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Data: Version 5 (V5) Release

Version 5 is the official end-of-mission dataset, spanning the complete 45-month period of Aquarius science data availability from 25-Aug-11 to 07-Jun-15. Improving the accuracy of Aquarius measurements has been a key activity to ensure that the data are most useful for science and society. Scientists and engineers have worked together to test and refine algorithms – or step-by-step procedures for calculations – used to process Aquarius's ocean surface salinity data. V5 data represents the state-of-the-art in remote sensing of salinity and, although the Aquarius Project has ended, the raw data are available and plans exist to continue working on improvements.

Processing Steps
Counts from Each Radiometer
Calibration of Radiometer Data
Antenna Temperature
Remove Space Contributions
Earth Antenna Temperature
Remove Antenna Pattern Effect
Correct for Faraday Rotation
Top of Atmosphere BT
Remove Atmospheric Contribution
Ocean Surface BT
Remove Surface Roughness Effects
Flat Ocean Surface (Specular) BT
Key processing steps that have been improved in the V5 data release are shown in bold in the table at right. Italics show interim values calculated during the stepwise process.

Learn About Instrument Calibration from Sid Misra
Updating processing algorithms requires calibration, the process of correlating instrument readings with a standard to check their accuracy. For Aquarius V5 data, this has been accomplished using data from in-water buoys as its reference sea surface salinity field (i.e., analyzed monthly Argo sea surface salinity from Scripps Institution of Oceanography).

The movie at left features JPL engineer, Dr. Sid Misra, who discusses corrections for instrument drift over time and correcting for "wiggles" in the calibration of radiometer data (see table at right). He also addresses rationale for no longer using the HYCOM model as the reference sea surface salinity field in V5 processing. This 34-minute video will be of interest to users of Aquarius data (transcript).

Key Changes to V5
As indicated in the "Processing Steps" table, Aquarius's radiometer data go through several steps before being converted to sea surface salinity.

One of these steps is removing space contributions, including reflection of radiation from the galaxy on the ocean surface. This was first addressed in V3 processing after comparing data collected over the same area when the satellite was ascending versus descending in its orbit. Why? The Aquarius pointing geometry was tilted (i.e., not pointing straight down) and the ocean surface can act like a mirror. Depending on which direction the satellite was moving, galactic radiation could be reflected toward or away from the instrument. For V5, the ascending-descending differences have been recalculated based on improved knowledge of the reflected galaxy.

Interestingly, the January 2015 launch of another L-band radiometer mission, NASA's SMAP (Soil Moisture Active Passive), has contributed to improved processing of Aquarius data. For V5, the model of reflected galactic radiation has been updated based on data derived from different SMAP viewing directions (i.e., comparison of data from the same location on Earth based on SMAP’s forward-looking and backward-looking observations). The advantage of this approach is that it encompasses effects of the model for galactic radiation.

Another step in Aquarius processing is removing atmospheric contributions, including correcting for oxygen absorption. Salinity signals - detected by Aquarius as microwave energy emission - originate from the ocean and propagate through Earth's atmosphere. Comprised of about 20% oxygen, the atmosphere absorbs some of this energy and re-emits it based on air temperature. Thus, to better calculate salinity in V5, the model for absorption of atmospheric oxygen has been changed to Liebe et al. (1992).

Another change to the V5 product is a new source of ancillary sea surface temperature (SST), the Canadian Meteorological Center (CMC). The CMC product has better quality SST at high latitudes when compared to previous processing versions.

The surface roughness correction model uses data collected by the Aquarius scatterometer to estimate the effect of wind-roughened ocean surface on Aquarius brightness temperature measurements. Scatterometers operate by transmitting a pulse of microwave energy towards Earth's surface and measuring the reflected energy (i.e., backscatter). In general, rougher ocean conditions will scatter more energy than smoother, more reflective, mirror-like ocean surfaces. For Aquarius V5 data, various components of the surface roughness correction model were updated, in particular the SST dependence of wind-induced emission from the ocean surface.

Maria Describes the Rain Impact Model
A targeted analysis of Aquarius data demonstrated a high correlation between the spatial distribution of rain and patterns of reduced sea surface salinity. Thus, the Rain Impact Model (RIM) was developed to predict the effect of precipitation on Aquarius's salinity measurements. Available from NASA's Physical Oceanography Distributed Active Archive Center (PO.DAAC), Aquarius V5 data include instantaneous rain rates, which are used to filter for rain in the calibration of radiometer data and also for validation of Aquarius salinity data (see "Validation of Aquarius Data," below). In addition, for Aquarius V5 data, rain masks are applied to remove the biases that are caused by the strong precipitation (i.e., are "rain-flagged").

To learn more about RIM, please view the 16-minute video (at left) featuring scientist Maria Jacob (transcript).

Julian Presents the New Sea Surface "Spiciness" Product
The previous Aquarius data release (V4) included a density product derived from Aquarius sea surface salinity and ancillary SST. The example at top right shows that areas of colder, saltier water have higher densities (red colors) while the tropics - where water is generally warmer and less salty due to rain - have lower densities (blue colors).

V5 includes a new, complementary "spiciness" product (example shown at lower right). Red colors indicate surface water that is warm and salty. Blue colors indicate colder, less salty seawater at the ocean surface. Spiciness data are uniquely suited to study the formation and movement of water masses and are available from the PO.DAAC.

In the 28-minute video (at left), Dr. Julian Schanze provides background on Aquarius's density and spiciness data, including how they are used to better understand our ocean (transcript).

Validation of Aquarius Data
Calibration of Aquarius data goes hand-in-hand with validation, interrelated processes commonly known as "Cal/Val". Validation occurs when the instrument's data accuracy is proven by independent means. The V5 Salinity Data Validation Analysis, led by Dr. Hsun-Ying Kao, documents the progressive improvement from processing versions 2.0 to 5.0 by comparing each version of Aquarius data with in-situ data.

Forty-five months of data - including mapped, averaged (monthly, seasonal), and time-series data - are used for various validation analyses, some of which are described briefly here:
  • Matchup maps – In-situ salinity data points are compared with Aquarius swath (Level-2) data at the closest point of approach (CPA), defined as being collected within 3.5 days and 75 km (47 mi) of the Aquarius footprint's boresight position.
  • Three-beam histograms – Scatter plots of in-situ salinity versus Aquarius salinity at matchup points (i.e., CPA) are presented for each Aquarius beam.
  • Triple point analysis – Co-located difference histograms for each beam of Aquarius V5 data are included for: (1) Aquarius/In-situ; (2) HYCOM model/In-situ; and Aquarius/HYCOM model. These are used to estimate root mean square errors for each data type.
The report also includes important "Notes of Caution" (Section 12.2) for data users such as radiofrequency interference, rain masks, land contamination close to coasts, and regionally dependent static and time-varying biases.