Measurement of the antiproton to proton ratio in cosmic rays using the Moon shadow with the L3+C detector

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dc.creatorPARRIAUD, J. F.
dc.date2002-10-15
dc.date.accessioned2026-07-07T02:05:43Z
dc.date.available2026-07-07T02:05:43Z
dc.descriptionThe observation of the Moon shadow effect with the L3+C detector is reported. The expected offset and elongation of the Moon shadow due to the geomagnetic field are clearly observed. A determination of the angular resolution and pointing error has beem performed through this observation. A preliminary upper limit of the antiproton to proton ratio in cosmic rays is given in the TeV region.
dc.descriptionpresented at "Rencontres de Blois 2002" 4 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0210334
dc.identifierhttp://arxiv.org/abs/astro-ph/0210334
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5186
dc.subjectAstrophysics
dc.titleMeasurement of the antiproton to proton ratio in cosmic rays using the Moon shadow with the L3+C detector
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