| S_V_FIBFOBFSC | Validation Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | - |
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| test | | - |
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| User Defined | | - |
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| CALLISTO_FLYBY_GALA | | - |
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| KAT_TRACKING | KAT module in tracking/ranging mode | 3GM |
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| USO_OPERATIONAL | Definition of 3GM units individual modes (unmuted)
power values source: JUI-3GM-INST-UM-001, v1.2 | 3GM |
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| USO_STANDBY | USO module in STANDBY (muted) mode | 3GM |
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| HAA_OBSERVATION | HAA module in observation (science) mode | 3GM |
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| HAA_CALIBRATION | HAA module in calibration mode | 3GM |
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| HAA_STBY | | 3GM |
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| DIAG_RX | GALA DIAG_RX mode. duration: 10sec | GALA |
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| SAFE | GALA SAFE mode. Duration: 10sec | GALA |
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| IDLE | GALA IDLE mode. Duration: 15sec | GALA |
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| PBS | | GALA |
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| SCIENCE | SCIENCE mode. Duration: 10sec | GALA |
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| Diagnostic | duration: 10sec | GALA |
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| Config | | GALA |
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| STBY | STANDBY mode. Duration: 20 sec | GALA |
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| CONFIG_ALLOFF | | JANUS |
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| CONFIG_ALLON | | JANUS |
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| Cover_act 2ms | | JANUS |
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| Safe | | JANUS |
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| Diagnostic | | JANUS |
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| Science | | JANUS |
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| Idle | | JANUS |
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| FW_activation | | JANUS |
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| STBY | | JANUS |
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| Cover_20ms-30s | | JANUS |
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| SERVICE3 | NECP value | MAJIS |
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| SCIENCE_MIN_1PE | NECP value | MAJIS |
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| SCIENCE_MAX | NECP value | MAJIS |
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| SCIENCE_AVERAGE | NECP value | MAJIS |
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| CALIBRATION_PEAK | NECP value | MAJIS |
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| CALIBRATION_AVERAGE | NECP value | MAJIS |
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| SERVICE2 | NECP values | MAJIS |
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| SERVICE1 | NECP values | MAJIS |
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| SAFE | NECP values | MAJIS |
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| OFF_DECONTAMINATION | analysis of SC data to derive power consumption during decontamination (NECP) has been performed by the team. Data coming from the post launch phase for heating lines | MAJIS |
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| OFF_SURVIVAL | for 2 channels (2.1 W for one single channel).
Numbers derived by the instrument team based on data coming from the post launch phase for heating lines. | MAJIS |
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| SCIENCE_LP | | PEPLO |
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| SCIENCE | | PEPLO |
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| STBY | | PEPLO |
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| S_LOG_FOBFSC | Light-only Gradiometer Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_LOG_FIBFOBFSC | Light-only Gradiometer Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_LOG_FIBFSC | Light-only Gradiometer Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_LON_FOBFSC | Light-only Normal Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_LON_FIBFOBFSC | Light-only Normal Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_LON_FIBFSC | Light-only Normal Mode. FSC Powered but producing no Science data.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| C_LO_FSC | Light-only FSC, No Fluxgates operating. Instrument in Config Mode with no Science data transmision to SSMM.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_L_FIBFOBFSC | Low-rate Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter.
Power is 13.3 (+4): The amount of the (+4W) needed is wholly dependent on the vault temperature. When the vault temp is at the minimum allowed then the MAGSCA Peltier needs this additional 4W to get the laser up to temperature. | JMAG |
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| S_L_FIBFOB | Low-rate Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_L_FOB | Low-rate Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_L_FIB | Low-rate Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_V_FIBFOBFSC | Validation Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter.
Power is 13.3 (+4): The amount of the (+4W) needed is wholly dependent on the vault temperature. When the vault temp is at the minimum allowed then the MAGSCA Peltier needs this additional 4W to get the laser up to temperature. | JMAG |
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| S_V_FIBFOB | Validation Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_V_FOB | Validation Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_V_FIB | Validation Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_G_FIBFOBFSC | Gradiometer Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter.
Power is 13.3 (+4): The amount of the (+4W) needed is wholly dependent on the vault temperature. When the vault temp is at the minimum allowed then the MAGSCA Peltier needs this additional 4W to get the laser up to temperature. | JMAG |
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| S_G_FIBFOB | Gradiometer Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_G_FOB | Gradiometer Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_G_FIB | Gradiometer Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_B_FIBFOBFSC | Burst Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter.
Power is 13.3 (+4): The amount of the (+4W) needed is wholly dependent on the vault temperature. When the vault temp is at the minimum allowed then the MAGSCA Peltier needs this additional 4W to get the laser up to temperature. | JMAG |
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| S_B_FIBFOB | Burst Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_B_FOB | Burst Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_B_FIB | Burst Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_N_FIBFOB | Normal Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_N_FOB | Normal Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_N_FIB | Normal Mode.
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter. | JMAG |
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| S_N_FIBFOBFSC | Normal Mode
The mode naming convention states whether the instrument is in SCIENCE or CONFIG with the first letter, the Macro Mode with the second letter.
Power is 13.3 (+4): The amount of the (+4W) needed is wholly dependent on the vault temperature. When the vault temp is at the minimum allowed then the MAGSCA Peltier needs this additional 4W to get the laser up to temperature. | JMAG |
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| SAFE | Automatically entered whenever a not nominal condition is encountered in any other Mode excluding Init-Standby Mode. | RIME |
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| OFF | RIME not powered | RIME |
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| SCIENCE_2 | Passive Radar Acquisition mode with 10% DC mode.
Telemetries from the NECP operation in SCIENCE_2 mode and found that the total power of RIME is 11.6W (divided in RDS: 8.87W and Tx: 2.74W). Some minor variations are visible during the instrument operation, up to 20mW. Probably in the future we may be able to model them but I think that their effect is negligible. | RIME |
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| SCIENCE_05 | Flyby Aquisition mode with 5% DC mode.
RIME observations during flyby with variable instrument parameters, high vertical resolution and deep penetration.
Since during flybys the instrument parameters (i.e. pulse repetition frequency) varies to adapt to the altitude and speed changes, both datarate and power consumption are not constant for the entire acquisition duration. Datarate max and min bound profiles could be computed analysing the instantaneous altitude and velocity w.r.t. the moon surface. Shielding from Jupiter noise is advisable but due to the sporadic nature of Jupiter noise RIME should be operated in the unshielded areas too. To be noted that during Europa Flybys the Jupiter noise shadow cone boundary is often very close to the trajectory around closest approach, thus very small variations of altitude and latitude of the CA can result in huge variations of the full Jupiter noise shadow duration.
The datarate strongly depends on the altitude uncertainty a priori knowledge. | RIME |
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| INIT | | RIME |
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| SCIENCE_10 | Flyby Acquisition mode with 10% DC mode.
RIME observations during flyby with variable instrument parameters, high vertical resolution and deep penetration.
Since during flybys the instrument parameters (i.e. pulse repetition frequency) varies to adapt to the altitude and speed changes, both datarate and power consumption are not constant for the entire acquisition duration. Datarate max and min bound profiles could be computed analysing the instantaneous altitude and velocity w.r.t. the moon surface. Shielding from Jupiter noise is advisable but due to the sporadic nature of Jupiter noise RIME should be operated in the unshielded areas too. To be noted that during Europa Flybys the Jupiter noise shadow cone boundary is often very close to the trajectory around closest approach, thus very small variations of altitude and latitude of the CA can result in huge variations of the full Jupiter noise shadow duration.
The data rate strongly depends on the altitude uncertainty a priori knowledge. | RIME |
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| SCIENCE_02 | | RIME |
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| INSIT_BURST_RADMOD3 | | RPWI |
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| INSIT_BURST_RAD_BURST | | RPWI |
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| INSIT_BURST_RAD_FULL | | RPWI |
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| INSIT_BURST_RAD_LOW | | RPWI |
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| INSIT_NOR_RADMOD3 | | RPWI |
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| INSIT_NOR_RAD_BURST | | RPWI |
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| INSIT_NOR_RAD_FULL | | RPWI |
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| INSIT_NOR_RAD_LOW | | RPWI |
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| INSIT_SLOW_RADMOD3 | | RPWI |
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| INSIT_SLOW_RAD_BURST | | RPWI |
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| INSIT_SLOW_RAD_FULL | | RPWI |
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| INSIT_SLOW_RAD_LOW | | RPWI |
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| INSIT_LOW_RADMOD3 | | RPWI |
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| INSIT_LOW_RAD_BURST | | RPWI |
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| INSIT_LOW_RAD_FULL | | RPWI |
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| INSIT_LOW_RAD_LOW | | RPWI |
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| CAL_DIAG | | RPWI |
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| SAFE_SERV | | RPWI |
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| STBY | | RPWI |
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| INIT | | RPWI |
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| OFF | From JUI-STATE Models_ORCD | UVS |
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| DECON | | UVS |
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| SCIENCE | | UVS |
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| CHECKOUT | | UVS |
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