PDS_VERSION_ID         = PDS3                                                 
RECORD_TYPE            = STREAM                                               
DATA_SET_ID            = {"CO-V/E/J/S/SS-RPWS-4-SUMM-KEY60S-V1.0",            
                          "CO-V/E/J/S/SS-RPWS-2-REFDR-ALL-V1.0",              
                          "CO-V/E/J/S/SS-RPWS-3-RDR-LRFULL-V1.0",             
                          "CO-V/E/J/S/SS-RPWS-2-REFDR-WBRFULL-V1.0",          
                          "CO-V/E/J/S/SS-RPWS-2-REFDR-WFRFULL-V1.0"}          
PRODUCT_ID             = "C15_TRIG_94"                                        
PRODUCT_VERSION_ID     = "1.00"                                               
PRODUCT_TYPE           = ANCILLARY                                            
INSTRUMENT_HOST_NAME   = "CASSINI ORBITER"                                    
INSTRUMENT_HOST_ID     = CO                                                   
INSTRUMENT_NAME        = "RADIO AND PLASMA WAVE SCIENCE"                      
INSTRUMENT_ID          = RPWS                                                 
OBJECT                 = TEXT                                                 
  PUBLICATION_DATE     = 2005-03-17                                           
  NOTE                 = "                                                    
      TRIG_94.TXT describes the RPWS instrument configuration for             
      the High Frequency Receiver (HFR), the Medium Frequency Receiver (MFR), 
      the Low Frequency Receiver (LFR), the Waveform Receiver (WFR),          
      the Wideband Receiver (WBR), the Langmuir Probe (LP), the Sounder,      
      and the onboard Dust detection algorithm when using Trigger 94."        
END_OBJECT           = TEXT                                                   
END                                                                           
                                                                              
                                                                              
Trigger 94 Description                                                        
                                                                              
Sequence: C15 (ESB)                                                           
                                                                              
Trigger 94 (ESB Langmuir Probe Checkout)                                      
                                                                              
     This mode is designed to test the Langmuir Probe and verify its proper   
operation. For about 10 minutes the LP performs once-per-minute               
down-up full-range sweeps, followed by 20-Hz density measurements for ~50     
seconds.  The rest of the RPWS instrument continues to run in the mode        
defined by Trigger 8C, although the WBR is paused for a second whenever a     
Langmuir Probe sweep is performed. Thus, this mode provides a Survey with     
fast temporal resolution and standard spectral resolution for periods during  
Earth Swing-by.  Fast Waveform measurements are made in the High-Band mode    
(0.1 - 2.5 KHz).  To achieve this elevated data rate, the low-frequency       
measurements on LFR are deleted.  Wideband Receiver measurements are made in  
the 10-KHz mode.  The RPWS frequency range covered is 23 Hz - 16 MHz.         
                                                                              
Receiver       Frequency Range  Sensors            Time between Snapshots     
-------------- ---------------- ------------------ ----------------------     
MFR            25 - 12 KHz      EX, BZ             32 seconds                 
HFR            3.6 KHz - 16 MHz EX, EW             6.625 seconds              
WFR            .01 - 2.5 KHz    EX, EW, BX, BY, BZ 20 seconds                 
WBR            .1 - 10 KHz      EX                 0.375 second               
Langmuir Probe N/A              Probe              60 seconds                 
                                                                              
The HFR is in SKR polarization mode, with no direction-finding.               
Thus, measurements are made on the dipole EX and the monopole EW.             
This mode is defined by:                                                      
                                                                              
          Correlations Channels    Integ.           Size Frequency            
Band Ant. Auto- Cross- per Band df Period Rep Steps kHz  Start - Stop         
---- ---- ----- ------ -------- -- ------ --- ----- ---- ------------         
ABC  2E   y        y      16    n  500    1              3.6-319 kHz          
H1   2E   y        y      2     n  80     1   36    25   325k-1.2MHz          
H2   2E   y        y      1     n  20     1   75    200  1.2M-16MHz           
                                                                              
Bands ABC require 1.58 sec to complete, H1 requires 3.28 sec, and H2 requires 
1.52 sec for a total of 6.38 sec per sweep. In practice, the time between     
spectra is 6.625 sec.