4 j 4 FIRM NO. Ge testal ants! ony 4 . . 4 i Vd pate A ok od oO NO { WIR tr USSR LOCATION NAME OF INSTALLATION DATE/ INFO DATE/SOURGE | PF DA MO YR EVAL PcoDE | counTRYY or R AA ; ‘ ounte Approved For eleass 2007/03/28 " CIRERDP96-0078¥R000500130081-6 CONTROL NO, SOURCE | 28 SEP 61 FBIS UNPUBLISHED IRKUTSK RADIATION LAB -- A SCIENTIFIC STATION TO STUDY SOLAR RADIATION 1s BEING SET UP BY THE USSR ACADEMY OF SCIENCES IN THE SPURS OF THE EASTERN SAYANY RANGE, MORE THAN 2,000 TWO THOUSAND METERS ABOVE SEA LEVEL, THE STATION WILL STUDY THE EFFECTS OF SOLAR RADIATION ON THE IONOSPHERE AND ON THE PROPAGATION OF RADIOWAVES ON THE EARTH. THEY WILL ALSO CONDUCT OBSERVATIONS OF COSMIC RAYS AND STUDY TERRESTRIAL ELECTRIC CURRENTS AND THE TERRESTRIAL MAGNETIC FIELD. . | (MOSCOW TASS ENGLISH EUROPE 1331 GMT 28 SEPTEMBER 1961--L) PROCESSING DATE “PRFIRM NO. —aaeowe=s CODE PS AF CHART ACTIVITY CODES a OL lth [ofee H98 | LOCATION s/T |NAME OF INSTALLATION : : Sy AL re EA I So Lark. ST! [_oarereounce || a ii. SICCREPORT ON AEROSPACE IN THE USSR: ' High altitude Observation Station in the South of Siberia SG1A s item (Ref. 6, 30 Sept 1961, p. 4) the first high the eastern part of the USSR is According to a new altitude station of the Sun Service in “peing opened in Sayan Mts. at an altitude of over 2,000 m. above sea level. “The station belongs to the mountain-solar expedition of the Institute of ‘Terrestrial Magnetism, Ionosphere and Radiowave Propagation of the Siberian “Branch, USSR Academy of Sciences. ‘The Sayan high mountains were chosen for scientific observations because - the Sun is covered by clouds only 17 days a year, on the average, in that region. The transparent, noticeably rarified air permits to conduct observations of the solar disk without the usual interferences. FORM USE PREVIOUS 12-60 326a coitions. B OMLY: resbrigd mans ionosphere, an a Poow- park 20, Hae Deed Tegeareh oO 7 s mo bhe ani in the earth. . tha gouge of Po Seeme ca 2 Boi 1 EES Gare. £58 Way OF i j Rees a bie earta oh ah gigniPieamre Pee. a : a GF AG RKOaL danth. aa well ag for daysavppenh ow. 9, hobed | , vor sucvevine mineral daposita. Tha study or tas aonespanid j i ane , a er ae in 2. = : vo ‘, rn . Pe ° cad wienetis, gales (oar). as. i be inatiuence of Ame OT PAULO os ah Z 2 feta TEENS 3 soe WAY ee ha ; bee 0 eee a. item the gua. —— a ye MOP Seer tate Paes eC yaw : - Approved: Fo sei'2004/03i: + aK0) pproved For Release! 2001/03/26 : ClA-RDP96-00787R000500130081-6 | ee a be OW wi ag: Gder Sess ead Tas VEL Ga We F..
Appiqved FoNgetéase 20UNGEASOIFREDRDP9e%07878 riludasecoos PS AF CHART } ACTIVITY CODES S/T] NAME OF INSTALLATION “Teee erence Moacnten's Ast PF —— CONTROL NO. SOURCE cra /OSI-RA/61-11 EVAL © D ae, : TNTITEIC NTE 1 Rp APOTT ATD FIRM NO. re | LOCATI “Te : Lp? KUT SK. PRINCIPAL RADIOTELESCOPES OF THE SOVIET UNION OVER SIBERIAN INSTITUTE OF TERRESTRIAL MAGNETISM, THE TONOSPHERE, AND RADIOWAVE PROPAGATION Alternate Name: Subordinate to: Rastern. Siberian Branch, Academy of Sciences, USSR Location: Irkutsk 52° N- 104° E Functional Description Engages in solar, cosmic ray, ionospheric, and geomagnetic research . Technical Description Personalities Other Information pproved For Release 2001/03/26 : CIA-RDP96-00787R0005001 F . ORM ANA oce pRevIOUS EDITIONS.