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Protons in near earth orbit

Authors :
J. Alcaraz
D. Alvisi
B. Alpat
G. Ambrosi
H. Anderhub
L. Ao
A. Arefiev
P. Azzarello
E. Babucci
L. Baldini
M. Basile
D. Barancourt
F. Barao
G. Barbier
G. Barreira
R. Battiston
R. Becker
U. Becker
L. Bellagamba
P. Béné
J. Berdugo
P. Berges
B. Bertucci
A. Biland
S. Bizzaglia
S. Blasko
G. Boella
M. Boschini
M. Bourquin
G. Bruni
M. Buenerd
J.D. Burger
W.J. Burger
X.D. Cai
R. Cavalletti
C. Camps
P. Cannarsa
M. Capell
D. Casadei
J. Casaus
G. Castellini
Y.H. Chang
H.F. Chen
H.S. Chen
Z.G. Chen
N.A. Chernoplekov
A. Chiarini
T.H. Chiueh
Y.L. Chuang
F. Cindolo
V. Commichau
A. Contin
A. Cotta–Ramusino
P. Crespo
M. Cristinziani
J.P. da Cunha
T.S. Dai
J.D. Deus
N. Dinu
L. Djambazov
I. D'Antone
Z.R. Dong
P. Emonet
J. Engelberg
F.J. Eppling
T. Eronen
G. Esposito
P. Extermann
J. Favier
C.C. Feng
E. Fiandrini
F. Finelli
P.H. Fisher
R. Flaminio
G. Fluegge
N. Fouque
Yu. Galaktionov
M. Gervasi
P. Giusti
D. Grandi
W.Q. Gu
K. Hangarter
A. Hasan
V. Hermel
H. Hofer
M.A. Huang
W. Hungerford
M. Ionica
R. Ionica
M. Jongmanns
K. Karlamaa
W. Karpinski
G. Kenney
J. Kenny
W. Kim
A. Klimentov
R. Kossakowski
V. Koutsenko
G. Laborie
T. Laitinen
G. Lamanna
G. Laurenti
A. Lebedev
S.C. Lee
G. Levi
P. Levtchenko
C.L. Liu
H.T. Liu
M. Lolli
I. Lopes
G. Lu
Y.S. Lu
K. Lübelsmeyer
D. Luckey
W. Lustermann
C. Maña
A. Margotti
F. Massera
F. Mayet
R.R. McNeil
B. Meillon
M. Menichelli
F. Mezzanotte
R. Mezzenga
A. Mihul
G. Molinari
A. Mourao
A. Mujunen
F. Palmonari
G. Pancaldi
A. Papi
I.H. Park
M. Pauluzzi
F. Pauss
E. Perrin
A. Pesci
A. Pevsner
R. Pilastrini
M. Pimenta
V. Plyaskin
V. Pojidaev
H. Postema
V. Postolache
E. Prati
N. Produit
P.G. Rancoita
D. Rapin
F. Raupach
S. Recupero
D. Ren
Z. Ren
M. Ribordy
J.P. Richeux
E. Riihonen
J. Ritakari
U. Roeser
C. Roissin
R. Sagdeev
D. Santos
G. Sartorelli
A. Schultz von Dratzig
G. Schwering
E.S. Seo
V. Shoutko
E. Shoumilov
R. Siedling
D. Son
T. Song
M. Steuer
G.S. Sun
H. Suter
X.W. Tang
Samuel C.C. Ting
S.M. Ting
M. Tornikoski
G. Torromeo
J. Torsti
J. Trümper
J. Ulbricht
S. Urpo
I. Usoskin
E. Valtonen
J. Vandenhirtz
F. Velcea
E. Velikhov
B. Verlaat
I. Vetlitsky
F. Vezzu
J.P. Vialle
G. Viertel
D. Vité
H. Von Gunten
S. Waldmeier Wicki
W. Wallraff
B.C. Wang
J.Z. Wang
Y.H. Wang
K. Wiik
C. Williams
S.X. Wu
P.C. Xia
J.L. Yan
L.G. Yan
C.G. Yang
M. Yang
S.W. Ye
P. Yeh
Z.Z. Xu
H.Y. Zhang
Z.P. Zhang
D.X. Zhao
G.Y. Zhu
W.Z. Zhu
H.L. Zhuang
A. Zichichi
Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'Annecy de Physique des Particules (LAPP)
Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)
AMS
Alcaraz, J
Alvisi, D
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
Béné, P
Berdugo, J
Berges, P
Bertucci, B
Biland, A
Bizzaglia, S
Blasko, S
Boella, G
Boschini, M
Bourquin, M
Bruni, G
Buenerd, M
Burger, J
Burger, W
Cai, X
Cavalletti, R
Camps, C
Cannarsa, P
Capell, M
Casadei, D
Casaus, J
Castellini, G
Chang, Y
Chen, H
Chen, Z
Chernoplekov, N
Chiarini, A
Chiueh, T
Chuang, Y
Cindolo, F
Commichau, V
Contin, A
Cotta–ramusino, A
Crespo, P
Cristinziani, M
Cunha, J
Dai, T
Deus, J
Dinu, N
Djambazov, L
D'Antone, I
Dong, Z
Emonet, P
Engelberg, J
Eppling, F
Eronen, T
Esposito, G
Extermann, P
Favier, J
Feng, C
Fiandrini, E
Finelli, F
Fisher, P
Flaminio, R
Fluegge, G
Fouque, N
Galaktionov, Y
Gervasi, M
Giusti, P
Grandi, D
Gu, W
Hangarter, K
Hasan, A
Hermel, V
Hofer, H
Huang, M
Hungerford, W
Ionica, M
Ionica, R
Jongmanns, M
Karlamaa, K
Karpinski, W
Kenney, G
Kenny, J
Kim, W
Klimentov, A
Kossakowski, R
Koutsenko, V
Laborie, G
Laitinen, T
Lamanna, G
Laurenti, G
Lebedev, A
Lee, S
Levi, G
Levtchenko, P
Liu, C
Liu, H
Lolli, M
Lopes, I
Lu, G
Lu, Y
Lübelsmeyer, K
Luckey, D
Lustermann, W
Maña, C
Margotti, A
Massera, F
Mayet, F
Mcneil, R
Meillon, B
Menichelli, M
Mezzanotte, F
Mezzenga, R
Mihul, A
Molinari, G
Mourao, A
Mujunen, A
Palmonari, F
Pancaldi, G
Papi, A
Park, I
Pauluzzi, M
Pauss, F
Perrin, E
Pesci, A
Pevsner, A
Pilastrini, R
Pimenta, M
Plyaskin, V
Pojidaev, V
Postema, H
Postolache, V
Prati, E
Produit, N
Rancoita, P
Rapin, D
Raupach, F
Recupero, S
Ren, D
Ren, Z
Ribordy, M
Richeux, J
Riihonen, E
Ritakari, J
Roeser, U
Roissin, C
Sagdeev, R
Santos, D
Sartorelli, G
Dratzig, A
Schwering, G
Seo, E
Shoutko, V
Shoumilov, E
Siedling, R
Son, D
Song, T
Steuer, M
Sun, G
Suter, H
Tang, X
Ting, S
Tornikoski, M
Torromeo, G
Torsti, J
Trümper, J
Ulbricht, J
Urpo, S
Usoskin, I
Valtonen, E
Vandenhirtz, J
Velcea, F
Velikhov, E
Verlaat, B
Vetlitsky, I
Vezzu, F
Vialle, J
Viertel, G
Vité, D
Gunten, H
Wicki, S
Wallraff, W
Wang, B
Wang, J
Wang, Y
Wiik, K
Williams, C
Wu, S
Xia, P
Yan, J
Yan, L
Yang, C
Yang, M
Ye, S
Yeh, P
Xu, Z
Zhang, H
Zhang, Z
Zhao, D
Zhu, G
Zhu, W
Zhuang, H
Zichichi, A
Source :
Physics Letters B, Physics Letters B, Elsevier, 2000, 472, pp.215-226, HAL
Publication Year :
2000

Abstract

The proton spectrum in the kinetic energy range 0.1 to 200 GeV was measured by the Alpha Magnetic Spectrometer (AMS) during space shuttle flight STS-91 at an altitude of 380 km. Above the geomagnetic cutoff the observed spectrum is parameterized by a power law. Below the geomagnetic cutoff a substantial second spectrum was observed concentrated at equatorial latitudes with a flux ~ 70 m^-2 sec^-1 sr^-1. Most of these second spectrum protons follow a complicated trajectory and originate from a restricted geographic region.<br />19 pages, Latex, 7 .eps figures

Details

Language :
English
ISSN :
03702693
Database :
OpenAIRE
Journal :
Physics Letters B, Physics Letters B, Elsevier, 2000, 472, pp.215-226, HAL
Accession number :
edsair.doi.dedup.....3eda329a4919a3b6e8b4eb7b24caf890