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.
The SCM Noise Measurement Workin Group (SNMWG) is in charge to prepare the operation (timeline, RPW config and associated flight procedures, expected data volume and power, etc.) and participate to the data analysis.
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Working Group 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