Table 1.

Summary of the most important electro-magnetic perturbations impacting RPW and characterized so far.

Label Description Corrupted Sensor Root Impacted Severity and
frequencies E/B cause sub-systems mitigations
1 Continuous emission ∼1.3 Hz B Unknown SCM, LFR TBD

2 Pulse of the Attitude and Orbit Control System (AOCS) synchronization 8 and 16 Hz B S/C AOCS LFR Low severity

3 SCM heater ≤100 Hz B SCM LFR Low severity, flagging the data

4 36 Hz and harmonics ≤200 Hz E Unknown LFR Medium severity

5 3 h periodicity perturbation in LF ≤500 Hz B Unknown LFR TBD

6 EUI science mode Broadband up to 1.5 kHz E and B EUI LFR Medium severity, should be taken care of during operations

7 Solo-HI 6.3 kHz ∼6.3 kHz E and B Solo-HI LFR Medium severity, should be taken care of during operations

8 ∼50 kHz From ∼30 to ∼60 kHz E Unknown TNR-HFR and TDS High severity

9 80 kHz ∼80 kHz and harmonics E S/C reaction wheels electronics TNR-HFR High severity, mitigation by RPW team

10 120 kHz ∼120 kHz and harmonics E and B S/C PCDU noise radiated by SA TNR-HFR and TDS High severity, mitigation by RPW team

11 ∼250 kHz 244.6, 255.5 kHz B MAG heater TNR Low severity, mitigation by flagging the data

12 ∼300 kHz Several frequencies around 300 kHz E S/C battery charging TNR High severity if not mitigated by ESA during operations

Notes. Their root causes are still under investigation. All the information and updates about the RPW EM contamination can be found online (https://rpw.lesia.obspm.fr/Engineering).

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