SH005
Connecting Remote and In Situ Observations to Understand the Dynamic Solar Wind and Transients

Session ID#: 162429

Session Description:
Recent additions to the Heliophysics System Observatory (i.e. SolO, PSP) alongside existing ground and space-based observatories provide an unprecedented multi-vantage-point view of the corona and inner heliosphere. One unifying science objective among these observatories is determining the physical processes that generate and energize the solar wind – a goal which hinges on connecting the in situ observed solar wind back to its solar source observed remotely. Further innovation to establish these connections requires coordinated efforts in observation, theory, and modeling to maximize the synergies between new and existing observatories.

We solicit contributions that connect remote corona and in situ solar wind observations to investigate the physical processes driving solar wind and transient events (e.g. SEPs, CMEs, CIRs, etc.) This session discusses the challenges in this interdisciplinary work and novel approaches to overcome them.
Index Terms:

7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7519 Flares [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Primary Convener:  Alicia Kathryn Petersen, University of Florida, Mechanical & Aerospace Engineering, Gainesville, FL, United States
Conveners:  Samuel Schonfeld, Boston College, Institute for Scientific Research, Newton, MA, United States and Samantha Wallace, NASA Postdoctoral Program / GSFC, Greenbelt, United States
 
Extrapolation and Topological Analysis of Magnetic Flux Ropes for Solar Eruption Events (1059643)
Wen He, University of Alabama in Huntsville, Department of Space Science, Huntsville, AL, United States and Qiang Hu, University of Alabama in Huntsville, Department of Space Science, Huntsville, United States
 
Reconstruction of in-situ measurements of CMEs using MHD simulation with IPS data observed from multiple ground-based stations (1065970)
Kazumasa Iwai1, Richard Andrew Fallows2, Mario Mark Bisi3, Daikou Shiota4, Bernard V Jackson5, Munetoshi Tokumaru1 and Kenichi Fujiki1, (1)Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan, (2)ASTRON, The Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (3)United Kingdom Research and Innovation - Science & Technology Facilities Council -, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom, (4)NICT National Institute of Information and Communications Technology, Tokyo, Japan, (5)Univ California San Diego, Center for Astrophysics and Space Sciences, La Jolla, CA, United States
 
Relating Remote and in situ Observations of Periodic Mesoscale Solar Wind Structures (1068155)
Nicholeen M Viall, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Larry Kepko, NASA GSFC, Greenbelt, MD, United States, Russell A. Howard, Applied Physics Laboratory Johns Hopkins, Laurel, United States, Mark Linton, US Naval Research Laboratory, Space Science Division, Washington, DC, United States, Simone Di Matteo, Catholic University of America, Washington, United States and Aleida Katherine Higginson, University of Michigan, AOSS, Ann Arbor, United States
 
Interpreting the Effects of Non-Equilibrium Ionization on Remote Sensing and In-Situ Observations Using Synthetic Data (1074174)
Judit Szente1, Enrico Landi2, Bart van der Holst3, Jim M Raines2 and Susan T Lepri2, (1)University of Michigan Ann Arbor, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (2)University of Michigan, Ann Arbor, MI, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
 
Investigations on helium abundance in background solar wind and interplanetary coronal mass ejections (1086879)
Yogesh .1, Dibyendu Chakrabarty1 and Nandita Srivastava2, (1)Physical Research Laboratory, Ahmedabad, India, (2)Udaipur Solar Observatory, Udaipur, India
 
Ace in the Hole: The Effect of Time-Dependent Magnetic Fields on Coronal Hole Development (1091932)
Emily Irene Mason1, Jon Linker2, Roberto Lionello2, Cooper Downs2, Ronald M. Caplan2, Viacheslav S. Titov2, Pete Riley3 and Marc L DeRosa4, (1)Predictive Science Inc., San Diego, United States, (2)Predictive Science Inc., San Diego, CA, United States, (3)Predictive Science, Inc., San Diego, United States, (4)Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, United States
 
Influence of coronal mass ejection orientation on dynamics in interplanetary space (1102868)
Karmen Martinic1, Mateja Dumbovic2, Manuela Temmer3, Astrid Veronig3 and Bojan Vrsnak2, (1)Hvar Observatory, Zagreb, Croatia, (2)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (3)University of Graz, Institute of Physics, Graz, Austria
 
Beyond Basic Drag - Effects of Solar Wind Pile-Up and High Speed Streams on CME Evolution (1108652)
Christina Kay, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, Stefan Hofmeister, Leibniz Institute for Astrophysics Potsdam, Potsdam, Germany and Erika Palmerio, University of North Dakota, Grand Forks, United States
 
Connecting White Light Images with In-situ Observations of Solar Wind Quantities for CME Simulations in the SWMF (1131271)
Hongfan Chen1, Yang Chen2, Xun Huan1, Bart van der Holst3, Shasha Zou3, Zhenguang Huang4, Nishtha Sachdeva3, Aniket Jivani1, Daniel Iong5, Ward Manchester3 and Gabor Toth6, (1)University of Michigan, Department of Mechanical Engineering, Ann Arbor, United States, (2)University of Michigan, Department of Statistics, Ann Arbor, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (4)University of Michigan-AOSS, Ann Arbor, United States, (5)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (6)University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Connecting White-light-Image-based Panoramic Solar WInd Map of Speed (WIPSWIMS) at heliocentric distance between 20 and 60 solar radii and solar wind in-situ observations at 1AU (1146927)
Xiaolei Li and Yuming Wang, University of Science and Technology of China, Hefei, China
 
Revisiting the Bastille Day Coronal Mass Ejection: Learning About the Eruption Through 3D MHD Time-Dependent Ionization Modeling of Heavy Ions (1148606)
Yeimy Rivera1, John Raymond2, Susan T Lepri3, Katharine Reeves4, Roberto Lionello5, Nicholas A Murphy6, Cooper Downs5 and Maurice L Wilson7, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Harvard Smithsonian Center for Astrophysics, Cambridge, MA, United States, (3)University of Michigan, Ann Arbor, MI, United States, (4)Smithsonian Institution, Cambridge, United States, (5)Predictive Science Inc., San Diego, CA, United States, (6)Center for Astrophysics | Harvard & Smithsonian, Cambridge, United States, (7)Harvard University, Cambridge, United States
 
Uninterrupted Tracking of Solar Wind Outflows Along Radial and Non-Radial Paths (1154921)
Nathalia Alzate1, Huw Morgan2, Nicholeen M Viall3, Angelos Vourlidas4, Daniel Seaton5, Simone Di Matteo6, Barbara J Thompson7, Teresa Nieves-Chinchilla8 and Craig DeForest5, (1)NASA Goddard Space Flight Center / ADNET Systems, Inc., Greenbelt, United States, (2)Aberystwyth University, Aberystwyth, United Kingdom, (3)NASA GSFC, Greenbelt, MD, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)Southwest Research Institute, Boulder, CO, United States, (6)NASA Goddard Space Flight Center / Catholic U. of America, Greenbelt, United States, (7)NASA/GSFC, Greenbelt, MD, United States, (8)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States
 
An Array of Low-Cost Machine Learning-Enabled Magnetometer Systems For Real-Time GIC Analysis and Prediction (1160987)
Mdshaad Mahmud and Talha Siddique, University of New Hampshire Main Campus, Durham, NH, United States
 
Distributions of ICME properties in the inner heliosphere from a database of ensemble MHD simulations (1183880)
Elena Provornikova1, Sarah E Gibson2, Anna V Malanushenko3,4, Angelos Vourlidas1, Viacheslav G Merkin5, Charles Nickolos Arge6, Kévin Dalmasse7, Natasha Flyer8 and Michael James Wiltberger9, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (3)NCAR, High Altitude Observatory (HAO), Boulder, CO, United States, (4)High Altitude Observatory, Boulder, United States, (5)The Johns Hopkins University, APL, Laurel, United States, (6)NASA Goddard Space Flight Center, Greenbelt, United States, (7)University of Toulouse, Toulouse, France, (8)National Center for Atmospheric Research, Computational and Information Systems Lab, Boulder, CO, United States, (9)National Center for Atmospheric Research, Boulder, CO, United States
 
Transients Released in Slow Solar Wind: Synthetic In-situ and Remote Observations by PSP (1193590)
Ziqi Wu, Jiansen He, Die Duan, Chuanpeng Hou, Zhuo Rui and Tianhang Chen, Peking University, Beijing, China
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