Polar-Orbiting Satellites

Polar-Orbiting Satellites

A disadvantage of geostationary satellites (Figure 9) is that their large distance from the earth's surface compromises their ability to capture fine detailed resolution of the planet surface. Satellites put in low earth orbit, typically 850 km (531 miles) above the surface, can resolve topographic and other environmental features as small as 1 km, and perhaps even much smaller. However, this close proximity to the earth's surface limits their field of view to a swath about 2,500 km (1,560 miles) wide as the satellite orbits the planet. Maximum areal coverage is achieved if the satellite orbits from pole to pole (Figure 10). By use of the last equation of the height derivation, with a satellite height above ground of 850 km, we get an orbital period of about 100 minutes. The satellite orbiting from pole to pole crosses the equator going from south to north every 100 minutes, and between these equator crossings the planet will have rotated by 28.8o. This allows the satellite to view a new swath that is adjacent to the west of the swath from the previous pass. By manipulating the height of the satellite, as can be seen from the equation for satellite period, the orbital period can be adjusted to give the desired degree of overlap between adjacent sweeps across the equator. Polar orbiting satellites are sufficiently close to the earth's surface to acquire high resolution data (Figure 11).

The NOAA website provides updated information on polar orbiting satellites.

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