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SCIENCE SPLINTER: 1pm Eastern, 10am Pacific, 7pm Paris, 2am Tokyo
Please contact the following to participate/contribute:
Hadi Madanian (hmadanian@swri.edu), Li-jen Chen , Imogen Gingen, Michael Starkey, Mihir Desai, Steven Schwartz
3-min flash talks plus discussion led by the chairs on solar wind events, shock nonstationarity, particle acceleration, ways to improve our understanding of shock processes using model-data comparisons, and other shock processes.
Goal: ID major projects/questions underway and those still to be addressed – Spawn further collaborations
SESSION NOTES AND LINE UP:
| Order | Speaker | Title |
|---|---|---|
| 0 | Session Chair | NOTES, Intro |
| 1 | Steve Schwartz et al. | Current Sheets in the Earth's Quasi-parallel Magnetosheath |
| 2 | Savvas Raptis | Jets downstream of quasi-parallel and quasi-perpendicular bow shock |
| 3 | Denny Oliveira | Can interplanetary shock impact angles control magnetospheric ULF wave activity? |
| 4 | Tomas Karlsson | Do SLAMS penetrate the bow shock? |
| 5 | Naoki Bessho | Kinetic waves and reconnecting current sheets in a quasi-parallel shock |
| 6 | Lynn Wilson | The discrepancy between simulation and observation of electric fields in collisionless shocks |
| 7 | Martin Lindberg | Entropy change across quasi-perpendicular shock |
| 8 | Imogen Gingell | Connecting Simulations & Observations of Kinetic Structures at the Bow Shock |
| 9 | Shan Wang | MMS observations of 3s ULF waves |
| 10 | Drew Turner | Formation of a fast magnetosonic shock |
| 11 | Li-Jen Chen | Solitary magnetic structures (isolated SLAMS): Dynamical origin |
| 12 | Hadi Madanian | What makes a shock layer? |
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