Hinode13/IPELS2019 Program

Full Program »

Tuesday, 3 September 2019
16:00 - 18:00

Event Space

Total 56 posters.

Using tracer particles to study the density variations of fibrils: Malcolm Druett, Stockholm University, Sweden; Jorrit Leenaarts, Stockholm University, Sweden

Observations of fine structures and fast dynamics in sunspot light bridges: HUI TIAN, Peking University, China; Jingwen Zhang, Peking University, China

UV bursts: magnetic reconnection in the lower solar atmosphere: Yajie Chen, Peking University, China; Hui Tian, Peking University, China; Hardi Peter, Max-Planck Institute for Solar System Research, Germany; Tanmoy Samanta, Peking University, China; Haiming Wang, Big Bear Solar Observatory, New Jersey Institute of Technology, United States; Wenda Cao, Big Bear Solar Observatory, New Jersey Institute of Technology, United States

Hinode and SDO Observations of a Two-Sided-Loop Coronal Jet: Toward a General Picture for Jets.: Alphonse Sterling, NASA/MSFC, United States; Louise Harra, PMOD/WRC; ETH-Zurich, Switzerland; Ronald Moore, NASA/MSFC; U of Alabama Huntsville, United States; David Falconer, NASA/MSFC; U of Alabama Huntsville, United States

Photospheric Magnetic Flux Cancellation and Associated Plasma Heating in the Upper Solar Atmosphere: Sung-Hong Park, ISEE, Nagoya University, Japan; KD Leka, NorthWest Research Associates, United States

Simulating nanoflares in the solar atmosphere: Analysis of synthetic observables: Helle Bakke, Rosseland Centre for Solar Physics, Norway; Lars Frogner, Rosseland Centre for Solar Physics, Norway; Boris Vilhelm Gudiksen, Rosseland Centre for Solar Physics, Norway

Convective stability in the solar photosphere: Jan Jurčák, Astronomical Institute of the Czech Academy of Sciences, Czech Republic; Markus Schmassmann, Leibniz-Institut für Sonnenphysik; Nazaret Bello González, Leibniz-Institut für Sonnenphysik; Matthias Rempel, High Altitude Observatory, NCAR; Rolf Schlichenmaier, Leibniz-Institut für Sonnenphysik

Experimental turbulent transport study with gradients and mean-flow: Taishi Ito, Graduate School of Science, Nagoya University, Japan; Kenichi Nagaoka, National Institute for Fusion Science-NINS/Nagoya Univeristy, Japan; Motoki Nakata, National Institute for Fusion Science-NINS/SOKENDAI, Japan; Shinji Yoshimura, National Institute for Fusion Science-NINS, Japan; Kenichiro Terasaka, Kyushu Univeristy, Japan; Yoshiki Hidaka, Kyushu Univeristy, Japan

Wave modes excited by photospheric p-modes & mode conversion in footpoints of coronal loops: Julia M. Riedl, KU Leuven, Belgium; Tom Van Doorsselaere, KU Leuven, Belgium

Small scale generation by Uniturbulence in structured plasmas: Tom Van Doorsselaere, KU Leuven, Belgium; Norbert Magyar, KU Leuven, Belgium; Marcel Goossens, KU Leuven, Belgium

Resonance Cavities - Wave amplification mechanisms in sunspot umbrae: David Jess, Queen's University Belfast, United Kingdom

Taylor Scale and Magnetic Reynolds Number Estimation via Two-Point Spatial Correlations: Carlos Cartagena-Sanchez, Bryn Mawr College, United States; David Schaffner, Bryn Mawr College, United States

Nano-Flare Analysis using Machine Learning Techniques: Toshiki Kawai, ISEE, Nagoya University, Japan; Shinsuke Imada, ISEE, Nagoya University, Japan

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; Jan Jurcak, Astronomical Institute of the Czech Academy of Sciences, Czech Republic; Kiyoshi Ichimoto, Astronomical Observatory, Kyoto University, Japan

A 2D two-fluid MHD code to model partially ionised plasma: calibration and benchmarking: Linh Le Phuong, Northumbria University, United Kingdom; Sergiy Shelyag, Deakin University, Australia; Gert Botha, Northumbria University, United Kingdom; James McLaughlin, Northumbria University, United Kingdom

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; Yukio Katsukawa, National Astronomical Observatory of Japan, Japan; SoLaBo-X project

Alfvén shocks: Polarimetric detections in the umbral chromosphere: Scott Houston, Queen's University, United Kingdom

How can subsurface magnetic reconnection change the elemental composition in the solar corona?: Lidia van Driel-Gesztelyi, UCL/MSSL, United Kingdom; Pascal Démoulin, Observatoire de Paris, LESIA, France; Deborah Baker, UCL/MSSL, United Kingdom; Gherardo Valori, UCL/MSSL, United Kingdom; David Long, UCL/MSSL, United Kingdom; David Brooks, George Mason University, United States

Evolution of anomalous coronal elemental composition in AR 12673: Deborah Baker, UCL/MSSL, United Kingdom; Lidia van Driel-Gesztelyi, UCL/MSSL, United Kingdom; David Brooks, George Mason University, United States; Pascal Démoulin, Observatoire de Paris, LESIA, France; Gherardo Valori, UCL/MSSL, United Kingdom; David Long, UCL/MSSL, United Kingdom

Time domain structures in magnetic flux rope experiments: Shawn Wenjie Tang, University of California, Los Angeles, United States; Walter Gekelman, University of California, Los Angeles, United States; Patrick Pribyl, University of California, Los Angeles, United States; Stephen Vincena, University of California, Los Angeles, United States

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; Durgesh Tripathi, IUCAA, India

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; Yukio Katsukawa, National Astronomical Observatory of Japan, Japan; Takayoshi Oba, ISAS/JAXA, Japan; Motoki Nakata, National Institute for Fusion Science, Japan; Kenichi Nagaoka, National Institute for Fusion Science, Japan; Tatsuya Kobayashi, National Institute for Fusion Science, Japan

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

Study on chromospheric heating by fast and slow MHD waves using realistic simulation: Yikang Wang, The University of Tokyo, Japan; Takaaki Yokoyama, The University of Tokyo, Japan

Investigating Hidden Energy in the Solar Corona Using Forward Modeling of Magnetohydrodynamic Waves: Vaibhav Pant, KU Leuven, Belgium; Norbert Magyar, KU Leuven, Belgium; Tom Van Doorsselaere, KU Leuven, Belgium; Richard Morton, Northumbria University, United Kingdom

Predictions of DKIST/DL-NIRSP observations for an off-limb kink-unstable coronal loop: Ben Snow, University of Exeter, United Kingdom

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; Jaroslav Dudik, Astronomical Institute of the Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic; Alena Zemanova, Astronomical Institute of the Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic; Juraj Lorincik, Astronomical Institute of the Academy of Sciences of the Czech Republic, Ondrejov, Czech Republic

Shock sub-structure in partially-ionised plasma.: Ben Snow, University of Exeter, United Kingdom; Andrew Hillier, University of Exeter, United Kingdom

Dynamics of solar isolated features observed by the Atacama Large Millimeter/submillimeter Array (ALMA): Juan Camilo Guevara Gomez, Rosseland Centre for Solar Physics, Norway; Shahin Jafarzadeh, Rosseland Centre for Solar Physics, Norway; Mikolaj Szydlarski, Rosseland Centre for Solar Physics, Norway; Sven Wedemeyer, Rosseland Centre for Solar Physics, Norway

Coupled MHD-PIC framework for magnetic reconnection: Frederik Clemmensen, Rosseland Centre for Solar Physics, Norway; Andrius Popovas, Rosseland Centre for Solar Physics, Norway; Boris Gudiksen, Rosseland Centre for Solar Physics, Norway

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; Adam Kobelski, WVU, United States; Sarah Jaeggli, NSO, United States; Sabrina Savage, NASA/MSFC, United States

Transition Region Response of Moving Magnetic Features: Hinode and IRIS observations: Sanjiv Tiwari, Lockheed Martin Solar & Astrophysics Laboratory, United States; Gayathri Gupta, Lockheed Martin Solar & Astrophysics Laboratory, United States; Bart De Pontieu, Lockheed Martin Solar & Astrophysics Laboratory, United States; Navdeep Panesar, Lockheed Martin Solar & Astrophysics Laboratory, United States; Ronald Moore, NASA Marshal Space Flight Center, United States; Ted Tarbell, Lockheed Martin Solar & Astrophysics Laboratory, United States

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; Alberto Sainz Dalda, Bay Area Environmental Research Institute, United States; Rebecca Centeno, High Altitude Observatory, United States; Yang Liu, Stanford University, United States; Neal Hurlburt, Lockheed Martin Advanced Technology Center, United States; Thomas Berger, University of Colorado, United States

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; Yusuke iida, Department of Science and Technology, Kwansei Gakuin University, Japan; Toshifumi Shimizu, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan

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; Yoshinori Suematsu, National Astronomical Observatory of Japan, Japan; Ryohko Ishikawa, National Astronomical Observatory of Japan, Japan; Javier Trujillo Bueno, Instituto de Astrofisica de Canarias, Spain; Yusuke Iida, Kwansei Gakuin University, Japan; Motoshi Goto, National Institute for Fusion Science, Japan; Ryouhei Kano, National Astronomical Observatory of Japan, Japan; Noriyuki Narukage, National Astronomical Observatory of Japan, Japan; Takamasa Bando, National Astronomical Observatory of Japan, Japan; Amy Winebarger, NASA Marshall Space Flight Center, United States; Ken Kobayashi, NASA Marshall Space Flight Center, United States; Frédéric Auchère, Institut d’Astrophysique Spatiale, France

Observations of Photospheric Magnetic Structure below a Dark Filament using the Hinode Spectro-Polarimeter: Takaaki Yokoyama, The University of Tokyo, Japan; Yukio Katsukawa, NAOJ, Japan; Masumi Shimojo, NAOJ, Japan

Cold and hot spicules observed with ALMA, IRIS and AIA/SDO: Masumi Shimojo, National Astronomical Observatory of Japan, Japan; Tomoko Kawate, Japan Aerospace Exploration Agency, Japan; Takenori J. Okamoto, National Astronomical Observatory of Japan, Japan; Takaaki Yokoyama, University of Tokyo, Japan

Spicule widths from high-resolution Ca II K observations: Tiago Pereira, Institute of Theoretical Astrophysics, University of Oslo, Norway; Vasco Henriques, Institute of Theoretical Astrophysics, University of Oslo, Norway

Temperature analysis of solar prominences by multi-wavelength observations: Sanetaka Okada, Kyoto University, Japan; Kiyoshi Ichimoto, Kyoto University, Japan; Aki Machida, Kyoto University, Japan; Satomi Tokuda, Kyoto University, Japan; Yuwei Huang, Kyoto University, Japan

What is inside a prominence bubble?: Arun Kumar Awasthi, University of Science and Technology of China, China; Rui Liu, University of Science and Technology of China, China

3D radiative MHD simulations of coronal rain formation and evolution: Petra Kohutova, University of Oslo, Norway

Numerical Simulations of Anemone Jets in the Solar Photosphere: Yuji Kotani, Kyoto University, Japan; Kazunari Shibata, Kyoto University, Japan

Where is the strongest field located in sunspots ? - A statistical analysis using Hinode/Spectro-Polarimeter -: Joten Okamoto, NAOJ, Japan; Takashi Sakurai, NAOJ, Japan

3DMHD simulation of nanoflare-like events in wave heated coronal loop: Takuma Matsumoto, NAOJ, Japan

Diagnostics of non-Maxwellian distributions in the solar corona: 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; Giulio del Zanna, DATMP, CMS, University of Cambridge, Cambridge, United Kingdom; Elena Dzifcakova, Astronomical Institute of the Czech Academy of Sciences, Ondrejov, Czech Republic; Helen Mason, DATMP, CMS, University of Cambridge, Cambridge, United Kingdom

Ellerman bombs and UV bursts; temporal and spatial correspondence: Viggo Hansteen, Bay Area Environmental Research Institute/LMSAL and RoCS/University of Oslo, United States

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; Jaroslav Dudik, Astronomical Institute, Academy of Sciences of the Czech Republic, 25165 Ondrejov, Czech Republic, Czech Republic; Giulio Del Zanna, Department of Applied Mathematics and Theoretical Physics, CMS, University of Cambridge, Wilberforce Road, Cambridge CB30WA, United Kingdom, United Kingdom; Helen Mason, Department of Applied Mathematics and Theoretical Physics, CMS, University of Cambridge, Wilberforce Road, Cambridge CB30WA, United Kingdom, United Kingdom; Leon L. Golub, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 01238, USA, United States; Amy R. Winebarger, NASA Marshall Space Flight Center, Mail Code ST 13, Huntsville, AL 35812, USA, United States; Sabrina L. Savage, NASA Marshall Space Flight Center, Mail Code ST 13, Huntsville, AL 35812, USA, United Kingdom

Properties of spicules inferred from IRIS observations via approximate Bayesian computation: Jiri Stepan, Astronomical Institute ASCR, Czech Republic; Akiko Tei, Kwasan and Hida Observatories, Kyoto University, Japan; Stanislav Gunar, Astronomical Institute ASCR, Czech Republic; Petr Heinzel, Astronomical Institute ASCR, Czech Republic

Doppler velocity differences between ions and neutrals in a solar surge: Yuwei Huang, Kyoto University, Japan; Tetsu Anan, National Solar Observatory, United States; Kiyoshi Ichimoto, Kyoto University, Japan

Strong Viscous Damping of Coronal Alfven Waves: Alexander Russell, University of Dundee, United Kingdom

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; Ryouhei Kano, National Astronomical Observatory of Japan, National Institutes of Natural Science, Japan; Takashi Sakurai, National Astronomical Observatory of Japan, National Institutes of Natural Science, Japan; Yong-Jae Moon, School of Space Research, Kyung Hee University, South Korea; Yeon-Han Kim, Space Science Division, Korea Astronomy and Space Science Institute, South Korea

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

Delta-spot Properties Observed with HMI from 2011-2018: Aimee Norton, Stanford University, United States; Mark Linton, NRL; Kalman Knizhnik; Lucas Tarr

A magentised plasma experiment for laboratory simulation of space plasma effects: Kevin Ronald, University of Strathclyde, United Kingdom; Alan Phelps, University of Strathclyde, United Kingdom; Bengt Eliasson, University of Strathclyde, United Kingdom; Adrian Cross, University of Strathclyde, United Kingdom; Colin Whyte, University of Strathclyde, United Kingdom; Bob Bingham, Rutherford Appleton Laboratory, United Kingdom; Kieran Wilson, University of Strathclyde, United Kingdom; Alan Cairns, University of St Andrews, United Kingdom; Mark Koepke, West Virginia University, United States; Craig Robertson, University of Strathclyde, United Kingdom; David Speirs, University of Strathclyde, United Kingdom; Philip MacInnes, University of Strathclyde, United Kingdom; Ruth Bamford, Rutherford Appleton Laboratory, United Kingdom

Plasmoid and blob structure of current sheet in TS-6 torus plasma merging experiment: Moe Akimitsu, The University of Tokyo, Japan; Qinghong Cao, The University of Tokyo; Keisuke Miki; Hiroshi Tanabe; Yasushi Ono

Mapping the acoustic cut-off frequency in the solar atmosphere: Stuart M. Jefferies, Georgia State Univ. & Univ. of Hawaii; Bernhard Fleck, ESA; Neil Murphy, JPL; Francesco Berrilli, Univ. di Roma Tor Vergata