September 2, 2015

Starting on 15 August 2015 (orbital rev 5064) and continuing to present day, there has been an anomalous drop in the echo power signal in the receiver of approximately 20 dB, which initially took place at 03:01:59 UTC. Both noise and signal power dropped but not by equal amounts. The Signal to Noise Ratio dropped by 10 dB. Corresponding with this drop in power was an increase of approximately 0.20 mA in current in the Scatterometer Electronics Subsystem (SES). ISS attitude has appeared normal during this time. Due to this anomaly the RapidScat Science Data Systems Team was initially unable to process the telemetry data to backscatter (Level 1B, 2A) or wind vectors (Level 2B). The operations team is still in the process of investigating the cause of the “reduced echo power” anomaly.  Several commands were sent to the instrument to aid in diagnosing the anomaly and to aid in recovering data production.
 
With some degradation in performance at low wind speeds, the ground data processing is now able to process science quality data and retrieve valid wind vector data. A preliminary review of the data has shown good correlation with pre-anomaly data. Data from orbits ranging from 5064 to 5127 and 5137 to 5152 will need special processing to account for variation in commanded instrument settings. Data from orbits 5127 through 5136 have been made available, as these data were processed when the instrument was first placed into the current configuration. We have also released data obtained from orbital rev 5152 and forward.
 
There were some unrelated events that also impacted the flow of RapidScat data:

 
There are several changes in the data going forward as a result of this persistent anomaly. The following changes affect all orbits forward from 5064:
 

  1. Wind direction (and to a lesser extent speed) accuracy are degraded for low winds. Winds above 6 m/s are not significantly affected but statistics for 3-6 m/s are noticeably worse especially in the middle of the swath.
  2. Rain flagging is now unavailable for the outer (single beam portion) of the swath. The IMUDH rain flag that the JPL wind retrieval has been using is corrupted because it uses the RapidScat Brightness temperature. With a 10 dB loss in SNR, brightness temperatures are no longer usable. So we are switching rain flags to use the Impact Quantity Rain flag which has been previously utilized to determine when to correct wind speeds for rain. The new rain flag does not use brightness temperature and is not available in the outer swath. The statistics of the rain impact quantity have not changed significantly as a result of this anomaly.

 
The improved rain speed correction for tropical cyclones (version 1.1) has now been turned off because it relies on brightness temperature. We are going back to the original rain correction used in the Version 1.0 L2B data processing.
 
As of now, the 12.5-km L2B wind vector data from orbital rev 5152 to 5242 are available. More data will continue to flow in sequentially each day with an approximate 7-day latency.
 
Concerned data users who are not currently registered with the PO.DAAC email list are encouraged to register to receive timely data announcement updates via email by contacting podaac@podaac.jpl.nasa.gov.

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