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Created Mar 12, 2019 by Carl Schaffer@schafferOwner

headers: coordinate uncertainties

fill solar x and y coordinate uncertainties to one disk diameter, as the only thing we are sure of is that we are pointing at the solar disk for those observation runs where we have no cross correlation of the gris coordinates. For the runs where a correlation is possible, we need to figure out a different method of estimating the uncertainty.

Edited Mar 21, 2019 by Carl Schaffer
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