Impact of El Niño and La Niña on SeaWiFS, MODIS-A and VIIRS Chlorophyll-a Measurements Along the Equator During 1997 to 2016

The Ocean Biology Processing Group at NASA's GSFC recently reprocessed satellite ocean color measurements (SeaWiFS, MODIS-A and VIIRS) to improve accuracy and enhance time-series interoperability and consistency between multi-mission datasets. We chose the 1°S-1°N region along the equator to examine the behavior of Chl-a in El Niño and La Niña events because this latitudinal width represented the scale of Ekman upwelling, which is hypothesized to be a primary mechanism of Chl-a variations along the equator. An El Niño (La Niña) event has five consecutive 3-month-average sea surface temperature anomalies (SSTAs) greater (less) than 0.5°C in the 5°S-5°N, 170°W-120°W region and a super El Niño event occurs when SSTA is greater than 2.0°C. The September 1997 (onset of SeaWiFS data) to July 2016 period contained two super El Niño events, four typical El Niño events and four La Niña events. In the equatorial Pacific Ocean from 135°E (longitude of the westernmost data) to 150°E, the average typical El Niño and La Niña values were approximately the same (0.13 mg m-3). From 150°E to 165°W, the approximate bowl-shaped longitudinal pattern of Chl-a data in the average typical El Niño reached minimum (0.08 mg m-3) at 170°E and then increased to a relatively uniform value of 0.20 mg m-3 from 160°W to the Galapagos, where Chl-a reached 0.45 mg m-3. Eastward from 150°E, Chl-a values in the average typical La Niña increased approximately linearly to 0.21 mg m-3 at 170°E, where Chl-a was 175% larger than that in the average typical El Niño. Chl-a values in the average typical La Niña were approximately 0.22 mg m-3 until the Galapagos, where values reached 0.55 mg m-3. Average Chl-a values in the super El Niño event in 2015-2016 were similar to those associated with the average typical El Niño, but the bottom of the bowl-shaped pattern was shallower and wider. However, the longitudinal pattern of Chl-a in the super El Niño of 1997-1998 differed significantly from the patterns of the average typical El Niño and super El Niño of 2015-2016. Also, Chl-a distributions in the Atlantic and Indian oceans will be described. Correlations between satellite surface wind vector measurements and Chl-a in El Niño and La Niña were not always consistent with the hypothesis of the important contribution of Ekman upwelling and will be discussed.