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Coined in the 1960s by a geographer named Evelyn Pruitt, the term remote sensing refers to the collection of data about Earth's surface (and atmospheric) features or phenomena without being in direct contact with such features or phenomena. This entry first provides background on electromagnetic radiation (EMR), which is the information link that enables the collection of data about Earth's surface without being in contact with the surface. Next, the entry discusses sensors that capture EMR and are mounted on platforms (aircraft or satellite), which enables the remote collection of different types of imagery. Finally, the principles and strategies of image interpretation for extracting geographic information are covered.

There are advantages and disadvantages in using remote sensing technology for geographic research and applications, relative to more conventional, ground-based or in situ (i.e., direct) observation methods. The primary advantage is that remote sensing enables spatially continuous and contiguous, large-area sampling of Earth's surface and atmosphere. This means that data are comprehensive, synoptic (i.e., many features are observed simultaneously), and efficiently collected. Other advantages are the noninvasive, nondisturbing nature of sensing remotely and the ability to collect data for areas that are inaccessible or inhospitable for making observations on the ground. Often, historical information on geographic features or conditions can only be derived through interpretation of archived imagery captured in the past. The main disadvantages of remote sensing are that remote observations are less detailed and precise and more uncertain than direct measurements made on the ground. Also, the sensing process, the image-processing steps, and the act of image interpretation all can yield more artifacts (i.e., false information) than would normally result when making in situ observations.

Electromagnetic Radiation: The Information Link

EMR is the important link that enables information about Earth's surface to be extracted. As the term suggests, both electric and magnetic fields are associated with EMR transfer, which can occur even in the absence of matter (i.e., in a vacuum). The orientation of the electric field determines the polarization of EMR. EMR travels at the same speed (the speed of light, or 300,000,000 m [meters] per second) through outer space and, effectively, through Earth's atmosphere, irrespective of wavelength or frequency. Wavelength and frequency are inversely related (i.e., short-wavelength EMR is high-frequency EMR).

All matter emits EMR, and the wavelength of emitted radiation is an inverse linear function of the temperature of the emitting material. A change in the electrical charge of matter, which can result from atomic-level changes in energy states or molecular-level motions such as vibration and rotation, causes EMR to be emitted. The sun emits shortwave radiation in an amount that is approximately equal to a blackbody (defined as a perfectly absorbing material that is in thermal equilibrium) having a temperature slightly less than 6,000 Kelvin. Earth's surface reflects incoming solar radiation (called solar irradiance) and emits long-wave radiation. The actual amount of radiation emitted by Earth surfaces also depends on the emissivity properties of different materials, which pertains to the efficiency of emission relative to a blackbody at the same temperature. Most of the EMR emitted by Earth surfaces is radiated within the thermal-infrared (TIR) part of the EMR spectrum at wavelengths ranging from 3 to 30 µm (micrometers), where 1 µm = 10–6 m.

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