Poster session (Group-A); Core time: 16:00-18:00 on 3 September (Tue).
A02 M. Druett (Stockholm U., Sweden)
A03 H. Tian (Peking U., China)
A04 Y. Chen (Peking U., China)
A05
A06
A07
A08
A09
A10A11A12A13A14A16A17A18A19A20A21A22A24
A25
A26A27A28A29A30
A31A32
A33
A35

Using tracer particles to study the density variations of fibrils
Observations of fine structures and fast dynamics in sunspot light bridges
UV bursts: magnetic reconnection in the lower solar atmosphere
Hinode and SDO Observations of a Two-Sided-Loop Coronal Jet:
A. Sterling (NASA/MSFC, USA)
Toward a General Picture for Jets.
Photospheric Magnetic Flux Cancellation and Associated Plasma
S.-H. Park (ISEE/Nagoya U., Japan)
Heating in the Upper Solar Atmosphere
Simulating nanoflares in the solar atmosphere: Analysis of synthetic
H. Bakke (RoCS, Norway)
observables
J. Jurčák (Astronomical InstituteConvective stability in the solar photosphereCAS, Czech Republic)
T. Ito (Nagoya U., Japan)
Experimental turbulent transport study with gradients and mean-flow
Wave modes excited by photospheric p-modes & mode conversion in
J. M. Riedl (KU Leuven, Belgium)
footpoints of coronal loops
T. Van Doorsselaere (KU Leuven,
Small scale generation by Uniturbulence in structured plasmasBelgium)
D. Jess (Queen's U. Belfast, UK)
Resonance Cavities - Wave amplification mechanisms in sunspot umbrae
C. Cartagena-Sanchez (Bryn Mawr Taylor Scale and Magnetic Reynolds Number Estimation via Two-Point
College, USA)
Spatial Correlations
T. Kawai (ISEE/Nagoya U., Japan) Nano-Flare Analysis using Machine Learning Techniques
S. Gunar (Astronomical InstituteOn the Influence of Hinode/SOT NFI instrumental effects on the visibility
CAS, Czech Republic)of simulated prominence fine structures in H-alphaA 2D two-fluid MHD code to model partially ionised plasma: calibration
L. Le Phuong (Northumbria U., UK)and benchmarking
SoLaBo-X: a cross-disciplinary research activity for heating, transport,
M. Nakata (NIFS, Japan)
and turbulence dynamics in solar/astrophysical and laboratory plasmas
S. Houston (Queen's U., UK)
Alfvén shocks: Polarimetric detections in the umbral chromosphere
L. van Driel-Gesztelyi (UCL-MSSL,How can subsurface magnetic reconnection change the elemental
UK)
composition in the solar corona?
L. van Driel-Gesztelyi (UCL-MSSL,
Evolution of anomalous coronal elemental composition in AR 12673
UK)
S. W. Tang (UCLA, USA)Time domain structures in magnetic flux rope experiments
Evolution and Plasma Diagnostics of the X-region connecting a set of
A. Ghosh (IUCAA & Kyoto U., India)
Trans-Equatorial Loops
R. Ishikawa (SOKENDAI/NAOJ,
Dynamics of the convective turbulence in the solar granulation studied byJapan)
the spectral line broadening and asymmetry
H. Eklund (RoCS-ITA-UiO, Norway) Shock wave propagation with high cadence solar ALMA time series
Study on chromospheric heating by fast and slow MHD waves using
Y. Wang (U. Tokyo, Japan)
realistic simulation
Investigating Hidden Energy in the Solar Corona Using Forward Modeling
V. Pant (KU Leuven, Belgium)of Magnetohydrodynamic Waves
Predictions of DKIST/DL-NIRSP observations for an off-limb kink-unstable
B. Snow (U. Exeter, UK)
coronal loop
E. Dzifcakova (Astronomical Institute Updated version of KAPPA package for the calculation of optically thin
CAS, Czech Republic)
spectra for the non-Maxwellian kappa-distributions
B. Snow (U. Exeter, UK)
Shock sub-structure in partially-ionised plasma.
J. C. Guevara Gomez (RoCS,Dynamics of solar isolated features observed by the Atacama LargeNorway)
Millimeter/submillimeter Array (ALMA)
F. Clemmensen (RoCS, Norway)
Coupled MHD-PIC framework for magnetic reconnection
Transient dynamics and energy transfer from the photosphere to the low
L. Tarr (NSO, USA)
corona: initial results from a coordinated ALMA, DST, Hinode, IRIS, andSDO observation campaign

A36 S. Tiwari (LMSAL, USA)
A37

N. Nitta (Lockheed Martin ATC,USA)A38 T. Oba (ISAS/JAXA, Japan)
A39

M. Yoshida (SOKENDAI/NAOJ,Japan)

A40 T. Yokoyama (U. Tokyo, Japan)
A41 M. Shimojo (NAOJ, Japan)
A42 T. Pereira (ITA-UiO, Norway)
A43 K. Ichimoto (Kyoto U., Japan)
A44 A. K. Awasthi (USTC, China)
A45 P. Kohutova (UiO, Norway)
A46 Y. Kotani (Kyoto U., Japan)
A47 J. Okamoto (NAOJ, Japan)

Transition Region Response of Moving Magnetic Features: Hinode andIRIS observations
Investigating the Magnetic Field in Sun’s Polar Regions in the Context ofUnderstanding and Predicting the Solar Wind at 1 AU
How does the solar surface convection form the asymmetry in spectral
profiles？
First Detection of Lyman-Alpha Scattering Polarization in Off-Limb
Spicules and Its Constraint on Their Magnetic Field
Observations of Photospheric Magnetic Structure below a Dark Filament
using the Hinode Spectro-Polarimeter
Cold and hot spicules observed with ALMA, IRIS and AIA/SDO
Spicule widths from high-resolution Ca II K observations
Temperature analysis of solar prominences by multi-wavelength
observations
What is inside a prominence bubble?
3D radiative MHD simulations of coronal rain formation and evolution
Numerical Simulations of Anemone Jets in the Solar Photosphere
Where is the strongest field located in sunspots ? - A statistical analysis
using Hinode/Spectro-Polarimeter 3DMHD simulation of nanoflare-like events in wave heated coronal loop

A48 T. Matsumoto (NAOJ, Japan)
J. Lorincik (Astronomical Institute
A49
Diagnostics of non-Maxwellian distributions in the solar corona
CAS, Czech Republic)
V. Hansteen (BAERA50
Ellerman bombs and UV bursts; temporal and spatial correspondence
Institute/LMSAL & RoCS/UiO, USA)
Diagnostics of the non-Maxwellian-distributions from Fe XVII–XVIII X-ray
E. Dzifcakova (Astronomical InstituteA51
coronal spectra: proposal for the Marshall Grazing-Incidence X-ray
CAS, Czech Republic)
Spectrometer (MaGIXS)
J. Stepan (Astronomical Institute
ASCR, Czech Republic)
A53 Y. Huang (Kyoto U., Japan)
A54 A. Russell (U. Dundee, UK)

Properties of spicules inferred from IRIS observations via approximate
Bayesian computation
Doppler velocity differences between ions and neutrals in a solar surge
Strong Viscous Damping of Coronal Alfven Waves
In-flight Calibration of the Hinode X-Ray Telescope: Correction for theA55 J. Shin (SSR/KHU, South Korea):
Scattered Lights
On the Evolution of Point-like Convective Collapse Events Seen in HighA56 Y. Suematsu (NAOJ, Japan)
Resolution Photospheric and Chromospheric Filtergrams of Hinode/SOT
A57 A. Norton (Stanford U., USA)
Delta-spot Properties Observed with HMI from 2011-2018
A magentised plasma experiment for laboratory simulation of space
A58 K. Ronald (U. Strathclyde, UK)plasma effects
Plasmoid and blob structure of current sheet in TS-6 torus plasma
A59 M. Akimitsu (U. Tokyo, Japan)
merging experiment
A60 B. Fleck (ESA)
Mapping the acoustic cut-off frequency in the solar atmosphere
Note: The "presenting authors" listed are the "contact authors" submitted.
A52

Poster session (Group-B); Core time: 16:00-18:00 on 5 September (Thu).
B01 L. Harra (UCL-MSSL, UK)
N. Kouassi (UFHB Abidjan, Côte d’Ivoire)
B03 V. Verma (USAC, India)
B04 M. Druett (Stockholm U., Sweden)
B02

B05 R. Dorst (UCLA, USA)
B06 A. Winebarger (NASA MSFC, USA)
M. V. Gutierrez Escate (IAFE
B07
CONICET--UBA, Argentina & Peru):
M. Talafha (Eötvös Loránd U.,
B08Hungary)
K.-S. Lee (U. Alabama Huntsville,B09USA)
B12
B13
B14
B15
B16
B17
B18
B19
B20
B21
B22
B23
B24
B25
B26
B27
B28
B29
B30
B31

Tracking the evolution of hot coronal plasma through `overlappograms' inresponse to magnetic flux emergence building up to an M2 flare
Geomagnetically Induction effects related to impulsive Space Weatherevents at low latitudes
Relationship of EIT Waves Phenomena with Coronal Mass Ejections
COCOPLOTs: imaging Halpha for a flare on 6th September 2017
Optical Ion Velocity Diagnostics in the Interaction of a Laser ProducedPlasma and an Ambient Magnetized Plasma
Unfolding EIS Slot Data
Sun's impact on Earth using Hα in comparison with Hinode data
Global dipole moment study using optimized surface flux transport model

Spectroscopic study of a limb flare observed by Hinode, SDO, RHESSI,
and STEREO
Critical Parameters of Photospheric Magnetic Field to Produce CMEs withP. H. Lin (ISEE/Nagoya U., Japan)
Active Region FlaresS. Masuda (ISEE/Nagoya U.,
Characteristics of big solar flares observed with RHESSI and NobeyamaJapan)
Radioheliograph
Back to the Surface: An Update on Coordinating Hinode Observations
H. Warren (NRL, USA)with the Parker Solar Probe Encounters
Improving Space Weather Forecasting With Wide-Field EUV
E. DeLuca (CfA, USA)
Observations
Particle acceleration and the evolution of nonthermal line broadening in
S. Matthews (UCL-MSSL, UK)solar flares
DeSIRer: a new, fast and flexible non local thermodynamic equilibrium
D. Orozco Suarez (IAA-CSIC, Spain)
inversion code
Diagnostic Capability of the Sunrise Chromospheric Infrared
Y. Katsukawa (NAOJ, Japan)
spectroPolarimeter (SCIP) for SUNRISE-3
K. Kihara (Kyoto U., Japan)
Statistical analysis of solar energetic particle events
M. Kubo (NAOJ, Japan)
High-precision & fast polarization measurements by SUNRISE-3/SCIP
Spatial Spectra of Magnetic Fields and Current Helicity by Using
T. Sakurai (NAOJ, Japan)
Hinode/SOT-SP Mosaic Magnetograms
Zebra-like spectral patterns in electron cyclotron emission ofM. Viktorov (IAP RAS, Russia)
nonequilibrium mirror-confined laboratory plasma
Solar cycle variation of coronal temperatures and emission measures
A. Takeda (Montana State U., USA)
(1991-2001) observed with Yohkoh Soft X-ray TelescopeFirst Step for Data Analysis of HINOTORI Soft X-ray Spectrometer (SOX)
T. Watanabe (NAOJ/NINS, Japan)
through IDL Routines
T. Hasegawa (U. Tokyo &General Formation Properties of the O I 1027 and 1028 Å lines near theISAS/JAXA, Japan)
Lyman β for the Diagnostics with Solar-C_EUVST
Chromospheric magnetic field: A comparison of He I 10830 Å
Y. Kawabata (U. Tokyo, Japan)
observations with nonlinear force-free field extrapolation
Polarization calibration of the Solar Magnetic Activity Research
D. Yamasaki (Kyoto U., Japan)
Telescope(SMART)
Polarization Calibration of the Chromospheric LAyer Spectro-Polarimeter
R. Ishikawa (NAOJ, Japan)(CLASP2)
A. Zemanova (Astronomical Institute Drift and Deformation of a Flux Rope Footpoint Observed during anCAS, Czech Republic)
Eruptive FlareM. Szydlarski (ITA-UiO, Norway)
SoAP - Solar ALMA Pipeline
Unified View of Solar and Stellar Flares : Can Superflares Occur on Our
K. Shibata (Kyoto U., Japan)
Sun ?

Fast filament eruption on 2017 April 23 detected by the Solar Dynamics
Doppler Imager (SDDI)
Estimation of solar ultraviolet irradiance by examining spectroheliogram ofH. Tanaka (Kyoto U., Japan)
Ca II K line
Lyman-Alpha Imaging Polarimetry with the CLASP2 Sounding Rocket
R. Kano (NAOJ, Japan)
MissionElectron Density Measurement at the Loop-Top Region of the 2017
N. Ono (NAOJ & U. Tokyo, Japan)
September 10 Solar Limb FlareK. Hori (NAOJ, Japan)
Visualizing the Hinode's results over the past 13 years
J. C. Guevara Gomez (RoCS,On the observation of a classical loop-prominence system during theNorway)
2017 September 10 flare
S. Nagata (Kyoto U., Japan)
The lateral motion of quasi circular flare ribbon to the quasi separatrix line
J. Lorincik (Astronomical InstituteObservations of three-dimensional magnetic reconnection in an eruption
CAS, Czech Republic)of a quiescent filamentParticle Acceleration in Quasi-Perpendicular Hall-Mediated Collisionless
D. Endrizzi (UW-Madison, USA)
ShocksS. Nishimoto (NDA, Japan)
Construction of Solar Flare EUV Emission Spectral Prediction Model
H. Tamazawa (Kyoto City U. of Arts, 1933 May 1 Goemagnetic Storm as an Example of Space weather EventJapan)
with No Sunspot
Flare Energy Release at the Magnetic Field Polarity Inversion Line During
I. Sharykin (IKI RAS, Russia)
the M1.2 Solar Flare of 2015 March 15. I. Onset of Plasma Heating andElectron Acceleration

B32 D. P. Cabezas (Kyoto U., Japan)
B33
B34
B35
B36
B37
B38
B39
B40
B41
B42
B43

B44 I. Sharykin (IKI RAS, Russia)

B45 I. Zimovets (IKI RAS, Russia)
B46 I. Sharykin (IKI RAS, Russia)
B47 A. Kawamura (Kyoto U., Japan)

Flare Energy Release at the Magnetic Field Polarity Inversion Line During
M1.2 Solar Flare of 2015 March 15. II. Investigation of PhotosphericElectric Current and Magnetic Field Variations Using HMI 135-second
Vector Magnetograms
Relationships between photospheric vertical electric currents and hard Xray footpoints in solar flares: statistical study for the 24th solar cycle
A Statistical Study of Seismically Active Solar Flares During 24th Solar
Cycle
Space Weather Utilities of Solar Flare Statistics based on Solar Cycle 23:
Sunspot, Flare, and Coronal Mass Ejection

J. Kasparova (Astronomical Institute
Modelling of chromospheric lines as observed during a C-class solar flare
CAS, Czech Republic)
Investigation of Free Magnetic Energy and Magnetic Helicity During M1.2
B49 I. Sharykin (IKI RAS, Russia)
Solar Flare of 15 March 2015 Using HMI 135-second Vector
Magnetograms
B48

B50 I. Sharykin (IKI RAS, Russia)
B51 J. Cheng (SHAO/CAS, China)
B52 H. Reid (UCL, UK)
B53 M. Weber (CfA, USA)
B54 J. Vievering (U. Minnesota, USA)
B55 K. Reeves (CfA, USA)
B57 N. Zambrana Prado (IAS, France)
B58 M. Varady (UJEP, Czech Republic)
B59 J. Reep (NRL, USA)
J. Rebellato (LCF/IOGS/CNRS &B60
CNES, France)
B61 S. Toriumi (ISAS/JAXA, Japan)

Fast Restructuring of The Magnetic Field in the Polarity Inversion Line
During M9.3 Solar Flare of 2011 July 30
Energy Release During Several M and X Class Flares
Combining LOFAR radio observations and simulations to understandsolar electron beam speeds and spatial expansion
Thermal Structure of Supra-Arcade Plasma in Solar Flares
FOXSI-2 Solar Microflares: Hard X-ray Spectroscopy and Multi-instrument
Differential Emission Measure Analysis
Solar X-ray Intensity vs. Magnetic Flux for Solar Cycle 24
Measuring relative abundances with SPICE, the EUV spectrometer onboard Solar Orbiter
Hybrid modelling of chromospheric HXR flare sources in the flare loops
Understanding the Evolution of He II Emission in Solar Flares
EUV mutlilayer coatings for Solar-C
The First Comparative Study of Data-driven Solar Coronal Field Models

B62 P. Bellan (Caltech, USA)How solar eruptions generate X-rays and energetic particles
B63 A. Savcheva (CfA, USA)
Local Quantities Analysis of Magnetofrictional and MHD Simulations
Note: The "presenting authors" listed are the "contact authors" submitted.

[Presentation instructions]・The panel size available for each poster is 90 cm (width) x 240 cm (height).
・Poster presentations are divided into two groups (Group-A and Group-B). The authors should bepresent at their posters in their assigned core times.
Group-A:
Posters can be put up from the morning of 3 September (Tue) until 17:00 of 4 September (Wed).
Core time: 16:00-18:00 on 3 September (Tue).
Group-B:
Posters can be put up from the morning of 5 September (Thu) until 17:00 of 6 September (Fri).
Core time: 16:00-18:00 on 5 September (Thu).