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p-Mode analysis of the IPHIR data

  • Part IV Observations of Solar Oscillations
  • Conference paper
  • First Online:
Progress of Seismology of the Sun and Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 367))

Abstract

The results of the IPHIR experiment on the USSR planetary mission to Phobos presented here are from data gathered during 160 days of the cruise phase of PHOBOS II to Mars, launched on 12 July 1988. The long uninterrupted observation produces a spectrum of the solar p-mode oscillations in the 5-minute range with a very high signal-to-noise ratio. Frequency and line shape determination is limited by the lifetime of the modes and the ‘noise’ from stochastic excitation. The temporal variation of the amplitudes of l = 0... 2 is discussed.

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References

  • Christensen-Dalsgaard, J. 1986, in Seismology of the Sun and Distant Stars, ed. by D.O.Gough (Reidel, Dordrecht), p.23.

    Google Scholar 

  • Elsworth, Y., Isaak, G.R., Jefferies, S.M., McLeod, C.P., New, R., Pallé, P.L., Régulo, C., and Roca Cortés, T. 1988, in Seismology of the Sun and Sun-like Stars, ed. E. Rolfe, ESA SP-286 (ESA Publication Division, Noordwijk), p.27.

    Google Scholar 

  • Fróhlich, C., Bonnet, R.M., Bruns, A.V., Delaboudinibre, J.P., Domingo, V., Kotov, V.A., Kollath, Z., Rashkovsky, D.N, Toutain, T., Vial, J.C., and Wehrli, Ch. 1988, in Seismology of the Sun and Sun-like Stars, ed. E. Rolfe, ESA SP-286 (ESA Publication Division, Noordwijk), p.359.

    Google Scholar 

  • Fróhlich, C., Toutain, T., Bonnet, R.M., Bruns, A.V., Delaboudinière, J.P., Domingo, V., Kotov, V.A., Kollath, Z., Rashkovsky, D.N., Vial, J.C., and Wehrli, Ch. 1990, in Proc. IA U Colloq. No. 121, Inside the Sun, ed. G. Berthomieux and M. Cribier (Klewer, Dordrecht), p.279.

    Google Scholar 

  • Jiménez, A., Pallé, P.L., Pérez, J.C., Régulo, C., Roca Cortés, T., Isaak, G.R., McLeod, C.P., and van der Raay, H.B. 1988, in Proc. IA U Symp. No. 123, Advances in Helio-and Asteroseismology, ed. J. Christensen-Dalsgaard and S. Frandsen, (Reidel, Dordrecht), p.205.

    Google Scholar 

  • Lazrek, M, Delache, P., and Fossat, E. 1988, in Seismology of the Sun and Sun-like Stars, ed. E. Rolfe, ESA SP-286 (ESA Publication Division, Noordwijk), p.673.

    Google Scholar 

  • Willson, R.C. 1982, Solar Phys., 74, 217.

    Google Scholar 

  • Woodard, M., and Hudson, H.S. 1983, Nature, 305, 589.

    Google Scholar 

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Author information

Authors and Affiliations

  1. Physikalisch-Meteorologisches Observatorium Davos, World Radiation Center, CH-7260, Davos-Dorf, Switzerland

    Claus Fröhlich

  2. Institut d'Astrophysique Spatiale, F-91370, Verrières-le-Buisson, France

    Thierry Toutain

Authors
  1. Claus Fröhlich
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  2. Thierry Toutain
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Editor information

Y. Osaki H. Shibahashi

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© 1990 Springer-Verlag

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Fröhlich, C., Toutain, T. (1990). p-Mode analysis of the IPHIR data. In: Osaki, Y., Shibahashi, H. (eds) Progress of Seismology of the Sun and Stars. Lecture Notes in Physics, vol 367. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53091-6_84

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  • DOI: https://doi.org/10.1007/3-540-53091-6_84

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-53091-6

  • Online ISBN: 978-3-540-46645-1

  • eBook Packages: Springer Book Archive

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