PDS_VERSION_ID                = PDS3                                          
DATA_SET_ID                   = "CO-S-MIMI-4-INCA-CALIB-V1.0"                 
PRODUCT_ID                    = "IENAIMG0_HO_2004314_000_00"                  
STANDARD_DATA_PRODUCT_ID      = "MIMI_INCA_ENAIMG_HO"                         
PRODUCT_TYPE                  = "BROWSE"                                      
PRODUCT_VERSION_ID            = "00"                                          
PRODUCT_CREATION_TIME         = 2013-030T23:28:54                             
                                                                              
RECORD_TYPE                   = UNDEFINED                                     
INTERCHANGE_FORMAT            = BINARY                                        
                                                                              
START_TIME                    = 2004-314T00:01:23                             
STOP_TIME                     = 2004-314T07:01:24                             
NATIVE_START_TIME             = "153230547.182"                               
NATIVE_STOP_TIME              = "153255748.182"                               
SPACECRAFT_CLOCK_START_COUNT  = "1/1478651211.000"                            
SPACECRAFT_CLOCK_STOP_COUNT   = "1/1478676413.000"                            
                                                                              
INSTRUMENT_HOST_NAME          = "CASSINI ORBITER"                             
INSTRUMENT_HOST_ID            = "CO"                                          
MISSION_PHASE_NAME            = "TOUR PRE-HUYGENS"                            
ORBIT_NAME                    = "a"                                           
TARGET_NAME                   = "SATURN"                                      
INSTRUMENT_NAME               = "MAGNETOSPHERIC IMAGING INSTRUMENT"           
INSTRUMENT_ID                 = "MIMI"                                        
                                                                              
^DOCUMENT               = "IENAIMG0_HO_2004314_000_00.PNG"                    
OBJECT                  = DOCUMENT                                            
  DOCUMENT_NAME       = "IENAIMG0_HO_2004314_000_00"                          
  DOCUMENT_FORMAT     = PNG                                                   
  DOCUMENT_TOPIC_TYPE = "BROWSE IMAGE"                                        
  INTERCHANGE_FORMAT  = BINARY                                                
  PUBLICATION_DATE    = 2013-030                                              
  SOURCE_PRODUCT_ID   = "IIMG0_2004314_0003"                                  
                                                                              
  DESCRIPTION         = "PNG file containing three rows by N                  
   columns of panels, where the bottom three rows are a continuation          
   in time of the top three rows. Each row contains spin averaged             
   high spatial energetic neutral atom (ENA) image skymaps (each one          
   accumulated over four sectors), displayed for one species and              
   time-of-flight (TOF) combinations from the INCA sensor of the              
   MIMI instrument on the Cassini spacecraft.                                 
                                                                              
   Row one contains the high TOF Hydrogen images, row two contains            
   the low TOF Hydrogen images and row three contains the low TOF             
   Oxygen images. The high TOF oxygen in the spatial products usually         
   has too little intensity to produce a good image, so we left it            
   out of the browse products to allow more image space on the page           
   for browse images that are more useful. The energy range for each          
   TOF range is shown to the right of each row. ENA images are                
   collected when a high voltage is present on the INCA collimator.           
   The value displayed is the log of the image intensity which is             
   counts/(centimeters squared*steradian*seconds*keV). The color              
   bars for each row are independent and are determined by the                
   minimum and maximum pixels in that row (i.e., for the entire day).         
                                                                              
   The energy ranges for the high spatial resolution hydrogen images          
   (TOF id is the value in the TOF column in the angle average files)         
   High TOF id 0 55-90 keV                                                    
   Low TOF id 7 24-55 keV                                                     
                                                                              
   The energy range for the high spatial resolution oxygen is                 
   Low TOF id 7 90-170 keV                                                    
                                                                              
   Each original image was 64 x 64 pixels and was transformed into            
   the following frame. The skymap frame is a dynamically defined             
   frame, defined as follows. The primary axis X is the INCA                  
   boresight axis. The secondary Z axis is the Z axis of the                  
   IAU_SATURN frame. The Y-axis completes the right-handed system.            
   The skymap display is defined to display every frame with the Z            
   axis up,  X axis into the page and Y axis out to the left. So in           
   the skymap, using this frame, Z or up is the spin axis of                  
   Saturn, into the page is the boresight.                                    
                                                                              
   Scaling has been applied to the image to normalize the apparent            
   size of Saturn, if;                                                        
   1. Saturn is in the field-of-view                                          
   2. The distance to Saturn is less than 100 radius to Saturn                
   3. The spacecraft is not spinning.                                         
   In periods where the spacecraft is going in and out of Z axis              
   spin mode, the images will appear un-zoomed and zoomed (non spin           
   mode).                                                                     
                                                                              
   If they are visible in the image, the orbit of Titan (dotted               
   line),  Titan center (dot), and the axis for Saturn equatorial             
   system frame (centered at Saturn) are displayed. The definition            
   of the Saturn equatorial system frame is the primary axis,                 
   labeled Z, is parallel to the Saturn spin axis.  The Y-axis is             
   then defined as the cross product of  this vector with the                 
   Saturn-Sun vector.  The X-axis completes the right-handed system           
   and is directed towards the Sun.                                           
                                                                              
   At the top of the page, the Rs=radius to Saturn, Lat=latitude in           
   IAU_SATURN frame, LT=Saturn Local Time, L=L value, local time of           
   Cassini relative to Saturn, Lon skr-wl= Longitude of Cassini in            
   the Saturn Kilometric Radiation (western longitude) frame. These           
   measurments are calculated at the start time of the first                  
   image."                                                                    
END_OBJECT            = DOCUMENT                                              
END