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About the preparation and analysis of the RPW/SCM noise measurements, to be performed during spacecraft Earth magnetic lobes crossing.

General

Purpose & Objectives

During the CP (TBC), Solar Orbiter will pass inside the Earth magnetic lobes, where the B field amplitude is very low. It is the occasion for RPW to measure the SCM sensitivity.

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Working Group

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Members

  • Xavier Bonnin – ROC manager (LESIA)
  • Milan Maksimovic – RPW PI (LESIA)
  • Olga Alexandrova – RPW/SCM operations scientist (LESIA) – WG leader
  • Diane Berard – RPW operations engineer (LESIA)
  • Matthieu kretzschmar – SCM config, data analysis (LPC2E)

Operation preparation

Context

The measurement will have to be done when the S/C is close to the Earth. In the current Feb. 2020 launch scenario this will only occurs during the first week of commissioning and during the Earth GAM at the end of the CP.

During these two phases, the operations will be driven by the MOC. Especially, the MOC will have to perform critical S/C manoeuvres during the GAM, which may interfere with the RPW operation requests for SCM measurement.

Overall timeline

Give here the overall timeline of the operation, including the expected instrument operating configurations.

Orbitography

Give here the orbitography (i.e., time versus S/C orbit/attitude)

Operation Constraints

Give here the operation constraints at RPW and SOLO levels (e.g., TM rate, PW, SOOP, etc.)

Command/Control

Give here the list of TCs required to execute this operation. (Link to procedures, IOR/PDOR can also be provided).

Data analysis

Expected data products

Give here the list of expected data products

Results

Give here the results of the data analysis (can be attached file, or link to references)

Meeting Notes

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Points of contact

  • Sylvain Lodiot – SOLO Operations manager – (MOC)
  • Eric Lorfevre – RPW system engineer (CNES)

Deliverables

Related resources

Meeting Notes

Action Items

Jira
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Attached Files

  • SCM_noise_31mai2018.pdf (slides presented by O.Alexandrova during RPW consortium meeting #21 at Dresden on June 2018)
  • TDS configuration : 
    View file
    nameRPW-5_TDS_inputs_SCM_Noise_V02.docx
    height250
  • LFR configuration : 
    View file
    nameRPW-5_LFR_inputs_V02.docx
    height250

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