DSpace at EWHA: A study of cosmic ray secondaries induced by the Mir space station using AMS-01

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A study of cosmic ray secondaries induced by the Mir space station using AMS-01

Title: A study of cosmic ray secondaries induced by the Mir space station using AMS-01

Authors: Aguilar M.; Alcaraz J.; Allaby J.; Alpat B.; Ambrosi G.; Anderhub H.; Ao L.; Arefiev A.; Azzarello P.; Babucci E.; Baldini L.; Basile M.; Barancourt D.; Barao F.; Barbier G.; Barreira G.; Battiston R.; Becker R.; Becker U.; Bellagamba L.; Bene P.; Berdugo J.; Berges P.; Bertucci B.; Biland A.; Bizzaglia S.; Blasko S.; Boella G.; Boschini M.; Bourquin M.; Brocco L.; Bruni G.; Buenerd M.; Burger J.D.; Burger W.J.; Cai X.D.; Camps C.; Cannarsa P.; Capell M.; Carosi G.; Casadei D.; Casaus J.; Castellini G.; Cecchi C.; Chang Y.H.; Chen H.F.; Chen H.S.; Chen Z.G.; Chernoplekov N.A.; Chiueh T.H.; Cho K.; Choi M.J.; Choi Y.Y.; Chuang Y.L.; Cindolo F.; Commichau V.; Contin A.; Cortina-Gil E.; Cristinziani M.; da Cunha J.P.; Dai T.S.; Delgado C.; Demirkoz B.; Deus J.D.; Dinu N.; Djambazov L.; D'Antone I.; Dong Z.R.; Emonet P.; Engelberg J.; Eppling F.J.; Eronen T.; Esposito G.; Extermann P.; Favier J.; Fiandrini E.; Fisher P.H.; Fluegge G.; Fouque N.; Galaktionov Y.; Gervasi M.; Giusti P.; Grandi D.; Grimm O.; Gu W.Q.; Hangarter K.; Hasan A.; Henning R.; Hermel V.; Hofer H.; Huang M.A.; Hungerford W.; Ionica M.; Ionica R.; Jongmanns M.; Karlamaa K.; Karpinski W.; Kenney G.; Kenny J.; Kim D.H.; Kim G.N.; Kim K.S.; Kim M.Y.; Klimentov A.; Kossakowski R.; Koutsenko V.; Kraeber M.; Laborie G.; Laitinen T.; Lamanna G.; Lanciotti E.; Laurenti G.; Lebedev A.; Lechanoine-Leluc C.; Lee M.W.; Lee S.C.; Levi G.; Levtchenko P.; Liu C.L.; Liu H.T.; Lopes I.; Lu G.; Lu Y.S.; Lubelsmeyer K.; Luckey D.; Lustermann W.; Mafia C.; Margotti A.; Mayet F.; McNeil R.R.; Meillon B.; Menichelli M.; Mihul A.; Monreal B.; Mourao A.; Mujunen A.; Palmonari F.; Papi A.; Park H.B.; Park W.H.; Pauluzzi M.; Pauss F.; Perrin E.; Pesci A.; Pevsner A.; Pimenta M.; Plyaskin V.; Pojidaev V.; Pohl M.; Postolache V.; Produit N.; Rancoita P.G.; Rapin D.; Raupach F.; Ren D.; Ren Z.; Ribordy M.; Richeux J.P.; Riihonen E.; Ritakari J.; Ro S.; Roeser U.; Rossin C.; Sagdeev R.; Santos D.; Sartorelli G.; Sbarra C.; Schael S.; Schultz von Dratzig A.; Schwering G.; Scolieri G.; Seo E.S.; Shin J.W.; Shoumilov E.; Shoutko V.; Siedling R.; Son D.; Song T.; Steuer M.; Sun G.S.; Suter H.; Tang X.W.; Ting S.C.C.; Ting S.M.; Tornikoski M.; Torsti J.; Trumper J.; Ulbricht J.; Urpo S.; Valtonen E.; Vandenhirtz J.; Velcea F.; Velikhov E.; Verlaat B.; Vetlitsky I.; Vezzu F.; Vialle J.P.; Viertel G.; Vite D.; von Gunten H.; Waldmeier Wicki S.; Wallraff W.; Wang B.C.; Wang J.Z.; Wang Y.H.; Wiik K.; Williams C.; Wu S.X.; Xia P.C.; Yan J.L.; Yan L.G.; Yang C.G.; Yang J.; Yang M.; Ye S.W.; Yeh P.; Xu Z.Z.; Zhang H.Y.; Zhang Z.P.; Zhao D.X.; Zhu G.Y.; Zhu W.Z.; Zhuang H.L.; Zichichi A.; Zimmermann B.; Zuccon P.

Ewha Authors: 양종만

SCOPUS Author ID: 양종만

Issue Date: 2005

Journal Title: Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms

ISSN: 0168-583X

Citation: Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms vol. 234, no. 3, pp. 321 - 332

Indexed: SCI; SCIE; SCOPUS

Document Type: Article

Abstract: The Alpha Magnetic Spectrometer (AMS-02) is a high energy particle physics experiment that will study cosmic rays in the ∼100 MeV to 1 TeV range and will be installed on the International Space Station (ISS) for at least 3 years. A first version of AMS-02, AMS-01, flew aboard the space shuttle Discovery from June 2 to June 12, 1998, and collected 10 8 cosmic ray triggers. Part of the Mir space station was within the AMS-01 field of view during the four day Mir docking phase of this flight. We have reconstructed an image of this part of the Mir space station using secondary π - and μ - emissions from primary cosmic rays interacting with Mir. This is the first time this reconstruction was performed in AMS-01, and it is important for understanding potential backgrounds during the 3 year AMS-02 mission. © 2005 Elsevier B.V. All rights reserved.