SH44A:
Linking the Solar Interior with the Corona: Observations, Models, and Data Assimilation II

Session ID#: 4407

Thursday, 18 December 2014: 4:00 PM-6:00 PM
2011 (Moscone West)
Chairs:  Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States and Junwei Zhao, Stanford University, HEPL, Stanford, United States
Primary Convener:  Irina Kitiashvili, NASA Ames Research Center, Moffett Field, CA, United States
Co-conveners:  Nagi Nicolas Mansour, NASA Ames Research Center, Moffett Field, CA, United States, Mausumi Dikpati, NSF-NCAR, High Altitude Observatory, Boulder, United States and Junwei Zhao, Stanford University, HEPL, Stanford, United States
OSPA Liaison:  Mausumi Dikpati, NSF-NCAR, High Altitude Observatory, Boulder, United States
Index Terms:

7507 Chromosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7529 Photosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7544 Stellar interiors and dynamo theory [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Virtual Option?: No
Swirl Theme: Convection and circulation across scales

Abstracts Submitted to this Session:

SH44A-01
Modeling the Convection Zone-to-Corona System over Global Spatial Scales (Invited) (4306)
William P Abbett, David John Bercik and George H Fisher, University of California Berkeley, Berkeley, CA, United States
SH44A-02
The Sun's Meridional Flow and Its Role in Magnetic Flux Transport and the Sunspot Cycle (Invited) (4003)
David H Hathaway, NASA Ames Research Center, Moffett Field, CA, United States and Lisa Upton, SSRC, Alexandria, United States
SH44A-03
Solar Meridional Flow from Helioseismic Observations (Invited) (4278)
Rudolf Komm, National Solar Observatory, Tucson, AZ, United States
SH44A-04
Dynamo Action and Meridional Circulation Dynamics in Eulag-MHD Global 3D MHD Simulations of Solar Convection (Invited) (4574)
Dário Manuel da Conceição Passos, CENTRA, Instituto Superior Técnico, Physics Dep., Lisbon, Portugal and Paul Charbonneau, Universite de Montreal, Montreal, QC, Canada
SH44A-05
Shaping Meridional Circulation in Solar and Stellar Convection Zones (Invited) (4841)
Nicholas Andrew Featherstone, University of Colorado at Boulder, Boulder, CO, United States and Mark S Miesch, CU/CIRES NOAA/SWPC, Boulder, United States
SH44A-06
Coronal Eruptions in Simulations of Magnetic Flux Emergence from the Convection Zone (Invited) (5039)
Fang Fang, High Altitude Observatory, Boulder, CO, United States, Yuhong Fan, NCAR, Boulder, United States and Scott William McIntosh, High Altitude Observatory, Boulder, United States
SH44A-07
Direct interlink of plasma in the convection zone and in the corona (21628)
Kiyoto Shibasaki, Nobeyama Solar Radio Observatory, Nagano, Japan
SH41B-4140
Measuring deep solar meridional flow by a new strategy (15159)
Ruizhu Chen, Stanford University, Department of Physics, Stanford, CA, United States; Stanford University, Department of Physics, Stanford, United States and Junwei Zhao, Stanford University, Stanford, United States
See more of: SPA-Solar and Heliospheric Physics