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4







               INTRODUCTION TO SOLAR POWER


               SYSTEM DESIGN
















               Essential steps required for solar power systems engineering design include site eval-
               uation, feasibility study, site shading analysis, photovoltaic mapping or configuration
               analysis, dc-to-ac power conversion calculations, PV module and inverter system
               selection, and total solar power array electric power calculations.
                  In previous chapters we reviewed the physics, manufacturing technologies, and
               design considerations applied to photovoltaic solar power cogeneration systems. This
               chapter is intended to provide a pragmatic approach for designing solar power systems.
                  In order to have a holistic understanding of solar power cogeneration systems,
               designers must have a basic appreciation of insolation concepts, shading analysis, and
               various design parameters that affect the output performance and efficiency of the
               overall system. In view of the California Solar Initiative (CSI) and other state rebate
               programs, which will be discussed in future chapters, the importance of system
               performance and efficiency form the foundation that determines whether a project
               becomes financially viable.


               Insolation


               The amount of energy that is received from the sun rays that strike the surface of our
               planet is referred to as insolation (I). The amount of energy that reaches the surface of
               Earth is by and large subject to climatic conditions such as seasonal temperature
               changes, cloudy conditions, and the angle at which solar rays strike the ground.
                  Because our planet revolves around the sun in an oval-shaped orbit with its axis
               tilted at approximately 23.5 degrees, the  solar declination angle (i) (shown in
               Figure 4.1) constantly varies throughout the revolution, gradually changing from
               +23.5 degrees on June 21–22, when Earth’s axis is tilted toward the sun, to −23.5
               degrees by December 21–22, when Earth’s axis is tilted away from the sun. Earth’s

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