Chapter 5 EO—Spectral Imagery The discussion of remote sensing up to this point has focused on panchromatic (black & white) imagery. Beyond recording obvious features of size and shape, remote sensing excels in capturing and interpreting color. Color systems also yield some spectacular imagery. For example, in this early “true-color” image from Landsat 7, we perceive the green hillsides and muddy runoff of the upper San Francisco bay (Fig. 5.1). 5.1 Reflectance of Materials The reflectance of most materials varies with wavelength. This allows spectral imagers, such as those on the Landsat missions, to distinguish different materials. Distinguishing between minerals is a fairly common goal for such work by geologists. In Fig. 5.2, different aspects of reflective spectra are illustrated. Spectra are the fingerprints of elements, deriving from their fundamental atomic characteristics, as indicated in our discussion of Bohr’s model of the hydrogen atom. One of the more important, and dramatic, spectral features found in remote sensing is the “IR ledge” at 0.7 µm, as found in Fig. 5.2.1 This dramatic rise in reflectance with wavelength makes vegetation appear bright in the infrared (old-style, black-and-white infrared film would show vegetation as white, for example). The military designs camouflage to mimic this behavior. The panchromatic sensors on Landsat, SPOT, IKONOS, and Quickbird extend well into the infrared, and as a result, vegetation is bright in their imagery. 1 Also occasionally termed the “red edge,” e.g., in D.N.H. Horler, M. Dockray, and J. Barber, “The red edge of plant leaf reflectance,” Int. J. Remote Sens. 4, pp. 273–288 (1983). 117 118 Chapter 5 Figure 5.1 Visible image of San Francisco from Landsat 7, April 23, 1999, flight day 9, orbit 117. ~1830Z With special thanks to Rebecca Farr, NESDIS/NOAA. The satellite is not yet in its final orbit, and not on the standard reference grid, WRS, so the scene is offset 31.9 km east of nominal scene center (Path 44, Row 34). Landsat has been the premier Earth resources satellite system for three decades. 5.2 Human Visual Response2 Before considering the spectral response of orbital systems, let’s consider human visual response. The sensitive elements of the eye are the rods and cones. Rods (which far outnumber cones) are sensitive to differences in brightness within the 2 See W.L. Teng, E.R. Loew, D.I. Ross, V.G. Zsilinsky, C. Lo, W.R. Philipson, W.D. Philpot, S.A. Morain, “Fundamentals of Photographic Interpretation,” 2nd ed. in Manual of Photographic Interpretation. W.R. Philipson (Ed.), American Society for Photogrammetry and Remote Sensing, Bethseda, MD, p. 67 (1997). Also see H.J.A. Dartnall, J.K. Bowmaker, and J.D. Mollon, “Microspectrophotogrammetry of Human Photorecepters,” in Color Vision: Physiology & Psychophysics, John Mollon, L. Ted Sharpe (Eds.), Academic Press, London (1983). EO—Spectral Imagery 119 Figure 5.2 Reflectance for some manmade and natural materials. Note how the olive-green paint mimics the grass spectrum in the visible to NIR, but then deviates. Figure 5.3 Human vision: The white curves indicate the sensitivity level for the three types of cones. The black curve indicates the sensitivity of the rods.3 middle of the light spectrum. The rods’ peak sensitivity corresponds to the peak in solar illumination. If we had only rods, we would see in shades of grey. 3 3 See John E. Dowling, The Retina: An Approachable Part of the Brain, Harvard University Press, Cambridge, Mass., (1987). See also H.J.A. Dartnall, J.K. Bowmaker, and J.D. Mollon, “Human Visual Pigments: Microspectrophotometric Results from the Eyes of Seven Persons,” Proceedings of the Royal Society of London B, 220 (1218), pp. 115–130 (1983). 120 Chapter 5 Cones provide our color vision. There are three types of cones: L-cones are sensitive primarily to red in the visible spectrum. M-cones are sensitive to green. S-cones are sensitive to blue. 5.3 Landsat In late July 1972, NASA launched the first Earth-Resources Technology Satellite, ERTS-1. The name of the satellite, and those that followed, was soon changed to Landsat. These have been the primary Earth-resources satellites ever since, utilizing multispectral imagery (MSI) with a spatial resolution of 30 m. The most recent in the series, and perhaps the last, is Landsat 7. The table below shows some of the parameters for the sequence of missions. Note the evolution in data storage technology, bandwidth, and the changes in downlink technology. Resolution has gradually increased with time. Landsat 7 added a 15-m GSD panchromatic sensor to the MSI sensors. Figure 5.4 shows the satellite orbit, and illustrates the 185-km viewing swath for the Enhanced Thematic Mapper (ETM) sensor, described below. The figure also reflects the different downlink options, as the sensor communicates with the Landsat Ground Station (LGS). Table 5.1 Landsat sensors and orbits. Satellite Landsat 1 (ERTS-A) Landsat 2 Landsat 3 On-Orbit/ Operating July 23, 1972– January 6, 1978 January 22, 1975–February 25, 1982 March 5, 1978– March 31, 1983 July 16, 1982–* Sensors*** MSS RBV MSS RBV MSS RBV Landsat 4 MSS TM Landsat 5** March 1, 1984– MSS to date TM Landsat 7 April 15, 1999–to ETM+ date (pan) Resolution (m) 80 80 80 80 80 30 80 30 80 30 30 15 Altitude (km) 917 Data Link 705 Direct downlink w/TDRSS (85 Mbps) Direct downlink w/recorder (15 Mbps) Direct downlink w/solid state recorders (150 Mbps) * TM data transmission failed in August 1993; satellite was used for maneuver testing. ** Landsat 6 failed due to a launching problem. *** RBV: Return Beam Vidicon; MSS: Multi-Spectral Scanner; TM: Thematic Mapper EO—Spectral Imagery 121 Figure 5.4 The nadir-viewing satellite images a swath 185 km wide. Figure 5.5 Subsequent orbits are displaced by some 2500 km to the west. There are 233 unique orbit tracks. 5.3.1 Orbit The Landsat missions have been sun-synchronous polar orbiters in circular orbits (LEO). The later missions operating at an altitude of 705 km. NASA’s Mission to Planet Earth has added several satellites in the Landsat 7 orbit—Terra, Aqua, SAC-C, and EO-1. They trail the older satellite by a few minutes in orbital sequence. An inclination of ~97° makes them sun-synchronous. Equatorial crossings were set at 9:30 am for Landsats 1, 2, and 3; 10:30 am for Landsats 4 and 5; and 10:00 am for Landsat 7. Landsats 4, 5, and 6 have orbit tracks set for 14.5 orbits per day. The repeat cycle is every sixteen days. Figure 5.5 shows the orbit track, and shows how the orbit shifts in local time (longitude). The orbit track for Landsat 7 is further illustrated in Fig. 5.6. The ground track is illustrated for 2 orbits. The satellite is on an ascending node on the night side, and descends southward on the day side. 122 Chapter 5 Figure 5.6 This orbit ground track corresponds to the San Francisco image above. The yellow spot just below Mexico City is the sub-solar point, April 23, 1999, ~1830Z. 5.3.2 Sensor: Thematic Mapper4 The first Landsats flew with a multispectral (MSS) imager and a TV-like sensor (the return-beam vidicon, or RBV). Beginning with Landsat 4, the primary instrument became the Thematic Mapper (TM), though the MSS was also carried to maintain continuity in archival, synoptic datasets. The TM sensor has provided seven bands of spectral information at 30-m resolution since 1982. On the most recent vehicle, Landsat 7, the instrument was revised as the Enhanced Thematic Mapper plus, or ETM+. The instrument features improved spatial resolution in the LWIR channel (60 m) and a new panchromatic band with higher spatial resolution (15 m). The discussion that follows addresses the ETM+ sensor. 5.3.2.1 Optics The optical design of Landsat predates large linear or rectangular arrays; it is of whiskbroom design. The telescope is a Ritchey-Chrétien Cassegrain, as seen with several earlier systems. The primary mirror (outer) aperture is 40.64 cm; the clear inner aperture is 16.66 cm. The effective focal length is 2.438 m, and the aperture is f/6. The instantaneous field of view (IFOV) for one pixel of the high-resolution panchromatic sensor is 42.5 µrad. 4 See http://ltpwww.gsfc.nasa.gov/IAS/handbook/handbook_toc.html
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