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SIBER SPIS sept 2011.pdf - IMBER

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<strong>SIBER</strong><br />

Science Plan and Implementation Strategy<br />

Re m o t e s e n s i n g s t u d i es<br />

The obvious starting point for carrying out regional studies in the IO is through the application<br />

of remote sensing to characterize physical and biological variability of these systems. Relevant<br />

measurements, with corresponding representative mission(s) with NASA as a principal<br />

contributor, include satellite ocean color (SeaWiFS, MODIS-Aqua), sea surface temperature<br />

(SST) (NOAA/AVHRR, MODIS-Terra/Aqua), sea surface height (SSH) (T/P and Jason), surface<br />

vector winds (QuikSCAT) and precipitation (TRMM). Remote sensing should be applied<br />

specifically to study the seasonal variability and transitions in IO boundary current systems,<br />

to define and characterize the dominant scales of spatial variability and also to characterize<br />

interannual variability, especially as it relates to climate change. Interdisciplinary remote sensing<br />

studies must seek to elucidate both the physical (SST and SSH) and biological (chlorophyll<br />

and primary production) dynamics and understand the impact of physical oceanography on<br />

biological processes in the IO. In addition to studies based upon the US deployed satellites<br />

noted above, opportunities exist to utilize remote sensing data obtained via other national<br />

agencies or multi-national consortia. For example, India’s Oceansat-1 and recently launched<br />

Oceansat-2 provide physical (SST and wind) and ocean color measurements starting from<br />

1999; straightforward provision of these high-resolution data to non-Indian scientists needs<br />

to be ensured. The European Space Agency (ESA) has also launched a number of satellite<br />

missions (e.g. ERS-1,2 and Envisat) that provide ongoing measurements of ocean color<br />

(MERIS), SST (AATSR), SSH (RA-2) and winds (ASCAT). In addition, since November 2009,<br />

ESA’s SMOS (Soil Moisture and Ocean Salinity) mission has been providing the first regular<br />

global mapping of sea surface salinity (SSS) (Berger et al., 2002). This remote sensing<br />

capability will soon be reinforced with the launch of NASA’s Aquarius mission that will also<br />

provide SSS measurements (Lagerloef et al., 2008). The continuous observations of SSS<br />

provided by SMOS and Aquarius will address a manifest need that <strong>SIBER</strong> should capitalize<br />

on, given the influence that the hydrological cycle exerts on the dynamics of the northern and<br />

eastern IO.<br />

As with boundary current studies, satellite observations can and should play a central role<br />

in studying seasonal, intraseasonal and interannual biogeochemical variability of equatorial<br />

waters of the IO. Many of the phenomena discussed above in Theme 2 are amenable to satellite<br />

studies, i.e. characterization of the typical annual cycle in surface temperature, sea surface<br />

height, chlorophyll and primary production and the physical and biogeochemical responses to<br />

perturbations associated with the IOD, the MJO, Wyrtki Jets and other high frequency forcing<br />

phenomena such as cyclones. Retrospective studies should be motivated. The satellite SST<br />

measurements based upon the AVHRR have been reprocessed and extend back in time to<br />

1981, i.e. that is a 30-year record. This record has been used to demonstrate warming globally,<br />

including the prominent response observed in the IO (Arguez et al., 2007). In the often cloudy<br />

regions of the IO, the SST microwave data (TMI and AMSR-E) are very useful, thanks to<br />

their ability to “see through clouds” and monitor strong cooling under convective systems (e.g.<br />

Duvel et al., 2004; Harrison and Vecchi, 2001).<br />

Ocean color data acquired by SeaWiFS, MODIS and other orbiting sensors extend from 1997<br />

to the present. These datasets have already been utilized to reveal anomalous biological<br />

distributions during IOD manifestations (Murtugudde et al., 1999; Wiggert et al., 2002) and<br />

phytoplankton bloom characteristics along the equator and within the STIO (Lévy et al., 2007;<br />

Uz, 2007; Wiggert et al., 2009) and blooms associated with the MJO in the SCTR (McCreary<br />

et al., 2009; Resplandy et al., 2009). However, more comprehensive elaboration of IO bloom<br />

dynamics and biophysical processes, and how these are impacted by the IOD, are needed.<br />

There has also been considerable effort in recent years to extend the utility of ocean color<br />

measurements from SeaWiFS and MODIS to provide estimates of net primary production<br />

and phytoplankton physiological state (Behrenfeld et al., 2005; Behrenfeld et al., 2009) and<br />

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