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§16.1  The Spectrum  of  Electromagnetic Radiation  489

                            log 10 A
                          17
                          16
                          15
                          14
                   l k m -  13
                          12
                                                       Electrical conductor
                          ц   Radio waves             - carrying alternating
                                                       current
                    1  m-  10


                   1 cm-
                  1 mm-   7

                          6
                                Far infrared           Molecular rotations
                          5      I
                                Near  infrared         Molecular vibrations
                    1/x,-  4  .
                                         i    i  Visible  -л  Displacement  of  outer
                          3          Ultraviolet —      electrons  of  an  atom
                                         i
                          2
                   1  m/x-  1     x-rays               Displacement  of  inner
                                                         \
                                                               ,
                                                       electrons  of  an  atom
                                     J
                    1  A-  0
                          -1                           Displacement of nucleons
                             y-rays                    .  r
                          -2                           in an atomic nucleus
                         u
                          - 3 -
                  Fig. 16.1-1.  The spectrum  of electromagnetic radiation, showing
                  roughly  the mechanisms by  which various  wavelengths  of radiation
                                                    8
                  are produced  (1 A  = Angstrom  unit =  1СГ  cm = 0.1 nm; l/x  = l  mi-
                           6
                  cron  = 10"  m).

                  Here h  =  6.626  X  10  34  J-s is  Planck's  constant. From these two  equations and  the  infor-
                  mation from  Fig. 16.1-1, we  see that decreasing  the wavelength  of electromagnetic radia-
                  tion corresponds  to increasing  the energy  of  the corresponding photons. This  fact  ties in
                  with  the various  mechanisms  that produce  the radiation.  For example,  relatively  small
                  energies  are released  when  a molecule decreases  its speed  of rotation, and the  associated
                  radiation  is  in  the  infrared.  On  the  other  hand,  relatively  large  energies  are  released
                  when  an atomic nucleus goes  from  a high energy  state to a lower  one, and the associated
                  radiation  is  either  gamma-  or  x-radiation.  The  foregoing  statements  also  make  it  seem
                  reasonable  that the radiant energy  emitted from  heated  objects  will tend toward  shorter
                  wavelengths  (higher energy  photons) as the temperature of the body  is  raised.
                      Thus far we have sketched the phenomenon of the emission  of radiant energy  or pho-
                  tons when  a molecular  or atomic system  goes  from  a high  to a low  energy  state. The re-
                  verse  process,  known  as  absorption,  occurs  when  the  addition  of  radiant  energy  to  a
                  molecular  or  atomic system  causes  the system  to go  from  a  low  to a  high  energy  state.
                  The latter  process  is  then what  occurs when  radiant energy  impinges  on a  solid  surface
                  and causes  its temperature to rise.
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