Solar Physics

, Volume 219, Issue 2, pp 217–230 | Cite as

EIT Observations of the 15 November 1999 Mercury Transit

  • F. Auchère
  • G.E. Artzner


The Mercury transit of 15 November 1999 has been observed from space by the SOHO and TRACE spacecraft. We exploited the data recorded by EIT/SOHO to determine the stray-light level and the plate-scale of the instrument. The asymmetric distribution of stray light across the images is confirmed, but the absolute amount was found to be higher than previously estimated. The plate scale averaged over wavelengths was found to be 2.627±0.001 arc sec pixel−1, in excellent agreement with two previous and independent determinations.


Mercury Excellent Agreement Absolute Amount Asymmetric Distribution Independent Determination 
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  1. Allen, C. W.: 1976, Astrophysical Quantities, 3rd ed., Athlone, London.Google Scholar
  2. Artzner, G. E., Auchère, F., Delaboudinière, J.-P., and Hochedez, J.-F. E.: 1999, in Fritz Merkle (ed.), Proc. SPIE, Design and Engineering of Optical Systems II, 3737, 32.Google Scholar
  3. Auchère, F., DeForest, C. E., and Artzner, G. E.: 2000, Astrophys. J. 529, L115.CrossRefADSGoogle Scholar
  4. Auchère, F. et al.: 1998, Astron. Astrophys. 336, L57.ADSGoogle Scholar
  5. Auchère, F., Hassler, D. M., Slater, D. C., and Woods, T. N.: 2001, Solar Phys. 202, 269.CrossRefADSGoogle Scholar
  6. Broadfoot, A. L., Kumar, S., Belton, M. J. S., and Elroy, M. B.: 1974, Science 185, 166.ADSGoogle Scholar
  7. Brown, T. M. and Christensen-Dalsgaard, J.: 1998, Astrophys. J. 500, L195.CrossRefADSGoogle Scholar
  8. Cudnik, B. M.: 2004, Solar Phys., this issue.Google Scholar
  9. Defise, J.-M.: 1999, Université de Liège, Ph.D. Thesis.Google Scholar
  10. Delaboudinière, J.-P. et al.: 1995, Solar Phys. 162, 291.CrossRefADSGoogle Scholar
  11. Elson, J. M., Rahn, J. P., and Bennett, J. M.: 1983, Applied Optics 22, 3207.ADSGoogle Scholar
  12. Jilinski, E. G. et al.: 1999, Astron. Astrophys. Suppl. 128, 605.Google Scholar
  13. Kendig, D. and Slater, G.: 1987, Sky Telescope 223.Google Scholar
  14. Moses, J. D. et al.: 1997, Solar Phys. 175, 571.CrossRefADSGoogle Scholar
  15. Schneider, G., Pasachoff, J. M., and Golub, L.: 2001, Bull. Am. Astron. Soc. 33.Google Scholar
  16. Schou, J., Kosovichev, A. G., Goode, P. R., and Dziembowski, W. A.: 1997, Astrophys. J. 489, L197.ADSGoogle Scholar
  17. Sinceac, V., Chollet, F., Laclare, F., and Delmas, C.: 1998, Astron. Astrophys. Suppl. Ser. 128, 605.CrossRefADSGoogle Scholar
  18. Wülser, J.-P. et al.: 1998, Solar Phys. 180, 131.CrossRefADSGoogle Scholar

Copyright information

© Kluwer Academic Publishers 2004

Authors and Affiliations

  • F. Auchère
    • 1
  • G.E. Artzner
    • 1
  1. 1.Institut d'Astrophysique SpatialeUniversité Paris SudOrsayFrance

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