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


Session ID#: 9061

Session Description:
The transport and deposition of non-thermal energy from the photosphere through the chromosphere and transition region into the corona drives the dynamics and energetics of the low solar atmosphere and holds the key to chromospheric and coronal heating and solar wind acceleration. The coupling between photosphere and corona also plays an important role in flare initiation. Our view of these processes is rapidly changing with the advent of high resolution imaging and spectroscopy covering a wide range of temperatures from photosphere to corona, coupled with advanced numerical simulations. This session is focused on new views of the mass and energy transfer between the photosphere and corona, and welcomes contributions using recent observations with IRIS, SDO and Hinode and/or numerical simulations of the coupled solar atmosphere. Contributions on full-atmosphere observations of flares using IRIS, SDO and Hinode are encouraged as well.
Primary Convener:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Convener:  Scott William McIntosh, High Altitude Observatory, Boulder, 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, United States
OSPA Liaison:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Index Terms:

7507 Chromosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7519 Flares [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

Observing Propagation of Magnetoacoustic Waves from the Photosphere to the Corona in Sunspot Regions (77235)
Junwei Zhao, Stanford University, HEPL, Stanford, United States and Ruizhu Chen, Stanford University, Stanford, CA, United States
On the Observation and Simulation of Solar Coronal Twin Jets (63244)
Jiajia Liu1, Fang Fang2, Yuming Wang1, Scott William McIntosh3, Yuhong Fan4 and Quanhao Zhang1, (1)University of Science and Technology of China, Hefei, China, (2)High Altitude Observatory, Boulder, CO, United States, (3)High Altitude Observatory, Boulder, United States, (4)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States
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 Liping1, Jiansen He2, Hardi Peter3, Chuan-Yi Tu2 and Xue Shang Feng4, (1)SIGMA Weather Group State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences, Beijing, China, (2)Peking University, Beijing, China, (3)Max Planck Institute for Solar System Research, Göttingen, Germany, (4)State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;, 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
Multifluid Modeling of the Partially Ionized Chromosphere with Effects of Impact Ionization, Radiative Recombination and Charge Exchange (82810)
Stefaan Poedts1, Yana G Maneva1, Alejandro Alvarez Laguna2 and Andrea Lani3, (1)KU Leuven, CmPA, Leuven, Belgium, (2)KU Leuven, CmPA, Dover, NH, United States, (3)von Karman Institute for Fluid Dynamics, CFD group, Aeronautics and Aerospace, Rhode Saint-Genèse, Belgium
Impact of the Ion-Neutral Interaction Effects in the Solar Chromosphere (75302)
Juan Martínez-Sykora, LMSAL, San Francisco, CA, United States, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Viggo Haraldson Hansteen, Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway and Mats Carlsson, University of Oslo, Rosseland Centre for Solar Physics, Institute of Theoretical Astrophysics, Oslo, Norway
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 Kim1, Vasyl Yurchyshyn1,2, Il-Hyun Cho1, Jaejin Lee3, Young-deuk Park1, Heesu Yang4, Kwangsu Ahn5 and Phil Goode2, (1)KASI Korea Astronomy and Space Science Institute, Daejeon, Korea, Republic of (South), (2)Big Bear Solar Observatory, Big Bear City, CA, United States, (3)KASI Korea Astronomy and Space Science Institute, Daejeon, South Korea, (4)Seoul National University, Department of Physics and Astronomy, Seoul, Korea, Republic of (South), (5)Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, CA, United States
Observations of Small-scale IRIS Bombs (Reconnection Events) in an Evolving Active Region (86506)
Chad Allen Madsen, Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States, Hui Tian, School of Earth and Space Sciences, Peking, China and Edward DeLuca, Harvard-Smithsonian Center for Astrophysics, 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, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States, Ronald Lee Moore, NASA Marshall Space Flight Center, Huntsville, United States and David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States
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, Katharine Reeves2, Yong-Jae Moon3 and Kap-Sung Kim1, (1)Kyung Hee University, Yongin, Korea, Republic of (South), (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (3)School of Space Research, Kyung Hee University, Yongin, South Korea
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, Department of Physics, Stanford, CA, United States, (2)University of Applied Sciences and Arts Northwestern Switzerland, 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 Gou1, Rui Liu1, Yuming Wang1, Kai Liu2, Bin Zhuang2, Quanhao Zhang1 and Jiajia Liu1, (1)University of Science and Technology of China, Hefei, China, (2)USTC University of Science and Technology of China, Hefei, China
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, 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, National Center for Atmospheric Research, High Altitude Observatory, Boulder, United States
Exploration and Parameter Study of Active Region Luminosity (65205)
Amber Lenon, Syracuse University, Syracuse, NY, United States, Samaiyah Farid, University of Alabama in Huntsville, Huntsville, AL, United States, Amy R Winebarger, NASA Marshall Space Flight Center, Huntsville, AL, United States and David Allen Falconer, National Space Science and Technology Center, Huntsville, AL, United States

See more of: SPA-Solar and Heliospheric Physics