Reconstruction of source and cosmic magnetic field characteristics from clusters of ultra-high energy cosmic rays

Astroparticle Physics

Volumn 9, Issue 1, 1998, Pages 65-78

  Sigl, Günter ^a   Lemoine, Martin ^a,b  

^a UNIVERSITY OF CHICAGO   (United States)

^b CNRS   (France)

Author keywords

Cosmic magnetic fields; Ultra high energy cosmic rays

Indexed keywords

EID: 0032092879     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0927-6505(98)00006-1     Document Type: Article

References (46)

1. [1] M.A. Lawrence, R.J.O. Reid, A.A. Watson, J. Phys. G 17 (1991) 733.
2. [2] N. Hayashida et al., Phys. Rev. Lett. 73 (1994) 3491; S. Yoshida et al., Astropart. Phys. 3 (1995) 105.
3. [2] N. Hayashida et al., Phys. Rev. Lett. 73 (1994) 3491; S. Yoshida et al., Astropart. Phys. 3 (1995) 105.
4. [3] N. Hayashida et al., Phys. Rev. Lett 77 (1996) 1000.
5. [4] D.J. Bird et al., Phys. Rev. Lett. 71 (1993) 3401; Astrophys. J. 424 (1994) 491; 441 (1995) 144.
6. [4] D.J. Bird et al., Phys. Rev. Lett. 71 (1993) 3401; Astrophys. J. 424 (1994) 491; 441 (1995) 144.
7. [4] D.J. Bird et al., Phys. Rev. Lett. 71 (1993) 3401; Astrophys. J. 424 (1994) 491; 441 (1995) 144.
8. [5] T. Stanev et al., Phys. Rev. Lett. 75 (1996) 3056.
9. [6] K. Greisen, Phys. Rev. Lett. 16 (1966) 748; G.T. Zatsepin, V.A. Kuzmin, Pis'ma Zh. Eksp. Teor. Fiz. 4 (1966) 114 [JETP. Lett. 4 (1966) 78].
10. [6] K. Greisen, Phys. Rev. Lett. 16 (1966) 748; G.T. Zatsepin, V.A. Kuzmin, Pis'ma Zh. Eksp. Teor. Fiz. 4 (1966) 114 [JETP. Lett. 4 (1966) 78].
11. [6] K. Greisen, Phys. Rev. Lett. 16 (1966) 748; G.T. Zatsepin, V.A. Kuzmin, Pis'ma Zh. Eksp. Teor. Fiz. 4 (1966) 114 [JETP. Lett. 4 (1966) 78].
12. [7] J.W. Elbert, P. Sommers, Astrophys. J. 441 (1995) 151.
13. [8] F. Halzen, R.A. Vazques, T. Stanev, H.P. Vankov, Astropart. Phys. 3 (1995) 151.
14. [9] J.L. Puget, F.W. Stecker, J.H. Bredekamp, Astrophys. J. 205 (1976) 638; F.W. Stecker, e-print astro-ph/9710353, Phys. Rev. Lett., to appear.
15. [9] J.L. Puget, F.W. Stecker, J.H. Bredekamp, Astrophys. J. 205 (1976) 638; F.W. Stecker, e-print astro-ph/9710353, Phys. Rev. Lett., to appear.
16. [10] G. Sigl, S. Lee, in: Proc. 24th International Cosmic Ray Conference, Vol. 3 (Istituto Nazionale Fisica Nucleare, Rome, 1995) p. 356.
17. [11] J.P. Rachen, P.L. Biermann, Astron. Astrophys. 272 (1993) 161.
18. [12] E. Waxman, Phys. Rev. Lett. 75 (1995) 386.
19. [13] E. Waxman, Astrophys. J. 452 (1995) L1.
20. [14] M. Vietri, Astrophys. J. 453 (1995) 883.
21. [15] M. Milgrom, V. Usov, Astrophys. J. 449 (1995) L37.
22. [16] E. Waxman, Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 114.
23. [17] P. Bhattacharjee, C.T. Hill, D.M. Schramm, Phys. Rev. Lett. 69 (1992) 567.
24. [18] C.T. Hill, Nucl. Phys. B 224 (1983) 469.
25. [19] G. Sigl, Space Sc. Rev. 75 (1996) 375.
26. [20] P.P. Kronberg, Rep. Prog. Phys. 57 (1994) 325.
27. [21] R. Plaga, Nature 374 (1995) 430.
28. [22] E. Waxman, P. Coppi, Astrophys. J. 464 (1996) L75.
29. [23] E. Waxman, J. Miralda-Escudé, Astrophys. J. 472 (1996) L89.
30. [24] M. Lemoine, G. Sigl, A.V. Olinto, D.N. Schramm, Astrophys. J., 486 (1997) L115.
31. [25] S. Lee, A.V. Olinto, G. Sigl, Astrophys. J. 455 (1995) L21.
32. [26] G. Sigl, D.N. Schramm, S. Lee, P. Coppi, C.T. Hill, Proc. Nad. Acad. Sci. USA, Vol. 94 (1997) p. 10501.
33. [27] G. Sigl, M. Lemoine, A.V. Olinto, Phys. Rev. D 56 (1997) 4470.
34. [28] Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996).
35. [29] S.C. Corbató et al., Nucl. Phys. B (Proc. Suppl.) 28B ( 1992) 36; M, Al-Seady et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 191.
36. [29] S.C. Corbató et al., Nucl. Phys. B (Proc. Suppl.) 28B ( 1992) 36; M, Al-Seady et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 191.
37. [30] M. Teshima et al. Nucl. Phys. B (Proc. Suppl.) 28B (1992) 169; M. Hayashida et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 205.
38. [30] M. Teshima et al. Nucl. Phys. B (Proc. Suppl.) 28B (1992) 169; M. Hayashida et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 205.
39. [31] J.W. Cronin, Nucl. Phys. B (Proc. Suppl.) 28B (1992) 213; The Pierre Auger Observatory Design Report, 2nd ed. (14 March 1997).
40. [31] J.W. Cronin, Nucl. Phys. B (Proc. Suppl.) 28B (1992) 213; The Pierre Auger Observatory Design Report, 2nd ed. (14 March 1997).
41. [32] J.F. Ormes et al., in: Proc. 25th International Cosmic Ray Conference, M.S. Potgieter et al., eds. (Durban, 1997) pp. 5,273; Y. Takahashi et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 310.
42. [32] J.F. Ormes et al., in: Proc. 25th International Cosmic Ray Conference, M.S. Potgieter et al., eds. (Durban, 1997) pp. 5,273; Y. Takahashi et al., in: Proc. Int. Symposium on Extremely High Energy Cosmic Rays: Astrophysics and Future Observatories (Institute for Cosmic Ray Research, Tokyo, 1996) p. 310.
43. [33] T. Stanev, Astrophys. J. 479 (1997) 290.
44. [34] G.A. Medina Tanco, e-print astro-ph/9801060, Astrophys. J. Lett., to appear.
45. [35] M.J. Chodorowski, A.A. Zdziarski, M. Sikora, Astrophys. J. 400 (1992) 181.
46. 20 eV from Space, Univ. Maryland, Nov. 13-15 (1997).