Measurements with TRACER: Discussion of results and future prospects

D. Müller; M. Ave; P. J. Boyle; F. Gahbauer; C. Höppner; J. Hörandel; M. Ichimura; A. Romero-Wolf; S. Wakely

Measurements with TRACER: Discussion of results and future prospects

D. Müller^*
, M. Ave
, P. J. Boyle
, F. Gahbauer
, C. Höppner
, J. Hörandel
, M. Ichimura
, A. Romero-Wolf
, S. Wakely

^*Šī darba korespondējošais autors

The University of Chicago
Karlsruhe Institute of Technology
Hirosaki University

Zinātniskās darbības rezultāts: Devums konferencē › Konferences raksts › koleģiāli recenzēts

18 Atsauces (Scopus)

Kopsavilkums

The individual energy spectra and relative abundances measured with TRACER, are compared with previous measurements in space and balloons, and with interpretations of air shower data. From the individual spectral slopes, we discuss constraints on models of cosmic-ray propagation through the galaxy. We also discuss the extrapolated high-energy abundances of the elements at the cosmic ray sources. The TRACER instrument is currently being refurbished for a second long duration balloon flight. The dynamic range of the measurement will then be extended to include the lighter cosmic ray nuclei, down to boron (Z = 5).

Oriģinālvaloda	Angļu
Lapas	89-92
Lapu skaits	4
Publikācijas statuss	Publicēts - 2005
Ārēji publicēts	Jā
Pasākums	29th International Cosmic Ray Conference, ICRC 2005 - Pune, Indija Ilgums: 3 aug. 2005 → 10 aug. 2005

Konference

Konference	29th International Cosmic Ray Conference, ICRC 2005
Valsts/Teritorija	Indija
Pilsēta	Pune
Periods	3/08/05 → 10/08/05

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title = "Measurements with TRACER: Discussion of results and future prospects",

abstract = "The individual energy spectra and relative abundances measured with TRACER, are compared with previous measurements in space and balloons, and with interpretations of air shower data. From the individual spectral slopes, we discuss constraints on models of cosmic-ray propagation through the galaxy. We also discuss the extrapolated high-energy abundances of the elements at the cosmic ray sources. The TRACER instrument is currently being refurbished for a second long duration balloon flight. The dynamic range of the measurement will then be extended to include the lighter cosmic ray nuclei, down to boron (Z = 5).",

author = "D. M{\"u}ller and M. Ave and Boyle, \{P. J.\} and F. Gahbauer and C. H{\"o}ppner and J. H{\"o}randel and M. Ichimura and A. Romero-Wolf and S. Wakely",

year = "2005",

language = "English",

pages = "89--92",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

TY - CONF

T1 - Measurements with TRACER

T2 - 29th International Cosmic Ray Conference, ICRC 2005

AU - Müller, D.

AU - Ave, M.

AU - Boyle, P. J.

AU - Gahbauer, F.

AU - Höppner, C.

AU - Hörandel, J.

AU - Ichimura, M.

AU - Romero-Wolf, A.

AU - Wakely, S.

PY - 2005

Y1 - 2005

N2 - The individual energy spectra and relative abundances measured with TRACER, are compared with previous measurements in space and balloons, and with interpretations of air shower data. From the individual spectral slopes, we discuss constraints on models of cosmic-ray propagation through the galaxy. We also discuss the extrapolated high-energy abundances of the elements at the cosmic ray sources. The TRACER instrument is currently being refurbished for a second long duration balloon flight. The dynamic range of the measurement will then be extended to include the lighter cosmic ray nuclei, down to boron (Z = 5).

AB - The individual energy spectra and relative abundances measured with TRACER, are compared with previous measurements in space and balloons, and with interpretations of air shower data. From the individual spectral slopes, we discuss constraints on models of cosmic-ray propagation through the galaxy. We also discuss the extrapolated high-energy abundances of the elements at the cosmic ray sources. The TRACER instrument is currently being refurbished for a second long duration balloon flight. The dynamic range of the measurement will then be extended to include the lighter cosmic ray nuclei, down to boron (Z = 5).

UR - https://www.scopus.com/pages/publications/84898982535

M3 - Paper

AN - SCOPUS:84898982535

SP - 89

EP - 92

Y2 - 3 August 2005 through 10 August 2005

ER -

Measurements with TRACER: Discussion of results and future prospects

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