SCIENTIFIC ABSTRACT TEXL, A. - TEYFEL, YA.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001755520003-3
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: March 14, 2001
• Sequence Number: 3
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

A.- LTELXL,,- Department of Pharmacology of the Medical Faculty of the J.E.
Purkyne Universitv (Farmakoloplicky ustav lt.karske EakulLy University
J.r. PLIrkyne) 11caa (prednosta) J. SAXIER, MD, CSc; Brno.
!'Eff-~cc of the Tea-Leaf Catechin Complex on Experlmental Inflammation."
V~nguL, ~a-O-Ir-i-'Lellcaru Ceskych, Vol 102, 1-11o 19, 10 May 63; pp 515-519.
Ab5tract [English surmnnry modif ied]: A Soviet -pr epa red tea tannin complex
when a(Iministered s.c. or p.o. at 100 mg /Kg along with 100 r.- 'K3 of
~zcorbic acid, significantly depressed hyaluronidase, cotton pellet,
-;oxnimlin or seroLonin granuloma in rats. Tannin with vitamin C also
si,-,nificantly increased urinary 17-ketusteroids. Tannin alone had no
"fec,
Eight graphs; 9 Western, 3 Soviet and 7 Czech references.

TEXL, Arnost , I
Effect of tannin on the activity of the utervs. Ser. mod. fac, mod.
Brunbnais 34,n'o.0'.3:99--207 '161.
- (UTERUS pharmacol) (TANNINS pbarmacol)
- -. I

PROCHAZKGVA-FRANKOVA, H.; TMI, J.
Effect of tarmin on hemorrhagb and Quick's prothrombin time.
Ser. Md. fac. mad. Brunensio 36-n0-5:21+9-257 163.
lo FarrakologicI7 ustav lelmrske fakulty university J.E,,
PUrkyne v Brno. Vedouci3 MUDr. Josef Sajner, C.So.
(TANNINS) (PROTHROMBIN TIME) I M ORRHAGE)
DIJECTIONS I INTRAVENOUS)
INJECTIONS, SUBCUTANEOUS)
~

M NR; AP6006094 RCE CODE: CZ 53 5/0114AY04/0317/0318
AUTHOR: Texl A.
"tf)
ORGO. Medical Faculty, Institute of Pharmacology, J. E. Purkyne Universityi, Brno
(Farmakologicky ustav lek. fak. university J. Ev. Purkyne)
TITLE: Mechanism of anti-inflmmatory effect of tannin [This paper was presented
during the Twelfth Pharmacologic Days, Smolenice, 26 Jan 65.1
SOURCE: Ceskoslovenska fysiologie, v. 14, no..4, 1965, 317-318
TOPIC TAGS: mouse, endocrinology, gland, carbohydrate, pharmacology, SLr~effect;
-ABSTRACT; Study in hypophysectomized and adrenomedulectomized mice with sterile
experimental granulomas indicates that the antiexudative effect of tannin requires
the presence df adrenal medulla and that its proliferative effect requires
activation of the pituitary-adrenal axix. Orig, art. has: 1: figure. (JPRS1
SUB CODE: 06 / SUM DATE: none / ORIG REF: 005
jrn

CZ7V CHOSLOVAKIA
M-L,-A~_; KONECIN, M.; Phar-macological Institute and Chair of Radiology
and Nucl6ar Medicine, Medical Faculty, J. Ev. Purkyre University
(Farmakologicky Ustav a Katedra Radiologie a Nuklearni Mediciny Lek.
Fak. UJEvP), Brno.
"On the Ilepatotoxic Effect of Acidum Tannicum.11
Prague, Ceskoslovenska Fysiologie, Voa 15, No 5, Sep 66, p bi-o
Abstract: The influence of tannic acid on tbe functioning of the liver
Ma-sij~v-estigated with respect both to the dose and the manner in which
it was administered. Experimentz on rabbits showed that 5C0 mg/kg of
tannin impaired the functioning of the liver after 1 and 2 days, Lower
amounts of tannin did not have any offect. Amounts of 500 and NO rng/kg
resulted in a decrease in the glycogen content of the liver, reduction of
the fat content, and ultirrately in a parenchymal degeneration. 6 Western
references. Submitted at 14 Days of Pharmacology at Smolenice, 16 Feb
66.
1/1

TEXL9 KIP inz.
The role of the Czechoslovak Scientific Technical Society in
introducing new techniques. Energetika, Cz 11 no.l:Suppl:
Energetika, 3.1 no.l:/+ 161.

inz.; KRENEK, Josef, inz.; BAYER, Vilem, inz.; PAGAK, Slavoj,
. EXL K
inz.; VYSKOCIL, Vaclav, inz.
The 1964 Meeting of the International Conference on Large
Electric Systems. Energetika Cz 14 no.12:622-644 D 164.

TEXL, Karel, inz.
In the path of best workers. Energetika Cz 13 no.7041-3142
jil 963.
1, Predseda, Ustredni vybor Ceskoslovenske vedecko-technicke
apoleanostiq sekee pro energetiku.

le.

cm"" T Rumnis L

B3. JWR. I ItZhAlal., Is. 1959, wa. 15520
-47nm
r
-ar."Ital. t
2.1,ri:41"U, a - qlsl =0
z
t
O
1
;. tA.') R P,
A'r f t
il
C I . j
Inarl-ised *:'Crtilit;;f 1. ...,U,.1 IS.adOW3 of
ofitern -ountdin$ (PU2ania).
IORIO. TUB. IStUdil al Gorastart -wron. Acm4, M ?11. OJUS,
1957, S. U0.1-2, 99-116
Vo ao6tmct.

*Drepen, vicrica

"'IFIT-M, D.
Juniperus in subalpine meadows. P. 90 NATURA Ducuresti
Vol* 7, no- 3., May/June 1955
SOURCE: MAL IL Vol. 5, no. 7j, July 1956

TEXTER, D.
Juniperus in subalpine meadows. p. go. NATURA. Bucuresti.
Vol. 7p no- 3, May/June 1955.
SOURCE: East'Buropean Accessions List (EEAL) Library of Congress
Vol- 5p No- 79 July 1956o
A

TEYDER, V.
Metal conveyer for freezing meat dumplings. Mias. ind. S"ISR
32 no.1:10-11 161. (MLRA .14:7)
1. Len:Lngradskiy tekhnologicheakiy institut kholodillnoy
promyshlennosti.
(Leningrad--Meat industry-Equipment and supplies)
(Qonveying machinery) (Automatic control)

TEYDER, V.A.., inzil.
Food freezing on a metal sheet. Khol.tekh- 40 no.3:33-36 llly-je
WIRA 16:9)
1. Leningradskiy tekhnologicheskiy institut kholodillnoy promysh-
lennosti.
(Refrigeration and refrigerating machinery)
(Food,Frozen)
163.

TEYDERI V.A., inzh.
Time needed for the freeziW of products laying on a ribbed
surface. Khol.tekhe 39 no.6:37-42 14-D 162. (MIRA 15:12)
1. Leningradskiy tekhnologicheskiy institut kholodillnoy
promyshlennosti.
(Food, Frozen)

TEnEft, V. A.
ODetermination of freezing ftme under variable corAitions of heat
exchange aver body surfaces**
Report presented at the 31th International Congress of Refrigerations
(IRR), Munich, West Germany, 27 Auc-4 Sep 63.

KOZLOV, I.To, dorozhuy7 master (stantsiya Kift Tashkentskoy dorogi);
TIMIRZ., A.Ve, dorozhny7 master (stantsiya Elva Fistonskoy dorogi);
PONUD, P.I., brigadir puti (stantsiya Perm' ); LOGTIN, F.G.;
NIMU, R.Ta.; PMNIX, N.M., dorozhnyy master (stantaiya Almaznaya,
Donetakoy dorogi); TIMDyxxlV, S.
Give us an answer. Put' i put. khoz. no.5:41-42 My 158.
(KRA 13:3)
1.3tarshir dorozhny7 master, stantstya Beahtau. Ordzhonikidzevokay dorogi
(for logvin). 2. Nachalinik distantaii, g.Pyarnu (for Ilukica). .
3.Starshi.v doroahnyy master, atantelya Karachev Hookovsko-Kiyevoko3r
dorogi (for Timofeyev).
(Ballast (Railroads))

OLILEKOP, Yu.A,, BTUNA, G.S.; GRAKOVICII, L.K.; BULOYCHIK, Zh.l.; TEYF,~_~~-
S
Acyl peroxides, Part 7t Sypthesis of asymnetrical diacyl peroxides of
aliphatic and hexahydroaralyphatic series. Zhur. org. khim. 1 no.2:82-
86 Ja 165. (MMA 18t5)
1. Beloruaskiy gosadarstvennyy universitet im. V.I.Lenina.

Tilly It V. (g.Shcherbakov).
Anomalous distrIbution of the aurora polaris. Aatron.tsir. n0,105:13 3 150.
(HUU 6:8 )
(Aaroras)

T,,,'Y F ". t I ) V.
Auroras
More about the aurora polarls of 28 October, 1951. AsLron. tsir. No. 123, 1952.
9. Monthl List of Russian Accessions, Library of Congress, May 1952 _ 44w, Uncl.

1. TCYDF,-1, V.
2. U33a (600)
4. Meteors
7. Observations of Lyraids mde in 1952 in Goi~kiy. Astron. tsir., No. 128, 1952.
9. Monthly List of Russian Accessions, Library of Congress, Kay -1953. Unclassified.

CHISTYAKOV. V.V.; TzT.FAI, V.G.
Visible boundary of noctilucent clouds. Astron.tsir. no.139:
9-12 je '53. (MLRA 7:1)
(Clouds)

'UYFSLI , V.G.
%-WAW_"!i2 IW~'
Meteor "swarms." Astron.tsir. no.138:11 My '53. (HLRA 7:1)
(Meteors--April)

TZI I, V*G*
Lunar eclipse of January 29, 1953. hatron.tsir. n0.135:18-19 F '53.
MWU, 6:6)
1. Shcherbakovskaya Astronomiabeekaya (lbeervatoriya.
(Zolipses, lunar -- 1953)

TAX 1, V.G.
Aids in the study of astronomy. liz. v shkole 13 no.4:74-75 Jl-Ag '53.
OffJU 6:6)
1. Ysesovuznoye Astronomo-Geodezicheskoye obahchostvo Gorlkiy.
(Astronomy--Study and teaching)

TMMI. V.G.
,Noctilueent clouds in 1953. Astron.tsir. no.142:12-14 5 153.
(VLRA 7:7)
1. GorIkovskoye otdoloniya VAGO.
(Clouds)

TJIYFJILI, V.G.
Aurora borealis soenbrom Gorkiy. Astron.tair. no.144:18 D 153.
NLRA 7:6)
1, Gorlkovskoys otdolonlye TAGO.
(Auroras)

Tly LI, V.G.
Noctilucent clouds in 1954. Astron.tair. no.154:16-17 1 154.
1. GorIkovskoys otdqleniy* VAGO, (HLPA 8:6)
(Glouds)

MRLI t M*
7EYMI , V.G.
'_
Observations of noctilucent clouds. Astron.tsir. no.149.25 My 154.
Off-RA 7--7)
1. GorIkovskoye otdolonlye VAGO.
(clouds)

VIdNe border noctitucerit cloads
addy-go'-Taue Altr" AV", Z-40 14!~
Zhu-K-Affirox. i S No
Refaff-Z - 7 M.1g; 1. illo if thl;
UpDcr border Of the apparen! height of ~octifucent clouds is
r detd. by the action ot ithravlolet tud6fion from the sun and
the screening effect of an 01 layer. then the height of thevi
effective (h layer depend3 on the phAm of tht %oW activity
;cycle. During the period of max, solar activity, MF 45-
'integration of Os'mals. under the effect of radiation of the
w9kyt-length range 22OG-31W A. It greater !n the terrestrial
1 Min, than In it period of min. activity, Radiation of 1300-
18W A - penetrates more deeply, -fortnius at. 0. Thus,the
height of the Or Layer decreAs" in the .od of ru.'", solar
,activity atw Increases in the period ; mitt. activity, and
idoes not remain at % height of 30 Ian., as was thought
fearlier. The height of the Off layck Is caled. 5y the fornsula:
H(:i:A) - 30 810.66 sin A kru., wherc is is the
variance In height of Vie effective 0, layer from the 30 Irm.
level; parameter A is found from the table published (-arlier
~(Referat.Zhur.;Astron.1053,No.1347). latheyearnfinnx.
'solar artivity, -.40'; In the year ofmiu. activity,
I% corresponding heights of the Or layer fire 20 and
ASLu;. Sometimes in Off: period of ruin. solar Activity the
tngtilarheights of the upper border of noctilueent clouds
't , tisfy the hypothesis of "a ray, tangent to the r~Arth's
surf2ce." . Anornattfus cas-A are diwm;, when two
-cd,
borders of noctilucent clou,45 are observed, tine over the
other, daring whi. solar activity- Thelow" border ti, fi
the hypmhe~;eti of the skrccaing of ult-raviolet b; "'.1
't 34 - Of "4 MY,
01 L'Iftf; IN UPPfr tAlPh , t1firM5 Oft hYPU111014
(AURCht to tht "fill'A illff,14,4r~"
TIM, for fiM(jjuV4N4j
clouds the connection tictwven .1 and IV. Wolf's 110, It In oil
prol-fability the ennticrtion betwezzi the height of lite eff".
tive 0, Liyer aral solar activitY. f Marjorie Kttiier

X&RMXNKO, V.V.; PIMOV, Tu.V.; TEYMI, Y.G.
Ivrids In 1952. Biul.VA" no.16: 28-33 155.
(Mat 8:6)
1. Moskovskoye otdeleuiya VA30. meteornyy otdol; Gorl- "
kovskoye otdoleniye TAGO.'sektalya nablyadateley4 Sim-
foropollskoye otdoleniye VAGO. Moteornaya stantsiya imeni
G.O. Zateyshchikova pri Mrymskoy statsit yanikh tekhnikov.
(Noteors--April)

TRYFELI V.G.
Reduction coefficients for photometric obseryntione of noctilucent
clouds, Astronoteir. no,159:25-27 MY'55. (MLRA 8:12)
1. Gortkovskoye otdelenlye Vsesoyusnogo astrono-geodezicheakogo
obahchestva
(Photometry, Astronomical) (Clouds)

~ r- . I
I C--- -,,, I- --,~- , Y ,--- ,
6HISTY,AKOV , V.P. (Kaliningrad); TSYFRLI, V.G. (Gorlkiy)
-- -
Nature of noctilucent clouds. Biul. VAGO no.19:17-30 156.
(MLRA 10:3)
(Clouds)

TEYFELI, V.G*
Noctilucent clouds. Nauka i zhian' 23 no-7:49-50 JI %56.
(Cloude) (Km 9:9)

TITMI, V;G.
of the partial lunar eclipse of Novesber 29, 1955.
.Astron.tairk. no.168:21-22 156. (MLaA 9:5)
1. Sektor astrobotanM AM Kas.MM. Alm-At&.
(39clipmes. Lunar--1955)

TBYYJILI, V.G.
Noctilucent clouds in 1955. Astron.tairk. no.168:23 '56.
(MLRA 9:5)
1. Sektor antrobotaulki AN K&s.SU, AlmmmAta.
(Clouds)

1
Noctilucent clouds. Trudy Sakt. astrobot. AN Xazakh. SSR 5:59-82 '57
(Clouds) (MIRA lOrA--)

0. /,.,; 0 3OV/35-59'-M44
Translation from: Referativnyy zhurnal, Astronomiya i G3odeziya, 1959, fir 9, p 60 (USSR)
AUTHORS: Teyfell, V.G., Teyfel!, Ya.A.
0
TITLE: A Trial Svectrophotometry of Saturn
PERIODICAL: Astron. tsirkulyar, 1958, Jan 11, Nr 188, pp 14 - 16
ABSTRACT: At the Observatory of the Sector of Astrobotany AS KazSSR in June 1S57,
the spectra of sections of Jupiter and Saturn were obtain;d with the aid
of an jgT- Itelescope, a magnifying camera and an ASP-94pectrograph.
The width of the spectrum of Saturn and its ring equalled 2 mm. The
microphotograms were measured on the If-Vapparatus within the limits from
400 - 590 m I.A- at 10 m f,- intervals. Tables are given of the ratios of
monochromatic intensities of the ring and edges of the disk to the intensity
of the center and the ratios of the intensities of the brightest zone of the
ring to the intensity in the center in different rays. The absolute values
of the color indices of the same sections of the planet and its ring were
obtained by comparing them with them 'q Oph spectrum. The obtained data are
contained within the limits from +0 .76 (E - the ring), and +1m.28 (center
Card 1/1 of the disk). I.I. Lebedeva

/,F;.) 0 69867
G./S,S-G SOV/35 59-9-7249
Translation from: Referativnyy zhurnal, Astronomiya i Geodeziya, 1959, Ur 9, p 61 (U33P)
ATYrHOR: Teyfell, V.G.
TITLE: On the Normal Color Indices of Lunar objects
PERIODICAL: Astron. tsirkulyar, 1958, May 26, Nr 192, pp 21 - 23
ABSTRACT: The spectrograms of the M8on obtained during 1957 - 1958, were measured on
the MF-4 microDhotometeAducross the dispersion at wavelengths of 550 and
443 mu.. By comparing to the spectrum of 10~ Aur a catalogue of normp-6L color
indices of 262 small sections of the lunar surface has been compiled. Each
value of CI is based on the measurements of 10 - 14 spectrograms. The color
indices are contained within the limits +0.'76 - +0'.97, their mean value is
+0.m85, the mean yellowness index is +0m28. The relation between the color
and brightness of lunar objects is confirmed.
N.P.K.
Card 1/1

69868,
SOV/35-59-9-7250
Translation from: Referativnyy zhurnal, Astronomiya i Geodezlya, 1959, Hr 9, p 61 (U53R)
AUTHOR: T~!ytej~,Y_G.
TITLE: On the Color-Versus-Brightness Relation for Sections of the Lunar Surface
PERIODICAL: Astron. tsirkulyar, 1958, August 26, Nr 194, pp 11, - 13
ABSTRACT: The spectra of Mare Serenitatis and Mare Tranquillitatis, obtained with a
high slit, were measured in 11 sections relatively to the reference point
located in Mare Serenitatis. The color excesses, CE, and the relative
brightnesses, lgj of these sections are given. All the data, with the
V200,
exception of 4 ues for the Sea of Brightness, confirm the correlation of
CR to lgj 500 which was established earlier by the author. It is shown t1nat
the relation is satisfactorily represented by theoretical curves, obta--i-led
under the assumption that the connection between the color and the bright-
ness is caused by the merging in different proportions of two substances,
each possessing a different color and brightness. The most probable expla-
nation for the existence of the color-versus-brightness relation on the
lunar surface is the assumption that originally, the whole crust of the
Card 1/2 Moon consisted mainly of bright, reddish and possibly acid rocks, Wit-h th
I '~~
vt

69868
SOV/35-59-9-72,1zo
On the Color-Versus-Brightness Relationfor Sections of the Lunar Surfae-'e
formation of the seas, the eruptions of dark lava flooded the remains of the crust,
and fusing with the bright substance, formed sections with different reflecting and
polarizing capacities and of a different color. Thus the color-versus-brightness
relation is probably connected with the inner processes.
N.B. Perova
Card 2/2

69869
ST-r/35-59-9-7254
Translation from: Referativnyy zhurnal, Astronomiya I Geodeziya, 1959, Nr 9, pp 1,51 - 62
(TuSSR)
AUTHOR: Teyfel-'V G.
TYM-E: The SpectrophotometX7 of Vesta
PERIODICAL: Astron. tsirkulyar, 1958, September 18, Nr 195, pp 3 - 5
ABSTRACT: Spectrograms were obtained during April - June 1956, on the BredlkhLn,
astrograph with a lens prism of V - 130, A spectral curve of the Vesta
was plotted in relation to a star of the GO class from the 4 best negati-ves
obtained In April. For each negative a spectrophotometric gradient of Vesta
in relation t'o a A2 star was determined for tin interval of 3E.0 0 M 'u,
u- a' ?L k-,? 500 InJA
An explicit change of the magnitude of the gradient of Vesta t
was observed. The gradient of Vesta in rela-t-ion to a F5 star in the inter-
val from 380 - 460 m I.,, obtained on July 13 - 14, 1956, for a whole series
of zpectrograms, systematically decreased from 1.57 to 0.76. The length of
Card 1/2 time during which the gradient diminished (3 hrs) is near to lvtlf the periol
I*-

The Spectrophotometry of Vesta
69869
SOV/3-45-59-9-7254
of the fluctuation of luminosity. The spectrum of Vesta is characterized by a maximm,
intensity at about & 480 m/4 and by the decrease in intensity towards the violet and
especially towards the red edge of the spectram.
M,V. Savel'eva
Card 2/2

SOV/315-59-9-7231
Translation from: Referativnyy zhurnal, A-=trono?n!7a i Geodezlyal 1959, Nr_ 9, P 61 (11751~-'F)
AUTHOR: Teyfell, V.G.
I
TITLE: On Spicti~gfl)ifferences Between the Sections of the~6=_ar Surface
PERIODICAL; Astron. tsirkulyar, 1958, October 16, Nr 196, pp 6
ABSTRAGP: From the spectrograms 0.1 the Moon obtained by the Se3tor of, Ast-robotany
of the AS Kaz3SR, spectral our-res of 90 sections of the lunar zurface ha'7e
been plotted in relation to the reference section, in Mare Vaoo-rim. 'rqe
spectrophotometric gradients at &?~. 390 - 620 m p. are given of :the most
characteristic morphologicall groups of lunar formations: sea regior-S,
continents, mountain formations., craters, rays and aureoles of the or-aters.
The existence of the color-versus -brightness relation Is con-fi-nmed ff%~r, t1--e
lunar surface.
N.P.K.
Card 1/1

1 tUll

TIMLIt T*G9
Distribution of Intensity on Jupiter's
absorption bands* IsToKOMI-PO fl4plan.
(Jupiter(Planot).Speetre)
disk in methane
'no 1-193-104 159-
ZKIM 13:7)

TICYWILI V.G.- TRYINLI, Ya.A,.
Experience in the spectrophotometry of Saturn. Tru4 Sekt.
astrobot,AN Kazakh SSR 7:64-68 139. (MIR& 13:5)
(Saturn(Planot)-Spectra)

TICYFEL, V.G.
Spectrophotometry of the soon's surface. Trudy Bekt.astrobot.
AN Ka2akh SSR 7:69-83 '59. (MIRL 13:5)
(Noon--Spectra)

KUPO. I.D.; TEYVNLI, T.G.
Some results of obsel, tions of Arend-Roland's comet 1956 h.
Trudy Sakt.astrobot.AN Usakh SSR 7:93-107 '59-
(MIRA 13:5)
(Comots,1956)

'TBYFBLI..V.G.
Color Index of Mare during the oppoBition of 1958. Astron.tsir.
no.202:1 Je 159. (MIRA 13:4)
1. Seirtor astrobotaulki AN KazSSR, Alma-Ata.
(Hurs(Pianet))--Oppouition. 1958)

-Txf7xLl9 V.G.
Color Index of Kars during the 1958 opposition. Astron.tslr*
no.204:10-11 S 159. (NIRA 13:6)
1.Sektor astrobotaniki AN KmzSSR.
(Kars (Planet)-OPposition, 1958:)

33,300
3.19S_0
83442
S/0,35/60/tOO/00 7/012/0 18
AOO 1/AO0 1
Translation from- Referativnyy zhurnal, Astronomiya i Geodeziya, 1960, No. 7,
P. 77, # 6452
AUTHOR: T
TITLE: On Spectral-Polarization Properties o~ Lunar Surface
PERIODICAL: Astron. tsirkulyar, 1959, okt. 15, No. 205, PP. 7-8
TEXT: During June-July 1959, the author took 108 spectrograms of 12
sections of the Moon with a 220-mm A?jT -7 (AZT-7) telescope near quadra"u'res.
In taking the spectrogra.,ns, the polarold, mo-anted in front of the Epectrograph
slit, was placed in three positions (position angles: 00, 600, 1200). Mono-
chromatic values of polarization degree Pk were calculated by V.G. Fesenkovis
formula (Astron. zh., 19,35, Vol. 12, No. 4, p. 309). The F,,k -valuee decrease
with an increase of wavelengths. In the range ), 4 420-620 m-1A the decreaze
amounts to 5-7%. The Pk -value in the spectra of lunar formations varies in
Card 11'2

63"2
S/035/60/000/007/012/018
AOOI/AO01
On Spectral-Pol-arization Properties of Lunar Surface
correspondence with the monochromatic values of their albedo, obeyIng the same
empirical relationship as the polarization in integrated radiation.
V.P. Fedorovich L/\/
Translator's note: This is the full translation of the original Russian abstract.
Card 2/2

L-,, Y f"-, L I'. L:L -
- , '. .) ~ i;~' ~' ! I I I . '.- I - 1-
~-, ~,:xf~ --.e, " Leingrgd, 1960, 10 pp., 250 cop. (Main Astronomical 0b-
servatory, AS USSR) (KL9 45-60, 122)

PHASE I BOOK EXPLOITATION SOV/5645
Teyfell, V. 0.
Spektrofotometriya poverkhnosti luny; avtoreferat dissertataii
na soiskaniye uchenoy stepeni kandidata fiziko-matematicheskikh
nauk (Spectrophotometry of the Surface of the Moon; Author's
Abstract of a Disoertation Leading Towards a Degree of Candidate
of Physics and Mathematics) IAningrad, 1960. 9p 250 copies
printed.
Sponsoring Agency: Akademiya nauk SSSR. Glavngya astropomicheskaya
observatorlya.
No contributors mentioned.
PURPOSE : This booklet is intended for astronomers and astrophysicist&
COVERAGE: The booklet is an outline and resume"of the author's
dissertation on the spectrophotometry of the lunar surface.
The author conducted spectrophotometric and spectrocolorimetric
studies of specific areas and objects on the moon's surface,
Card 1/2

Spectrophotometry of the Surface (Cont.) SOV/5645
whose spectral curves and color properties were investigated.
The content of each chapter of the original dissertation is
briefly discussed. Their topics are as follows: Ch. I - seleno-
graphic and optical studies; Ch. 11 - oolorimetry and speotro-
photometry of the moon; Ch. III - photographic registration
of the spectrophotometry of the lunar surface; Ch. IV - quan-
titative determinations of normal indicators of color of a
large number of small areas on the moon's surface; Ch. V - spec-
trograms of lunar details along the line of dispersion; CIL VI -
discussion of the results obtained. A conclusion and a sup-
plement (containing a catalog of the normal indicators of color
of 262 lunar details and a catalog and atlas of spectral
curves of 90 units of the lunar surface) follow the chapters.
The work was performed at the Sektor astrobotaniki Akademii
nauk Kazakhskoy SSR (Astrobotanical Sector of the Academy of
Solences Kazalftkaya SSR). No personalities are mentioned. There
are 9 references to articles by the author which contain the
results of this work.
TABLE OF CONTENTS: None given.
AVAILABLE: Library of Congress (QB591.T4)
Card 2/2 JA/ron/jw
10-17-r6i

T M-TEL, V. C;.
"Color And Spectral PrcpexAes Of The Lunar Surface."
paper presented at IAU SMosiul,. a the Moon., Leningrad, USSR, 0-8 Dec. 6o.
The following conclusions may be made from a spectral photometric study of 90 areas
of the lunar surface.
(1) The intensity of the majority of objects varies smoothly with wwirelength. There-
fore the differences can be characterized uniquely by the color index or color excess.
(2) The color differences on the lunar surface do not exceed OT25 in units of CI.
(3) The formations show a color-brightness dependence. The dependence gradients and
correlation coefficients for different areas of the Moon are given.
(4) The noted dependence is apparently a result of the tectonic evolution of the Moon,
during which the initial lunar crust collapsed and the material of the crust was
melted in different proportions with the darker greenish lava.

AUTHOR: Teyfel', V..G.
35747
S/035/62/000/002/020/052
A001/A101
TITLE: Some results of spectrophotometnj of Uranus
PERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 2, 1962, 55-56,
abstract 2A471 ("Tr. Sektora astrobotan. AN KazSSR", 1960, v. 8,
76-80)
TM: Spectrogrpms were obtained in 1956-1958 at the observatonj of the
Section of Astrobotany by means of an A 3T -7 (AZT-7) telescope with anA C11 -9
(ASP-9) spectrograph (slit width 0.100 mm) on Agfa Spektral Rot Rapid plates.
With the purpose of studying continuous spectrum and absorption bands, spectro-
grams n -24 (P-24) and P-42 pertaining to 1957 and 1958 respectively were
processed on a M45 -4 (Mr-10 microphotometer. Comparison stars were ~1 Leonis
and Geminorum. Intensity distribution in the Uranus spectrum relative to
these comparison stars is presented in the table. Using these data the values
of Uranus color index were calculated for two systems of A ranges: visible
CIV, i. e. containing the effect of absorption bands, and true C'T (expressing
energy distribution in the continuous spectrum beyond the bands), See the table:
Card 1/2

It
S/035/62/0c)0/002/020/052
Some results of spectrophotometry of Uranus AOOI1AIOI
The difference between CIT and CIV
Ranges of 54o - 56o 536 - 576 expresses the effect of methane
spectrum (m,tt 430 - 450 42o - 46o absorption bands which change the

color of the planet toward the blue.
CI P-24 + 1.00 + 1.01 The cause of the difference between
T P-42 + 0.75 + 0.77 the negatives of P-24 and P-42 is
P-24
CT + o.64 + 0.46 not clear. Contours are plotted
V
P-42 + 0.42 1 + 0.40 for methane absorption bands
0
0
60
0
d
4
k~6
'
and 5
, an
19
3
, 597
, 57
equivalent widths are calc ulated with allowance for dispersion, both in a
rigorous way and assuming its mean values. The CH4 band X 5970 is distinctly
divided into 3 components, since it represents the result of superposition of
several vibrational bands. There are 5 references.
1. Lebedeva
[Abstracter's note: Complete translation]
Card 2/2

TgrFILI V.G.
Spectrophotometry of the mon's surface. Pt.2: Catalog of color
indices of lunar objects. Truc4r Sekt,astrobot. AN Kazakh. SSR 8:
130-151 160. (MMA 13:12)
(Noon-spectra)

Tyrml, V.G.
Spoctroph.otometry Of the soonig gurf&co, Pt~3t Differences In
the spectral proportion of lunar formations. Trudy Sekto astrobote
AN Kazakh. SSR 8%152-164 160. (MIRA 13S12)
(Xoon-Spectra)

S/035/62/00/002/021/052
A001/AlOl
3, 0 0 Nr
AUTHOR: Teyfel', V.-G.
TITLE: Some considerations on the state of the lunar surface
PERIODICAL: R.eferativnyy zhurnal, Astronomiya i G&odeziya, no. 2, 1962, 56,
abstract 2A477 ("Tr. Sektora Astrobotan. AN KazSSR", 1960, v. 8,
165-170)
TEXT: The author advances a hypothesis according to which the color-
brightness relationship observed on the Moon is a result of both exogenous
processes, consisting in the fusion of different rocks, and a subsequent super-
position of the products of re-making of the lunar surface acted upon by
meteorites and other exogenous factors. The following simplifying assumptions
are made: continents and mountainous regions on the Moon are composed mainly
of acid rocks, and maria of dark basic rocks; the substance which arises under
the action of meteorites represents a combination of the original rock and some
additional substance which is the same for continents and maria. Optical
properties of the lunar surface are calculated with these data, and the results
obtained are compared with observational results. This leads the author to the
Card 1/2

S/035/62/0rjc)/bo2/021/()52
Some considerations on the state ... AG01/AlOI
conclusion that the lunar rocks could have been similar in optical properties
with terrestrial acid and basic magnatic rocks only in early historical periods.
During the subsequent periods of the lunar history, differences in brightness
and color of the original lunar surface have been obliterated by the action of
endogenous processes. The effect of meteorites and other exogenous factors led
to a further reduction of brightness-color contrasts and to the appearance of
the reddish hue characteristic of the entire lunar surface. There are 9
references.
I. Lebedeva
[Abstracter's note-. Complete translation]
Card 2/2

SIO 3 5/6 21600100 2/0 22/0 5 2
AOO1/A1O1
AUTHOR: TPvfe1__V G_
TITLE: Spectrophotometi-j of asteroids Vesta (4) and Eunomia (15)
PERIODICAL: Referativnyy zhurnal, Astronomiya I Geodeziya, no. 2, 1962, 57,
.abstract 2A486 ("Tr. Sektora astrobotan. AN KazSSR", 1960, v. 8,
171-175)
TFXT-. In April -July 1956, 24 spectrograms of the asteroid Vesta were
obtained in Alma-Ata on a Bredikhin astrograph with'the objective prism UV ( r
130) on the plates: Agfa Astro Panchromatisch, Agfa Isopan ISS and Agfa Spe~_
tral Rot Rapid with exposures from 15 to 60 min. Spectrophotometric tying was
made on the basis of 3 images of stars of approximately the same magnitude,
belonging to classes A2, GO and F5. For the range from X~ 380 to 500 M,LL the
author obtains mean values of the relative spectrophotometric gradient of Vesta
relative to the A2 star, 9VA =+1.73 + 0.07, and relative to the GO star
+0.39 + 0.04. In the spectrum section 'A > 500 M,'~ 9VA'P--O. During the
n%h=t from 173 to 14 June, 1956, 7 spectrograms of Vesta with exposures of 15 min
and 15-min pauses were obtained on one negative, with the purpose of detecting
Card 1/2

S/035/62/000/002/022/052
Spectrophotometry of asteroids ... A00IIA101
possible short-periodic color variations. The spectrophotometric gradient
relative to the P5 star, shown in the table, reveals a gradual decrease with
time (during 3 hours) from 1.57 to 0.76. The spectral curve of Vesta, plotted
according to the four April negatives, is represented by a drawinfr, and a table.
The spectrum of Vesta is characterized by an intensity peak near A 480 m,1, and
reduction of intensity to the violet and especially to the red end. The results
obtained are compared with those of other investigators. Spectrophotometric
gradients in the ran8e from D,400 to 520 m /0- relative to the AO star were
determined from two spectrograms of the asteroid Euno~ia obtained in 1955 with
2-hr exposure. The spectral curve of Eunomia relative to the GO star was
plotted on the basis of two observations. The.color index of Eunomia, determined
m m m
from the AO star, is + 0.57 + 0.02, and from the GO star it is + OM54 + 0.02.
There are 6 references.
I. Lebedeva
[Abstracter's notes: Complete translation]
Card 2/2

TEMLI, V.G.
Golor contrasts on the lunar surface In the visible
spectrum. Vest.AM Kazakh.SSR 16 no.20-77-84 F 160.
KRL 130)
(moon)

A~UTHOR:
TITLEt
83232
S/O33/6O/037A04/oo8/ol2
E03~/9314
Teyfell, V.G.
Spectropolarimetry of some Parts of the Solar Surface
~7,
No. 4,
PERIODICAL% Astronomicheskiy zhurnal, 1960, Vol.
PP- 703 - 708
TEXT: Spectrograms of two regions on the lunar surface were
obtained in June and July, 1959, near quadrature.. The 200 mm
7 was used in conjunction w1th the ASF
telescope A~~ 0-9 ~spectrq'-
graph, in whichca polaroid plate was placed in front o the alit.
The polaroid could be rotated and the spectra were recorded with
the,,polaroid in three positions, namely, y = 0, 60 and 120 09
respectively. The degree of polarization was determined from
Fesenko-wls formula given by Eqs. (1) and (2), where 11. 12 and V11
13 are the intensities corresponding to the three positions of
the analyzer. The degree of polarization was measured as a
function of wavelength. Altogether 108 spectrograms of twelve
regions on the lunar surface were obtained. The coordinates of
the regions are given in Table 2. The monochromatic values of
Card 1/3

83232
S/033/60/037AD4/008/012
EO
,:~ 24
Spectropolarimetry of some Parts e3lkolar Surface
the degree of polarization and-the polarization angle which were
obtained from these spectrograms are given in Tables 3 and 4.
Figs. I and 2 give the monochromatic degree of polarisation as
a function of wavelength for the regions listed in Table 2. it
was found that the monochromatic polarisation has a definite
tendency to decrease with increasing wavelength. The decrease
in the degree of polarization is, on the average, 0.04 - 0.06 in
the region 400 - 600 m-~L. The variation of polarization with
wavelength is due mainly to the dependence of polarization on the
monochromatic albedos of lunar formations. The polarisation
obtained in the various regions in the spectrum can. to some
extent, be influenced by ft luminescence of lunar material.
Calculations show that this effect can reduce the degree of
polarization in some parts of the spectrum by 0.02 - 0-05. How-
ever, the systematic change in polarisatIon is largely due to the
variation in the albedo with wavelength.
Card 2/3

83232
S/033/60/037AO4/008/012
Spectropolarimetry of Some Parts %q-3J4131401ar Surface
There are 2 figures, 4 tables and 13 references: 2 German,
2 French, I Czech, 1 English and 7 Soviet. / .
ASSOCIATION: Sektor astrobotaniki Akademii nauk KazSSR [IX
(Astrobotany Division of the Ac.Sc., KazSSR)
SUBMITTED: October 3, 1959
Card 3/3

TXYFELII V.G.
Color-brightneso dependence for 62 regions of the lunar surface
near the epoch of full moon* Astron.tair. no.209:10--12 Hr '60.
(M MA 13 . 9)
1. Sektor astrobotaniki Al ]EazSSR, Alma-Ata.
(Moon-Surface)

88828
,~ log 2
(IvC7 - d/21)
Traralation from: Referativnyy zhurnal,
P. 59, # 2A482
AUTHOR: Ta 'el' V.G.
3/035/61/000/002/013/016
A001/A001
Astronomiya i Geodeziya, 1961, No. 1,
T=: Intensity of Absorption Bandsof CH4 at 6190 A in Jupiter Spectrum
in 1959
PERIODICAL: "Astron. tairkulyar", 1960, No, 210, apr 15, PP. 11 - 14
TEXT: In 1959 the author obtained 210 spectrograms of Jupiter with an
aim of studying latitude differences in the equivalent width Wn of band CH4 at
~, 6190 found by Hess in 1953 4RZhAstr, 1954, No. 2, 2296). The results of the
present study do not confirm Hess's results. The mean Wr7 = 18.2 A with devia-
tions for different zones of + 2 A and the root-mean-square deviation within
each zone of + 1.8 A. The author studied zones from +100 to -100 and from + 300
to-t- 600 of latitude. The mean depth in the band center Rr, = 0.206. If the
observed time variations of Wn are assumed to be real (within 16-21 A), then the
optical and linear thickness of the gaseous layer varies by about 2 times, which
Card 1/2

88828
S/035/61/000/002/013/016
A001/AO01
Intensity of A;sorption Banda of Mj at 6190 A in Jupiter Spectrum in 1959
can be explained by oscillations In altitude of the Jupiter cloudy layer. This v/
hypothesis does not contradict the assumption on the existence on Jupiter of
a thin gaseous layer above the cloudy layer, expressed by N.P. Barabashov (RZh-
Astr, 1958, No. 11, 7429).
V. Bronshten
Translator's note: This is the full translation of the original Russian abstract.
Card 2/2

TEYFELI~ V.G.
Spectrophotometry of the equatorial region of Jupiter in 1959,
Astron.tair. to.2-153-7-9 -0- 160. (MIM 34:3)
1, Sektor astrobotaniki AN Ka2SSR Alma-Ata.
(Jupiter(Planbtl)

TLYMI v V. G.
Spectrocolorimetric Charactetistico of the lunar Aristarchus Crater
oystem. Astron. tsir. no.215:9-11 0.160. (MnA 34:3)
1. Sektor astrobotaniki AN KazSSRv;Alm&-Ata.
(Moon-Surface)

Y, 8.2 2
S/035A2/000/006/040/064
A001/A101
AUMOR: Teyfel', V. G.
TITLE: Color properties of the lunar surface according to observations
close to true full moon
-PERIODICAL: Referatirnyy zhurnal, Astronomiya i Geodeziya, no. 6, 1962, 64,
abstract 6A483 ("Izv. Komis. po fiz. planet", 1961, no. 3, 56 - 67)
TEXT: Normal color indices of 1,442 sections of the lunar surface were
determined on the basis of spectrograms of 62 regions of the Moon obtained on
September 16 - 17, 1959, at phase angles from 40331 to 3046'. With allowance for
random errors the amplitude of differences in color indices turns out to be not
more than OT25. The existence of a color-brightness relation for features of the
lunar surface is confirmed. There are 8 references.
Author's summary
[Abstracter's note: Complete translation]
Card 1/1

OC7
AUTHORs Teytell, V.G.
TITLE: Planetary spectra
PERIODICAL: Priroda, no.6, 1961, 39-45
21899
3/026/61/000/006/002/003
D045/D114
TEET; This arti6le deals with the application and results of spectroscopic inves-
tigations of the planets. The author, in dealing with investigations of the pre-
sence of carbon dioxide and water vapor in the atmosphere of Venus, refers exclu-
sively to American research in this field. In 1953, N.A. Kozyrev found'tvo absorp-
tion bands of In unknown molecuI6'in the violet range of the Venus spectrum at
4120 and 4372 1 wavelengths. Subsequent observations showed that this molecule is
also contained in the earth's atmosphere- Whilst photographing spectra of the
night side of Venus with the aid of a 50-inch reflector at the Krymskaya astrofi-
zicheskaya, observatoriya (Crimean Astrophysical Observatory) he noticed for tte first
time weak emission bands on the limb of the night side of the disk. These bands
were identical to the nitrogen emission bands observed in the spectra of -the
earth' s aurora. The existence of several of these bands was substantiated by the
findings of the astronomer G. Newkirk in 1958. Their intensity indicates that the
nocturnal glow on Venus is 50-80 times brighter than that on the earth. G.A. Ti-
Card 1/4

18 9
S/026 1 /002/003
Planetary spectra D045/D114
!khov,.H3ad of the Sector of Astrobotany of the Academy of Sciences of the Kazakhs-
kaya SSR and his associates have demonstrated that under the severe climatic con-
ditions on Mars plants can absorb infrared rays. The chlorophyll band becomes
wider but less noticeable and is the same as the spectra of terrestrial plants un-
der conditions of low temperatures. New data in favor of the hypothesis on the
existence of plant life on Mars were recently obtained in the USA. In discussing
the presence of hydrogen and its compounds in the atmospheres of Jupiter, Saturn,
Uranus and Neptune, the author refers to American research and states that N.T.
Bobrovnikov'sq D.I. Yeropkin's and his own observations confirm those by S.Hess
(USA), viz. the intensity of the methane bands does not Increase towards the edges
of Jupiter's disk. Calorimetric and spectrophotometric observat 'ions on the moon's
surface are now being carried out by N.P. Barabashov, Y.I. Yezerskiy and V.A. Fedo-
rets in Khar1kov, V.V. Sharonov in Leningrad, A.N. Sergeyeva in Kiyev, T.A. Polo-
zhentseVa in Pulkovo and the author in Alma-Ata. Lunar rocks differ less by their
spectral properties than the terrestrial granite and basalt-type rocks. The
brighter details on the moon's surface are more reddish, and their color and rela-
tive brightness are proportionally interdependent. The brightness in the moon's
spectra increases with the transition from short to long waves. The degree of po-
larization of lunar details slightly changes with the wavelength of reflected sun-
light and increases towards the blue end of the spectrum. This phenomenon is well
Card 2/ 4

~99
Planetary spectra
3/026/61/000/006/002/M3
D
.045/DI14
explained by N.A. Umov's effect, i.e. by the degree of polarization depending on
the brightness of the surface which scatters the light in different wave lengths.
Investigations of the spectral-polarization properties of lunpr objects, although
only just beginning, seem useful for explaining the composition of lunar rocks.
Increased brightness of lunar details during an eclipse are explained by the Czecho-
slovakian astronomer F. Link as being caused by luminescence of some parts of the
moon,due to the action of ultraviolet solar radiation. According to N.A. Kozyrev,
luminescence on the moon's surface may be caused by currents of solar corpuscles.
He found that the brightness and luminescence of the crater Aristarch differed mar-
kedly from that of the surrounding lunar surface. This indicates the presence of
a special substance in the crater. Moreover, the author recently noticed in this
crater a deviation from the interdependence between color and brightness common to
all the other sections in this part of the moon. In 1958, Kozyrev and V.M. Yezers-
kiy, whilst making spectral observations, found that gas is liberated from the cent-
ral peak.of the crater Alphons. N.T. Bobrovnikov, according to microphotograms of
12 asterdidd;I.established that they have no trace of gases and that the distinc-
tions in their spectral reflecting power are fairly large. AS. Deych in Pulkovo
obtained a spectrogram of the asteroid Vesta, on which he determined that the vio-
let part of the spectrum was actually weakened compared with the spectra of sun-
Card 3/4

21899
3/026/61/000/006/002/003
Planetary spectra D045/Dll4
type stars. The observations of Bobrovnikov, the author and others also seem to in-
dicate~- that Vesta periodically changes its color in accordance with the period in
which it changes its brightness. Calorimetric observations of the asteroids have
shown that their color varies greatly. In summing up, the author speaks of nume-
rous problems of planetary astrophysics still to be solved by spectral methods and
mentions that, to expedite their solution, new, powerful telescopes equipped with
spectral apparatus will shortly be put into operation in the USSR. There are 1
Soviet-bloc reference and 6 figures.
ASSOCIATIONt Akademiya nauk Kazakhskoy SSR (Academy of Sciences of the Kazakhskaya
SSR), Alma-Ata.
Card 4/4

__~ ~E~LV-~G.
Noctilucent clouds observed in Central Asia. Astron.tsir.
no.218:25-26 F 161. (MIRA 14:7)
1. Astrofizicheskiy institut, AN KazSSR.
(Clouds)

TEYFELI V G.
Photometry of the continucus spectrum of the equatorial zone of
Jupiter. Izv.Astrofiz.inst. AN Kazakh.SSR 13:54-61 162. (14IPUI 3-5:6)
Pupiter (Planet)--Spectra)
.".00

44274
S/503/62/015/000/001/003
AOO1/A1O1
AUTHOR:, Teyfell, 4. 0.
TITLEz On distribution of ejected substance in small haloes of lunar
craters
SOURCE; Akademiya ~auk Kazakhskoy.SSR. Astrofizicheskiy institut. Iz-
vestiya. v. 15, 1962, 63 - 76
TEXT: The.present article represents a part of the study of haloes and
ray systems of lunar craters. It describes photometric studies of small haloes
of five lunar craters: M6sting A, Hipparchus C, Euclides, Abulfeda E and Gcm-
bart A. The radii of these haloes do not exceed 60 km. The underlying assump-
tion on which this investigation is based, is that the observed distribution of
brightness in the halo of ejected substance reflects, to some extent, th~ quan-
titative distribution (number of particles) and qualitative one (their optical
properties) of the substance around the crater. Two beat begatives of the
Moon's southern hemisphere taken by N. V. Mikhaylova and the author were chosen
for photometric studies. Two of the investigated haloes, those of Hipparchus C
Card 1/5

S/503/62/015/000/001/003
On distribution of ejected substance in... AOO1/A1O1
and Gambart A, have a distinct ray structure; the craters of Abulfeda E and
Diclides are surrounded by diffuse haloes without indioations of a ray struc-
ture. The negatives of the lunar surface sections including the haloes of the
listed'craters were measured with a MO -2 (PT, -2) microphotometer and photometric
.--maps with isophotes, in intervals of 0.05 or 0.1 units of crater intensity, were
plotted. The isophotes show that the halo brightness of all investigated era-
ters decreases smoothly toward periphery, both in red and green light. The V\
brightness'of craters turns out to be 1.5 - 3 times as high as the brightnc-,s
of' the brightest parts of the haloes. On the basis of the brightness distribu-
tion and assumptions made, the distribution of substance In the haloes was cal-
..'culated and the curves, quantity of substance versus distance from the center,
were plotted for all five craters (see Figure 2 attachea). The data obtained
'made-it possible to estimate approximately the mass of ejected substance. As-
!s,uming it to be dust-like and having the specific gravity equal'to 3.33 g/cm3
.'(average moon's density), the mass of substance ejected from a crater and forming
:a bright halo turns out to be of the order of 100,000 tons. Assuming the mean
velocity of substance ejection to be 0.2 kn/sec, the energy of.explosion leading
.to formation of-haloes is calculated to'amount to 1021 erg. However, the energy
'Card 2/5

S/503/62/015/000/001/003
On distribution of ejected substance in... A001/A101
necessary for the formation of a crater amounts, according to K. P. Stanyukovich
and assuming the numerical data for the craters in question, to 1024 erg. It
means that only an insignificant fraction of substance of lunar rocks forming
the walls of a crater is ejected in the form of a halo and rays. Considering
conditions of ejection and comparing different versions, the author finds out
that the most probable version of ejection is as followsi the substance was
ejected mainly at small angles ('J 4 1150) to horizon and with a small dispersion
of initial velocities. The theoretical curve plotted according to these condi-'--
tions shows' a close-agreement-with the,observational ones, with exception of the
halo of the Hipparchus C crater. There are 5 figures and 3 tables.
Ca~-d 3/5

On distribution of ejected substance in...
Figure 2.
al
45
46
41
f to
46
42
W
011
S/503/62/015/000/001/003
A001/AlOl
41
P 40 41 40 41 40 V to YI. CV At 43 41 -U 0 41 0 49 W
Card 4/5

On distribution of ejected substance in...
Figure 2 (cont'd)
v
AK#m*E
40
0 U V WO 40 41 0 491 P

-q,/,r,03/6Z/015/000/()01/003
A001/AlOl

40-
45 -

48 43 43 46 47 40 40
Card 5/5

-- T&FEL IJ-- V.-G--
Height of the u er boundary of Jupiter's Red Spot. A-stronstair,
no.232-.8-13. D IPU, (MIRA 16-4)
0
1. Astrofizicheakiy institut AN KazSSR.
(Jupiter (Planet))

'at r, r .. I - -
T F, Yl,-& L' , v . C, . 0j. nik,l),
; jies in Kazakhstan. -Ve3T. ;.I,, Kazakh. Ss?
Lurlar aTid pLarieta'- F Tl- .1 a _
(11, [R], I--, : I'l "
20 rio.8:9-1.7 ~g 164.

TEMLI, V*G*
Spectrophotometry of methane absorption bands cn Jupiterls
disk in the near infrared regicn (0.7-1.0u~). Astron. zhur.
43 no. 1:154-156 Ja-F 166 (IMIRA 19:2)
1. Astrofizicheskiy institut AN KazSSR. Subnitted June 18,
1965.

Aci.=iox mts AP4o45o62 S/0031/64/ODO/006/0009/0017
JWTHOR3 ~e~ejl, V. G. (Cwwdidate of physico-m-Athomatical aciences)
TITLEt Investigations of the moon and the planets in Kazakhstan
SOURCE: AH KazSSR* Veatniks no. 8, 1964, 9-17
TUPIG TAGS: moonq planet., spectrophotometry, spectrocolorimotry, atmosphere
ABSTRACT., The author points out some aspects of lunar and planetary study that
need most attention at the prevent timo. His paper is a suminary of tile kind of
work done since 1956 at the Asbrofizicheskiy institut (Astrophysical Institute)
and the former Sector astrobotaniki (Astrobotanical Section) Ali KazSSR. Tile
physical properties of the moonli 3mrface have been studied by spectrophobometric
and spectrocolorimetric methods. Polarization studies of the moon's surface have
revealed absorption and polarization characteristics. Photometric and spectral
i, studies of the earth-Grroup planets have been made, and systematic spectropliotomet-
ric and phctographic investigations have been directed taward the "blue smoke" of
liars., the nature of which is not yet known. The theoretical possibility of tile
existence and size of magnetic fields on Mars and Venus and the possibility of'
radiation belts around these planets have received special attention, Detailed
studies have also been made of the larger planets. Observations of continuous
a,ra-jl/2
-4

ACCESSION NRs AP4oh5o62
spectra in the visible and ultraviolet regions have been made f or Jupiter,$ Saturn.,
and Uranus. Present studies are of three General types, depending on the character
of the object being investigated% the moon (with no atmosphere), the planets of
the earth type (Mars and Venus, with atmospheres of low density), and the giant
planets (with very thick$ nontransparent gaseous envelopes, and with chemical
compositions differing markedly from that of the earth group). The basic trend of
planetary studies in Kazakhstan may be stated as the search for (and study of)
inconstant phenomena and processes in the atmospheres and on the surfaces of
planets and satellites of the solar system at the present stage of evolution of
the system* This program also aims at a study, of the connection between the
indicated processes and both internal factors and solar activity.
ASSOCIATIONs none
SUBMITTEDs 00
SUB CODE& AA
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TEYFELI, V.G., kand.fiz.-matem. nauk
Atmospheres of distant planets. Priroda 53 no. U:23-33 16-4.
(MIRA 18:1)
1. Astrofizicheskiy institut AN KazSSR, Alma-Ata.

TEYFELI, V.G.
Photometric properties of the red spot on Jupiter. Astron.
zhu- 41 n0-3:531-538 MY-Je 164. (MRA 17:6)
1. Astrofizicheskiy institut AN KazSSR.

TEYGELI V.G.; PRIBOYr-,VA, N.V.
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Intensity of methane absorption in the band CH4 6190 A on Jupite-rls
disc. Izv. AN Kazakh. SSR. Ser. fiz.-mat.nauk no.lt6l-73 163.
(MA 17:4)

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~ 171 P E r 1 9it-
Ultraviolet abEorptin in the contintioutt spectruir, c-f
Izv AN Kazakh. S.')?. Ser. flz.---ma--.najk no.1374-77 163.
(MIRA 1?,4)

TEYFFEL' , V-,Ltor German-ovich; SKAILKOVSKIY, L., red.
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[What the stars tell ugj 0 cl- 'emgovoi,iat Ah,-a-
Ata, Kazakhskoe gos. id-vo, 1964. 141 1). (MIRA 17:12)

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ACCESSION MR! A?50001114
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ACC NRt AP602754 5 SOURCE CODE: UR/0384/66/000/003/0028/0035
'AUTHOR: Teyfell V. T. (Candidate of physico-mathematical sciences)
ORG: none
1ITLE: Two new enigmas associated with the planet Jupiter
;SOURCE; Zemlya i vselennaya, no. 3, 19660 28-35
IOPIC TAGS: Jupiter planet, band spectrum, planetary astronomy
IABSTRACT: Two phenomena observed on Jupiter which have no satisfactory explanation ar
0
I~d -scribed. The first was observed by US astronomer Spinrad in 1961, who discovered
hat the slope of lines in the ammonia band with a wavelength of 6450 A is substantial
1y, less than what would have been expected. Possible explanations for this phenomena
proposed by various scientists are discussed and evaluated. The second unexplained
'phenomena is associated with temperature elevations on regions of Jupiter which are
:shaded by two of its satellites. Two physical explanations which have been proposed
for this phenomenon are analyzed by the author. The first explanation attributes the
lphenomenon to variations in the transmission properties of the atmosphere for thermal
adiation. The second explanation is based on the proposition that there is an in-
crease in the concentration of matter which is relatively opaque to thermal radiation.
The author shows that both of these explanations contain contradictions and concludes
hat the phenomenon Is not yet properly explained. Orig. art.'hass 8 figures.
SEB CODE: 03/ SUBK WE i none
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TOROPOVAP T.P.; TEYFELI, Ya.A.
Measurement of solar aureoles at various elevations above sea level.
Izv AN Kazakh. OSSR, Ser. fizo-mat.nauk no.1:93-102 t63.
(MIRA 17t4)