Page 156 - Rashid, Power Electronics Handbook
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10  Diode Recti®ers                                                                                 145

                 10.3.1 Three-Phase Star Rectifiers
                 10.3.1.1 Basic Three-Phase Star Rectifier Circuit
                 A basic three-phase star recti®er circuit is shown in Fig. 10.7.
                 This circuit can be considered as three single-phase half-wave
                 recti®ers combined together. Therefore, it is sometimes
                 referred to as a three-phase half-wave recti®er. The diode in
                 a particular phase conducts during the period when the
                 voltage on that phase is higher than that on the other two     FIGURE 10.7  Three-phase star recti®er.
                 phases. The voltage waveforms of each phase and the load are
                 shown in Fig. 10.8. It is clear that, unlike the single-phase
                 recti®er circuit, the conduction angle of each diode is 2p=3,  sum to zero. Therefore, it is preferable not to have star-
                 instead of p. This circuit ®nds uses where the required dc  connected primary windings.
                 output voltage is relatively low and the required output
                 current is too large for a practical single-phase system.  10.3.1.2 Three-Phase Inter-Star Rectifier Circuit
                   Taking phase R as an example, diode D conducts from p=6
                                                                      The transformer core saturation problem in the three-phase
                 to 5p=6. Therefore, by using Eq. (10.1) the average value of the
                                                                      star recti®er can be avoided by a special arrangement in its
                 output can be found as
                                                                      secondary windings, known as zig-zag connection. The modi-
                                                                      ®ed circuit is called the three-phase interstar or zig-zag
                                        ð 5p=6
                                      3
                                V ¼         V sin y dy        ð10:42Þ  recti®er circuit, as shown in Fig. 10.9. Each secondary phase
                                 dc
                                             m
                                     2p  p=6                          voltage is obtained from two equal-voltage secondary wind-
                                                                      ings (with a phase displacement of p=3) connected in series so
                 or                                                   that the dc magnetizing forces due to the two secondary
                                                                      windings on any limb are equal and opposite. At the expense
                                         p 
                                       3   3                          of extra secondary windings (increasing the transformer
                               V ¼ V  m     ¼ 0:827 V m       ð10:43Þ
                                dc
                                       p 2                            secondary rating factor from 1.51 VA=W to 1.74 VA=W), this
                                                                      circuit connection eliminates the effects of core saturation and
                 Similarly, using Eq. (10.6), the rms value of the output voltage  reduces the transformer primary rating factor to the minimum
                 can be found as                                      of 1.05 VA=W. Apart from transformer ratings, all the design
                                                                      parameters of this circuit are the same as those of a three-
                                    s 
                                        ð 5p=6                        phase star recti®er (therefore, they are not separately listed in
                                      3            2
                               V ¼          ðV sin yÞ dy      ð10:44Þ
                                              m
                                L
                                     2p  p=6
                 or
                                         p
                                s 
                                           
                                  3   p    3
                         V ¼ V m       þ      ¼ 0:84 V m      ð10:45Þ
                          L
                                  2p 3    4
                 In addition, the rms current in each transformer secondary
                 winding can also be found as
                               s 
                                        p
                                          
                                 1   p    3
                         I ¼ I m      þ      ¼ 0:485 I m      ð10:46Þ
                          s
                                 2p 3    4
                 where I ¼ V =R.
                             m
                        m
                   Based on the relationships stated in Eqs. (10.43), (10.45)
                 and (10.46), all the important design parameters of the three-
                 phase star recti®er can be evaluated as listed in Table 10.3.
                 Note that, as with a single-phase half-wave recti®er, the three-
                 phase star recti®er shown in Fig. 10.7 has direct currents in the
                 secondary windings that can cause a transformer core satura-  FIGURE 10.8  Waveforms of voltage and current of the three-phase star
                 tion problem. In addition, the currents in the primary do not  recti®er as shown in Fig. 10.7.
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