LOGS OF MAY 8, 2010

12-min averaged IQUV data have been re-processed for the time range:
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2010.04.24_04:51:12-2010.04.26_17:18:10

The reprocessing is using the new parameters for the 12-min averaging.
NB: there is a gap in coverage every 12 hour when HMI was retuned.

12-min averaged IQUV data have been processed for the time range:
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2010.05.01_19:21:45_TAI-2010.05.03_19:29:15_TAI

NB: 2010.05.01_19:24:00_TAI and 2010.05.01_19:36:00_TAI are missing because 5 calibration sequences were taken from 19:22 to 19:38.

l.o.s. observables cropped 50 pixels off the limb have been processed for:
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2010.05.01_19:21:45_TAI-2010.05.03_19:29:15_TAI

NB: the coverage is about 99.4%. There are a few gaps due to daily calibration 
sequences
NB2: the statistical keywords (like DATARMS) are calculated over the entire 
uncropped area, including the 50 pixels off the limb, and therefore might not 
be representative of the rms variation in the solar disk.
Over the time range studied, the rms variation in l.o.s. field strength
in the quiet Sun was about 15.5 Gauss.