Click the time stamp to go to the specific talk.

0:00 Start
21:13 Reconnection in the Corona: A Call to ARMS, Richard Devore, NASA GSFC
43:27 Solar Reconnection: the Beginning of the Problem, but Also the End?, Hantao Ji, Princeton University
1:07:00 Modeling Particle Acceleration during Magnetic Reconnection in Macro-scale Systems, James Drake, Univ. of Maryland, College Park
2:11:53 Thermal Non-Equilibrium: As Fascinating and Important as Spiro Himself!, James A. Klimchuk, NASA GSFC
2:34:24 Thermal Non-equilibrium Near Magnetic Null Points Leading to the Formation of Coronal Rain and Prominences, Wei Liu, LMSAL/BAERI
2:54:55 Simulation of Thermal Nonequilibrium Cycles in the Solar Wind, Roger B. Scott, US Naval Research Laboratory
3:14:36 The Missing Cool Corona in the Flat Magnetic Field around Solar Active Regions, Alphonse C. Sterling, NASA MSFC
4:49:42 Characterizing the L1 In Situ Observed Solar Wind that Originates from the Magnetic Open-closed Boundary Identified by ADAPT-WSA, Samantha Wallace, Embry-Riddle Aeronautical Univ.
5:11:13 Simulations of Solar Jets, Etienne Pariat, Laboratoire de Physique des Plasmas, CNRS
5:31:19 Mesoscale Solar Wind Density Structures Created by Interchange Reconnection in the Solar Corona, Nicholeen Viall, NASA GSFC
5:52:10 Prospective Implications of EUV Coronal Plumes for Magnetic-network Genesis of Coronal Heating, Coronal-hole Solar Wind & Solar-Wind Magnetic Field Switchbacks, Ron Moore, UAH/ CSPAR/NASA MSFC
7:11:20 Interchange Reconnection and the Structure of Coronal Holes, Craig DeForest, SwRI
7:34:55 On the Role of Small-Scale Reconnection in the Dynamics of the Coronal and Solar Wind Plasma, Nour E. Raouafi, JHUAPL
7:56:14 Is Spiro AWSoM?, Igor Sokolov, Univ. of Michigan, Ann Arbor
8:13:22 CME and Pseudo-streamer Dynamics, Sophie Masson, Laboratoire de Physique des Plasmas, CNRS
8:29:46 Mapping the Martian Separatrix Web, Aleida Higginson, NASA GSFC