3D Reconstruction of Photospheric Velocity Fields Inside a Magnetic Network Cell

Details 3D Reconstruction of Photospheric Velocity Fields Inside a Magnetic Network Cell 3D Reconstruction of Photospheric Velocity Fields Inside a Magnetic Network Cell

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..358...84d&link_type=abstract

Solar Polarization 4, ASP Conference Series, Vol. 358, Proceedings of the conference held 19-23 September, 2005, in Boulder, Col

Computer Science

Scientific paper

A complete insight of the dynamics of the plasma flows and their interaction with the magnetic field is important to understand the solar convective layer. Such an interaction determines the spatial configuration of the magnetic field in the outer layers of the solar atmosphere. In order to investigate the interaction between the photospheric velocity field and emerging magnetic elements, observations with high spatial, spectral, and temporal resolution are necessary. We present a 3D reconstruction of the photospheric velocity field of a quiet region centered on a large scale (˜ 30 Mm) structure of magnetic network and an analysis of the photospheric plasma dynamical properties below a cluster of magnetic structures.

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