The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment

S. Kodaira; M. Hareyama; N. Hasebe; T. Miyachi; K. Sakurai; W. R. Binns; J. R. Cummings; M. H. Israel; J. T. Link; B. F. Rauch; L. M. Scott; S. Geier; R. A. Mewaldt; L. M. Barbier; J. W. Mitchell; G. A. De Nolfo; R. E. Streitmatter; C. J. Waddington

doi:10.1142/S0217751X05029861

The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment

S. Kodaira
, M. Hareyama
, N. Hasebe
, T. Miyachi
, K. Sakurai
, W. R. Binns
, J. R. Cummings
, M. H. Israel
, J. T. Link
, B. F. Rauch
, L. M. Scott
, S. Geier
, R. A. Mewaldt
, L. M. Barbier
, J. W. Mitchell
, G. A. De Nolfo
, R. E. Streitmatter
, C. J. Waddington

Department of Physics

Research output: Contribution to journal › Article › peer-review

Abstract

A precise measurement of elemental abundances of galactic cosmic rays from charges Z = 20 to 34 was made by TIGER balloon experiment. Using the various path lengths in the atmosphere between 4 and 16 g/cm² from the TIGER flight data, we derived the attenuation length of iron nuclei with the energy above 2.5 GeV/n in the atmosphere. As the result, we obtained the attenuation length of 15.5 ± 0.6 g/cm² which is consistent with previous results of balloon measurements.

Original language	English
Pages (from-to)	6702-6704
Number of pages	3
Journal	International Journal of Modern Physics A
Volume	20
Issue number	29
DOIs	https://doi.org/10.1142/S0217751X05029861
State	Published - Nov 20 2005

Keywords

Cosmic ray
Elemental abundance
Heavy nuclei
Interaction mean free path

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10.1142/S0217751X05029861

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Kodaira, S., Hareyama, M., Hasebe, N., Miyachi, T., Sakurai, K., Binns, W. R., Cummings, J. R., Israel, M. H., Link, J. T., Rauch, B. F., Scott, L. M., Geier, S., Mewaldt, R. A., Barbier, L. M., Mitchell, J. W., De Nolfo, G. A., Streitmatter, R. E., & Waddington, C. J. (2005). The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment. International Journal of Modern Physics A, 20(29), 6702-6704. https://doi.org/10.1142/S0217751X05029861

@article{de9e80e3fe9742bb92d67c46a950cd9c,

title = "The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment",

abstract = "A precise measurement of elemental abundances of galactic cosmic rays from charges Z = 20 to 34 was made by TIGER balloon experiment. Using the various path lengths in the atmosphere between 4 and 16 g/cm2 from the TIGER flight data, we derived the attenuation length of iron nuclei with the energy above 2.5 GeV/n in the atmosphere. As the result, we obtained the attenuation length of 15.5 ± 0.6 g/cm2 which is consistent with previous results of balloon measurements.",

keywords = "Cosmic ray, Elemental abundance, Heavy nuclei, Interaction mean free path",

author = "S. Kodaira and M. Hareyama and N. Hasebe and T. Miyachi and K. Sakurai and Binns, \{W. R.\} and Cummings, \{J. R.\} and Israel, \{M. H.\} and Link, \{J. T.\} and Rauch, \{B. F.\} and Scott, \{L. M.\} and S. Geier and Mewaldt, \{R. A.\} and Barbier, \{L. M.\} and Mitchell, \{J. W.\} and \{De Nolfo\}, \{G. A.\} and Streitmatter, \{R. E.\} and Waddington, \{C. J.\}",

year = "2005",

month = nov,

day = "20",

doi = "10.1142/S0217751X05029861",

language = "English",

volume = "20",

pages = "6702--6704",

journal = "International Journal of Modern Physics A",

issn = "0217-751X",

number = "29",

}

Kodaira, S, Hareyama, M, Hasebe, N, Miyachi, T, Sakurai, K, Binns, WR, Cummings, JR, Israel, MH, Link, JT, Rauch, BF, Scott, LM, Geier, S, Mewaldt, RA, Barbier, LM, Mitchell, JW, De Nolfo, GA, Streitmatter, RE & Waddington, CJ 2005, 'The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment', International Journal of Modern Physics A, vol. 20, no. 29, pp. 6702-6704. https://doi.org/10.1142/S0217751X05029861

TY - JOUR

T1 - The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment

AU - Kodaira, S.

AU - Hareyama, M.

AU - Hasebe, N.

AU - Miyachi, T.

AU - Sakurai, K.

AU - Binns, W. R.

AU - Cummings, J. R.

AU - Israel, M. H.

AU - Link, J. T.

AU - Rauch, B. F.

AU - Scott, L. M.

AU - Geier, S.

AU - Mewaldt, R. A.

AU - Barbier, L. M.

AU - Mitchell, J. W.

AU - De Nolfo, G. A.

AU - Streitmatter, R. E.

AU - Waddington, C. J.

PY - 2005/11/20

Y1 - 2005/11/20

N2 - A precise measurement of elemental abundances of galactic cosmic rays from charges Z = 20 to 34 was made by TIGER balloon experiment. Using the various path lengths in the atmosphere between 4 and 16 g/cm2 from the TIGER flight data, we derived the attenuation length of iron nuclei with the energy above 2.5 GeV/n in the atmosphere. As the result, we obtained the attenuation length of 15.5 ± 0.6 g/cm2 which is consistent with previous results of balloon measurements.

AB - A precise measurement of elemental abundances of galactic cosmic rays from charges Z = 20 to 34 was made by TIGER balloon experiment. Using the various path lengths in the atmosphere between 4 and 16 g/cm2 from the TIGER flight data, we derived the attenuation length of iron nuclei with the energy above 2.5 GeV/n in the atmosphere. As the result, we obtained the attenuation length of 15.5 ± 0.6 g/cm2 which is consistent with previous results of balloon measurements.

KW - Cosmic ray

KW - Elemental abundance

KW - Heavy nuclei

KW - Interaction mean free path

UR - https://www.scopus.com/pages/publications/29844445600

U2 - 10.1142/S0217751X05029861

DO - 10.1142/S0217751X05029861

M3 - Article

AN - SCOPUS:29844445600

SN - 0217-751X

VL - 20

SP - 6702

EP - 6704

JO - International Journal of Modern Physics A

JF - International Journal of Modern Physics A

IS - 29

ER -

The attenuation length of cosmic ray iron in the atmosphere obtained by tiger experiment

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