ON THE DETECTION OF H₂ FROM INTERSTELLAR CLOUDS IN THE WAVELENGTH RANGE 4.4MU RO 28.2MUBUSSOLETTI E.1973; ASTR. AND ASTROPHYS.; GERM.; DA. 1973; VOL. 23; NO 1; PP. 125-129; BIBL. 27REF.Serial Issue

HIGH RESOLUTION SPECTRA OF THE STRATOSPHERE BETWEEN 30 AND 200 CM^-1BALUTEAU JP; BUSSOLETTI E.1973; NATURE PHYS. SCI.; G.B.; DA. 1973; VOL. 241; NO 105; PP. 113-114; BIBL. 14 REF.Serial Issue

THE TEMPERATURE OF INTERSTELLAR POROUS GRAINSBLANCO A; BUSSOLETTI E.1980; ASTROPHYS. SPACE SCI.; NLD; DA. 1980; VOL. 67; NO 1; PP. 105-110; BIBL. 12 REF.Article

HIGH RESOLUTION SPECTRA OF THE STRATOSPHERE BETWEEN 30 AND 200 CM^-1.BALUTEAU JP; BUSSOLETTI E.1975; SPACE RES.; NETHERL.; DA. 1975; VOL. 15; PP. 131-137; BIBL. 14 REF.; (PLENARY MEET. COSPAR. 7. PROC. OPEN MEET. WORK. GROUPS PHYS. SCI; SAO PAULO, S.P.; 1974)Conference Paper

RELATIONSHIPS BETWEEN THE ENHANCED DIURNAL VARIATION OF COSMIC RAYS AND THE INTERPLANETARY MAGNETIC FIELD.BUSSOLETTI E; D'AMBROGIO G.1975; LETTERE NUOVO CIMENTO.; ITAL.; DA. 1975; VOL. 13; NO 6; PP. 209-212; BIBL. DISSEM.Article

THE EQUATORIAL ANISOTROPY OF THE COSMIC RAYS AND ITS CORRELATIONS WITH THE INTERPLANETARY MAGNETIC FIELD, FOR 1965-1966BUSSOLETTI E; IUCCI N.sdIN: COSMIC RAYS. 12TH INT. CONF. HOBART, TASMANIA, AUST., 1971; HOBART, TASMANIA; MERCURY-WALCH; DA. S.D.; VOL. 2; PP. 595Conference Paper

INFRARED EFFICIENCY FACTORS FOR TWENTY MATERIALS WHICH ARE CANDIDATES FOR INTERSTELLAR DUST.BUSSOLETTI E; ZAMBETTA AM.1976; ASTR. AND ASTROPHYS., SUPPL. SER.; GERM.; DA. 1976; VOL. 25; NO 3; PP. 549-570; BIBL. 34 REF.Article

NUBI FREDDE E GRANI INTERSTELLARI. = NUAGES FROIDS ET GRAINS INTERSTELLAIRESBUSSOLETTI E; BORGHESI A.1976; MEM. SOC. ASTR. ITAL.; ITAL.; DA. 1976 PARU 1977; VOL. 47; NO 2; PP. 125-158; BIBL. 2 P.Article

DIFFUSION PROCESSES OF COSMIC RAYS WITH ENERGIES BETWEEN 2 AND 20 GV DURING FORBUSH DECREASES: THE DIURNAL EFFECTBUSSOLETTI E; GERANIOS A.1972; NUOVO CIMENTO, B; ITAL.; DA. 1972; VOL. 11; NO 1; PP. 53-67; ABS. ITAL. RUSSE; BIBL. DISSEM.Serial Issue

THE DIURNAL EFFECT OF COSMIC RAYS AND ITS DEPENDANCE ON THE INTERPLANETARY MAGNETIC FIELDBUSSOLETTI E; IUCCI N.1972; IN: COSMIC PLASMA PHYS. PROC. CONF. FRASCATI, ITALY, 1971; NEW YORK; PLENUM PRESS; DA. 1972; PP. 359-364; BIBL. 4REF.Conference Proceedings

THERMAL EMISSION SPECTRA OF SILICATES FROM PLANETARY NEBULAE.BUSSOLETTI E; BALUTEAU JP; EPCHTEIN N et al.1976; ASTROPHYS. SPACE SCI. LIBRARY; NETHERL.; DA. 1976; VOL. 55; PP. 133-141; BIBL. 15 REF.; (SOLID STATE ASTROPHYS. PROC. SYMP.; CARDIFF, WALES; 1974)Conference Paper

DETERMINATION OF ATMOSPHERIC PRECIPITABLE WATER VAPOUR AND TURBIDITY PARAMETERS FROM DIURNAL INFRARED HYGROMETER AND TURBIDIMETER DATABORGHESI A; BUSSOLETTI E; FALCICCHIA G et al.1982; INFRARED PHYS.; ISSN 0020-0891; GBR; DA. 1982; VOL. 22; NO 3; PP. 149-155; BIBL. 16 REF.Article

A TENTATIVE EVOLUTIONARY SEQUENCE FOR CARBON STARS DERIVED FROM CIRCUMSTELLAR SHELL PARAMETERSBUSSOLETTI E; ROSSI L; BLANCO A et al.1981; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1981; VOL. 76; NO 2; PP. 341-349; BIBL. 12 REF.Article

A SEARCH FOR CARBON STARS IN THE AFGL CATALOGUEALTAMORE A; SMRIGLIO F; BUSSOLETTI E et al.1980; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1980; VOL. 72; NO 1; PP. 159-165; BIBL. 10 REF.Article

THE 2200 A EXTINCTION HUMP AND POROUS GRAPHITE GRAINSBLANCO A; BORGHESI A; BUSSOLETTI E et al.1980; ASTROPHYS. SPACE SCI.; NLD; DA. 1980; VOL. 68; NO 2; PP. 505-508; BIBL. 11 REF.Article

MUTUAL RELATIONSHIPS BETWEEN ICE MANTLE AND SILICATE CORE PROPERTIES OF INTERSTELLAR GRAINSBUSSOLETTI E; BLANCO A; BORGHESI A et al.1978; MEM. SOC. ASTR. ITAL.; ITA; DA. 1978; VOL. 49; NO 1; PP. 251-260; BIBL. 15 REF.Conference Paper

A NEAR INFRARED PHOTOPOLARIMETER.BLANCO A; BUSSOLETTI E; MELCHIORRI B et al.1976; INFRARED PHYS.; G.B.; DA. 1976; VOL. 16; NO 5; PP. 569-575; BIBL. 3 REF.Article

Optical properties of carbonaceous materialsBUSSOLETTI, E; COLANGELI, L.Symposium - International astronomical union. 1989, Num 135, pp 147-153, issn 0074-1809Conference Paper

FAR IR EMISSION OF THE GALACTIC PLANE AT HIGH LONGITUDESBUSSOLETTI E; GUIDI J; MELCHIORRI F et al.1982; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1982; VOL. 105; NO 1; PP. 184-187; BIBL. 24 REF.Article

A SEARCH FOR S STARS IN THE IRC AND AFGL CATALOGUESBORGHESI A; BUSSOLETTI E; ROSSI L et al.1981; ASTROPHYS. SPACE SCI.; ISSN 0004-640X; NLD; DA. 1981; VOL. 79; NO 2; PP. 435-441; BIBL. 18 REF.Article

Cosmic dust: from space to laboratoryBUSSOLETTI, E; COLANGELI, L.Rivista del nuovo cimento. 1990, Vol 13, Num 12, issn 0035-5917, 70 p.Serial Issue

CONSIDERATIONS ABOUT THE ABSORPTION EFFICIENCY OF DUST PARTICLES IN THE INFRARED.BUSSOLETTI E; BORGHESI A; LEGGIERI G et al.1975; ASTROPHYS. SPACE SCI.; NETHERL.; DA. 1975; VOL. 34; NO 1; PP. 191-197; BIBL. 9 REF.Article

Simulation of cometary infrared spectra using laboratory extinction data of carbonaceous materialsCOLANGELI, L; BUSSOLETTI, E; PAPOULAR, R et al.Icarus (New York, NY). 1990, Vol 86, Num 1, pp 198-207, issn 0019-1035, 10 p.Conference Paper

Extinction spectra of amorphous carbon submicron grains in the UV-visible rangeCOLANGELI, L; CAPOZZI, V; BUSSOLETTI, E et al.Astronomy and astrophysics (Berlin. Print). 1986, Vol 168, Num 1-2, pp 349-353, issn 0004-6361Article

HIGH RESOLUTION INFRARED SPECTRA OF THE EARTH'S ATMOSPHERE III-AIRBORNE OBSERVATIONS IN THE 100-140 CM^-1 RANGE.BAWTEAU JP; MARTEN A; BUSSOLETTI E et al.1977; INFRARED PHYS.; G.B.; DA. 1977; VOL. 17; NO 4; PP. 283-291; BIBL. 18 REF.Article