The opportunities offered by SCADM for the study of surface phenomena related to interior structure and dynamics

Astronomy and Astrophysics – Astronomy

Scientific paper

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Mission Planning, Solar Activity, Solar Probes, Spaceborne Astronomy, Sun, Chromosphere, Solar Corona, Spaceborne Experiments

Scientific paper

The physical processes to be probed by experiments may be grouped as large scale flows, oscillations, and chromospheric/coronal diagnostics. While the fundamental concerns and observational equipments are similar within each class, different investigations may tell different things about the Sun. Observational requirements are listed for experiments to study (1) plasma-magnetic field interactions; (2) interior structure via oscillations; (3) chromospheric and coronal tracers; (4) rotation, meridional flows, and giant cells; (5) the depth dependence of rotation; (6) EUV luminosity; (7) intensity fluctuations and tracers; and (8) diameter oscillations, the effects of noise and time-string on experiment results are assessed.

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