References

References


  1. See e.g. R. Davis Jr., K. Lande, C.K. Lee, P.Wildenhain, A. Weinberger, T. Daily, B. Cleveland, J. Ullman; Proc. 21st International Cosmic Ray Conf., Adelaide, Australia, in press (1990).

  2. K.S. Hirata et al., Kamiokande II Collaboration; Phys. Rev. Lett. 65(1990)1301.

  3. SAGE Collab., A.I. Abazov et al.; Phys. Rev. Lett. 67(1991)3332.

  4. GALLEX Collab., P. Anselmann et al.; Phys. Lett. 285B(1992)376.

  5. M. Spiro, D. Vignaud; Phys. Lett. 242B(1990)279.

  6. J.N. Bahcall, H.A. Bethe, Astrophysics Preprint IASSNS-AST 90/14, Princeton (1990).

  7. H. Harari; Phys. Lett. 216B(1989)413.

  8. Letter of intent, CHARM II Collaboration - Ferrara Univ. - IHEP (Zeuthen) - Nagoya Univ.(Japan) - Rome Univ. (Emulsion group), CERN - SPSC/89-46.

  9. N. Ushida et al.; Phys. Rev. Lett. 57(1986)2897.

  10. N. Ushida et al.; Nucl. Instr. Methods 224(1984)50.

  11. S. Aoki et al.; Nucl. Instr. Methods B51(1990)466.

  12. A. Artamonov et al.; Nucl. Instr. Methods A300(1990)53.

  13. M. Adinolfi et al.; Nucl. Instr. Methods A311(1992)91.

  14. B. Hoffmann, H.E. Roloff, Zeuthen (IHEP), preprint 1990.

  15. D. Acosta et al.; Nucl. Instr. Methods A294(1990)193.

  16. D. Acosta et al.; CERN-PPE/90-172.

  17. CERN/DRDC/90-23, DRDC/P1.

  18. M. Holder et al.; Nucl. Instr. Methods 148(1978)235.

  19. K. de Winter et al.,CHARM II Collaboration; Nucl. Instr. Methods A278(1989)670.

  20. D. Geiregat et al., CHARM II Collaboration; Phys. Lett. 232B(1989)539.

  21. G-Beam is a new Monte Carlo Programme to simulate the neutrino beam. Ch. Foos, CHARMEII Collaboration, Internal Note (1989), unpublished.

  22. N. Ushida et al. (531); Phys. Lett. 206B(1988)375.

  23. M.E. Duffy et al. (E613); Phys. Rev. D38(1988)2032.

  24. M. Aguilar-Benitez et al. (LEBC); Z. Phys. C40(1988)321.

  25. J. Dorenbosch et al. (CHARM); Z. Phys. C40(1988)497.

  26. H. Abramowicz et al. (CDHS); Z. Phys. C15(1982)497.

  27. D. Geiregat et al., CHARM II Collaboration; Phys. Lett. 247B(1990)131. The flux integral has been determined from inclusive nm interactions (NC and CC) with an uncertainty of 1 4.7%.

  28. CCFR Collaboration, W.H. Smith et al.; Nucl. Phys. B (Proc. Suppl.) 31(1993)262.

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JV / 17 Jan 1994