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THE USE OF BALLOONS IN ASTRONOMICAL RESEARCH.HILLIER RR.1975; J. BRIT. INTERPLANET. SOC.; G.B.; DA. 1975; VOL. 28; NO 12; PP. 810-815Article

SPACE OBSERVATIONS OF THE ZODIACAL LIGHT.WEINBERG JL.1976; LECTURE NOTES PHYS.; GERM.; DA. 1976; VOL. 48; PP. 3-18; BIBL. 2 P. 1/2; (INTERPLANET. DUST ZODIACAL LIGHT. PROC. IAU-COLL. 31; HEIDELBERG; 1975)Conference Paper

TROPOSPHERIC GRAVITY WAVES: THEIR DETECTION BY AN INFLUENCE ON RAWINSONDE BALLOON DATALALAS DP; EINAUDI F.1980; Q. J. R. METEOROL. SOC.; ISSN 0035-9009; GBR; DA. 1980; VOL. 106; NO 450; PP. 855-864; BIBL. 21 REF.Article

SBARMO, ITS SCIENTIFIC AIMS AND ITS ORGANISATION.DE FEITER LD.1976; S.B.A.R.M.O. BULL.; FR.; DA. 1976; VOL. 6; NO 3; PP. 147-151Article

A BALLOON-BORNE IONIZATION SPECTROMETER WITH VERY LARGE APERTURE FOR THE DETECTION OF HIGH ENERGY COSMIC RAYS.ATALLAH K; CLEGHORN TF; MODLINGER A et al.1975; NUCL. INSTRUM. METHODS; NETHERL.; DA. 1975; VOL. 124; NO 2; PP. 461-476; BIBL. 9 REF.Article

THE SPECTRUM OF COSMIC ELECTRONS WITH ENERGIES BETWEEN 6 AND 100 GEV.MEEGAN CA; EARL JA.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 1; PP. 419-424; BIBL. 8 REF.Conference Paper

ASTROPHYSICAL IMPLICATIONS OF THE ISOTOPIC COMPOSITION OF COSMIC RAYS.MAEHL R; HAGEN FA; FISHER AJ et al.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 1; PP. 367-372; BIBL. 7 REF.Conference Paper

RESULTS ON THE COSMIC RAY CHEMICAL COMPOSITION AT ENERGIES UP TO 100 GEV/NUCL.SCHMIDT WKH; ATALLAH K; CLEGHORN TF et al.1976; ASTR. AND ASTROPHYS.; GERM.; DA. 1976; VOL. 46; NO 1; PP. 49-59; BIBL. 14 REF.Article

MEASUREMENT OF THE PRIMARY COSMIC ELECTRON SPECTRUM.SILVERBERG RF.1975; G.S.F.C.-X-661-75-218; U.S.A.; DA. 1975; PP. 1-25; BIBL. 2 P. 1/2Report

MEASUREMENTS OF 3HE AND 4HE NUCLEI USING A BALLOON BORNE TELESCOPE.WEBBER WR; SCHOFIELD NJ.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 1; PP. 312-317; BIBL. 15 REF.Conference Paper

A COSMIC GAMMA-RAY BURST ON 1975 MAY 14.HERZO D; DAYTON B; ZYCH AD et al.1976; ASTROPHYS. J.; U.S.A.; DA. 1976; VOL. 203; NO 3 PART. 2; PP. L115-L118; BIBL. 14 REF.Article

INTENSITY OF PRIMARY ELECTRONS ABOVE 10 GEV.FREIER P; GILMAN C; WADDINGTON CJ et al.sdIN: INT. COSMIC RAY CONF. 14; MUENCHEN; 1975; MUENCHEN; MAX PLANCK INST.; DA. S.D.; VOL. 1; PP. 425-430; BIBL. 11 REF.Conference Paper

OBSERVATION DES RAYONS COSMIQUES SOLAIRES DURANT L'ERUPTION DU 29 AVRIL 1973BAZILEVSKAYA GA; KURNOSOVA LV; LOGACHEV VI et al.1976; IZVEST. AKAD. NAUK S.S.S.R., SER. FIZ.; S.S.S.R.; DA. 1976; VOL. 40; NO 3; PP. 457-461; BIBL. 4 REF.; (KORPUSK. POTOKI SOLNTSA RADIATS. POYASA ZEMLI YUPITERA. MEZHDUNAR. SEMIN. 7. MATER.; LENINGRAD; 1975)Conference Paper

MESURES DES RAYONNEMENTS GAMME SECONDAIRES SUR DES AEROSTATS A HAUTE ALTITUDE ET DES STATIONS ORBITALESIYUDIN AF; OZEROV YU V.1975; KOSM. ISSLEDOV.; S.S.S.R.; DA. 1975; VOL. 13; NO 4; PP. 609-611; BIBL. 13 REF.Article

THE ENERGY SPECTRUM OF COSMIC RAY ELECTRONS BETWEEN 10 AND 1000 GEV.ANAND KC; DANIEL RR; STEPHENS SA et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 36; NO 1; PP. 169-175; BIBL. 17 REF.Article

A COMPARISON BETWEEN NIMBUS 5 THIR AND ITPR TEMPERATURES AND DERIVED WINDS WITH RAWINSONDE DATA OBTAINED IN THE AVE II EXPERIMENT.ARNOLD JE; SCOGGINS JR; FUELBERG HE et al.sdIN: CONF. AEROSP. AERONAUT. METEOROL. 7. SYMP. REMOTE SENSING SATELL.; MELBOURNE, FLA.; 1976; BOSTON; AM. METEOROL. SOC.; DA. S.D.; PP. 276-283; BIBL. 7 REF.Conference Paper

ADVANCES IN GAMMA-RAY BURST ASTRONOMY.CLINE TL; DESAI UD.1976; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1976; VOL. 42; NO 1; PP. 17-27; BIBL. 9 REF.Article

ATMOSPHERIC TIDAL MEASUREMENTS AT 50KM FROM A CONSTANT-ALTITUDE BALLOONBALLARD HN; BEYERS NJ; MIERS BT et al.1972; J. APPL. METEOROL.; U.S.A.; DA. 1972; VOL. 11; NO 7; PP. 1138-1149; BIBL. 16REF.Serial Issue

BALLOON RESEARCH1977; SPACE RES.; NLD; DA. 1977; VOL. 17; PP. 777-832; BIBL. DISSEM.Conference Paper

HIGH-LEVEL CIRCULATION STUDIES BASED ON RAWINSONDE, ROCKETSONDE AND SATELLITE OBSERVATIONS.FINGER FG; GELMAN ME; MCINTURFF RM et al.1974; SPACE RES.; NETHERL.; DA. 1974; VOL. 14; PP. 17-29; BIBL. 9 REF.; (OPEN MEET. WORK. GROUPS 16TH PLENARY MEET. COSPAR. PROC.; CONSTANCE; 1973)Conference Paper

WIND MEASUREMENT TECHNIQUES AVAILABLE FOR THE MIDDLE ATMOSPHERE PROGRAMGAGE KS; VANZANDT TE.1981; J. GEOPHYS. RES.; ISSN 0022-1406; USA; DA. 1981; VOL. 86; NO C10; PP. 9591-9598; BIBL. 40 REF.Conference Paper

DIE DIFFUSE KOSMISCHE GAMMASTRAHLUNG. = LE RAYONNEMENT GAMMA COSMIQUE DIFFUSSCHOENFELDER V.1975; FORTSCHR. D. PHYS.; DTSCH.; DA. 1975; VOL. 23; NO 1; PP. 1-69; BIBL. 2 P. 1/2Article

L'ANALYSE DES COMPOSANTS DE LA HAUTE ATMOSPHERENAUDET JP.1979; ORION; CHE; DA. 1979; VOL. 37; NO 170; PP. 4-8; ABS. GERArticle

HIGH RESOLUTION INFRARED SOLAR OBSERVATIONS BY BALLOON.ZANDER R.1976; INFRARED PHYS.; G.B.; DA. 1976; VOL. 16; NO 1-2; PP. 125-127; BIBL. 9 REF.; (INT. CONF. INFRARED PHYS., PROC.; ZURICH; 1975)Conference Paper

PHOTOMETRY OF THE ZODIACAL LIGHT WITH THE BALLOON-BORNE TELESCOPE THISBEHOFMANN W; FREY A; LEMKE D et al.1976; LECTURE NOTES PHYS.; GERM.; DA. 1976; VOL. 48; PP. 52; BIBL. 2 REF.; (INTERPLANET. DUST ZODIACAL LIGHT. PROC.; IAU-COLLOQ. 31; HEIDELBERG; 1975)Conference Paper

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