Present large scale photometric and helioseismic data may be related to spatial and temporal deviations from an otherwise static, spherical solar convection zone (SCZ). New space experiments combine precise photometric, helioseismic, and magnetic observational capabilities (like SOHO and MDI) and will provide data needed to understand the interaction of magnetic fields and global scale circulation in the SCZ. Even simple physical arguments make it clear that the anticipated accuracy of these new experiments virtually guarantees new constraints on models of the SCZ.


    Access

    Access via TIB

    Check availability in my library


    Export, share and cite



    Title :

    Inferring solar structure variations from photometric and helioseismic observations


    Contributors:
    Kuhn, J. R. (author)


    Publication date :

    1991-01-01



    Type of media :

    Miscellaneous


    Type of material :

    No indication


    Language :

    English


    Keywords :



    Inferring subsurface supergranular flow directly from helioseismic correlation data

    Woodard, M. F. / European Space Agency | British Library Conference Proceedings | 2006


    Helioseismic sensing of the solar cycle

    Komm, R. / Howe, R. / Hill, F. et al. | British Library Conference Proceedings | 2006


    Helioseismic probing of solar dynamo flows

    Ruzmaikin, A. / Lindsey, C. | NTRS | 2002


    Helioseismic sensing of the solar cycle

    Komm, R. | Online Contents | 2006