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Applied Optics

Applied Optics

APPLICATIONS-CENTERED RESEARCH IN OPTICS

  • Vol. 42, Iss. 19 — Jul. 1, 2003
  • pp: 3970–3980

Effects of proton irradiation on glass filter substrates for the Rosetta mission

Giampiero Naletto, Alessio Boscolo, Jeffery Wyss, and Alberto Quaranta  »View Author Affiliations


Applied Optics, Vol. 42, Issue 19, pp. 3970-3980 (2003)
http://dx.doi.org/10.1364/AO.42.003970


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Abstract

The Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) instrument on board the Rosetta spacecraft, a mission of the European Space Agency to comet P/Wirtanen, includes two cameras for acquiring images of the comet. A set of interference filters deposited upon glass and fused-silica substrates will be added to the cameras for wavelength tuning. For this mission of more than 10/years in an interplanetary environment, the requirement of preserving the optical characteristics of the filters is a critical one. We checked the variation in the transmission of some filter substrates after proton irradiation that simulated the solar wind. To produce a situation that is representative of the interplanetary environment, we irradiated proton fluences at three energies: 1.5 × 1011 protons/cm2 at 4 MeV, 1.9 × 1010 protons/cm2 at 8 MeV, and 7.1 × 109 protons/cm2 at 18 MeV. Seven substrates were tested: three Suprasil-1; three colored glasses, namely, OG590, KG3, and RG9; and one quartz. In addition, two interference filters were checked. The results obtained show that Suprasil-1 is rather insensitive to this irradiation, whereas very small reductions in transmission, of the order of a few percent, occur for colored glasses. The transmission of these filters was remeasured 2 years after the irradiation, and showed a general decrease in the transmission reduction.

© 2003 Optical Society of America

OCIS Codes
(120.2440) Instrumentation, measurement, and metrology : Filters
(160.2750) Materials : Glass and other amorphous materials
(160.4670) Materials : Optical materials
(350.2450) Other areas of optics : Filters, absorption
(350.5610) Other areas of optics : Radiation
(350.6090) Other areas of optics : Space optics

History
Original Manuscript: September 23, 2002
Revised Manuscript: March 13, 2003
Published: July 1, 2003

Citation
Giampiero Naletto, Alessio Boscolo, Jeffery Wyss, and Alberto Quaranta, "Effects of proton irradiation on glass filter substrates for the Rosetta mission," Appl. Opt. 42, 3970-3980 (2003)
http://www.opticsinfobase.org/ao/abstract.cfm?URI=ao-42-19-3970


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References

  1. G. Schwehm, Y. Langevin, ROSETTA/CNSR A Comet-Nucleus Sample-Return Mission. ESA Special Publication 1125, (European Space Agency: Paris, 1991).
  2. More information on the Rosetta mission can be found at the Web page http://sci.esa.int/rosetta/
  3. N. Thomas, H. Keller, E. Arijs, C. Barbieri, M. Grande, P. Lamy, H. Rickman, R. Ro-drigo, K. -P. Wenzel, M. A’Hearn, F. Angrilli, M. Bailey, M. Barucci, J. -L. Bertaux, K. Briess, J. Burns, G. Cremonese, W. Curdt, H. Deceuninck, R. Emery, M. Festou, M. Fulle, W. -H. Ip, L. Jorda, A. Korth, D. Koschny, J. -R. Kramm, E. Kürt, M. Lara, A. Llebaria, J. Lopez-Moreno, F. Marzari, D. Moreau, C. Muller, C. Murray, G. Naletto, D. Nevejans, R. Ragazzoni, L. Sabau, A. Sanz, J. -P. Sivan, G. Tondello, “OSIRIS—the Optical, spectroscopic and Infrared Remote Imaging System for the Rosetta orbiter,” Adv. Space Res. 21, 1505–1515 (1998). [CrossRef]
  4. The OSIRIS acronym derives from an old configuration of the instrument, when the optical design still had spectroscopic and infrared capabilities. After several modification in the design, in the present configuration only imaging in the visible and the near ultraviolet remains, but the instrument name has not changed.
  5. K. Dohlen, M. Saisse, G. Claeysen, J. -L. Boit, “Optical designs for the Rosetta narrow-angle camera,” Opt. Eng. 35, 1150–1157 (1996). [CrossRef]
  6. G. Naletto, V. Da Deppo, M. G. Pelizzo, R. Ragazzoni, E. Marchetti, “The optical design of the wide angle camera for the Rosetta mission,” Appl. Opt. 41, 1446–1453 (2002). [CrossRef] [PubMed]
  7. Multilayer insulation (MLI) is commonly used to provide thermal insulation. MLI usually consists of 25-μm thick polyester or polyamide layers or films that are metallized with aluminum or gold on one or both sides.
  8. T. Appourchaux, “Effect of space radiation on optical filters,” in Passive Materials for Optical Elements II, G. Wilkerson, ed., Proc. SPIE2018, 80–91 (1993). [CrossRef]
  9. D. Doyle, R. Czichy, “Influence of simulated space radiation on optical glasses,” in Space Optics 1994: Space Instrumentation and Spacecraft Optics, T. Dewandre, J. S. in-den Baeumen, E. Sein, eds., Proc. SPIE2210, 434–449 (1994). [CrossRef]
  10. P. Silverglate, E. Zalewski, P. Petrone, “Proton-induced radiation effects on optical glasses,” in Damage to Space Optics, and Properties and Characteristics of Optical Glass, J. Breckinridge, A. Marker, eds., Proc. SPIE1761, 46–57 (1992). [CrossRef]
  11. M. Shetter, V. Abtreu, “Radiation effects on the transmission of various optical glasses and epoxies,” Appl. Opt. 18, 1132–1133 (1979). [CrossRef] [PubMed]
  12. A. Gusarov, D. Doyle, A. Hermanne, F. Berghmans, M. Fruit, G. Ulbrich, M. Blondel, “Refractive-index changes caused by proton radiation in silicate optical glasses,” Appl. Opt. 41, 678–684 (2002). [CrossRef] [PubMed]
  13. T. Appourchaux, G. Gourmelon, B. Johlander, “Effect of gamma-ray irradiations on optical filter glass,” Opt. Eng. 33, 1659–1668 (1994). [CrossRef]
  14. P. Grillot, W. Rosenberg, “Proton radiation damage in optical filter glass,” Appl. Opt. 28, 4473–4477 (1989). [CrossRef] [PubMed]
  15. S. Pellicori, E. Russel, L. Watson, “Radiation induced transmission loss in optical materials,” Appl. Opt. 18, 2618–2621 (1979). [CrossRef] [PubMed]
  16. G. Possnert, J. Lagerros, H. Rickman, “Radiation damage in OSIRIS filter substrates,” in Advances in Optical Interference Coatings, C. Amra, H. Macleod, eds., Proc SPIE3738, 428–435 (1999). [CrossRef]
  17. R. Fry, D. Nacthwey, “Radiation protection guidelines for space missions,” Health Phys. 55, 159–166 (1988). [CrossRef] [PubMed]
  18. D. Gorney, “Solar cycle effects on near-Earth plasmas and space systems,” J. Spacecr. Rockets 26, 428–435 (1989). [CrossRef]
  19. P. Foukal, Solar Astrophysics (Wiley, New York, 1990).
  20. R. McGuire, T. V. Rosenvinge, F. McDonald, “The composition of solar energetic particles,” Astrophys. J. 301, 938–947 (1986). [CrossRef]
  21. J. King, “Solar proton fluences for 1977–1983 space missions,” J. Spacecr. Rockets 11, 401–407 (1974). [CrossRef]
  22. M. Walt, Introduction to Geomagnetically Trapped Radiation Space Science (Cambridge U. Press, Cambridge, (1994). [CrossRef]
  23. R. Mewaldt, “The elemental and isotopic composition of galactic gosmic ray nuclei,” Rev. Geophys. Space Phys. 21, 295–303 (1983). [CrossRef]
  24. D. Chcnette, W. Dietrich, “The solar flare heavy ion environment for single-event upsets: a summary of observations over the last solar cycle,” IEEE Trans. Nucl. Sci. 31, 1217–1225 (1984). [CrossRef]
  25. J. Feynman, T. Armstrong, L. Dao-Gibner, S. Silverman, “New interplanetary proton fluence model,” J. Spacecr. Rockets 27, 403–410 (1990). [CrossRef]
  26. J. Feynman, T. Armstrong, L. Dao-Gibner, S. Silverman, “Solar proton events during solar Cycles 19, 20, and 21,” Solar Phys. 126, 385–401 (1990). [CrossRef]
  27. J. Feynman, G. Spitale, J. Wang, S. Gabriel, “Interplanetary proton fluence model: JPL 1991,” J. Geophys. Res. 98, 13281–13294 (1993). [CrossRef]
  28. J. Gaffey, D. Bilitza, “NASA/National Space Science Data Center trapped radiation models,” J. Spacecr. Rockets 31, 172–176 (1994). [CrossRef]
  29. A. Tylka, J. Adams, P. Boberg, B. Brownstein, W. Dietrich, E. Flueckiger, E. Petersen, M. Shea, D. Smart, E. Smith, “CREME96: a revision of the Cosmic Ray Effects on Micro-Electronics code,” IEEE Trans. Nucl. Sci. 44, 2150–2160 (1997). [CrossRef]
  30. National Space Science Data Center at Goddard Space Flight Center, Greenbelt, Md. Web page: http://nssdc.gsfc.nasa.gov/space/ .
  31. The SPENVIS project is funded by the ESA through the General Support Technologies Programme. The project was developed by the Belgian Institute for Space Aeronomy, with sub-contractors Space Applications Services and the Paul Scherrer Institute. SPENVIS is registered as ESA contract 11711-W01. Web page: http://www.spenvis.oma.be/spenvis/ .
  32. “ROSETTA: experiment interface document part A: issue 2 Rev. 0,” Tech. Rep. (European Space Agency, Paris, 1999).
  33. C. Tranquille, E. Daly, “An evaluation of solar-proton event models for ESA mission,” ESA J. 16, 275–297 (1992).
  34. B. Nielsen, B. Torp, C. Rangel, M. Simplicio, A. Consiglieri, M. DaSilva, F. Paszti, J. Soares, A. Dodd, J. Kinder, M. Pitaval, P. Thevenard, R. Wing, “Improvement of corrosion resistance of M50 bearing steel by implantation with metal ions,” Nucl. Instrum. Methods Phys. Res. B 59/60, 772–777 (1991).
  35. A. Straede, “Ion implantation as an efficient surface treatment,” Nucl. Instrum. Methods Phys. Res. B 68, 380–388 (1992). [CrossRef]
  36. D. Bisello, M. Descovich, A. Kaminsky, D. Pantano, J. Wyss, A. Zanet, “Radiation damage of oxygenated silicon diodes by 27 MeV protons,” Nuovo Cimento A 112, 1377–1382 (1999).
  37. J. Wyss, D. Bisello, D. Pantano, “SIRAD: an irradiation facility at the LNL tandem accelerator for radiation damage studies on semiconductor detectors and electronic devices and systems,” Nucl. Instrum. Methods Phys. Res. A 462, 426–434 (2001). [CrossRef]
  38. J. Ziegler, J. Biersack, U. Littmark, The Stopping and Range of Ions in Solids (Pergamon, London, 1985).
  39. We made simulations by using 27-MeV protons orthogonally incident onto aluminum absorbers. The means and dispersions (rms) reported refer to samples of 2000 events for each case.
  40. Unfortunately it was not possible to measure the substrate transmission immediately after the irradiation. In fact, the irradiation was concluded during the night, much later than was initially foreseen, and the Department of Chemistry-Physics where the spectrophotometer was available opened only the following morning.

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