ADCull:
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Eliminate HSA measurements that do not fit the predicted curves. You need
a rough attitude estimate to use this routine effectively.
This routine uses the leading edge data as the reference. dev
is the fractional deviation from the estimated data.
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Form:
[tLE1Cull, tTE1Cull, tLE2Cull, tTE2Cull] =
ADCull( el, jDEpoch, tLE1, tTE1, tLE2, tTE2, sA, jD, spinRate,
cant, dihedral, rA, dec, dev )
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Inputs
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el Keplerian elements
jDEpoch Epoch for the measurements
tLE1 (n,1) Leading edge time HSA 1
tTE1 (n,1) Trailing edge time HSA 1
tLE2 (n,1) Leading edge time HSA 2
tTE2 (n,1) Trailing edge time HSA 2
sA Sun angles (rad)
jD Julian dates corresponding to the above
spinRate Spin rate (rad/sec)
cant (2) Cants
dihedral (2) Dihedral angles
rA Estimated right ascension
dec Estimated declination
dev Allowable fractional deviation from the estimated data
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Outputs
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tLE1Cull Culled leading edge times HSA 1
tTE1Cull Culled trailing edge times HSA 1
tLE2Cull Culled leading edge times HSA 2
tTE2Cull Culled trailing edge times HSA 2
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Children:
Common: Graphics/NewFig
Common: Graphics/XLabelS
Common: Graphics/YLabelS
Common: Transform/RaDec2U
Math: Linear/Dot
SC: Sensor/HSAData