Welcome
15:00 - 15:10: Join the call + Introduction
Proposal pitches
15:10 - 15:20 |
David Pegg, The Open University |
Explosive volcanism, what we can learn and what it might tell us about Mercury |
15:20 - 15:30 |
David Pegg, The Open University |
Tectonics, both local structures and large scale implications |
15:30 - 15:40 |
Indhu Varatharajan, DLR |
ML driven spectral analysis for maximising the Mercury surface science using integrated spectroscopy approach |
15:40 - 15:50 |
Jack Wright, The Open University |
What can Bepi tell us about volatile diven processes on Mercury? (morphology/morphometry? Volatile identity?) |
15:50 - 16:00 |
Jakub Vaverka, Charles University |
Plasma surface interaction (surface charging), dust charging and transport |
16:00 - 16:10 |
Joana Oliveira, ESA |
Are charged particles behaving differently near the known weak crustal magnetic fields? |
16:10 - 16:20 |
Nicolas Bott, CRPG-LESIA |
Chemical (e.g. what about Fe?) and mineralogical composition of the surface, and its evolution (e.g. space weathering) |
16:20 - 16:30 |
Ryan Dewey, University of Michigan |
How do characteristics of Mercury's surface affect the frequency/strength of the magnetospheric field-aligned currents? |
16:30 - 16:40 |
Simon Lindsay, University of Leicester |
What can PIXE tell us about the surface (examples: does it illuminate PSCs? better characterised low E input?) |
16:40 - 16:50 |
Weijie Sun, University of Michigan |
The influences of solar extreme events on Mercury's surface and exosphere, i.e., the sputtering. |
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SEIS Discussion
End of the meeting