SH41B:
Linking the Solar Interior with the Corona: Observations, Models, and Data Assimilation I Posters

Session ID#: 3541

Thursday, 18 December 2014: 8:00 AM-12:20 PM
Poster Hall (Moscone_South)
Chairs:  Nagi Nicolas Mansour, NASA Ames Research Center, Moffett Field, CA, United States and Mausumi Dikpati, NSF-NCAR, High Altitude Observatory, Boulder, United States
Primary Convener:  Junwei Zhao, Stanford University, HEPL, Stanford, United States
Co-conveners:  Nagi Nicolas Mansour1, Irina Kitiashvili1 and Mausumi Dikpati2, (1)NASA Ames Research Center, Moffett Field, CA, United States(2)NSF-NCAR, High Altitude Observatory, Boulder, United States
OSPA Liaison:  Junwei Zhao, Stanford University, HEPL, Stanford, 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:

 
Quantifying Photospheric Processes Using a New Pixel Dynamics Model (4882)
Anthony Rasca, CU CIRES/NOAA SWPC, Boulder, United States, James Chen, Naval Research Lab, Washington, DC, United States and Alexei A Pevtsov, National Solar Observatory, Tucson, AZ, United States
 
Magnetic Flux Concentrations in Stratified Turbulent Plasma Due to Negative Effective Magnetic Pressure Instability (12139)
Sarah Jabbari1,2 and Axel Brandenburg1,2, (1)Stockholm University, Stockholm, Sweden, (2)Nordic Institute for Theoretical Physics, Stockholm, Sweden
 
Three Dimensional Chromospheric Temperature Structure of Sunspot (26719)
Debi Prasad Choudhary, California State University Northridge, Department of Physics and Astronomy, Northridge, CA, United States, Christian Beck, National Solar Observatory - SP, Sunspot, NM, United States and Reza Rezaei, Kiepenheuer–Institute for Solar Physics, Freiburg, Germany
 
Do New Solar Active Regions Trigger Flares in Existing Regions? (26890)
Yixing Fu and Brian T Welsch, University of California Berkeley, Berkeley, CA, United States
 
Realistic Modeling of Multi-Scale MHD Dynamics of the Solar Atmosphere (13934)
Irina Kitiashvili1, Nagi Nicolas Mansour1, Alan A Wray1, Seokkwan Yoon1 and Alexander G Kosovichev2, (1)NASA Ames Research Center, Moffett Field, CA, United States, (2)New Jersey Institute of Technology, Center for Computational Heliophysics, Edison, NJ, United States
 
Improving Synchronic Maps with Far-Side Active Region Emergence (Invited) (5332)
Lisa Upton, Southwest Research Institute Boulder, Boulder, CO, United States and David H Hathaway, NASA Ames Research Center, Moffett Field, CA, United States
 
Morphological model for quadrupolar δ sunspots (15929)
Kan Takizawa and Reizaburo Kitai, Kwasan and Hida Observatories, Kyoto University, Kyoto, Japan
 
Current and Kinetic Helicity of Long-Lived Activity Complexes (14129)
Rudolf Komm, National Solar Observatory, Tucson, AZ, United States and Sanjay Gosain, National Solar Observatory, Boulder, CO, United States
 
Detection of Fast-Moving Waves Propagating from Penumbra to Outside of Sunspots in the Photosphere (Invited) (5034)
Junwei Zhao, Stanford University, Stanford, United States, Ruizhu Chen, Stanford University, Department of Physics, Stanford, United States; Stanford University, Department of Physics, Stanford, CA, United States and Thomas Hartlep, BAER Institute, NASA Ames Research Center, Moffet Field, CA, United States
 
Temporal Evolution of Solar Interior Meridional Flow (17276)
Junwei Zhao, Stanford University, HEPL, Stanford, United States, R. S. Bogart, Stanford University, Stanford, CA, United States and Ruizhu Chen, W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, United States
 
Importance of Solar Atmospheric Coupling on P-Mode Power within Magnetic Elements (7035)
Andrew Gascoyne, University of Sheffield, Sheffield, S10, United Kingdom and Rekha Jain, University of Sheffield, Sheffield, United Kingdom
 
Measuring the Solar Meridional Circulation Using Local Helioseismology (25231)
Benjamin Greer, University of Colorado at Boulder, Boulder, CO, United States, Bradley Hindman, University of Colorado Boulder, JILA & Applied Mathematics, Boulder, United States and Juri Toomre, Joint Institute for Laboratory Astrophysics, Boulder, United States
 
Coronal Dynamics at Recent Total Solar Eclipses (17565)
Jay M Pasachoff1, Muzhou Lu1, Allen Bradford Davis1,2, Marek Demianski1, Voyto Rusin3, Metod Saniga4,5, Daniel B Seaton6, Robert Lucas7, Bryce A Babcock1, Ron Dantowitz8, Pavlos Gaintatzis9, Christina Seeger1, Craig Malamut10 and Amy Steele1,10, (1)Williams College, Williamstown, MA, United States, (2)Yale University, Astronomy, New Haven, CT, United States, (3)Astronomical Institute of Slovak Academy of Sciences, Tatranská Lomnica, Slovakia, (4)Slovak Academy of Sciences, Bratislava, Slovakia, (5)University of Technology, Vienna, Austria, (6)Southwest Research Institute, Boulder, CO, United States, (7)Sydney University, Sydney, Australia, (8)Clay Center Obs., Brookline, MA, United States, (9)Aristotle University of Thessaloniki, Thessaloniki, Greece, (10)Wesleyan University, Astronomy, Middletown, CT, United States
 
Heartbeat Of the Sun Derived With PCA From Solar Background Magnetic Field And Its Use For Prediction Of the Solar Activity (25595)
Valentina V Zharkova, Northumbria University, MPEE, Newcastle-Upon-Tyne, United Kingdom, Simon G Shepherd, University of Bradford, School of Engineering, Bradford, United Kingdom, Helen Popova, Lomonosov Moscow State University, Physics Department, Moscow, Russia and Sergei Zharkov, University of Hull, Physics and Mathematics, Hull, United Kingdom
 
Coupling and Correlation-analysis Between the Northern and Southern Hemispheres' Solar Cycle Features based on Sunspot Area Data (11768)
William Nolan Wilson, Lyndon State College, Lyndonville, VT, United States and Mausumi Dikpati, NSF-NCAR, High Altitude Observatory, Boulder, United States
 
Improving Solar Cycle Prediction Using Variational Data Assimilation in a Mean-Field Dynamo Model (10123)
Ching Pui Hung, Agrosphere Institute (IBG-3) Forschungszentrum Jülich, Deutschland, Germany, Laurene Jouve, IRAP - Observatoire Midi Pyrenees, Toulouse, France, Sacha Brun, CEA Commissariat à l'Energie Atomique Saclay, Gif-Sur-Yvette Cedex, France; AIM, CEA, SACLAY, France and Alexandre Fournier, Université de Paris, Institut de Physique du Globe de Paris, CNRS, Paris, France
 
Extrapolating Solar Dynamo Models Throughout the Heliosphere (14280)
Bradley Taylor Cox1,2, Mark S Miesch3, Kyle Augustson2,4 and Nicholas Andrew Featherstone4, (1)Bridgewater College, Physics, Bridgewater, VA, United States, (2)High Altitude Observatory, Boulder, CO, United States, (3)CU/CIRES NOAA/SWPC, Boulder, United States, (4)University of Colorado at Boulder, Boulder, CO, United States
 
Reconstructing meridional flow speed variation from synthetic magnetic observations by using EnKF data assimilation (25650)
Mausumi Dikpati, NSF-NCAR, High Altitude Observatory, Boulder, United States and Jeffrey L Anderson, University Corporation for Atmospheric Research, Boulder, United States
 
Large-scale flows and magnetic fields in solar-like stars from global simulation with and without tachocline (19834)
Gustavo Guerrero, UFMG Federal University of Minas Gerais, Belo Horizonte, Brazil, Alexander G Kosovichev, New Jersey Institute of Technology, Center for Computational Heliophysics, Edison, NJ, United States, Piotr K Smolarkiewicz, European Centre for Medium-Range Weather Forecasts, Wokingham, United Kingdom and Elisabete M de Gouveia Dal Pino, IAG Institute of Astronomy, Geophysics and Atmospheric Sciences, Sao Paulo, Brazil
 
A Babcock-Leighton solar dynamo model with multi-cellular meridional circulation in advection- and diffusion-dominated regimes (27211)
Bernadett Belucz1, Mausumi Dikpati2 and Emese Forgacs-Dajka1, (1)Eotvos Lorand University, Budapest, Hungary, (2)NSF-NCAR, High Altitude Observatory, Boulder, United States