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SPP/FIELDS Team. Keith Goetz University of Minnesota Goetz@umn.edu. Agenda. Stack Connectors galore Boom 3.5m SA Noise L3 Requirements 5nT Sub-system ICDs in the works EDTRD comments due. Block Diagram. Main Electronics Package. Top Panels, Under EMC cover. Left Side Panels.
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SPP/FIELDS Team Keith Goetz University of Minnesota Goetz@umn.edu
Agenda • Stack • Connectors galore • Boom • 3.5m • SA Noise • L3 Requirements • 5nT • Sub-system ICDs in the works • EDTRD comments due
Main Electronics Package Top Panels, Under EMC cover Left Side Panels
FIELDS MAG Boom hinge SCM V5 MAGo MAGi
FIELDS MAG Sensors • Order is to be determined by FIELDS • Separation is important • Boom length maybe given • May not shrink • DC MAG Alignment • Z axes are co-linear and parallel to S/C Z (roll) axis • X axes are parallel and parallel to S/C X axis • Y axes are parallel and parallel to S/C Y axis • SCM Alignment • X, Y and Z axes are maximally un-aligned with S/C and MAG axes?
Array Noise Solar arrays will make noise Solar arrays will move as a function of solar distance Noise models give results that are not too bad – 2nT Noise from the array pair could be somewhat better one way that another based on identical array wiring or reversed array wiring FIELDS has a vote Where would we like our noise? X? Y? Z?
L3 DC MAG requirements As written, the DC MAG spec is inadequate MAG shall be capable of measuring 3D vector magnetic fields from SPP, as follows: -- frequency range: DC to greater than 100 Hz; -- maximum field intensity: -65000 to +65000 nT; -- cadence: up to 2x the highest frequency in vectors/sec; -- minimum sensitivity (excluding external noise sources) better than: 4 nT in 65000 nT range; 0.1 nT in 1000 nT range; -- accuracy: 5nT; -- in three orthogonal components. Accuracy should be? Vector accuracy of 1 degree? Maximum range ok? ±65knT? ±128knT?
Subsystem ICDs Coming along
Environmental Spec • EDTRD rev – • Comments? • Due Friday