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CONFIG_ALLOFF JANUS
CONFIG_ALLON JANUS
DIAG_RXGALA DIAG_RX mode. duration: 10secGALA
SAFEGALA SAFE mode. Duration: 10secGALA
IDLEGALA IDLE mode. Duration: 15secGALA
KAT_TRACKINGKAT module in tracking/ranging mode3GM
USO_OPERATIONALDefinition of 3GM units individual modes (unmuted) power values source: JUI-3GM-INST-UM-001, v1.23GM
USO_STANDBYUSO module in STANDBY (muted) mode3GM
HAA_OBSERVATIONHAA module in observation (science) mode3GM
HAA_CALIBRATIONHAA module in calibration mode3GM
HAA_STBY 3GM
S_LOG_FOBFSCLight-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
S_LOG_FIBFOBFSCLight-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
S_LOG_FIBFSCLight-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
S_LON_FOBFSCLight-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
S_LON_FIBFOBFSCLight-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
S_LON_FIBFSCLight-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
C_LO_FSCLight-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
S_L_FIBFOBFSCLow-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
S_L_FIBFOBLow-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
S_L_FOBLow-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
S_L_FIBLow-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
S_V_FIBFOBFSCValidation 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
S_V_FIBFOBFSCValidation 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.-
S_V_FIBFOBValidation 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
S_V_FOBValidation 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
S_V_FIBValidation 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
S_G_FIBFOBFSCGradiometer 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
S_G_FIBFOBGradiometer 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
S_G_FOBGradiometer 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
S_G_FIBGradiometer 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
S_B_FIBFOBFSCBurst 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
S_B_FIBFOBBurst 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
S_B_FOBBurst 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
S_B_FIBBurst 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
S_N_FIBFOBNormal 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
S_N_FOBNormal 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
S_N_FIBNormal 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
SAFEAutomatically entered whenever a not nominal condition is encountered in any other Mode excluding Init-Standby Mode.RIME
OFFRIME not poweredRIME
SCIENCE_2Passive 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
SCIENCE_05Flyby 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
SERVICE3NECP valueMAJIS
test -
Cover_act 2ms JANUS
PBS GALA
SCIENCE_MIN_1PENECP valueMAJIS
SCIENCE_MAXNECP valueMAJIS
SCIENCE_AVERAGENECP valueMAJIS
CALIBRATION_PEAKNECP valueMAJIS
CALIBRATION_AVERAGENECP valueMAJIS
SERVICE2NECP valuesMAJIS
SERVICE1NECP valuesMAJIS
SAFENECP valuesMAJIS
OFF_DECONTAMINATIONanalysis 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 linesMAJIS
OFF_SURVIVALfor 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
Safe JANUS
Diagnostic JANUS
Science JANUS
Idle JANUS
User Defined -
CALLISTO_FLYBY_GALA -
S_N_FIBFOBFSCNormal 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
INSIT_BURST_RADMOD3 RPWI
INSIT_BURST_RAD_BURST RPWI
INSIT_BURST_RAD_FULL RPWI
INSIT_BURST_RAD_LOW RPWI
INSIT_NOR_RADMOD3 RPWI
INSIT_NOR_RAD_BURST RPWI
INSIT_NOR_RAD_FULL RPWI
INSIT_NOR_RAD_LOW RPWI
INSIT_SLOW_RADMOD3 RPWI
INSIT_SLOW_RAD_BURST RPWI
INSIT_SLOW_RAD_FULL RPWI
INSIT_SLOW_RAD_LOW RPWI
INSIT_LOW_RADMOD3 RPWI
INSIT_LOW_RAD_BURST RPWI
INSIT_LOW_RAD_FULL RPWI
INSIT_LOW_RAD_LOW RPWI
CAL_DIAG RPWI
SAFE_SERV RPWI
STBY RPWI
INIT RPWI
INIT RIME
SCIENCE_10Flyby 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
SCIENCE_02 RIME
DECONT UVS
SCIENCE UVS
CHECKOUT UVS
STBY UVS
SCIENCE_LP PEP
SCIENCE PEP
STBY PEP
FW_activation JANUS
STBY JANUS
Cover_20ms-30s JANUS
SCIENCESCIENCE mode. Duration: 10secGALA
Diagnosticduration: 10secGALA
Config GALA
STBYSTANDBY mode. Duration: 20 secGALA

100 modes