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                   IAM―Efficiency adjusting factor
  IAM is an acronym 
                  for Incidence Angle Modifier and is simply a numeric value 
                  with refers to the amount of available solar radiation 
                  striking the absorber of the collector A value of 1 is 
                  achieved when the collector is perpendicular to the suns rays, 
                  and therefore receiving maximum radiation. Any collector 
                  that is installed at a fixed angle (generally equal to the 
                  location's latitude), will experience decreased radiation 
                  levels (IAM value < 1) in the morning and afternoon when 
                  the sun is not perpendicular to the absorber surface. When 
                  comparing performance between flat plate collectors, evacuated 
                  tube collectors with a flat absorber, or those that using 
                  reflective panels,IAM is not very important because they 
                  usually have a fairly similar set of transversal and 
                  longitudinal IAM values. The value of most concern for fixed 
                  angle collectors is transversal IAM, as this reflects the 
                  solar radiation throughout the day. Longitudinal IAM is useful 
                  when looking at installation angle, and the changes in heat 
                  output throughout the year as angle of the sun above the 
                  horizon changes between winter and summer. The longitudinal 
                  and transversal IAM values for the Century Sun solar collector are 
                  as follows: 
                  
                  
                    
                    
                      | 
                         0  | 
                      
                         0o   | 
                      
                         10o   | 
                      
                         20o   | 
                      
                         30o   | 
                      
                         40o   | 
                      
                         50o   | 
                      
                         60o   | 
                      
                         70o   | 
                      
                         80o   | 
                      
                         90o   |  
                    
                      | 
                         Kq (longitudinal)   | 
                      
                         1.0   | 
                      
                         1.0   | 
                      
                         1.0   | 
                      
                         0.99   | 
                      
                         0.97   | 
                      
                         0.93   | 
                      
                         0.85   | 
                      
                         0.71   | 
                      
                         0.46   | 
                      
                         0.0   |  
                    
                      | 
                         Kq (transversal)   | 
                      
                         1.0   | 
                      
                         1.02   | 
                      
                         1.07   | 
                      
                         1.15   | 
                      
                         1.28   | 
                      
                         1.50   | 
                      
                         1.49   | 
                      
                         1.29   | 
                      
                         0.75   | 
                      
                         0.0   |    
                   As you can see FROM the above graph, Century Sun solar 
                  collector has a curve which is quite different to the other 
                  two collectors . This is due to the cylindrical absorber area, 
                  which passively tracks the sun throughout the day. At 40-50o 
                  there is no light lost between the tubes, and no tube overlap, 
                  hence a peak in relative performance. This is ideal, as during 
                  this period (mid morning through mid afternoon) solar 
                  isolation levels are quite highest. The peak at 70o provided 
                  by the ET-reflect is of little benefit as this angle 
                  corresponds to early morning or late afternoon when solar 
                  insolation levels are very low. The flat plate collector's IAM 
                  values DROP away FROM 1 as the angle increases, and as such 
                  solar conversion efficiency is only at peak levels at midday。 
                   
                  Because of the round shape of the solar tubes, 
                  the absorber passively tracks the sun FROM 40o either side of 
                  midday (9:20am to 2:40pm). The cosine adjusted IAM values 
                  confirm this, as the collector maintains a value of close to 1 
                  up until 40o, beyond which the tubes start to overlap and the 
                  relative surface area decreases. Flat plate collectors, and 
                  other collectors with flat absorbers display a fairly standard 
                  bell curve, only peaking at midday. 
                  
                  
                    
                    
                      | 
                            | 
                      
                         0o  | 
                      
                         10o  | 
                      
                         20o  | 
                      
                         30o  | 
                      
                         40o  | 
                      
                         50o  | 
                      
                         60o  | 
                      
                         70o  | 
                      
                         80o  | 
                      
                         90o  |  
                    
                      | 
                         AKT collector  | 
                      
                         1.0  | 
                      
                         1.0  | 
                      
                         1.01  | 
                      
                         1.02  | 
                      
                         1.06  | 
                      
                         0.95  | 
                      
                         0.69  | 
                      
                         0.45  | 
                      
                         0.17  | 
                      
                         0.0  |  
                    
                      | 
                         Flat Plate  | 
                      
                         1.0  | 
                      
                         0.97  | 
                      
                         0.91  | 
                      
                         0.82  | 
                      
                         0.71  | 
                      
                         0.57  | 
                      
                         0.4  | 
                      
                         0.19  | 
                      
                         0.03  | 
                      
                         0.0  |    To 
                  understand how the tubes passively track the sun throughout 
                  the day, refer to the diagram below 
 
  When looking 
                  at the tubes FROM above (0o) each tube's surface is clearly 
                  visible, and therefore exposed to the maximum amount of 
                  sunlight. At this angle however some light is lost between the 
                  tubes, and therefore because this is used as a reference point 
                  for the IAM value of 1, when the gaps close up, the IAM value 
                  with actually increase (a greater % of light shining on the 
                  collector is actually being absorbed).
  When the sun 
                  reaches an angle of 40o which correlates to 2h 40min before or 
                  after midday, the solar tubes are still fully visible with no 
                  gaps between, and no overlap. It is at this point that the 
                  pure IAM values reach their peak. The tubes are exposed to all 
                  the sunlight shining towards them, and all the tubes are still 
                  perpendicular to the sun. This is why even at this point the 
                  cosine adjusted IAM is still 1. 
                  As the angle increases, the tubes start to 
                  overlap, shading each other. They are still facing the sun, 
                  but the actual surface area of absorber exposed to the 
                  sunlight is reduced. Only a small amount of sunlight falls 
                  beyond 40o (early morning and late afternoon), and so this 
                  decrease surface area has minimal influence on the total daily 
                  energy output of the collector.  
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