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Tuesday Agenda

Tuesday Agenda. 0950 Summary of 2010 Modeling Meeting Mahadevan 1020 Coffee Break 1040 Front/Filament processes McWilliams 1100 Front/Filament processes Ozgokmen 1120 New simulations/Exp. guidance Molemaker 1120 Stirring by mixed patches Lelong 1140 Some recent results Smith

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Tuesday Agenda

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  1. Tuesday Agenda 0950 Summary of 2010 Modeling Meeting Mahadevan 1020 Coffee Break 1040 Front/Filament processes McWilliams 1100 Front/Filament processes Ozgokmen 1120 New simulations/Exp. guidance Molemaker 1120 Stirring by mixed patches Lelong 1140 Some recent results Smith 1155 IW’s, Vortical modes, PV, etc. Samelson 1210 Lunch 1310 June 2010 Virtual Experiment Ledwell 1325 2010 Pilot Experiment Report Levine et al. 1340 Discussion of hypotheses to test Kunze + all and how best to test them 1400 New simulations/Exp. guidance Molemaker 1430 Intro to new proposed 2011 exp plan Shearman 1500 Coffee 1520 INFLO: Field Support; issues Harcourt 1540 and data serving Harcourt 1600 2012 Experiment: Goals, Plans Lee/D’Asaro 1620 Discussion 1640 Summary; Goals/plan for Wed. Ledwell

  2. Wednesday Agenda - 2011 Experimental Plan Morning 0830 Breakfast Snacks, Coffee 0900 Intro D'Asaro 0920 Quick review of field assets Field PIs (1-2 slides ea) and ship resource needs 1000 Coffee 1020 Plan for a non-frontal exp Sundermeyer 1040 Plan for a filament/front exp Shearman 1100 Detailed 3-ship use plan D'Asaro 1130 Sci party, groups, chief All for each ship, final decisions 1200 Lunch

  3. Wednesday Afternoon 1300 Plan for developing INFLO Harcourt between now and June 1330 Breakout into groups: Field operations group Possibly subgroups by ship Modelling plans group Possibly subgroups 1500 Coffee 1530 Summary of breakout group deliberations 1550 Summary of decisions/mtg results Ledwell 1610 Assignments 1630 Next meeting/events

  4. LatMix Hypotheses Primary Hypotheses: 1. Inhomogeneous IW mixing creates PV anomalies that are responsible for significant isopycnal mixing. 2. Mesoscale straining leads to a cascade of both tracer and PV variance to submesoscales that is responsible for significant submesoscale isopycnal mixing. 3. Non-QG, submesoscale instabilities feed a forward cascade of energy, scalar and PV variance which enhances both isopycnal and diapycnal mixing.

  5. Goals of the Meeting Plan for the 2011 Field Experiment 3 Ships Aircraft/LIDAR INFLO Remote sensing, model products to ships Data from ships, aircraft, assets to shore/back out to ships Data Reporting Data Management Supporting Models (Plan for a Virtual Experiment in Spring 2011) Plan for future modeling activities

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