Page 158 - Intro to Space Sciences Spacecraft Applications
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Remote Sensing
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                      shows a portion of the infrared spectral band and not the entire electro-
                      magnetic spectrum. Frequency ranges with poor transmissivity are known
                      as absorption bands, while regions where radiations pass through rela-
                      tively unaffected are called windows. As an example, we can see well dur-
                      ing the day because the atmosphere is practically transparent to the visi-
                      ble frequency range; but a couple of hours at the beach doesn’t burn us too
                      badly because most of the ultraviolet radiations of the sun are absorbed
                      high in the atmosphere. A particular remote sensor’s purpose may be to
                      observe and measure some phenomenon at the earth’s surface, in which
                      case it must negotiate frequencies with significant atmospheric absorption
                      and  use  the  window  frequencies.  Many  sensors,  sometimes  called
                      sounders, wish to measure atmospheric or ionospheric conditions and will
                      intentionally select frequencies of observation that interact with and mea-
                      sure high-altitude phenomena.
                        The component of the total energy received by the remote sensor from
                      just the su$ace  is given by:





                      where




                      which shows the dependency of the received energy on the spectral output
                      of the sun F,)  and the effects of the transmissivity z(k) on the energy prop-
                      agation.  Similar  equations  exist  for  the  other  components  of  the  total
                      received energy which are also dependent on these factors. The total ener-
                      gy received by the remote sensor is the sum of these radiations which, when
                      expressed in equation form, constitute the radiative transfer equation:




                      where the total Rayleigh scattered input is given by IqtOt,, and I*  is the
                      received aerosol scattered component.
                        The reduction of this raw received information is quite complicated and
                      requires some prior knowledge of the behavior of the atmosphere. Over
                      many years, algorithms have been developed which are used to reduce the
                      unrefined sensor source or raw data and identify the physical processes
                      which contribute to the total energy received by the remote sensor. Algo-
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