Poster schedule (last update: 2016-08-18):
This is the schedule for poster presentations at the conference.
Click
here
for the program of oral presentations.
Instructions for poster presentations:
The presenters will be required to display their works
during the two designated days (Mon-Tue or Wed-Thu).
The poster size should be smaller than
A0 size of 841 mm (width) x 1189 mm (height).
September 5 - 6 (Mon - Tue):
-
Pa-01 - Yusuke Iida (Kwansei Gakuin University)
Detection of Meridional Flow from Magnetic Elements Motion on The Solar Surface -
Pa-02 - Masumi Shimojo (National Astronomical Observatory of Japan)
What Solar Data will ALMA Provide to Us in Cycle 4 and Beyond? -
Pa-03 - Navin Joshi (Kyung Hee University, South Korea)
Possible Interaction of Two Filaments of Different Chiralities in 3D -
Pa-04 - Stanislav Gunár (Astronomical Institute of the Czech Academy of Sciences)
Prominences in the Age of ALMA: Synergies between High-resolution Radio and Optical Observations and 3D Modeling -
Pa-05 - Mark Weber (Harvard-Smithsonian Center for Astrophysics)
DEM maps with Hinode/XRT + SDO/AIA -
Pa-06 - Stephane Regnier (Northumbria University)
Low to High Frequency Heating of Multi-stranded Coronal Loops -
Pa-07 - Charalambos Kanellas (University of Oslo)
Investigating 4D (3D + Time) Solar Coronal (Joule) Heating Events in MHD Simulations -
Pa-08 - Krishna Mooroogen (Northumbria University Newcastle)
Measuring Kink Waves in the Internetwork H-α Chromosphere -
Pa-09 - Inigo Arregui (Instituto de Astrofisica de Canarias)
Inference of the Magnetic Field Strength from Oscillations in Solar Atmospheric Waveguides -
Pa-10 - Pia Zacharias (University of Oslo)
New Insights into the chromosphere-corona mass cycle -
Pa-11 - Clara Froment (Institut d'Astrophysique Spatiale)
Long-period Intensity Pulsations as the Manifestation of the Heating Stratification and Timescale in Coronal Loops -
Pa-12 - Dae Jung Yu (KU Leuven)
Excitation and resonant absorption of standing kink oscillations -
Pa-13 - Masahito Kubo (National Astronomical Observatory of Japan)
Ubiquitous Fast Propagating Intensity Disturbances in Solar Chromosphere -
Pa-14 - Tetsu Anan (Kyoto University)
Spicules and Network Bright Points -
Pa-15 - Steven Saar (SAO)
Long-term Study of Properties of X-ray Bright Points and Related Structures with Hinode XRT -
Pa-16 - Kiyoto Shibasaki (Solar Physics Research Inc.)
Cause of Loop-Top Plasma Concentration and Temperature Dependent Up-Flow -
Pa-17 - Susanna Parenti (Institut d'Astrophisique Spatiale)
Off-Limb Hot Thermal Plasma Properties of AR 11459 with SOHO/SUMER and Hinode/EIS Observations -
Pa-18 - Jayant Joshi (Stockholm University)
Upper Chromospheric Magnetic Field of a Sunspot Penumbra: Observations of Fine Structure -
Pa-19 - Graham Barnes (NWRA)
Estimating the Lorentz Force at the Photosphere -
Pa-20 - Shinsuke Imada (Institute for Space-Earth Environmental Research (ISEE), Nagoya University)
Temporal Evolution of the Current Sheet During the Flux Emergence -
Pa-21 - (withdraw)
-
Pa-22 - Sargam Mulay (University of Cambridge)
Temperature and Density Structure of a Recurring Active Region Jet -
Pa-23 - Naoto Nishizuka (National Institute of Information and Communications Technology)
Relationship Between Chromospheric Anemone Jets in an Active Region and Photospheric Magnetic Field Dynamics -
Pa-24 - Shuoyang Wang (The University of Tokyo)
Study of Tearing Mode Coupling in a Single Sheared Current Sheet via MHD Simulations -
Pa-25 - Navdeep Panesar (NASA Marshall Space Flight Center)
A Series of Streamer-Puff CMEs Driven by Solar Jets from the Active Region 12192 -
Pa-26 - Yoshiaki Oi (The University of Tokyo)
Flux Rope Formation and Eruption in a Quadrupolar Active Region Holding a Delta-spot -
Pa-27 - Rohit Sharma (National Centre For Radio Astrophysics, TIFR, Ganeshkhind, Pune - 411007)
On The Bright Loop Top Emission In Post Eruption Arcades. -
Pa-28 - Jack Carlyle (University of Oslo)
A Set Of Flare Models For Observational Solar Physicists -
Pa-29 - (withdraw)
-
Pa-30 - Yuta Notsu (Kyoto University)
High dispersion spectroscopy of solar-type superflare stars with Subaru/HDS -
Pa-31 - Ivan Sharykin (Space Research Institute of RAS)
Observational Investigation of Energy Release in the Lower Solar Atmosphere of a Solar Flare -
Pa-32 - Akiko Tei (Kyoto University)
Dynamic Response of the Chromosphere in a Solar Flare Based on Spectroscopic Observations -
Pa-33 - Johan Muhamad (Nagoya University)
MHD Data-driven Simulation for Studying Solar Flare Trigger Mechanismns -
Pa-34 - Takuya Shibayama (ISEE, Nagoya University)
Fast Magnetic Reconnection Supported by Sporadic Small-scale Petschek-type Shocks -
Pa-35 - Tomoko Kawate (ISAS/JAXA)
High Temperature EUV lines at H-alpha Flare Kernels -
Pa-36 - Satoshi Inoue (Max-Planck Institute for Solar System Research)
Onset Process of an X2.2-Class Solar Flare on 2011 February 15 -
Pa-37 - Miho Janvier (Institut d'Astrophysique Spatiale)
Evolution of Flare Ribbons, Electric Currents and QSLs During Flares -
Pa-38 - Elena Dzifcakova (Astronomical Institute of the Czech Academy of Sciences)
Diagnostics of the Kappa-Distribution from EVE Flare Spectra -
Pa-39 - Satoshi Masuda (Nagoya University)
Microwave Observations of White-Light and No White-Light Flares -
Pa-40 - Denis Cabezas (Kyoto University)
"Dandelion" Filament Eruption and Coronal Waves Associated with a Solar Flare on 2011 February 16 -
Pa-41 - Takahiro Hasegawa (University of Tokyo)
Magnetic Helicity Injection in A Flare-Productive Active Region -
Pa-42 - Anand Joshi (NAOJ)
A Trio of Confined Flares in AR 11087 -
Pa-43 - Takuya Takahashi (Kyoto University)
Energetics study on flux rope eruption driven by magnetic reconnection in turbulent current sheet -
Pa-44 - Shin'ichi Nagata (Kyoto University)
The Rapid Photospheric Vector Magnetic Field Evolution Observed during an Impulsive Flare in NOAA 12403 -
Pa-45 - (withdraw)
-
Pa-46 - Naoto Nishizuka (National Institute of Information and Communications Technology)
Machine-learning Flare Prediction Using Vector Magnetogram and Chromospheric Brightening -
Pa-47 - David Williams (European Space Agency)
The Velocity Field of Cool Erupting Filament Material in 3D Using Resonant Opacity -
Pa-48 - Seiji Yashiro (The Catholic University of America)
Coronal Mass Ejections form Non-sunspot Regions and their Space Weather Consequences -
Pa-49 - (withdraw)
-
Pa-50 - Jeffrey Reep (National Research Council Post-doc, Naval Research Laboratory)
Building a Multi-threaded Flare Model with RHESSI, Hinode, and IRIS -
Pa-51 - Ozora Kanou (Nagoya university)
Study of The Generation/Disappearance Processes of Coronal Hole Using Large-Scale Image Data -
Pa-52 - (withdraw)
-
Pa-53 - Yuto Bekki (The University of Tokyo)
Numerical Study of Double-Cell Type Solar Meridional Circulation Based on Mean-Field Hydrodynamic Model -
Pa-54 - Kirill Kuzanyan (IZMIRAN, Russian Academy of Sciences)
Current Helicity in the Solar Cycle, the Properties of Turbulent Magnetic Field from Mosaic SOT/SP Raster Scans and Messages for Dynamo Theory -
Pa-55 - Chiaki Ichimura (The university of Tokyo)
Non-Kinematic Flux Transport Dynamo Including the Effect of Diffusivity Quenching -
Pa-56 - Carlos Quintero Noda (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
Characterization of Spectral Lines for Chromospheric Polarimetry with Sunrise/SP and Solar-C/SUVIT -
Pa-57 - Ted Tarbell (Lockheed Martin)
Hinode SOT Images Coaligned with SDO and IRIS Level 2 Data Products -
Pa-58 - Noriyuki Narukage (National Astronomical Observatory of Japan)
Temporal variation in the Ly-alpha linear polarization observed with the CLASP sounding rocket -
Pa-59 - Kentaro Yaji (National Astronomical Observatory of Japan)
EPO Coordinated Observations for High School Students - Let's observe the sun with Hinode ! - -
Pa-60 - Melania Cubas Armas (Instituto de Astrofísica de Canarias (IAC), Avda Vía Láctea S/N, 38200 La Laguna, Tenerife, Spain)
Uncertainties In The Solar Photospheric Oxygen Abundance Determination
September 7 - 8 (Wed - Thu):
-
Pb-01 - Bruce Lites (National Center for Atmospheric Research)
Exploring Quiet Sun Magnetism at High Polarimetric Sensitivity: Internetwork Fields Are Indeed Dominantly Horizontal -
Pb-02 - Yoshiaki Kato (University of Oslo)
Automatic Detection of Vortex Flows in the Solar Chromosphere -
Pb-03 - (withdraw)
-
Pb-04 - RAMESH CHANDRA (KUMAUN UNIVERSITY NAINITAL)
QUIESCENT FILAMENT ERUPTION ON 29 SEPTEMBER 2013 -
Pb-05 - SANJAY KUMAR (KYUNG HEE UNIVERSITY, YONGIN-SI, SOUTH KOREA)
Decay-Less Standing Longitudinal Oscillations in Hot Coronal Loops -
Pb-06 - (withdraw)
-
Pb-07 - Sergiy Shelyag (Northumbria University, Newcastle upon Tyne)
The role of partial ionization in chromospheric heating -
Pb-08 - Girjesh Gupta (Inter-University Centre for Astronomy and Astrophysics (IUCAA))
Spectroscopic Evidence of Temperature Dependent Damping of Alfvén Waves in the Off-limb Solar Corona -
Pb-09 - Shunya Kono (The University of Tokyo)
1.5D Numerical Simulations of Alfven Waves in the Chromosphere: Reflection and Mode Conversion -
Pb-10 - Bernhard Fleck (ESA)
Testing Wave Propagation Properties in the Internetwork Chromosphere with ALMA, IRIS and Ground-based Observations -
Pb-11 - (withdraw)
-
Pb-12 - Munehito Shoda (The University of Tokyo)
New 1D Modelling of the Chromosphere-Corona-Solar Wind System Including Heating by Shocks and Turbulence -
Pb-13 - Krishna Prasad Sayamanthula (Queen's University Belfast)
Propagation and Damping of Slow Magnetoacoustic Waves in Sunspots -
Pb-14 - Artem Ulyanov (P.N. Lebedev Physical Institute of RAS)
Recurrent High-speed Chromospheric Evaporation Registered with Spectroheliograph MgXII/SPIRIT -
Pb-15 - Nur Shariff (UNIVERSITI TEKNOLOGI MARA)
Signal Processing of Solar Radio Burst Data in E-CALLISTO Network (Malaysia) -
Pb-16 - Pradeep Kayshap (Inter-University Centre for Astronomy and Astrophysics (IUCAA))
On the relationship between Cool and Hot Jets -
Pb-17 - Takahito Sakaue (Kyoto University)
Observational Study on the Acceleration Mechanism of a Solar Jet by Spectral Analysis -
Pb-18 - Shin-nosuke Ishikawa (ISAS/JAXA)
CLASP/SJ observation of time variations of Lyman-alpha emissions in a solar active region -
Pb-19 - Nooshin Jamshidi (Ferdowsi University of Mashhad)
Multi-Wavelength Study of the Magnetic Field Structure of a Sunspot -
Pb-20 - Daikou Shiota (Nagoya University)
Development of Nonlinear Force-Free Field Extrapolation Analysis Environment on the basis of Hinode/SOT-SP and SDO/HMI -
Pb-21 - Antonia Savcheva (Harvard-Smithsonian Center for Astrophysics)
Comprehensive Study of Jet Properties with Hinode, IRIS, SDO, and Magnetic Field Modeling -
Pb-22 - (withdraw)
-
Pb-23 - Zety Hamidi (UNIVERSITI TEKNOLOGI MARA)
An Observation of Broken Type II Solar Burst on 13th November 2012 at the National Space Centre, Malaysia by Using the CALLISTO System -
Pb-24 - Kyoko Watanabe (National Defense Academy of Japan)
Statistical approach for the origin of white-light emission of white-light flares -
Pb-25 - Sabrina Savage (NASA MSFC)
Observational Signatures of Magnetic Reconnection in the Extended Corona -
Pb-26 - Adam Kobelski (University of Alabama in Huntsville)
Supra Arcade Downflows with XRT Informed by Dipolarization Fronts with THEMIS -
Pb-27 - Natasha Jeffrey (University of Glasgow)
The Spatial and Spectral Distributions of Solar Flare Ions from Extreme Ultraviolet Spectroscopy -
Pb-28 - Alan Title (Lockheed Martin Advance Technology Laboratory)
Flare clustering -
Pb-29 - Yuta Notsu (Kyoto University)
Statistical properties of superflares on solar-type stars with Kepler data -
Pb-30 - Ivan Sharykin (Space Research Institute of RAS)
High Resolution Observations of Flare Energy Release in Twisted Magnetic Configuration from Hinode -
Pb-31 - Kosuke Namekata (Kyoto University)
Statistical Research on Solar White-Light Flares and Comparison with Superflares on Solar-type Stars -
Pb-32 - Hisashi Hayakawa (Kyoto University)
Carrington event observed in East Asia: testimonies from historical documents in the Far East -
Pb-33 - Shinsuke Takasao (Nagoya University)
Oscillatory Nature of Solar Flares: What Can We Learn from Observations? -
Pb-34 - Naoyuki Ishiguro (Nagoya University)
Double Arc Instability in the Solar Corona -
Pb-35 - Shohei Nishimoto (National Defense Academy of Japan)
Statistical Analysis of Solar Flare Spectra for the Influence of Solar-Terrestrial Environment -
Pb-36 - Hiroyuki Maehara (National Astronomical Observatory of Japan)
Starspot Activity and Superflares on Solar-type Stars -
Pb-37 - Elena Dzifcakova (Astronomical Institute of the Czech Academy of Sciences)
Non-equilibrium EUV Spectra Formed by the Electron Beam -
Pb-38 - Giulio Del Zanna (University of Cambridge)
Recurrent flares observed by Hinode/EIS -
Pb-39 - Yusuke Kawabata (The University of Tokyo)
Studies on Homologous Flares at Quadrupolar Magnetic Field Using Force-Free Field Modeling -
Pb-41 - Jeongwoo Lee (Seoul National University)
Evolution of Magnetic Separatrix due to Multiple Eruptions -
Pb-42 - Nariaki Nitta (Lockheed Martin Solar and Astrophysics Laboratory)
Observations of Flare Ribbons in Eruptive and Non-Eruptive Events -
Pb-43 - Daikichi Seki (Graduate School of Advanced Integrated Studies in Human Survivability, Kyoto University)
The Relation between The Tendency of Filament Eruptions and The Characteristics of Filaments -
Pb-44 - Kumi Hirose (Kyoto University)
A Statistical Study of Filament Disappearances using Hα Full Disk Images -
Pb-45 - Masaki Yoshida (The Graduate University for Advanced Studies)
Structures of Turbulent Plasma Motions in the Cusp Region of the 2015 Mar 7 Flare -
Pb-46 - Yihua Yan (National Astronomical Observatories, Chinese Academy of Sciences)
Analysis of a Backside CME Event on 11 Nov 2014 -
Pb-47 - Elena Kupriyanova (KU Leuven)
Diagnostics of the Source of Quasi-Periodicities During the Circular Ribbon Flare -
Pb-49 - Antonia Savcheva (Harvard-Smithsonian Center forAstrophysics)
Data-constrained Simulation of CME Initiation and Propagation: Comparison with Observations -
Pb-50 - Tanmoy Samanta (Indian Institute of Astrophysics)
Spectral Properties of Transition Region and Coronal Lines of an Equatorial Coronal Hole -
Pb-51 - Shinsuke Imada (ISEE, Nagoya University)
Towards Predicting Next Solar Cycle -
Pb-52 - Haruhisa Iijima (Nagoya University)
New Surface Flux Transport Code Based on the Yin-Yang grid -
Pb-53 - Masashi Fujiyama (Nagoya University)
Study of Differential Rotation and Meridional Flow using Solar Surface Magnetic Field Observation -
Pb-54 - Kirill Kuzanyan (IZMIRAN, Russian Academy of Sciences)
The Study of Solar Cyclicity in Tilt and Helicity of Large-Scale Magnetic Field Using a Century Long Synoptic Data Series of Filament Data -
Pb-55 - Alberto Sainz Dalda (High Altitude Observatory)
A Statistical Comparison Between Hinode-SOT/SP and SDO/HMI Magnetic Field Data Products -
Pb-56 - Neal Hurlburt (LMATC)
An Integrated Solar Observation and Event Search Tool using the Heliophysics Events Knowledgebase (HEK) -
Pb-57 - Lindsay Glesener (University of Minnesota)
Recent Results from the Focusing Optics X-ray Solar Imager -
Pb-58 - Kiyoshi Ichimoto (Kyoto University)
New Birefringent Tunable Filters and Their Applications for Study of Chromospheric Dynamics -
Pb-59 - Edward DeLuca (Harvard-Smithsonian Center for Astrophysics)
An EUV Wide-Field Imager and Spectrometer for the ISS -
Pb-60 - David Williams (European Space Agency)
Solar Orbiter Science Operations: Not A Typical Heliophysics Mission