Poster session (Group-B), coffee/tea

Total 60 posters.

Tracking the evolution of hot coronal plasma through `overlappograms' in response to magnetic flux emergence building up to an M2 flare

Louise Harra, UCL-MSSL, United Kingdom

Takahiro Hasegawa, University of Tokyo, Japan

Kyoung-Sun Lee, University of Huntsville, United States

David Long, UCL-MSSL, United Kingdom

Toshifumi Shimizu, ISAS, Japan

Sarah Matthews, UCL-MSSL, United Kingdom

Hirohisa Hara, NAOJ, Japan

Magnus Woods, UCL/MSSL, United Kingdom

Geomagnetically Induction effects related to impulsive Space Weather events at low latitudes

Nguessan Kouassi, Université Félix Houphouet Boigny Abidjan - Cote d' ivoire, Côte d’Ivoire

Vafi DOUMBIA, Université félix Houphouet Boigny Abidjan - Cote d' ivoire, Côte d’Ivoire

Boka Kouadio, Université félix Houphouet Boigny Abidjan - Cote d' ivoire, Côte d’Ivoire

Relationship of EIT Waves Phenomena with Coronal Mass Ejections

Virendra Verma, Uttarakhand Space Application Center, India

COCOPLOTs: imaging Halpha for a flare on 6th September 2017

Malcolm Druett, Stockholm University, Sweden

Alex Pietrow, Stockholm University, Sweden

Carolina Robustini, Stockholm University, Sweden

Gregal Vissers, Stockholm University, Sweden

Optical Ion Velocity Diagnostics in the Interaction of a Laser Produced Plasma and an Ambient Magnetized Plasma

Robert Dorst, UCLA, United States

Peter Heuer, UCLA, United States

Martin Weidl, UCLA, United States

Derek Scaeffer, Princeton University, United States

Carmen Constantin, UCLA, United States

Steve Vincena, UCLA, United States

Shreekrishna Tripathi, UCLA, United States

Walter Gekelman, UCLA, United States

Dan Winske, Los Alamos National Laboratory, United States

David Larson, Lawrence Livermore National Laboratory, United States

Christoph Niemann, UCLA, United States

Unfolding EIS Slot Data

Amy Winebarger, NASA MSFC, United States

Kyoung-Sun Lee, University of Alabama Huntsville, United States

Harry Warren, Naval Research Laboratory, United States

Katharine Reeves, Smithsonian Astrophysical Observatory, United States

Sabrina Savage, NASA MSFC, United States

Christian Bethge, Universities Space Research Association, United States

Sun's impact on Earth using Hα in comparison with Hinode data

Maria Victoria Gutierrez Escate, Instituto de Astronomía y Física del Espacio (CONICET­-UBA), Buenos Aires, Argentina, Peru

Germán Diego Cristiani, Departamento de Física, Universidad de Buenos Aires (UBA), Buenos Aires, Argentina, Argentina

Global dipole moment study using optimized surface flux transport model

Mohammed Talafha, Eötvös Loránd University, Department of Astronomy, Hungary

Kristóf Petrovay, Eötvös Loránd University, Department of Astronomy, Hungary

Spectroscopic study of a limb flare observed by Hinode, SDO, RHESSI, and STEREO

Kyoung-Sun Lee, The University of Alabama in Huntsville, United States

Hirohisa Hara, National Astronomical Observatory of Japan, Japan

Kyoko Watanabe, National Defense Academy of Japan, Japan

David, H. Brooks, George Mason University, United States

Anand D. Joshi, National Defense Academy of Japan, Japan

Shinsuke Imada, Nagoya University, Japan

Phillip Dang, Software Developer at Call Box, United States

Toshifumi Shimizu, ISAS/JAXA, Japan

Sabrina L. Savage, NASA Marshall Space Flight Center, United States

Critical Parameters of Photospheric Magnetic Field to Produce CMEs with Active Region Flares

Pei Hsuan Lin, Institute for Space-Earth Environmental Research, Nagoya University, Japan

Kanya Kusano , Institute for Space-Earth Environmental Research, Nagoya University, Japan

Daikou Shiota, National Institute of Information and Communications Technology (NICT), Japan

Satoshi Inoue, Institute for Space-Earth Environmental Research, Nagoya University, Japan

K.D. Leka, Institute for Space-Earth Environmental Research, Nagoya University; NorthWest Research Associates, Inc, Japan

Characteristics of big solar flares observed with RHESSI and Nobeyama Radioheliograph

Satoshi Masuda, ISEE, Nagoya University, Japan

Sam Krucker, University of Applied Sciences Northwestern Switzerland, Swaziland

Stephen White, Air Force Research Laboratory, United States

Back to the Surface: An Update on Coordinating Hinode Observations with the Parker Solar Probe Encounters

Harry Warren, NRL, United States

David Brooks, George Mason University, United States

Improving Space Weather Forecasting With Wide-Field EUV Observations

Edward DeLuca, Center for Astrophysics - Harvard & Smithsonian, United States

Particle acceleration and the evolution of nonthermal line broadening in solar flares

Sarah Matthews, UCL-MSSL, United Kingdom

Louise Harra, PMOD-WRC/ETH Zurich, Switzerland

Ryan French, UCL-MSSL, United Kingdom

David Long, UCL-MSSL, United Kingdom

Lidia van Driel-Gesztelyi, UCL-MSSL/LESIA Observatoire de Paris/Konkoly Observatory, United Kingdom

DeSIRer: a new, fast and flexible non local thermodynamic equilibrium inversion code

David Orozco Suarez, Instituto de Astrofísica de Andalucía (IAA-CSIC), Spain

Carlos Quintero Noda, Rosseland center for solar physics, Norway

Basilio Ruiz cobo, Instituto de Astrofísica de Canarias, Spain

Han Uitenbroek, National Solar Observatory (NSO-USA), United States

Ricardo Gafeira, Instituto de Astrofísica de Andalucía (IAA-CSIC), Spain

Diagnostic Capability of the Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) for SUNRISE-3

Yukio Katsukawa, National Astronomical Observatory of Japan, Japan

Jose Carlos del Toro Iniesta, IAA-CSIC, Spain

Sami K. Solanki, MPS, Germany

Masahito Kubo, National Astronomical Observatory of Japan, Japan

Carlos Quintro Noda, Univ. of Oslo, Norway

Hirohisa Hara, National Astronomical Observatory of Japan, Japan

Toshifumi Shimizu, ISAS/JAXA, Japan

Takayoshi Oba, ISAS/JAXA, Japan

David Orozco Suarez, IAA-CSIC, Spain

Andreas Lagg, MPS, Germany

SUNRISE-3 SCIP team

Statistical analysis of solar energetic particle events

Kosuke Kihara, Department of Astronomy, Kyoto University, Japan

Yuwei Huang, Astronomical Observatory, Kyoto University, China

Nobuhiko Nishimura, Institute for Space Earth Environmental Research, Nagoya University, Japan

Seiji Yashiro, The Catholic University of America, United States

Nariaki Nitta, Lockheed Martin Advanced Technology Center, United States

Kiyoshi Ichimoto, Astronomical Observatory, Kyoto University, Japan

Ayumi Asai, Astronomical Observatory, Kyoto University, Japan

High-precision & fast polarization measurements by SUNRISE-3/SCIP

Masahito Kubo, National Astronomical Observatory of Japan, Japan

Yukio Katsukawa, National Astronomical Observatory of Japan, Japan

Toshifumi Shimizu, ISAS/JAXA, Japan

Takayoshi Oba, ISAS/JAXA, Japan

Carlos Quintero Noda, University of Oslo, Norway

Yusuke Kawabata, University of Tokyo, Japan

Kiyoshi Ichimoto, Kyoto University, Japan

Shin’ichi Nagata, Kyoto University, Japan

Jose Carlos del Toro Iniesta, IAA-CSIC, Spain

David Orozco suárez, IAA-CSIC, Spain

Juan Pedro Cobos Carrascosa, IAA-CSIC, Spain

Antonio C. López Jiménez, IAA-CSIC, Spain

María Balaguer Jimenez, IAA-CSIC, Spain

Spatial Spectra of Magnetic Fields and Current Helicity by Using Hinode/SOT-SP Mosaic Magnetograms

Takashi Sakurai, National Astronomical Observatory of Japan, Japan

Kenichi Otsuji, Kwasan and Hida Observatories, Kyoto University, Japan

Kirill Kuzanyan, IZMIRAN, Russian Academy of Sciences, Russia

Zebra-like spectral patterns in electron cyclotron emission of nonequilibrium mirror-confined laboratory plasma

Mikhail Viktorov, Institute of Applied Physics of Russian Academy of Sciences, Russia

Nikita Semin, Institute of Applied Physics of Russian Academy of Sciences, Russia

Alexander Shalashov, Institute of Applied Physics of Russian Academy of Sciences, Russia

Dmitry Mansfeld, Institute of Applied Physics of Russian Academy of Sciences, Russia

Egor Gospodchikov, Institute of Applied Physics of Russian Academy of Sciences, Russia

Sergey Golubev, Institute of Applied Physics of Russian Academy of Sciences, Russia

Solar cycle variation of coronal temperatures and emission measures (1991-2001) observed with Yohkoh Soft X-ray Telescope

Aki Takeda, Montana State University, Dept. of Physics, United States

Loren Acton, Montana State University, Dept. of Physics, United States

First Step for Data Analysis of HINOTORI Soft X-ray Spectrometer (SOX) through IDL Routines

Tetsuya Watanabe, NAOJ/NINS, Japan

Hideaki Tonooka, ISAS/JAXA, Japan

Ken Ebisawa, ISAS/JAXA, Japan

Yoshinori Suematsu, NAOJ/NINS, Japan

General Formation Properties of the O I 1027 and 1028 Å lines near the Lyman β for the Diagnostics with Solar-C_EUVST

Takahiro Hasegawa, The university of Tokyo, ISAS/JAXA, Japan

Carlos Quintero Noda, University of Oslo, Norway

Toshifumi Shimizu, ISAS/JAXA, Japan

Chromospheric magnetic field: A comparison of He I 10830 Å observations with nonlinear force-free field extrapolation

Yusuke Kawabata, The University of Tokyo, Japan

Andrés Asensio Ramos, Instituto de Astrofísica de Canarias, Spain

Satoshi Inoue, Nagoya University, Japan

Toshifumi Shimizu, Institute of Space and Astronautical Science, Japan

Polarization calibration of the Solar Magnetic Activity Research Telescope(SMART)

Daiki Yamasaki, Department of Astronomy, Kyoto University, Japan

Shin'ichi Nagata, Astronomical Observatory, Graduate School of Science, Kyoto University, Japan

Kiyoshi Ichimoto, Astronomical Observatory, Graduate School of Science, Kyoto University, Japan

Polarization Calibration of the Chromospheric LAyer Spectro-Polarimeter (CLASP2)

Donguk Song, National Astronomical Observatory of Japan, Japan

Ryohko Ishikawa, National Astronomical Observatory of Japan, Japan

Ryouhei Kano, National Astronomical Observatory of Japan, Japan

Hirohisa Hara, National Astronomical Observatory of Japan, Japan

Kazuya Shinoda, National Astronomical Observatory of Japan, Japan

Masaki Yoshida, SOKENDAI/National Astronomical Observatory of Japan, Japan

David E. McKenzie, NASA Marshall Space Flight Center, United States

Javier Trujillo Bueno, Instituto de Astrofisica de Canarias, Spain

Frederic Auchere, Institut d'Astrophysique Spatiale, France

Laurel Rachmeler, NASA Marshall Space Flight Center, United States

Takenori Okamoto, National Astronomical Observatory of Japan, Japan

Ken Kobayashi, NASA Marshall Space Flight Center, United States

Toshihiro Tsuzuki, National Astronomical Observatory of Japan, Japan

Fumihiro Uraguchi, National Astronomical Observatory of Japan, Japan

Drift and Deformation of a Flux Rope Footpoint Observed during an Eruptive Flare

Alena Zemanova, Astronomical Institute of the CAS, Czech Republic

Jaroslav Dudik, Astronomical Institute of the CAS, Czech Republic

Guillaume Aulanier, LESIA, Observatoire de Paris, Psl Research University, CNRS, Sorbonne Universites, France

Julia Thalmann, University of Graz, IGAM/Institute of Physics, Austria

Peter Gomory, Astronomical Institute, Slovak Academy of Sciences, Slovakia

SoAP - Solar ALMA Pipeline

Mikolaj Szydlarski, Institute of Theoretical Astrophysics - UiO, Norway

Unified View of Solar and Stellar Flares : Can Superflares Occur on Our Sun ?

Kazunari Shibata, Kyoto University, Japan

Fast filament eruption on 2017 April 23 detected by the Solar Dynamics Doppler Imager (SDDI)

Denis P. Cabezas, Kyoto University, Japan

Kiyoshi Ichimoto, Kyoto University, Japan

Ayumi Asai, Kyoto University, Japan

Kenichi Otsuji, Kyoto University, Japan

Takako T. Ishii, Kyoto University, Japan

Satoru UeNo, Kyoto University, Japan

Daikichi Seki, Kyoto University, Japan

Kazunari Shibata, Kyoto University, Japan

Estimation of solar ultraviolet irradiance by examining spectroheliogram of Ca II K line

Hiroki Tanaka, Kyoto University, Japan

Lyman-Alpha Imaging Polarimetry with the CLASP2 Sounding Rocket Mission

Ryouhei Kano, National Astronomical Observatory of Japan, Japan

Ryohko Ishikawa, National Astronomical Observatory of Japan, Japan

David E. McKenzie, NASA Marshall Space Flight Center, United States

Javier Trujillo Bueno, Instituto Astrofisica de Canarias, Spain

Donguk Song, National Astronomical Observatory of Japan, Japan

Masaki Yoshida, The Graduate University for Advanced Studies (Sokendai), Japan

Joten Okamoto, National Astronomical Observatory of Japan, Japan

Laurel Rachmeler, NASA Marshall Space Flight Center, United States

Ken Kobayashi, NASA Marshall Space Flight Center, United States

Frederic Auchere, Institut d'Astrophysique Spatiale, France

Electron Density Measurement at the Loop-Top Region of the 2017 September 10 Solar Limb Flare

Nozomi Ono, National Astronomical Observatory of Japan / Department of Astronomy, Graduate School of Science, The University of Tokyo, Japan

Hirohisa Hara, National Astronomical Observatory of Japan, Japan

Visualizing the Hinode's results over the past 13 years

Kuniko Hori, National Astronomical Observatory of Japan, Japan

Masumi Shimojo, National Astronomical Observatory of Japan, Japan

Hirohisa Hara, National Astronomical Observatory of Japan, Japan

On the observation of a classical loop-prominence system during the 2017 September 10 flare

Juan Carlos Martinez Oliveros, University of California Berkeley, United States

Sam Krucker, University of California Berkeley, United States

Juan Camilo Guevara Gomez, Rosseland Centre for Solar Physics, Norway

The lateral motion of quasi circular flare ribbon to the quasi separatrix line

Shin'ichi Nagata, Kyoto University, Japan

Satoshi Inoue, Nagoya University, Japan

Daiki Yamasaki, Kyoto University, Japan

Observations of three-dimensional magnetic reconnection in an eruption of a quiescent filament

Juraj Lorincik, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic

Jaroslav Dudik, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic

Guillaume Aulanier, LESIA, Observatoire de Paris, Meudon, France

Alena Zemanova, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic

Elena Dzifcakova, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic

Particle Acceleration in Quasi-Perpendicular Hall-Mediated Collisionless Shocks

Douglass Endrizzi, University of Wisconsin Madison, United States

Construction of Solar Flare EUV Emission Spectral Prediction Model

Shohei Nishimoto, National Defense Academy, Japan

Kyoko Watanabe, National Defense Academy, Japan

Shinsuke Imada, Nagoya University, Japan

Toshiki Kawai, Nagoya University, Japan

Tomoko Kawate, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan

Kyoung-Sun Lee, The University Of Alabama In Huntsville, United States

1933 May 1 Goemagnetic Storm as an Example of Space weather Event with No Sunspot

Harufumi TAMAZAWA, Kyoto City University of Arts, Japan

Hioaki ISOBE, Kyoto City University of Arts, Japan

Reizaburo KITAI, Bukkyo University

Takahiro SAKAUE, Kyoto University

Satoru UENO, Kyoto University

Flare Energy Release at the Magnetic Field Polarity Inversion Line During the M1.2 Solar Flare of 2015 March 15. I. Onset of Plasma Heating and Electron Acceleration

Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Zimovets, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Myshyakov, Institute of Solar-Terrestrial Physics (ISTP) of the Russian Academy of Sciences, Siberian Branch, Russia

Natalia Meshalkina, Institute of Solar-Terrestrial Physics (ISTP) of the Russian Academy of Sciences, Siberian Branch, Russia

Flare Energy Release at the Magnetic Field Polarity Inversion Line During M1.2 Solar Flare of 2015 March 15. II. Investigation of Photospheric Electric Current and Magnetic Field Variations Using HMI 135-second Vector Magnetograms

Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Zimovets, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Myshyakov, Institute of Solar-Terrestrial Physics (ISTP) of the Russian Academy of Sciences, Siberian Branch, Russia

Relationships between photospheric vertical electric currents and hard X-ray footpoints in solar flares: statistical study for the 24th solar cycle

Ivan Zimovets, Space Research Institute of RAS, Russia

Ivan Sharykin, Space Research Institute of RAS, Russia

Weiqun Gan, Purple Mountain Observatory of CAS, China

A Statistical Study of Seismically Active Solar Flares During 24th Solar Cycle

Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia

Alexander Kosovichev, New Jersey Institute of Technology, United States

Space Weather Utilities of Solar Flare Statistics based on Solar Cycle 23: Sunspot, Flare, and Coronal Mass Ejection

Akito Kawamura, Astronomical observatory, Kyoto University, Japan

Modelling of chromospheric lines as observed during a C-class solar flare

Jana Kasparova, Astronomical Institute of the Czech Academy of Sciences, Czech Republic

Akiko Tei

Petr Heinzel

Michal Varady

Investigation of Free Magnetic Energy and Magnetic Helicity During M1.2 Solar Flare of 15 March 2015 Using HMI 135-second Vector Magnetograms

Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Zimovets, Space Research Institute of Russian Academy of Sciences, Russia

Sergei Anfinogentov, Institute of Solar-Terrestrial Physics (ISTP) of the Russian Academy of Sciences, Siberian Branch, Russia

Ivan Myshyakov, Institute of Solar-Terrestrial Physics (ISTP) of the Russian Academy of Sciences, Siberian Branch, Russia

Fast Restructuring of The Magnetic Field in the Polarity Inversion Line During M9.3 Solar Flare of 2011 July 30

Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia

Ivan Zimovets, Space Research Institute of Russian Academy of Sciences, Russia

Energy Release During Several M and X Class Flares

JIANXIA CHENG, Shanghai Astronomical Observatory, CAS, China

JIONG QIU, Montana State University, United States

Combining LOFAR radio observations and simulations to understand solar electron beam speeds and spatial expansion

Hamish Reid, University College London, United Kingdom

Eduard Kontar, University of Glasgow, United Kingdom

Thermal Structure of Supra-Arcade Plasma in Solar Flares

Mark Weber, Harvard-Smithsonian Center for Astrophysics, United States

Katharine Reeves

David McKenzie

Sabrina Savage

FOXSI-2 Solar Microflares: Hard X-ray Spectroscopy and Multi-instrument Differential Emission Measure Analysis

Juliana Vievering, University of Minnesota, United States

P. S. Athiray

Lindsay Glesener

Juan Camilo Buitrago-Casas

Shin-nosuke Ishikawa

Noriyuki Narukage

Daniel Ryan

Sophie Musset

Andrew Inglis

Steven Christe

Säm Krucker

Solar X-ray Intensity vs. Magnetic Flux for Solar Cycle 24

Patricia Jibben, Harvard-Smithsonain Center for Astrophysics, United States

Kathy Reeves, Harvard-Smithsonian Center for Astrophysics, United States

Measuring relative abundances with SPICE, the EUV spectrometer on board Solar Orbiter

Natalia Zambrana Prado, Institut d'Astrophysique Spatiale, France

Eric Buchlin, Institut d'Astrophysique Spatiale, France

Hardi Peter, Max Planck Institute for Solar System Research, Germany

Hybrid modelling of chromospheric HXR flare sources in the flare loops

Michal Varady, Faculty of Sciences, University of J. E. Purkyne, Czech Republic

Zdenek Moravec , Faculty of Sciences, University of J. E. Purkyne, Czech Republic

Jana Kasparova, Astronomical Institute of Czech Academy of Sciences, v.v.i., Czech Republic

Understanding the Evolution of He II Emission in Solar Flares

Jeffrey Reep, NRL, United States

Harry Warren, NRL

George Doschek, NRL

Nicholas Crump, NRL

Graham Kerr, NASA GSFC

EUV mutlilayer coatings for Solar-C

Jennifer Rebellato, Laboratoire Charles Fabry, IOGS, CNRS & CNES, France

Evgueni Meltchakov, Laboratoire Charles Fabry, IOGS, CNRS, France

Sébastien de Rossi, Laboratoire Charles Fabry, IOGS, CNRS, France

Xueyan Zhang, Institut d'Astrophysique Spatiale, CNRS, France

Frédéric Auchère, Institut d'Astrophysique Spatiale, CNRS, France

Franck Delmotte, Laboratoire Charles Fabry, IOGS, CNRS, France

The First Comparative Study of Data-driven Solar Coronal Field Models

Shin Toriumi, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan

Shinsuke Takasao, National Astronomical Observatory of Japan, Japan

Mark Cheung, Lockheed Martin Solar and Astrophysics Laboratory, United States

Chaowei Jiang, Institute of Space Science and Applied Technology, Harbin Institute of Technology, China

Yang Guo, Nanjing University, China

Keiji Hayashi, NorthWest Research Associates, United States

Satoshi Inoue, Nagoya University, ISEE, Japan

How solar eruptions generate X-rays and energetic particles

Paul Bellan, California Institute of Technology, United States

Byonghoon Seo, California Institute of Technology, United States

Ryan Marshall, California Institute of Technology, United States

Pakorn Wongwaitayakornku, California Institute of Technology, United States

Magnus Haw, California Institute of Technology, United States

Quantities Analysis of Magnetofrictional and MHD Simulations

Antonia Savcheva, Harvard-Smithsonian Center for Astrophysics, United States

S. Tassev

S. Inoue

W. Shelley

S. Farid