Log in

Observations of low-degree solar oscillations with few detector elements

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

The detection of low-degree solar oscillation modes with a specific low-resolution detector configuration is investigated. The detector is part of an instrument (the Luminosity Oscillations Imager) in the VIRGO package, to be flown on SOHO. Various problems such as p- and g-mode sensitivity, B and roll angle effects, modes isolation, cross-talk and guiding effects are treated for a given detector configuration. The computed sensitivity will enable the instrument to detect any type of modes for l < 6.B and roll angle effects can be compensated by using adequate filters for mode isolation. Guiding effects are small for p-modes. Also some other complex high-degree mode effects are treated.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price includes VAT (Germany)

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Allen, C. W.: 1973, Astrophysical Quantities, 3rd edition, The Athlone Press, London.

    Google Scholar 

  • Andersen, B. N.: 1988, in E. Rolfe (ed.), Seismology of the Sun and Sun-Like Stars, ESA SP-286, p. 381.

  • Andersen, B. N., Domingo, V., Jones, A. R., Jiménez, A., Pallé, P. L., Regulo, C., and Roca Cortés, T.: 1988, in E. Rolfe (eds.), Seismology of the Sun and Sun-Like Stars, ESA SP-286, p. 381.

  • Berthomieu, G. and Provost, J.: 1990, Astron. Astrophys. 227, 563.

    Google Scholar 

  • Brown, T. M.: 1985, Nature 317, 591.

    Google Scholar 

  • Christensen-Dalsgaard, J.: 1984, in Solar Seismology from Space, JPL Publ. 84–84, p. 219.

  • Edmonds, E. D.: 1957, Angular Momentum in Quantum Mechanics, 2nd edition, Oxford University Press, Oxford.

    Google Scholar 

  • Fröhlich, C., Andersen, B. N., Berthomieu, G., Crommelynck, D., Delache, P., Domingo, V., Jiménez, A., Jones, A. R., Roca Cortés, T., and Wehrli, C: 1989, ESA SP-1104, 19.

  • Harvey, J.: 1988, in E. Rolfe (eds.), Seismology of the Sun and Sun-Like Stars, ESA SP-286, p. 55.

  • Kosovichev, A. G.: 1986, Izv. Krymsk. Astrofiz. Obs. 75, 22.

    Google Scholar 

  • Libbrecht, K. G. and Kuhn, J. R.: 1984, Astrophys. J. 277, 889.

    Google Scholar 

  • Libbrecht, K. G. and Zirin, H.: 1986, Astrophys. J. 208, 413.

    Google Scholar 

  • Provost, J. and Berthomieu, G.: 1988, in E. Rolfe (eds.), Seismology of the Sun and Sun-Like Stars, ESA SP-286, p. 387.

  • Rhodes, E. J. Jr., Deubner, F.-L., and Ulrich, R. K.: 1979, Astrophys. J. 227, 629.

    Google Scholar 

  • Tomzcyk, S.: 1988, Ph.D. dissertation, University of California, Los Angeles.

    Google Scholar 

  • Toutain, T. and Gouttebroze, P.: 1988, in E. Rolfe (eds.), Seismology of the Sun and Sun-Like Stars, ESA SP-286, p. 241.

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Appourchaux, T., Andersen, B.N. Observations of low-degree solar oscillations with few detector elements. Sol Phys 128, 91–110 (1990). https://doi.org/10.1007/BF00154150

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00154150

Keywords

Navigation