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On the way to the determination of the cosmic ray mass composition by the Pierre Auger fluorescence detector: The 'minimum momentum method'

Conference Paper
Publication Date:
2003
Short description:
On the way to the determination of the cosmic ray mass composition by the Pierre Auger fluorescence detector: The 'minimum momentum method' / Aramo, C., Ambrosio, M., Donalek, C., D'Urso, D., Erlykin, A.D., Guarino, F., Insolia, A., Longo, G., Tagliaferri, R.. - (2003), pp. 13-19. (Thinking, Observing and Mining the Universe Sorrento, Italy 22-27 Sep 2003).
abstract:
We propose a possible approach for the determination of very high energy
cosmic ray primary mass A based on the information provided by the
reconstruction of shower longitudinal development in the Earth
atmosphere. We refer to an apparatus such as the Pierre Auger
Observatory, which is a unique "hybrid" UHECR detector. The surface
detector (SD) and air fluorescence detector (FD) of the observatory are
designed for observation of cosmic ray showers in coincidence, with a
10% duty cycle, with resulting data expected to be superior in quality
especially for the primary energy E-0 which is determined with a 5%
accuracy. We present results obtained using an approach for the
determination of A in the individual event based on only FD information
(MMM - 'Minimum Momentum Method'). This approach shows that, if the
entire information contained in the longitudinal profile is exploited,
reliable results may be obtained.
Iris type:
4.1 Contributo in Atti di convegno
List of contributors:
Aramo, C.; Ambrosio, M.; Donalek, C.; D'Urso, D.; Erlykin, A. D.; Guarino, F.; Insolia, A.; Longo, G.; Tagliaferri, R.
Authors of the University:
D'URSO Domenico
Handle:
https://iris.uniss.it/handle/11388/211772
Book title:
Thinking, Observing and Mining the Universe
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