PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2012-06-29 NOTE = " TRIG_B4.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 Reciever (WBR), the Langmiur Probe (LP), the Sounder, and the Dust detector algorithm when using Trigger B4." END_OBJECT = TEXT END Trigger B4 Description Sequence: S05, ... Trigger B4 ( Titan deltaN/N mode) This mode assumes a background survey mode, such as 8A or A0, is running. The duty cycle of the Langmuir Probe and the WFR are increased. The WFR is connected in 3-channel mode to the two voltage-biased cycliners, EU and EV, and their voltage is set to +5V. The third WFR channel is connected to the LP sphere, which is biased at +4V. Every 10 seconds a 1024-sample (per channel) data set is acquired by the WFR in 2.5KHz mode. The Langmuir Probe performs a sweep every 20 seconds and between sweeps, does a 256-sample density mode measurement at 20 Hz. The MFR is connected to the EW antenna, since the EX antenna is being used in deltaN/N mode. Also the LFDR and MFDR use the EW antenna for their electric field measurements (in addition to the BX antenna). They each acquire data once a minute. 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. Measured bitrate was about 55 kbps when in S&ER-3 mode, measured during C39. In C40, at a higher rate telemetry mode, the measured bitrate was 99 kbps. Receiver Frequency Range Sensors Snapshot Spacing -------- ---------------- ----------------------- ---------------- LFR 1 - 25Hz EW, BX 60 seconds MFDR 70Hz - 1.7KHz EW, BX 60 seconds MFR 25 - 12 KHz EW, BZ 32 seconds WFR .1 - 2.5 KHz EU(+5V),EV(+5V),LP(+4V) 24 seconds HFR 3.6 KHz - 16 MHz EX, EW 10 seconds LP N/A Langmuir Probe 20 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 500 1 3.6-319KHz HF1 2E y y 2 n 20 1 60 25 0.325-1.825MHz HF2 1E n n 1 n 10 1 72 200 1.825-16.225MHz Bands ABC require 1.580 sec to complete, H1 requires 1.573 sec, and H2 requires 0.886 sec for a total of 4.039 sec per sweep. The hfr cycle time is 10.000 seconds. 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.