2021 May

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Revision as of 16:45, 16 May 2021 by Dgary (talk | contribs) (Created page with "[http://www.ovsa.njit.edu/wiki/index.php/Expanded_Owens_Valley_Solar_Array#Observing_Log Back to Observing Log] == May 16 == '''14:14 UT''' The first few scans today were usi...")
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May 16

14:14 UT The first few scans today were using the "usual" correlator equalizer coefficients (8.0). However, a test I ran earlier today indicates that my recent changes to the ADC settings has caused this equalizer setting to be quite a bit too high. After some thought, I have decided to set them to 2.0 as of this scan at 14:14 UT, which will allow most of the auto-correlations to be in a linear range. However, this will require a new expression for "desat" correction of the auto-correlation saturation. Any data taken from now may have to be reanalyzed by the pipeline, up until the date when I get the new expression defined and implemented.