Chairs: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States and Viggo H Hansteen, Institute for Theoretical Astrophysics, Oslo, Norway
Primary Conveners: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Co-conveners: Viggo H Hansteen, Inst Theoretical Astrophysics, Oslo, Norway and Karel Schrijver, Lockheed Martin Adv Techn Ctr, Palo Alto, CA, United States
OSPA Liaisons: Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
Extremely Large Euv Late Phase of Solar Flares
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 Univ, Fairfax, VA, 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
Yan Xu1, Chang Liu1, Wenda Cao2, Ju Jing1 and Haimin Wang3, (1)NJIT-Cent Solar Terrestria Res, Newark, NJ, United States, (2)Big Bear Solar Observatory, Big Bear City, CA, United States, (3)New Jersey Institute of Technology, Newark, NJ, United States
Continuum Emission from a Microflare Kernel Observed by IRIS
Adrian Nigel Daw1, Adam F Kowalski1,2, Jean-Pierre Wuelser3, Gianna Cauzzi4,5, Joel C Allred1 and Steven Christe1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Maryland, College Park, MD, United States, (3)Lockheed Martin Solar and Astrophysics Laboratory, San Jose, CA, United States, (4)INAF-Ossevatorio Astrofisico di Arcetri, Firenze, Italy, (5)National Solar Observatory, Tucson, AZ, United States
Observations and Implications of Large-Amplitude Longitudinal Oscillations in a Solar Filament
Judith T Karpen1, Manuel Luna Bennasar2, Kalman Joshua Knizhnik3, Karin Muglach4, Holly Robin Gilbert1, Therese Ann Kucera1, Vadim M Uritsky5 and Tilaye Tadesse Asfaw1, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Istituto de Astrofisico de Canarias, Las Palmas, Tenerife, Spain, (3)Johns Hopkins University, Baltimore, MD, United States, (4)Artep Inc., Ellicott City, MD, United States, (5)Catholic University of America, Washington, DC, United States
Analysis of Inter-moss Loops in the Solar Transition Region with IRIS and SDO/AIA: Automatic Event Detection and Characterization
Brian Fayock, University of Alabama in Huntsville, Space Science, Huntsville, AL, United States; Center for Space Plasma and Aeronomic Research, 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
Igor Sokolov, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Bart van der Holst, University of Michigan, Ann Arbor, MI, United States and Tamas I Gombosi, Univ of Michigan, Ann Arbor, MI, United States
Wave Propagation in the Internetwork Chromosphere: Comparing IRIS Observations of Mg II h and k with Simulations
Bernhard Fleck, European Space Agency, Villanueva De La Can, Spain, Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Jorrit Leenaarts, Stockholm University, Stockholm, Sweden, Tiago M.D. Pereira, University of Oslo, Oslo, Norway and Thomas Straus, INAF/OAC, Naples, Italy
Why Is Non-thermal Line Broadening of Lower Transition Region Lines Independent of Spatial Resolution?
Bart De Pontieu, Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, Scott William Mcintosh, High Altitude Observatory, Boulder, CO, United States, Juan MartÃnez-Sykora, LMSAL, San Francisco, CA, United States, Hardi Peter, Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany and Tiago M.D. Pereira, University of Oslo, Oslo, Norway
Observables of Ion-Neutral Interaction Effects in the Solar Chromosphere
Juan MartÃnez-Sykora1, Bart De Pontieu2, Viggo H Hansteen2,3, Tiago M.D. Pereira3, Jorrit Leenaarts4 and Mats Carlsson5, (1)LMSAL, San Francisco, CA, United States, (2)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States, (3)Institute for Theoretical Astrophysics, Oslo, Norway, (4)Stockholm University, Stockholm, Sweden, (5)University of Oslo, Oslo, Norway
Macrospicule Jets in On-Disk Coronal Holes
Mitzi Adams, NASA Marshall Space Flight Center, ZP13, Huntsville, AL, United States, Alphonse C Sterling, NASA Marshall Space Flight Center, Huntsville, AL, United States and Ronald L Moore, University of Alabama in Huntsville, CSPAR, Huntsville, AL, United States
Prevalence of Micro-Jets from the Network Structures of the Solar Transition Region and Chromosphere
Edward E DeLuca1, Hui Tian1, Steven R Cranmer2, Kathy Reeves3, Mari Paz Miralles4, Patrick McCauley2 and Sean McKillop2, (1)SAO, Cambridge, MA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (3)Smithsonian Institution, Cambridge, MA, United States, (4)Harvard-Smithsonian CfA, Cambridge, MA, United States
Hi-C Observations of Penumbral Bright Dots
Shane Alpert1,2, Sanjiv K. Tiwari1, Ron L Moore1, Sabrina L Savage1 and Amy R Winebarger1, (1)NASA Marshall Space Flight Center, Huntsville, AL, United States, (2)Rice University, Dept. of Physics and Astronomy, Houston, TX, United States