Introduction to the Physics and Techniques of Remote Sensing. Jakob J. van Zyl
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images on demand in many different modes. Satellites are now acquiring images of other planets in more spectral channels and with better resolutions than what was available for the Earth two decades ago. And as the remote sensing data have become more available, the number of applications has grown. In many cases, the limitation now has shifted from the technology that acquires the data to the techniques and training to optimally exploit the information embedded in the remote sensing data.
Figure 1.11 Sea surface temperature derived from ship observations (a) and from the Seasat Multispectral Microwave Radiometer (b). (c) shows the difference.
Source: From Liu (1983). © 1983, John Wiley & Sons.
Figure 1.12 Backscatter data acquired over the Amazon region (insert). The different curves correspond to different incidence angles. Data were acquired by the Seasat Scatterometer at 14.6 GHz and at VV polarization.
Source: Bracalante et al. (1980). © 1980, IEEE.
Figure 1.13 Profile of Tharsis region (Mars) acquired with Earth‐based radar.
Figure 1.14 Profiles of an unnamed impact basin on Mars using Earth‐based radar. The set of profiles shown correspond to the box overlay on the figure.
1.3 Remote Sensing Space Platforms
Up until 1946, remote sensing data were mainly acquired from airplanes or balloons. In 1946, pictures were taken from V‐2 rockets. The sounding rocket photographs proved invaluable in illustrating the potential value of photography from orbital altitudes. Systematic orbital observations of the Earth began in 1960 with the launch of Tiros I, the first meteorological satellite, using a low‐resolution imaging system. Each Tiros spacecraft carried a narrow‐angle TV, five‐channel scanning radiometer, and a bolometer.
In 1961, orbital color photography was acquired by an automatic camera in the unmanned MA‐4 Mercury spacecraft. This was followed by photography acquired during the Mercury, Gemini, Apollo, and Skylab missions. On Apollo 9, the first multispectral images were acquired to assess their use for Earth resources observation. This was followed by the launch in 1972 of the first Earth Resources Technology Satellite (ERTS‐1, later renamed Landsat‐1), which was one of the major milestones in the field of Earth remote sensing. ERTS‐1 was followed by the series of Landsat missions.
Figure 1.15 Sea surface height over two trenches in the Caribbean acquired with the Seasat altimeter.
Source: Townsend (1980). © 1980, IEEE.
Figure 1.16 Shaded relief display of the topography of California measured by Shuttle Radar Topography Mission using an interferometric SAR.
Figure 1.17 Subsurface layering in the ice cover and bedrock profile acquired with an airborne electromagnetic sounder over a part of the Antarctic ice sheet.
Earth orbital spacecraft were also used to acquire remote sensing data other than regular photography. To name just a few, the Nimbus spacecraft carry passive microwave radiometers, infrared spectrometers, and infrared radiometers. The Synchronous Meteorological Satellite (SMS) carried visible and IR spin‐scan cameras. Skylab (1972) carried a radiometer and a radar scatterometer. Seasat (1978) carried an imaging radar, a scatterometer, and an altimeter.
In the 1980s and 1990s, the Space Shuttle provided an additional platform for remote sensing. A number of shuttle flights carried imaging radar systems. In particular, the Shuttle Radar Topography Mission, flown on the Space Shuttle in 2000, allowed global mapping of the Earth’s topography.
Remote sensing activity was also expanding dramatically using planetary spacecraft. Images were acquired of the surfaces of the Moon, Mercury, Venus, Mars, the Jovian and Saturnian satellites, Pluto, numerous Asteroids and comets, and of the atmospheres of Venus, Jupiter, Saturn Uranus, and Neptune. Other types of remote sensors, such as radar altimeters, sounders, gamma‐ray detectors, infrared radiometers, and spectrometers were used on a number of planetary missions.
The use of orbiting spacecraft is becoming a necessity in a number of geophysical disciplines because they allow the acquisition of global and synoptic coverage with a relatively short repetitive period. These features are essential for observing dynamic atmospheric, oceanic, and biologic phenomena. The global coverage capability is also essential in a number of geologic applications where large‐scale structures are being investigated. In addition, planetary rovers are using remote sensing instruments to conduct close‐up analysis of planetary surfaces. Over the last decade, with the advances in detectors, light optics, microwave technology, antennas, materials, spacecraft technology and data systems, there has been a great expansion in the development, deployment, and utilization of remote sensors. These will be discussed throughout this textbook.
1.4 Transmission Through the Earth and Planetary Atmospheres
The presence of an atmosphere puts limitations on the spectral regions that can be used to observe the underlying surface. This is a result of wave interactions with atmospheric and ionospheric constituents leading to absorption or scattering in specific spectral regions (Figure 1.19).
Figure 1.18 Comparison of temperature profiles acquired with a microwave sounder (NEMS)