SCIENTIFIC ABSTRACT FESENKOV, V.G. - FESENKO, N.G.

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• Collection: Scientific Abstracts
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• Document Creation Date: November 2, 2016
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• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

.)/6 j /()n!/00()/00-1/007
On the conditions (if observation s/,io-
and hence
o .3o 1.8o
go
10 54.4 io
Thus, the ovej-~Ijj deg-ree of polari7.atirin is large atid very neorly
constant right down to 00~ However, under real conditions the
polarization by dit--.t matter should be intich ~.tualler. Thu9t, for
example, Ye. V., Pya -xkovs kaya- Fes ejikova (W-V.5.- Izvestlya
Astrofizicheskogo insti.tuta AN Kn,-rSS4, 1991), v.8) has succeeded
in separating thescattering indicatvix of dry aerosols in the
Libyan Desert intr? fiinctions T-Pprosenting light vibration~z in the
,above two mituntly perpendicular pLa"e-,. these re-sillts are
emploved, then th.-I Volarization di-triJifition is fotind to he
0 10 2o 4 o 50 6o 9() 120
2 'i 24.2 26:1 2-8-0 29~7 !I.,() -:) 1, . 8'30. 821.4
The zvvNi probiem is to seyiarate tho- zodiacaL light from the
Card 4/5

conditions oir observati.on ... Sl';()-:Yl .,/()(()/0() P 7
r. o 32 Ii, 5 1 It
hnckground sky intensity. Tt i, pointed olit that tbe conditiotis
whicil pertaiji diirbig total. oclipso iwo vory aimilnr to thoA0
giviiig rimeto Nky 1.1lumi.n.-itton d6ring stinrise and st.111set.
Thereforf~, the allthor's theory of* t-;,Hlight can be used to compute
the backgrottiid -intertsity. A gener,;O, docteription is given of
how tile backg-rourld i.111.011t3i.ty C-oll tl(-' takeyl inf.-.o acr-wint. There
ro I figure and t, v fe r e n e ns Y ~iov-iet-bloc and 2 rjon-Sovi.et-bloc.
Card
RA, Effll! T,

--9,/0-35/62/000/007/051/083
A001/AlOl
AUTHOR: Fesenkov; V. G.
TITLE:' On the nature of.com6ts and conditions of their falling on Earth
PERIODiCAL: Referativnyy zhurnal, Astronomiya i Geode,ziya, no. 7, 1962, 76-77,
abstract 74550 (In collection: "Meteoritika", no. 21, Moscow,
1961, 3-14)
TEXT: The upper limit of comet mass, determined from the absence-of pertur-
baiions~ is equal to 1012ton. Assuming that their cores represent-compact swarms
of individual particles, their sizes can be estimated from the known brightness of
the comets as b6ing I cm. Small sizes of particles are corroboratea also by polar-
ization of cores, similar to that of aerosols. Absence of bolides in meteoric
streams originated by comets indicates uniformity of particles. According to
Roche's criterionj the core is not a bound .whole at a small distance from the Sun.
Cometary spectra indicate the presence of CO, CH, CN, etc. oasily evolving at a
temperature 'below OOC, which also confirms the disperse nature of the core. Passirg
through perihelion, even high-melting partioles of the core evaporate and then
condense again. Accelerations of some comets are explained by reactive momenta
Card -1/.-.2

S/035/62/000/007/051/083
On the nature of comets and... A001/A101
which the core particles experience during evaporation, At prestnt it is estab-
lished that the character of orbits of both long-periodic and short-periodic
comets agrees with the notion of the origin of these bodies from the field of
parabolic comets. Condensation of cometary core particles in interstellar condi-
tions is doubtful. More probable is th& formation in the protoplanetary cloud or
during a Sun passage across a cloud of cosmic dust. Initially highLmelting elements
condense into particles, then hydrogen forms a thin layer.- around to which occlude
atoms of cther elements. Formation of a H20 grain of 0, 5/,Lsize will take-il,000
years. Cometary. particles will represent complicated aggregates of metallid -and
silicate grains with sticked molecules of water, CH, eta'. A compact clustering of
such particles serves as a core of a nonperiodic comet. In encountering with the
Earth, the comet will disintegrate in the atmospheres, even at a great mass, as
a result of the enormous area of the cross section, giving rise to a powerful air
shock wave. Its'remains will fall on Earth merely in disintegrated state. There
are 13 references.
I. Zotkin
[Abstracter's note: Complete translation]
Card 2/2
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3 ME 0, 1 ~ 1, ZE
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oil
FF=NKUyrY.G-[Fesenkov, V.G.] (USSR); KRINOV, E.L. (USSR)
Was the so-ca2led Tungus meteorite a comet? Elet tud 16 no,21:664-
666 21 My 161.
P., UA
-,A KH
4
YNIA) MIMI-
kP- I WO 511

MR-
~--MENKOV, V.G.
Man in space means the beginning of a now era in the development
of science. Astron.zhur. 38 no.2;1-IV Mr-Ap 161. (IMU 14.-1,)
(Astronautics)
(Coptio phyoics)

Pop=-!-
S/033/61/038/006/001/007
E133/E435~
AUTHOR:
TITLE,. On the density of meteoric. material in -interplanetary
space and the possible existence of a dust cloud round
the Earth
PERIODICAL: -Astronom.,icheskiy zhurnal, v.38, no.6, 1961, ioO9_1015
.TEXT: The~mass of meteor.lcmaterlal, collected by- the Earth, is-
given by F. Watson (Ref.l.* Between th Planets, l9k8l Harv. Observ..
v-105? 1937V 623) as--,O-.36 to.4.6 x log tons per year. E. Whipple
(Ref.2,. Paper presented-at the Agtronautical Symposium, San Diego,
i956) gives the figure 0.7 x 10 from a study of visual and-
.photographic meteors. An alternative approach is via a study of
the cosmic dust in 'the atmosphere-(Ref,3: H. Pettersson, Sgient.
Amer. v.20Z, no.2,.196o).- This gives aafigure of 14 x 10 ton 's
per year but is very uncertain, Again, the meteogic dust found-in
deep sea deposits indicates-a gain of about 5 x 10 tons per year
(Ref.4*. H.-Petterson and Rotshi, Geochim. et cosmochim. acta-,,1950).
The author first of' all considers-how much material should-be
collected from in .terplanetary space-by the Earth., This dlependk; on
whether it is assumed that the material is stationary or not.
Car& 1/3

S/033/61/0311/006/ooi/007
On the density of meteoric .00, 9133/E435
lie calculates that there should be either 2-79'x 103 or
0.535 x 10 particles/kO, for an assumed relative velocity of the
Earth and interplanetary medium of 30 and 5 ivn/sec respectively.
(The average radius ofa part icle is assumed to be IOIL~)
The material density .--an also be deduced from the zodiacal light.
This can be done by finding the brightness of the light,
talculating the optical depth and, hence, finding the particle
densi-ty~ The author shows that ihe order of magnitude of the
,result does not depend on the particular scattering function used.
Assuming thebrIghtness of the zodiacal light to be 25 fifth
magnitude stals pez, unit solid angle, he obtains an optical depth
.73 x 10-8 for I A.U~ The corresponling particle density can
of 6
only be calculated if the particle-!distribut-4on witb sizt and the
scattering coeff1c;Ient variatIon with' -size are known. III
assumed that the former, is given by
dN
and the latter is proportional to yP, where P 2 f or r 0. 5
Card* 2/ 3

S/033/61/038/006/001/007
On the density of meteoric E133/E435
The total mass of dust with n the limits-of the Earthis orbit is
then found to Ibe 1.61 x 101~ g, i.a. considerably less than I'S
given by the direct methods mentioned'at the beginning of the
article, This suggests that the Earth is surrounded by an
increased concentration of dust, If we assume that particles in
this dust cloud-are broken up by the action of solar radiation, and
so form a tail, we-.can also explain the counterglow. There are
I table and 4 non-Soviet-bloo-references. The four references to
English language publicatmions read'as-follows; Ref.l., Ref.2"
Ref-3-' - all as quoted in text; Ref.533 J. Vood, Astrophys, J..
no.1, 1958.
SUBMITTEDg August 10, 1961
Card'3/3

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ki~'.are- alr6~dy.-.-.
nglromidust parUcleo".-_

47.

FMNKaV, V.G.
Aetronabur. 39 lio.4683-590
5--a-h-d-Origin of comets* (MM 15:7)
n,.Ag t 62,
(comets)

S/0265/6-2/000/0,08/002/005
D050/D113
ILUTF
Fesenkov, V.G., Academician
TITIZ,:. The nature of the Tungus phenomenon. Not a meteorite, but a covet
PERIODICAL: Priroda, no..8, 1962, 24-31
TMT: The'author discusses the cause of the Tungus phenoxcnon and, bascd on
acewulated data and research recently conducted by the Nomitet po meteoritan
AN SSSR (Committee on Meteorites., AS USSR), the Institut goolchimii i analWches-
koy Ichimii im. V.1. Vernadskogo A.N SSSR (Institute of Geochemistry and Analytical
Chemistry im. V.I. Vernad~kiy, AS USSR)) the Pochvennyy instilait (Soil Institute)
and the Glavnyy botanichebkiy sad AN SSSR (Main Botanical Garden, AS USSR), he
concludes that it was caused by the fall of a covet. His hypothesis is based on;
(1) the orbital. motion of the Tungus cqsmic body - a motion characteristic of
comets only; (2) the direction of the fall; (3) the existence of a tail pointing
away from the Sun; (4) lack of meteoric matter at the place of collision; (5)
increased luminosity of the nocturnal sky, observed soon after the collision; (6)
the noticeable dimness of the FArth13 aVmosphere, caused by comparatively coarse
particles: Investigation's are continuing. There are 9 figures and I table.
Card 1/1

LEBEDKINA, Ye.D.; FEWROV, V.M.; FAYNBERG, V.Ya., kand.fiz,matem.nauk;
BARCRUKOV, A.I., kand-teklin.nauk; FESENKOV, V.G., akademik;
YUCHEROV,'-N.F., doktor khim.nauk; DZERD2,N-EVSKIY, BZ., Prof.;
SUAPIRD, G.S., doktor tekhn.nauk; KUTAGINA, O.S.; UDA14ITSOVA, Z.V.,
doktor istor.nauk; LIKIIACHEV, D.S.
Brief notes. Vest. AN SSSR 32 no.1:119-130 Jaf.,62. (MIRA 15:1)
(Scientific societies) (Research)

FESENKOV, V.G.., akademik
Flights to the moon and mars to fonow. Priroda 51 no 9:21-22
s 162. Wl~i 15:9)
(Space flight to Mars)
(Space flight to the Moon)

S/259/02/000/012/002/002
E073/EI55
AUTMM: F"SeMkovi V. AcAdemicinn
T 1 "'LE': The wystcri es of the planet tiars. Present views and:
y potlic.-Ses
I'l (If., I CA 1, Nauka i teldihika, no.12, 1962, 38-39
LOVO-1-1 PoNtUllltOJISI a regular network of artificially
bij-iji 4~~;iiiais on var-5, but the French astrononter Antoniade has shown
that. n~- x-f--gni'lar no-tworic of cozials exists and that the individual
cana-l-ti do not rl~present contirittaus littes. This was fully*confirmed
by 1(-t-oy aii%l Dnlf'uss of tlie vir- du Midi Observatory.
N.1.. Iarilhashov in KharIkov found that the I.artian seas which
looked careen coilipareo to the reddish deserts have j .Ln reality a
reddi!.11 till,rt, when comjmrr.~d witli a whito screen. Ftirthermore,
thoir -~pr~etra do not c(ifitain the slightest indication of chlorophyl
baiid!z whicli jiust exist i1i liighly deve.loped plants on Karth.
T00inA, has for mariy ytars visited various zones of the USSR,
i1o c-hiei(late the spectraJ t.-~at%ires of light reflected from plants
iiii-14?r varjotis clii-iiat.ic coziditions. lie concluded that the i,ntensity
of.' such Ninds Jargely depetids on seasonal and climatic conditions.

5/259/62/000/012/002/002
Tilt- lityste.ries or thp plaiiet Pars. ... . ::-
E073/EI55
irtid#~j- ttic cxtrerie,ly severe conditions of ~'ars, the plants could
I?vrIlaI!.-j ar..Cjirn;Ai'Lsf!d thf-111splVes so as to lose as little of the
ir rntliation nti po.-isible. The rel'Acetivity of the dark spots
on t-'.Ars would therefore. b(, v-ry siria]-J, particti.larly in the red and
infrared, which is in great contrast to conditions on Earth.
Ilowever, the exi.9tence (if p-1-nitts ruris cotinter to other facts. in
the atwosj)h~irp of Pars no moleraiAar oNygen or water vapour could
he df-tr!cted, even a thoij.,iandth of that found on Earth. This. tells
ag,ainst' the existence. of higrhly developed plant life which could
-to support animal IjfP. Photometric observations of
V.V. Sharonov, N.N. Sytinskaya, N.P. Barabashov and others show
tbat Partian I'seas" as well as deserts have fully analogous
properties as regards the nature of their reflected light. This
further discounts the existence of plant life, which is always
distitigiii-c,hed by rich branchlilAgS Or shapes. Analysis of the
thermal conditIons of tile light and dark regions on Narsj and
comparisoii with the apprnpriato reflectivities, also seein to
preclude plant life. on absorbing solar radiation the Vartian
"sen-411 heat up, like all inorganic body, whereas living matter
always tises tip the high-freq~icncy solar energy for chemical
Card 2/4

Thr. lily-, tv r i vs of the planet J-.iars. S/259/62/600/012/002/002
E073A] 55
.t alld 'lot Cor --;jwpJe I)IF!at rime. TIJV tileory that
I-Jimf, JAI'v exh-its tm r,*;,rq lvirgely derives from tile illvariance and
t-tolh i I i Uy ol, 1.1m. tint-k mpotn ott N,~arq, claiming that if they did not
~,,,iiLaiii phwiit.~ they 1-imild br!cnwe covered by sand-storms which--:Cz,6m
tillio fo Ciislv- ner-tir on T."ars.- Thi.,; vJow Is not wel.1 fotinded, since
fill "ir"O"i INF.H.himt pinntm w~v4,rtbvIr.-mm exhibit considerable
di(Tvj-nce.-t in ret'lectivity (Libyai) Desert, th4- Aswan-Sudan area).
of recfmt jifmtographs with pliotograpbs made during
the last. celtitiltry show great chawres. ~IcLaughlin proposed to
comleet thc~ formation of IIseft-411 with voicanic activity and tried
the rolief of th,~, sea to th~.- direction of: wind in the
-~.-artian atmosphere. From him 1,Qlarimetric measurements, Dolfuss
ti'l-ed 11(i silow t1wit oil -*ar.~; liflijid watf!r cannot exist and is
djrt!c(A-y trai-i5Cormied iiito vapour. Accordintr to viss, all the
feattires on tile siarface as we.11. as ill tile atmosphere of
Ear5A Call bo explained by varlims nitrogen compotinds, and wider
thest, cowlitions no or-anic -1 U:c can exist. ilowever, during the
"1.,.,t oppositions in 1956 awl J()5A, tile existence of simple
ov,frztll~j.c carboliydrate compounds was detectpd, particularly in the
Cavil 3/11
g
M? ST-R

The mysteries of the pJanot Mars. S/259/62/000/012/002/002
E073/El-55
dark spots, of Vnrs. !inch met-hime-type compounds can form also
d1iring vol.canic activity but the factsthat they are invariably
connected with the daric Itsea.411, i.e. the surface of tile planet,
and that they are not presetit iii the spectrum of any plant life,
sug.gest organic life oii ~:ars. The anthor conc1ndes that there are
no higher plants and nnimals o" Mars but allows that lower
primitive forms of each may exist.
There are 3 figures.

FESENKOV, V.G., akademik, otv. red.j KRINOV, Ye.L.., wm. otv.
red.; RAKHLIN, I.Te., red. izd-va; TIKHOMIROVA, S.G.,
tekhn. red.
(Sikhote-Alin' Iran meteorite ahowerl. Sikhote-Aliiakli,
zheleznyl mateoritnyl do2hd'. Moskva, Izd-va AN S5SR.
Vol.2. 1963. 370 p. (MIRA 16:11)
1. Akademiya nauk SSSR. Komitet po meteoritam.
(Sikhote-Alin' Range-Meteorites)

AMBARTSUIVAN, V.A.,, akademik; ASRATYAN, E.A.; BOGOLYUEOV, N.N.,
akader-ik; VIVOCRADOV, A.P., akademik; GDt7ETSINShIY, A.G.;
KNUNYANTS, I.L., akademik; KOCRETKOV, N.K.,- KUHSANOVI A.L.,
akademik; MELINIKOV, O.A.; NEWEYANOV, A.1%, akademik;
IJESMEYANOV, An.N., doktor khim. nauk; ORREIMOV, IN.,
akademik; FOLIVANOV, M.K., kand.fiz.-mat.nauk; FEUTOV,O.A.,
RYZHKOV, V.L.; SPITSIN, V.I., akademik-; TA124, I.Ye., akademik;
FESE11KOV V.G I _!~ksdemik; FOK, V.A., akademik; SHCHERBAKOV,
demik
FRANK, I.M.; FRANK3 G.M.; KHOKHLOV2 A.S.,
doktor khim. nauk; SHEMYAKIN, M.M., akademik; ENGELIGARDT,
V.A., akademik; SHAPOSHNIKOV, V.11., akademik; BOYARSKIY,V.A.j
LIKHTENSHT-M], Ye.S.; WAZEWSEVA, V.N., red.izd-va; KLYAYS,
Ye.Y., red.izd-va,- TARASMIKO, V.M., red.izd-va; POLYAKOVA,
T.V., tekbn. red.
(As seen by A scientis: From the Earth to galaxies, To the
atomic nucleus, From the atom to the molecule, From the
molecule to the organism] Glazami uchenogo: Ot Zemli do ga-
laktik~ K iadru atoma domolekuly, Ot molekuly do organizma.
Moskva, Izd-vo AN SSSRI 1963. 736 p. (MIRA 16:12)
1. Akademiya nauk SSSR. 2. Chlen-korrespondent AN SSSR (for
Asratyan, Ginetsinskiy, Kochetkov., Mellnikov, Reutov, Ryzhkov,
Frank,I.M., Frankp GJQ
(Astronomy) (Nualoar.physics) (Chemistry) (Biology)

S/033163/0o/ool/mA16
E032/E314
AUTHOR: Fesenkov, ViG.
TITLE: gleii- ~uc~ono ~ photometric observations of zodiacal
light for the effect of tropospheric scattering
'PBRIODICAL:. Astronomicheskly zhurnal, v. 40. no. 1. 1963,
31 - 37
TEXr: it is supposed that each al ement of zodiacal light may
be regarded as an external source. of light illuminating the EbLrth a.
atmosphere in a way similar to that of the Sun. An algebraic
procedure is outlined wheroby a roduction factor K , by which the
observed brightness of the zodiacal light, freed from the effects
of ionospheric.and stellar components,:-must be multiplied in order,/
to obtain its true b righ tness, which will then i 'nclude only the
effect of the ordinary atmospheric extinction. The procedure
involves numerical evaluation of integrals containing scattering
functions, intensity distributicns and functions of geometrical
parameters. The scattering ihdicatrix for the Earth' S^ atmosphere'
is taken to be of the form
Card 1/2

FESENKOV, V~G*
Table for the reduction.of photometric observations of zodiacal
light for the effect of:tropospheric scattering. Astron. zhur.
40 no.5.i882-888 S-0 163. (MIRA- 16:11)

MOWN
FESENK(IV G.
Isopbotes of the zodiacal light',11'rom observations-made in
Egypt in the fall of 1957* Aot6~.zhur. 40 no.6tlO85-1094
N-D 163. (MIRA 16t~;2)
-P

FESENKOV, V.G., akadmaik
Mrs and organic life. Pr1roda, $2 noo2s22-26 163.
(MIRA 16s.2)
Imars Wumet)) (Life an other Planets)
IIHMMMOW-M

FAYNEMI) I.B., red.
[Life in the universe) Zhizn' vo VBelennoi. Moskva~ lzd-vo
NiSnanie," 1964. 53 p. (N6voe v zhizni.. nauke, tekhaike.
IX Seriia: Fizika, matematika, astronomiia, no.8)
IMIRA 1?: 5)

ACCESSION NIL.; AT4035826, B/FZ4/64/000/024/0034/0036
AMOU: Feisenkov~#,V. G~ (Academician)
TITLE: Meteorites and the problem of the origin of,the elements in a galactic
system
SOURCE: Mr SSSR. Nomitet po meteoritam. Miteoritika, No. 24, 1964, Trudy*
Desyatoy Hateoritnoy konferentaii -v Leningrade 29 mays, - I iyunya 1962 C., 34-36
TOPIC TAGSi ' galaxyo supernova, heavy element, element, radioactive dust, galactic
syst~M, meteoAte, radioactive 4ecay
ABSTRACT: The radioactive decay of elements is one of the simplest and most reg-
ular irreversible processes in nature; it has been concluded that radioactive ele-
r~ents and therefore all the heavy elements involved in the earth's formation and
in the formation of the other planets, have'an age of only 5-6 billion years, that
is, considerably less: than -the estimated age of our Galaxy. It has been sh
oVn on
the basis of the best:available evidence that the only knowa process capable of
creating heavy elements, including radioactive elements$ is the explosieu of a
supernova. Such phenomena are rare in the'present-day Galaxy - approximately
one such event per huadred years. But it appears difficult,to asinne that these
rare.supernovaecaa-stipply the galactic need for such elements. It is probable
5 Card 1/2

ACGMION. AT4035828 '8/2"4f64/090/024/00611006
'ADMOR: 'Feseakov, V O~' 0 a an.
(A aaemi I
TITIZ: The a, 0 orizomets,
SOURCE: AN RSSR. 1comitet polmeteoritame :Meteoritika, No 24, 1964, Txqidy*
Da~yatoy Hetearitnor konferentaii v Lsaingrm!de 29 miya -,I iyunys 1962 61-65
TOPIC TAGS: astrophysics, comet, cometary head, comet formation, Tungus Meteorito
ABSTRACT: It has become obvious in recent years that the Tungus meteorite was,in
fact a small eomet; study of the-Tungus meteorite can-therefore yield'much infoi-~
MatiOn c0ncex`n1n,6f the nature of comets. However, istudy of the Tungus comet or
meteorite rec ires that investigators approach their work with a clear understand-
Lu
ing of the characteristics of comets; thin paper is abiief review of this prob-
lem. Comets are either periodic or nonperiodicl'but it can' be assumed that all
--- have the sa,mb chemical compositioh, internal -structure and degree of instability.
On this basis it can be assumed that all have a: cc=on origin. S. K. Sy*rovatskiy,
omeis in'the-form of 6ompadt"i-4 "*df more o 'fge-
-ilhas postulated that t* lefts 1a
ok c
:.~'--Vartic.les could be ejected from the major planets or their satellites; the foruL.-
';he manifestations o
tion of comets in one of t f 6oamic vuleanism. However,-the
possibility'o~f all-comet's develCoping in this -&-ir it; most improbable. The out-
Card 1/2

'Nor -1;12 __:_ -gem me R
4-CEMMEW-A
AV,
NR.:: AT4035828
c of,comets, instabilityj is discuss an Jadiw
~standing characteristi ed. Observat i9
comitary nuclei do not:consint of solid masees, but of compact clutters
of particles (lapable of yielding.great quantities of gases. The contention of
me ry
various authors that a cc t can contain ordinary meteorsis incorrect. Comets
nuclei consisli of loosely connected matter capable of turbulent evaporation when
subjected to twiall heating and ejecting finely disperse matter and various gases,
Al
such as CH, Gro, C CN and in some cases CO. XateneLty distribution in cometary
%lap to the solar spectrum. Estimates of the possible mass ofa.
spectra correspon
typical comet should be based on use of those parameters in which the entire mass
is -nnifested. Certain.comet experience a jump-in their orbital'acceleration.
a
Other characteristics of comets ire, given. Comets can form only at very low teza_
peratures,.at great distances from the sun, for all practical purposes in inter-
stellar space. Orig. Art. hav. 3formulas.
ASSOCIATION:-,~.Komite.t.po,mateoritamol.Akademiya nauk (committee on Hettorites,:,-C
Academy of Solenceavaw)
;SUBMITTED: 040i DAMACQ: !2819ay".- ENCL. 00
q. SUB CODE: AA,!:, NO RW SOW, 003 on=::. 008
Cord
-77-

!ACCESSION NR: A74035840, 8/2534/64/000)'024/0177/0179
fAUTHOR: a
demician)
Anomalous light phenomena:asaociated with the falling of the Tungus.
~meteorite
ISOURCE: AN SSSR. Komitet po meteoritam. Meteoritika, no. 24, 1964. Trudy*
;Desyato7 Meteoritnoy konferentsii v Leningrade 29 maya 1 iyunya 1962 gi., 177-179
;TOPIC TAGS: Tungas meteorite, meteorite, atmospheric phenomenon, comet, cosmic
~dust
ABSTRACT: A sharl? increase in the luminosity of the night sky on 30 June 1908 wad
jobserved over an t~xtensive area. It was characterized by an increase in the in-
:te:nsity of the continuous spectrum and therefore was caused by the scattering of
sunlight on dust particles in the earth's atmosphere. Before the fal.ling of the
Tungus meteorite i:he brightness of tha night sky wan normal, and thf. night of 29
.,June 1908 was the same. An anomalous brightness of the night sky occu-:red on 30
~June 1908, immediately following the falling of the meteorite. A doy la~elq this
~brightness had decreased by a factor of 10 and then disappeared completely. The
artomalous brightnass extended on that day only as far west as Ireland and only as

L~ard
.ACCESSION NR; AT4035840
,far east as Vanavara. This indicates that the phenomenon was caused by'a cloud of
:cosmic dust penetrating into the atmosphere, orig~natlrig from the site of falling
!Oj- the Tungus meteorite and moving in a direction away from the sun. These dust.
:particles were associated with the meteorite even*before its encounter with the
:earth and moved away from the earth at a velocity whicli was very small in compar-
.i-;on with the earth's orbital velocity. The source of particles obviously was the
,tail of a comet. The position of the BOUtbern boundary of the anomalous brightness
:indicates that the particles of the tail of the Tungus comet were held at a height
:of about 600 km and then were carried back into sr-4ce under the influence of light.,
,pressure. -Conditions therefore quickly returled to normal, It is noted that many
jauthors have attributed many optical phenomena to the 12alling of the meteorite, but
:w,,'.~thout justification. A change in the optical properties of the daytime sky and a
Xeneral significant increase in atmospheric extinction over an extensive partoof
the earth set in only considerably later than the falling of the meteorite. As a
result of the explosion at'a height of 6-7 km the principal mass of the meteorite
~was carried off In the lower atmosphere as far as the ifest coast of the United
States, but about, two weeks were required for this to occur.' These and other
~considerations aro said to be convincing evidence of the cometary nature of the
:Tungus meteorita. 0
2/3

NR AP6ch659
p P r
-osmogony, an" th? effect Of COSMIC ad'-,,t!cr~'cn them
n
sed 'Phe meteorite ':~rcbi Qm maY
Mutual e
C a. r d 1.
4MM' 7z
NOR '-G:-
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L ~P4o46592
NR:
A - ----- 00 ENCL: 00
REF SoV. 003
SUB CODE: AA
-E
1.1

Kw&
'JD
-P~ ~iPr-h/Pae-2 S Dh r0' DU G7jTf
pl; C. 1; -;Ogg s/oo?6/6J4/coo/oia/cco2/oao7
-n-ryv, G .(Academi -ian)
T L F Meteorites and the origir of the solar system
S -AIRCE: Priroda, ro. 10, 1964, 2-7
meteor-Ite, meteorite composition, solar system, solar system oricin,
superno,.a
TN,-- man\ theories of cosnzgeny, here listed bt-lc-fly by the author, may
P r i v i f
R-io

Tr - -I-
-~i- 1p
Aelcrmi ne,- ra d -3 C t n1j, I
-,O-C L -a
z., a,c an age of 1,-5 x 109 year5. Nuclear 5~nthesi 10 Stif- , L" 'USIOr)
hf-- IUn a nd so on to form the 1'qhter e I em,!rl t v v r n*'
.~s the higher terperatures a n, pi e ~, s u r t s
w+~,Ich r,-.Ult In release, by ShoCk w-3veS in ail Jirect ioos, thus enriching

..3r r -
,n a, o .~av j Pmer s

p f
N

1,701.
ACCESS I
R;
6~r f tit 1' nt-- ltli.
W e
tA4 +14 ago n:agreeme Wt
I Ou 6trs
the age of the mateorltes.---Thts fqAtes that the sun and planets were tormed by a
ess to %it t zexp os Ori-t!4f: a neirby supernova. From the rate of decay
.,sing roc
assume,: I Z71
-to ai artdi~ca-~carrespanding to that of
oF 1 b j~ one.
cin deduce that thi! time betweer Pu,.1ear synthesis and solidification dal
of asterol
M.'terlal Was only '!(10-30.0 Millionryears. The author then discusses formation of
t6 CIO n
Vc-rzktarton And short--lived radioactivity.
T~,e latter Is requi red. to~ heat,the -a-iteraidal material to 900-iOOOC to C!xp lal n the
j t
crystalline structure, Ong ~ a-
t- ~thia,:.thtrd generation of stars in thl S:~ ;
g3laxy with a dlfferen~~ relatIve-4buridance of:heavy elemetits from that of older
stars. Simillar supernova- explos tons accompartted by shocinfaves in Interstellar gas
are still occurring, as,in the-case.of.Cygnis where there Is a radial outward
mevement at io.--Zo~lQil,*,O-,-e-e,*7-,"(~.7ti J---.. a strong radia-iscarcet
T'- cfars noiw- rt t.
~soo - mive~-apar :b--com[nof independent but ~ fol 1C'KdwF
- t :1-P evohj- onary path. The assoclatAd p)aisti r,innor nf 'Bourse be. seen.
"-riq- art. has: 4 'Agures.
ASSOCIAT014: none
UU
EN G L.7; 0 0
-SW
14 R EF', V-:- `00
2/ I've. '0 K-

/h b G_ 0A
Vi
9 A IN-T /T-3:t SM03 3 16_34 /04 11016 /100111006
AUGL; SION -R 6-ps"o 12,
A t: R Fosenkov V. G.
TIT'.&: The optical. propertieg, of the dwit cloud surrounding the
r i. h
SOURCE: 5~ 1964,- 1001-10G6.
apt c3L prop `iEirre'st-~&Lal_ dusts 'cloud, equal de i:
TOPIC TAGS: e r, y
Wts!;: 1'. RA C T
to CU ate:,, on, a purely theoretLeal
_'F._th6'
basis, tile gp.~i c a pr pertiel "o- - e -aosmic,'-du t~~#-Ioud surround-
tile earth, as observed fi6m the- eart'a after comystote cessation or
CWA 1. 1 sh t I t was assumed that the equal density -iurfaces can be
-rep v e a en te d,l~by_el I df_- ra ta t io relative to the plane of the
e c. J, i t: th, 14 t re din S
is'~ zero -id- the.._'immediata,
of -th4'_ t4.'rth and---
wi.-th- istance
an
dens L-t `6ie_4_ it, at La Ily- z vi th, istaace
d
_:C& CU' _on,
-xefjuired_~t
'tJoil tfte -at
di
0 if tar#ig ffij([Uait~rt it-a-dE'
Vo 6m- -1
--t A.I.-scattex-10-- -A' M0113phe
_7,
4K

-'NO; R F
4.~_A
adti, VT ~111_izeck~~C~219;~~_i3l~
I; tdhce-~, 6*f-- the, su --Is --shiTt An i-thli-.taaximum
.J. -&(Vat. of- thd.-.--' ust: -cloud- s o- &
sitf: tdiedtly_-~
kd-,

FESENKOV., V. G.
Orb:U, of the Tunguska meteorite. tx1teorltika no.25il63-167 164.
(Mllk 17:9)

0~' sata!!''~Os ":e, azz--~'1--,
..e-n-63 of aerosols of at~---osvaaric and ccs---~c cr,~
el --Jist7-ibution of atmosphtiric ozone. As the er;~,a-"s t,',,a earth's
fa C S
itnes s we a kens r,1pidI7. Th IS IWO ak e7lil-f:
-9 'rac z ion ion, re s1-,' f -cm a 7. -a On
-;7 -1i"ik and, hfnc~ docrea-'e L"I area-'- ZO -7~: "Z1'-3
-orsion denands on the height of the cbserver (or object) above the earth. The
act-or is signiricant in the effect or. artificial satellites and my be azou-
~eaause our knowladga o'L atmsphar5c .9 in the
~'--w dczen ki-lometers o" the atm(sphere is good. sc,:=r- -,ause of
1,, lk-
01-"I a -1 MUM

ACCESSION- NR:... T5G320Iz,'.'I'--
bri. ghi'.nass Ue4lblatlg- iU EltMOS-916fi eztiha tion in tho layers of the at =-sphere
due ~~)&rtly to riolecular acattering of 1 Int biat cnio:-'--Iy to ~ha effect of at=-6S--
i-9
pheric aelrosoln and.ozonei. Obsezvjitions are made at, dlffe~-emt -wavalenglhs in tha
visible range ';o pur.-;it dzsic'r~~'V'110:2 of Ithe difterant Causes, or the popor-'.....
i,.A,ons of each., Wavelengths sugdested are 0.60 microns in the oraqce regilon,'
0.42-0.45 nicr)ns ip the violet, and D.70 microng in the extreire red. Ozo6e has
a in tie 0.60 micron region, Observations should 'De bet-'Im before weak--
enin~; Degins, L.e,, several degrees before the satall"Lte anters earth's
sziuQow, ordar for proper construction of the phoiometric curve, to permit,
ton: of -q.,bangk tness,
proper evaluat
ASSOC itiit' AN- M2Akhak(V- IR.0 Ajt~--Ata--
4AIf X~
Cal
777 00 $UB;-cb
SU
0
it -110

KULIKOV, Konstantin Alekseyevich; FESM&OV, V.G., akademik, otv. red.
[The first astronauts on the moon; description of the moon
and the astronomical phenomena observable from its surface]
PeM-e kosmo.navty na Lune; opisanie Lurq i astronordeheskikh
iavlenii., nabliudaemykh a ee poverkhnosti. Moskva, Nauka,
1965. 188 P. (MIRA 18:4)

t in 6fio*m._th0 froi
A
b
-con
inoblo
looribtituent ~Of~- gEV
lbate Ioon nobulaoj.-,~
-,iL --- 6--i--tjjrjd
~':_ASSOCIATIONs: nond
;v~Aw
om -_~ WhL Oh
InL,-tho, -tic)
gR

tv

7 7
p 0 385
M,_

6ei re 'the'knglal of: lari- 50". --."lite observ0d
m- -7.
0 zdtioii is
ym

inearity -of
the antle.
e ttud solar tfine:~ a ows eat
a f Polarizatioa':with:tfi h rA 11~7~-ifiat:
'the polarization--of hi
pIrde r.. s C'atterf rde&',_` Or.
art. ;__7
t

V,
20Ka_
UBMTTED y65 -ENCLi

_:SlM
CODE
l

00
XO REr 1
ATWPRESSI

J..

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cwd

A dif N ~R, M019M SOURCE CODE: UR/0033166/ 043/003/0599/0605
AUTHOR: Fesenkov, V. G.
ORG: Meteoriticcommitte~, Academy of Sciences SSSR (Komifet po meteoritam
Akademii nauk S�S_R_~
TITLE: I~nterplaei ary dust and methods for investigating it
SOURCE: Astronomicheskiy zhurnal, v. 43, no. 3, 1966, 599-605
TOPIC TAGS: interplanetary dust, zodiacal light, sky brightness, zenithal,distance,
ecliptic plane, absolute indicatrix, asteroid, isophot system, periodic comet
ilk,
ABSTRACT: Interplanetary dust causes zodiacal light, which is spread over the whole
sky. Zodiacal light is mainly concentrated near the ecliptic, and its brightness
increases with proximity to the sun. The intensity of this light is characterized
by isophots- and polarization. Isophots are taken from results obtained by scanning
the sky brightness at various zenithal-distances parallel to the horizon and at
various subhorizon positions of the sun. The intensity of sky illumination by
reflected light from particles of interplanetary dust can be determined by-eliminat-
ing the light 'reflected from air molecules and the luminescence of some gases. The
remaining illumination is zodiacal light. The brightness of the zodiacal-light
component may be determined by measuring the sky brightness at the pole of the
ecliptic and eliminating lines which-do not belong to the zodiacal ligh~t. These
I Card 1/2 UDC: 523.59

03346----
L Cor.4
ACC NRt AP6019673
-measurements and the measured polarization make it poi3sible to determine the -value
of the zodiacal--light component. The brightness of zodiacal,light was determined b'
y
.this method and was found to be equal to 1/20 of the sky brightness at the pole of.
the ecliptic. The distribution of dust around the sun and its density in the-place
of the ecliptic can be determined by means of a known absolute indicatrix of dust
dispersion. Interplanetary dust does not result from the crushing of asteroids
because that quantity of dust does not satisfy the isaphot system obtained from
observations. [be stability of the quantity of inter?lanetary dust is explained by
the decay of peiiodic comets which restores the quantity of dust falling to-the sun.
Measurements of Ltwilight at symmetrical points in the sky make it possible
determine the brightness of the zodiacal light which can characterize,'the optical
properties of the terrestrial atmosphere. Orig. art...has: 3 figures and 13 formulas.
[EGI
SUB CODE: 04/ SUBM DATE, llDec65/. ORIG REF: 004/. 0TH REF: 00.1/ ATD PRESS
7. ~5 all

1
7

A
012
P6 P59

_~;(),-concei-'ire th4t an ap b f disinteg d

prqc.ia le, part: 0 .
ar rate
Aaatter-would-1W ejected into'sOace and would enter-the -sphere -of
attnction-_ of "the_ far.'more massivie ea rth. --Inot her l'ossible way inA
which the dust cloud could- be replenished ~is from the brakin of
9
raeteor3 or mic;~omateorites near the earth or the capture of meteor
Liatter. 'As al beady pointedin Ud: -article - _. in- to the

ordinary :matea t
rs observed:in;the:a mosphere:at heights of about
1,00 km, there I s -a far greater 'of -lmsteors'which simply pan-
6 trate the extq,)nsive layers of~ the earthIs-atmosph6;e at far great-,,
eir - heights - -and ~ again enter -inter
plaaet~ry:ipace-. .~ Thereare many
such meteor bodies. which:lrevo ~ariound-tthq.eiithlqr-a'.long time
'
'
grackally..repl(onishin .thb_,_&6t ~
Another posAbU 'source is*
&
~rom~ the brakiiig. Of. - closmic PaAiclesv Orig.:art haij: 9-.figureso
IJPRSI

EQ
-03 SOM DATE: hole -
SB CODE:,

F

-ACC NRt Ap'7006059
SOURCE CODM, UR/0384/66/000/004/0018/0022~'.-
(Academician)
AUTHORs FeibntV V
!DRG*., none
TITM. Can, comets cons fat. of antimatter?. q
-22
SOURCE: Zeml a I vselennaya, no.-Aq-19669 18
~y
ToPid.TAGSt antimatter, comet, meteor, star
SO CODE: 03
ABSTRACT: The literature,on the ssibility of connits consisting of
PO
antimatter is reviewed. Academician Fesenkov.successively considers the
meteor matter in interplanetary space, meteor streams and the penetration of'
meteor matter into the earthts atmosphere, nature and origin of cometse
ease
.,He notes that in the Galaxy antimatter can be manifosted by the rel
'pf. energy as a result of the-annihilation process during collis;on with
ordinary matter. Btirbidge aW Hoyle, for example, have found that
all the energy of.molecular and.turbulent motions; of the Inter-
if
stellar medium (approximately 10-11 erg/cm-3) Is determined by
annihilation, the ratio of antimatter to matter should be less than
one-ton-millionth. These authors conclude that the existence of stars
consisting of antimatter Is extremely improbable and probably impossible*
The annihilation of matter should also be-accompanicid by radio emission*
However, observations show tht!. Lihere is no such raelto emission from
individual interstellar clouds, but only nebular such as the Crab nebulap
:ftebulae in Cygnusq atce, remnants of supernovae. This and many other
facts Indicate It Is extremely unlikely that antimatter exists in the
.'_,qalqXy In the form of scattered matter or Individual. stars. It can be

ACC N-Ru AP7010707 SOURCS CODEt UU0364166/000/005/0005/0014
AUTHOR: Fasenkov V G. .,(,Academician)
ORO: none
TITLE: Natureiaf the moon
SCURCE: Zemlya'l vselennaya, 'no. 5, 1966 5-14
T021C TAGS: lurtar ten, perature, lunar crater.ilunar topography, lunar
.Optic property, lunar.orbit
SUB CODE: 03
ABSTRACT: Acadl~niclan V. G. Fasenicov has summarized our current Icnowledge
.of the moon in-the article cited,below. The following subjects, among
others, are con''3idered: the earth-moon as a double planet; the gradual
withdrawal of ti'nia moon from the earth; origin of the noon; tidal evolu-
tion of the earth-moon system; the lunar orbit'in thet past; thermal history
of the moon; radar observations of the noon; character of the lunar
interior; figure of the moon; history and nature of the lunar surface;
causes of changes of lunar relief; possibilities of Wnar volcanism;
nature of the.lunar seas and continents- ~F%th"' of the fortiat - on of
111nar craters; influence of cosmic rayW (. ijar wind; 0 ti It
oJ: the lunar kirface. Orig. art. hass : e sc P ca.4 properties
6 figures, -40.291/ i
- -III - . . . -, .1
Cdrcr
L

ACC NRi AP701
3154 SOURCE cora: UR/0025/65/000~01VO082 082
AUTHOR; Fesenkoy, V. G., (Academician; Chairman of Comnittee); Imshenetskiy,,'
A (AEA&
A. in; Director of Institute)
ORG: EFRE5EM,017' Cormilttee on llcteor!tes, Ari SSS,,t (rolilitet po meteorita-m
Ali SSS 11, f1a'zTt;V1I3Y
Institute of lrlicrobiolo3y, S~s',t (Institut
mil-roblologil AN SSSR)
TITLE: Collection of new meteorites
SOURCE: Nauka Lzhiznt,'no. 12P 1965, '82
TOPIC TAGS: meteorite, meteor. observation
SUB CODE; 03
ABSTRAM.
Another feature arUil e- in th'd Soviet prdbd -666iiragei"the
readers to be vigilant in a search for new meteorites. General in-
formation is presented,, such as that*three meteorites XAU. to earth
'Ann-dally in each area6 of a -4114on square idaometers. . Only 1, 800
met.4iorites have been discovered throughout the world. -The Academy,of
1/2
Card
0233 09XV

. . I . . . . . . . . . . .
ACC NR:
AP7013154
Sqiences USSR has a~ collection or 300 !Wisfazf 'aft(f -foroign meteorites,,
.one of the largest in the world. During the past two hundred years
only 134 meteorii.es have been discovered.in Russia; about half were
observed during I*alling, while the other half cannot be identified as
to dat*e of falling, During the last ten years the Committee.on,
.1-lieteorites of the Academy of Sciences has received only twelve new'
-meteorites* Almost all were found by chance by local inhabitants.
;The authors empho,size how impbrtant it is for peopleto report sus-
pected meteorite finds to-the Acade:kv of Sciences and note that'there*
is an established,mozietarr reward for each find. Particular emphasis
sis..giyen to the.importance of findingpgwly ;allen, meteorites that
Mirght contains evilence on the 'iOdstence of lif in space. cordngly,~
-instructions are given on the proper recovery, storage and paicking of
-finds in order to prevcnt aV. contamination., It is requested that =all
(10-20 g) pieces of suspected meteorites be sent to thZ Adaldemy of
.Sciences for ana%rais, whila*great care is.taken,to.safegua:6 the main
-body until.a report is -givenk: ORS: 34',593
2/2

FESENKOVA, L.V.
Can there belife on Mars? Zem.i vsel. 1 no-5:57-60 S-0 165.
(MIRA 18:11)
ti
F
MEN

Fesenkova, 11. G. "On the problem of the influence of the meclanical cormpos-1-
tion of soil on tho dynamics of salt format- on". Izvestiya A]-,-d. ante/ Azerltaydzh.
SSR, 1941p No. 10, p. 27-41, (Resume in Azerbaijani).
SO: U-3042, 3.1 Mw-ch 53, (Letopis 'Zhurnal.Irly'kh Statey, No. 8, 191,9).

. . . . . . . .. . . . . . .

:-Vitt E 1
W
.

7.
T
V
w
i
.
i7

E'~

ZAkdjA -Y. X., iF lbi
Ff
P- P EaUhab)e by HCL and P leuchable b~ 0 H tn
;~-subdividcd into wg and a,
rn a. y and ~~etaccous M,;:11,, -:w
."~r the sedsmCtIts move% 1"
tLe art. Thm-so& comain fjk~

be eitdbY 4W MfaiA W. NILOH~ Rcl,ext
pr
lmo.'"iOlUrAosily p

7

USSR/DUeases of Pam Animals. Diseases Caused by R-1
Bacteria and Fungi.
Abo Jour: Ref Zhur-Biol,, No 18s 1958o 8352B
Author : Drapalyuk, Ye. I.; Kulik.9 I.A.; Solov"va., Ye. M,;
Fesenkova N.S.-
Inst : No no tute is given
Title : Comparative Diagnostic Values of IJIEV /Ukrainian
Institute of Zxperimental Veterinary Ife-dicine
a 7
Tuberculoprotein and of Commercialay Produced
Tuberculin for Cattle,
Orig Rib: Veterinariya, 19589 No 1., 55-59
Abstract: 666 heads of cattle kept in tuberculosis isolators
and in a conditionally healthy envIronoment, were ex-
amined for tuberculosis with 1J19V tuberculoprotein
and commercially produced tuberculin used simultaneous-
ly. The first preparation provedmore valuable since
1,3 times more animals-reacted to it., and since rea-
GardIA ctions occurred faster,, and were more pronounced.
16

22267
5/109/61/006/005/014/027
D2 OVD303
AUTHORS: Siulinap G.Ai0*..Feshchenkov G.A. (Deceased)
3+
TITLE: Spin levels of Fe ion in corwidum
PERIODICALs. Itadiotekhnika i,elektrAika, v. 6, no. 5, 1961v
E106 614
TEXT: Good widerstanding of the electron paramagnetic resonance of
the Fe3+ ion in corundum islof great importance in designing para-
magnetic amplifiers since, because of small distances between the
spin doublet, a small or even no magnetic field, permits the reali-
zation of paramagnetic amplifier in the centimetric frequency-rang
as stated in T.,S. Vornivprko and A.M. 'Prokhorov (Ref. 1: ZhETT,
19519~ 36, 919j and J%N. King, ana it.*. Terhune (Ref. 2t J. App-
Phys. 19599 30, 1844)..For an arbitrary orientation of axes of the
magnetic field and of the trigonal axis, the Fe3+ ions form two
magnetic non-equivalent systems according to L.S. Korniyenko and
A.M. Prokhorov (Ref. 3: Z,hETT, 1957, 33, 805) and G.S. Bogle and
Card 1/7

2226
09/61/006/005/014/027
Spin le-vele ~of ... D201/D303
H.P. Symmons,(Ref. WPioca- Phys. S'oc. 1959, 73, 5~1) each produc-
ing its own System,of,llines of various intensities. The richness of
this spectrwa permitsa good stidy-of cross-relaxation phenomena in
a paramagnetic amplifier. The original work of analy8is,of the pa-
ramagnetic resonance of the Fe3+.ion in A12 0*3 was carried out by
L.S. Korniyeriko and-A.M. Prokhorov (Ref. 3s Op.cit.), who,shdwed
that the observed~spectrum.of'the electron paramagnetic resonance
can be explained by the-spiii-Hamiltonian as proposed by B Bleaney
iind R.S. Trenam (Ref.,6: Proc Roy. Soo., A., 1954, 223, ;); they
.also measured'its condtants a; room temperatures. The evaluation of
Eigen-values and of wave functions for parallel orientation was
done by V.M.'Vinokurov, M.M. Zaripov and N.R. Yafayev (Ref. 7: ZhE
TTI 1959, 37, 312). In the present article the authorSevaluate the
numerical values of the levels of energy for an arbitrary orienta-
tion of the magnetic Xield.with respect to,the trigonal axis in the
planes, for which all ions are magnetically equivalent. Numerical
results are compiled as tables and graphs which permit determina-
Card 2/7

'2214
I OY961/606/00 5/01 ~/027
Spin. levels, s0f D303
tion of the -ralue of,,.the magnetic fieldi -the orientation,of the
crystal and. #he wave'length of.
6 'the subsidia y radiation. This per-
mits d ig of
es n a paramagnetic bLmplif i e'r for.a given frequency,band
an4 evaluati6n of.the 'probabilities of tranSition f or the main and
the subsidiary.,radiation.,:The 6plitting of spin levels of the Pe3+.
ion in oorundi'6.is described by 'the a in-Haxailtonian of the form
p
4 ~4 + &24- Ts (S + 1) (3
4-41 M+3 3 - 1)]
+D I+
F 35 P. -30 S (S + 1)
A:
+ 25 -6 (S + 1)+ 3 SI
w e ef 'Iotive.'gpin 5-) 8 a 1 8 opera e
I here S th f
tors of th
2 x 3r z
spin projecti'on on.'the-axes of the co-ordinate sy'stems, for which
z-axis coinoilles with the trigdnal ~ xis of symmetry of the c
a rystal
-of tlit~ epin-projections'in the c tibi c
field; :Sg i operators,
Card 3/7

22261

Spin levels of s/iog/61/006/005/014/027
-
D201/ 303

'Vi h sin a 8+2b
"
hsin
ct
T
1+ 2 4 cos
al
At
fk .

0 3

yhsincg
8 -P2b

hsifia
0

COS
a
0 .0.
-
h
l
a
s
n
T
3
h cos a
0
0 h sin a
10-b

h
ll
cos
a

Card
5/7

22267.,
S710!)/61/006/005/014/627,11
Spin levele'Of D201/D303
13 a'- -F 0. 2 V5- a
where Hp b are dimensionless quanti-
D 3
ties. The Eilen-values are~the roots of the secular equation
0, (4)
where It oan,be: shown~ that these roots are real numbers. The-
authors have!~,numerically evaluated in 33'q. in the internal a = 0
goo o h O~: - 5.9, in. steps A h = 0. 1 1 nioc 50. The behavior of'
energy levelis with thechanging magnetic field is graphically repre--..
sented for Ob = 009 30o, 60o and 900 respectively. The qppendix
gives the -values of:energy of-spin levels E of the FeXl' ion in
corundum for eight.orientations of the extelln'al magnetic field rela-
tive to the 'trikopal axis of the crystal (Ot 0.1 15, 309 45, 60t
75, 900) in isteps -,6h = .012 (,6H 364.5 oersted). It has to be
calcuj~6ib-ns
pointed out- 'that in ..,the value
Card 6/7

212%67109/6 1/006/00 5/014/0 27
Spin levels of ... D20'1/D303
6~ a - P +
= 3.1104 has to be added to matrices (3). The authors
-D 12
express their gratitude -to AOM. Prokhorov Emd I.Z. Korniyenko for
their interfist and help. There are 5 figures, an appendix with ta-
bulated numerical results, and 7 references: 3 Soviet-bloc and 4
non-Soviet-b-loc. The references to the English-language publicati-
ons read as 'follows: J.E. King, RA. Terhune, J. App. 1 Phys-v 1959
309 1844; G.S. Bogle, H.F. Symmons, Proo. Phys. Boo., 1959, 73o
531; N. Bloe-mbergm, S. ~hapiro, P.S. Persham, J.0. Artman, Phys.
Rev., 1959,,114, 445; B. Bleaney, R.S. Trenam, Proc. Roy. Soc., A.,
1954, 223, 1.
SUBMITTED: Yarch 29p 1960
Card 7/7

XORNIYENko, L.S.;_FESHCHENKO, G.A. [deceased]
Oalculation of the matrix elements of the transitions between
i?e3+ ion levels in corundum for an important practical case.
Hadiotekh. i elektron 7 no.7tl241-1243 162, (KRA 15'-6)
(Paramagnetic resonance and relaxation) (Ferrates)
(Corundum)

MALITSEV, :?.M..; FESHCHEWO; I.M,
... . ...............
Spectrophotometric method for the identification of alcohol
admixtures. Khar, prom, no.lt4l-43 Ja-Mr 165. (IURA 1814)
ITS WE

FWHCHEVKOI N.G.; ALSKSEYEVA, TeIt; KIRSANOV, A.V.
Allcylationof phosphorus diiodi4e with higher alkyl
ialideb.~ Zhursob.khim. 33 no.3:1013-1014 Mr 163. (MIRA 16:3)
1. Inst44 organicheokoy kbimi:L AN UkrSSR.
(Ph
(Zorus iodides)
1 iodides)

'i, JAM-
lii~~7k' MZ~~
FESHCHENNO I.-I.- NAMYATOV, G.N.; VISHNEVETSKIY, M,L,; GLOVATSKIY,, A.B.;
,---I
Putting into operation a41ntering department at the Karaganda
Metallurgical Plant. Stall 24 no.8-.676-6.78 Ag 164.
(KRA 17:9)

.---;-!PSR/Organic Chemistry. Synthetic Organic Chemistry. E-2
Abs Jour: Ref.Zhur Khl*iya, No, 8, 1957,~ 268786
Author Babichev,- F.S.j Feshchenko, N.Gi,
Miroshnichinko, .' n.-9- -
' kir 7Z- If/h I /.
Inst _-v SZ9 -Ulvly~ C--'SxevCA'enkO
Title (Bensothiazolyl-2)-Alkylearboxy:Lic,,Acids. IL
6-Nitro and 6-Aminobensothiazolylalkylearbox'ylic
.Acids.
Orig Pub: Ukr, k.hima-, zh.t.1956, 22,t No. 4t 511+ - 517.
Abstract: -(6-nitrobeiizo-thiazlyl-2)-pro:pionic acid (IV),
V(6-nitrobenzothiazblyl-2)-butyric acid M
. (6-nitrobenzotliiazolyl,.12)..;va~leric acid -(VI5
and acid .(VII),O
reduced to corresponding 6-amirioacida'i(IVa
VIIa),w'ith Sn and HC1 were synthetized by the
Condensation of 2-amino-5-nitrophenylmercaptan (I)
Card 1/1+
--------------------------------------- ......-

UR~SRAP*ganic Chemistry. *Synthetic Organic Chemistry. E-2
Joixr: Ref Zhur Khimlya No,-, 8 1957 26878.
-with anhydrides of succinie IIJ10 5giutaric
(III) adipic or phthalic acids; -(6-motoxy-
ben~w~hiazolyl_2)rpropionic aciet (VIII) and
V -(6.-'ketoxybenzothiazolyl-2)-biityric -acid (IX)
-were prepared by condensation ol' potassium 2-'-'
amino-5-mothoxyphtny3-morcaptide with II or III;
IVa and VIIa were converted conforming to
Sandmeier into-,4-(6-dyanbenzottiiazolyl-2)-
propionic acid, meltin point 1990 and o-(6- -
chlorobenzothiazol 1-2 -banzoic'stold (yield 56%,
'melting point 1930T, respectively. 6.3 9 of 19
3.7 g of II and 15 ml Of CzH6 aive.boiled 1 hour
and IV (yfeld 71% meltin -Point 1630) is
.separated; methyi eater M) (raelting point 170-
1720); anilide A) (melting point 165-1670).
The following are'producaganalogically (the yield
Card 2A
USSR/Organic Chemistry. Synthetic Organic Chemistry. E-2
Abs Jour: Ref Zhur fdamlya, No. 8, 1957, 26878.
In % and melting points in 0c Of V to VIIP -
th4ir-ME and:A are enumerated: V - 529 1499
72-73 '147-148.1 vi - 63 9 94 (frika benzene)
127-1N 1~p;- vii - 819 242 1656-1680 200-202.
1 g of 6n 'is .addid'to the hot solutio of TV -
VII in 10 ml 'of concentrated HC:Lq it is heated
1 1. hour, alkalized--with 12%-ual'isolution of NE4+OH9
filtered the solution is neutralized with di-
luted HH and the following are separated (the
yield in % and tho boiling poirybs in OC of-IVa
VIIa and of their'benzoates are enumerated:
IVa - 79-59 2180 230; ME, melting point 1620-
Va - 77.8 141 242- VIa - 55 133 163- or hia-
Oj 133 W 'or VHA - 83, 216., 25~. 3~ 9 of
55
K i in 130 mi of aXdohol-is added in three stages
to 30 g of 6-rdetdxyphenylenethiRzothionine
Card 3/4

KIRSANOV, A.V.; PESHCHENKO, N.G.
Trichlorophosphazosulfonenitroaryls and the productB of their
hydrolysis. Zhur.ob.khim. 27 no.10:2817.-2820 0 157.
(MIRA 11:4)
I-inatitut nrpantChA2knv lehlmll AkAAAMH nAUk SSSR-

C,// -F
A 1: -A 1 Oh S Kirs_,nov, A. N. Feshchranko, Y. G.
TITIZ:
PERIODICAL:
~ABSTRACT:
Card 1/3
,/A
Trkiiathoxy-.and Trittrorjpbos,)Iiaeosu:Lfonnitror,',ionyl.3 und Diestcre of
Ifitro,r~hcnl,tlc~ulfonaai0ophosphoric Acido _J triaroksifoz-
i'azosullfonnitrofenily i diefiry nitrofcnilsull,--'on.-.~.iidofos'Lorn,,I~.b
kialot)
Mitmr, 1Obshchey kliiiaii, 1-956, Vol. 28, TTr 2, Pi:- 339 343 (USSR)
Trimethox.- and triaro)qphosphasosu:Lfonnitroplic-nyls (I) end diesters
of nitrophen,floulfonaraidoph6sphoric'acids (II) wure synthesized for
the purpose of investigating their insecticidic properties and as
ZL starting point rfor the production of N-phos]~boi:ic acid, deriva-
tives of 3ulfanilamides. (I) --;as obtained by intcraction of tri--
c:hlorophosphasosulfonnitrapbc-riyls (reference 1) with i.~wthylate and
sodium arylates in a benzene zolution (reference 2)t, Trimetho-V-,_
triphenoxy-, tri-p-eblorotri-1henoxy-, tri-o- and tri-p-trinitro-
I;riplienoxyphosphasoziulfor.e-o-, ri-i- and p-nitrophen,' rls (I) (table 1)
were obtained in this manner. (I) represent colorlesJ crystalline
oubstances of a neutral character. 'hey do not di3coive in water.
T
~erimethoxypbosphaziot3ulfonnitrophenyls (III) within one hour saponi-
fy on boiling with 96% alcohol to the corresponding diesters (XIV).

75-2-13/64
Trimethoxy- and Ti-iaroxylihosphaeosulfonnitrophenyls and Diesters of Nitrophenyl-
sulfontimidophosphoric Acids
Triphcnox,,,,pl,iospliasosul:Connitrophenyls (IV) do not c'Liawre under the,
same cona
dition!~. Trimethovr- and triplienocypliosrhasosulfonnit 0-
phonyls ii'lelt at co-,iparatLvely low teaperatures (frzri rr, - 10'T C).
(1) do not saponify upon the influence of aqueous alk:-line solutions,
vhich i2 e;cplained by their insolubiliLy in vi~ter. In ncueous alka -
line L;pirit zolutiona they cavily saponify to (II). 1;11t;- (n) can
i.iore conveniently be produced from diciiloroanhydridcu of iiitrophe-
n;f1sulfonauidopho-ophoric acids (reference 1) by means of the in-
fluunce of sodium arylates and - mctliylate in a dioxane solution.
Thus dimetbyl-, di-p-chlorodipbenyl-10i-o- Lmd di-p-nitrodiphenyl
ethers of o-, m- and p-nitrophenyloulfonar,-,idophouplioric acidu (II)
(table 2) were produced. (II) coji be elim-inated in the form of
stilts, but it is more convenient in 'he form of free diesters.
(II) represent cPmj~aratively hioli-melting (from 134 - 19400, cry.-
stalline, colorleso. substances insoluble in water. 'Picy melt at
far higher.temperatures than'the corresponding (I), with the ex-
ception of two p-nitrophenoletheru (XI and XIII) ahich Aelt under
the corresp ondin,-, (I). (II) are monobasic acido w-hich exactly tetra-
te in the presence o .f phenolphthalein and yield viell-crystallizing
and vrater-soluble sodium salts. It is interestin.- that the sodium
salts Of the p-clilorophenylethers of nitrof~lienylsvlfonai-tidopho3-Dhor-
Card 2/3 ic, acids on. withdrawal of the water solutions by the ether co:a-.

75-2-13/64
Trimethoxy- and Triaroxyphosphaaosulfonnitrophenyls and Diesters of Vitrophenyl-
sulfonamidophosl,horic Acids
pletely Go over into*the ether layer. Sodium salts of other diesteis
are not withdravin fron the water solution by the ether. '.ehere are
2 tables, and 1 Slavic reference.
ASSOCINTION: Institute for OrGanic Chemistry AS Ukrainian SSR
(Inctitut- organiches"loy 1,.himii Akaderiiii nauk USSR)
SUBMITTED: Duceiuber 24, 1956
AVAILABLE: Library of Congress
Card 513

79-28-4-41-1/60
AUTHORS2 Kirsanov,-A. V. Feshchenko, IT, G.
TITLEi Eater 0'f Aminoplien'ylsulfonamido-l"hosphoric Acids (Efiry
aminofenilsullfonamidofoefornykh kislot)
PERIODICALs Zhurnal Obshchey-Khimiij1958,Vo1,,28,, Nr 4~PP-1049-1052(USSR)
ABSTRACTs Dimethyl- anddiphenyl eater of o-,, m-9 and p-aminophenyl-
sulfonamido-phosphoric acids (formula I) were produced ac-
cording to the following reaction schemes
HCOOH
NO C H SO NH -4- - 110 206H4SO2N-PC13 IN, ITO 2C6 H4SO21MPOC'2---.>
2 6 4 2 2 _ffI
5
- > 1102C6H
s02 NHPO(OR )2 -6 --H--)' lfll2C6H
So2NHPO (OR )2
4
4
2NaOR
The reduction of diesters of the nitrophenylsulfonamido-phoo-
phoric.acids was performed with hydrogen at presenee of a
palladium catalyst in alcoholic solution at room temperature
and at a pressure of ca. 100 torr. The yields were quantitative-
Card '1/4 ly. The diester produced by this way form colorless crystals,

Ester of Aml.nophenylsulfonamido.-Phosphoric A, ci (is
79-20--4-43/60
which have only weakly basic, but strong acid properties. They
solve readilyin aqueous soda solution and can be titrated as
monobasic acids. Their aqueous solutions react acid with Congo
red. 'The dimethyl eater of the aciinophenylsulfonamido phos-
phoric acids-are readily soluble in hot water and can be di-
azotized on the usual conditions (as aniline). The correspond-
ing diphenyl ester are in hot water diffivultly to solve,in
alcohol more readily soluble. They can be diazotized on the
same conditions an aromatic amines with electronegative sub-
stituents (e.g. nitroaniline).
The amiden of the o,,, m- and p-aminobenzenesulfonic acids~
to the derivatives of which belong the compounds of the ,
formula 1. have little different inelting points 05309 1420
163'). The' lowest melting point Y9LS the m.-isomeric, the high-
est -the p-isomeria (Ref 3). At the corresponding isomeric
compounds of theformtila I on the contrary the melting points
ate far from each other. The highest melting point here has
the m-isomerieg the loveat 'the o-~;"m meric. The ortho amino-
compounds of the formula I are at room temperature very readi-
ly soluble in acetone, the para-inomeric only with difficulty
Card 2/4 and in case of heating. The meta-isomerics are practically

79-28-4-43/60
Eater of Aminophenylsulfonamido-Phosphoric Acids
Card 3/4
insoluble in acetone. For the strong change of the melting
points as well as for the great differences of the solu-
bility in acetone the following explanation is probablet
In the case of the o- and p-isomerics intra.. and inter-
molecular hydrogen bindings form, the formation of which
in case of.the m-isomerics is complicated or impossible.
The influence of the hydrogen bridges upon the melting
points of the amides of the aminobenzenesulfonic acids
is because of absem e of the polarizing influoue of the
phosphoric acid rest essentially lower; therefore the
melting points of the isomerics are close together.
For the characteristic of the compounds with the-formula
I their benzoyl derivatives were produced according to
the method by Schotten.-Baumann. These compounds form color-
less crystals, which have strong acid and no basic proper-
ties. Their aqueous solutions ri~act acid with Congo red..
The melting points partly are higher and partly are lower
than the melting points of the oorresponding compounds of
the formula I.
In an experimental part the synthesis and the properties

79-28-4-43/60
Ester of kninophenylaulfonamido-PhoBphoric Acids
of'the compounds of' the formula I and of their benzoyl deri-
vatives are described exactly. There are 2 tables and 4
references, 4 of 'which are Sovidt.
ASSOCIATIons Institut organicheskoy khim-4i Aicademii na4k Ukrainskoy SSR
(Institute for Organic Chemistry,AS Ukrainian SSR)
SUBMITTEDs February 149 1957.
Card 4/4

M,
5,3630 77398
SOV/79-30-1-59//78
AUTHORSt' Kirsanov, A. V.., Feshchenko, N. G.
TITLE: Esters of Aminobenzoylamidophosphoric Acids
PERIODICALs Zhurnal obshchey khimii, 1~960, Vol 30, Nr 1, pp 267-
270.(USSR)
ABSTRAM Esters of aminobenzoylamid,ophosphoric acids were syn-
thesized according to the following scheme:
+ 11000H
T40,C.H4CONH2,t='P29 NOAH.CON-PC13111
NOjjC5H4CONjjPOCj2[1j �!-'tolla. r1O2CsH4CON11PO(OR)2j2j
Pt
NH2q1hCQMHPO(OR)j,-
Dimethyl and diphenyl esters of nitrobenzoylamidophos-
phoric acids were obtained by the previously described
methods (A. V. Kirsanov, Izv. AN SSSR, OKhN, 1954, 646;
A. V. Kirsanov,.R. G. Makitra, ZhOKh, 26, 905, 907,
Card 1/4 1956, and others). The nitrobenzoylamidophosphoric -

Esters of Aminobenzoylamidophosphoric Acidis 77398
SOV/79-30-1-59/78
acid's were reduced to the esters of aminobenzoylamido-
phosphoric acid in an alcoholic solution in the presence
of a platinum catalyst. Yields and the properties of .
the esters are given in Table 1...In order to character-
ize the above esters, their benzokl derivatives were .
prepared by the Schotten-Baumann reaction (see.Tabl.e 2).'
There are 2,tables; and 3 Soviet references.
ASSOCIATION: Institute of Organic Chemistry, Academy of Sciences,
Wrainian SSR.(Institut organicheskoy khimil Akademii
nauk Ukrainskoy-SSR)
.SUBMITTEDs Januai-j 19, 1959
Card 2/4

Esters of Aminobenzoylamidophosphoric Acids 77398
SOVIAT9-30-1-591'78
Table 1. Dimethyl and diphenyl esters of aminobenzoyl-
.ami'dophosphoric acids of the type NH 2CA CON11PO(OR )2
Card 3/4
0 CH3 82 wArneejesl 14U-1520 iIA9, C9111304N21' 11.48 + +

M
CH
70
l
l
r
h
1125
127 11.60
24
11
C
11
N
0
11
48 +
3 a
co
sm
a
Fr - .
, 13
P
9
4 . +
11.07 +
P G113 84 olcolvifrfirms 169-170 1132, CqIljj04N2l' 1 .48
11:23
o Co 115 01 700/0 alcokol, W-W 7.62, C11111104N,P 7.61 - + + - +
needlet . 7.42
rn C611r, 9t 700/0*lohkrJ-,, t67-169 7.45, C,911,,04N2P 7.6t - + - - +
net dlis 7.43 +
CoHd 97 benzene or-- M-M 7.52, C191117041NIsP 7.61 + - +
alcohol, 7.42

STALLJ-
CRY CA
4m ZAT MELT1140 FOU10 EMPIAWAI I.ALIC1111 SOLUVII.O*Y'"
R VIA 1A0N14D#A41P- POINT N FOR14ULA
FrARANCE u
IK u- inscluile a+ 6 SIT hf
+ slightly SoJublTaf 20: 050d readily volump- at If;
t 501UWV- of 440

Esters of kninobenzoylaniidophosphoric Acids 77398
SOV/'79-30-1-59/78
Table 2. Benzoyl derivatives, of the dimethyl and
diphenyl esters of aminobenzoylamidopbosphoric acids
of typez 0 6 H 5 COMIC 04 CONHPO(OR )2'
POSITION JW I MELTING
0
0 C113 98 1162-1640
In C113 731,165-168
p CH3 94 '186--188
0 cotla 96 :171--173
m Calig 86 i82--18A
p C,11, 93 193-495
Card 4/4

FZSHCHEM, N.G.; XULWIOV# A.V.
Phoilphoars iodides, , Zhar, ob. khim. 30 n0-9:3041-3043 S l6o.
(MEU 13:9)
1. Inatitut organicheakoy khimii Akademii hauk Ukrainskoy SSR.
(Phosphorus iodide)

FESENKO N G.; ROGOZHKI9,, V.I.
Acc%=lation of phosphorus and nitrogen coupounds in TSialyanak
Reseirvoir during 1954-1957 and changee in their diacharge at the
vateir gauge point of the bydroelectric center. Gidrakhim. mt.
30:3.0-31 160. (MIRA 13:9)
1. Gidrokhimicheskiy institut AN SSSR, lovocherkasak.
(TSimlyansk Reservoir-Water-Couposition)
(Phosphoras) Olitrogen)

FESFANKO, N. (6
Chenical composition of vpa~-ters of the Northern Donets River in
its most polluted stretch. fidrokUm. mat. 30:65-74 160.
(MM 13:9)
1. Gidrokhimlcheskly Institut AN SSSR, Novocherksawk.
(Worthern Donets River-Water-Composition)