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 = "C25_TRIG_80" 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 = 2005-04-01 NOTE = " TRIG_80.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 80." END_OBJECT = TEXT END Trigger 80 Description Sequence: C23, C24, C25 Trigger 80 (Direction-Finding Survey) This mode is designed to provide a Survey with fast temporal resolution and standard spectral resolution for periods during Jupiter Flyby. Periodic Waveform measurements are made. The entire RPWS frequency range (1 Hz - 16 MHz) is covered. Receiver Frequency Range Sensors Time between Snapshots -------- ---------------- ------------------ ---------------------- LFR 1 - 25 Hz EX, BX 32 seconds MFR 25 - 12 KHz EW, BZ 32 seconds WFR 1 - 25 Hz EX, EW, BX, BY, BZ 160 seconds HFR 3.6 KHz - 16 MHz EU, EV, EW 32 seconds The HFR is in direction-finding mode for its entire frequency range from 3.6 KHz to 16 MHz. Thus, measurements are made on all three monopoles EU, EV and 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 8 y 250 1 3.6-319 kHz H1 2E y y 1 y 80 1 76 50 325k-4.1MHz H2 2E y y 1 y 80 1 61 200 4.0M-16MHz Bands ABC require 1.69 sec to complete, H1 requires 13.06 sec, and H2 requires 10.50 sec for a total of 25.25 sec per sweep. However, to allow time for LFR and MFR snapshots to occur without interference, one complete sweep is done every 32 seconds. To avoid the interference from the DF mode, the MFR uses the EW antenna.