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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:

OrderSpeakerTitle
0Session ChairNOTES, Intro
-1Katy GoodrichWhat We Know and What We Don't Know About Shocks.
1Steve Schwartz et al.Current Sheets in the Earth's Quasi-parallel Magnetosheath
2Savvas RaptisJets downstream of quasi-parallel and quasi-perpendicular bow shock
3Denny OliveiraCan interplanetary shock impact angles control magnetospheric ULF wave activity?
4Tomas KarlssonDo SLAMS penetrate the bow shock?
5Naoki BesshoKinetic waves and reconnecting current sheets in a quasi-parallel shock
6Lynn WilsonThe discrepancy between simulation and observation of electric fields in collisionless shocks
7Martin LindbergEntropy change across quasi-perpendicular shock
8Imogen GingellConnecting Simulations & Observations of Kinetic Structures at the Bow Shock
9Shan WangMMS observations of 3s ULF waves
10Drew TurnerFormation of a fast magnetosonic shock
11Li-Jen ChenSolitary magnetic structures (isolated SLAMS): Dynamical origin
12Hadi Madanian

What makes a shock layer?








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