About the preparation and analysis of the RPW/SCM noise measurements, to be performed during spacecraft Earth magnetic lobes crossing.
Introduction
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 – Operation constraint, control/commandROC manager (LESIA)
- Milan Maksimovic – RPW PI (LESIA)
- Olga Alexandrova – Orbitography, RPW/SCM config, data analysisoperations scientist (LESIA) – WG leader
- Diane Berard – RPW operations engineer (LESIA)
- Matthieu kretzschmar – RPW SCM config, data analysis
Operation preparation
Overall timeline
Give here the overall timeline of the operation.
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, etc.)
Command/Control
Give here the list of flight procedures and IOR (PDOR?) required to execute this operation
Data analysis
Expected data products
Give here the list of expected data products
Results
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- (LPC2E)
- Antonio Vecchio – RPW operations support scientist (LESIA)
Points of contact
- Sylvain Lodiot – SOLO Operations manager – (MOC)
- Eric Lorfevre – RPW system engineer (CNES)
Deliverables
Related resources
Meeting Notes
Action Items
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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 name RPW-5_TDS_inputs_SCM_Noise_V02.docx height 250 - LFR configuration :
View file name RPW-5_LFR_inputs_V02.docx height 250