SH51C:
Mass and Energy Transfer Between the Solar Photosphere and Corona I Posters

Session ID#: 2888

Friday, 19 December 2014: 8:00 AM-12:20 PM
Not an Option (Moscone West)
Chairs:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Viggo Haraldson Hansteen, Institute for Theoretical Astrophysics, University of Oslo, Oslo, Norway
Primary Convener:  Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Co-conveners:  Viggo Haraldson Hansteen, Inst Theoretical Astrophysics, Oslo, Norway and Karel Schrijver, Lockheed Martin Adv Techn Ctr, Palo Alto, CA, 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]
7529 Photosphere [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7546 Transition region [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Virtual Option?: No

Abstracts Submitted to this Session:

 
Extremely Large Euv Late Phase of Solar Flares (8618)
Kai Liu1, Yuming Wang2, Jie Zhang3, Xin Cheng4, Rui Liu1, Chenglong Shen5 and Shui Wang1, (1)USTC University of Science and Technology of China, Hefei, China, (2)University of Science and Technology of China, Hefei, China, (3)George Mason University, Department of Physics and Astronomy, Fairfax, United States, (4)Nanjing University, Nanjing, China, (5)University Science & Technology of China, Hefei, Anhui, China
 
Negative Flare Emissions Observed in Euv By SDO/AIA (9876)
Yan Xu, Institute for Space Weather Sciences, New Jersey Institute of Technology, Newark, United States, Chang Liu, NJIT-Cent Solar Terrestria Res, Newark, NJ, United States, Wenda Cao, Big Bear Solar Observatory, New Jersey Institute of Technology, Big Bear City, United States, Ju Jing, New Jersey Institute of Technology - Institute for Space Weather Sciences, Newark, United States and Haimin Wang, New Jersey Institute of Technology, Edison, NJ, United States
 
Continuum Emission from a Microflare Kernel Observed by IRIS (29819)
Adrian Nigel Daw1, Adam F Kowalski1,2, Jean-Pierre Wuelser3, Gianna Cauzzi4,5, Joel C Allred6 and Steven Christe6, (1)NASA Goddard Space Flight Center, Greenbelt, United States, (2)University of Maryland, College Park, United States, (3)Southwest Research Institute, Boulder, United States, (4)National Solar Observatory, Boulder, United States, (5)INAF-Ossevatorio Astrofisico di Arcetri, Firenze, Italy, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
The Temperature Structure of Some Typical Flare Loop Systems (15065)
Tingyu Gou, Rui Liu and Yuming Wang, University of Science and Technology of China, Hefei, China
 
Chromospheric Acoustic Oscillations in Active Flaring Regions (2325)
Teresa Monsue, Vanderbilt University, Nashville, United States, Frank Hill, National Solar Observatory, Tucson, AZ, United States and Keivan Stassun, Vanderbilt University, Nashville, TN, United States
 
When and How Does a Prominence-like Jet Gain Kinetic Energy? (6509)
Jiajia Liu, Yuming Wang, Rui Liu, Quanhao Zhang, Kai Liu, Chenglong Shen and Shui Wang, USTC University of Science and Technology of China, Hefei, China
 
Damped Large Amplitude Oscillations in a Solar Prominence and Coronal Loops Triggered By Coronal Waves Associated with a Single Flare (9955)
Quanhao Zhang1, Yuming Wang1, Rui Liu1, Jie Zhang1,2, Chenglong Shen1, Kai Liu1 and Shui Wang1, (1)University of Science and Technology of China, Hefei, China, (2)George Mason University, Department of Physics and Astronomy, Fairfax, United States
 
Observations and Implications of Large-Amplitude Longitudinal Oscillations in a Solar Filament (26498)
Judith T Karpen1, Manuel Luna2, Kalman Joshua Knizhnik3, Karin Muglach4, Holly Robin Gilbert5, Therese Ann Kucera6, Vadim Uritsky7 and Tilaye Tadesse Asfaw6, (1)NASA GSFC, Greenbelt, United States, (2)Istituto de Astrofisico de Canarias, Las Palmas, Tenerife, Spain, (3)US Naval Research Laboratory, Washington, DC, United States, (4)Artep Inc., Ellicott City, MD, United States, (5)National Center for Atmospheric Research, Boulder, United States, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)Catholic University of America, Washington, United States
 
Analysis of Inter-moss Loops in the Solar Transition Region with IRIS and SDO/AIA: Automatic Event Detection and Characterization (31500)
Brian Fayock, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States; University of Alabama in Huntsville, Space Science, Huntsville, AL, United States, Amy R Winebarger, NASA Marshall Space Flight Center, Huntsville, AL, United States and Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Threaded-Field-Line Model for the Transition Region and Solar Corona (31745)
Igor Sokolov1, Bart van der Holst2 and Tamas I Gombosi2, (1)University of Michigan Ann Arbor, Climate and Space Sciences and Engineering, Ann Arbor, United States, (2)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Why Is Non-thermal Line Broadening of Lower Transition Region Lines Independent of Spatial Resolution? (28346)
Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Scott William McIntosh, High Altitude Observatory, Boulder, United States, Juan Martínez-Sykora, LMSAL, San Francisco, CA, United States, Hardi Peter, Max Planck Institute for Solar System Research, Göttingen, Germany and Tiago Mendes Domingos Pereira, University of Oslo, Oslo, Norway
 
Observables of Ion-Neutral Interaction Effects in the Solar Chromosphere (29236)
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; Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, United States, Tiago Mendes Domingos Pereira, Institute for Theoretical Astrophysics, Oslo, Norway, Jorrit Leenaarts, Stockholm University, Stockholm, Sweden and Mats Carlsson, University of Oslo, Rosseland Centre for Solar Physics, Institute of Theoretical Astrophysics, Oslo, Norway
 
Cool Plasma Observed in the FUV using IRIS (28519)
Don Schmit, Cooperative Institute for Research in Environmental Sciences, Boulder, CO, United States and Davina Innes, Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany
 
Macrospicule Jets in On-Disk Coronal Holes (19095)
Mitzi Adams, NASA Marshall Space Flight Center, ST13, Huntsville, AL, United States, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States and Ronald Lee Moore, University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States
 
Exploring Euv Spicules Using 304 Ang He II Data from SDO/AIA (10610)
Ian Ross Snyder1, Alphonse C Sterling2, David Allen Falconer1 and Ron L Moore1, (1)National Space Science and Technology Center, Huntsville, AL, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States
 
Prevalence of Micro-Jets from the Network Structures of the Solar Transition Region and Chromosphere (6915)
Edward DeLuca1, Hui Tian2, Steven R Cranmer1, Katharine Reeves3, Mari Paz Miralles4, Patrick McCauley1, Sean McKillop1 and IRIS, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)School of Earth and Space Sciences, Peking, China, (3)Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States, (4)Center for Astrophysics, Harvard & Smithsonian, Cambridge, United States
 
Comparing High-speed Transition Region Jets in Coronal Holes and Quiet Sun Regions (16229)
Rebecca T. Arbacher, Columbia University of New York, Palisades, NY, United States, Hui Tian, School of Earth and Space Sciences, Peking, China and Steven R Cranmer, Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States
 
Hi-C Observations of Penumbral Bright Dots (14603)
Shane Alpert1,2, Navdeep Kaur Panesar2, Ron L Moore2, Sabrina L Savage2 and Amy R Winebarger2, (1)Rice University, Dept. of Physics and Astronomy, Houston, TX, United States, (2)NASA Marshall Space Flight Center, Huntsville, AL, United States