The ARGO program consists of a balloon-borne mm and sub-mm telescope, devoted to the observation of diffuse radiation in the wavelength range between 2 mm and 300 mum, at angular scales between 10' and 5-degrees. We review here the impact of such observations in different fields ranging from Atmospheric Physics to Cosmology. We also quote the results obtained from ARGO's first flight in 1989, and we describe the improved version of ARGO we are currently developing.

Debernardis, P., Deluca, A., DE PETRIS, M., Epifani, M., Gervasi, M., Maoli, R., et al. (1992). THE ARGO PROJECT - SCIENTIFIC TARGETS, 1ST RESULTS AND FUTURE PERSPECTIVES. IL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. C, GEOPHYSICS AND SPACE PHYSICS, 15(6), 993-1011 [10.1007/BF02506691].

THE ARGO PROJECT - SCIENTIFIC TARGETS, 1ST RESULTS AND FUTURE PERSPECTIVES

GERVASI, MASSIMO;
1992

Abstract

The ARGO program consists of a balloon-borne mm and sub-mm telescope, devoted to the observation of diffuse radiation in the wavelength range between 2 mm and 300 mum, at angular scales between 10' and 5-degrees. We review here the impact of such observations in different fields ranging from Atmospheric Physics to Cosmology. We also quote the results obtained from ARGO's first flight in 1989, and we describe the improved version of ARGO we are currently developing.
No
Articolo in rivista - Articolo scientifico
Scientifica
Background radiation, Astronomical observation: far infrared, Astronomical and Space-research instrumantation
English
993
1011
19
Debernardis, P., Deluca, A., DE PETRIS, M., Epifani, M., Gervasi, M., Maoli, R., et al. (1992). THE ARGO PROJECT - SCIENTIFIC TARGETS, 1ST RESULTS AND FUTURE PERSPECTIVES. IL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. C, GEOPHYSICS AND SPACE PHYSICS, 15(6), 993-1011 [10.1007/BF02506691].
Debernardis, P; Deluca, A; DE PETRIS, M; Epifani, M; Gervasi, M; Maoli, R; Masi, S
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/10281/34245
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