously during the period of observation, from 2.0 in 1953 to 0.8
in the summer of 1959. During large geomagnatic disturbances followed by auroral
displays in low latitudes., T increases anomalously to vaL-es greater than 300K,
OH
and this is followed by an anomalous decrease in intensities of the OH bands. The
author concludes that the seasoaal variations in kH and ToH and their anomalous
variations during large geomagnetic disturbances may be due to powerful vibrational
~motion'9 of the upper atmosphere ronowed by vertical displacements of emission
layers, Origo art& ban; .9 figures, 6 tablesj and 15 formulas.
Card 215

ACCESSION NR: AT3012981
ASSOCIATION: Astrofizich. observatozdya, Abastumani (Astrophysical Obser'vatory)
SUBMITTMi 00 DATE AGO 150at63 ENCL: 02
'ER:
50 CODR3 PHs AS NO REF SM 018 OM 009
Card 3/5

ACCESSION NRs AT3022982 4/25OV62/000/029/0077/009~
AUTHOR: Fishkova, Le Me
TITLE: Variations in intensity and three dimensional distribution of 6$62
emis3ion in ni&t &U'S)AW
SOUrCE: Abastumani. Aqtrofiziche observatoriya. Byul., no. 29 1962.
Isslodovan1ya. po programme HDG i mozhdunarod. geofix* sotrudaichostva, 77-91
TOPIC TAGS:. night air glow., spectrography, galactic contamination,, bydrogen,
telluric. corona
ABSTRACT I Results of apectrographic observation or H,,e emission in night airglow
at the Abastri-akaya astrofisicheskaya observatoriya (Abastumani Astrophysical
Observatory) for 1956-61 are reported. Seasonal variations in the intensity of
Hc>e. for the direction 670H show a mWolm in July aad a lesser maximum in March
for each of the four years., though the March maximma is not usually so well defined
or consistent, Only in polar regions is the July iwdalm obsirved. The March
submmimm is dae to galwbic contudnation, Ths 11 n dwbUt of th4 X6583
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ACCESSION NAt AT3022962
line began to appear with increasing Hcs< The g&Lwtic paft of the emission was
measured by conoaring siniltansou roKUngs at the given direction and In the
polar region. The effects observed are due to resoiwnce scattering of solar Lyman
radiation by neutral bydrogen atom in the te22uric corona and in the upper
atmospheres The seasonal variations of Ho< with ammer awd-im are related to
seasonal variation in height of the earth's shaAaw Jn the direction of observation.
Comparison of the seasonal H., curve with data on h3,drogen concentration in the
telluric corona above the edge of the shadow shows the amplitudes of both
distributions to be sindla , The intensity ratio 1,,l /]:.2 was obtained for
several,
directions., and the values are tabulated* Orig. art, but 5 figures and 2 tab2as.
ASSOCIATION: Abastummzd* Astroftsich* observatorlya, (Abastumni Astrop4yeical
i Observatory)
WBMITM O0Apr62 DATE ACQs 1.50at63 EWLv 00
SUB CODEt A4 ES NO 1UW SOV a al 0THM# 009
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KALANDAD2E, N.B.; SALUKVADZE, G.N.,- f~qYA, L.M.
Relative transmittance of the objective of the 40cm. refractor and
of the correcting lens for the 36c'm. Schmidt telescope of the
Abastumani Astrophysical Observatory. Blul. Abast. astrofiz. obser.
no.28:205-207 162. (MIRA 16:7)
(Abastumani astrophysical observatory)

ACCESSION MR: AT4034380 S/Z66$31000010/0035/0039
AUTHORt FishkoY*,_1#,_H.
TITLE: Tht spatial distribution and vikiriations of H outs Alpha emission in this
nightglow
SqURCE; AN SSSR. Mezhduvedomstvanny*y geofiniebookiy komitat. IV razdal
pr6grammy* MGG: Polyarny*ye #iyaniya i avecheniya nocbnc-go neba. Sbornik statey,
no. 10, 1963, 35-39
TOPIC TAGS: meteorology, geophysics, aurora, nightglow, atmospheric emission, hydro-
gen emission, H sub Alpha emission, seasonal nightglow variation
ABSTRACT: The article deals with spectrographic observations carried out during
1958 - 1961 at the Abastumanskaya astrofizicheskaya observatoriya (Abastil-ni
Astrophysical Observatory) in terms of the determination of the absolute intensity,
seasonal variations and spatial distribution of HA emission in the nightslow.
The spectra were photographed on an SP-48 spectrograph of high light admittance
vith a basie*direction of observations Z = 670 N. A total of 115 different spectra
of the night sky were obtained and processed. An annual repetition for four years
of a maximum IH.( in July was observed, with a second maximum noted in March. A
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ACCESSION NR: AT4034380
seasonal variation curve in given, MiLch indicates, again averaged out for the en-
tire four-year period, a change of from 5 - 7 rayleighs in the winter to 20 - 25
rayleighs in the summer. The March v=imum in the direction 670 N is explained by
the imposition of the galactic component. An attempt is; also made to explain the
marked summer maximum, and it is pointed out that in the spectrograms of the Sumer
period with intensive P6( emission there are no traces of the N11 line. In order
to study the intensity distribution over the vault of the heavens, during a number
of nights spectrographic observations were made in two directions simultaneously
(Z = 700 N and Z =200 S); the author gives the result as 170N I= 1.73 * 0.14.
120S
Beginning in July of 1961, observations were carried out simultaneously on two
SP-48 spectrographs, one of which was directed at point Z -- 670 N and the other
either at the Pole (Z2 = 480 N) or southward in the direchon of the antisolar
point. Measurements were conducted of the intensity ratio Tz /]:z2 in both-directione
for the line Hok (rH,,) and the line P2 (6. 1) OH (z.OH). A tabie of results is given.'
Cases were clearly evident in which rB.4 was distorted ky the galactic component*
The ratio of the H intensity in the direction 670 N to the Hak. intensity at the
Pole for all the n4bite indicated in the table from July through January remained
approximately constant. In July& when maximum H#A. was observed in the direction
Card 2/3.

ACCESSION NR: AT4034380
67o N, 11,A was also intensive at the Pole. Since, in the region of the Pole, the
stellar component does not change in the course of a year, the constancy of the
ratio X67/1 8 serves as proof that the Hor. summer maximum is not the result of the
influence o~ the galactic component. The mean value of 167 = 1.4 f* 0.1. The
M
correction factor for the exclusion of the galactic coaq)onent is - 1.7. This value
was used to correct the 1H0% values in March-April, an neasured in the direction
670 Np with the result that the March maximum disappearad. Observations in the
antisolar direction showed that as the antisolar point Ls approached, the intensity
of He. emission decreases and is minimal at the antisolar point. In the view of
the author, the seasonal variations in Ho-. intensity obuerved at Abastumani and its
space distribution are beat explained by the appearance of Hoo. in the nightglow
spectrum as the result of the resonance scattering of solar radiation in the lines
of the Lyman series in the neutral hydrogen of the geocarona and upper terrestrial
atmosphere, Orig. art, has: 1 table and 4 figures.
ASSOCIATION: Mezhduvedometvenny*y geofixicheskiy komitet AN SSSR (Interdepartmental
Geophysics Committee, AN SSG&)
SUB R : 00 DATE ACQt 12uy64 HNGL; 00
SUB CODS: ES NO REF SOVt 003 OTHERi 003
Card 3/3

FISHKOVA L. M.
"R Emission in the Airglow."
report presented at the 13th Gen Asseubly IUGG, Berieley, Calif, 19-31 Aug 63.

FISHKOVAY L.M..; MARTSVAIADZE) N.Me
Distribution of hydrogen in the upper atmosphere and terrestrial
corona. Astron. tsir. no* 253:1-4 J1 163. (MIRA 17:5)
1. Abastumanskaya astrofizicheskaya observatoriya AN Gnizinskoy
SSR*

Is 11 K OVA) t4l
AID P 5070
Subject USSR/Engineering-welding
Card 1/1 Pub. 107-a - 10/11
Authors Lomakin, V. I. and N. I. Fishkova
Title : The SL-60A electric rive
Periodical : 3var. proizv., 6, 31-32, Je :1956
Abstract ; The authors describe the SL-60A electric riveter designi.-
ed for welding sheet metal and structural steel of 2 to
5 mm thick. The riveter's technical characteristics and
Its design, the complete installation and its performance
are presented. Three drawings, 1 photo and 1 table.
Institution : None
Subsitted : No date

AUTHDRs F1sWwft* NA. 32-11-3.V60
TITIJs Short Reports (II) (KoroUlys soobehoheniya)
PMRIODICAL% Zavodskaya. Laboratoriya, 1957, VOL 23, *Mr 11, PP- 1360-1361 (USSR)
ABSTIMi In this paper the application of speotrconalysis for the determination
of the sauminim and mqpnium oontent isk a sino distillate is rs-
oommetWeds In order to create the necesuary oonditions for spectral
analysis and for the oonstruotion of the oorresponaing graduation
diagram synthetio standard samples wort used# which had been prauosd
from a repeatedV checked alloy Zn-Al-*& with a Os 35% aluminta oon-
tent and a 0,4* magnesium oontext. Thus, the standards had an alu-
4nu- oontent of Otis 0.05, 0.02 and 0.101% ands oorrespondinglyo a
WALSMOSiUM OVAIOnt of O.u, o.o6, o.o24 ana m12%. A speatrogmph
9 -22" with 3-stage reducier, a generator " -1" with omtact
breakers and a stiorophotonstier "X -2" were used; ignition oVerage
me 0.1 A. aistanot along the arc 2.5 vat &31-k of the sp*otzvgmpb
0,025 mat and the film used were of the "Spektralluyye" tMe 1.
The possibility of reproducing the resiats determined was within the
Card 1/2 limits of the oontentst 0.005-0.2% alwAnuz and 0.001-0.2% magnesium.

Short Reports (II) 32-11-3V6O
1
% I
AMMUTIM: PodoUk' Plant for Metals (Pcdollskiy savad vtorldbafth
mullow)
ATAIWLIs .%, Library of Congmes
card W2

t- I -S r)aiv
R

FISHK,q~t_A~_L~ ICKLIT. L.N.
Spectrum analysto,of potassium. calcium. and sodium chlorides
in flux salts* Zav.lab, 26 no-5:566-567 160- (KIRA 13:7)
1e Podollakly sayod vtorichnykh tevetnykh metallov.
(Potassium chloride-4peatra) (Calcium ebloride-Spectra)
(Salt--Spectra)

PISHKOVA, S. M.
USSR/Geophysics - Radiation, Infrared Night Sky 3. Jul 50
*Distribution of Brightness of Right-Sky rmfrarvd Rediation Over the Celestial
Arch, 0 Ye. N. Pavlons S. F. Rodiamys, M, S. Sominskiy, S. M. Fishkova,, Phys
Inst., Leningrad State U imeni A. A. Zhdanov,, and Ht Ellbras Expedition of Aced
Sci USSR
*Dok Ak-Nauk SSSRP Vol LXXIII,, No 1. pp 69-72
Infrared -81 reamto of night MW in fall 19/+9 on Mt E1111rus (2t200 and 4,200 a elevation)
using photometers with secondary-electron electrostatic tubs. Confirmed infrared radiatiom
maximum, at midnight. Found intensities of 1.12 x 10-2 and 3-07 x 10-2 erg/aq cm see otered,,
respectively, for heights of 2,200 and /+,,200 m. Found rad1ating layer to be 900 km high.
Submitted 4 May 50 by Aced A. A. Lebedev.
166T29

24.2ooo 77304
SOV/57-30-2-1/18
AUTHORS: Kellman, V. M., Yavor, S. Ya., Fi
TITLE: Achromatic Marnetic Mirrors
PERIODICALi Zhurnal tekhnicheskoy fiziki, 1960, Vol 30, Nr 2,
pp .129-137 (USSR)
ABSTRACT: To achieve a deflection or d1splacement of non-
monochromatic beams of charged particles without sep-
arating them according to energy, Kellman and Lyubimov
(Izv. AN SSSit, ser. f iz. p 18, 155, 1954) used a _,kag-
netic mirror viliose marfnetic -ield vector potential A
satisfies the equation:
A Re [- 4:0 (y A., =-- A.,,= 0,
where H and Ic are constants. For a 1)articular choice
Card 1/13 of k, oRe can find an angle CL, for the incoming

Achromatic Magnetic Mirrors 77304'
SOV/57 -30-2-1/18
particles, such that all parlu-icles of various energies
entering 'the field at that a:.-igle in t'ne central plane
describe similar trajectorie,3 and emerge out of the
field at the point of entrari4-,e as a single be,-~-,m
(see Fig 1).
y
Fig. 1. Similar trajectories in an
achromatic magnetic mirror. CLO)
C:)
an-le of Incidence; lal) angle of
CD
reflection.
Card 2/13

Achromatic Magnetic Mirrors 77304
SOV/57-30-2-1/18
In addition to checking the known values of CL 0 for
Ic ='l and Ic = 2, the authors of this Raper evaluated
the necessary k's for angles CLO = 30 and CLO = 450.
Mirrors with OL -_ 30 0 angles arranged along sides of
an equilateral triangle or mirrors with CLO = 450
forming a parallelogram could.then be used to maintain
closed trajectories of particles. The authors start
from the solution ofthe differential eQuation of
motion for charged particles in the central plane
of a two-dimensional magnetic field, which for the
initial conditions x. Yo = 0 has the f=ii:
eHn In all
x ?;ICU dy. (5)
Sill a)
~k
Card 3/ 13

Achr6matic Magnetic Mirrors 773011
SOV/57-30-2-1/18
Here e, m, and v are charge, mass, and velocity,
respectively, of the particle; c is veloc4ty of light;
ni
M 0 where m0 is rest mass of the particle.
Yl _2
_v /c2
In the central plane (z = 0) the field has, the value:
II. = HY = 0, 11, = lid`, (4)
where k can take integer and fractional values. Using
the known values for k versus CLO: Ic = 1, CLO = 900;
Ic = 2, a0 = 400; and Ic = 3, ao 7- 280, the authors
constructed an approximate curve k = k(ao ). Choosing
approximate k values, they calculated curves by per-
forming numerical integration of Eq. (5). Typical
curves are Wesen-.ed on Fig. 3. From the form of the
Card 11/13 curve they could decide If k should be increased or
decreased to obtain the desired correct Curve.

Aciiromatt Magnetic Mirrors
Card 5/13
I,
4J.
J
77304
SOV/57-30-2-i/18
Fig. 3. -Trajectory of charged particles in the
central plane of the mirror, with Ic = 2.75 at In-
cidence angles of' 28, 30, and 320.

Achroniat-LIMa--netIc M.Lx,.r,oi,z3
77304
SOV/57-30-2-1/18
The results O-r CRlCLIIationo are coritalned in Table A.
Ta 1) 1 e A . (a) Initial conditictil,; (b) data obtained
by iii-mievIcal IntegratIon of system of Eqo. (7);
I.
da (' a obt,-Llned by tIItfI1rUr].C',0- ILIP,)~' 111's
,Eq. (10); (d) degrees.
Card 6/ 13
c
N. 7. .1. Y$

2 40.7 3 0 46.2 -7.4 --0.71 1.88
2 40.7 0 2.00 36.6 -2 * 6 0.76 -1.12
3 27.6 3 0 29.0 4.0 --0.61 1.67
3 27.6 0 1.00 28.0 -1.7 -1.18 1.90
1.81 45 3 0 51.7 -9.2 --0.8.1 2.01 -5.4 2.08
1.81 45 1 2.1 ,
~ 1-1 -
1
-4 110 -1.92 -2.6 -2.58
2.75 30 3 2 .
0
9 --0.67 1.68 8.2 1.82
2.75 30 0 0 .50 2,9-5 2.4 --0 '26 1.08 4.4 1.17
2.75 30 0 2.00 27.7 -4.2 ---0.58 -0 .03 17.0 4.67

Achromatic Magnetic Mirrors
773011
SOV/57-30-2-1/18
This table contains also data about trajectories not
lying in the central plane, obtained by two methods.
0
One is by numerically integrating the exact syqtem
of equations of motion:
k '0"; (k are tg
d2y 0110
(Y2 -I- Z') Y Cos (L are tg -i- z sill k are tg.L X
Him
X [C _f_ !yl -1- .2) C,)S
(k are tg
k Y
d-tz ell
7_ -I (y2 _#_ Z2 Y Sill (k are tg z Cos (k arc tg
5'. "ICv F
C -4- eflu (Y'2 -- =2) 2CW; karctg
X incv k
(7)
Card 7/ 13

Achromatic Magnetic Mirrors 773011
SOV/57-30-2-1/18
where s is length of path traveled by the particle,
C is a constant which is a ..unction oo initial
conditions. The other is by inteLgratin,,-, the
approximate equation by Khu:?gin:
d2z It k - I qk_j)
= 171-'0) ~L-` (k - I)y"sin a,, r. (10)
T.2 [("Ov _k Y
denotes the angle between the XY plane and initial
PzRicle direction for particles starting In the central
plane (see Fig. 6);' z is the initial distancefrom the..
0
XY plane.tcr particles enter1n7 the field parallel to
the XY plane; yi Is the angle between direction of the
exit of the particle and the central plane; OLI is the
angle between the projection of that direction in the XY
-plane and the negative Y axis d1rection. In all
g ~10
Card 8/13 cases the quantity jF-c-v was equal to 0.04 per cm

AchromatIc Magnetic Mirrors 77304
SOV/57-30-2-1/18
Figure 6 repre3ents an interesting case where a parti-
cle entering the field parallel to the central lane
comes out again parallel to that plane (curve 2~.
A field with such a special k value can then be used
for displacement of parallel beams of particles with
various energies.
Card 9/ 13

cm
1 3 J 6
Y'C
...........
to
Cm
Cm
Card 10/13
X, Col
-104
7-)
7
SOIT/57-30-2-1/18
Fig. 6
(caption on
next card)

Achromatic~ Magnetic Mirrors 773o4
SOV/57-30-2-1/18
Caption to Fig. 6.
Fig. 6. Projections on YZ and X~( planes of two
space trajectories in a field with k 1.81. Initial
conditionst trajectory (1)1 X0 = Yo zo = 0,
GLO = 450.9 -/. =030; trajectory (2): x0 = yo = 0, z0
= 2 emp CLO := 45, 1/0 ~ 0 . Crosses indicate
trajectories w1th the same~initial conditions, but
computed using the method of Khurgin.
Gaing a method described by Kellman and Lyubimov,, the
authors constructed a field for k = 1.81, and its values
agreed fairly well with Eq, (4). Rirther improvements
were obtained by means of additional windings on
the shielding and the magne, ~ laminas. The authors
Card 1l/ 13 point out that one can obta.1ii the desired result,

Achromatic Magnetic Mirrors 77304
SOIT157 -30-2-1/18
i. e.' the deflection or displacement of a nonmono-
chromatic charged particle beam by utilizing two
mirrors with a lateral displacement of particles of
different energies in the manner indicated on Fig. 10.
Fig. 10. Deflection of a noimonochromatic beam by
means of two mirrors with noncompensated displacements.
Card 12/13

Achromatic Magnetic Mirrors
ASSOCIATION:
SUBMITTEDs
77304
SOV/57-30i-2-1/18
Thereare 10 figures; 1 table; and 6 references, 5
Soviet, I U.S. The U.S. reference is: W. K. H.
Fanofsky, J. A. McIntyre, Rev. Sci. Instr., 25, 287,
1954.
Physico-tecluical Institute AS USSR, Leningrad (Fiziko-
tekhnicheskiy institut AN SSSR, Leningrad)
July 6, 1959
Card 13/13

DYMNIKOV, A.D.; FISHKOVA, T.Ya.; YAVOR, S.Ya.
System,of four quadrupole lenses, analogous to axially symaetric
lenses. Izv. AN SSSR. Ser. fiz. 27 no.9tI131-1134 S 163.
- (MMA 16t9)
1. Fiziko-tekhnicheskiy institut im. A.F.1offe AN SSSR.
(Electron optics)

-ISF
YAVOR, S. Ya.~ fYK4FKUf, A. D-.-; 11 IKOVYI--T.- Ya.; -5-11PAY, G~ It.
"Electromagnetic achromatic systems."
report submitted to 3rd European Regional Conf, ELectron Microscopy, Prague,
26 Aug-3 Sep 64.

AUTHOR: Dv*znnikov, A. ID64- FiChkOVOL, Ya.; Ya Vor, S. Ya.
TITLE.- Electron--optical propetfitia-6f-a-pe-eudo-a-cis,rrrietric quadrupole Sygm
SOURCE. Radiotekhnika felektronikai V. :9. no. 10, 1964, 1828-1831
TOPIC TAGS:-.q' drupole lens., axisymetric systern
ua
r~s_work (Zb-TF.--19
A B ST IRA CM - -7 s_xs-a_~continuatiarLo _mn ear-Uar-autho '33s_l~
7,.851). A se t of quadrupole lenses similar to an axisymetric system is
es, the field of each one
tigated.:- -The set - comprise-d-four-quadrupole -lena
being turned by 900 with respect to the field of the preceding one. Two identical
outer lenses may be different from two identical inner lenses. The field inside
the lena is assumed to be constant** outside the lens, equal to zero; field distribu-
tions within the lenses are represented by equivalent rectangles (see Enclosure
1). Formulas for the focal lengths and positions of the foci depending on the
Card 1/3
J

ACCES SION NR: AP4009920 S/0057/64/034/001/0053/0059
AUTHOR-,Fishkova, T,Ya.; Shpak, Ye.V.; Yavor, S.Ya.
TITLE: Charged particlW escape from a reflected electron discharge
SOURCE: Zhurnal tolchnichoskoy giziki, v.34, no.1, 1964, 53-59
TOPIC TAGS: gas discharge, reflected electron discharge, charged particle escape,
anomalous charged particle escape, discharge in magnetic field
ABSTRACT: The transverse escape of charged particles from a gas discharge in a
longitudinal magnetic field was investigated. Electron reflecting electrodes were
provided at the two cmds of the discharge region to increase the ionization. Except
for the higher degree of ionization achieved, the experiments were similar to those
reported by J.F.Bonnal, G.Brilford and C.Manus (Phys.Rev.Lett.6,665,1961; Report
No.9 at the Salzburg Conference,1961), and similar anomalous results were obtained.
The discharge tube was 200 cm long and 17.8 cm in diameter. The two reflecting elec-
trodes were 11.6 cm in diameter and were separated by 105 cm. One reflector carried-
a hot cathode 2 or 3 cm in diameter. The discharge current was received by one or
more cylindrical anodes somewhat smaller in diameter than the reflecting electrodes.
Card ~ 1/3

ACC.NR: AP4009920
I'Ihen a single anode was employed, it was provided with two wall probes, one located
midway between the two reflecting electrodes, and one located 16 cm from this mid-
point. With the discharge tube filled with argon at 5 x 10-4 to 10-3 mm Hg' dis-
charge currants up to 10 A at potentials up to 500 V were observed in longitudinal
magnetic fields up to 2100 Oo..Tho degree of ionization was determined from the at-
tenuation of 3.2 cm, and 0.85 cm microwaves. Xonizations up to 7% were deduced from
the 3.2 cm measurements. A highly ionized filament was produced on the axis of the
discharge by admitting gas through an opening in the center of one of the reflectms.
The ionization in this filament was estimated from the, 0.85 cm microwave measure-
ments at 50% or greater. When several anodes were employed, the current to the calt
tral anode was negative (preponderance of negatively charged particles collected),
and the currents to the remaining anodes were positivo. The currents to all the an-
odes behaved in a similar way as the magnotic field wets varied: when the field was
increased from zero the current would first decrease Cin absolute value), roach a
sharp minimum at a small value of the field, increase to a broad maximum, and final-
ly decrease again at high fields. The pas itive ion current to the central wall
probe of the single anode was measured as a function of the longitudinal magnetic
field while the total discharge current was hold constant by adjusting the applied
potential or the cathode temperature. In those measurements the probe was kept
r,?13
Cc

ACC.NR: AP4009920
30 V negative with respect to the anode. The positive ion current first increased
with increasing field, then decreased to a broad minimum, and finally increased
again at high fields. The initial increase and subsequent decrease of the ion cur-
rent are briefly discussed. The anomalous increase of the ion current at high field
strengths is not explained.. Orig.art.has; 8 figures.
ASSOCIATION: Fiziko-tekhnicheskiy institut im.A.F.IoVe AN'SSSR, Leningrad (Physi-
cal-Technical Institute, AN SSSR)
SUBMITTED: 12Nov62 DATE ACQ: 1OPeb64 EXCL: 00
SUB CODE: PH NR REP SOV: 002 OrHER: 003
3/3
Card

EWA -14b-
L 128?2-� -tiff - EPA JLA~EE 1G.
Af
1 (410
;SMSD ESD (dp)/t~SD
- ------ S/M57/0/034/0091/1711/1714
ACCSSSION XR_ 286
ikow A vi-;
AM
AUMOR
T Ya e@ -PAT
:
g1ja
coub ruoli low
SQU=t ZhUZTAI teMudaheakay-:911did vid$4, UO-gol,904. LILL-L7119
quadrupole
TOPIC V
- a
combined ei
ew tb&t can he NdO achrOwtic by Proper cho=ic
trastatic ara Wgnqtlc quadrupole I
04~ the r"'a of the electric to the w8natic riaid (I
191TY 31,1439,1961; 33f3saim3i
In the Present short. COMW.MLCOLM tt4y diacuss the apbqrica,
tion in the corwazong be -a
P-1=0 Of- A: lens of this typt :for w1dch the fleld confI&VM_
J.
L.O., fO? vh1ch the fielda 1tre indeparxient of one C&rtog-.
i ian.cQordinate, the axis ot ~whjch gerves vj.tbe RKL5 0t Me tew.
equations &to taken f The traJectory
and it is norted tbA
the eQuAtiOnO __ ail written by;A.Sep%ier.-(C.R. 256$23.ZS,i9(YS) contain vu error. The
sPherical aberration in tha-fjrSt:G&ugg
planai _d/f L'tan3l (Where d is the,distamaa
in the image Plane of the' traJsc;tdry fr= the ax1go C III the focal Jezgtftr and L, in!
1/2

ACCESSION NR,: AP4019973 s/bo,2o/64/154/06/1321/1324
AUTHOR: Dy*m. nikov,IA. Do; Vishkova, To Yao; Yavor, So Yaw
TITLE: Spherical aberration of a two-dimensional electrostatic
quadrupole lens without antisymmetric planes
7SOURCE: AN SSSR. Doklady*, v. 154, no. 6, iS64, 1321-1324
TOPIC TAGS: spherical aberration of electrostatic lens, quadrupole
electrostatic lens, electron microscope lens, spherical aberration
-correction, electron microscope, spherical aberration
!ABSTRACT: In the present paper, a method has been developed for the
correction of spherical aberration which is based on the maintaining
of symmetry planes of the field in the absence of antisymmetry planes,
An example of such asymmetry is presented by an electrostatic lens
which has different distances between electrodes of the same sign.
The possibility of such a correction is shown on a two-dimensional
electrostatic quadrupole lens. In the equations for trajectories of
Cord 1/2

ACCESSION NR: Ap4ol9973
charged particles, terms are consid&ed which are necessary for the
,computation of aberrations of the third order. The computation shows
that spherical aberration cannot be compensated along the whole image.
The length of the linear image is not greatly affected by spherical
aberration. The suggested method of correction permits one either to
.reduce the spherical aberration along the whole length of the image,
or to completely compensate it in the center. Orig. art. has: 3 fig-
ures and 24 equations.
ASSOCIATION: Fiziko-tekhicheslciy institut im. A. F. loffe Alcaderrdi
-Naulc SSSR.(Physics-EngineerinG Institute, Academy of Sciences, SSSR)
SUBMITTED; 24Sep63 DATE ACQ: 23Mir64 ENCL: 00
;SUB CODE: PH NO REF SOV: oo4 OTHER: 000
Card 2/2*

DY1,fNIKOV, A.D.;_,fISflKOVA,,T.Ya.; YAVOR, S.Ya.
Electron-optical properties of a pseu.doaxially-symmetrical
quadrupole system. Radiotekh. i elektron. 9 no.10:1828-1831
o 64. (MIRA 17:11)
1. Fiziko-tekhnicheskiy institut im. A.F. Ioffe AN SSSR.

DYI,%IKOV, A.D.; FE]JIKOVA, Ma.; YAVOR, S.Yzi.
Spherical aberration of a composite quadruprile lens. Zhur. tekh. fiz.
34 no.9tI711-1714 S 164. (MIRA 17:10)
1, Fiziko-takhnicheskiy institut imeni, Toffe AN SSSR, Leningrad,

~ o,
~ I-
l I
--- -,- --
.. I . I, I: .A 111. I-- . ~, -- .1 ,- -'. 7 r ,
- : I .-I. . - --- .-.,'' , : - . , ~ ". -1.I1 .1
- - . --- -. . -- A~ , - - - -. - . ~: .-. ~ .-
L! -*, -, i -:ff
,I-,--.- - ~, 77

~-66
i
.ACCESSION N'Rt AP5017204 U11/0020/65/ 1-62/7666/i~W .~2e~18
AUTHORS*. Dymnikov, A. Fishkova, T. Ya.; Yavor, S. Ya.
V Y,
:TITLE: Spherical aberration of a combined quadrupole lens,with
re c tangular f le Id distribution ('5'
~SOURCE; AN SSSR. Doklady, v.. 162, no. 6, 1965, 1265-1268
,TOPIC TAGS: electron optics, magnetic quadrupole lens
~ABSTRACT: In order to get around the mattematical difficulties invol
~ved in using a rectangular model for the calculation of spherical
iaberrations, the authors have derived for the sphorical aberration
iexpressions which do not contain the derivatives of the fields in ex-
!plic:Lt form. These expressions were obtained by solving, by pertur-
i,bation theory, trajectory equations given in an earlier paper (ZbTF
v. 34 1711, 1964),, and by subsequently transforming the obtained
formulas by integration by parts. The particular analysis pertains to
a field which is bounded in the axial direction when a pointlike object
lying on the axis, as well as its linear Image, are both situated.in
Card 1/2

L
IACCESSION NR: AP5017204
ia field.-free space. Plots of the coefficients of spherical aberration,,
.;obtained on the basis of these calculations, are included. The re-,
isults were compared with experimental data for a parallel beam and
~were found to be in good agreement. This report was presented by
;B. P. Konstantinov. Orig. art. has: 3 figures7 and l9formulas

L 36550-66 EWT(I)/T IJP(c)
ACC NRi AP6015754 SOURCE CCDE: UR/0048/66/030/005/0739/0741
( 4r IV
AUTHOR: Dymnikov,A.D.; Fishkova,L-i-Is..'i
ORG: none
TrrlE* Dependence of the spherical aberration coeffic:ients of a quadrupole lens on
the object distance (rectangular model) /Report, Fifth.All-Union Conferenge on
Electron Microscopy held in Busy 6-8 Jui7y 196!C/ p
SOUWE*. AN 88SR. Izvestiya, Seriya fizicheakaya, v. 30, no. 5, 1966, 739-741
TOPIC TAGS: electron opt~ics spherical aberration, magnetic quadrupole lens,
static field
ABSTRACT: Equations given elsewhere by the present authors (Dokl. AN SSSR, 162, 1265
(1965)) have been employed to calculate, with the aid of a computer, the spherical
aberrations of magnetic and electrostatic quadrupole lenses. Curves are presented
showing each of the four spherical aberration coefficients of both types of quadrupol
lens as functions of the object distance for different values of the excitation. The
principal spherical aberration coefficient for the converging plano is always positiv,
and has a minimum; the relation between excitation and object distsace for the minimu
value of this coefficient is presented graphically. The spherical aberration in the
width of a linear image in the median plane for a magnotic quadrupole lens is comptre

L 36550-66
ACC NRt AP6015754
with the.corresponding quantity for an analogous axially symmetric lens; for equal
object distances and focal lengths, the quadrupole lens has the smaller spherical
aberration. Orig. art. has: 4 formulas, 9 figures, ani 1 table.
SUB CCDZ- 20/ SUIM DATE* 00/ ORIG FdF: 001/ am HRF: 001
2/2.

ARTSIMOVIGH) G.V., kand. tekhn. nauk; ASYCRENKO, Ye,I.,, kand. teklin. nauk;
STARKOV, V.I.., inzh.; MOSKA""EIIKO, V.P., inzh.; FISFMAN, A.I., inzh.
Using hard-alloy tools in boring frozen soils with the BKGM, machines.
Stroi. i dor. mash. 10 no.lOt24-25 0 165. (MIRA 18tJO)

SMMMEIYI M. - Ta.; 'CHMMUOVp A. N.; FISHLER-B. W.
p
The GEFK-130-17-5 owing armt I ver railroad crane. Transp.
stroi. 13 no.41 ,34-36 Ap 163. (NMU 1694)
1. G:Lavnyy tekbnolog mostestraitelinogo tresia No. 2 (for
Shklovskiy). 2. Starstiy-Inshener Voesaymnogo nauabno-
iseledovateltakogo inatitut tranaportnogo stroitelletva,
Mininterstva transportnoge stroitalletva (for Charkasov).
3. Veduohahiy konstruktor Uglicbskogo remontio-mekhanicheakogo
zavoda (for Mahler).
(Cranes, derricks, etk)
(Bridge construction-3quipment and-suppliin)

FISHMAN, A.
Combining mass participation and skill. Voen. znan. 41 no.8:38-39 Ag
165. (MJRA 18:7)
1. Predsedatell strelkovoy sektsii Vsesoyuznogo dobrovollnogo obshr-hestva
sodaystviya armli, aviatsit I flotu SSSR pryadillno-nitochnogo kombInata
imani S.M.Ktrova, Leningrad.

KAFTSEVY N.N., inzh.; FISHMAN, A.M., inzh.
Machining holes with burnishing broaches. Mashinostroenie
no.3s43-44 MY-Je 165. (KM l8s6)

MIZIN9 V.G.~ Inzh.; SAFONOV, B.P., inzh.; SERN, G.V., inzh., KOROBEYNIKOV,
V.V., inzh. B D inzh.; -,TRAKHOV, V.M., inzh. NIKITIN, Yu.K.
Production of 75% farrosilicon v''Lth coke !,.'rom a charge with
an Increased content of Oas cor.' 3tall 225 no.2:133-135
F 165. (MIM 18: 3)
1. Kutnetskiy zavod ferrosplavov I Kuznet!;kiy filial Vostochnogo
nauchno-issledovatellakago uglekhimicheigkogo Instituta.

,.Accmuff um- Ap4p3gog a/C)191/64/000/005/0066/006T
!.AUTHOR: Kovehina., L. Do; Fiabiman, B* No
TITIZ: Hermetic sealing of articles witit epoxide caq-)ouzx1 under vacuum
SOURCE: Plasticheakiye maeW., noo 5., 1964,, 66-67
TOPIC TAGS: hermetic sealings equipmentp apparatuss epo.)dde sealingp epoxide
coating., vacuum casting apparatus
ABSTRACT: Equipment was designed for the hermetic ocaliag of articles with epoxy
cctipounds under vacuum (fig. 1). In this apparatus a nuuber of articles to be
coated am arranged on the turn table (fig. 2)., the system is put'under 740-750 mm
1~Hg vacuum) the epoxy is poured onto the article in the vicinity of the pour spoutp
epo;,-4 flow is shut off, the table is rotated and epoxy coating repeated un"Vil ea~
successiwe article b" been treated, Orig. art. has: 3 figures.
ASSOCIATIM. None
SUBUTTED % 00 ENCLi 02
Card
3./4
'V

ENNKMM
1, . ? I
I : I
0 i I
k 4 ~.1
i
I

.iACCESSION NR: AM35log ENCLOSURE: 01
Fig. 1e Va6tm casting
!I-push button control
2--pouring spout
3"c0aical stopper
~4--hopper (for epoxide)
i5--stopcock for vacu= release
~6--Yacuua gage 0
.7--l=P

:8--cover 6
19--window
10--housing
11--tum table
12--reducing gear

CqLd-V4

ACCESSION MR:
AP4035 ENCLOSM 02
M9
"Fig. 2. General view and drive
1;mechanism for turn tables W.
I- -supporte for tum table
2--tumtable
3- -reducing gear
4--electria motor
P~,
4/4

PHASE I BOOK EXPLOITATION 479
Bezrukov, V.M.; Glukh, Ye. M.,* Kostin, K.F!.,* Neyman, Z.B.,,,
Fishler, Ya. L.; Chetchuyev, G.A.
Urallskiy zavod elektromashinostroyeniya (The Ural Electrical
Machine-building Plant) Moscow, Mashgiz, 1957. 125 P.
(Seftes: It istorii mashinostroyeniya ne Urale, vyp. 7)
4,000 copies printed.
Tech. Ed. ; Dugina, N.A.; Editorial Board of Series: Aleksandrov,
A.I., Candidate of Technical Sciences; Bogachev, Doctor
of Technical Sciences,-*Volbkov, A.A., Candidate,ot Historical
Scieneds,% Dovgopol, V.I.; Kozlov, A.G., Senior Scientific Worker,
Archives Pept.; Sustavov, M.I., Engineer.
PURPOSE: This book is intended for engineers, technicians and
scientists. It can also be of use to students, agitators,
propagandists and machine-building workers.
Chrd 1/3

The Ural Electrical Machine-building Plant 479
COVERAGE: The book contains a brief history of the construction
and development of the Ural--Electrical Machine-building Plant
and a detailed description of the progress achieved in designing
and building various kinds of machinery including water-wheel
generators)a-c and d-c electrical machines, transformers, high-
voltage equipment, mercury-are rectifiers and machines for the
electrification of the national economy. Plans for the future
development of the plant and of the production of the electrical
industry in general are also discussed. The book is the seventh
isseaed in the series "1z iatorii maahinostroyeniya na Urale"
(Tridtory of Machine -building in the Urals) which will contain a
total of ten books. No personalities are mentioned. There are
no references.
TABLE OF
CONTENTS:
Foreword 3
Ch. I. Construction and Development of the Plant 5
Card 2/3

The Ural Electrical Machine-building Plant 479
Ch. II. Ural Water-wheel aenerators
Ch. III. Improvement of Electrical MachInery
Ch. IV. Development of Transformer Construction at
the Plant
.Ch. V. Production of Mercury-arc Rectifiers-
Ch. VI. High-voltage Systems
Ch. VII. On a Scientific Basis
Ch. VIII. Work, Study and Leisure
AVAILABLE: Library of Congress
-TJPA3v
8-5-5B
15
38
41%
77
96
115
121
Card 3/3

Conference on the Developmental Problems of the SOV/105-58-7-21/32
Production of Transformers in the USSR o 5-6 Nor 15%,, Moscov
(Elektriobestvo, 1W, No- 7., PY. 82-83)
and voltage and about.the shortcomings in the assembling which
are due to the manufacturers.S.A.Gorodetskiy (Glavelektromontazh
MS RSFSR) spoke about the abolition of the revision of the re-
movable part of the autotransformere at the assembling site, and
about several constructive changes in power transformers and about
the measures necessary for a mass connection of the transform era
without drying. A. M.Sarkisyan (Gleivaellelektro MSKh SSSR) spoke
about the electrification on the open country and the demand of
open country districts on the electrical industry. K.A.Yegikyan
(Armelelektrozayod) reported on neir transformer constructions.
Ya.L.Fishler (chief of the construction office in the works "Ural-
elektroapp~aratll) also reported on transformer constructions. The
conference found serious shortcomings in the organisation of
scientific research work and a lack of engineers and designers.
1. Transformers--Development 2. Transformers--Production
3. Conference
Card 3/3

Sf)V/110-59-7-6/19
AUTHOR: Fishler Ya L Engineer
TITLE: Transformer Manufacture at the "Uralelektroapparat Works
(Transformatorostroyeniye na zavode 'tUralelektroapparat")
PERIODICAL: Vestnik Elektropromyshlennosti.,1959,Nr 71pp 27-31 (USSR)
ABSTRACT: The 'Uralelektroapparat" works produces power transformers
in ratings from 50 to 60 000 VA, mainly for supplying
mercury-are rectifiers. The works has developed a series
of transformers type TMRU rated from 420 to 12 800 kVA for
supplying mercury-are rectifiers having d.c. output from
500 to 10 000 A at 230 to 3300 V. Double-star secondary
windings are used and usually some of the transformers in
a sub-station have star-connected primaries and some delta.
Equalising reactors are installed in the transformer tanks.
The transformers of this series have been fully tested on
short-circuit; the test circuits are described. A new
series of rectifier transformers is being developed,
employing cold-rolled steel for higher efficiency and
economy in material. Information is given about a number
of advantages that transformers of the new series are
Card /L~ expected to have. A transformer of the new series is
illustrated in Fig 1. A few of them have been built but

Sov/110-59-7-6/19
Transformer Manufacture at the "Uralelektroapparat" Works
the rate of introduction will depend on the availability
of cold-rolled steel. A consi(~erable number of
transformers are being supplied for railway electrifi-
cation. In addition to the widely-used rectifier
transformers type TYRU-6200/35 for a d.c. output of
1000 A at 3300 V, the works has developed and is
delivering transformers type ML-11000/10 for supplying
bridge-connected pairs of mercury-arc rectifiers with
outputs of 2 x 1125 A at 3300 V. As transformer type
TMR-11000/10 is of high efficiency the increased losses in
the bridge circuit rectifiers are fully compensated.
On-load voltage control of railway electrification
transformers offers numerous advantages and accordingly
the works have developed transformers type TMRN-15000/10
by means of which the rectified voltage can be controlled
over the range 3600 - 4000 V with primary voltage
variations of +5 and -10%. Considerable economy will
result from using 110 V transformers in traction sub-
Card 2/4 stations instead of using doubl-e transformation.
Transformers type TMR-11000/110 have been developed for
supplying bridge-connected pairs of rectifiers with
outputs of 2 x 1 125A at 3300 V. Transformers of 110 V

SOV/110-59-7-6/19
Transformer Manufacture at the "Uralelaktroapparat" Works
with on-load voltage control are also being developed.
Rectifier transformers type TMRIJ-16000/10 for d.c.
outputs of 3000 A at 3300 V, have been developed to supply
circuits with two rectifiers in series per phase. A
series of transformers exemplified in Fig 2 is for
tropical service. They are in ratings from 100 to 2000
kVA and are filled with non-inflammable fluid. Being
fireproof, they can be installed indoors in industrial
premises alongside the equipment to be supplied. Special
series transformers have been developed for the self-
excitation circuits of large al-ILternators and synchronous
capacitors. The primary winding is connected in series
with the stator winding of the alternator and the
secondary current is used for excitation. In this way
additional excitation can be provided under short-circuit
conditions. Dry-type transformers developed for rectifier
excitation of the 30 and 50 MW hydro-alternators of the
Stalingrad station are illustrated in Fig 3. A number
of special transformers have been designed for various
Card 3/4 large industrial drives. Dry transformers for rectified
currents of 1200, 1800 and 3600 A have been developed

SOV/110-59-7-6/19
Transformer Manufacture at the IrUralelektroapparat" Works
for forming mercury~arc rectifiors. These transformers,
illustrated in Fig are of very compact construction
and use air-blast ventilation. Special sectionalised
limiting reactors for currents up to 200 kA have been
developed for high-voltage test equipment in short-
circuit testing laboratories. Such a reactor is
illustrated in Fig 5. The 7-year plan provides for
doubling the production of transformers and extending
Card 4/4 therange of types.
There are 5 figures.

FISHIJMq Yd-OL49 inzh.
IA7w P(mor 1-10 kv. olezt-ic tranofoymers. Vew'.
32 no.12.'Ll--.15 D 161. (MIRA 14222)
(Elects:ls- transformers)

GURAVIGH, Solomon, Ostpovich; FISMAN, Abram.Aronovich- CEAPSKIT, O.U.,
==A_
:redaktor; KOTMOVA, T6K=I""rwTWffffMr
[Oil economW of machine-tractor stations and state farms] Nefte-
khozIaIstvo MTS I sovkhozov. Moskva, Goo., izd-vo oallkhoz. lit-ry,
.109 p
1956-' WRA 10:2)
(Machine-tractor stations)
(state fares) (Petroleum productm,--Storage)

KRICUO, Xatvey SomenavIch; JJ=KAN. A&IO , inshener. rat sensent; OK"mmm,
IA., kandidat a.-khe naux, redMor-, 12ITTILINA, L.A., rodaktor;
XISINA, Yeel.. tokhnichookly rodaktor.
[Losses in the processing of wine by-products suil wore of preventing
thou] Poterl pri pererabotke pobochnykh produktar vinogradnago vine-
deltia i borlba a mint. Moskva, Pishchtrpromizdat.- 1955. 98 P-
(Win* anii wine making) 9:5)