SH007
Solar Processes and Implications for Magnetic Activity: From the Interior Through the Surface and into the Heliosphere II

Monday, 7 December 2020: 20:30-21:30
Virtual
Primary Convener:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States
Convener:  Mausumi Dikpati, NCAR, Boulder, CO, United States
Primary Liaison:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States
Chairs:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States and Mausumi Dikpati, NCAR, Boulder, CO, United States
OSPA Liaison:  J Todd Hoeksema, Stanford University, HEPL, Stanford, CA, United States
20:30
SH007-01
Global-Scale Convective Flows: Window into the Dynamo (Invited) (702027)
Nicholas Andrew Featherstone, University of Colorado Boulder, Applied Mathematics, Boulder, CO, United States; Southwest Research Institute Boulder, Boulder, CO, United States, Bradley Hindman, University of Colorado Boulder, JILA & Applied Mathematics, Boulder, CO, United States, Keith A Julien, Univ of Colorado--Boulder, Applied Mathematics, Boulder, CO, United States and Geoffrey M Vasil, University of Sydney, Sydney, Australia
20:34
SH007-02
Properties of the Sun’s Giant Cellular Flows and their Implications for the Sun’s Activity Cycle (684135)
David H Hathaway, Stanford University, Stanford, CA, United States and Lisa Upton, Space Systems Research Corporation, Alexandria, VA, United States
20:38
SH007-03
Solar-Cycle Variation of the Subsurface Flows of Active and Quiet Regions (758763)
Rudolf Komm, National Solar Observatory, Tucson, AZ, United States
20:42
SH007-04
Helioseismic Constraints on the Solar Interior Dynamics and Dynamo (742774)
Alexander G Kosovichev, New Jersey Institute of Technology, Department of Physics, Edison, NJ, United States, Nicholas Brummell, University of California Santa Cruz, Santa Cruz, CA, United States, Mausumi Dikpati, NCAR, Boulder, CO, United States, Gustavo Guerrero, UFMG Federal University of Minas Gerais, Belo Horizonte, Brazil, Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States, Rudolf Komm, National Solar Observatory, Tucson, AZ, United States, Sylvain Korzennik, Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, Valery Pipin, Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, Russia, Johann Reiter, Technical University of Munich, Munich, Germany, Andrey Stejko, New Jersey Institute of Technology, Edison, NJ, United States, Roger K Ulrich, UCLA, Los Angeles, CA, United States and Joern Warnecke, Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
20:46
SH007-06
Continuous Subsurface Flow Measurements for Solar Cycle 23 from MDI Spherical Harmonic Time Series (762261)
Sushanta C Tripathy1, Shukirjon Kholikov2 and Kiran Jain1, (1)National Solar Observatory, Tucson, AZ, United States, (2)NSO/GONG, Tucson, AZ, United States
20:50
SH007-07
Explaining Empirical Relationships Found in Sunspot Number and Area Time Series with a Simplified Dynamo Model (729169)
Sushant Mahajan and Xudong Sun, University of Hawaii at Manoa, Institute for Astronomy, Honolulu, HI, United States
20:54
SH007-08
Inferring Plasma Flows in the Solar Photosphere & Chromosphere using Deep Learning and Surface Observations (757918)
Benoit Tremblay, Laboratory for Atmospheric and Space Physics, Boulder, CO, United States; National Solar Observatory, Tucson, AZ, United States, Kevin Reardon, National Solar Observatory, Boulder, CO, United States, Raphael Attié, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Andrés Asensio Ramos, Instituto de Astrofísica de Canarias, Tenerife, Spain, Maria Kazachenko, University of California Berkeley, Berkeley, CA, United States; University of Colorado at Boulder, LASP, Boulder, CO, United States and Dennis Tilipman, University of Colorado at Boulder, Astrophysical & Planetary Sciences, Boulder, CO, United States
20:58
Q&A Discussion
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