Page 12 - 83 basic knowledge of astronomy
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where Ω could be, for example, a solid angle subtended by a radio source
                      (see Figure 10).


                      7.4    Power/Energy/Radiation Flux Density S

                      The power/energy/radiation flux density S is the quantity of radiation en-
                      ergy, over the whole frequency range, incoming through a cross section of
                      unit area, per unit time. Therefore,
                                                           ∞
                                                           Z
                                                      S =    S ν dν.                            (3)
                                                           0
                         When we are interested in the “received” power flux density only, we
                      restrict the range of integration to the observing bandwidth ∆ν, i.e.,
                                                           Z
                                                      S =    S ν dν.                            (4)
                                                          ∆ν
                                                                 −2
                         The unit of power flux density is: W m .

                      7.5    Spectral Energy Density per Unit Solid Angle u                      ν

                      The spectral energy density per unit solid angle, u ν (s), is the volume density
                      of the radiation energy incident from a certain direction s, per unit solid
                                                                                            −1
                      angle, and per unit frequency bandwidth. The unit is J m   −3  Hz −1  sr .
                                                        dσ
                                               s



                                                               c dt



                              Figure 11: Radiation energy per unit solid angle in a tube.

                         Let us consider a cylindrical tube with a cross section of area dσ perpen-
                      dicular to the ray propagation direction, and with a length cdt, which is the
                      distance travelled by the radiation during a time interval dt at light speed c
                                     8
                                           −1
                      ( = 2.998 × 10 m s ) (see Figure 11). The radiation energy dU ν (J Hz      −1
                       −1
                      sr ) per unit solid angle, and per unit frequency bandwidth, contained in
                      the cylinder may be expressed either in terms of the spectral energy density
                      per unit solid angle, u ν (s), or in terms of the intensity I ν (s), as:
                                                 dU ν = u ν (s) cdt dσ,
                                                 dU ν = I ν (s) dt dσ.                          (5)


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