Ocean Colour


Ocean colour observations from NASA satellites have been routinely available for nearly two decades; initially with the launch of the SeaWiFS sensor in 1997, then MODIS Terra and Aqua in 1999 and 2002 and, most recently, with VIIRS on Suomi/NPP launched in 2012. 

While NASA has sought to make products from these missions available, they have typically been in the form of derived products (e.g. Chlorophyll-a) binned and mapped at 4 or 9 km resolution globally and often are also time-averaged. These data sets are often less suitable for coastal applications, developing regional algorithms, or for characterising product accuracy through in-situ matchups, where finer spatial resolution data is desired. 

To address these needs, the IMOS Ocean Colour Sub-facility has supported the assembly of Australasian Ocean Colour archives of raw data from all fours satellite missions and established a processing system, based on NASA’s standard ocean colour processing software (SeaDAS), at the National Computational Infrastructure (NCI).  The IMOS Ocean Colour Sub-facility also supports validation of this data through the assembly of an Australian Bio-Optical Data Base and the collection of in-situ observations.

Instrumentation and Data

Ocean colour data streams include water radiance from the DALEC ship-based and Lucinda Jetty SeaPRISM radiometers and optical properties from the in water measurements at Lucinda Jetty.

The Lucinda Jetty Coastal Observatory (LJCO) above and in-water optical measurements are acquired with the objective to support satellite validation and remote sensing algorithm development. Currently, LJCO is the only southern-hemisphere ocean colour validation site integrated into NASA’s AERONET-OC global network of ground-based radiometers and one of a few sites globally that combines the acquisition of both atmospheric and in-water optical measurements to help unravel the inaccuracies in remotely-sensed satellite ocean colour products due to the optical complexity of coastal waters and the overlying atmosphere. 

This system, the “Dynamic above water radiance and irradiance collector” (DALEC) was developed in Australia by “In situ Marine Optics (IMO)” and measures simultaneously sea and sky radiance together with down-welling hemispherical irradiance during autonomous ship-based deployments. The DALEC sensor head contains three compact hyper-spectral spectroradiometers (Carl Zeiss Monolithic Miniature Spectrometers), as well as a GPS and pitch and roll sensors, and is designed to be mounted on a boom positioned over the water, typically off the ship’s bow.

The IMOS Bio-Optical Data Base is unique in its nature as it collates all bio-optical data types collected by members of the Australian bio-optical community. The formats for the Bio-Optical Data Base were developed together with NASA’s Ocean Biology and Biogeochemistry Program. As such the holdings compare well with the international standards. This central location of bio-optical data has allowed for easier uptake by international space agencies such as NASA and European Space Agency (ESA) and international projects such as ESA’s Ocean Colour Climate Change Initiative (OC-CCI) and working groups under the International Ocean-Colour Coordinating Group (IOCCG).

The ocean colour data are available at multiple levels through the processing chain, ranging from at-sensor radiances through to at-surface reflectances, and derived in-water properties, including both standard NASA-supported and experimental products. Additionally it is possible to obtain these data at the various processing levels before they have been remapped or aggregated (in either space or time) enabling their use in a wider range of applications.