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O. Palamara

Researcher at University of Salento

Publications -  15
Citations -  677

O. Palamara is an academic researcher from University of Salento. The author has contributed to research in topics: Neutrino & Detector. The author has an hindex of 12, co-authored 15 publications receiving 662 citations.

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Journal ArticleDOI

Measurement of the atmospheric neutrino-induced upgoing muon flux using MACRO

M. Ambrosio, +135 more
- 27 Aug 1998 - 
TL;DR: In this article, a measurement of the flux of neutrino-induced upgoing muons ( ν >∼ 100 GeV) using the MACRO detector is presented, where the ratio of the observed to expected events integrated over all zenith angles is 0.74 ± 0.036 (stat) ±0.13 (theoretical).
Journal ArticleDOI

Seasonal variations in the underground muon intensity as seen by MACRO

M. Ambrosio, +133 more
TL;DR: In this article, the authors search for a correlation between variations in the underground muon rate, Nμ, and seasonal temperature variation in the atmosphere with high statistical significance and find that these correlations are present with high significance.
Journal ArticleDOI

The observation of up-going charged particles produced by high energy muons in underground detectors

M. Ambrosio, +128 more
TL;DR: In this article, an experimental study of the production of up-going charged particles in inelastic interactions of down-going underground muons is reported, using data obtained from the MACRO detector at the Gran Sasso Laboratory.
Journal ArticleDOI

Muon astronomy with the MACRO detector

Steven Ahlen, +129 more
TL;DR: In this article, the authors analyzed a sample of 1.8×10 6 muons with E μ ≥ 1.3 TeV collected by the first and second supermodules of the MACRO detector at Gran Sasso during the period 1989 February to 1991 February.
Journal ArticleDOI

High energy cosmic ray physics with underground muons in MACRO. II. Primary spectra and composition

M. Ambrosio, +118 more
- 01 Aug 1997 - 
TL;DR: In this article, the spectral indexes of the fitted energy spectrum are 2.56{plus_minus}0.05 for E{lt}500 TeV and 2.9{plus-minus} 0.3 for Elt}5000 TeV with a gradual change at intermediate energies.