SCIENTIFIC ABSTRACT N. DENISOV - N.M. DENISOV

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SCIENTIFIC ABSTRACT
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DEITISOV, N. A man can do anything. Grazhd. av. 18 no.6:24-25 Je 161. (MIRA 14:7) (Air pilots) DEKISOV, IT., pollovnik IIA,om SU.1ing-rad to J13erl1n;n three hundred battle pictvi-es lo.,, IAkov Rim~m. Reviewed 1~-.y N. Denisov. Sov. foto 21 io. 12:214 F 161. -14:2) Oforld WF-r, 193S'-1945--Photography) (Riwnin, Wcov) DENISOV, N. Improtant seconds. Kryl.rod. 12 no.10:6-8 0 161. (MIRA 15:2) (Air Pilots) (Aeronautics--Competions) AVMN= IMs AIGODU91 B/C-01 00/la/OD03/0()03 2/63/0 M?Mt Bormzb)s go srA AnAmw if %out r4ouc"I c I m I Wbw# WlOvcidz-,, OMMI PAWIfts 15 am 63s, 3. colo 1-b =20 no: omosa ic or v, WLovoay =Mt It I* amt,UWA that V, ArkovskV, vu at the. *~wwdxmm durinc, the Inumchus of vosto)m 1., 2$ ')A 40 0* sbcowliclal of coummitics 10 ~,Z; var.,60S omm 111n): am ammoom w The Mum* Rev OUZ wa"N~ on "Vm lwz betwo t1m n-WIS or tho vowto%*3 wmk IWU*4,p the Chief' Dmionm LOS the Vfttok Aputabkpi w* the 4048M 40 QMlwnwt1cv*.,,,* jiuv in vkuru Vgkonku, So anal^Lml mink an I=XbWAM lo amemlizaticn& and the amickly ebiUiW to oBlm the riot amisim In caplex altwtims." Card ACMUMM" jilymm mw this SWI I*Ud" 3016UMOW In-OMMAUM Vith tbd VMbokbS Mot# tho mimmum no thl) tolm !~W! mol m 1''d ftbmbmkr ingbad of tho tam WkWftj 14MMMIA Taly IlkaWn W the Omni WA detwbmat ommmim, ft*MrJMY*llO tSIA23PAUrb 1111 AUM modiftlW6 komdlq~ to Stmembo ona Dontoovp be ymms ion vitit elW qMj he In qxlet aml In daUbento in his A PM.ift VC UAS lonobi MOR SAPUlmot aboM in q***&bAp OSSIM31 we w0migoods Ila wthas staus "asoNow betas hw ftlo= =*- %V vith snob ImOoks " IM* Sat tV SWA iNcImUM to Te Fo JVkMM%3,7* IQV Vo lXfttl= Ilt than tUk% 08 Gft~un co=WpU cC Us ftvolqpM ct opw Um*laolW SM99vog V* abo urA dvv*U;W*4 the U11111k Me At um AM! IMM63 Card 1/2 DENISOVI N. I I - - -1 v- ~~t, The main formla. Izobr. i rats. no.1-106 163. (MIRA 36:12) 1, Direktor aukonnoy fabriki. "Krasnyy Oktyabrl", Surok, Penzenskoy obl, ZHOMOV, Yu.. (UA3FG); DENISOV, N. (UA3XN) Short and ultrashort radio waves. Radio no.liV Ja 165. (MIRA 18W Ju I N.A. KRILICHEMlY, M., redakbor; ZMNMSO-V -N A , redaktor; YBMOV, P.R., redai-tor; TROFINOT. redaktor. [Progrossive practice of buildtore in the oil industry; materials of a conference of innovators of the Main Western Petrole Construction trast] Peirsdavoi typyt neft ianikov-atroit ale i; me- terialy soveshchanila novatorov glavzapadneftestroia. Hoskva, Gos. nainchno-takhn. Izd-vo neftianoi i gorno-toplivnoi lit-ry, 1952. 61 p. (HLRA 7:8) 1. Randia (1923- U.S.S.R.) Ministerstro neftyanoy promysh- lennosti. (Builcling) (Petroleum industry) DENISOV, N. A. N15 735-591 Uchet i analdz proizvoditellnosti truds i zarabotnoy p1tty v stroitell- D3 stve neftyanoy prorqyshlennosti, (Calculation And Analysis Of The Operating Efficiency And Wages In The, Building: Up Of The Petroleum. Industr7, By) N. A. Den15-v1w i A. P. Chebotayev. Vloskva, Gostoptekhizdat, 1952. 128 p. tables. DINISOV, N. lwwwoft, - a Fulfillment of output norms and the productivity of labor. Sots.trud no.6:121-122 Je 157. MRA 10:7) 1. Rachallnik otdola truda i sarplaty Glavtaentroneftestroya. (Construction industry--Production standards) RUMYANOV, Mikhail VaBillyerich; DAUSOV,H.A., inzhener, redaktor; KRYUfJXR,Tu.V., redaktor; YM~VFI'r.8.*'~'~lrekhaicheakiy redaktor [Complex mechanization of painting work] Opyt kompleksnoi makhanizataii maliarnvkh rabot. Moskva, Goo.izd-vo lit-ry po stroitel'stvu i arkhitekture, 1955. 49 p. (KIRA 9:3) (Faint machinery) DENISOV, N.A 1. (Hosk-7a) Piecework payment system for construction workman. Stroi.pred. neft.prom.1 no-3:26-27 My 156. (MTAA 9:9) (Pleicework) (Construotion worl"ers) Ae~-7111'150 ~/, 41/" /)~ DIUN IS OV -- IVANCHUKOV, A.F., nauchvy red.; KRYUGIM, Yu.Y., red.izd-va; ""10ROM7, E.K., tekhn.red. [Organizing the training of workers in the construction industry] Organizatelia obucheniia rabochikh na Aroike. Mosima, Goe.izd-vo lit-ry po stroit.i arkhit.. 1957. 27 P. (MIRA 11:1) (Building trades-Study and teaching) C-2. Y" Z' C\ -C 'o DINISOV, Ilikoloy AleksandxgkIL; VOVZEWAK, P.N., nauchuyy red. IMYLIGAR, luoy's, ~44-orz'Mvc;-, BLIXIA. S.M., takhn. red. [Ilxporience in organi Ing mixed brigades] Opyt organizataii kom- plak-onykh brigad., Ko:kva, Gos.izcl-vo lit-ry po strolt i arkhIt., 1957~, 58 P* WHA 11:2) (Construction industry) DINISOV, N.G. Anaver to P.I.Kuznet,sovla letter concerning X.G.Deninov's article. Zhur.eksp. i teor.fiz. 24 no-3:368 My '53. (W-RA 7:10) (Kuznetsov, P.I.) UsSR/Physics waves in ionsphere FD-2980 Card 1/1 Pub. 146 - 21/28 Author Denisov, N. G. Title In-t"(rra!cmt"i"o"n"oroowr'dinary and extraordinary waves in the ionosphere and the magnification effect of reflected signals Periodical Zhur. eksp. i teor. fiz., 29, September 1955, 380-381 Abstract The electromagnetic field of a wave propagated in an inhomogene- ous magnetoactive medium (ionosphere) generally cannot be repre- sented in the form of a superposition of independent extraordinary and ordinary waves; taking into account of the inhomogeneity of the medium leads to the fact that in the propagation of waves of one type in the medium waves of the other type arise, this inter- action existing in the entire expanse of the inhomogeneous medium (however, under the conditions of the io~,.-sphere, a slowly varying medium., noticeable interaction occurs nLy in bounded regions, out, side of which it is extremely small). Only under conditions of small interaction can one talk about the separation of a field in- to ordinary and extraordinary waves. In connection the present writer obtains an expression for the coefficient of reflection for normal incidence. He thanks V. L. Ginzlburg for posing the theme and for his assistance. Four references: e.g. Ya. L. Al'pert, V. L. Ginzburg, Ye. L. Feynberg, Rasprostvraneniye radiovoln [Prop- agation of radio waves], Moscow, 1953; B. N. Gershman, Sbornik pamyati Andronciva, 1955. Institution Gor'kiy State University nn 'Inr_r_ USSR -F'j E /V C7 ,I A/ tdiophysics.- Radio-Waves Vrtq%gatlon Abs Jour i Ref Zhur - Fizika, No 5, 1957, No 12532 Author i Denisov, N.G. Inst I Not given 1-5 Title t Effect of a Constant Magaetic Field on the Resonant Effect Observed, Upon Raflootioil of an Eleatromapatio Field from an Inhomogeneous Plasma. Orig Pub i Radiotaklm. i elektronika, 1956, 1, No 6, 732-738 Abstract i The author establishes the presence of a resonance in the refleation of radio waves from an inhomogeneous gyrotropio plasma, at the 1(y7el where the frequency of the incident wave coincides with the natural frequenoy of the plasma oscillations. In a medium without absorption, the field Card 8 USIM/Radiophysics. Ridio-Waves ptoMgi(tion 1-5 I Abs Jour t Ref Zhur - FizikEL,, No 5, 1957, No 12532 Abstract t of the waire inoreELSOB at this level to infinity. Esti- mates show that upon reflection of waves from the ionoB- phers, the influence of the resonant region is insignifi- cant. Also disouEtsed is the influence of the plasma waves that arise, at the resonant level. Card 1 21/2 k N N, G, $UBJECT. USSR ]?HYSCIS CARD 1 / 2 PA - 1890 AUTHOR DENISOVtN.G. TITLE on a Meo-ulllanty of the Field of an Electromagnetic Wave which is Propagated in an Inhomogeneoua Plasma. PERIODICAL iurn.ekap i teo:r.fis#31,faso-4,6oq-61q (1956) Issued: ; / 1957 In the course of various pre,rious works cited it was not explained how the amplitude of the growing field behaves in a medium with absorption, and what physical significance this peouliarity has in a medium without absorption. These problems will form the object of a close examination in the course of the present work. At first the special features of the field of the electromagnetic wave in the case of an inclined incidence on to the linear layer of a medium, the proper- ties of which depend only on the z-ooordinatep are investigated. From this investigation the following result was essentially obtained: For an isotropic plasma with slowly changing properties the increase of fieldstrength in the domain of low values of 6 (z) in the case of large angles of incidences is of no importance whatever. However, in the case of small angles ~ 0 - 2 - 20 (V eff 103) this effect bocomes noticeable and the existence of a point with E 0 causes a oonaideMbla change in the form of the solution behind the point of reflection. The increase of the strength of the electric field of the standing wave is then not balanced by existing absorption. V Zurn.eksp.i teor.fio,J31,faso.4,609-619 (1956) CARD 2 / 2 PA - 1890 Thd influence exercised by plasma waves is then approximatively taken into account. In media with very low absorption the anomialous behavior of the corresponding solutions is conserved and the actual. behavior of the field re- mains without an explanation, because in an inhomogeneous medium also other factors are able to play an important part. The oheracteriatio behavior of the vertical componont B z of the field of an electromagnetic wave propagated in an ionizing medium with plane layers suggests a certaiia connection between this phenomenon and certain resonance properties of the quasineutral plasma. Resonance occurs where the f:requency oi of the inciding wave is identical with the eigenfrequency W 0 of the plasma oscillations. Such a dependence of JEZ12 on the coordinate is characteristic of the idealized problem in which every kind of scattoring of the energy of a standing electromagnetic wave is neglected. The width of the corresponding "resonance curve" is on this occasion determined by absorption. However, in an inhomogeneous plasma also an other mechanism of the diosipation of energy is possible, viz. the pro- duction of plasma waves. The existence of a sharply changing longitudial com- ponent of the electric field causes a spatial inhomogeneity of the electron gas. In all such"diaturbed" domains of the medium the electrons perform oscillations the amplitude of which grows with a growing approach to the point of resonance. Taking the heat motion of electrons into account leads to equations of a higher order. INSTITUTION: State University Gorlkij -AOTHTA OMM"N, B.N., GIVZBUR% V.L. I DMUSOV) 53-4-Y/7 TITU The Propagation of zlectromag Waves in a k1lasma (in the Iono-spnere). .1 OR~aprostraneniye elektromagnitnylch voln v plasme (ionosfere) -Russian). MRIODICAL Uspekht Fiz. Nauk, 1957, Vol 61, Nr 4, Pp 561-612 Received 6,4957 Reviewed 7/1957 ABUTRACT starting out from the monograph by la.L.Allpert, V.L.Ginsburg, BI.Feynberg "The Propagation of Radio Waves" (Raspostraneniye rediovoln- Gostekhizdat, 1953, the paper under review deals with some problems of this field which have been clarifiedto a certain extent since the publication of the mono- graph. The consideration of the neat motion of electrons in a homogeneous medium in the magnetic field leads to the octurrence of plasma waves, the consideration of the heat motion of iona, on the other hand, results in low-frequency magnstohydrodynamic and quasi-acoustic waves, both with dis- persion. In Inhomogeneous media it is possiblo that we have cases where the approximation of geometrical optios is no more permissible and where an in- teraction of waves taikes place which would be independent in the homogeneous or quasi-homogeneous case. This ti the case in the absence of a magnetic field at vertical incidence in the proximity of the reflection point and at oblique incidence in the proximity of the point (aJ) a 0, at the exi- stence of a magnetic field at a stall angle between the wave normal and the magnetic field (multiplication of the reflected radio si,-rtals), and at Card 1/2 the beginnIng of the layer where the concentration ofthe electrons still is The PropEqation of I~Lectromagnetic Waves in a Plasma 53--4-4/7 (in the Ionosphere). small. For the latter case the paper under roview computes the boundary polarAation of the short waves which leave the ionosphere for a certain model of the ionosphere, but it is unable to offer any, new information about the ionosphere. (With 18 reproductions, 73 references). AtiSOCUTION PRESENTED BY 6UBMITrED AVAILABLE Library of Congress Card 2/2 t io - I I VI . G., V. A. Vlovlk im-L- iy) M "The Wave Propagation in Mediums With Random Heterogeneities". report presented at the All-Union Conference on Statistical Radio Physicis, Gorlkiy, 13-18 October 1958- (Izv. vyssh uchev zaved-Radiotekdi., vol. 2, No. 1, pp 121-127) COMPIXTE card under SIKDDV, V4*-I.) DE-IWSOV, N. G. "The Wave Propagation in a Plane-Laminar Meditun With Statistical Hetero- geneities". report presented at the All-Union Conference on Statistical Radio Physics, GorIkiy, 13-18 October 1950- (Izv. vyssh uchev zaved-Radiotekh., vol. 2, No. 1, pp 121-127) COMPLETE card under SIFOROV, V. I.) 0601 AUTHOR: Denie*v, N.G. SOAr/JL41-1-5-6-5/28 TITLE: ia-ve Pi"rop:*;a-tMon In a Planar Laminary Medium Containing Statistical Inhomogeneitles PERIODICAL: Izvestiya vysshikh uchebstykh zavedeniy, Radiofizika, 1.958, Val 1, Nr 5-6, pp 34-40 (USSR) ABSTRACT: It is assumed tha:t the waves propagate in a medium Wimse refractive index is a point function of the height z and undergoes random fluctuations with respect to its average value n(z) . The problem can be solved by dividing the non-uniform medinn into a number of flat layers. The thiclmess of these layers should be small enough ca as to make it possible to assume that each layer is statistically uniform. On the Dther hand, each layer should contaill,a large number of kahomogenelties so that the correlation between the layers can be neglected. The,probability W(zV ) that a ray which passed a tbiclmesB z wilj- havo a dIrectioA detennined by the angle -Y is defined by (M.A. Leontovich - Ref 3): Cardl/5 06461 eze.1-zi-i-6-5/28 iov Wave Propagation in a Planar Laminary e m on aining Statistical Inhomogeneities OW d-Y sin sin,# (D - - - az ab, a'Y dz The diffusion coefficient D in Eq. (2) is defined by the-statlatical properties of an elementary layer and.is given (L.A. Chernov g Ref 1, M.A. Loontovich - Ref 3)J by Eq (3), where j is the average square value of the deflection angle of the initial direction, at the exit from a layer having a thickness 4z . The final expression for the diffusion coefficient is: (An)- D T n2 (6) where t denotes the scale of the random Anhomogenelties. If ~%V is comparatively small, the solution of Eq (2) is in Card2/5 the form of Eqs (8). From this, it is found that the average 05h61 SOV/141-1-5-6-5/28 Wave Propagation in a Planar Laminary Medium Containing Statistical Inhomogeneities square of the incidence angle fluctuations is given by Eq (9). If the non-uniform layer has a thicimess z 0 Eq (9) is in the form of Eq (9a). Since the average square fluctuation of the refractive indjax is given by Eq (10), Eq (9a) can be written as Eq (11). The above formulae are valid for the p1ane-waves whose incidence is normal tjD the layer. It is of interest to define the same parameterv for the case of an incllndd :Lnc:L&exLce. The problem can be solved by considering Eq (15) (L.A. Chernov - Ref 2), where n' denotes the refractive index of a non-uniform layer, S is a unit vector of the tangent to the ray and 6 is a linear co-ordinate measured along the ray. The average square value of the ray deviation (due to the random fluctuations) is now expressed by Eq (20), where N(r) is the correlation function of the refractive index. By introducing a diffusion coefficient D , as defined by the isecond equation on P 38, Eq (20) can be written in the J-.orm of Eq (21). The fluctuation of the Ca.rd3/5 intensity of a ray which passed through an inhomogeneous 06461 1 28 Statistical Wavg, Propagation in a Planar Laminary 1-?eVVu'm1_4~;ni_a:Cn'Vng Inhomogeneities layer can, be evaluated by using the method of L.A. Chernov (Ref 2), provided that the average refractive index-is independent of the co-ordinates. If the refractive Index is represented by the last equation on P 38, Eq (15) leads to Eqs (22). The first- two of these can be written as Eqs (23). Consequently, thio lateral displacements of a ray at the exit from the non-homogeneous layer, having a thickness z , are given by Zqs (24). The relative change of the ray intensity Is, thex-efox-e, deternaned by Eq (25). Integration of Eq (25) leads to Eq (26). Consequently, the average square fluctuation of the intensity is given by Rq (27). The correlation function of this equation is defined by the last equation on P 39. The expression for the average square fluctuation can, therefore, be written as Eq (28). If the thickness of the layer z 0 is much smaller than the scale of the inhomogeneities, Eq (28) can be written as Eq (29). When the correlation function is in the form: Card4/5 N = exp(-r2/t2) I o6461 SO%~4j-1-JLZ%7Aj,5j-',U'8,,,g Statistical Wwre Propagation in a planar Laminary 8 ium Inhomogenelties ts.giv.9u.by F4 (31). This the average square fluctuAt"31- wh formula indicat*5 that thefluctuAtiOnz-J-niDr-"e an n in a layer ten" to 0 (at a certain level)- All the above formulae were derived for the waves with an infinite front. The results can be used, however, for the evaluation of the fluctuations in wave beama,provId-ed that the tran verse dimensions are greater than those of the random inhomogeneities. The author makes acknowledgment to V.L. Ginzburg for discussing this work and for valuable remarks. There are 5 references, 4 of which are Soviet and 1 English. ASSOCIATION: Issledovateltakiy rad.1ofizichaskiy InstItut. prl Gorlkov.skom universitete (Research Radiophysics Institute of the Gorlkiy University) SUBMITTED: May 23, 1958 Card 5/5 o6462 AUMOR: Denisov, N.G. SOV/141-1-5-6-6/28 TITLZ: Wave Scattering in a Planar LamiLaryMedium PERIODICAL: Izvestiya vysahl-kh uchebnykh zave4eniy, Radiofiz:Lka, 1958, Vol 1, Nr 5-6, pp 41 - 48 (USSR) ABSTRACT: The problem is formulated as follows. The average value of the permittivity z is a function of the height z . The random deviations of the permittivity be from its average value are comparatively small. The problem of finding the scattered field consists, therefore, of finding the field of elementary radiators whose power is determined by 4v and by the field cfthe primary wave. If the field at r, = 0 is E 0 and the wave enters the non-uniform layer without reflection, the field at a height z is given by: z E -ik.indz + i(ot( k ~rnw c Cardl/5 06~62 sov/141-1-5-.6-6/28 Waive Scattering in a Planar Laminary Medium- The scattering volume. can be divided -Into elementary volumes dV . The dipole moment of such a volume Ls given by Eq (2). It Is now necessary to determine the fi-eld of an elameptaLry rAAiator- situated In a non-untform layer. The radiation can be.approximait.ely represented by Eq (3), where r ip the distance between the radiator and the point of obser- vation, i is "he ax4p a between the vector k and the direction tf the dipolt')Izoment. The field at the output of a noz-uniform layer (due to a dipole situated at a height z ) can 'be written In the form.of Eq (4), where -&0 amd y 0 are the angles detex=luing the direction of a ray at the exit of a-layer,and R 0 is tbLe radius vector at the point of observation, This filn t1on f in Eq (4) is given by Eq (5), wheire d4- is the spherical angle of the radiation "tube" at the source level and dS 0 is thVi area of the "tube" at a. level z = zo The square of the intensity of the scattered field can be written In the form of Eq (8). This can also be represented by Eq (10), Card2/5 or, finally, as Eq (11). The average square value of the 06462 SOV/141-1-5-6-6/28 Wave Scatterimg in a Planar Laminary-Medium intensity in, therefore, In the form.of Eq (12), where is the correlation function.-of tha-.-.per-ittivity fluctuations. The effective scatterIng.cross-sectlon !a,, therefore, given by Eq (13)- If the correlation function is exponential, the scattering cross-section is expressed by Eq (15). The above formulae are valid for a plans wave. In order to daterinine the scattering of spherical waves, it is necessary Vo take into account the divergence of the rays of the primary waves. In this case, the average square value of the scattered field Is given by Eq (23), where d im determined by Eq (13). The quantity df~ denotes thq spherical angle of the ray tube of a radiator which I# situated at_&,dis~tance h 1 from-the non-uniform layer; dS1 is thecross-section of the tube at the beginning,of the non-uniform layer (z = 0 - Figure 1). For a point situated on the_ aXiS z at a distawe h2 from the upper Card3/5 boundary of a flat layer (Figure 1), the average square field o6h62 ig/141-1-5-6-6/28 Wave Scattering in a Planar Laminary fe ium is given by Eq (24). This can further be written as Eq (28), where r and are defined in Eqz (26) 4ind (27). The firtal expression for the scatteied field is given by: "o TN72 nk2 t v 092 1102 0 dz (35). 0 ~, I., r- ) 2 C 2 0 This formula Is 4imilar to Eq (22) except for the divergence factor: 2)_2 There. -are 5 ref-e-r-ences, of which 1 is English and 4 are Soviet; I of the Soviet references is translated from EnglIsh. Card4/5 o6462 SOV/141-1-5-6-6/28 Wavo Scattering in a Plan&r Lamina y Medium ASSOCIATION: Issledovatellskiy radiofizichaskiy institut pri Gor1kovskom universitete (Radiophysics Research Institute of Gorlkiy University) SUBMITTED: November 21, 1958 Card 5/5 506-2-46/ro A UTH I OR Denisov, IT. G. TITLE- On the Problem of the Absorption of BlectromaUnctic Waves Within the Resonance Ranges of an InhomoEeneous Plasma (K voprosu o pogloshchenii elc!ktrom----.nitnyl"-b voln v reno- U nansnyhh oblastyakh, neodnorodrioy plaziny) PERIODICAL: Zhurnal Eksperimentallnoy i TEloreticheskoy Fiziki, 1958, Vol. 34, Nr 2, PP 528 - 529 (USSR) ABSTRAM The phanomenologic description of the proparation of electro- magnetic waves in a plasma is based on the possibility of the introduction of the index of refraction of the medium. Pirst the author refe= to several earlier works dealinr., .iith the same subject. K. G. Budden (reference 3) computed the absorption within the vicinity of the sinCular point of the index of refraction for the most simple model of an in- homogeneous layer. The complete solution of this problem can be obtained for the case of awak inhomogeneous plasma. Card 113 The present viork gives the results of such an investiL-lation. 56-2-46/51 On the Problem of the Absorption of Electromagnetic Waves Within the Re- sonance Ranges of an Inhomogeneous Plasma In a Tieak inbomogeneous medium the interacticn of the o_rdi- nary and extraordinary ray can be neglected, rith the ex- ception of the spacial case to be investigated later on. For reasons of simplicity the author restricts himself to the investigation of the transverse propagation, althouz-h the final formulae can easil-v be generalized. In the trans- verse propagation the index of refraction of the extraordi- nary wave has a singular point. For the derendence of this index of refraction on the concentration of electrons a for- mula is put down. A formula is also given for the reflection coefficient. The maximal value of the absorption coefficient in about 35; ~- In the calculation of the absorption within the range of resonance the interaction of the various types o:C waves must be taken into account only in the case of qua- silongitudinal propagation. Then various details are short- ly discussed. The absorption effect discussed here is con- nected with the transition of electromagnetic waves to plas- ma waves. The mechanism investigated here, can, by the way, only explain the appearance of the triplet. Multiple reflec- Card 2 tions can not occur. There are 6 refer;nces, 4 of which are -/O'V1C_ . 05494 AUTHOR: Denis ov sov/141-2-2-19/22 TITLE: Amplitude and Phase Fluctuations of a Wave Passing Through a Layer with Ralkdom. Inhomogeneities PERIODICAL- Izvestiya vysshil-di uchobnykh zavedeniy, Ftadiofizika, 1959, Vol 2, Nr 2, pp 316 - 318 (USSR) XBSTRACT: Previous analyses have considered either a layer with constant average. parameters (L.A. Chernov - Ref 1 and V.I. Tatarskiy .. Ref 2) or a layer in which only the intensity, e.g. of turbulence, varied (Ref 3). In the case considered here, besides the regular variation in refractive indelil, there are random inhomogeneities whose mean int-ensity depends on height. Starting from the scalar wave, Eq (1), and -suppos:Lng that'the scale of the random Inhomogeneity Is much larger than the wavelength and much smaller than the scale of regular changes in pexMittivity, a simplified 3xpression for the potential f. is Eq (5). The solution to this equation is in terms of' Fourier integrals for variables x and y , as shoum in Ref 2. Card 1/2 05494 SOV/141-2-.2-19/22 Amplitude and Phase Fluctuations of a Wave Passing Through a Layer with Random Inhomogeneities The inhomogeneous layer has a thickness LI and contains within it a randomly non-uniform layer of thickness, L 0 The correlation function for complex phase is Eq (10), wbich practically coincides with the expression obtained in the work of H. Scheffler (Ref 7), with approximate getometric optics. V.L. Ginzburg advised in this work. There are 7 references, of which 5 are Soviet, 1 German and 1 English. ASSOCIATIM Issledovatel'skiy radiofizicheskiy institut pri Gor1kovskom universitete (Radiophysica Research Institute of Gorlkiy University) SUBMITTED: February 13, 1959 Card 2/2 67528 Agl' Z.3 a 0 AUTHOR: Denisov, N.G. SOV/141--2--3-5/26 ""rIm"ale""o? the Accuracy of the Adiabatic Invariant TITLE: An Es PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika, 1959, Vol 2, Nr 3, PP 374 376 (USSR) ABSTRACT: The adiabatic invariant: 11M = mv2/2H const .i. -i\. holds in the case of motion of a charged particle In a slowly varying magnetic field H . where v-L is the component of the electron velocity perpendicular to the direction of the external magnetic field. How far this relation holds has been a matter of some controversy. If one introduces a small parameter describing the rate of change of the magnetic field, then it is knomn that the adiabatic invariant holds with an accuracy up to the square of the small parameter (Ref 1). It has been shown (Ref 2) that in the case of a uniform slowly varying field the adiabatic invariant holds to an accuracy which is Cardl/2 proportional to exp(-A/a) , where A is a constant and 01 7 5Y b SOIV14.L-2-3-5/26 An Estimate of the Accuracy of the Adiabatic Invariant a is a small parameter describing the rate of chan~,e of the magnetic field. The present paper is ol-3o ~;oncernecj with the case of a uniform field which -was considered ir. Ref 2 and it is shown that the above *-o estimates of the accuracy are not contradictory but refor to different conditions. There are 4 references, 2 of which are Soviet and 2 German. ASSOCIATION3 Issledovatel'skiy radiofizicheskiy institut pri GorIkovskom universitete (Radiophysics Research Institute of Gorlkiy Univel~-SIT-y-j-- SUBMITTED: April 2, 1.95!) Card 2/2 DENISOV, N.G.; ZVEM, V.A. Some questions of the tbeory of wave prolxLgation in media with random InhomogensitiOB; SUrVOT. ISV.VYS.UCheb.zav.; radiofiz. 2 no.4,:521-542 159. (MIRA 13:4) 1. Nauchno-isslednvatellekiy rp-diofiziclieskiy inatitlit pr', Gorlkovskom univoraitete. (Radio waves--Scattering) 80139 9, looo S/141/59/002/06/021/024 EO AUTHORS: Dentso Polyard Deni.sov,N.G. and ~20K4 '~~t~"Aie"Wvubw TITLE. AmplituVe""and Phase Fluctuations in a Wave Propagated in a Non-uniform. Absorbing Medium -".I PERIODICAL: Izvestiya vysshikh uchebnykh zavedieniy, Radiofizika, 1959, Vol 2, Nr 6, pp 1010 - 1012 (USSR) ABSTRACT: Usually, fluctuations in the wave parameters are calculated without taking into account absorption in the medium. The present note is concerned with a method for taking absorption into account. It is assumod that the mean value of the complex dielectric oonstant e1 in the layer depends on z . In that case, the propagation of a scalar -wave is described by an equation of the form given by Eq (1), where A cl(x, y, z) represents random changes in the complex dielectric constant and k 0 = w/o where w is the frequency of the wave and c is velocity of light. If the layer is sufficiently then the solution can be written in the form Cardl/3 E = exp R, (x, Y. Z) (x, Y, Z) and 1. the regular, and 80139 Amplitude aLnd Phase FLuctuations uniforip Absorbing MediUE2 s/14i/59/002,/06/021/024 MkEi4ropagated in a Non- in a v are given by E(Is (2) and (3). The time dependence is harmonic (e'01;) . The random functions in Eq (3) are then (otpanded into a Fourier integral in x and y , so that Eqs (4) and (5) are obtained. It is assumed that tho paint of observation z = L 1 is outside the region in which irregular changes inthedielectric constant are present (L ~-. L 0) . Using Eqs (6), (7) and (8), the real. anti the imakInary parts of the solution (4) can be written in the form given by Eq (9). The change in the amplitude anti the phase due to absorption over distances of the oreler of the seale of the random irregularities L is negligible. The analysis is continued to obtain the correlation functlon for the complex phase. It is shown that in amplitude and phase calculations absorption need not be -taken into account if the condition given by Eq (1!5) is satLsiried. That is equivalent to saying that in the geometrical-optics zone.abisorption need not be taken Card2/3 into account. In the ionosphere this condition may no~ ,,- 80139 S/141/59/002/06/021/024 EVaVF,": -14 Amplitude and P1mise Fluctuations in a e PPopagated in a Non- uniform Absorbing Medium hold for frequemcies w < 2T107elec-1 and in the lculation of scattering In the E-layer absorption c a. must be taken into account in this frequency region. There atre 3 Soviet references. ASSOCIATION: Nauchno-issledovatel'skiy radiofiZicheskiy institut pri Gor1kovskom universitete (Scientific-research RadiophySio In ititute of Gor1kiy Iniversity) SUBMITTED: October 7. 1959 Card 3/3 AUTHOR: N,,.G.2anisoy - SOV/109- - -4-3-7/38 TITLE: '7'-Absorption of Radiowaires in the Resonant Regions of a Non-Homogeneous Plasma (0 pogloshchenii radiovoln v rezonansnykh oblastyakh neodnorodnoy plazmy) PERIODICAL: Radiotekhnika i Elektronika, 1959, Vol 1+,. Nr 3, pp 388-397 (USSR) ABSTRACT: A magnetically active plasma is generally characterised by two refraction indices. It is known that for certain values of the electron concentration, one of these indices tends to infinity. This condition of the plasma can be referred to as the resonant regiong since it is caused by the resonant properties of the plasma (Refs 172). For the purpose of analysis it is assumed that the plasma 1:3 situated in a magnetic field H and that the electron concentration is dependO only on the co- ordinate z. If the direction of the horizontal magnetic field coincides with the axis x, the wave equation for the system can be Written as: 2"V 2 1 - v U - v) ) Fy = 0. Card 1/4 ~ + ko (1) dZ2 1- u- V SOV/109- - -4-3-7/38 Absorption of Raddowaves in the Resonant Regions of a Non- Homogeneous Plasma where the various parameters are defined by Eq (2), and Wjj is the gyromagnetic frequency of an electron. Eq (1) describes the propagation of the extraordinary wave whose refraction index is expressed by Eq (3), If the function v of Eq (1) is linear and has a slope a, Eq (1) can be written as Eq (4) where 1 - u - v = t . The general solution of Eq 0+1 can be found on the basis of the approximation of geometrical optics and is in the form of Eq (5). This can also be written as Eq (7). If the extraordinary wave impinges on a ncn-uniform layer from the left, it Is found on the basis of Eq (9) Ithat the refraction coefficient is given by Eq (11), If the wave impinges from the right, it is shown that no refraction takes place. A more accurate expression for the refraction coefficient R is given by Eq (16). The modulus of the refraction eoefficient can, the::~eforej be expressed by Eq (17). The arameters 6 and S in Eq (17) are defined b7 Eqs R8) and (19). For 6,.., 15 is Card 2/4 8 1 iven by Eq (20) and Eq (17) ~Tan be written as Rq (2 ~. A graph of Eq (21) is shown in Fig 3. If the sov/log--4-3-7/38 Absorption of Radiowaves in the Resonant Regions of a Non-Homogenoous Plasma P3'Operties of the medium (plasma) change as a function of z , and if the magnetic field of'-the earth Ho is at an angle m with respect to the axis z 9 the solution of the equations describing the propagation of plane waves along the axis z is in the form of Eq (22). Here n, and n2 denote the refraction coefficients of the ordinary and the extraordinary waves; the remainin parameters of' Eq (22) are defined by Eq (23). Eq f22) is derived on the basis of the approximation of geometri- cal optics. The equation is not applicable in the regions where the reflection or interaction of the two waves takes place. The presence of the interaction results in a change of the constants al 2 and d1,2 in Eq (22). However, if the lower integration bouftdary A in Eq (22) is chosen, so that the point A is situated to the right of the interaction regiong the resulting solution of Eq (22) doseribes the incident and the reflected wave to the right of the point A . The solution in -the area to the left of the interaction Card 3/1+ region is also in the form of Eq (22), but the values of SOV/109- --4-3-7/38 Absorption.of Radjowaves in the Resonant Regions of a Non- Homogeneous Plasma the constants are different. These constants are expressed by Eq (21+). The author expresses his gratitude to ir.L. Ginzburg for his valuable remarks. There are )+ figures, 1 appendix and 8 references, )+ of Card 4/1+ which are Soviet, 3 English and 1 German; the appendix discusses the solution of Eq SUBMITTED: September 5, 1957 S/141/601003/02/005/025 .4192/9382 AUTHOR: Denisov, N.G.- TITLE: Influence of the Reflection Region on the Scatterinoof Radiowaveselin thojonosbhere.,'Y PERIODICAL: Izvestlya vyssh1kh uchebrxykh zavedeniy, Radiofizika. 1960, Vol 3, Nr 2, pp 208 - 215 ABSTRACT: It is assumed that in a nonhomogeneous ionospheric layer, whose permittivity e(z) is dependent on the height z there exist also random fluctuations As(x,y,z) . The investigation of the problem can be based on the solution of the following scalar equation: '&Y + ir" w/o) (1) " [ E (Z) +- AS (X, Y, Z)3Y = 0 (ko 0 The solution is in the form 41 = Yo *Wl where yo is the solution for the case when Ac = 0 Cardl/5 The function Y, can be found by solving: L/11c", S/141/60/003/02/005/025 Ejg2/�28 Influence of the Reflection Region on e aitering of Radiowaves in the Ionosphere tiY k2 VWY k 2A eye (2) - 0 1 0 It is seen therefore that the problem amounts to the determination of the field in a nonhomogeneous medium for the case of a given distribution of sources. The equation. can be solved by representing the random functions Y- 1 and A c in. the form of Fourier integrals dependent on the variables x and y (Ref 3). Two functions ITI and f defined; by Eqs (3), are introduced. The function Q satisfies Eq (4). For a linearlayer in which e = -az E (4) can be written as Eq (5), where C = az and 0 satisfies Eq (6). The solution of Eq (6) is in the form of Eq (7), where v is the Airy fi4nction and A 0 is the amplitude of the incident wave at the boundary of the non--homogeneous layer. The general solution of Eq (5) is in the form of 1Pq (10). The compa7ent of the scattering Card2/5 field at the boundary of the layer =.-I) can therefore I -,--/ s/14i/60/003/02/005/025 t~224Ea~? Influence of the Reflection Region on c ering of Radiowaves in the Ionosphere be expressed by Eq (13)- If the random irregularities form a fine diffraction grid, having, a thickness d