Sökning: onr:"swepub:oai:DiVA.org:kth-41927" > Relative nuclear ab...
Fältnamn | Indikatorer | Metadata |
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000 | 03082naa a2200673 4500 | |
001 | oai:DiVA.org:kth-41927 | |
003 | SwePub | |
008 | 111003s2006 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-419272 URI |
024 | 7 | a https://doi.org/10.1016/j.asr.2006.02.0502 DOI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Casolino, M.4 aut |
245 | 1 0 | a Relative nuclear abundances inside ISS with Sileye-3/Alteino experiment |
264 | 1 | b Elsevier BV,c 2006 |
338 | a print2 rdacarrier | |
500 | a QC 20111003 | |
520 | a The experiment Sileye-3/Alteino was first operational on board the international Space Station between 27/4 and 1/5/2002. It is constituted of a cosmic ray silicon detector and an electroencephalograph and is used to monitor radiation environment and study the light flash phenomenon in space. As a stand-alone device, Sileye-3/Alteino can monitor in real time cosmic ray nuclei. In this work, we report on relative nuclear abundance measurements in different regions of the orbit for nuclei from B to Fe in the energy range above similar or equal to 60 Mev/n. Abundances of nuclei such as 0 and Ne relative to C are found to be increased in respect to particle composition outside of the station, whereas the Fe group is reduced. This effect could be ascribed to nuclear interactions with the hull of the station. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a cosmic rays | |
653 | a nuclear abundances | |
653 | a International Space Station | |
700 | 1 | a Bidoll, V.4 aut |
700 | 1 | a Minori, M.4 aut |
700 | 1 | a Narici, L.4 aut |
700 | 1 | a De Pascale, M. P.4 aut |
700 | 1 | a Picozza, P.4 aut |
700 | 1 | a Reall, E.4 aut |
700 | 1 | a Zaconte, V.4 aut |
700 | 1 | a Fuglesang, Christer4 aut |
700 | 1 | a Vittori, R.4 aut |
700 | 1 | a Carlson, Peru KTH,Partikel- och astropartikelfysik4 aut0 (Swepub:kth)u1ua4u32 |
700 | 1 | a Galper, A.4 aut |
700 | 1 | a Korotkov, M.4 aut |
700 | 1 | a Popov, A.4 aut |
700 | 1 | a Vavilov, N.4 aut |
700 | 1 | a Avdeev, S.4 aut |
700 | 1 | a Berighin, V.4 aut |
700 | 1 | a Petrov, V. P.4 aut |
700 | 1 | a Salnitskii, V. P.4 aut |
700 | 1 | a Shevchenko, O. I.4 aut |
700 | 1 | a Trukhanov, K. A.4 aut |
700 | 1 | a Shurshakov, K. A.4 aut |
700 | 1 | a Boezio, M.4 aut |
700 | 1 | a Bonvicini, W.4 aut |
700 | 1 | a Vacchi, A.4 aut |
700 | 1 | a Zampa, G.4 aut |
700 | 1 | a Zarnpa, N.4 aut |
700 | 1 | a Mazzenga, G.4 aut |
700 | 1 | a Ricci, M.4 aut |
700 | 1 | a Spillantini, P.4 aut |
710 | 2 | a KTHb Partikel- och astropartikelfysik4 org |
773 | 0 | t Advances in Space Researchd : Elsevier BVg 37:9, s. 1685-1690q 37:9<1685-1690x 0273-1177x 1879-1948 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-41927 |
856 | 4 8 | u https://doi.org/10.1016/j.asr.2006.02.050 |
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