SH044
Solar and Heliospheric Physics: General Contributions IV Posters

Tuesday, 15 December 2020: 04:00-20:59
Poster
Primary Convener:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Conveners:  Romina Nikoukar, Johns Hopkins Applied Physics Laboratory, Laurel, MD, United States and Elizabeth MacDonald, National Aeronautics and Space Administration, Minneapolis, MN, United States
Primary Liaison:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States
Chairs:  Christina O Lee, Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA, United States and Noé Lugaz, University of New Hampshire Main Campus, Durham, NH, United States
OSPA Liaison:  Christina O Lee, Boston College, Institute for Scientific Research, Chestnut Hill, MA, United States
 
Super-resolution of Solar Magnetograms (707966)
Paul James Wright1, Xavier Gitiaux2, Anna Jungbluth3, Shane Maloney4, Carl Shneider5, Alfredo Kalaitzis6, Atılım Güneş Baydin7, Michel Deudon6, Yarin Gal8 and Andres Munoz-Jaramillo9, (1)Stanford University, W. W. Hansen Experimental Physics Laboratory, Stanford, CA, United States, (2)George Mason University, Fairfax, VA, United States, (3)University of Oxford, Oxford, United Kingdom, (4)Trinity College Dublin, Dublin, Ireland, (5)Center for Mathematics and Computer Science (CWI), Multiscale Dynamics, Amsterdam, Netherlands, (6)Element AI, London, United Kingdom, (7)University of Oxford, Department of Engineering Science, Oxford, United Kingdom, (8)University of Oxford, Department of Computer Science, Oxford, United Kingdom, (9)SouthWest Research Institute, Boulder, CO, United States
 
Generation of Solar Magnetograms, UV, and EUV images from Galileo Sunspot Drawings by Deep Learning (673952)
Harim Lee, Kyung Hee University, Yongin, Korea, Republic of (South), Eunsu Park, Department of Astronomy & Space Science, Kyung Hee University, Yongin, South Korea and Yong-Jae Moon, School of Space Research, Kyung Hee University, Yongin, South Korea
 
Denoising solar magnetograms by a novel deep learning method for image translation (679418)
Eunsu Park1, Yong-Jae Moon2, Daye Lim2 and Harim Lee1, (1)Kyung Hee University, Yongin, Korea, Republic of (South), (2)School of Space Research, Kyung Hee University, Yongin, South Korea
 
Super-resolution of SDO/HMI Magnetogram Using Novel Deep Learning Methods. (689897)
Sumiaya Rahman1, Yong-Jae Moon2, Eunsu Park3, Il-Hyun Cho4 and Daye Lim2, (1)Yongin-si, Gyeonggi-do, South Korea, (2)School of Space Research, Kyung Hee University, Yongin, South Korea, (3)Department of Astronomy & Space Science, Kyung Hee University, Yongin, South Korea, (4)Kyung Hee University, Astronomy and Space Science, Yongin-si, South Korea
 
Elliptical Surfaces For The Potential Field Source Surface Model (692613)
Martin Alexander Kruse II1, Verena Heidrich-Meisner1, Lars Berger2 and Robert F Wimmer-Schweingruber3, (1)University of Kiel, Kiel, Germany, (2)Institute for Experimental and Applied Physics (IEAP), Christian-Albrechts-University of Kiel, Kiel, Germany, (3)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
 
Mitigation of Coronal Hole Obscuration for Open Flux Estimates (704211)
Ronald M. Caplan, Cooper Downs and Jon Linker, Predictive Science Inc., San Diego, CA, United States
 
Statistical Analysis of Photospheric Vertical Current Structure in Flaring Active Regions (752138)
Maria Kazachenko, University of Colorado at Boulder, LASP, Boulder, CO, United States
 
MHD Simulation of the 13 December 2006 Eruptive Flare of AR10930 (718901)
Yuhong Fan, National Center for Atmospheric Research, HAO, Boulder, CO, United States
 
Using Quadrature Observations from the STEREO and SOHO Satellites to Identify the Relationship Between Coronal Dimmings and CMEs (755365)
Drew Manning1,2 and Larisza D Krista2, (1)Colorado College, Physics, Colorado Springs, CO, United States, (2)University of Colorado at Boulder, CIRES, Boulder, CO, United States
 
Characteristics and Importance of "ICME-in-Sheath" Phenomenon and Upper Limit for Geomagnetic Storm Activity (671912)
Ying D. Liu, Chong Chen and Xiaowei Zhao, NSSC National Space Science Center, CAS, Beijing, China
 
Magnetic field fluctuation properties in CME-driven sheath regions (689183)
K Emilia J Kilpua1, Simon Good2, Matti M Ala-Lahti3, Adnane Osmane2, Dominique Fontaine4, Lina Hadid5, Emiliya Yordanova6 and Miho Janvier7, (1)University of Helsinki, Department of Physics, Helsinki, Finland, (2)University of Helsinki, Helsinki, Finland, (3)University of Helsinki, Physics, Helsinki, Finland, (4)CNRS, Paris Cedex 16, France, (5)École Polytechnique, Paris, France, (6)IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, (7)Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, Orsay, France
 
Critical factors affecting change in CME orientation (709776)
Reka Moldovan Winslow1, Noé Lugaz1, Antoinette Broe Galvin2 and Camilla Scolini3, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)Univ of New Hampshire, Durham, NH, United States, (3)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium
 
Estimation of halo CME mass using synthetic CMEs based on a full ice-cream cone model (715027)
Hyeonock Na and Yong-Jae Moon, School of Space Research, Kyung Hee University, Yongin, South Korea
 
On the Quasi-Three Dimensional Configuration of Magnetic Clouds (715441)
Qiang Hu, University of Alabama in Huntsville, Department of Space Science and CSPAR, Huntsville, AL, United States, Qiu Jiong, Montana State University Bozeman, Bozeman, MT, United States, Paulett Creyke Liewer, Jet Propulsion Laboratory, Pasadena, CA, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Chunming Zhu, Montana State University, Physics, Bozeman, MT, United States
 
A model to understand the flux rope distortions resulting of the propagation (725751)
Teresa Nieves-Chinchilla1, Christina Kay1, Hebe Cremades2 and Laura Balmaceda3, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Organization Not Listed, Washington, DC, United States, (3)George Mason University, Fairfax, VA, United States
 
CME--CME Interactions as Sources of CME Helio-Effectiveness: the Early September 2017 Events (728152)
Camilla Scolini1,2, Emmanuel Chané1, Manuela Temmer3, Jens Pomoell4, K Emilia J Kilpua4, Karin Dissauer3, Astrid Veronig3, Erika Palmerio5, Mateja Dumbovic6, Jingnan Guo7, Luciano Rodriguez8 and Stefaan Poedts9, (1)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, (2)SIDC, Royal Observatory of Belgium, Brussels, Belgium, (3)University of Graz, Institute of Physics, Graz, Austria, (4)University of Helsinki, Helsinki, Finland, (5)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (6)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (7)University of Science and Technology of China, Hefei, China, (8)SIDC, Royal Observatory of Belgium, Uccle, Belgium, (9)KU Leuven, Centre for mathematical Plasma-Astrophysics, Department of Mathematics, Leuven, Belgium
 
Interactions Between Coronal Mass Ejections (702609)
Mary Eby1,2, Tatiana Niembro Hernandez3,4, Kristoff W Paulson2,4, Stephanie Colon5,6, Michael Louis Stevens4, Linda F Wilson7, Anthony W Case2,4 and Kelly E Korreck2,4, (1)Texas Lutheran University, Seguin, TX, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (3)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)University of Puerto Rico Rio Piedras Campus, San Juan, PR, United States, (6)Center for Astrophysics | Harvard-Smithsonian, Cambridge, United States, (7)Texas Lutheran University, Seguin, United States
 
The characteristics of suprathermal electrons for small-scale magnetic flux rope events observed near 1AU (671485)
Kyung-Eun Choi1, Dae-Young Lee1, Hee-Eun Wang2, Seunguk Lee2, Kyung-Chan Kim3 and Kyung Sun Park2, (1)Chungbuk National University, Cheongju, Korea, Republic of (South), (2)Chungbuk National University, Cheongju, South Korea, (3)Daegu University, Gyeongsan, South Korea
 
Stability Properties and Intermittent Failed Eruptions of Arched, Line-Tied Magnetic Flux Ropes (683350)
Andrew Alt1, Hantao Ji2, Jonathan Jara-Almonte2, Jongsoo Yoo1, Sayak Bose2 and Masaaki Yamada2, (1)Princeton University, Princeton, NJ, United States, (2)Princeton Plasma Physics Laboratory, Princeton, NJ, United States
 
Analysis of the Helical Kink Stability of Differently Twisted Magnetic Flux Ropes (675186)
Marta Florido-Llinas, Polytechnic University of Catalonia, CFIS, Barcelona, Spain, Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Mark Linton, US Naval Research Laboratory, Washington, DC, United States and Luiz Fernando Guedes dos Santos, Catholic University of America, Physics, Washington, DC, United States
 
Optimization of Magnetic Flux Ropes Modeled with the RBSL Method* (683755)
Viacheslav S. Titov, Cooper Downs, Tibor Torok, Jon Linker, Ronald M. Caplan and Roberto Lionello, Predictive Science Inc., San Diego, CA, United States
 
Properties of Streamer Wave Events Observed during the STEREO Era (749506)
Andrei Zhukov1, Bieke Decraemer1 and Tom Van Doorsselaere2, (1)Royal Observatory of Belgium, Brussels, Belgium, (2)KULeuven, Leuven, Belgium
 
IPSCAT: A Catalogue of Solar Transients Identified through Interplanetary Scintillation Analysis (756223)
David Barnes, United Kingdom Research and Innovation – Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Harwell Campus, United Kingdom, Mario Mark Bisi, United Kingdom Research and Innovation – Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Oxfordshire, United Kingdom, Jackie A Davies, United Kingdom Research and Innovation - Science & Technology Facilities Council - Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom and Richard Anthony Harrison, UKRI STFC Rutherford Appleton Laboratory, RAL Space, Harwell Campus, Didcot, United Kingdom
 
Deflection Flows as Measured by STEREO/PLASTIC: Statistics and Causes (753354)
Nada A Al-Haddad1, Antoinette Broe Galvin2 and Noé Lugaz1, (1)University of New Hampshire Main Campus, Durham, NH, United States, (2)Univ of New Hampshire, Durham, NH, United States
 
Characteristics of a long-lived CIR and the corresponding depression in the GCR flux (734826)
Bojan Vrsnak1, Mateja Dumbovic1, Manuela Temmer2 and Bernd Heber3, (1)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (2)University of Graz, Institute of Physics, Graz, Austria, (3)University of Kiel, Kiel, Germany
 
Heliocentric Distance Variation of Interplanetary Field Enhancements (687287)
Christopher T Russell1, Hanying Wei2, Hairong Lai3, Timothy Simon Horbury4, Marco C M Velli2, Helen O'Brien5, Vincent Evans6 and Virginia Angelini6, (1)University of California, Los Angeles, CA, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)Sun Yat-Sen University, Guangzhou, China, (4)Imperial College London, Department of Physics, London, SW7, United Kingdom, (5)Imperial College London, London, United Kingdom, (6)Imperial College London, Department of Physics, London, United Kingdom
 
Inherent Spatial Scales of Solar Wind Periodic Structures Found in ACE/SWICS Data (685678)
Irena Gershkovich1, Susan T Lepri1, Nicholeen M Viall2 and Simone Di Matteo2,3, (1)University of Michigan, Ann Arbor, MI, United States, (2)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (3)Catholic University of America, Physics Department, Washington, DC, United States
 
Recent Solar Wind Proton and Alpha Observations by STEREO PLASTIC (703232)
Antoinette Broe Galvin, University of New Hampshire Main Campus, Durham, NH, United States, Lorna Ellis, University of New Hampshire, Durham, United States, Lynn M Kistler, Univ New Hampshire, Durham, NH, United States and Sarah J Auriemma, University of New Hampshire Main Campus, Durham, United States
 
Changes in Alpha-to-Proton Ratios During Periodic Solar Wind Density Structures (728895)
Larry Kepko, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Nicholeen M Viall, NASA GSFC, Greenbelt, MD, United States