Influence of low-degree high-order p-mode splittings on the solar rotation profile

  1. García, R.A. 1
  2. Mathur, S. 1
  3. Ballot, J. 2
  4. Eff-Darwich, A. 34
  5. Jiménez-Reyes, S.J. 4
  6. Korzennik, S.G. 5
  1. 1 Centre National de la Recherche Scientifique
    info

    Centre National de la Recherche Scientifique

    París, Francia

    GRID grid.4444.0

  2. 2 Max Planck Institute for Astrophysics
    info

    Max Planck Institute for Astrophysics

    Garching bei München, Alemania

    GRID grid.452596.9

  3. 3 Universidad de La Laguna
    info

    Universidad de La Laguna

    San Cristobal de La Laguna, España

    GRID grid.10041.34

  4. 4 Instituto de Astrofísica de Canarias
    info

    Instituto de Astrofísica de Canarias

    Santa Cruz de Tenerife, España

    GRID grid.17423.33

  5. 5 Harvard-Smithsonian Center for Astrophysics
    info

    Harvard-Smithsonian Center for Astrophysics

    Cambridge, Estados Unidos

    GRID grid.455754.2

Journal:
Solar Physics

ISSN: 0038-0938

Year of publication: 2008

Volume: 251

Issue: 1-2

Pages: 119-133

Type: Article

Export: RIS
DOI: 10.1007/s11207-008-9144-5 SCOPUS: 2-s2.0-50249105673 GOOGLE SCHOLAR lock_openOpen access editor
Data source: Scopus