PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2005-06-01 NOTE = " C40_TRIG_BE.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 BE." END_OBJECT = TEXT END Trigger BE Description Sequence: C40, ... Trigger BE ( Titan millisecond mode) This mode assumes a that either Nighttime survey 8E or SEDDF mode A0, is running. The HFR runs in millisecond mode for approximately 56 seconds of every 64-second interval, and then performs one normal analysis using fast time constants. The millisecond mode frequency is changed every 64 seconds, stepping from 775 KHz to 1525 KHz, and finally to 3025 KHz. The WFR is run in the usual 5-channel mode, except that its 3rd channel, normally connected to BX, is now connected to the Langmuir Probe sphere, which is set to a fixed bias of +4V. The LP performs a sweep every 640 seconds, and between sweeps does a fixed bias (+4V) density mode measurement every 16 seconds. The WBR acquires data in 80-KHz mode. Sounder is disabled, and dust detection is disabled in this mode. The target bit rate is 100 kbps. In C40 the measured bitrate was 99 kbps. There was an error in the C40 test --- because the preceding mode was normal survey (8A) instead of the recommended 8E or A0, the HFR performed its normal analysis every 72 seconds instead of the planned 64 seconds. Receiver Frequency Range Sensors Cycle Time -------- -------------------------------- ------------------- ------------ MFR 25 - 12 KHz EX, BZ 32 seconds WFR 1 - 25 Hz EX,EW,LP(+4V),BY,BZ 320 seconds WFR .1 - 2.5 KHz EX,EW,LP(+4V),BY,BZ 320 seconds HFR 3.6 KHz - 16 MHz EX, EW 64 seconds HFR msec mode at 775, 1525, 3025 KHz EX 2.5 seconds LP N/A Probe 640 seconds WBR 0 - 80 KHz EX 0.125 second The HFR is in a modified "Composite Survey" mode, which includes both auto- and cross-correlations for H1, and should be set up to use the faster integration constants of the "Night-time" survey mode, running either trigger 8E or A0 or A8 prior to this trigger. 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 1000 1 3.6-319 kHz H1 2E y y 2 n 20 1 60 25 325k-1.8MHz H2 1E n n 1 n 10 1 72 200 1.8M-16MHz Bands ABC require 3.16 sec to complete, H1 requires 1.57 sec, and H2 requires 0.65 sec for a total of 5.62 sec per sweep. However, the time between analyses is set to 10 seconds to avoid interference from the LP sweep. No Sounder measurements are made in this mode. No onboard dust detection is done either.