SIBER SPIS sept 2011.pdf - IMBER
SIBER SPIS sept 2011.pdf - IMBER
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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