SCIENTIFIC ABSTRACT NIKOLSKIY, A. P. - NIKOLSKIY, A. V.

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• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

hITOLISM9 L. P.
Ofte, Dially Tarlatlons In Disturbances of the YACnatle Field in Hi&b Latitude.*
ft"b. Aftog KdAt pp 5-59,v 1938
I- ~ uwa~#~ 4-b.33 7d-

! ::-, L-.
Photographing Auroro-~ Borcolea in Tikh-jyn Bay.
rroblemq Arktikl, 1939, no. 10/11, P 131-1103.

A.! .
"on tho~ miture nf gooma motic dislurbanc93.0 Priroda (11), TV ~-12, 1.91-7.
Translation-0- 146077, 22 July 1954.

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" --Ilskly, % - . *T*I-.'!! , 11 , , " I na - -. '. r c C~ - , -, r. - -, f! t 1 c4,- ~s v
Frobi-1%, 1, 1 ~-? /. " ,-:-, - . 47-,'~ ~, ,I
so: 12 Feb. ~.,, (Lo-topin I I Z~-,urro I f nykh Stztay, ':.). c, 1-~,4 )).

I- *~, ,
7-1 -~ FL L LF~ t .
Terbetint -*On the nature of t4e % verage vgrittions at bigh la Mules In tte
disturbed mgmtic fi,914,,O Probler7 krktiki, 1948 (Published In 19400, Lo. 3
p. 79-94, - Bibliop 15 ite"
S09 U-4355, 14 luomt 53, (tatopla 'Zhurnal 'n7kh StAtey, No. 15, 1949.)

Nfi K, C, 12 t, K
timiceophymi.cs Magwtic f Ield of WM FD-2900
CG.V IL12 Pub - 45 - 11/11
Author [Mollskiyo A. (reviewer)
Title Handbook on the variable magnetic f teld or the USM
Periodical Izv- AN SSSR, Ser. georiz., Nov-1)cc 1955, 561-565
Abstract Review of Spravochnik po peremernoW mgaLtno= polyu SSM, of 268
pages, published 1954 in 600 copies by the Flydrviseteorological Press
for 16.30 rubles. The material of the handbook is given tabular form
(M tables) and also In the form of graphs (95 graphs), which give
Information on the variable magnetic field in all regions of the USM,
representing the data of 18 active magnetic observatories (12 of which
disposed In the middle latitudes and 6 In the Arctic) and covering
the period from 1938 to 1948- It was compiled by scientific associates
of the Scientific Research Institute of Terrestrial ttgnatism under
the editorship of V. I. Afamelyeva, and Is valuable both for theo-
retical Investigations in geophysicr. and also for practical engLneerg;
working the field of geological prospccting by w4g&etlc methods. The
reviewer notes that the variableness or the FArth's magnetic field
is flue mainly to the action of the Sun. In the main this handbook
is necessary for investigators of physical phenomena occurring in the

Card 2/2
Ab3tract : uawr layers of the FArth's atmosphere at a
higher; e.g. normal and abnormal ionization,
disturbances, etc., radio wave propaotion,
Institution : -
Submitted : -
FD-2900
height of 80-W0 O= and
polar lights, rognetic
etc.

llwwsur, L.P.
Cn- -4SC N.JP.Boagk&Walg &Md W.G. lariamwole &rtlele llrabm K
asswUng to "" of the FmIeveldt Madmotte Oboorva*4m7 for
1916-1939.0 TrWiy IIIZK &o.11:111-119 155. MIL 996)
(WaVottes, Terre4rUL)

OnOL(sirr, AOP*
-mOte distibdies at segmette dfsturt~ In Ike, polar region
or Uts Aratte. Vskl. M ~ log se.5ag".02 Ago 1"60
(am 9cle)
10 querrale
reefttffl~ mmimthm Toy@ mmlolkwas
(Arette formotrtal)

1: U01. I Iqlav. A I S.
"Distribution of Magnetic Disturbancss In the Arctic Region Near the
Polo. 0
Me ThUgmstlon Association of Goommontimm md Aermcow; Abatracte
of the Reports at the II Generol Aseembly of the Laternational. Uhlcmm of
Geodesy Obd Geophjrelcm) Moscow, Izd-vo AN SM, 1957. 46 p.
Abstamats Inv0dw chuVe In the magnetic field us the main Indication of
dldturUOOM ID fth h16b lAtItu&W- nw forwis MA uvILtuds of the daill rat* or
dIdUltsZkOft we detamalmd. by the effect of the ewrtble pwwmwat magmtIc field
an the imoffil" Jets or solar particle*. fto diurnal variations In hI& A
lat,46des are, Very cmViez. Observations neer the polo sugmest the 4XIStenow of a
toeon
,%_j some of Increased Intensity avid ftequemy of mpatlc d.14twbences close
to 80 WMAVIOUG latiGu4s. Thin Is veU In accoge with the studios of aurmul,
avA lonampberic d1sturbomes and fits the tbooretlc&l ftndt of AlfTen.

WIVOL(MTO A.P.r red.1 MMHZKIKL, LP., tokhn*rode
- u
EswulfA Of =Cast* *We. v tiew V polar oWervatortse twtog
l"if-I"51 an" 11617 mattleft sautudeldt witarefft ob"I I.,
ts&-io *Mrdiwl tramportl 1957* LActlimbesidt
Institut. *a "I. .2m) ~ Odu ut?)
(Antle reeem.-IbCuttin, femstrtal-4&")

lalowsurt, A.P.
---------------------------------r
ftstrilation of awaotle disturbRaces to the Antarctic, Prou,.Arkt,
60621241-244 157. (KU Us 12)
(Astaratle regions-ftaotlaw, forrestrtal-Socular urtation)

j i
AUTHOR: Nlkollakly, A.P. 3T-11-6/18
TITLZi egarding N. p. Ben,koys's and M. 0. Borlsova's article
Index K Basso an Date frow the Favlovsk PAgnetle Observ-
atory for the Years 1916-19390 (Po povodu stat'i
X.P. Ben1kovoy I K. 0. Borlaovoy *Indeks K po dannyu
Pavlovskoy magnitnoy observatoril za 1916-1939 gg.")
PIRIODICAL: Trudy Nauchno-isoledovatel skogo instituta zesnogo
wagnetizaa, 1957, Nr 11(21i, pp. 111-118 (USSR)
ABSTRACT: This Is a review on the frequency d1stributlan of mg-
natic activity and the dally, yearly and 11-year cycles.
The following authors are mentioned: Kalitina , G.N.
Mishin,, V.N.,, and Kozlk, S. M. There are 2 figures ;nd
4 references, all USSR.
AVAILABIA: Library of Congress
Card 1/1

OT301 1101of KIT - P. ?A - 2241
TITLIC JWROA~81019rftpvdi-ro Distribution of Radio Blackouts in ligh,4Latitudes
(I Yoprosu o googratichtakox roprodolonit Y wyookikh shlrotakh
anomal'nogo pogloshaheniya radiovoln v atzooforo).
PERIODICA1 DokladjY Akademli Bank SSSR, 1957,Vol112,Wr 4,yp 628-6~1 (U.S.S.R.)
Received 4/1957 `- Reviewed 5/1957
LBSTRAOT The ocourranoo of those absorptions is In many o4soe oonneatel with
the simultansous occurrazice of magnetic disturbances. This fact
allowed the asnmption that'the reason of thee# absorptions Is the
penetrating of solar particle& into the upper layers of the atuo-,
sphere of the earth., One of the problems investigated hitherto only
little concerns the dependence of the time of the maximum (ir. the
daily course of the probability of the oacuy4&no* of absorptions)
on the geographical situation. Such absorptions have been found
ostly to occur during the first half of the djq., Some previous
:
orke bearing on.the matter are discussed In short.
The author believes it boat to choose such a time as corresponds to
the irAo4iate m&xisnla on the ourv* of daily- dlstribut~or, of' absorp-
tion-probability. The author also o&rri*4 out this. Aftable can-
tains, thee* moment# relative to local time an& the *as* relative to
Greenw1oh-tice. The maximum of absorption-probability (,which **air#
during the first half of the day) agrees well.with the time of t1*
oaourr&nco of the maxisrum.of riatitutinal magnetic disturbanceal for
Card t/2 those ionoophoro-st&tlona for which data, concerning magnetic. eatir ty

AMOR KMOL'Sillr , A. P.
FL - 225t
TITLN -
Distribution of Kognotic Disturbance* LZL the Lnt-
&ratio (K vapraou o geograficheakon raspro4olouLl asgultalkh
vosmuskshoury v antarktike). I
MIODICAL Voklady Akadeall Wauk SUR, 1957,T01 1129ffr 59PP 846-84a
ItesoLved 4/1957 Reviewed 4/1957
ABSTRACT It soul& be of interest to verify to what sztent the rules govern-
Ing the geographia distribution of - - Mag *tic Usturb"464
-
-
(amok as art encountered in &ratio rogiii
if
Yapply also In thoant-
aratio. If the leolinse of the simultaneous occurrence of matutinal,
nagastle disturbance La &ratio region@ haw* the shape of spirals,
which wind themselves out of the pole of homagenoome magnotIsation
in the ftroation of the hands of a clock$ the spiral@ In aatar4tte
regions oust emerge from the pole In the opposite Unction. Certain
assumptions are now to be made coscornine the rules possibly govern-
ing maCmetle disturbancee In the unexplored antarctic regions the
sacuracy of which could Ve vorMst by observations mAo In saaaoc-
ticsi with the coning geophysical year. The system of spirals moving
In an antLcloakwLse direction is here plotted In the antarctic In
such a manner that the point of the homogeneous magnetization of the
system of spirals agrees with the polo of the honagensous magnoti-
nation of the antarctic. Furthermore, the system of spirals is turned
in such a manner that It sCroon best with the observed datao If the
three *'*look spiral Is plotted through Cap* Donalson, the 20 o'slook
Card 5

PA - 2251
On the geographic Distribution of maenstlo Disturbances to the
Antarctic.
ASSOCIATION Institute for the Arctic Scientific Research of the Northern Naln
Sea Routs.
PMUTRD BY T.T.SKULZYKIN, member of the Academy, an 23. -1. 1956
IFUNUTT 11. 9. 1955
AVAILABLZ Library of Congress
card 3/3

Alf /- If
AUTHOR Nikollskly, 'fi.p. 20-1-2-2/54
?ITLE ft the Planetary Distribution of Ionospheric Nagnetle Disturb-
anoss and Aurorae
(0 planeternas raspr*delenit nagnitno- Ionoefernykh wozmushchenly
I polyarnykh siyaniy)
PERIODICAL Doklady "Adenti ftuk SSSR, 1957, Vol. 115, Pr 1, pp. 84 - OT
(USSR)
ABSTRACT The author finds out the possible location of the four StOrmer's
ones with Increased penotration of protons into the terrestrial
tnovphere In which an Increased Intensity of the magnetic Iono-
:
spheric disturbanGes as well as of aurorae art to be observed.
The author starts from the known facts on the geographic dlatribu-
tion of these phenomena. An analysis of the Isochronous curves of
the maximum of magnetic disturbances speaks In favour of the fact
that on the Western hemisphere the protons con advance to a lati-
tude of 400. From 8 - 12 o'clock (worldtino) favourable condi-
tions for the advance of protons may even exist to equatorial
reas of the earth. Tho author points at experimental data in
;avour of this unexpected congequenco. Me ex4ct Investigation
of the experimental data on magnetic Ionosperio disturbances
Card 112 made it possible to outline In first approximation the con* A

NIKOWSKIL, A.P.
Diurnal distribution of Irregular magactic dieturbarms at Idgh-
latitude staticas or the western and eastern twaispheres. Geasag,
I aer. 4 no.5s968-971 3-0 164. (MRA 17111)
1. Arkticheskiy I antarktichaskiy namchno-issledovatelfakty institAt.

- : . 'r- F - - - - 7 - -
T7 r-
zwrym-~,G-Fmy~V A, P- 7-L Fr-
"Olm ths DmdMzat1OU Of DK11Y Varlatiocs of VAgnatia ActivIty,"
pa"r suboltted,, 5th Men, Assomblyp CMIO, Intl. 060*ysical Yoar, V46cow, 1-9
August 1958

:,- ~, V"', -,-, I V , ,
~ , ie V.,
"on the Methodic Proble=x Camected wits, Ccoqnrlng Yhgnatlc- Distur"-,ccs c.1 the
Artic and Antarctic,"
p4W gmaa-Aed at Um IM Gaawal AssmZty oC Um IAU, liuscov, Aug ISrA.

C-O 0
8330
3/169/60/000/00-Tr,~ ir~r_ 16
A005/AOOl
"'ranslation fromt Referativnyy zhurnal, Geof Izika, 1960, Not. 7, p. 2CO,, 64Q5
AVrHOR: NikWskir. A.
ticcraumpol&r Region
T=t _jti~aDix~turban~cevln~ ~the A~raa'~'
PERIODICALt V ab.t Probl. Severa., No. 1, Mostow, AN SM, 1958, pp. 116-132
I A large number of observations showed that the m&xixrim nightly
magnietic disturbances at MI. stations of the globe occur at. thA jfc&1 m."dniet
(-t 2 hours). The nightly magnetic disturbances In tht- zone or IL-1-m- ftur'aft'~ -~Y
are mout Intense. The Instants of occurrence of trkming ani d&'.'.y m,"Ima of
the magnetic activity vary for the vario-us stations in wide limttt; theroforo,
the dvaignatims "morning" and "daily," are conditional. Analyzing- the feat-are-,
of the geographic distribution of a.^ magnetic d1sturbances In. the
region allowed also the conclusion that a second Internal z7,ne of enhar,~:C-J.
Intensity of magnetic disturbances must exist In addition to the zone earlier
Card 1/2

~ , -T lr~' ~ T r: ~' 1 ,
- . _--.i f f -, r~~
"On the problem of diurnal distribution of Irregular =ar-.netic disturbances In
high latitudes."
report presented at the Intl. Association of Geomagncti= and Acroncmyp Sym2oslu= an
Rapid Ge(xmgnetic Variations, Utrecht, Ketherlarids, 1-4 Sep 59-

lr]XOLCSKrr, L.P.
Kurnal, dletrIbutloa of active pwieds of maCastle disturbances
to high latitudes. Vftv.-Iomoef. "an. no.1:7-11 159.
(KIPA 13: 1)
(Mcnetic starms)

- 111MLIOUT, A.P.
NotMd of ca"arlog mgmtIc disturbances In the Arctic avA the
Antarctic. VAgn.-Ionoof. vfmu. no-1930-33 '59. (KllA 13:1)
(Arctic rogloss-Nagootlew, Terrestrial)
(Antarctic roglose-Yagootlem# TemstrIal)

3 (6)
AUTIORS 51kWokly, A. P. SOT/20-127-1-2t/65
TITLZ: solar Protons an the Cause of Katinal- and Nocturnal Wagneti:
Perturbations In High Latitude* (Solnechnne protony kak
prichina, utrannikh i nochnykh magnitnykh votauahcheMy Y
wyeakikh shlrot&kh)
PZRIODICAL: Doklady Akadeall nauk SSSRq 1957, Vol t2T, Sr 1, py 82 - 85
(USSR)
ABSTRACT: As a result of the Investigations carried out in antarctic re-
gion* from 1938 to 1948, the author discovered now facts and
]on for these phenoments and he also undertook several attempts
at explaining their nature. Because of the extended knowle4ge
now available concerning magnetic perturbations In high latitu-
des, eons of the conclusions arrived at at that time as well as
none of the explanations given Kunt now be revised from a now
point of view. The author first given a report on his earlier
assumptions* Later investigations, vhich were based on a volu-
&Inoue observation material and on a large number of stations,
permitted now conclusions to be drawn with respect to the na-
ture of magnetic perturbations in high latitudes. It was shown
Card 1/4 in this connection that the isochronons curves of the matin,61

Solar Protons as the Cause of Katinal- and Nocturnal 507/20-12T-1-21/65
Xagnetic Perturbations in High Latitudes
maximum of xagne,tio perturbation# consist of spirals emerrinr,
from the pole of hamaCensous mxCnet1z&t1on and rotating
wine. The author believes that the Stoermer particles comin..-
from the sun descend along this spiral. In this case, the za-
tinal perturbations must be caused by protons. At present,
certain experiment$ Lre being carried out with a view of re-
vivIng the Birkeland-Stoormer theory of polar currents and z&C-
netLo phenomenao By the direct observation of the matinal me-
xiaua of magnotto perturbations the author was able to follow
the spirals in the longitudinal direction only over a limited
stretch of the order of 1800. From Stoermer's theory it follow&
for terrestrial conditions that the actual spiral of the des-
cent of protons in arctic regions extends to 3600* AccoMing to
Warner's thooryq the spiral of the descent of charged p&r-
tioles (among then also protons) in arctic regions contains d:p-
seine in which the trajectories of the protons are condensed.
Theo* domains are concentrated for 15; 20; 02 ard 08 o'clock
of local geomagnetic time, and are here described as the do-
main* AOB,C,D. The nocturnal maximum of aagnatic perturbations
Card 2/4 to produced by the sun or the effect* of Stoerwor's zones B

folar Protons " the Cause of Utinal- and Nocturnal SOT/20-127-1-21/65
Magnetic Perturbations Is ligh LaMv4os
and Co If thIs Is correct# both satinal- and the nocturnal sag-
notLe perturbations ore the result of the fact that protons
alone penatrat* into the upper zones of the terrestrisl atmos-
phere* Kowevor, this conclusion is in contradiction to the au-
thor#* ass-mption that matinal- and nocturnal perturbations art
cau:;d by particles of various signs (i.e. by electrons and pro-
ton . Without removing this contradiction, It was not possible
to give a more,oxact interpretation of the observed facts. By
analysis of %h* conclusions artivad. at ott the basis of Stoormers
theorr., it is possible to *11minatt this contradictions Accord-
ine to a formda developed by Statratro the angular distance of
the deviation of the spiral fros, the pole depends *specially
al'so an th* rtloolty of the corpuscle*. With Increasine the or-
Greg* velocity of the protons contained In the proton flux, the
spiral as a whole shifts toward South and Southeast, The shift-
Lae of the nocturnal maximum towards an earlier time of the day
say also be explained by great gtorsep if it In assumed that
also the nocturnal maximum Is due to protons# and that It is
located on the spiral of their descent. further details are men-
CarA 3A tionod. iccording to the result$ obtained by the present paper,

Solar Protons an the Cause of Matinal- and Nocturnal SOr/2c-t2T-1-2t/65
Magnetic Perturbations in E[Igh Latitu4es
It to necessary to take Stoomer's theory Into account to a
considerable extent for the purpose of explaining the origin
of magnetic ptrturbations In high latitudes. There are 2 f1g-
urea anOL 12 references, 6 of which are Soviet.
ASSOCIATION; Arktichankly I antarkticheakly nauchno-Iseledovatollskiy
Inst1tut (&ratio- and kntarotte Scientific Research Institute)
PRESXKTED: February 4. 1959, by 1. V. Shultykin, Academician
SUBMITUD: february 4, 1959
Card 4A

t
5010T. K.K.. otv. red.; K"SINOT, l.f., tacectitotll oty.red.; TRIS&UM's
A.S., xammotitoll oti.red.; AERITASMM. A.P., ied.; &fffflTSlElr.lr.9k..rt469
TORMT. P.5.. red.; DDIaLM. I*Ko, reds; KATJra=o S.T., redo;
KOA02KWICII, Te.Se. rode; MIKOLIKIT, A.P., rele;MATICH, X.O.,
redol MEMBR, G.M., rod.,"Amr.-cre.- redo; OLVICH. &Be*
rod,j MLINSKArA, L.C. red.1sl-vat MOOMM. L-Pov tWo.rodo
[Report on observations completel by the Soviet Antarctic Ex-
pedition In 1957 and 1958] Otchat o nablindenitakho vypolmennykh
govetsket antarktichWwi skspeditelel T 1957 1 1958 mg.
Soveto;.alu ekspeditalla, 1955-1958. Leningrad,
lxd-vo "Karskoi ---nrt," 1960. 39 p (InformteloWl biul-
Istlalo ).C) (KM 13:6)
U.-Iturctic r~)gio:,.i-2mislan exploration)

- HILOWULT, A.F.
A~~Soce of the meam, latonsity of Amcwtic ALcttvtty an latttud*
&&d longitude. Probl.Att.L Astarict. ao-3:a5-9-1 160.
WRA 1) 19)
(ftesettsm, Terrestrial)

,7 A006/A 10 t
Mikollskly. A.P.
TI"M On the problem or the geographical distribution oC aurora polaris
in the Arctic
FTRI~DTCAL: Raterativnyr zhurnal. Georizika, no. 7, 1,061, 34, abatract 70243 (V
ab. "Isaled. polyarn. siyaniy, no. 4", Koscow, AN &~M, 196. 14-
19, English awmary)
7---y7l, On the bas!a of contemporary dat& onthe geographical diatributicn
-,,r au-zra Polaris and magnetic disturbances, the author considers-that neither
'he- Pri~r nor the Veatayn zone can be regarded as fully real, since they were
tooth plotted on the basis of non-equivalent and IncompAtible obanrvation data.
In some high-latitude regions of the northern.hemisphere the Isachasms are plot-
'led by taking into accm-it the appearance of both nocturnal and early aurcra.
(north-eastern Canada and touthern Greenland regions), whereas. for other regiont
(Surazi. only nightfall and nocturnal pclar auroras were taker, Into account,
On the ;adsia of an analysis of observations carried out in the Central Arctic by,
Soviet air expeditions and the drifting stations *fforth PC le"L during 1948
C&r4d 1/2

MOSKM TA; KMTATW, N.A.; IMCLIKff, A.?,,- FRDCNBKOi. K,K.
Developuent of geophysical research in the Aretie during the
past 40 years. Probl. ArIct. i Antarkt. no. 4:97-110 ,6o.,
(KLRk 11:1Z)
(Arctic regions-Osophysical, research.)
i

2 -114 20
3/169/6 1/WO/UOTM7/!V-k
3. IV A0061ALGI
AUMMt Nikol'skly, It.P.
TIM-. On the Iodation of the zone of aurvra polarls in the Antarctle
FMIODICAL: Referativnyy zhurnal. Geefizika, no. 7, 1961, 35, abstract ?(;246
("Inform. bryul. Sov. antarkt. ekspeditall". 1960. no. 24, ~8 - 41) 1fr
MIT; A, review of studtea published by a number of authors who attempt-ed
to deO%rmine the location zones of auroras polaris in the Antarctic, Indicaten
that the Antarctic zons t& probably situated over the soithern geogr&phIcal
p-,Le, i.e. sharply asymmetrically In respect to, the zone of aiiroraa polarls in
~he Arctic. Min a3ymrretry is difficult to explain merely by the difference in
the structure of the magnetic field of the Earth. Such a discrepancy may also
~e t-nlp4ned otherwise, If, contrarily, one starts from. the syn!mtry In the run
of' p~jrorA polv-49 and magnetic disturbance phenomena, causetd by the intmiBlcn CC
solar corpuscles, in the Arctic and Antarctic. Based on an analysle, of' magnetic
disturbances in the Arctic, the author advances the hypothesis that In the cIr-
cumpolar region or the Arctic there, Is a second none, with a raised frequency ani
Intfirsity of magnetic disturbances and auroras polarLs. This assumed second zcjne
Carl 1/2

87767
3/19,9/61/WO/OOZ/021/039
00 V/, /to VO A005^001
Trwalatlon frows ReferatIvayy steurnal, Geof talks. 1961, No. 2, P. 39, # 20281
AUTHORa MIkollskIz, A.P.
Tr=s On the Global Distribution of Magneti-c-lonospheric Disturbances
PMIODICAL% "Tr. Arkt. I Aptarkt. n. -i. in-te, 1960, Vol. 223, pp. 5-20
TEXTs The conclusions earlier obtaineJ by the withor for the Arctlo on tre
helical shape of the Isochrones ot the xorning maximum of mWmtlo disturbances
and on the existence of a seconi circumpolar reglon of enhan:el Int4~r-sity of
magi&4tio disturbances arip verified by Uze study of gecgraphical dI&trIL-,JtIcn of
the w4ming magnetto d1sturbances In the Antarotiv region, It Is concluded cr. the
commmity of regularities tn the arctic and antar.-.1i disturbances and an the
opposite direction of evolution of tne helices - isochmnes of dIsturbance xaxlSwM
Because these hellms, ropresent the projections of trajectories of the solar
corpuseles penetrating into the Earth's attrov;nere, the distribaticn of ancmalcus-
ly high absorption caused also by the solar corpwmclos Is considered for the
corroboration of the obtained map of geographical dAirtribation of magnetic
Cand 1/2

*v n
A005/AOOl
On the Global DIstribution of Vagnotic-lam"pheris DIsturtances
disturbances. A close corne:~ticn is det4cted in tho, na"re of geographical
distribution of the anomalous absorption arA the corning mWet!c disturbances.
The possibility to discussed of the exteniden of the hellces of settling to
rtgions of lower latitudes. It is ocanoludod on a ateow.1sm, genoral for the
ent1ro Earth, of the orIgUmt1or. of magnetle-lonosph*r1c disturbances and aurora.
There are 17 references.
L. Lyakhovs
Translator's notei This is tl*.e full translation of I-.e original Russlan abstract.
C&M 212

89755
S/ 169/6 1/000/0C 2,100 8/039
14/00 A005/A001
Translation from: Referativnyy zhurnal, Geoflzlka, 1961, No. 2, P. 3, # 2G17
AUTHORi Ulkol'skly, A. P.
Tr=e Some Problems in the Methods of Investigation of Magnotlo Disturbance
PERIODICAL: "Tr. Arkt. i Antarkt. n.-I. in-ta% 1960, Vol. 223, PP. 150-171
TMW: The author criticizes the method of studying the magnstio activity
which Is based on the derivation of the averaga, charecteristIcs (tho'SD- and Dst'
variations) of the phenomenon and puts in the forefront the necessity of the study
of IrrWAar variations; he considers the field of the SD- and DWYarlations as
a sumexT field of a great number of Irregular disturbances occurring simultaneous-
ly. The possibility of application of the statistical methods to geophysics I
considered. It is pointed out that It is necessary for statistical averaging :r
g*ophysical data to Investigate, every tbw the problem, whether vasential aspects
of the phenoom an got lost In the averaging process. The applicability of the
mathematical methods, In particular of the harmonical anelysIs, to the investiga-
tIons of the Earth's variable mAign*t1o field In considered. The necessity of
Card 1/2

89755
sl1691611OW1002100039
A005/AOOl
Soto Problems In the Methods of Investigation of Magnetic Disturbances
sah"&tLsLn6 the phenomma, when applying the mathematical analysis, may lead to
the diversion from avrtala essential aspects of the phenomenon. The application
of the hsruculeal analysis to the average statistical variations of geophysical
.lownts Is siqwdlent only when these variations reflect the periodical chaniges
:x1atant In nature, but do not appear as a superposition of irregular processes.
L. 1-yakhova
Translator's notes This Is the rull translation of the original Russian abstract,
Card 212

HUOL'SiUY, A.P.
Possible causes of the irregular sotions of ionization: cloud&
associated with auroras. JJoL,1.AJI ObSE 04 rjo.2041-34-4 6
160. (KIRA 1):9)
1. Arktichaskiy" L antarkticheskiy, inatitut Olaveevnorputt.
Predat%vleao aka&. Y.T.5huleftinyu.
(Auroras) (GIOUIS)

I
'T:KOrs;-, 1 0 A. P.
A
"Oh the 0--ographinal Mstrtb%itlon nf thr- ilmis -)f ljit, Sf)1'Jr CsrTral(~.--Aar
Tmptng-vntiv in the Artic. ((r-2-P2))
re-,,ort anbriittext for the Intl. C,3nf. on Comnic Tltya Fnrth St-Im'; (ITTTAF)
Kyo",3, NI-vin 4-15 S"t. 1961

S/169/62/000/GO6/083/093
3,100 D228/D304
A'j 12".~ 10 11 Nikollskiy, A. P.
'1' LL Position of the second auro.-al zone and thz relation
of morning radiances to magnatic d-laturbances
Referat;vnyy zhurnal, Gcof-'-ika, no. 6, 1962, 24, alb-
stract ~G140 (V ab. Polyarn. Giyaniya 4- avecheniye
noolin. no. 7, 1-14. , AN 1961, 37-42)
The suggestior, that there is a second zone of auroras and
::~aznetic diL;tua-bancea was expressed by the author (RZbGeofiz, no.
4, 1957, 3661) on the grounds oi` the ana3~a-ls of.the course of mag-
natic disturbances at hig.h-latitude stations. In the present art-
...cle the author cites certain data of a number of research workers,
which may serve as fui-ther proof for the possibility that there is
a second zone. 10' references. Z-Abotraoter's note; Complete trana-
lation.1
Card 1/1

s/169 62/JrfvK,6/065/093
3,1910 D304
1)228Y,,~
~A,-,, 1OR: Nikollskiy, A0 P.
of thL. auro-
;;OTQ in A-,CZIC ar~~
-!YY Zhur a!, 'r-62, 2~~, a,5-
jtracT. OGI42 (V BID. Polyarn.
no c hn *nebat rAo* 71
2 "he IGI'so :roble.-, Include%J L~ ";azk of (.Ifj*e-uIn`ng Io-
I A
Lation o,,--~* the zone of -~he maxiMum freoue,rcy a-A intensity of t;;;-
.~oras in An-varctica. it was nreviou3ly noted th;-,-. -,,*:-,e ;%ntarctl-c
auroral zone has ar, Ovident iondenoy to pass through the geoj,-.-a-
phic pole. Such a disposition for ti.,.e auroral zon.) In .r.,!.arctica
differz abruptly from thc: Arctic zone's poai-.--on, whic,. i3 za- pre-
OQnt. known from more exten3ive and rollable data. 'a's
y is explaincd by the actual
cult to re-DgnJze t*.-,.&t. this L-ay-etz-
azy,-=atry or the earth's -nagnetic field. T-1--a difference can be
explained i.; another way if one proceeds fro= the conviction that
C~ard 1/3

3/1 69/62/000YOW/085/093
Gaujez of -.he asymmetry D228/D304
thu mornin6 observations. in other words, the aurora! zone found
lor An-.a~-ctica mzay actually consist of the ac&zent3 oil two zones:
oac I zone, aasociated d'--:h morning radiances, and
ond tinnexr~
4
_Q firs, (normal) zone, associated -ad ances. The d4-3-
poui -. .4 - - A.
,ion of the Antarctic stations dur4nZ; '2e 1GY, like teat for
the stations operating there previousli.4, was evidently such that
thu effect of the existence of two different zones for morning and
ni~,;I-At radiances was displayed espocially atrongly. Z_,kbatracterls
note: Complato txanslation.,7
Card 3/3

6/169/62/000/004/060/103
D228/D3O2
AUTHOR: Nikollskiy, A.P.
TITLE: 30 years of work at the polar magnetic station In
Tikhaya Bay
PERIODICALs Referativnyy zhurnal. Geofizika, no. 4. 1962t i0
abstract 4G1 (V ab. Probl. Arktiki I Antarktikio no. 9
Lot Norsk. transportv 1961, 104)
TTEXTt The magnetic station In Tikheya Bay was orpnize4 In 1931 in
connexion with the 2nd International Polar Year* observations were
made continuously to 1958. when the observatory was moved 75 km
north-eastwards to Kheys Island. The results of the observations of
ttie Tikhaya-Kheysa magnetic observatory have served as material for
a large number of scientific investigations. At present t4e Kheys
Island observatory is a complex sophysical observatory- LAbstraa-
tor's notes Complete translatlo4-
card 1/1 *

Daily variation of magnetic disturbances at the Coomagnetic pole in
Antarctica. Geomar. I aer. I no.3:781-785 S-0 461. (KIRA 15:1)
16 Arkticheskty L antarktichookiy nauchno-issledovatollitkiy Institut.
(Antarctic reFions--K&V*tIsx, Terreetrial)
(Arctic regions-Mognetism, Terrestrial)

NML-ISUYF A.P.
"m entrollitW roIe of georagmtic tim in, tht developmut of
jp- tLe distrubanoes. GeowCe L &oral n*.6t955-9,59 " (61.
(KDtL 15t2)
L Arktiahddtiy I antarktlehookiy nauetWo-ImIsdovatol'skly
ImUtut,
(FAcmetim,, Tsr"Strw)

vilm'sKilt A.P.
------------------------
-41- symomw for the exIstonce of a sooond m - -1 f atic
dijtwban"s in tho matern Iretle. Coom . I aorl na.609;-994 "
,61. . (KML 1512)
Is I Afttlabnkly I anUrktIabeekly nsuabna-Lawledomtell skly inatitato
OiOAG reeam-ap-stim, Twmtrua)

IGUTOY,g V.S.; NILIAMv N.A.; NIZOLISKI'r. L.?.
7
R40dto of COMPIW61dal stuftes in the central LVGUO,, FOGU.,
Arkt.1 Antarkt. na,11165-74 162. (MMA 1612)
(Arctic regloss-4kCastlem, Terrestrial)
(Arctic reglaft*-ronospheric redia, vave propagation)

4LL55
41"IMIOC0006101111M I
A160/A1Ol
AUTHORt Rikollxkly, A. F.
T1TL9t A comparison of the m W stia disturbance in high latitude& with
Stgroor's th*or7
PMIODICALt UeomWetiza I. seronomly&, V. 2t no. 6, 1962, 1122, - 1125
TEXTt The author investigate& the data orr the me etie disturbance at the
Chelyuskin. cape, CIT-4 (SP-4) and SP-6 stations, arA compares these data W116i.
St8rmer's theory. It is shown that the average Interval lengthof the Increased
valuos of magnetic disturbance is 6 to 8 hours. The spatis.1-time distribution
of Irregular magnetic disturbances in.the Arctic is satisfactorily explained on
the basis of St8rmer's theory In a number of respects. It was determined that
the most typical. form of & diurnal variation of the magnetic disturbsnce-,in high
latitudes is a curve with three m&ximat a morning, an evening and a night,
maximum. Figure 1, 1 presents dAt& of the Chelyuskin &otation, and Figure 1.0. 2 -
of the SP-6 station,for summer 1957- During this period, the SP-6 station was
almost on the same geomagnetio latitude as the Chelyuskin one, but W east ftom
Card 1A

-A/2-03/62/002/006/012/M
A comparison of the magnetic dIaturtAnce In... Ai6o/Aioi
and the conclusions of Wrmer4a theory prove that It is possible to ute It for
qualitative explanations of some aspects or this phenomenon. Wrmer's theory
should be further developed an the basis of data of the processes In outer spa**,
and the obtained data have to be checked with date oC other similar *Uttong#
There are 3 figures, and I table.
A&SMIATIONs Arkticheekly I antarkticheakly nauchno-lasledovateltaal;! tnetttut
(Arctio uA';Antarctlo Scientific Rizoarch InsUtute)
SUEMTTEDs June 23, 1962
card 3A

RIKOLISKIft A.P.
Starner's tbeory and modern aeronomy. TrwV AM11 Ul no.4i
7-19 162. (WRA 15"8)
(Auroras) (IkgmtAc storms)

RIKOLISKIYO A.F.
cl--,- -
Fossible a-tums of IrroCalar movewnts of Lomixed c1mide, cor-
nectod vith aurorae. Trudy AAKII 241 no.4&29-3& 162.
(MIRA 150)
(Polw rvgione-lonosphers) (Auroras)

MIKOLISKlYt A,P.
Stnietwe or an irr*Cular part or a field or a-qgr*tLe dLsturban4es
on CaW ChelyuAlne TrvAjr AAKIr 241 na.400-98 162.
(HIRA 1599)
(C2p* Challuskin.-YaVietic storma)

h521
8/20 1 - V3/001/013/022
A.UTI[ORt* Hikal 1-k-ix,-A. P. A061YA126
TITU-t Characteristics of the daily distribution of irregular
magnatia disturbances between.the goomagnetic and, geographic
poles in Arctica,
FERIODIGALs Gsomagnatizm. i weronomiya, v. 31 no. 1, 1963, 104 112
TEXTr The data of the drifting stations U-3 (5P-5) and, CrI-7
which were between the geomagnetic and geographic poles during
10 months in 1954 - 1955 and during 7 months in 1958 - 1959, were examined-
The daily course of the magnetic activity, estimated by changes of the
distvrbance vector in the horizontal plane, has four aaxima (9.31 ).91
20.6, and 14.0 hours local time). Fluatuations are + 1.0 hour. The inten-
aIty or the aaxima differs in different months. The good agreement be-
tireen the times at which the four maxima occur and the times at wl~ich the
ahock zones are formed on the precipitation spirals of the Stbruer psr.
ticles (9.01 2.81 20.0, and 15.6 hours) is pointod;out. An smalogy-is
established between the observations described &~d,those made at Alert
btation and at Fort Konger. accordance with C.'Stbrver (The Polar
Card 112

OL'F &sit
Comments on V,K* Klshtn and I.A. ZtruUn's article "Scom problems
of magnetic activity. rart low Goomag. 1 sere 3 no,2070-
373 Kr-AP 163. (KIRA 17t2)
1. Arkticheakly i antarkticheekly nauchno-Iseledavatel'skly
institute

Reality of the diurral pariodietty of mgnetle activity. Gemate
L &sr. 3 no.6rU39-1141 1~-D 163. , (MIRL 1,6 t 12)
I., Arkticheekly, i antarktichaskiy nauchno-issledovat4l'okir
inatitut,

I It 1. 11Y, Q LIt:; K r,1.f. - 1. A.F..
Use of some conclusions of StUrmer's theory for the explanation
of certain regularities of ugnatic disturbances at high
latitudes. Geonag. i car. 4 no.ltl4l-150 Ja-F 164.
(KIU 170)
1. Arktidlieskiy i antarkticheAly nnuchnc-i&ffIodcrv&trVrkIr
inatitut,

ACCESWON NR: AP4041043 5/0120164/000/003/0168/0169
AUTHOR: Nikol'skiy,- A. P,; Kordonskiy. G. A.
TITLE., Effect of the distance between tne x-ray tube and the specimen upon. the
sensitivity of fluorescent x-ray spectrometera
SOURM Pribory* I tekhnika, skaperimenta. no. 3e 1964, 168-169,
1. TOPIC TAGSt spectrometer, x ray spectrometer. fluorescgnt spectrometer
tl:' ABSTRACT: Experiments, on; an optical simulator established that the, distance
between the exit window of a BKhV-G x-ray tube and a 30 x IS.-nun specimen can
I be varied within 10-50 mm. without Impairment to the sensitivity of a fluorescent
spectrometer if the angle of fluorescence collection is varied, correspondingly.
The model was not an exact simulator insofar as the x-ray tube anode radiation is'
anisotropic; however, the results are considered acceptable because the
anisotropy within a small. solid angle is insignificant. Orig. art. has: 2 figures.
~Wd

FM 'EWT I )/FCC/FW~(v i ~F' -A/9.vC( "Pv"/Pt-40/
b AJ:) 4 aq., V,
I Oil M AP4046290
9/0203/64/0000CIS/09(9/39
1MikO11GkqL 'A. P.
vowc n" It 11, WL&m ~~w ~uw~
~atilwiim In t4gli latitedes in the Wastarn and %satern flestophores
~nv~maqntv t I LIN I sier ronont v st , w. no
J A,;& s [tragulat magnocic %I i es t v r i, an ce Itcoetagnetic
a , vi;ilar corpuscular stre a rs t e r r e r I -al acrav"nhe re , cosmic
r i d .4 'F 'r to TI-Wic t --," 0 v- , M a n c-, fj 0~ t i v k t -,-~Qo-m4grif, rl C t too
.'T Thriv maxtirn o f t T T knaviQ ~ 1. c 4 1
4 1 oil cc 21 tn thr
i n t ha a f t e rp non n f j A n ri v v a o n 1,i e t e n t h e
~~i o TI-t 4v u o tv a x in ot
o v a I n i i um a n e t
toIt1i solar rar p uF r a r s~ t r o a t~ o c It penetra t 41 1 n to Ole
k v-,sl at-,roaphere, coif I; p, o t I'le a o a b 'I o r p t 10 n 0 a a m I
-In '1 141 F; 0 p a r o n Q f Aj A c, o m1p A r I & r~ r~ o f tho rates
-j I or gsomagnettt: d I t tl rb ar re a a, loviet. ptationg vith thoso
An 49 4 f t%n gtatioag Ig Vade. SPOC101 de P.On t I an t a as 6 to the Cang-F
a L 3, m Ch u r ch t I w1, a ra t e n a x a a n (I their chanaea are not

I~S IX III AP4046298-
-1 it
Sotivity ot, so nttio
Not", C tbo vis
re
Chill
kilan -from -Chu r #s#!, two
r 41 t. Qof MagottIC actIvIty Vern drn%.rn for nine Pr4tione W!"hin
~;P'MM$-Iottc latitucria bel t fr--1 W fo 1,13' In. t~," Porthern bota-
r,ot, io which an incre-a9c ill P~Czjvit~~ In the ggonaRnetic time in-
ular nagroatlc dim-
-i4l frovi 3 to $ p.m. wgks iletocled, T ~ i n T r, ,,
)iinctin iore allka all over the Arctic ap vben th;i Pt-qtIons oboarve
s r 4! a t i on a 6 t h e % o I a r c o ru a ~. u I a r a t r 6, a m,4 Orig. 4rt. host
o r 1- 11
&1 0 1 -Atktichook I v I r~, ti ! -lid, 4~' ~ w Im-doviv, *I �kLy
f~rctlc and Avt*r-tiv gri-r-tIfIc Rasearch Institute,
TT I,) j O)Feb64 AT D P PU 9 5 PNCLI 00
CODE I AA 190 RE F SO'q 004 0-1 HER 004

A SION XR: AP4036782
6/0M/94/02#/005/"77/"79
AUMCM: Mkollskly, A.P.
TITLEt ~;~;erwu;az` 7a0r"CA'-1'C'Ul&t1MC UA IMOUSIty Of tLUGCOSCM441 excited by
polychromatic x-ray bean ffenort, Seventh Conference an X-Itay Spectroscopy hold in
Yerevan 23 gap to I ant 140-
SOURCZ: AX "MR. lavestiya. tortya fIxIcheskaya, v.24, &*A, 1944, STT-479
TOPIC TAQ9: x-ray excitation, tll;roscence intatral
ABSTRACT: The evaluation.of the "fluorescence Lntscral"
Lq
I. M~ L*('- - '*) (I - C-ACA.*-q e-W-4.
X3 + x
in which thos exponential factors take account of the finite thickness of the sample
and the absorption of the primary bean by the x-ray tube window$ was approximately
reduced to the evaluation of tabulated exponential integraU. go details of the re-
duction am given, emeopt to any that the "quadratic integral approximation" (M. 1.
Demidavich, LA.Marem, Be Z,gbuva lava, ChislawyOre metody* WMILSaMseatcla.M. IN*
was employed. Tke error Is reasonably small (4100 for 9 limm of elements with
CWd 1A

ACCZSSICW Us AP4031BU2
U de Z -c. 60, but the fozuula to not adequate for Ea lines of *tomato with, 60 4 Z 4
A similar approKlastlon to the Integral obtained by dividing the Latogrand by &,&nd
which Is aceoidingly appropriate when the Intensity Is def Land as energy flux rather
than photon flux, Is, however, sufficiently accurst* even for tke heavy o1ments.
When nottiter espaneattal factor aced be constdored, the integral to elosiontary, but
its expression In term of the lagarttka AM the Inverse, tangent Is Involved. For
this case an appnoLustiom I& given based an the theorem of the a"& and the "ousp-
tion that the appropriate meem, is the arLtbmtLe mesa of the Units of integration
(the wavelengths of the Duaw-Kunt limit and the absorption edge respeatLyely)a
Orig.artAsse 11 forowl".
AWOCUT109t TeastraVasla labeestarLys avtomtLki (Central Autonatles Laboratory)
S=MTMI 00
X= 0=4 or
DATX MM Muss"
0 OW ICN& 04
930=0 00
01SUCOM
OW 2.4

z ft~ T- 2
-A --- ---
131
N , AP5027009
A711-10111, X'"Iyukvina, Ye. F. A. P. YCV1FLrr'--- r. YFA.
,~'2,U-,: none
TITEFE: Construction and, techritual PZ ;1QLU-WjALSLa-111t1!r
S, 0 UR F :PrIbory 1. tekhnika ekspe.-itri,nta)~)no. 5, 196.5, 71-73
IOPP'l TAGI; gas discharge counter, proportional ccunter
ABSTRA-,r: A proportional -counter dc,.-AlFried for detecticti, of 1-10-kev x-rad-l'aticri is
dr--vcrlbed. To.jreet the requiront-nt or it lnrg,~,-firf~a irif.iat arerture of rzinir-.un thick-
the*da~aign contalni with tv--~ 10-p Al film Apott-turva 25 x 11; Mi
each. 'To reduce nttenuntlon of fluorec-cent rarliatiem by the vurroimr1ing n1r, The
c-,un-ter itself is placed in it varivAn whiln th~! rcTrain~s,!r ji thr.- unit In siv-11,1,ected to
1 norr-5.1 atnorpheric pressure. Provisiona art, for ccraiccting thr! otAput of the
counter to ocintillation counter. The activ(-, clfm~!rits of the counter are a stai
less Ptenk cylindrical cathode 25 tmi in a tungnter, wire mnode 0.0,'~ =s in.
dl,IM~.t-er, and a gras mixture or 90% Ar and 1Q% whi-h I-, panae-~. through the counter
interior 4tt a rrite of 5-20 c"13/min. Fig. I !ihow:i tht! output piilv,~ lielght tin a func-
tion of the applied potential. The linefir regicri c~~rreBpcnrla to a F.-,Fis avalanche fac-
tf)r rringe or (1.3-1.6) x 1.04. The efficiency of the couriter na a function of wave-
length is Bbown In Fig. 2. The effectiveness of the cciinter in dete-~ting hard rad a-
Card r,

ACC Nib A115027009
tion Is limited by the inadequate attenuating properties of the arFcn e&$; for soft
i
Fig'. 1. Pulse bbight as a
fwiction of applied potential
Fig. 2. Cownter efficiency as a,
function of Wavelength
1 - CrLlculAted; 2 - experimental.
1 - Fi~Kcj; 2. ZnK,
radiatlono it is lir-ited by the thickness of the chthode a-,erture. Most effective
radiation range is 3-4 kev. Orig. a-rt, h": 2 fig-area wnd 4 for=ulas. [BD)
StM CODE: NP/ SUBM DATE: 20Jui6h/ OPIG ',:U-,F: 001/ A47D PRESS: '*_2
Card

ACCESSION.NR: AT5022288 UR/3136/64/0001618/0001/0016
A7111OR: Mishakova, A. P. ; Nikol'skiy, 3. A. 61
TITIX: Paired angular torrelation of secondary particles in c,osmic s
with energy E sub 0 greater than 10 ouper 1~ ev
SOURCE-, Moscow. In9titut_atwmoy_ener&iL. Daklady, IAE-618, 1964. Parnaya
uglot%ya korrelyataiya vtorichnykh ch'astiits v koanicheskikh livnaykti a
en(!rj;iyoy Eo~>10110v, 1-16
TOPIC ThGS: cosmic ray shower, secondary coRmic ray, cosmic ray particle
AV;n, AGIN ExperLnuantal distributions of paired angles between seconciary cosmic
ray particles with energy E. > 1011 ev are compared with calculated distributions
obtatned by essuming the absence oi asyc-termatic angular correlation of shower i
parttcle.s. A good agreement betwcotn the calculated and experimental dL*trLbu-
tiryns is observed. The results obtcined are analyzed from the standpoint of
the erUstence of unstable shower particles which decay ~'nto particleA of short
lifetime, "In conclusion, the authors express their appreciation to Prof. I.J2
GuTevich for numerous dLscussions and for re,ilewing the results." Orig. art.
hast 7 figures and 9 formulas.
Card 1/2

4 tl 1. e - Ar
Ju- I-U"tvmw
ACC-011110-MARt- -AISO222"
ASSOCEMON: mme
SUMUTUED: 00 FNCL: 00 s uB onE AAj NP
.10 REF SOVi 002 6MER: 003

L Lt~,,77-66 W7(1)/Fq/XWA(h) GW
ACC AP
6oo6669 MM", V, UR/0203/66/006/001/0140/0141.~
AVY11OR: Mikollskiy, A. F.
ORG: Arctic and Antarctic Scientific Research Institute (Arkticheskil I antA_
1ticheskiy nauchno-lealedovatellskiy InGtitut
7'171,E: Correlation between magnetic activity and disturbances in the ionoopheric
F2 layer
1-1-01MCF.- Geomagnetizm I aeronomila. Y. 6. no. 1, 1966, 14o-lhl
Topic TAGs- ionospheric disturbance, magnetic perturbation, forbidden period,
geotmSnetic time
J
ABSTRACT: In order to compare Ionospheric disturbances vith magn!!qc perturb&-
tions, both phenomena were studied simultaneously uning dalva obtained over mny i
ears. Peaks in magnetic perturb,-.tions at varioun hours of the day vere taken
y
from Chelyuskin, Dikson, Tikni, and Uelen (Welen) stntions. The appearance
of geomagnetic peaks Occurs very seldom between o8oo and 1400 hr local geomag-
netic time. This tire interval in considered to le the forbidden period. Ion-
ospheric perturbations In the F2 layer coincide with the forbidden period and
'-Card UDC: 550.388-2:550-385 J

L 15777-66
ACC HR: Ar6oo6669
have a negative sign, Yorbidden periods increase an the station latitude de-
creases. The length of the forbidden-period in -Aikai and Welen is from 07D0 to
1500 hr local geomagnetic time. The duration of the fcorbidden period at
Chelyuskin is about 4 hr., 001g..art. has: I figixre~ (EGI
SUB CODE: 04/ SM DATEt. C)4jan65/ ORIG RM 003/ ATD MSS: b 0
L Card_ 2/2

or D
t
-PL 21j~ ~78-~66
A] SOURCE CODE: uP,/Oi8i/66/c03/0014/l203/l2jL,
'AUTHOR.t Nikoll skiy, A. P. /,3
scow no e o ee oya (Moskovskiy Institut stall 16
splavov)
le,
TITLE: The mechanism of electric conductivity of ferrites
SOURCE: Fizika tverdogo tela, v. 8. no. 4, 1966# 1208-1211
TOPIC TAGS: ferrite, electric conductivity, x ray spectrum, spectral
line, line broadening, crystal lattice structure, line splitting
~
ABSTRACT: The author has made a simultaneous study of the electric con-
ductivity of ferrites of the system k-O-Al203-Fe203 and of the x ray
lines of FeK 135 (3d-O 19) characterizing the energy spectrum of the 3d
electrons. The tests were made witn eight samples or different relative
compositions and resistivitles. The results show that on g,.)Ing from the
Isample with the minimum resistivity to that with the highent resistivity
the x-ray lines broaden In the vicinity mC the peak and kinks appear In
Ithe contours, corresponding to splitting of the central peak. It Is
'concluded from an interpretation of the teat results that the 3d elec-

ACC NA& AP60!2486
2+ 3+ 01?
trons can execute jumps between the iona Fe and Fe wh1ch are located
in nonequivalent points of the lattice. 7hiG becomes possible as a re-
i
sult of the approach of the coaponents of the splitting of the levels of
3d electrons In the tetrahedral and octahedral sites by the crystal
field. A similar behavior of the FeK 135 lines and the electric resistiv-
ity is observed in the ZnAA.204-NIFe2 04ferrimagnetic system. The author
thanks S. S. Gorelik for help with the work and a discussion Of the
results,, M GO-777hevakin for supplying the magnestum-aluminate ferrW
,samples. Orig. art. has: 3 figures and 2 tables.
CODE: 20/ SM3M DATE: llMaV65/ ORIG REF: 002/ OTH REP: 001

AT7003562 -SOURCE. OODE: UR13116j66[28Gj0-00,-j0GT6j008S
AUTHOR: N1k*VsLdL, A. P.
%MMM
ORG: none
TITLE: Time-space distribution of anomalous absorption in the ionosphere
SOURCE: Leningrad. Arkticheekly 1, artarkticheekly nauchno-iseledovatel'skly
Institut, Trudy, v. 2W, 1966. Iseledovanlya magnitno-ionoefernykh vatmushcht-
niy I rasprostranoniya radiovoln v Arktike L Ardarkilke (Studies of magnetic and
Ionospheric disturbances and radio wave propagation in the Arctic and Antarcticl,
76-95
TOPIC TAGS: tonospheric absorption, Ionosphere, anomalous absorption,
absorptton distribution/Soviet Arctic
ABSTRACT: Time-space distribution of anomalous absorption in the Ionosphere (a
deter ined on Ow basis of observations made during the winter 196311994 by the
network of rheametria stations Weatod in the Soviet Arctic. The following conclu-
alone are reached: 1) a tendency of an Increase In the occurrence of maximal
absorption values was observed at about 4. 10-12. IT. 19 and 24 hre CMT;

-~;'ACC
"'4 AT7003582
2) at higher latitude stations (up to Ad 7 r) the relative weight of cases with
maximum absorption In the 8-44 hr Interval Is higher than at tonal stations;
3) the distribution of Increases in the daily occurrence of maximal absorption is In.
good agreement with th.* daily distribution of the posics of magnetic disturbance.
Orig. art. has: 6 ttguros and L tablt. (DWI
SUB CODE: 041
212

NIKOLIMTO A.P.; KORDWSrrr, G-A-
EXfoct, of the distance between an X-my tube and t~a specimn
under study w the sensitivity of fluorescent X-ray spectro-
meters. Pribe i to", eksp. 9 no.3&168-169 tfj~j t64
(HIRA 18cl)
.10 73mtral'taya laboratorlys aytomatikle

A,. F.
Goologricat structure arvI n1rarxis In t!ia- eaaVar,, pirt ci~ t~.!! Chkl,~.Ask
Panimula.
Trudy Arkt lust Val. 104, 1938
30% Trudy Arktichookogo Hanchno-Tsaladovatal'skogo
Institah, GUMP, Council of Ministars. Vol. 201,
1948

'I 'T v -F
IL AA
At
I a F
AmweGad. two, WOR
ow wameaff 14. 4-04-v
kca"m tbp fewive recur ad, f6a'a"', OW The (T.4"CON
mmme me el 'tin-owd. Owmeq."
Soo
6 OtACLOW-K UNWOM CLIAW .106
r T T
0 00
0 0 0 0 0 0
1
see
x00
Soo
wee
goo
411010
so*
@G0
too
lf.all 49 0.0 Ito
a
0000 as *9 0,0*000 to 0
0 o * 0 0 0 0 0 0 0 0 o o o 0 0 0
fail!

I ~ . -K -I , : . T,r
.L. zj IIjL "I.IL, ~. V
2. OW)
4. Wolframit-e Group - Altai Lountains
7. 1. Gramitoids or the Altai and Falbin; 2. !~AnoraloFy 1.-)f tlhe wolfra7-,ite off the
Altai and Kalbin.; 3. T-Aes of walfra-ite deposits of tLe Altai ivil K,.'111,in.
(Abstract). hv. Glav. Lq--r. geOl. fon. . no. 2. P/1147-
9. YonthIZ List of guisslan Acceqnlon2, Library of ~;onj,.revs, 1-tirch 11y53. Unclassified.

UKOLISErfli.p.
us= (600)
C-solo(Tostnt'grop ble-64ock'"; Gooloa- ukrolm
Stratign?* of the KAMI Itoc rocim. V*U. AN SM 92 no, 6J952. I
Mudmo- saUdavatollskly, G"logichaskii rmtitut. rod. 17 '/ea. I95L'
SOs VUVQ JLAO of IMS" Ag=ASMUbmry of Cvucrdn, My 1952. Unal.

SIKOLISKIT, A. -7.
Petrology - Altai Kouztmins
Nag= of *mall tntntnione of the Altai. I&v, AN SSSR. Ser. geol. No. 2, 052
Monthly List of kv slan Accercians. tatbrary of Confrovto. J~Lly 1952. UXMA~ SIFIFD*

NIKOLISKIT, A.P.
I-ftft rmwww"ft-w
tale schists wA serpentines of tbel northem psrt~ of the SaksapmIc gone of
trevoroaWya. IST*st. Akad. Uuk S.S.S.R., Ser. Geol. '5Z, X*-3, 130-5.
(CA 47 no.M12155 t53) (NIMA 6tO

1. EXMISKITt A. P.
2. usm (6oo)
4. Rocks,, rpsous - LIUL Hountains
7. Conoerning the artiale ON94p& of small intrusions of the Lltat.0 A. P. KikolOskiy-.
Reviewed bT G. M. Shcherba. Ity, 0 SSSR. Ser. geol, go. 2, 1953.
9. Month List of Russian Accessions, Library of Congress, APrI1 - 1953, Uncl.

ur,"3/ c4olojW Boa review
Car'l I/X Pub 46 10/24
Av Vic ra Nlkoltdkly. A. P.

Title I Blamed criticism
Nr1WiOO1 'I Izir, AN &SSR. Ser. geol. 129-134, Nov-Dlec 1954
Abotrict I Rebuttal Is give-n to the criticism of a report vritten by tiie AU
on the subject of, Me Geology ct the KriToy Rog RegionsO El*von
V.~M references (1939-19.54)o
In5titution t ....*
sutnni t ted % June 8# 19.54

mikol I skii I a article* on %be ooloar of' IrIver log. low.
~. ver.pox. 19 w.2.-152-136 Mr-Ap 154. (XW ?t?)
(KrivW&V Oseleff) (ftkollskii, A.?.)

-KkY 1~
A.P1.51kallskiits viewv ort the, stratigraphy &aA structure of
Pr*-C"Irian rocks of Krivar tog. rsy.AIF SM. Iler.pol. 19 w.2:
156-161 Or-Ap 154. (=A 7t7)
(Kriver lot-4001offe stratigraphid) (Gooloff, Stratigeaphia-
KrlvW log) (likoltekit. A.?.)
9

IMLIKIr, A.F.
f-~
S~ pmusm or
99-106 1550
vw arigto of bltratherod dopwlta. ftv. I ao,10:
( --Rh- detry) r" 8: 9)

^%- JM~W AeP*
-1111, ft~.
fin aselato 04P at - ad slammle et WAratm mod Ww AlUl
dateralsod by Ow wam "time mfted sompared with opwtfte
polealad speolmme Isfaw ober. V~ w.Ift?O--76 '56.
(vlm%ts*-jml4&r6w "stno (an lotk)
(Allat 16matates-&dUarew "ties)

15-57-6-11216
Translation from: Referativny zhurnal, Geologiya, 1957, Nr 8.
p 151 (USSRT
AUTHOR: Mikol'skiy, A. P.
TITLE: --rie-E-s~somaZ'ites, of the Iron-Bearing Quartzites of the
Eastern Part of the Ukrainian Crystalline Shield and
the Origin of Rich Iron Ores (Vietasomatity thelezistylb
kvartsitov vostochnoy chasti Ukrainskogo kristalliches-
kogo shchita i voprosy genezi9a bogatykh thelenznykh
rud)
PERIODICAL: Sov. geologiya, 1956, sb. Nr 50, pp 28-53
ABSTRACT: The author gives a description of the metasomatic
processes developed in the strata of the iron-bearing
quartzites of the eastern part of the Ukrainian
crystalline shield. He presents the most intensively
developed phases of replacement as follows: 1) for-
Card 1/3 mation of iron ores of the magnetite type of the

15-57-8-11216
Metasomatites of the Iron-Bearing Quartzites (Cont.)
was converted into martite. The formation of the massive magnetite
ores of the Korsak-Mogila was connected with the granitization of
the magnetite quartzites, accompanied by the loss of considerable
amounts of Fe. 1nCqn_*&iVe riebeckitization and replacement of the
cummingtonite by rhodualte freed for migration considerable masses
of Fe. In sections with an extensive development of amphibole-
magnetite schists, quartz and amphibole were replaced by Fe, which
led to the origination of rich amphlbole-magnetite ores. The
processes of carbonate replacement were also often accompanied by
the formation of rich ores; this was possible In connection with
albitization and quartzification. The author associates sodium
replacement among the iron-bearing quartzites of the shield with
the formation of aplitic granites and migmatites of the late Pre-
cambrian period.
Card 3/3 1. V. Kunayev

SIKOLISKIY; A.P.
. Genoste of granitaids Im the eastern part of the Ukrulnian
Crystalline Sbield. Worm.abor. UOLVEI n0.22:93-70 C59.
(Dat"r Va2loy, -Rocke) (IUM 24,12)

NJULIBUT, A.P.,, YXLPIHOY,, TM,13rfV, N.A., r_-_,_-hnr7 rel.f rMilliOll,
t
Olkmlogia and "tallocanic 4tudr of tba O"tftn wt of the Oxainfan
cmystall1w. shiel4l "*logo-=* W Ilognicn4ekit ocharkrawtochrat
ch"ti Ukrainskogo shchita. to-ningrad, 1960. 163. (leninved.
Tassoiusari geolo&icheskli inatitut. bmdr. vol.,n).
(XDA' 13:11)
(Daleper Tallep-4tologr, Sammie)

UUAKW. N.A. C.- NINDLISIM, A.P. -
Obt"onatit" Is Fr*4mbrian Iron quartzites of the Ukralme Uste
ZW 15 woZ4tl?'-Z7 f6O,e OWMA 13cul
(Ukr&tm&--C*l&rtxit*)
(9kralme-jutmaouktite)

~-rk idemik'
Clawnyy Ye.t-'%., red.itd.va; IOf~'~,EVER, tei+.-I.red.
[Yetasomatites of the rrivoy Rap are teltl Netascommatity Lrivora?~.r~ ji-O
rudnoro poissa. Moskva, IrAi-vo Alcad.nauk SSSR, 1961. 204 p.
(A-ademlia nauk SSSR. LaLoratoriia reolorli dokerbrlia. Trudy,
n0.13). (PURA 1.11:1)
1. Chlen-korrespondent AN SSSR (for Yeliseyev).
(Krivoy RoF Basi,,-Ketasomitite)

ISP IT .4 o i .
-- ~- - ~
Met.,Lmor %= , L' Ih to 1; FV~ - Jr ; r, - ,., . -,,, , i - ~ r. ',- a L -,,11, h. e 4
-pnrt of -re A%te.)f-T- r!- .. .*~: ', t - - ", f. c 1 0 k1'; ~~ t": . r. 0 0 19 t
'"ILPA 1'7:0,)
91-100 1(,,.

TIrMfIKTVV' ff.; LUC=, K.T., redmiad-va; MKIN, T,41-v t*kba-'*do
dopmw~-- -
[~Vowtlt of the wtiosal sessaw of the Naple's IMPOUG Of
ftiderta; statistical date Isavitto marodnogs, 160swet'ra
mrsdael respabliki 20141MAL; statlattabiedde, pdtagatelte
4ekwe, TvAsktwegiadat, L"So 231 Pe (IUU NO
(ftlarts-Statisties)

HATKIE7, To.; 111KOLIOX - ranaiator)- PAWK~-XV, V.F.[tr,-n.,v1atorjT
U,A.S, (t
V XANIN, V.I. [trarm-lator]; SAVU11YOOV, V.I' -(tra lAtor) I FU -
ZI8V G.R.(ftwalat=j; IrMANOY,, S.H.Ctrous. mrh VI ITSVILIT.,
red,,; OLIMIC3, Tu,Ta,p red.; PRIVARTUrAp tookhae red@
[Labor productivity and tbereproduction of tba, weans, cf produc-
tion under sociLlim] Proisvoditel'Doet"truft i vospecizvodstyo
pri, sotsialism. Pod rede A.I.VikentleTa. Prodisl. V.S.Reachinm.
Moskva, led-To inoatre lit-ryjf 196L, 269, pe (KIRL 14tJO)
opw4vuL U; farodnoy Rospubliki Bollaril (for Kateyev).
":r productivity) Zoonomi4e)
i;b
(

D I zes a rt,.-Alon "InvastleAL(I-ri (sf i r f
Quality in the Cnna of Fialch Grtnding tha
P-ardened ~Aael with bound ALrrisiv..ic."
25/4/5',)
honcow taitorachnnivil Inst.
SO Vechirviva Moskvi
Sum 71

111KOw"Irt A.T.
.....
Charactortatice of surfmae layers of teaverat at"t subjoetet to
grIMIag and haalaC. Trudy fte. pe tach. pewarbb. me.tt69-79 On.
(Reel) (Grtuding and polishing) (=A loss)

VIZOWKIT, A,V.
Implallou of tko preades of lapplog wlth wtbretim barc TrMy
$mop* ka4hop"Orkho U094tZ36-21s) 0590 (YUA 13:6)
(OrtadinC and pollstdog)

V-
wr/3916
GMk Kad"lls pe tommugn
mmainaftroyealys
Oswvla7% -are" TymakayraixToditellaago ShIf y"aus (sulls P*16100 JA
216-p"ftativity ftladim) Ogamp MAWX, 1960- P- 3,=C
sopus PrIat".
NL (MIS pw): ye. IT. OLS20WO Doctor at TMARUNI selft"WO Ptwwmmr;
W. (b&ldi* book): A. T. P"Ovp UWIWW; T*W6 Not To go IMIkla;
SuRgIn Nd. for Uteratuxe = VOT md mutrummt OommuWtum
(mews): V. V. 1zhavi"tlys amcinver.
I TkU book Is lmt4ndG4 for teeboloal persamel la ggUl grISdIft,
cwf~: SIN WIJACUOU Of SrUelfit da&U vith "J~ of *Melftt
grludlM e nrt&Uj, the tbeary of grindlft,, t1w mdwolm OC Mw ftt%ift
actIft of zml- p ablp faustlamp "d tbg qffoct or owtgft f&Mm 4a
uw fraftativiv of UN PlAdim proosse. amb"is is a"* giv" to UO
aft4matlom of the grindLeg yx ooess. A m mA i v of utlel" 6"I Vith ma
pladla of asAides md titealm 41a". go pw"mUtj" ~" =MUM".
Wex4maes f*LUm "eh artleu.
Card 1/6

Nola rr*lamw (amt.)
TWX W dwv~f
From ths SdItar
*002jewo Y*, N, [Doe-Ar of TOCIMICal 641ROMSO Prafasawle Machadmis of
the C%ttIng Actiou of Ahras!Te Grains In ariadfM
%~ author dt&=x*t* arreagmmauts spacing, d1smulanx# m4 geowtry
of abrasive min . ?he tb*M of Via as of ddp formaUen med
the thlakmass of the IQw nma"A by a single grain we &I" dU4a~d*C
Formo 9, A, (Owadidate of Tachn-4aal Balances]. AmmUsle of TMn at go
Yana loc. in Omwactiin With tbia (kametry of U4 GrIndlag-lboal ftrftse 30
Molls A V, [Caadldate of fechaleal SCIMOSS). Wfect Of TWIMN
-tz!~--M,:rOftzCa4tiylty In Qr1ladrIftl Orladift
So wMw descrDne a mw&Jiod for deUrulaing oAl~ feedft ratep
=It p-osew betv"n vart sad ifteIg aad the akittlag dayth of elmle
gralas zwoessary far the maximas ittillcatlan of griudbg a6w1s,
TWwers V. S. (VaNm#,J. trfeet. of Un Onamtry of an Abraelve Waft
OR ir"yo-wisles of th* Grinding VbA*1
aar4 216

awle ft*lem
9",15918
So authev d1smades tite m2atImildpa botmem this r*All of an webwe
md, the suglas of peaks rAd vaLlso of ebmive gralag, aft"
dmlm In two yrojectlous by sums of am VIA dravlog oppwabw
built We tba wyatm of an ordinary blOACICAl 214MOOP. YAVd-
Motion of the w1crageops was adjasw to the grit alme
Imllysp 4. D, Iftvtosear]. 21w rmwy of aw Waddzg OpU in 4naftjmL
&1&4189 as a Sol* or 110-proftativIty lbehinq
1*0 ar'.1c2o In a wtu4 of the grlndlng opKmtl= and its ragm2witles.
AwlQ9 the tAdes dlx4umsd am offset of pecoveslag factme an the
VISMY Of StlAdUg'v ChOON 10 GWttlAig actlomof a griedift &~*2.
0"r tM 'bowl 11f6 NA *almg everstlous ~d the offect at i6mal
an pmftctlv:Ety.
=wlx=lrwj, To. a. ft-it21plas of ligh-ptaftetivity a-Luduw ad rts
Awtowtlom
SW 4evLeA USIA with tlw prInelplas of p2malme h3gh-preftativity
grIA4189 ona the Lw.=Pox%tl4u of a system of mt4matlam Into CrIodL*g
GPOVOtIftwe Noth vabjeets a--* dlxmx4w4 In, aamactlom vith the r4l-
dael.lam of cmtting t!jmp the SCUWVmmnt of gs gt"jUty,, uA tko
Card 3/6