MAHASHOT. N.P.; LTPSKIY,_._YU, - N.
First results of studying photographs of the other side of
the moon. Astron.tair. no.206:1-4 D 159. OURA 13:6)
1. Karlkovskaya astronomicheskaya, observatorlya (for
Barabashov). 2. Astronomicheakiy institut, is. Shternberga
(for Lipskiy).
(moon--surface)
BARARASHOV, N.P., red.; MIMIL07, la.A., red.; LIPEKIY, Yu.N., red.
[Atlas of the other side of the moon] Atlas obratnoi atorony
LunY. Koskva,, 1960. 149 p. illus. ((Ybrazovaniia, vyiavlennye
na obratnoi storone Iqmy pu fotografilam, polucheniym avtoma-
ticheskoi m-ezhplanatnoi stantsiei 7-go oktiabris 1959 gods).
(MIRA 13:12)
1. Akademiya nauk SSSR. 2. Astranomicheskaya observntoriya pri,
Kharlkovskom gosudarstvennom universitet im. A.M.Gorlkogo (for
Barabashov). 3. Gosudars'u'vennyy astronomicheskiy institut im. F.K.
Shternberga, Moskva (for Lipskiy).
Noon--Surface)
/Y (Shternberg Astron. Inst, YWCOW)
_LH16 ~j ~,,
"On. The Methods Of Studying The Photographs Of The Reverse Side Of The Moon Pxd
Some Results Received."
paper rm*m presented at I Symposium on the Moon, Leningrad, USSR, 6-8 Dee 6o.
A short characteristic of conditions that took place during the time of anapping of
the reverse side of the Moon is given as well as the peculiarity of the first negatives
obtained with the aid of the automatic interplanetary station. A short description of
an especially worked out method and some other methods used for the studying of the
photographs is also given.
There were found out about 500 Moon formations altogether, 252 of them were put to the
first category of reality, 190 of them to the second category and 57 to the third one.
The report has a short characteristic of the map of the formations found at the reverse
side of the Moon. The estimation of the exactness of definition of coordination of the
new formation is given. A description of some of them is quoted. A short description
of the Atlas of the reverse side of the Moon is given.
In virtue of all materials obtained the following conclusions are drawn: the hemi-
spheres of the Moon are asymmetrical in the hollows of the surface. At the reverse
side of the Moon there are no such long and deep hollows as the Oceanus Procellarum,
Mare Imbriu, Mare Serenitatis. The largest part of the moon surface has a high albedo
like mountainous regions. The formations of reverse side and visible side of the
Moon are similar in their nature and structure. Undoubtedly there are craters with
the central mountain) ray systems and mountainous obdects. The influence of the rapid
hesitations of the temperature during the time of eclipses on the character of the
Moon relief Is not considerable.
1AP37M, Yu. N.
f tli~~ 1.1 on a-~' D
k1c,,y ol PhotiC7ruph- of the F:ir 3;,!~
A S
of Sinj-ul ::- Featur, vealed on Its SuroLa(-,e.
-port pr s;~nted ~_i ~ the In'- rnational 'm ,n the moon, hebl at tl~e
I
Pulkovo Cbs,-rvAorjj Le-aingrad, T3 !. P 6-8 Dec 19~-O.
87256
16 6 (0 1; / /,70 S/033/60/ 037/oo6/ol5/022
3,1SS19 E032/E5-0
AUTHOR.- Lipskiy, Yu. N.
TITLE: A Method of Studying Photographs of the Reverse Side of
the Moon and Some of the Results Obtained
PERIODICAL: Astronomicheskiy zhurnal, 1960, Vol-37, No.6,
pp. 1043-1052 + 5 plates
TEXT: The third cosmic rocket carrying the Automatic
Interplanetary Station (AIS) was launched in the Soviet Union on
October 4, 1959. The orbit intended for the AIS was to take it
round the moon, followed by return to Earth. On October 7, at
3h3Om UT, when the AIS was at a distance of 65 200 km from the
centre of the moon, the photographic apparatus was brought into
operation by remote control from the Earth's surface and the other
side of the moon was photographed. The photography was terminated
after a further ItOn' at a distance of 68 400 km, The exposures were
automatically varied and the photographic camera was equipped with
two objectives (focal lengths 200 and 500 mm, respectively) so that
images of the moon 10 mm and 25 mm in diameter were obtained. A
special device mounted on the AIS then automatically developed,
Card 1/5
872156
S/033/60/037/006/015/022
E032/E514
A Method of Studying Photographs of the Reverse Side of the Moon
and Some of the Results Obtained
fixed and dried the photographic film. A special 35 mm film was
employed, suitable for processing at high temperatures. The image
obtained on the negative was then transformed into electrical
signals. These signals were obtained by scanning the photograph in
parallel lines, the amplitude of the signal depending on the density
of the negative. In order to reduce the effect of noise and
interference, the signals were modulated before transmission to
Earth. On reception at the Earth's surface, the signals were
pappmon an mn)[noTIE 'Callu] they were, recorded
by various devices. Among these were lphutorecor"cr,-sa
reproduced the image on the original negatives on a 35 mn, film, and
"magnetic recorderd1which gave an image which was magnified by a
factor of 10. Detailed data have been published In the Atlas of the
Reverse Side of the Moon issued by the Academy of Sciences, USSR.
The analysis of the data obtained In this way, tite development of
methods for recogniz3-ng details on the photographs, tfie. composition
of a catalogue of all the formations etc,, were carried out in
Card 2/5
7 255 '
S/033/60/037/oo6/ol5/022
E032/E5i4
A Method of Studying Photographs of the Reverse Side of the Moon
and Some of the Results Obtained
Moscow at the Astronomical Institute imeni Sliternberg (GAISh) and
the Tsentrallnyy nauchno-issledova-7-ellskiy institut geodezii,
aerofotos"yemki i kartografii (Central Scientific Research Institute
for Geodesy) (TsNIIGAiK). The work at the latter institution was
directed by N. A. Sokolova. An independent study of the data was
carried out by the Pulkovo Astronomical Observatory and the
Astronomical Observatory of the Khar1kov University. Since the
photographs were obtained at full moon (relative to the AIS), all
the photographs had a rather low contrast owing to the absence of
shadows. Three methods were employed to analyse the photographs,
namely, 1) the superposition method; 2) photographic masking,
3) photometric section. In the first method a number of photographs
were superimposed on each other and it was found that the visibility
of the details was considerably improved as compared with single
negatives. This method has the advantage that 'noise' and
interference effects are not increased in the same proportion as
the -visibility of zhe required details. The superposition was
carried out with the aid of three projectors. Each of the
Card 3/5
87256
S/033/60/037/006/015/022
E032/E514
A Method of Studying Photographs of the Reverse S.id-e of the Moon
and Some of the Results Obtained
projectors produced an image of the corresponding negative on a
semi-transparent screen. The three images were made coincident by
superimposing all the well-defined regions. The outlines of other
details could then be drawn on the screen. In the second method,
the maximum contrast between given parts of the negative was
reduced by masking, without reducing the small contrast differences
between details within these regions. In the third method the
negatives were examined photometrically. A preliminary list is
given of the positions of the various details recognized on these
photographs. The general conclusion is that the two lunar hemi-
spheres are asymmetric. The reverse side of the moon does not
exhibit extensive depressions analogous to, for example, the Oceanus
Procellarum or Mare Serenitatis. The depth of the larger
depressions on the other side of the moon is very much smaller than,
say,the depth of Oceanus Procellarum. Objects located on the other
side of the moon do not differ in their nature and structure from
formation5 on the visible side of the moon. Definite evidence was
Card 4/5
S/033/60/037/oo6/ol5/60-2
E032/E514
A Method of Studying Photographs of the Reverse Side of the Moon
and Some of the Results Obtained
obtained for the existence of craters. Regions covered by craters
with high reflection coefficients occupy a large part of the surface
of the reverse side of the moon. Acknowledgments are expressed to
L. A. Bondarenko, K. I. Degtyareva and A. I. Goyna (members of
staff of GAISh) for their assistance. There are 5 figures, 1 map
and 5 Soviet references.
ASSOCIATION: Gos. astronomicheskiy in-t imeni P. K. Shternberga
(State Astronomical Institute imeni P. K. Shternberg)
SUBMITTED: October 18, 1960
Card 515
KULAGIN, S.G.; KOVBASYUK, L.D.; DAGAYEV, M.M.; IAZAREVSKIY, V.S.;
DEMIDOVICH, Ye.G.,- BWNSHM, V.A.; YAKWHTOVA, H.S. (Leningrad);
KUROCIIMI, Me.; DOKUCHAYEVA, O.D.; SHCHERBINA-MICYU)VA, I.S.;
MAESVICH, A.G.; 111 ~KIY ju~N~~ MARTYNOV, D.Ya.,- ARSENTIYEV, V.V.;
MOROZI V.I.; MASEVICH, A.G.; PERELI, Yu.G.; BAKULIN, P.I.,, otv.
red.; KULIKOV, G.S., red.; AKHLAMOV, S.N., tekhn. red.
(Astronomical calendar; yearbo-ok.Variable part, 1962] Astrono-
micheskii ka2endarl; ezbegodnik. Peremennaia cbastl,, 1962. Red.
kollegiia: P.I.Bakulin i dr. Moskvap Gos.izd-vo fiviko-matem.
lit-ry, 1961. 259 P. (Vswioiuznoe as-tronomo-geodezioheskoe ob-
shebestvo, no.65) (mk 14:12)
1. Gosudarstvennoye astronomo-geodezicheekoT e obshcbestvo (for
Kalugin, Kovbasyuk, Lazarevskiy, Demidovic . 2. Moskovskoye ot-
deleniye Vsesoyuznogo astronomo-geodezicheskogo obshchestva (for
Dagayev, Bronshteng Kurochkin).
(AstrononW-Yearbooks)
S 560 61/000 1009 /001a /009
AUTHOR:
TITLE:
Lipskiy, Yu. N.
Special features of the first hotographs of the far side of the
p
moon
PERIODICAL: Akademiya nauk SSSR. Iskusstvennyye sputniki Zemli, no. 9,
1961, 3-19
TE n station launched. October 7
-XT: Data obtained by the automatic interpla etary
1959, were studied at the State Astronomical Institute imeni Shternberg and the
Scientific Research Institute of Geodesy and Cartography in Moscow, the Main
Astronomical Observatory in Pulkovo, and the Astronomical Observatory of
Khar1kov University. The main difficulties encountered were due to 1) the fact
that the photos werc obtained at close to full- m oon- illumination conditions and
2) interference. To bring out details, the method.oircorhbined superposition
of negative's was employed; in this process thret~ negatives of the same scale
Card 1/ 3
Special features of the first photographs.... S/560/6liOOO/009/00la/(109
are combined by simultaneous projection. By this method the contours of the
Mare SFnythii and -the lighting in the Sea of Moscow were revealed; however, its
effectiveness was limited by the presence of static in the form of belts cross-
ing over the image. The method of photographic ffiatkiag made it possible to
reduce maximum contrast between different sectors of the negative without
weakening the small contrast differences between details within the sectors
Four photos of the far side were obtained in this manner; however, the con-
trast on them was still great. The photometric sections method, consisting
in the amplification of weak contrasts by radio means, was most effective.
The sections were selected by sampling in accordance with the photometric
features of the sectors to be interpreted. A total of 200 photometric sections
were used. The properties of different sectors of the photographs for separate
photometric sections were subjected to detailed analysis. The greatest number
of.details appear or,*the sections of negatives obtained with long-focus objec-
tives. All 499 defined formations were broken down into three Categories ac-
cording to the degree of reliability. The configuration and internal structure
of objects on the visible side were also refined. The most interesting feature
Card 2/ 3
Special features of the first photogra-phs.. .
S/560/61/000/009100la/009
on the far side was the Sea of Moscow, one of the darkest formations, extend-
ing 300 km in a northwesterly direction. It is of uniform brightness and has
a bright detail, indicative of a peak.. in the center. Near th,~,. north pole there
is a group of craters wbose image clearly shows relief; they include the clearly
defined Tsiolkovskiy Crater. the Sovetskiy Range, extending 1000 km, con
sists of individual elevations with a high coefficient of reflection. One of the
brightest formations is -the crater Bruno, which* is apparently the center of a
ray system. It is concluded that the moon is asymmetrical relative to the
plane dividing it into the visible and invisible parts. No large seas occur on
the far side. 'The total area of the Sea of Moscow.and the Sea of Dreams is
of the same order as that of the Sea of Rains, but. their depth is not great.
Craters with a' high coefficient of reflection occupy a large part of the, surface
of the far side; no specific special features were detected there.
Card 3/3
20498
S/025/61/CGC/0,03/008/012
_3,1S_r0 (Ias7i 106 A166/A127
AUTHOR: Lipskiy, Yu. N.., Senior Scientific Associate (see
Assoc ion -
TITLE: Studying the photographs...
PERIODICAL: Nauka i zhiznl, no. 3, 1961, 27-31
TEXT: The article deals with the techniques used in ob-
taining photos of the reverse side of the Moon and the results ob-
tained from analyzing them. Photography was carried out at full
moon so that the whole hemisphere was illuminated,and also con-
tained some of the objectives visible from Earth in the western
rim of the Moon's disc. This was of assistance in working out the
selenographic. coordinates of objects recorded on the reverse side.
Equipment installedin the automatic interplanetary station pro-
vided for automatically varying exposure times to ensure the best
photographic results for sections of the lunar surface differing
in albedo. The negatives obtained were scannecL, amplified, modu-
Card 1/3
20498
S/025/61/000/003/008/012
A166/A127
Studying the photographs ...
lated and transmitted to earth where they were recorded on tape
and reconverted into images which, in turn, were photographed. In
deciphering the photos specialists had recourse to photometric
sections, i.e., weak contrasts between details on the negatives
were brought out by amplifying selected frequency bands in the
tape recordings of the photos. This method helped to eliminate
atmospheric distortion recorded on earth, and greatly improved
the detail visible on the final negatives. Some 499 objects were
detected on the photos, divided according to degree of reliability
into three categories. Category I contained 252 objects on 3 or
more negatives; category II contained.190 objects on not less than
two negatives; category III contained 57 objects recorded on one
primary negative. These categories have been indicated on the map
of the reverse side of the Moon. A description of the Mare Hum-
boldtianum, the Mare Marginis and the Mare Australe, as they have
Card 2/3
2o498
S/025/61/000/003/008/012
studying the photographs ... A166/A127
been reproduced from the lunar photos. These photos also indicate
that the reverse side of the Moon is largely composed of craterous
areas with a high reflection coefficient. There are 3 photos (1
of the author, and 2 on page 26 of the reverse 3ide of the Moon)
ASSOCIATION: Gosudarstevennyy astronomicheskiy institut imeni
Shternberga (State Astronomical Institute imeni
Shternberg)
Carcb 3/3
89688
6/"
A166/AO27
AUTHORs Lipsk~,_N~Yul
TITLE: First Photographs of the Reverse Side of the Moon
PERIODICALs Priroda, 19 1430. 1, Pp. 35-40
TEXT& The first photographs of the reverse side of the moon were
taken from the Soviet Automatic Interplanetary Station with a two-lens
camera with respective focal lengths and apertures of 200 mm and 195 and
500 mm.and 10.5. The negatives were developed on bord the station,
scanned, converted into radio signals, amplified and relayed to earth.
Here they were converted into visual pictures and also recorded on tape
for future processing. Some of the interference and atmospherics detract-
ing from the clarity of the pictures could be filtered out during process-
ing. The Glavnaya astronomicheskaya observatoriya AN SSSR (main Astrono-
mical Observatory of the AS USSR) at Pulkovo and the Astronomicheskaya
observatoriya Kharlkovskogo gosudarstvennogo universiteta (Astronomical
Observatory of the Khar1kov State University) cooperated on the photograph-
Card l/ 2
8~688
First Photographs of the Reverse Side of the Moon S/026/61/000 I/001/00YO07
A166/AO27
ic and transmitting equipment installed on the space craft. The Astrono-
michesky institut imeni P.K. Shternberga (Astronomical Institute imeni
P.K. Shternberg) and the Tsentralnyy nauchno-issledovatellskiy institut
geodezii i kartografii (Central Scientific Research Institute of Geodesy
and Cartography) worked together in Moscow to study material, develop
methods of deciphering the photographs, describe the objects photographed,
establish their coordinates, calculate the cartographic grid and prepare
maps and a globe of the Moon. Since all the photos had to be taken at
full moon, detail on the negatives was very blurred due to lack of shadow
depth and general overexposure. To solve this problem, the photos were
deciphered from the tape recordings by boosting a selected band of fre -
quencies. All frequencies above and below the selected band remained un-
changed which increased the contrast of the selected band. This revealed
many details which would be invisible on the normal negative. The results
of the observations are contained in a detailed map of the reverse side
of the moon in a scale of D10,000,000. There are 6 photos, 2 diagrams,
1 map and 1 Soviet reference.
ASSOCIATIONa Gosudarstvenng astronomicheskiy institut im.P.K. Shternberga
(State Astronomical Instituteim. P~K. Shternberg)
Card 2/2
LIPSK~Y ,; BONDARENKO, L.N.; LEPIKHIN, R.S.; LYASHCHENKO, V.P.;
-- , Yu.R
PORREGEL15, M.M., SUGROBOV, N.K.
New means of astronomic observations; study of celestial bodies
by means of television. Priroda 52 no.7t96-99 Jl 063.
(MIRA 16:8)
1. Astronomichaskiy institut im. P.K.Shternberga, Moskva.
(Television in astronomy)
L-11166-66 Elfr(l) GW
~C " AP6000365 SOURCE CODE: UR/0286/65/000/021/0058/0058
[AMONRS: Lipskiyo Yu. N.; Pospergells`~
P me me
ORG: none
TITLE: Electronic polarimeter. Class 42, No. MOW Za'mounced by State Astr
ical Institute, im, P, K,, Shternberg (Gosudarstvennyy astronomicheskii-nista
SOURCE: Byuneten' izobreteniy i tovarzWkh znakov, no, 21., 19650 58
TOPIC TAGSS
polarimeter, light polarization
ABSTRACT: This Author Certificate presents an e:Lectronle po2arJM't!3r for spectral
measurements of the parameters.of elliptically polarized light. The device contains
an-optical-mechanical light modulator, a phototube, and an electr-)nic device for
analyzing the information, To measure an four Stokes parameters, to increase the
sensitivityl and to elimine instrumental errors, the optical-imehanical modulator
is in the form of a movable phase aohromatized plate and polaroid and a fixed
polaroid (see Fig. 1). 7be analyzing electronic device contains three independent
electronic channels. Phase detectors and detectors of the reference values of the
operating frequencies are placed in'each channel*
Card- UDC:
L 11166-66
ACC NRj .4p6GM365
Fig* I* I - Phase achromatized platel
2 - rotating Polaroid;
3 - fixed Polaroid;
4 - nonochromator;
5 - phototube.
Orig, arts hass I diagram,
SUB COM 1 20/ SUBM DATE s IlMar64
card 2
FA-CC NR- AP6022190
SOURCE CODE:
AUTFIOR:- Lipskiy, Yu. N.';Gurshteyn, A. A.,
ORG: State Astronomical Institute Im. P. K. Sht
stvennyy astronomicheskly Institut)
TITLE: The space age and the exploration of the moon\
(Gosudar-
SOURCE: Priroda, no. 6, 1966, 6-18
artificial satellite
TOPI "TAGS: moon, space station, lu1nar surface, satellite photc-.aphy,
/Ranger artificial satellite, Zond-3 artificial satellite) IAM-9 artificial satellite,
Luna-10 artificial satellite
ABSTRACT: The author discusses lunar exploration and recent discoveries of lunar
characteristics, presenting both US and Soviet achievements in this field with
191se of the Soviet. General details on the lZunching and flight of the
emphasis on t4
Soviet Luna- 9fnterplanetary automatic station are given. Ti-ie discovery of the
asymmetrical morphological structure of the lunar surface by Soviet photographs
of the dark side of the moon is described in detail. The missions of the nine US
Rangers and the flight of the Soviet Zond-3 are described. The discovery of
C..,d 1 / 2 UDC: 523. 3. 34. 39
UR/0026/66/000/006/0006/0018
r
ACC NRt A P-don-1-9-0
talassoids, unusual ring-shaped depressions on the back side of the moon is
discussed, and the continental formation of the lunar surface is confirmed. The
new phase in lunar exploration which started with the Inilding of Luna-9 on tile
moon is discussed. The luna soil is found to have high porosity and extremely
low heat conductivity. The space soundings of the US Rangers are describeVriefly.
The discovery of "dimple-c raters" is explained. The mission of "Luna-10" is
analyzed, and forecasts on the scientific program of lunar exploration for 1975-
1985 are given. Orig. art. has: 10 figures. [GC]
SUB CODE: 03L22/- SUBM DATE: none/
C.,d 2/2MT
L 04105-67 _ EWT(1)/T/F'-'; -2 JJP(c) JGS/GW
C NRs AP6033175 SOURCE CODE: IJH/0033/66/043/005/'1111/1118
AUTHOR: LIRskty4 Yu. N.
ORG: none 6
TITLE : Names of formations Identified on the far side of the moon \r'~'
SOURCE: Astronomicheskiy zhurnal, v. 43, no. 5, 1966, 1111-1118
TOPIC TAGS: moon, lunar surface, lunar photography, lunar landing, satellite
/Zond-3
ABSTRACT: Following a discussion of all available materials, the Commission of
the Soviet Academy of Sciences for naming formations identified on the dark side Qf
the moon approved 150 names and 149 biographic references to scientists for whollp
v~rmations were named. A full list, Including coordinates and diameters of the
f4rmations, to included in the original article. The formations were photographed'
b~ Zond-3. An outline map listing the objectives named and a photograph of the
irea are also given. The Commission decided to suggest names for two regions
located on the visible side of the moon, on which the firat hard and soft landings
occurred. Orig. art. has: 2 figures.
SUB CODIE~hO3,14,22/ SUBM DATE: none/
Card UDC: 523. 39
A C C NIR -AP6030231 SOURCE CODE: UR/0030/66/000/008/0044/0050-
AUTHOR: Lipskiy, Yu. N. (Doctor of physico-mathematical sciences)
ORG: none
TITLE: Outstanding achievement of Soviet astronautics
SOURCE: AN SSSR. Vestnik, no. 8, 1966, 44-50
TOPIC TAGS: lunar landing, lunar photography, lunar surface, lunar flight
ABSTRACT: This article is a stmimary and review of the Soviet book entitled Pervyye
panorc;ry lunnoy poverkhno3ti (The First Panoramas of the Lunar Surface). The follow-
~ing topics in the book are reviewed: the landing of the Luna-9, the equipment of
Ltuia-g, the panoramic photographs made by Luna-9, the nature of the rocks observed*by
Luna-9, the nature of lunar relief and lunar craters. The feat of the Luna-9 in attri-
buted in :.arrge measure to the efforts of the late S. T. Korolev. Orig. art. has: 3
photographs.
SUB CODE: 22/ SUBM DATE: none/ OTH REF: 00"~
UDC:
ard 1/1
A
MCC NR:
-A-117 30549 COD1," :U i/0293/ /,C~6/0) 12/0)22,
j_T4o_ N.; Pskovskiy, Yu. P.; Gurshteyn, A. A.; Shav-`. V. V.;
AUTHO-IS
Pospergelis,
07ZG: none
TITLZ: Current problems of lunar surface morpholopj
SOURCE: Kosmicheski-ye issledovaniya, V. 4, no. 6, 1966, 912-922
TOPIC TAGS: moon, selenography, lunar crater, lunar probe, lunar satellite, lunar
surface, lunar topography, morpholoa, astrononW, mars planet, mars pr,~be
ABSTRAUP: In this profusely -illustrated article use is made of photoC:--iphs ta1-en by
"Zond-3, " "-'una-3, " and the American satellites to analyze the surfac.-, featurei of
the moon and to comnare the moon with other celestial bodies. The svu-face of the moon
is divided into coniinental and marine moses. These are described --uit-i classified
according to their sizes, shapes, and locations, as are craters, mount;:.in ranges, and
Older hypotheses pertaining to the inv-:.--ble lunar
radial 'issures (see Fig. 1). 1.i L
hemisphere are either sustained or di.8pr-.ved. Newly discovered deprei:.~;-ons on the
invisible hemisphere are discussed, and their origin is hypothetically explained. The
impact theory pertaining to the formation of the lunar relief is criticized on the
basis of the regularity in the location and distribution of many features. The
analogy between the lunar and the Martian surfaces is analyzed and explained W*ith the
Card 1/3 UDC: 523-34
ACC NRi A?7WO549
7.
A.A,- 11-:1
W
L
e-I A
.4
.7 7.,.
:7#
4
Fig
Continental -r-6-Stion --be"mm
crater with a radial systemin 04~ Oc9anus ProcellaT=-and-Mare Ori-entale. Bright
-lower right of the phbtograph i ir A.
illustration represents a re--ctifi~~Gn of a photograp4 gium T"'is
Card 2/3 taken from the earth and
UNIOEII-SY *J--,- Franz (Der mond. -2 te~ ,
1912)
ACC NR:
help of photo,-,raphs taken by `,:,-riner-4, and the problem2 of e
'tacked in ihe future are sugoe3t,~:d au- F.
~ -hr- ~hora thank L. Ln.
a
Rodionova, and V. V. Novikov, co-workers a'. the Division of Lunar and -,-axletai7
Physics of the State Astronomical Institute J-m. P. K. Shternberg (0-ILIde-- fiziki Luny i
planet Gosudarstvc.--iogo astronomicheskogo instituta), for their help. -,Tig. art. has:
8 photogra,)hs, 2 charts, and 1 table.
SUB CODE: 03/ SUBM DATE: O7jul66/ ORIG RU: 004/ OTH REP: 019
SLOY, A., RIFDL. 0. ; technicka upoluprnco: ANTOS, Sl.; LIPSKY, A.
Body weight and body height in old patients in Czechoslavakia.
Sborn.lek.63 no-1:11-17 A 161.
1. IV. interni klinika fakulty vooobeennho lekaretvi Univorcity
Karlovy v Praza, Drodnosta prof.dr. M.rucik; II. patologickoana-
tomicky ustav fakulty vaeobecneho lekarstvi University Karlovy v
Praza, prednosta prof.dr. V.Jedlicka.
(BODY WEIGHT in old age)
(BODY WEIGHT in old age)
- - * -, A, dat 4 chpr-~." --j,
i . .. I i-:r, B.-I.. :-ardidat takhricivtn'117h
4 nauk.
~.fifiio rrtlny I iro,)n, n ripw *r--O l... - ---, -:!, et, nr4,IrLNo~rtnj-. i'rlroui
46 j! 1-
(: :?A 10- Q',
I r3 r! lay ~. . ~7 +I-;-.---- ,
UPSMAN, Z. P.
Lipsman, Z. P. - "Clinioo-Roentgenological Characterization of the ~%ndlln.,Iar
Joint tn the Case of Various Forms of Occlusion." Min Public Health RSFSR1
Moscow Med Stomatological Inst, Mozeow, 1955 (Dissertation for the Degree
of Candidate of Veterinary Sciences)
SO: Knizhuaya Letopist, No. 24, Moscow, Jun 55, PP 91-104
-LIMON,, )JIM;L4, mgr inze; PALUSZKIEWIGZ1 Bronislawa, mg-r; MWAMIKA,
Helena, mgr inz.
Used_~ngipe oils and their recovery, Rafta Pol 19 no*5:
117-M My i63.
1. Centralne Laboratorium Technologii Nafty., Warazawa.
P1011V631042100310021003
Resistance of D204/D307
g,ains in veight in the presonec o' petrolcm:i oil 1)roducts -...,cre very
low. concluG3.011c': C-,)O..Y-j)olYjVjj.4Cjo. and cpo:.-y-mclaviinc lacquers are
practically iinsolubic in -nctroleum products but i-.iay a'bsorlb small
amou-,its of hydrocarbons on prolon,~(,d heati-cv,. They are in
hot polar scIvents, rrmll in benzc~n'c; adliesion iss _,cslz on
sandblasted ancl --hosphated-, Gur-faccs, but is sstc Tit on greasy
mctals. The coating was thm sprayed in 5 layers onto a sandblasted
"I L
experi,mental cistern 2301?, was liardened at 35-500r', and was still
intact after I year of cmploitation. The lacquer is therefore suit-
able for protecting steel cistzrns against water and other substances
occurring in mi-acral water. There are 2 tables.
,iII,S,';Qv-AI,,'GION Centralne Laboratorium TecIrmologii Nafty, Uddziax
117 iiarsZaV71C (Central Laboratory of Petroleum Technol-
ogy, Warsaw Department)
S U iTi , I I T'fZ D." iu,-Iust 7. 1962
Card 2/2
r rl
t.3
Vi
YVI;
Ce me r, t i nf.., anci lcwerli-.~ I.-e oeccricl, intermedlate s*~r-..g---Ji.?
the deep Aral-Sor well No.l. isuren!e no.2:26-271 165.
Trer,' "Fra
Knlsncf,r~ ',ra .. eni, jn;iLiL::*,
akadenlik.LL Cubkinti.
BRUMSHTLON , H.S., rjrof.,- LIPSCII, E.D.
Work of the Aatrak'aan Soc-lety of' Fathoanatomi54a fcrr 1959-1962.
krkb, pat. 25 no-8294-95 163 (MIRA 17 24)
1. Pred,3adatell AEA-z-akhanakago obshchesLva patologoanatomo-r
(for Rrjaiahte~ii). 2. SoAre-tarl Astrakhanskago obahchestre pa-
tolog6anatomov (for Lipson).
LIPSON, E.D. (Astrakharil ,)
Angiography of the brain in sl,J,llb~rn infants and -jead nemates.
Arkh. pat. 27 no.3:65-71 165. (MIRA 18:5)
1. Kafedra patologicheskoy anjLomiL (zav. - prof. M.S. Brunshteyn)
Astrakhanskogo meditsinskogo instlLuta.
Z1111,111SKIY, K.A., kand.tekhn.moik, dots.-, LU'JON, G.t%., !j1;i1r!1hiy propcxluvatijil
Usin,- sW)s in corstriicting foiindation bases on qriicksand.
3bor.trw1.V1Si no.4:4?-51 '58. (MIR& 12:8)
(Folintlat i anti) (Soil mochanics)
LIP50111 G.A., propoda,ratol'; ALPKS:1Y1"T, V.M., prepodavrital'
Instrument for determining tho nontnnt of moisture in sollo.
Suggested by G.A.Lipson, V.M.A1e1csee-/*. Rats., iznbr.predl.v
stroi. no.16:104-107 160. (MIRA 13:9)
1. Voronezhalcly Inzhenerno-atroltelinyy institut. Voronezh. ul.
XX-lotlyR Oktyabrya, d. 146-a.
(Moisturo-Moasurement)
UiICLOV, A.K.; ALEVMEYET, V.1%; LIPSON, G.A.; 1,:E:..W,'OVA, G.F., red.
i.zd-va; J111111KOVA, T.M., tekhn. red.
(Soil ii.oisture and present rethods of detemi ining it'j';I-azzb-
nost' gruntov i sovremonnye metody ee opredeleniia. Moskv~--,
Cosgooltekhizdat, 1962. 133 p. (FJRA 15:11)
(Soil moisture)
-ning -he qrIc-,e 'ry
on 10053 Solls." Nn. ")in,i.L in-kh.j!.. Tin. o
LIPSOU, Yu. P.
Treatment of chronic highmoritis with iodolipol. Vest. otorin.
no.2:83-86 162. (MIRA 15:2)
1. Iz kafedry bolezney ukha, gorla i nosa Nav. - prof. I. M.
Burakov) Astrakhanskogo gosudarstvennogo moditsinskogo instituta.
(COUTRAST M::DIA) (MAXILLARY SIOS-DISEASPS)
LIPSON, Yu.P.
State of skin capLiLlaries in some otorhinolar,"gologic&l dise4effo
Zhur.ush,,nos,i gor.bol.22no.6al9-23 N-D'62. (MIRA 1617)
1. Iz PrivolzhBkoy rayornoy bollnitay Aatakbanvl,-:- - !!,lti
I--
nyy rukovoditall- zave kafedrou bolezray ukhu,govia - Astra-
khanskogo meditsinokogo instituts. prof. I.M.Hurskov).
(0T0nHn;OlATBG0WGY) (CAPILLARIES-PMMABILITY)
A
Poland /themical Technology. Chemical Products 1-15
and Their Application
Treatment of solid mineral fuels
Abs Jour: Referat Zhur - Khimiya, No 9, 1957, 31827
Author : Lipszynski Stefan
Title : Ways of Increasing the Benzene Output of Coking
Plants
Orig Pub: Koks, 8mola, gaz, 1956, 1, No 3, 90-92
Abstract: The possibilities are considered of increasing
the benzene output of Polish coking plants,
essentially in two ways: 1) by intensifying the
process of coke gas cooling (and if difficulties
are encountered -- by increasing the amount of
absorbent oil utilized in the benzene scrubbers)
and benzene recovery from the oil absorbate;
C ard 11,42
Poland /themical Technology. Chemical Products 1-15
and Their Application
Treatment of solid mineral fuels
Abs Jour: Referat Zhur - Khimiya, No 9, 1957.. 31827
2) by increasing the benzene concentration in the
coke gas; it is noted that the last mentioned
measure can be effected by regulating the coking
process (by adjusting the degree of comminution
of the batch, more uniform heating of the furnace
chamber walls, etc), and to a still greater ex-
tent by introducing into the upper portion of the
furnace chamber petroleum residues, especially
residues that are rich in paraffins.
Card 2/2
I'C' -3 a(! -to Y'TIO 'TP 71-~
p, ti
-LIFTAK, Ferenc, dr., okleveles mernok, adjunktus
Spra.( distribution of sprinkler irrigation in case of different
nozzle patterns. Vizugyt kozl no.3:369-403 '62.
1. Epitoipari es Kozlekedesi Muszaki Egyetem I.sz.Viz-
apitestan! Tanszeke.