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Remote sensing acquires and interprets small or large-scale data about the Earth from a distance. Using a wide range of spatial, spectral, temporal, and radiometric scales remote sensing is a large and diverse field for which this Handbook will be the key research reference. Illustrated throughout, an essential resource for the analysis of remotely sensed data, The SAGE Handbook of Remote Sensing provides researchers with a definitive statement of the core concepts and methodologies in the discipline.

Optical Remote Sensing of the Hydrosphere: From the Open Ocean to Inland Waters

Optical remote sensing of the hydrosphere: From the open ocean to inland waters

Keywords

ocean colour, marine optics, phytoplankton and satellite oceanography.

Introduction

This chapter will primarily deal with optical remote sensing, but also mentions the use of sensors that cover the wider breadth of the electromagnetic spectrum as there is an increasing focus on sensor synergy and what all forms of remote sensing can tell us. Optical remote sensing is the detection (primarily from airborne and satellite-mounted sensors, but can also include ship and ground-mounted sensors) of the incident sunlight, in the visible and near infra-red (NIR) parts of the electromagnetic spectrum, reflected from the surface after passive interaction with the water and its constituents. Ocean colour is the spectral variation of water-leaving radiance, Lw (downwelling solar irradiance that penetrates the water surface, interacts with the water body and is backscattered towards the sensor), that can be related to the concentrations of the optically active constituents such as phytoplankton pigments, coloured dissolved organic material (CDOM) and suspended particulate matter (SPM). This chapter introduces the technology of hydrospheric optical remote sensing through a discussion of the sensors commonly used, followed by a description of the associated techniques that have been developed to determine biogeochemical variables. A short discussion of example applications and a brief summary of the current status and future trends of the field conclude the chapter.

The Past, Present and Future

The History of Satellite Ocean Colour

The first spaceborne ocean colour images were obtained through hand-held cameras on the manned space missions in the 1960s and they clearly demonstrated the potential of satellites for monitoring SPM along the coasts, and the colour variation due to phytoplankton (e.g., Badgley and Childs 1969). The first quantitative work was undertaken by Clarke et al. (1970) who used an airborne spec-troradiometer to record the spectral variation of water-leaving radiance above waters with different phytoplankton concentrations. The observations demonstrated a change in the water-leaving radiance spectra with increasing chlorophyll-a concentrations (chl), and that the atmosphere had a notable effect, namely that scattering increased as measurements were recorded at increasing altitude.

Satellite monitoring of the coastal zone was made possible by the Earth Resources Technology Satellite (later renamed Landsat, with Landsat-1 launched in July 1972; Goward et al., in this volume), but the first dedicated marine sensor was the Coastal Zone Color Scanner (CZCS) launched in October 1978 onboard the Nimbus-7 satellite. Ocean colour satellites have generally been launched into polar orbits (following a path that passes close to the North and South Poles) so that almost the entire Earth is covered, with a small amount of overlap at low latitudes and a greater overlap at higher altitudes, as different parts of the Earth's surface are viewed during successive orbits.

CZCS was a proof of concept sensor with a number of design specifications and objectives that included defining requirements for future ocean colour instruments. The sensor recorded the upwelling visible radiance in four wavebands (Table 27.1) with a broad NIR waveband to differentiate sea from land and cloud, and a thermal infra-red band (10.5–12.5 μm) to detect Sea Surface Temperature (SST) variability. CZCS also possessed a tilting mechanism, which pointed the scan plane up to 20 degrees forward or aft of nadir along track, which helped the sensor avoid sunglint (sunlight reflected from the sea-surface without interacting with the components within the water). Finally, the detectors had four gain settings to allow observations at a range of radiance levels and hence sun angles. However, CZCS was operated on an intermittent schedule (due to power demands), the sensor lost the thermal infrared waveband within the first year, and the other wavebands began degrading from 1981 onwards, although they remained useable to some degree until 1984.

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