Tri-phonic helioseismology: Comparison of solar p modes observed by the helioseismology instruments aboard SOHO

  1. Toutain, T. 1
  2. Appourchaux, T. 2
  3. Baudin, F. 3
  4. Fröhlich, C. 4
  5. Gabriel, A. 5
  6. Scherrer, P. 6
  7. Andersen, B.N. 7
  8. Bogart, R. 6
  9. Bush, R. 6
  10. Finsterle, W. 4
  11. García, R.A. 8
  12. Grec, G. 1
  13. Henney, C.J. 9
  14. Hoeksema, J.T. 6
  15. Jiménez, A. 10
  16. Kosovichev, A. 6
  17. Roca Cortés, T. 10
  18. Turck-Chièze, S. 8
  19. Ulrich, R. 9
  20. Wehrli, C. 4
  1. 1 Observatoire de la Côte d’Azur
    info

    Observatoire de la Côte d’Azur

    Niza, Francia

    GRID grid.440460.2

  2. 2 European Space Research and Technology Centre
    info

    European Space Research and Technology Centre

    Noordwijk-Binnen, Holanda

    GRID grid.424669.b

  3. 3 National Solar Observatory
    info

    National Solar Observatory

    Boulder, Estados Unidos

    GRID grid.487716.b

  4. 4 Phys.-Meteorologisches O., World Radiation Center
  5. 5 Institut d'Astrophysique Spatiale, CNRS/Université Paris XI
  6. 6 Stanford University
    info

    Stanford University

    Stanford, Estados Unidos

    GRID grid.168010.e

  7. 7 Norwegian Space Centre
    info

    Norwegian Space Centre

    Oslo, Noruega

    GRID grid.436929.3

  8. 8 Saclay Nuclear Research Centre
    info

    Saclay Nuclear Research Centre

    Saclay, Francia

    GRID grid.462763.2

  9. 9 University of California Los Angeles
    info

    University of California Los Angeles

    Los Ángeles, Estados Unidos

    GRID grid.19006.3e

  10. 10 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    GRID grid.17423.33

Journal:
Solar Physics

ISSN: 0038-0938

Year of publication: 1997

Volume: 175

Issue: 2

Pages: 311-328

Type: Article

Export: RIS
DOI: 10.1023/A:1004949832159 SCOPUS: 2-s2.0-0031318796 GOOGLE SCHOLAR
Data source: Scopus