SH31B
Mass and Energy Transfer between the Solar Photosphere and Corona II Posters

Wednesday, 16 December 2015: 08:00-12:20
Poster Hall (Moscone South)
Primary Conveners:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Conveners:  Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States
Chairs:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States
OSPA Liaisons:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Observing Propagation of Magnetoacoustic Waves from the Photosphere to the Corona in Sunspot Regions (77235)
Junwei Zhao, Stanford University, Stanford, CA, United States and Ruizhu Chen, Stanford University, W. W. Hansen Experimental Physics Laboratory, Stanford, CA, United States
 
On the Observation and Simulation of Solar Coronal Twin Jets (63244)
Jiajia Liu, University of Science and Technology of China, Hefei, China
 
Origin of the High-speed Jets Fom Magnetic Flux Emergence in the Solar Transition Region as well as Their Mass and Energy Contribuctions to the Solar Wind (82254)
Yang Liping, SIGMA Weather Group State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences, Beijing, China
 
Beyond spicule dynamics: spicule and fibril spectroscopy at high spatial and temporal resolution (82960)
Tiago Mendes Domingos Pereira, Institute for Theoretical Astrophysics, Oslo, Norway and Luc Rouppe van der Voort, University of Oslo, Oslo, Norway
 
Connections between heating processes in the chromosphere, transition region and low corona (85905)
Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Tracing Flows in the Solar Atmosphere Using the Bifrost Stellar Atmosphere Code (82150)
Pia Zacharias, University of Oslo, Institute of Theoretical Astrophysics, Oslo, Norway
 
Multifluid Modeling of the Partially Ionized Chromosphere with Effects of Impact Ionization, Radiative Recombination and Charge Exchange (82810)
Dr. Stefaan Poedts and Yana G Maneva, KU Leuven, CmPA, Leuven, Belgium
 
Impact of the Ion-Neutral Interaction Effects in the Solar Chromosphere (75302)
Juan Martínez-Sykora, LMSAL, San Francisco, CA, United States
 
Small Scale Dynamo Magnetism And the Heating of the Quiet Sun Solar Atmosphere. (Invited) (75555)
Tahar Amari, CNRS, Ecole Polytechnique., Paris Cedex 16, France
 
Simultaneous observations of Ellerman bombs by NST and IRIS (83171)
Yeon-Han Kim, KASI Korea Astronomy and Space Science Institute, Daejeon, South Korea
 
Observations of Small-scale IRIS Bombs (Reconnection Events) in an Evolving Active Region (86506)
Chad Allen Madsen1, Hui Tian2 and Edward E DeLuca2, (1)Boston University, Center for Space Physics, Boston, MA, United States, (2)SAO, Cambridge, MA, United States
 
Visibility of Hinode/XRT X-Ray Jets at AIA/EUV Wavelengths, a Temperature Indicator (74077)
Daniel Bakucz Canario, University of St Andrews, St Andrews, United Kingdom
 
An Analysis of A Tornado-Like Prominence Observed by SDO (66707)
Wensi Wang, University of Science and Technology of China, Hefei, China
 
Study on the temperature and density of erupting prominences associated with coronal mass ejections (82308)
Jin-Yi Lee1, John C Raymond2, Kathy Reeves2, Yong-Jae Moon1 and Kap-Sung Kim1, (1)Kyung Hee University, Yongin, South Korea, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
 
Magnetic Properties and Spectroscopic Diagnostics of the Formation of Magnetic Flux Ropes (63308)
Xin Cheng, Nanjing University, Nanjing, China
 
A self-consistent combined radiative transfer hydrodynamic and particle acceleration model for the X1.0 class flare on March 29, 2014 (70977)
Fatima Rubio da Costa1, Lucia Kleint2, Alberto Sainz Dalda3, Vahe Petrosian1 and Wei Liu4, (1)Stanford University, Stanford, CA, United States, (2)School of Engineering Institute of 4D Technologies, Windisch, Switzerland, (3)High Altitude Observatory, Boulder, CO, United States, (4)Bay Area Environmental Research Institute Palo Alto, Palo Alto, CA, United States
 
A Double Candle-Flame-Shaped Solar Flare Observed by SDO and STEREO (64631)
Tingyu Gou, University of Science and Technology of China, Hefei, China
 
Modeling the Emission from the 15 February 2011 Solar Flare using Multi-Filamented Simulations (82602)
Joel C Allred, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Determining the Energy Transport Through the Photosphere into Corona with HMI (80006)
Peter W Schuck and Spiro K Antiochos, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Coronal Heating: Testing Models of Coronal Heating by Forward-Modeling the AIA Emission of the Ansample of Coronal Loops (86785)
Anna V Malanushenko, High Altitude Observatory, Boulder, CO, United States
 
Exploration and Parameter Study of Active Region Luminosity (65205)
Amber Lenon, Syracuse University, Syracuse, NY, United States
 
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