Abstract
The goals of the TREK experiment, now in place on the MIR Space Station, are to resolve and measure the composition of both odd-Z and even-Z cosmic-ray nuclei up to uranium, to measure the isotopic composition of Fe-group nuclei, and to search for transuranic nucleic and exotic particles such as strangelets. To collect tracks of ultraheavy cosmic rays, exterior panels holding an array of BP-1 phosphate glass 1.2m2 in area and 16 plates thick are now mounted outside the Kvant-2 module on MIR. Heaters and relays regulate the temperature of the glass at 25°±5°C. The detectors will record ∼103 cosmic-ray tracks withZ≥50 during ∼2.5 years. An interior panel consisting of an array 0.09 m2 in area and 32 plates thick and mounted on the inside wall of the Soyuz spacecraft (attached to the Space Station) will collect tracks of about 13000 Fe and 500 Ni nuclei.
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Binns, W. R. et al.: 1987,Phys. Rev. C36, 1870.
Binns, W. R. et al.: 1989,Astrophys. J. 346, 997.
Cartwright, B. G., Shirk, E. K., and Price, P. B.: 1978,Nucl. Instr. Meth. 153 457.
Drach, J.: 1987, ‘HNC: a Detector to Study Ultraheavy Cosmic Rays’, Ph.D. Thesis, University of California, Berkeley.
Drach, J., et al.: 1985,Proc. 19th Int. Cosmic Ray Conf. La Jolla 2, 131.
Fleischer, R. L., Price, P. B., and Walker, R. M.: 1975,Nuclear Tracks in Solids, University of California Press, Berkeley.
Fowler, P. H. et al.: 1976,Proc. Ninth Int. Conf. Solid State Nuclear Track Detectors, Munich 2, 1007.
Fowler, P. H. et al.: 1987,Astrophys. J. 314, 739.
Gerbier, G., Guoxiao, Ren, and Price, P. B.: 1988,Phys. Rev. Letters 60, 2258.
Hainebach, K. L. et al.: 1974,Astrophys. J. 193, 157.
Lowder, D. M.: 1991, inProc. Workshop on Strange Quark Matter, Aarhus, Denmark.
Mewaldt, R. A.: 1989, in C. J. Waddington (ed.),Cosmic Abundances of Matter, American Institute of Physics Conf. Proceedings, No. 183.
Mewaldt, R. A. et al.: 1980,Astrophys. J. 236, L121.
Meyer, J.-P.: 1985,Astrophys. J. Suppl. 57, 173.
O'Sullivan, D.: 1991, private communication.
Price, P. B. and Drach, J.: 1987,Nucl. Instr. Meth. B28, 275.
Price, P. B. et al.: 1987,Nucl. Instr. Meth. B21, 60.
Raisbeck, G. M. et al.: 1975,Proc. 14th Int. Cosmic Ray Conf. Munich 2, 560.
Salamon, M. H., Price, P. B., and Drach, J.: 1986,Nucl. Instr. Meth. B17, 173.
Shirk, E. K. and Price, P. B.: 1978,Astrophys. J. 220, 719.
Tarlè, G., Ahlen, S. P., and Cartwright, B. G.: 1978,Phys. Rev. Letters 41, 771.
Tarlè, G., Ahlen, S. P., and Price, P. B.: 1981,Nature 293, 556.
Thompson, A.et al. (1981,Proc. 11th Int. Conf. on Solid State Nuclear Track Detectors, Bristol, England.
Thompson, A. et al.: 1990,Proc. 21st Int. Cosmic Ray Conf. Adelaide 4, 441.
Wang, Shicheng, Barwick, S. W., Ifft, D., Price, P. B., and Westphal, A. J.: 1988,Nucl. Instr. Meth. B35, 43.
Westphal, A. J.: 1991, Ph.D. Thesis, University of California at Berkeley (in prep.).
Westphal, A. J., Price, P. B., and Snowden-Ifft, D.: 1992 (in prep.).
Wiedenbeck, M. E.: 1990,Proc. 21st Int. Cosmic Ray Conf., Adelaide 11, 57.
Witten, E.: 1984,Phys. Rev. D30, 272.
Woosley, S. E. and Weaver, T. A.: 1981,Astrophys. J. 243, 561.
Young, J. S. et al.: 1981,Astrophys. J. 246, 1014.
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Price, P.B., Lowder, D.M., Westphal, A.J. et al. TREK: A cosmic-ray experiment on the Russian space station MIR. Astrophys Space Sci 197, 121–143 (1992). https://doi.org/10.1007/BF00645077
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DOI: https://doi.org/10.1007/BF00645077