http://www.cnr.it/ontology/cnr/individuo/prodotto/ID5792
The atmospheric nightglow in the 300-400 nm wavelength. Results by the balloon-borne experiment BABY (Articolo in rivista)
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- Label
- The atmospheric nightglow in the 300-400 nm wavelength. Results by the balloon-borne experiment BABY (Articolo in rivista) (literal)
- Anno
- 2002-01-01T00:00:00+01:00 (literal)
- Alternative label
Catalano O., Agnetta A., Biondo B., Celi F., Di Raffaele R., Giarrusso S., Linsley J., La Rosa G., Lo Bue A., Mangano A., Russo F. (2002)
The atmospheric nightglow in the 300-400 nm wavelength. Results by the balloon-borne experiment BABY
(literal)
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- Catalano O., Agnetta A., Biondo B., Celi F., Di Raffaele R., Giarrusso S., Linsley J., La Rosa G., Lo Bue A., Mangano A., Russo F. (literal)
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- Presentazione dellesperimento chiamato Background Bypass (BABY) per la misura del background UV durante un volo transmediterraneo avvenuto nellestate del 1998. (literal)
- Note
- ISI Web of Science (WOS) (literal)
- Titolo
- The atmospheric nightglow in the 300-400 nm wavelength. Results by the balloon-borne experiment BABY (literal)
- Abstract
- The balloon-borne experiment, named BAckground BYpass (BABY) belongs to a
wider program that has as its final goal the detection and study of high-
energy cosmic rays from space (satellite, Space Station). An information
of fundamental importance for this class of projects concerns the
nighttime background light. The instrument designed to detect fluorescence
photons is basically composed of two collimated photomultipliers: a single
photon-counting PMT and a charge integration PMT. We briefly report the
details of the design, operation and performance of the detector, which
was designed and completely built at the IFCAICNR Institute in Palermo.
Preliminary analysis and results of the nocturnal background in the range
of 300 are presented for the whole duration of the flight during the
1998 Mediterranean balloon flight campaign. A substantial part of the
flight was at night over the sea.
(literal)
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