Page 162 - Intro to Space Sciences Spacecraft Applications
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Spectral (Radiometric) Performance            Remote Sensing   149


                        The spectral performance of a sensor depends on the frequency (or wave-
                      length) of the radiation which the sensor is designed to detect. The wave-
                      length(s) used  to make a measurement is selected based on the radiative
                      (radiometric) properties of  the target and/or on other considerations, such
                      as  interaction  with  or  avoidance of  the  atmosphere or  ionosphere. For
                      instance, in clouds, water occurs as aerosol-sized particles of liquid rather
                      than vapor. Clouds absorb and scatter electromagnetic radiation at wave-
                      lengths less than about 0.3 cm. Sensors are designed to take advantage of
                      this  effect  to  measure  atmospheric  characteristics.  Only  radiation  of
                      microwave and longer wavelengths is capable of penetrating clouds without
                      being significantly scattered, reflected, or absorbed. These (radar) fkequen-
                      cies are commonly used when information below cloud layers is desired.
                        The spectral performance of a system is a measure of how well the sys-
                      tem  uses  these  frequencies  (or  combinations  of  frequency ranges)  to
                      extract information on a desired target. Much of the success of a remote
                      sensor depends on knowledge of the radiometric properties of the target.
                      These targethcene characteristics determine the relative strength or inten-
                      sity of  observed signals based  on their reflectance, absorption, or other
                      properties for the particular frequencies involved.

                      Temporal Performance

                        The  temporal  performance of  a  remote  sensor is  a  function  of  the
                      repeated observations of  a phenomenon based  on the expected rate of
                      changes in that phenomenon. Global winds change on an hourly or daily
                      basis while changes in the earth’s geodetic shape or magnetic field may
                      take years or millennia to occur. The observation rate of  a specific phe-
                      nomenon or area is a function of the orbit in which the satellite is placed
                      and the sensor FOV produced by the scan pattern. An orbit and scan pat-
                      tern can be preferentially designed to create a revisit sequence and local
                      time observation tailored to a particular application.




                         Early remote sensing satellites were  technology and  lift capacity con-
                      strained, resulting in relatively simple sensors designed to observe singular
                      regions of the electromagnetic  spectrum. Modem satellites tend to maximize
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