1. Coordinated Observations between MPO and MMO Harri Laakso ESA/ESTEC, Noordwijk

2. Introduction Scientific output of the mission will increase significantly by collecting coordinated observations between MPO instruments between MMO instruments between MPO and MMO instruments We can ignore here instrument suites (and those who share their DPU) as the suites will take care of their coordinated observations Why now? - To find out  key links between instruments for operations planning & commanding cycle  requirements on the mission level (e.g., mass memory, telemetry, power etc) √√√√

3. Aspects on Coordinated Observations  Analysis of the observations by one instrument requires/needs other data from another instrument  Simultaneous data?  Does it need to be collected at the same time (within a second or minute) or  Is it enough to be collected within a few hours (i.e., slowly varying features) or (nearly) any time during the mission (I.e., permanent features)  Which variable? And instantaneous, spin-average, or what?  How frequently?  Is it enough that it is done on a campaign basis; e.g. for calibration purpose, and if so, once a week or what?  Does it have to be done regularly, i.e., the other data are essential input data?  Are the other data needed onboard or on ground?

4. Synergies between MPO and MMO Two-point observations  Simultaneous two-point observations are always valuable and in planetary environments quite rare Supporting data  Analysis of the observations from one spacecraft require/need additional data, e.g., about environment & conditions given by the other spacecraft, such as  MPO needs solar wind and/or magnetospheric data from MMO  MMO needs solar and/or planetary data from MPO

5. MPO Instruments BepiColombo Laser AltimeterBELATopographic mapping Italian Spring AccelerometerISANon—gravitational accelerations of the spacecraft Magnetic Field InvestigationMERMAGDetailed description of planetary magnetic field, its source and interaction with Mercury Radiometer and Thermal Imaging Spectrometer MERTISGlobal mineralogical mapping (7-14 µm), surface temperatures and thermal inertia Mercury Gamma-Ray and Neutron Spectrometer MGNSElemental surface and sub-surface composition, volatile deposits on polar areas, Mercury Imaging X-ray SpectrometerMIXSElemental surface composition, global mapping and composition of surface features Mercury Orbiter Radio Science Experiment MORECore and mantle structure, Mercury orbit, fundamental science, gravity field Probing of Hermean Exosphere by Ultraviolet Spectroscopy PHEBUSUV spectral mapping of the exosphere Search for Exospheric Refilling & Emitted Natural Abundances SERENA: Elena, MIPA, PICAM, Strofio Composition, vertical structure and source and sink processes of the exosphere Solar Intensity X-ray and particle Spectrometer SIXSMonitor solar X-ray intensity and solar particles in support of MIXS Spectrometers and Imagers for MPO BepiColombo Integrated Observatory SIMBIO-SYS: HIRC, STC, VIHI Optical high resolution and stereo imaging, Near-IR (<2.0µm) imaging spectroscopy for global mineralogical mapping

6. MPO Instruments, 1 No coordinated observations necessary between MPO and MMO BepiColombo Laser AltimeterBELATopographic mapping Italian Spring AccelerometerISANon—gravitational accelerations of the spacecraft Mercury Orbiter Radio Science ExperimentMORECore and mantle structure, Mercury orbit, fundamental science, gravity field Spectrometers and Imagers for MPO BepiColombo Integrated Observatory SIMBIO-SYS: HIRC, STC, VIHI Optical high resolution and stereo imaging, Near-IR (<2.0µm) imaging spectroscopy for global mineralogical mapping

7. MPO Instruments, 2 Some synergy issues may exist between MPO and MMO Mercury Radiometer and Thermal Imaging Spectrometer MERTISGlobal mineralogical mapping (7-14 µm), surface temperatures and thermal inertia Mercury Gamma-Ray and Neutron Spectrometer MGNSElemental surface & sub-surface composition, volatile deposits on polar areas Mercury Imaging X-ray SpectrometerMIXSElemental surface composition, global mapping and composition of surface features

8. Strong synergy issues between MPO and MMO MPO Instruments, 3 Magnetic Field InvestigationMERMAGDetailed description of planetary magnetic field, its source and interaction with Search for Exospheric Refilling and Emitted Natural Abundances SERENA: Elena, MIPA, PICAM, Strofio In-situ study of composition, vertical structure and source and sink processes of the exosphere Probing of Hermean Exosphere by Ultraviolet Spectroscopy PHEBUSUV spectral mapping of the exosphere Solar Intensity X-ray and particle SpectrometerSIXSMonitor solar X-ray intensity and solar particles in support of MIXS

9. Overview Table of Coordinated Observarions x x x x xx x x xxxx xxxxxx xxxxxxx x xxx xxx xxx x x x x x x x x x xx xx x x x x x x x x x