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December 31, 1967
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7. tl~4.~2__-_, L ~9178_66 EWT(-l)/FCC/EWA(h) _GW ACC NR: AP6o:L8864 SOURCE COM 'UR/ao376.5/005/005/0 AUTHOR: Skr~p~, G. V.; Krivophapkin, Pe 9 aITLkly, G. F.1 Filippov, Vo A. ORG: Institute of Astropjg~sical Research and Aeronomy. Yakutsk Branch, SO AN SSSR WSWO (Institut kosmofizicheskm issiedovaniy i aeronomii Takatslmgo filiald SO by the crossed telescope TITIE: Study of tho anisotropy of -2Qzda_rAys a maUod SOURCEi Geomagnetirm i aeronomiya, V- 5, no. 5, 1965, 817-425 TOPIC TAGS: cosmic ray anisotropy, goomagnetic field, solar activity 7 ~_ ABSTRACT: A method is proposed for taking into-account distortions -of anfao,41 .,tropy of cosmic rays by the geomagnetic fiel4,gnd the directional dia- ` J muted matrices restoring gram of the instrument. The authors have com the true vector of anisotropy for instruments of the Yakutsk complex. Computations were made using coupling coefficients for different zenith ,angles and three forms of the energy spectrum of anisotropy. Using the ~matrices the authors have restored the true vectors 'of anisotropy for :the neutron component for three epochs of solar activity (1958-1964). ,Readings of azimuthal telescopes were used in finding the true vectors and the vectors.of the atmospheric influence for the earth's surface and. for'depths,of V.20 and 60 m (water equivalent). An evaluation'-is given: ,of the degree of agre:ement between the derived vectors and three,forms., Card 1/2 uDc: 323o163 7-7 - -x ------- ------- L 01 4 5S EW-i FG! -;b '4 ACC NR.- AT6027220 SOURCE CODE: AUTHOR: Krymskly, G. F.; Almukhov, A. M.; Skripin, G. V.; K Kuz'min, A. 1. ORG: none TITLE: New method for studying the anisotropy of cosmic rays SOURCE: AN SSSR. Sibirskoye otde i rasprost~r-vneniya radlovoln. Iss-ledovaniya po geomagnetizmu i aeronomff (Studies in geo- magnetism and aeronomy). Moscow, Izd-vo Nauka, 1966, 105-110 TOPIC TAGS: cosmic ray anisotropy, cosmic ray intensity, cosmic ray ABSTRACT: A method is proposed for determining the instantaneous characteristics of the anisotropy of cosmic rays. The method will make it possible to obtain the anisotropy dis- tribution in the merldional planes and to study the anisotropy of phenomena characterized by abrupt changes in the isotropic background (such as the Forbush decreases), all of which was not possible using the method of diurnal variations. The method proposed makes use of the fact that the world-wide network of stations established during the IGY makes it possible to determine the neutron component with an hourly statistical accuracy of 0. 1% and, thereby, Card 1/2 I ACC NRj AT6027220 D to determine the anisotropy characteristics over a 2-hr observational period, provided that its amplitude exceeds the mean amplitude by a factor of more than 2. A distinctive feature of the method is the representation of the distribution of cosmic-ray intensity over the celes- tial sphere in the form of a series in spherical functions and the use of the first spherical harmonic of the series. The expression for the first harmonic yields the amplitude of the anisotropy vector and an expression for the Intensity in an arbitrary direction at an angle to the direction of anisotropy vector. The spherical analysis reduces to the solution of a system of lines ~;quationB with four unknowns. The solution of the system determines the isotropic portica of cosmic-ray intensity as well as three components of the anisotropy vec- tor. The coefficients at the unknowns are calculated and tabulated for 38 stations, taking Into account the effect of the geomagnetic field on the charged-particle trajectories, and also the energy spectrum of the variations. OrIg. art. has: 6 formulas and I table. SUB CODE: 04/ SUBM DATE: 25Dec65/ ' ORIG REF: 012/ OTH REF: 002 Card 2/2 L 04886-67 LW'C( 1 VEWT(q~"/FCC I FV( 1 C; L1/("W ACC NR: AT6027221 SOURCE CODE: UR/0000/66/000/000/0111/0118 AUTHOR: Kuz'mIn, A. 1. ; Krymskiy, G. F. ; KrIvoshapkin, P. A. ; SkrIpin, G. V. ChIrkov, N. P.; Sbafe , G. V. ORG: none TITLE: The nature of cosmic ray variations SOURCE: AN SSSR. SiblKqtoye otdgjcWxe_,_~IbI~s I rasprostranenlya radlovoln. Issledovanlya po geomagnetlzmu I aeronomit (Studies In geomagnetism and aeronomy). Moscow, Izd-vo Nauka, 1966, 111-118 TOPIC TAGS: cosmic ray intensity, solar cycle, magnetic field ABSTRACT: A brief survey Is given of available data concerning the variation of cosmic ray intensity and the effect responsible for this variation. The effects of fluctuations of the iiiagnetospherc and temperature fluctuations In the upper atmosphere on cosmic ray variations are examined, Cosmic ray flares with energies up to 10 Bev, and their association with Forbush decreases are discussed in relation to t~F. ir effect on cosmic ray variations. The I 1-year variations, 27-day variations, and solai~ diurnal and annual variations are shown to be closely interrelated, and to hxve modulation of galactic cosmic rays by the radial Inter- Card 6 7 ACC NR: AT6027221 planetary field as their common source. All existing observations on the variation of cosmic ray intensity are seen to indicate the existence of an external (with respect to the sun) radial interplanetary magnetic field and the predominant contribution of the dynamic effects of the field's disturbances to the modulation of galactic particles. An Important feature of the field's configuration (deduced from observations. of the variation of cosmic ray Intensity, and also from other unrelated data) Is its oblateness with respect to the plane of the ecliptic or the solar equatorial plane. SUB CODE! 04/ SU13M DATE: 25Dec65/ ORIG iiEr: 026/ OTH REP: 009,, Card 2/2 ACC NRi AR6027539 SOURCE CODE: UR/0313/66/000/005/0044/00447 Alr,.HOR: Krymskiy, G. F.; Altukhov, A. M.; Krivoshapkin, P. A.; Kuzlmin, A. 1; ,Skripin, G. V. -TITLE: A new method for investigating cosmic ray anisotropy SOURC'--;': Ref. zh. Issledovaniye kosmicheakogo prostranstva, Abs. 5.62.298 .RZ? SOURCE: Sb. Issled. po geomagnetizmu i aeron. M., Nauka, 1966, 105-110 TIAGS: cosmic ray anisotropy, linear equation, earth magnetic field, particle trajectory, radiation spectrum, variational problem iABSTRACT: A method using the spherical analysis of data from a worldwide network of i !stations is suggested in order to obtain the instantaneous characteristics of cosmi iray an-isotro-py. The analysis can be reduced to solving a system of linear equation: ,With four unknowns. The solution determines the isotropic intensity and three compo- nents of tne aii:'-sotropy vector. Introduced is a calculation for the coefficients !for the unknowns in the equations for each station. The effect of the earth's maxnet- lic field on particle trajectories, as well as differences in t4e energy spectraforiso-I .%.ropic and anisotropic variations, is considered. Abstract. LTranslation of abstractJ,- i'SUB CODE: 04 [Card 1/1 SHIPINA) G,~ F PtLlynological characterisz-ics of Mesozoic sediments in the Vilyuy Lowland. N'auch.socb. LA-FAII SS6.R cj.7-39-r-8 '.62. (I-LIBA 16:3) (VIlTay Lowland-Palyiriclogy) SHITOVA , A,Ye,; SIMIPINETS, G.M. Drying of beech wood. B=.i der.prom. no.1.45--47 Ja-4-Ir 162. NIRA 15:5) 1. Livovskiy lesotekhni.-,heskiy institut (for Shitava) 2. Chinadiyevskiy domostroitel'-n;yy fanernyy kombinat 4or Skripinets). (Beech-.-Drying) -1 4 11 . 1'. L 7973-6 EWT.(3-~/i~dP(m)/EWT(m)/EWP(W)/Z,;WA(d)/T"2/EWP(k)fFc~3(k)/STC(*)/EwA(1) WWIFM T ACC NR: AP5026692 SOURCE CODE: UR/0258/65/005/00510940/0945. AUTHOR: Skripinichenko. S. Yu. (Moscow) ORG: None TITLE: Longitudinal long-term perturaation movement of an airplane with a float- ing tail assembly SOURCE: Inzhenernyy zhurnal, v. 5, no. 5, 1965, 940-945 TOPIC TAGS: aircraft tailq_~ , perturbation theory, aerodynamic stability, flight- s -on i crf 2 d v n j & Mj a L mechanics, -su ABSTRACT: The presence of a floating tail assembly can exert a noticeable effect: on not only the short-term, but also on the long-term movement, as a result of a significant change in the characteristics of its turn-Ing moments depending on the. Mach number of the flight. This is particularly important in supersonic flight and in takeoff and landing (See Fig. 1) Cord 1/3 UDC: 53 3. 0. 013-. j~ ?92140, ACC NR: AP5026692 yat, Y r X Fig. 1 '!T"77 The article derives and solves a system of equations to describe the perturbation Movements. It is demonstrated that the long.-term movement of an airplane with i~ a floating leading tail assembly can, with sufficient accuracy for engineering pur- poses, be described by a system of differential equations of the second order. A floating tail assembly can exert a significant effect on the long-term movement of an airplane, especially under supersonic flight conditions. The effect of a floating' tail assembly on the long-term movement depends basically on the magnitude of C.,d 2 13 L 7923.66 ACC NR: AP5026692 the turning moments of the planes of the floating tail assembly, according to the Mach number of the flight. OrIg. art. has: 16 formulas, 3 figures, and 2 tables SUB CODE: ME/ SUBM DATE: 12Oct64/ ORIG REF 002/ OTH REF: 003 Card 3/ T-M ~- SYRIPINSKIY, F., mekhanik Small-size rice MY- '59. processing unit. Muk.-elev. 'prom. 25 no.5:23 (MIRA 12:8) (Rice processing machines) SKRIPITSYN, V.Ye. nTruck frames" by D.B. Gellfgat, V.A. Oshnokov. Reviewed by V.E. Skripitsyn. Avt. prom. 27 no. 5:48 bly 161. (MIRA 14:5) 1. Moskovskiy avtozavod imeni Ilkhacheva, (Motortrucks-Design and construction) (Gellfgat, D.B.) (Oshnokov, V.A.) cv .-'uc n n s cnc a T- I e i--r iL., i --, r(i r i i ry :An H J, ~r t, (.,_.i --n e, r, c-2 c f (, 1! id i,, Le o CX Eflect wit 2,41-wifh1orophenoxyricelic acid oil tomatoes with Iti f iz -&I diet. N. F. Ski-it, -BA (M. V. I., hill on 0 m e oil "IV St ate Ulliv.. Movow.). 'P31,11v Akad. Sa.k I d ,N.S.R. 73. 457-CV(K 2.4-1) vocrAly trt~" It Ir bellericiA effect of rertillrerl owl the toula t" ef"j, and the fi ar,cuv" .,lualu"I with difTercul ,,,let. uf nutrimm tur niagnitied by '-',4-1). Its b"1 ril"t Out- up t lite 1-im f-." of mix. nutrition. In the pte,tcrice of 2.4-1) wilt: fruit does -inn( show the formation of phytin rhat :iw-