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 = "C11_TRIG_56" 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_56.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 56." END_OBJECT = TEXT END Trigger 56 Description Sequence: All Trigger 56 (STV LFR Noise Check) This trigger is based on a mode used in a series of tests that were performed before launch, and is designed to test the noise detected by the LFR receiver. Receiver Frequency Range Sensor Cycle Time Snapshot Size -------- --------------- ---------------- ---------------- ------------- LFR 1Hz-25Hz EX,EW,BX,BZ 16.000 Seconds MFR 25Hz-12KHz EX,EW,BX,BZ 32.000 Seconds WFR 1Hz-40Hz EX 32.000 Seconds 512 WFR 1Hz-40Hz EW 16.000 Seconds 512 WFR 1Hz-40Hz BX 16.000 Seconds 512 WFR 1Hz-40Hz BZ 16.000 Seconds 512 The trigger steps the LFR through the following antenna choices (the MFR is also switched to the same antenna. The data is dual routed through the LFR and the WFR. 128 seconds EX 128 seconds EW 128 seconds BX 128 seconds BZ