Hinode-13/IPELS 2019
 OpenConf Peer Review & Conference Management System

Monday, 2 September 2019
9:30-17:00
(Gallery 1)
17:00-19:00
(Event Space)
Tuesday, 3 September 2019
9:15-10:00
(Event Space)
10:00-10:20
(Ito Hall)
(Ito Hall) Session Chair: Takashi Sakurai, National Astronomical Observatory of Japan
10:20-10:50
Constraining coronal heating with multiwavelength measurements Lindsay Glesener, University of Minnesota, United States
10:50-11:20
Waves and turbulence in the solar wind Dipankar Banerjee, Indian Institute of Astrophysics, India
11:20-11:50
Laboratory Experiments on Plasma Waves Relevant to Solar and Space Plasmas Walter Gekelman, University of California, Los Angeles, United States
11:50-12:20
Parker Solar Probe: First Results After Three Solar Encounters and Outlook Nour E. Raouafi, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, United States
12:20-12:40
First results from the FIELDS instrument suite on Parker Solar Probe Stuart Bale, University of California, Berkeley, United States
12:40-13:00
Three-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence Munehito Shoda, National Astronomical Observatory of Japan, Japan
13:00-14:00
Ito Hall Auditorium
Session Chair: Jorrit Leenaarts, Stockholm University Session Chair: Walter Gekelman, University of California, Los Angeles
14:00-14:30
EUV spectroscopy of active regions from view point of coronal heating mechanisms Paola Testa, Harvard-Smithsonian Center for Astrophysics, United States Radiation Belt Wave Observations on the Van Allen Probes and Opportunities for Lab Experiments Craig Kletzing, The University of Iowa, United States
14:00-14:20
14:30-14:45
The drivers of active region outflows into the slow solar wind David Brooks, George Masin University at JAXA, Japan Overview of the Basic Plasma Science Facility: the physics of waves relevant to space plasmas Troy Carter, UCLA, United States
14:20-14:40
14:45-15:00
IRIS Mg II Observations and Non-LTE Modeling of Off-limb Spicules in a Solar Polar Coronal Hole Akiko TEI, Kyoto University, Japan Turbulence and structure formation by magnetic reconnection Joerg Buechner, Max Planck Institute for Solar System Research, Germany
14:40-15:00
15:00-15:15
Wave heating of the lower solar atmosphere Shahin Jafarzadeh, Rosseland Centre for Solar Physics, University of Oslo, Norway Alfven wave experiments in the Large Plasma Device-Upgrade at UCLA Mark Koepke, West Virginia University, United States
15:00-15:20
15:15-15:30
Shock heating energy in an umbra of a sunspot with integral field unit spectroscopy Tetsu Anan, National Solar Observatory, United States Inhomogeneous energy density driven instability as the most appropriate theory for the interpretation of broadband turbulence in the high-latitude region Alexander Chernyshov, Space Research Institute of the Russian Academy of Sciences, Russia
15:20-15:35
15:30-16:00
Magnetic Reconnection in the partially ionized low solar atmosphere Lei Ni, Yunnan observatories, Chinese Academy of Sciences, China Generation and role of turbulence in Kelvin-Helmholtz vortices at Earth’s magnetopause Hiroshi Hasegawa, Institute of Space and Astronautical Science, JAXA, Japan
15:35-15:50
Laboratory Excitation of the Kelvin-Helmholtz Instability in an Ionospheric-Like Plasma Yu Liu, University of Science and Technology of China, China
15:50-16:05
16:00-18:00
(Event Space) A02: Using tracer particles to study the density variations of fibrils Malcolm Druett, Stockholm University, Sweden A03: Observations of fine structures and fast dynamics in sunspot light bridges HUI TIAN, Peking University, China A04: UV bursts: magnetic reconnection in the lower solar atmosphere Yajie Chen, Peking University, China A05: Hinode and SDO Observations of a Two-Sided-Loop Coronal Jet: Toward a General Picture for Jets. Alphonse Sterling, NASA/MSFC, United States A06: Photospheric Magnetic Flux Cancellation and Associated Plasma Heating in the Upper Solar Atmosphere Sung-Hong Park, ISEE, Nagoya University, Japan A07: Simulating nanoflares in the solar atmosphere: Analysis of synthetic observables Helle Bakke, Rosseland Centre for Solar Physics, Norway A08: Convective stability in the solar photosphere Jan Jurčák, Astronomical Institute of the Czech Academy of Sciences, Czech Republic A09: Experimental turbulent transport study with gradients and mean-flow Taishi Ito, Graduate School of Science, Nagoya University, Japan A10: Wave modes excited by photospheric p-modes & mode conversion in footpoints of coronal loops Julia M. Riedl, KU Leuven, Belgium A11: Small scale generation by Uniturbulence in structured plasmas Tom Van Doorsselaere, KU Leuven, Belgium A12: Resonance Cavities - Wave amplification mechanisms in sunspot umbrae David Jess, Queen's University Belfast, United Kingdom A13: Taylor Scale and Magnetic Reynolds Number Estimation via Two-Point Spatial Correlations Carlos Cartagena-Sanchez, Bryn Mawr College, United States A14: Nano-Flare Analysis using Machine Learning Techniques Toshiki Kawai, ISEE, Nagoya University, Japan A16: On the Influence of Hinode/SOT NFI instrumental effects on the visibility of simulated prominence fine structures in H-alpha Stanislav Gunar, Astronomical Institute of the Czech Academy of Sciences, Czech Republic A17: A 2D two-fluid MHD code to model partially ionised plasma: calibration and benchmarking Linh Le Phuong, Northumbria University, United Kingdom A18: SoLaBo-X: a cross-disciplinary research activity for heating, transport, and turbulence dynamics in solar/astrophysical and laboratory plasmas Motoki Nakata, National Institute for Fusion Science, Japan A19: Alfvén shocks: Polarimetric detections in the umbral chromosphere Scott Houston, Queen's University, United Kingdom A20: How can subsurface magnetic reconnection change the elemental composition in the solar corona? Lidia van Driel-Gesztelyi, UCL/MSSL, United Kingdom A21: Evolution of anomalous coronal elemental composition in AR 12673 Lidia van Driel-Gesztelyi, UCL/MSSL, United Kingdom A22: Time domain structures in magnetic flux rope experiments Shawn Wenjie Tang, University of California, Los Angeles, United States A24: Evolution and Plasma Diagnostics of the X-region connecting a set of Trans-Equatorial Loops AVYARTHANA GHOSH, IUCAA/ Division of Astronomical Observatory, Kyoto University, India A25: Dynamics of the convective turbulence in the solar granulation studied by the spectral line broadening and asymmetry Ryohtaroh Ishikawa, SOKENDAI / National Astronomical Observatory of Japan, Japan A26: Shock wave propagation with high cadence solar ALMA time series Henrik Eklund, Rosseland Centre for Solar physics, Institute of Theoretical Astrophysics, University of Oslo, Norway A27: Study on chromospheric heating by fast and slow MHD waves using realistic simulation Yikang Wang, The University of Tokyo, Japan A28: Investigating Hidden Energy in the Solar Corona Using Forward Modeling of Magnetohydrodynamic Waves Vaibhav Pant, KU Leuven, Belgium A29: Predictions of DKIST/DL-NIRSP observations for an off-limb kink-unstable coronal loop Ben Snow, University of Exeter, United Kingdom A30: Updated version of KAPPA package for the calculation of optically thin spectra for the non-Maxwellian kappa-distributions Elena Dzifcakova, Astronomical Institute of the Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic A31: Shock sub-structure in partially-ionised plasma. Ben Snow, University of Exeter, United Kingdom A32: Dynamics of solar isolated features observed by the Atacama Large Millimeter/submillimeter Array (ALMA) Juan Camilo Guevara Gomez, Rosseland Centre for Solar Physics, Norway A33: Coupled MHD-PIC framework for magnetic reconnection Frederik Clemmensen, Rosseland Centre for Solar Physics, Norway A35: Transient dynamics and energy transfer from the photosphere to the low corona: initial results from a coordinated ALMA, DST, Hinode, IRIS, and SDO observation campaign Lucas Tarr, NSO, United States A36: Transition Region Response of Moving Magnetic Features: Hinode and IRIS observations Sanjiv Tiwari, Lockheed Martin Solar & Astrophysics Laboratory, United States A37: Investigating the Magnetic Field in Sun’s Polar Regions in the Context of Understanding and Predicting the Solar Wind at 1 AU Nariaki Nitta, Lockheed Martin Advanced Technology Center, United States A38: How does the solar surface convection form the asymmetry in spectral profiles？ Takayoshi Oba, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan A39: First Detection of Lyman-Alpha Scattering Polarization in Off-Limb Spicules and Its Constraint on Their Magnetic Field Masaki Yoshida, SOKENDAI (The Graduate University for Advanced Studies), Japan A40: Observations of Photospheric Magnetic Structure below a Dark Filament using the Hinode Spectro-Polarimeter Takaaki Yokoyama, The University of Tokyo, Japan A41: Cold and hot spicules observed with ALMA, IRIS and AIA/SDO Masumi Shimojo, National Astronomical Observatory of Japan, Japan A42: Spicule widths from high-resolution Ca II K observations Tiago Pereira, Institute of Theoretical Astrophysics, University of Oslo, Norway A43: Temperature analysis of solar prominences by multi-wavelength observations Kiyoshi Ichimoto, Kyoto University, Japan A44: What is inside a prominence bubble? Arun Kumar Awasthi, University of Science and Technology of China, China A45: 3D radiative MHD simulations of coronal rain formation and evolution Petra Kohutova, University of Oslo, Norway A46: Numerical Simulations of Anemone Jets in the Solar Photosphere Yuji Kotani, Kyoto University, Japan A47: Where is the strongest field located in sunspots ? - A statistical analysis using Hinode/Spectro-Polarimeter - Joten Okamoto, NAOJ, Japan A48: 3DMHD simulation of nanoflare-like events in wave heated coronal loop Takuma Matsumoto, NAOJ, Japan A49: Diagnostics of non-Maxwellian distributions in the solar corona Juraj Lorincik, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic A50: Ellerman bombs and UV bursts; temporal and spatial correspondence Viggo Hansteen, Bay Area Environmental Research Institute/LMSAL and RoCS/University of Oslo, United States A51: Diagnostics of the non-Maxwellian-distributions from Fe XVII–XVIII X-ray coronal spectra: proposal for the Marshall Grazing-Incidence X-ray Spectrometer (MaGIXS) Elena Dzifcakova, Astronomical Institute, Academy of Sciences of the Czech Republic, 25165 Ondrejov, Czech Republic, Czech Republic A52: Properties of spicules inferred from IRIS observations via approximate Bayesian computation Jiri Stepan, Astronomical Institute ASCR, Czech Republic A53: Doppler velocity differences between ions and neutrals in a solar surge Yuwei Huang, Kyoto University, Japan A54: Strong Viscous Damping of Coronal Alfven Waves Alexander Russell, University of Dundee, United Kingdom A55: In-flight Calibration of the Hinode X-Ray Telescope: Correction for the Scattered Lights Junho Shin, School of Space Research, Kyung Hee University, South Korea A56: On the Evolution of Point-like Convective Collapse Events Seen in High-Resolution Photospheric and Chromospheric Filtergrams of Hinode/SOT Yoshinori Suematsu, National Astronomical Observatory of Japan, Japan A57: Delta-spot Properties Observed with HMI from 2011-2018 Aimee Norton, Stanford University, United States A58: A magentised plasma experiment for laboratory simulation of space plasma effects Kevin Ronald, University of Strathclyde, United Kingdom A59: Plasmoid and blob structure of current sheet in TS-6 torus plasma merging experiment Moe Akimitsu, The University of Tokyo, Japan A60: Mapping the acoustic cut-off frequency in the solar atmosphere Bernhard Fleck, ESA
Wednesday, 4 September 2019
(Ito Hall) Session Chair: Yasushi Ono, University of Tokyo
9:30-10:00
Magnetic reconnection and particle acceleration in space and the laboratory James Drake, University of Maryland, United States
10:00-10:30
Spectroscopic Observations of Current Sheet Formation and Evolution Harry Warren, NRL, United States
10:30-11:00
Ion and electron heating characteristics of magnetic reconnection in high field flux tube merging experiments Hiroshi Tanabe, Graduate school of frontier sciences, university of Tokyo, Japan
11:00-11:30
(Event Space)
Ito Hall Auditorium
Session Chair: Marc DeRosa, LMSAL Session Chair: James Drake, University of Maryland
11:30-11:45
Detection of Strong Photospheric Downflows Accompanying Magnetic Cancellation in Collisional Polarity Inversion Lines of Flare- and CME-Productive Active Regions Georgios Chintzoglou, Lockheed Martin Solar and Astrophysics Lab, United States Fast reconnection in partially ionized plasmas Jonathan Jara-Almonte, Princeton Plasma Physics Laboratory, United States
11:30-11:50
11:45-12:00
Thermal Evolution of Plasmoids in Current Sheet of a Solar Flare Noriyoshi Ishizuka, The University of Tokyo / National Astronomical Observatory of Japan, Japan Roles of Particle Dynamics in Merging Processes of Two Spherical-Tokamak-Type Plasmoids Ritoku Horiuchi, National Institute for Fusion Science, Japan
11:50-12:10
12:00-12:15
Coronal and chromospheric observations of pre- and post-flare plasma evolution David Long, UCL/MSSL, United Kingdom Kinetic Theory of Driven Magnetic Reconnection C. Z. Cheng, University of Tokyo / Princeton Plasma Physics Laboratory, Japan
12:10-12:25
12:15-12:30
Observations and Modelling of White Light Solar Flares Graham Kerr, NASA/GSFC, United States Thermal Structures and Plasma Motions in Current Sheet of Eruptive Solar Flares Hirohisa Hara, National Astronomical Observatory of Japan, Japan
12:25-12:40
12:30-12:45
Ted Tarbell san and Hinode mission Yoshinori Suematsu, National Astronomical Observatory of Japan, Japan Guide-field induced halting of magnetic reconnection in laboratory experiments Julien Fuchs, CNRS, LULI, France
12:40-12:55
12:45-13:00
Comments from Ted's friend Alan Title, LMSAL, United States
13:00-14:00
Ito Hall Auditorium
Session Chair: Luis Bellot Rubio, IAA-CSIC Session Chair: Paul Bellan, California Institute of Technology
14:00-14:30
Prevalent Small-scale Jets in the Solar Atmosphere HUI TIAN, Peking University, China The dynamics of supersonic plasma flows interaction with the magnetic arch in a laboratory setup Mikhail Viktorov, Institute of Applied Physics of Russian Academy of Sciences, Russia
14:00-14:20
14:30-15:00
Realistic simulations of solar active regions: From emergence to eruption Feng Chen, University of Colorado, United States Importance of axi-symmetry of the 1/1 kink mode (2-D or 3-D) in determination of the reconnection time scales in the sawtooth instability Hyeon K. Park, UNIST, South Korea
14:20-14:40
15:00-15:15
Unipolar versus bipolar internetwork flux appearance Milan Gosic, LMSAL/BAERI, United States An MHD Modeling of the initiation and Dynamics of the X9.3 Flare Observed in September 2017 Satoshi Inoue, Institute for Space-Earth Environmental Research, Nagoya University, Japan
14:40-14:55
15:15-15:30
Small-scale magnetic flux sheet emergence observed with Hinode Catherine Fischer, Leibniz-Institute of Solar Physics (KIS), Germany Intermittent evolution of heliospheric magnetized structures: from Solar Braids to Magnetic Knots Ilan Roth, University of California, Berkeley, CA, United States
14:55-15:10
15:30-15:45
Observing 8 kG magnetic fields in a bipolar light bridge using Hinode/SP Sebastian Castellanos Duran, Max-Planck-Institut für Sonnensystemforschung, Germany Non-local generation of plasma in a magnetic nozzle. Alex Bennet, Australian National University, Australia
15:10-15:25
Three-dimensional MHD turbulence reconnection by coupling among multiple tearing layers Takaaki Yokoyama, The University of Tokyo, Japan
15:25-15:40
15:45-16:15
(Event Space)
(Ito Hall) Session Chair: Kazunari Shibata, Kyoto University
16:15-16:45
Magnetic Reconnection in the Earth’s Magnetosphere Robert Ergun, University of Colorado, United States
16:45-17:05
Collisionless reconnection in the Terrestrial Reconnection Experiment (TREX) Jan Egedal, UW-Madison, United States
17:05-17:25
Revisiting thermodynamics properties of electrons in nearly collisionless expanding plasmas Christine Charles, The Australian National University, Australia
17:25-17:45
Numerical study of accretion discs Ryoji Matsumoto, Chiba University, Japan
18:00-18:30
19:00-21:00
(Hotel Chinzanso Tokyo)
Thursday, 5 September 2019
(Ito Hall) Session Chair: Edward DeLuca, Center for Astrophysics - Harvard & Smithsonian
9:30-10:00
Solar dynamo: achievements and perspective Hideyuki Hotta, Chiba university, Japan
10:00-10:30
A Laboratory Model for the Parker Spiral and Solar Wind Cary Forest, University of Wisconsin, Madison, United States
10:30-10:50
Solar Soft X-ray Variations from the 2008 - 2019 Solar Cycle inferred from CORONAS/SphinX, GOES/XRS, Hinode/XRT, MinXSS, NuSTAR, and RHESSI Instruments Christopher Moore, Harvard-Smithsonian Center for Astrophysics, United States
10:50-11:20
(Event Space)
(Ito Hall) Session Chair: Takaaki Yokoyama, University of Tokyo
11:20-11:40
Reconnection Microjets in Solar Coronal Loops Patrick Antolin, University of St Andrews, United Kingdom
11:40-12:00
Evolution of Transient Inverse FIP Composition in a Solar Flare Deborah Baker, MSSL/UCL, United Kingdom
12:00-12:30
Space weather and high-energy phenomena Miho Janvier, Institut d'Astrophysique Spatiale, France
12:30-13:00
Predictability of Solar Flares Based on Satellite Observations and Magnetohydrodynamic Instability Models Kanya Kusano, ISEE, Nagoya University, Japan
13:00-14:00
Ito Hall Auditorium
Session Chair: Masahito Kubo, National Astronomical Observatory of Japan Session Chair: Ritoku Horiuchi, National Institute for Fusion Science
14:00-14:30
Asteroseismology of Sun-like stars and the connexion to the Sun Othman Benomar, NAOJ, Mitaka, Japan Cross-discipline study of the two-fluid dynamics and energetics of the magnetic reconnection in laboratory and space plasmas Masaaki Yamada, PPPL, Princeton University, United States
14:00-14:15
14:30-14:45
Hinode Observation of Sun’s Polar Regions over a solar cycle Daikou Shiota , National Institute of Information and Communications Technology (NICT), Japan Plasma acceleration during magnetic reconnection in the terrestrial magnetosphere, laboratory, and at the Sun Li-Jen Chen, NASA Goddard Space Flight Center, United States
14:15-14:35
14:45-15:15
Magnetic Field of Solar Eruptive and Non-Eruptive Events Xudong Sun, University of Hawaii, United States Formation of anomalous velocity distribution based on the pickup-like ion motions during magnetic reconnection Shunsuke Usami, National Institute for Fusion Science, Japan
14:35-14:55
15:15-15:30
Broad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3 class Flare Observed by Hinode/EIS Vanessa Polito, BAERI/LMSAL, United States First Results form TS-6 and ST-40 Tokamak Merging Experiments, -Global and Local Energy Conversion of Magnetic Reconnection in Laboratory Plasmas Yasushi Ono, University of Tokyo, Japan
14:55-15:10
15:30-15:45
SMALL-SCALE JETS OBSERVED AT SITES OF FLUX CANCELATION Navdeep Panesar, LMSAL/BAERI, United States Kinetic simulations of the dynamic magnetotail Samuel Totorica, Princeton University, United States
15:10-15:25
15:45-16:00
A systematic study of non-thermal emissions to search for characteristics of white-light flares and comparison with magnetic features Kyoko Watanabe, National Defense Academy of Japan, Japan Studying Magnetospheric Collisionless Beam Instabilities and ULF Waves in the Laboratory Peter Heuer, University of California, Los Angeles, United States
15:25-15:40
Magnetic moment of thermal plasma: Revisiting the Bohr-van Leeuwen theorem Kiyoto Shibasaki, Solar Physics Research Inc., Japan
15:40-15:55
16:00-18:00
(Event Space) B01: 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 B02: 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 B03: Relationship of EIT Waves Phenomena with Coronal Mass Ejections Virendra Verma, Uttarakhand Space Application Center, India B04: COCOPLOTs: imaging Halpha for a flare on 6th September 2017 Malcolm Druett, Stockholm University, Sweden B05: Optical Ion Velocity Diagnostics in the Interaction of a Laser Produced Plasma and an Ambient Magnetized Plasma Robert Dorst, UCLA, United States B06: Unfolding EIS Slot Data Amy Winebarger, NASA MSFC, United States B07: 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 B08: Global dipole moment study using optimized surface flux transport model Mohammed Talafha, Eötvös Loránd University, Department of Astronomy, Hungary B09: Spectroscopic study of a limb flare observed by Hinode, SDO, RHESSI, and STEREO Kyoung-Sun Lee, The University of Alabama in Huntsville, United States B12: 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 B13: Characteristics of big solar flares observed with RHESSI and Nobeyama Radioheliograph Satoshi Masuda, ISEE, Nagoya University, Japan B14: Back to the Surface: An Update on Coordinating Hinode Observations with the Parker Solar Probe Encounters Harry Warren, NRL, United States B15: Improving Space Weather Forecasting With Wide-Field EUV Observations Edward DeLuca, Center for Astrophysics - Harvard & Smithsonian, United States B16: Particle acceleration and the evolution of nonthermal line broadening in solar flares Sarah Matthews, UCL-MSSL, United Kingdom B17: DeSIRer: a new, fast and flexible non local thermodynamic equilibrium inversion code David Orozco Suarez, Instituto de Astrofísica de Andalucía (IAA-CSIC), Spain B18: Diagnostic Capability of the Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) for SUNRISE-3 Yukio Katsukawa, National Astronomical Observatory of Japan, Japan B19: Statistical analysis of solar energetic particle events Kosuke Kihara, Department of Astronomy, Kyoto University, Japan B20: High-precision & fast polarization measurements by SUNRISE-3/SCIP Masahito Kubo, National Astronomical Observatory of Japan, Japan B21: Spatial Spectra of Magnetic Fields and Current Helicity by Using Hinode/SOT-SP Mosaic Magnetograms Takashi Sakurai, National Astronomical Observatory of Japan, Japan B22: 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 B23: 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 B24: First Step for Data Analysis of HINOTORI Soft X-ray Spectrometer (SOX) through IDL Routines Tetsuya Watanabe, NAOJ/NINS, Japan B25: 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 B26: Chromospheric magnetic field: A comparison of He I 10830 Å observations with nonlinear force-free field extrapolation Yusuke Kawabata, The University of Tokyo, Japan B27: Polarization calibration of the Solar Magnetic Activity Research Telescope(SMART) Daiki Yamasaki, Department of Astronomy, Kyoto University, Japan B28: Polarization Calibration of the Chromospheric LAyer Spectro-Polarimeter (CLASP2) Ryohko Ishikawa, National Astronomical Observatory of Japan, Japan B29: Drift and Deformation of a Flux Rope Footpoint Observed during an Eruptive Flare Alena Zemanova, Astronomical Institute of the CAS, Czech Republic B30: SoAP - Solar ALMA Pipeline Mikolaj Szydlarski, Institute of Theoretical Astrophysics - UiO, Norway B31: Unified View of Solar and Stellar Flares : Can Superflares Occur on Our Sun ? Kazunari Shibata, Kyoto University, Japan B32: Fast filament eruption on 2017 April 23 detected by the Solar Dynamics Doppler Imager (SDDI) Denis P. Cabezas, Kyoto University, Japan B33: Estimation of solar ultraviolet irradiance by examining spectroheliogram of Ca II K line Hiroki Tanaka, Kyoto University, Japan B34: Lyman-Alpha Imaging Polarimetry with the CLASP2 Sounding Rocket Mission Ryouhei Kano, National Astronomical Observatory of Japan, Japan B35: 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 B36: Visualizing the Hinode's results over the past 13 years Kuniko Hori, National Astronomical Observatory of Japan, Japan B37: On the observation of a classical loop-prominence system during the 2017 September 10 flare Juan Camilo Guevara Gomez, Rosseland Centre for Solar Physics, Norway B38: The lateral motion of quasi circular flare ribbon to the quasi separatrix line Shin'ichi Nagata, Kyoto University, Japan B39: 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 B40: Particle Acceleration in Quasi-Perpendicular Hall-Mediated Collisionless Shocks Douglass Endrizzi, University of Wisconsin Madison, United States B41: Construction of Solar Flare EUV Emission Spectral Prediction Model Shohei Nishimoto, National Defense Academy, Japan B42: 1933 May 1 Goemagnetic Storm as an Example of Space weather Event with No Sunspot Harufumi TAMAZAWA, Kyoto City University of Arts, Japan B43: 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 B44: 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 B45: 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 B46: A Statistical Study of Seismically Active Solar Flares During 24th Solar Cycle Ivan Sharykin, Space Research Institute of Russian Academy of Sciences, Russia B47: 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 B48: Modelling of chromospheric lines as observed during a C-class solar flare Jana Kasparova, Astronomical Institute of the Czech Academy of Sciences, Czech Republic B49: 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 B50: 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 B51: Energy Release During Several M and X Class Flares JIANXIA CHENG, Shanghai Astronomical Observatory, CAS, China B52: Combining LOFAR radio observations and simulations to understand solar electron beam speeds and spatial expansion Hamish Reid, University College London, United Kingdom B53: Thermal Structure of Supra-Arcade Plasma in Solar Flares Mark Weber, Harvard-Smithsonian Center for Astrophysics, United States B54: FOXSI-2 Solar Microflares: Hard X-ray Spectroscopy and Multi-instrument Differential Emission Measure Analysis Juliana Vievering, University of Minnesota, United States B55: Solar X-ray Intensity vs. Magnetic Flux for Solar Cycle 24 Kathy Reeves, Harvard-Smithsonian Center for Astrophysics, United States B57: Measuring relative abundances with SPICE, the EUV spectrometer on board Solar Orbiter Natalia Zambrana Prado, Institut d'Astrophysique Spatiale, France B58: Hybrid modelling of chromospheric HXR flare sources in the flare loops Michal Varady, Faculty of Sciences, University of J. E. Purkyne, Czech Republic B59: Understanding the Evolution of He II Emission in Solar Flares Jeffrey Reep, NRL, United States B60: EUV mutlilayer coatings for Solar-C Jennifer Rebellato, Laboratoire Charles Fabry, IOGS, CNRS & CNES, France B61: The First Comparative Study of Data-driven Solar Coronal Field Models Shin Toriumi, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan B62: How solar eruptions generate X-rays and energetic particles Paul Bellan, California Institute of Technology, United States B63: Quantities Analysis of Magnetofrictional and MHD Simulations Antonia Savcheva, Harvard-Smithsonian Center for Astrophysics, United States
Friday, 6 September 2019
(Ito Hall) Session Chair: Hyeon Park, UNIST
9:30-10:00
Laboratory study of ideal MHD instabilities and magnetic reconnection relevant to solar eruptive phenomena Hantao Ji, Princeton University, United States
10:00-10:20
How solar eruptions generate X-rays and energetic particles Paul Bellan, California Institute of Technology, United States
10:20-10:40
Mapping the Magnetic Field of Flare Coronal Loops David Kuridze, Aberystwyth University, United Kingdom
10:40-11:00
Flare-productive Active Regions: Hinode’s View and Beyond Shin Toriumi, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan
11:00-11:30
(Event Space)
(Ito Hall) Session Chair: Louise Harra, UCL-MSSL
11:30-11:50
First Results of the Chromospheric LAyer Spectro-Polarimeter (CLASP2) Ryohko Ishikawa, National Astronomical Observatory of Japan, Japan
11:50-12:10
NuSTAR observations of the quietest Sun Iain Hannah, University of Glasgow, United Kingdom
12:10-12:30
The Solar-C_EUVST mission Toshifumi Shimizu, ISAS/JAXA, Japan
12:30-12:50
Synergy Science with DKIST and Solar-C_EUVST Lucas Tarr, National Solar Observatory, United States
12:50-14:00
Ito Hall Auditorium
Session Chair: Dipankar Banerjee, Indian Institute of Astrophysics Session Chair: Joerg Buechner, Max Planck Institute for Solar System Research
14:00-14:15
Science Objectives of the Solar-C_EUVST Shinsuke Imada, Nagoya University, Japan Collisionless shocks in laboratory and space plasmas. Robert Bingham, University of Strathclyde, United Kingdom
14:00-14:20
14:15-14:30
Effect of non-equilibrium ionization on the solar EUV/X-ray spectral diagnosis Haruhisa Iijima, Institute for Space-Earth Environmental Research, Nagoya University, Japan Effect of electrostatic ion two-stream instability on the laser-driven collisionless shock ion acceleration in multi-ion species plasma Youichi Sakawa, Institute of Laser Engineering, Osaka University, Japan
14:20-14:40
14:30-14:45
EUVST instrumental design and observation capability Tomoko Kawate, ISAS/JAXA, Japan Modeling of astrophysical jets under conditions of laser relativistic magnetoactive plasma Vadim Belyaev, Central Research Institute of Mashine Building, Russia
14:40-14:55
14:45-15:00
Solar Orbiter and possible synergy science with Solar-C_EUVST Sami Solanki, MPS, Germany Full particle-in-cell simulation of the interaction between two plasmas for laboratory experiments on the generation of magnetized collisionless shocks with high-power lasers Takayuki Umeda, Institute for Space-Earth Environmental Research, Nagoya University, Japan
14:55-15:10
15:00-15:15
On single point plasma diagnostics in the solar corona using the DKIST Thomas Schad, National Solar Observatory, United States Role of the Biermann effect in 3-D magnetic reconnection in laser-driven experiments and space plasmas Jackson Matteucci, Princeton University, United States
15:10-15:25
15:15-15:30
Satellite mission: PhoENiX (Physics of Energetic and Non-thermal plasmas in the X (= magnetic reconnection) region) Noriyuki Narukage, National Astronomical Observatory of Japan, Japan
15:30-16:00
(Event space)
16:00-17:30
(Ito Hall) Discussion chair: Masaaki Yamada, Princeton Plasma Physics Lab.
Closing Ceremony: Toshifumi Shimizu, ISAS/JAXA

 



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