Table of contents
Combined revision comparison
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20May2019 Implemented loading of PIMA-fitted residuals for rate and acceleration (1st, 2nd order). Resulted in an improvement in SNR~11 to SNR~24 in 600s. The latter600ss. The HOPS fringe plot shows that not all of the phase wander could be compensated. Might have to find a way to fit the higher-order terms (jerk/3rd, 4th, 5th) that the priori polynomials from ASCASC a priori polynomials do contain.
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Version from 15:17, 20 May 2019
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20May2019 Implemented loading of PIMA-fitted residuals for rate and acceleration (1st, 2nd order). Resulted in an improvement in SNR~11 to SNR~24 in 600ss. The HOPS fringe plot shows that not all of the phase wander could be compensated. Might have to find a way to fit the higher-order terms (jerk/3rd, 4th, 5th) that ASC a priori polynomials do contain.
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Version as of 15:19, 20 May 2019
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20May2019 Implemented loading of PIMA-fitted residuals for rate and acceleration (1st, 2nd order). Resulted in an improvement in SNR~11 to SNR~24 in 600s. The latter HOPS fringe plot shows that not all of the phase wander could be compensated. Might have to find a way to fit the higher-order terms (jerk/3rd, 4th, 5th) that the priori polynomials from ASC do contain.
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