The measurement of global scale surface dynamics

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Imaging Techniques, Solar Oscillations, Solar Rotation, Sun, Velocity Measurement, Calibrating, Electromagnetic Noise, Fourier Transformation, Mission Planning, Sensitivity, Telemetry

Scientific paper

The SCADM mission implicitly contains a requirement for a fundamentally new type of satellite instrument: a very sensitive (approximately 1 m s/1) imaging velocity detector. This is needed to measure global oscillations and global circulation patterns, but the sensitivity requirement is so severe that it has not yet been met even with ground based instruments. In this presentation, the various possible sources of noise and other errors in such a device are considered, and the more detailed instrumental requirements are developed. This leads to the conceptual design of a velocity graph that appears to achieve the necessary sensitivity and imaging capability within a resonable weight and volume.

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