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RPWI_INITRPWI Transient mode while instrument is initialising after being powered onRPWI
RPWI_STANDBYRPWI Safe mode where the instrument can survive indefinitely and where memory patch, dump and check commands are acceptedRPWI
RPWI_In_situ_burst_Radar_mode_3The RPWI In-situ_burst + Radio_mode_3 mode: - Makes continuous In-situ_burst mode measurement. In addtion to in-situ_slow modes, In-situ_burst mode adds continuous measurements of electric and magnetic fields at higher cadence (763 smpl/s) as well as more frequent snapshots at higher frequencies (MF - 50 ksmpl/s and HF - 312 ksmpl/s); - Radio mode TBDRPWI
RPWI_In_situ_burst_Radio_FullThe RPWI In-situ_burst + Radio_Full mode: - Makes continuous In-situ_burst mode measurement. In addtion to in-situ_slow modes, In-situ_burst mode adds continuous measurements of electric and magnetic fields at higher cadence (763 smpl/s) as well as more frequent snapshots at higher frequencies (MF - 50 ksmpl/s and HF - 312 ksmpl/s); - Makes detailed radio emissions from Jupiter as well as moons (Ganymede, Callisto, Europa). Will also support RIME measurements, giving the background natural radio emissions. Monitor the radio emission spectrum as well as polarization.RPWI
RPWI_In_situ_burst_Radio_burstThe RPWI In-situ_burst + Radio_burst mode: - Makes continuous In-situ_burst mode measurement. In addtion to in-situ_slow modes, In-situ_burst mode adds continuous measurements of electric and magnetic fields at higher cadence (763 smpl/s) as well as more frequent snapshots at higher frequencies (MF - 50 ksmpl/s and HF - 312 ksmpl/s) - Makes full plasma wave measurements and high-time resolution monitoring up to 1.6MHz as well as cover the low frequency and DC electric field and density measurements.RPWI
RPWI_In_situ_slow_Radar_mode_3The RPWI In-situ_slow + Radio_mode_3 mode: - Makes continuous In-situ_slow mode measurement, the basic in-situ modes; - Radio mode TBDRPWI
RPWI_In_situ_slow_Radio_burstThe RPWI In-situ_slow + Radio_burst mode: - Makes continuous In-situ_slow mode measurement, the basic in-situ modes; - Makes full plasma wave measurements and high-time resolution monitoring up to 1.6MHz as well as cover the low frequency and DC electric field and density measurements.RPWI
RPWI_In_situ_slow_Radio_FullThe RPWI In-situ_slow + Radio_Full mode: - Makes continuous In-situ_slow mode measurement, the basic in-situ modes; - Makes detailed radio emissions from Jupiter as well as moons (Ganymede, Callisto, Europa). Will also support RIME measurements, giving the background natural radio emissions. Monitor the radio emission spectrum as well as polarization.RPWI
RPWI_In_situ_normal_Radar_mode_3The RPWI In-situ_normal + Radio_mode_3 mode: - Makes continuous In-situ_normal mode measurement. In addtion to in-situ_slows modes, In-situ_normal mode adds short durations snapshots if electric and magnetic fields at higher frequencies (LF – 763 smpl/s, MF - 50 ksmpl/s and HF - 312 ksmpl/s - Radio mode TBDRPWI
RPWI_In_situ_normal_Radio_FullThe RPWI In-situ_normal + Radio_Full mode: - Makes continuous In-situ_normal mode measurement. In addtion to in-situ modes, In-situ_normal mode adds short durations snapshots if electric and magnetic fields at higher frequencies (LF – 763 smpl/s, MF - 50 ksmpl/s and HF - 312 ksmpl/s - Makes detailed radio emissions from Jupiter as well as moons (Ganymede, Callisto, Europa). Will also support RIME measurements, giving the background natural radio emissions. Monitor the radio emission spectrum as well as polarization.RPWI
RPWI_In_situ_normal_Radio_burstThe RPWI In-situ_normal + Radio_burst mode: - Makes continuous In-situ_normal mode measurement. In addtion to in-situ modes, In-situ_normal mode adds short durations snapshots if electric and magnetic fields at higher frequencies (LF – 763 smpl/s, MF - 50 ksmpl/s and HF - 312 ksmpl/s - Makes full plasma wave measurements and high-time resolution monitoring up to 1.6MHz as well as cover the low frequency and DC electric field and density measurements.RPWI
OBSOLETE_RPWI_In_situ_low_Radio_burstThe RPWI In-situ_low + Radio_burst mode: - Makes continuous In-situ_low mode measurement, the lowest in-situ possible power and TM, which implements only the Mutual Impedance sweeps and DC electric field measurements; - Makes full plasma wave measurements and high-time resolution monitoring up to 1.6MHz as well as cover the low frequency and DC electric field and density measurements.RPWI
OBSOLETE_RPWI_In_situ_low_Radar_mode_3The RPWI In-situ_low + Radio_mode_3 mode: - Makes continuous In-situ_low mode measurement, the lowest in-situ possible power and TM, which implements only the Mutual Impedance sweeps and DC electric field measurements; - Radio TBDRPWI
RPWI_In_situ_low_Radio_FullThe RPWI In-situ_low + Radio_Full mode - Makes continuous In-situ_low mode, the lowest in-situ possible power and TM, which implements only the Mutual Impedance sweeps and DC electric field measurements; - Makes detailed radio emissions from Jupiter as well as moons (Ganymede, Callisto, Europa). Will also support RIME measurements, giving the background natural radio emissions. Monitor the radio emission spectrum as well as polarization.RPWI
RPWI_DLRPWI observation during downlink windowsRPWI
OBSOLETE_RPWI_EUR_BURSTObservation with set up for closest approachRPWI
OBSOLETE_RPWI_EUR_FULLThe full mode for RPWI observationRPWI
OBSOLETE_RPWI_EUR_NORMNormal RPWI modeRPWI
OBSOLETE_RPWI_EUR_LOWObservation combining the modes required when 'far' from the CA, typically before and after 8.5 h from CARPWI
OBSOLETE_RPWI_MAGN_In-situ_BurstN/ARPWI
OBSOLETE_RPWI_MAGN_In-situ_NormalN/ARPWI
OBSOLETE_RPWI_GAN_Radio_BurstUsed for radio occultation of Jovian radio emissions to infer the ionospheric spatial structure. RPWI
OBSOLETE_RPWI_GAN_In-situ_LowTMN/ARPWI
OBSOLETE_RPWI_GAN_In-situ_NormalMakes continuous detailed RPWI observations that satisfy most SciRD requirements below 1.6 MHz. Main science targets here are the ionospheric/magnetospheric electric currents and electrodynamics, including sub-surface ocean characteristics. RPWI
OBSOLETE_RPWI_GAN_Radio_PassiveRadarThere are several ways of doing passive radar under investigation. We have chosen the most resource hungry mode for this table. One of the RWI antenna nulls (X, Y or Z) should point towards Jupiter with +/-1 deg accuracy. Monitoring HOM and DAM Jupiter radiation with reflections from ionosphere, surface and sub-surface layers (ocean/bedrock) to determine ionosphere and ice sheet thickness. Due to lower frequency (below 3 MHz), RPWI will reach deeper than RIME.RPWI
OBSOLETE_RPWI_GAN_Radio_FullMake more detailed radio emissions from Jupiter as well as Ganymede. Will also support RIME measurements, giving the background natural radio emissions. Monitor the radio emission spectrum as well as polarization.RPWI
OBSOLETE_RPWI_GAN_Radio_SlowMake survey of radio emissions from Jupiter as well as Ganymede. Will also support RIME observations, giving the background natural radio emissions. Monitor the radio emission spectrum.RPWI
OBSOLETE_RPWI_GAN_In-situ_BurstMakes full plasma wave measurements and high-time resolution monitoring up to 1.6MHz as well as cover the low frequency and DC electric field and density measurements.RPWI

28 observation definitions