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Session Proposal: Solar Orbiter: Solar-Heliospheric Connections and First Out-of-the-Ecliptic Observations (AGU25)

SH029
Solar Orbiter: Solar-Heliospheric Connections and First Out-of-the-Ecliptic Observations

Session ID#: 250855

Session Description:
The Solar Orbiter mission, an international cooperation between ESA and NASA, is currently orbiting the Sun with an orbital inclination of ~17 degrees with respect to the solar equator at heliocentric distances ranging from 0.29 to 0.90 au. This inclination provides a unique vantage point to explore both southern and northern solar latitudes that have never been observed from near the ecliptic plane. The rich in-situ and remote-sensing data sets collected by Solar Orbiter during its trajectory offer multiple opportunities to probe the connection between the Sun and the inner heliosphere. This session invites contributions that enhance the goals of the Solar Orbiter mission, including observations from Solar Orbiter's unique vantage point, combinations with other observational assets, numerical simulations, and theoretical developments that increase our understanding of the connections between the Sun and the heliosphere.
Index Terms:

7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7513 Coronal mass ejections [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7514 Energetic particles [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
Primary Convener:  David Lario, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Conveners:  Fernando Carcaboso, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, Astrid Veronig, University of Graz, Institute of Physics, Graz, Austria and Don Hassler, Southwest Research Institute, Boulder, United States
 
Solar Orbiter: Mission Status and Science Highlights (1846978)
Miho Janvier1, Teresa Nieves-Chinchilla2, David Lario3, Daniel Mueller1 and for the Solar Orbiter Team, (1)European Space Agency, ESTEC, Noordwijk, Netherlands, (2)NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States, (3)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States
 
Understanding the complex morphology of a CME: multi-view analysis and numerical modeling (1850278)
Cecilia Mac Cormack, NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, Abril Sahade, NASA Goddard Space Flight Center, Greenbelt, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, United States, Phillip Hess, George Mason University Fairfax, Fairfax, United States, Robin C Colaninno, Naval Research Laboratory, Washington, DC, United States and Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States
 
Probing Transition Region–Solar Wind Connectivity with SPICE and SWA/HIS Instruments (Invited) (1853569)
Tania Varesano, University of Colorado Boulder, Boulder, United States and SPICE consortium
 
Simultaneous Energetic Ion Onsets in 3He-rich Solar Energetic Particle Events (1855865)
Glenn M Mason, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Athanasios Kouloumvakos, The Johns Hopkins University. Applied Physics Laboratory, Laurel, United States, George C Ho, southwest Research Institute, San Antonio, United States, Robert Colby Allen, Southwest Research Institute, San Antonio, United States, Raul Gomez-Herrero, University of Alcala, Space Research Group, Alcala de Henares, Spain, Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany and Javier Rodriguez-Pacheco, University of Alcalá, Space Research Group, Alcalá de Henares, Spain
 
Solar Energetic Particles Observed by Solar Orbiter at High Latitude (1857345)
George C Ho1, Glenn M Mason2, Robert Colby Allen3, Samuel Hart3, Athanasios Kouloumvakos4, Robert F Wimmer-Schweingruber5, Javier Rodriguez-Pacheco6 and Raul Gomez-Herrero7, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (3)Southwest Research Institute, San Antonio, United States, (4)The Johns Hopkins University. Applied Physics Laboratory, Laurel, United States, (5)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (6)University of Alcalá, Space Research Group, Alcalá de Henares, Spain, (7)University of Alcala, Space Research Group, Alcala de Henares, Spain
 
An investigation of the shock properties for "nose-like" solar energetic particle events (1857619)
Athanasios Kouloumvakos1, David Lario2, Glenn M Mason1, Robert Colby Allen3, Grant Berland4, Zigong Xu5, Laura Rodriguez Garcia6, Immanuel Christopher Jeba Raj7, Zheyi Ding8, Nicolas Wijsen9, George C Ho10, Christina Cohen11, Angelos Vourlidas12, Pete Riley13, Edmond C Roelof12, Evangelos Paouris1, Savvas Raptis14, Javier Rodriguez-Pacheco15, Donald G Mitchell1, Robert F Wimmer-Schweingruber16 and Matthew Hill12, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Goddard Space Flight Center, Greenbelt, United States, (3)Southwest Research Institute, San Antonio, United States, (4)Johns Hopkins University Applied Physics Laboratory, SES, Laurel, United States, (5)California Institute of Technology, Pasadena, CA, United States, (6)European Space Agency / ESAC, Madrid, Spain, (7)University of Turku, Turku, Finland, (8)KU Leuven, Centre for mathematical Plasma-Astrophysics, Dover, NH, United States, (9)KU Leuven, Centre for mathematical Plasma-Astrophysics, Leuven, Belgium, (10)southwest Research Institute, San Antonio, United States, (11)Caltech, Pasadena, United States, (12)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (13)Predictive Science Inc., San Diego, United States, (14)KTH Royal Institute of Technology, Division of Space and Plasma Physics, Stockholm, Sweden, (15)University of Alcalá, Space Research Group, Alcalá de Henares, Spain, (16)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
 
Latitudinal structure of the heliospheric magnetic field and solar wind in the inner heliosphere: results of the first Solar Orbiter out of ecliptic orbit (1860653)
Timothy Simon Horbury1, Stuart D Bale2, Andrei Fedorov3, Lorenzo Matteini4, Mathew James Owens5, Dr. Erika Palmerio6, Tamar Ervin7, Adam Finley8, Samuel Badman9, Yeimy Rivera10, Joseph Wang11, Philippe Louarn3, Christopher John Owen12, Michael Louis Stevens13, Roberto Livi14, Davin Larson9 and Phyllis Whittlesey14, (1)Imperial College London, Department of Physics, London, SW7, United Kingdom, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (4)Imperial College London, Department of Physics, London, United Kingdom, (5)University of Reading, Reading, United Kingdom, (6)Predictive Science Inc., San Diego, CA, United States, (7)Predictive Science Inc., San Diego, United States, (8)CEA Saclay DSM / LSCE, Gif sur Yvette, France, (9)University of California Berkeley, Berkeley, United States, (10)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (11)Imperial College London, London, SW7, United Kingdom, (12)UCL, Mullard Space Science Laboratory, Dorking, United Kingdom, (13)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (14)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States
 
Update on Monitoring the Solar Orbiter SPICE Instrument Radiometric Response (1862325)
William T Thompson, ADNET Systems Inc. Greenbelt, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Dispersive out-of-ecliptic solar particle events observed by EPD on Solar Orbiter (1877547)
Robert F Wimmer-Schweingruber1, Javier Rodriguez-Pacheco2, George C Ho3, Alexander Warmuth4, Lars Berger1, Glenn M Mason5, Raul Gomez-Herrero6, Zheyi Ding7, Säm Krucker8, Alexander Kollhoff1, Francisco Espinosa Lara6, Patrick Kühl9, Robert Colby Allen10, Erik Jentsch1, Ignacio Cernuda11, Yulia Kartavykh7, Sindhuja Gunaseelan7, Sebastian Fleth12 and Sandra Eldrum1, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)Universidad de Alcalá, Space Research Group, Alcalá de Henares, Spain, (3)southwest Research Institute, San Antonio, United States, (4)Leibniz Institute for Astrophysics Potsdam, Potsdam, Germany, (5)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (6)University of Alcala, Space Research Group, Alcala de Henares, Spain, (7)University of Kiel, Institute of Experimental and Applied Physics, Kiel, Germany, (8)University of Applied Sciences and Arts Northwestern Switzerland, Windisch, Switzerland, (9)Christian Albrechts Universität Kiel, Kiel, Germany, (10)Southwest Research Institute, San Antonio, United States, (11)University of Alcala, Alcala de Henares, Spain, (12)Institute for Experimental and Applied Physics (IEAP), Christian-Albrechts-University of Kiel, Kiel, Germany, Kiel, Germany
 
Bidirectional Solar Energetic Particle Events at Solar Orbiter (1887504)
Zheyi Ding1, Robert F Wimmer-Schweingruber1, Yu Chen2, Lingling Zhao3, Patrick Kühl4, Alexander Kollhoff1, Liu Yang1, Lars Berger1, Javier Rodríguez-Pacheco5, George C Ho6 and Glenn M Mason7, (1)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (2)University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, Huntsville, AL, United States, (3)Center for Space Plasma and Aeronomic Research, Huntsville, United States, (4)Christian Albrechts Universität Kiel, Kiel, Germany, (5)University of Alcalá, Department of Physics and Mathematics, Madrid, Spain, (6)southwest Research Institute, San Antonio, United States, (7)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
 
Assimilating SO/PHI-FDT far-side observations in ADAPT-WSA: Implications for source region and S-web connectivity of the solar wind and SEPs. (1891876)
Samantha Wallace1, Vincenzo Andretta2, David Lario3, Nicholeen M Viall4, Spiro K Antiochos4, Daniel da Silva5, Samuel Schonfeld6 and Charles Nickolos Arge5, (1)Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, (2)INAF - Osservatorio Astronomico di Capodimonte, Napoli, Italy, (3)Goddard Space Flight Center, Greenbelt, United States, (4)NASA GSFC, Greenbelt, United States, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (6)Air Force Research Laboratory Albuquerque, Albuquerque, United States
 
Do density-depleted regions trailing CMEs survive in the inner heliosphere? (1899567)
Carlos Roberto Braga1, Vamsee Krishna Jagarlamudi1, Angelos Vourlidas1, Guillermo A Stenborg1 and David Lario2, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States
 
Out-of-the-Ecliptic Dust Investigation via Solar Orbiter RPW Observations (1915565)
Mitchell Shen1, David Malaspina2, Petr Pokorny3, Jamey R Szalay1, David Pisa4, Jan Soucek5, Arnaud Zaslavsky6, Milan Maksimovic7 and Stuart D Bale8, (1)Princeton University, Department of Astrophysical Sciences, Princeton, United States, (2)University of Colorado, Astrophysical and Planetary Sciences Department, Boulder, United States, (3)Catholic University of America, Department of Physics and Astronomy, Washington, DC, United States, (4)Institute of Atmospheric Physics, Czech Academy of Sciences, Prague, Czech Republic, (5)Inst. of Atmospheric Physics, Praha 4, Czech Republic, (6)CNRS, Observatoire de Paris, LESIA, Meudon, France, (7)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (8)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Solar Wind Characterization using Tomography and WSA (1929586)
Diego Lloveras1,2, Laura Balmaceda1,2, Alberto M Vásquez3, Federico Nuevo3, Evangelia Samara1,4, Charles Nickolos Arge1 and Teresa Nieves-Chinchilla5, (1)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (2)George Mason University Fairfax, Physics and Astronomy Department, Fairfax, United States, (3)Instituto de Astronomía y Física del Espacio (UBA-CONICET), Buenos Aires, Argentina, (4)The Catholic University of America, Washington, DC, United States, (5)NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States
 
Solar wind compositions near Heliospheric current sheet at 0.3-1 AU: Solar Orbiter Heavy Ion Sensor observations (1930605)
Keiichi Ogasawara1, Ryan M. Dewey2, Antoinette Broe Galvin3, Timothy Simon Horbury4, Susan T Lepri5, Stefano A Livi6, Philippe Louarn7, Christopher John Owen8 and Jim M Raines5, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Laboratory for Atmospheric and Space Physics, Boulder, United States, (3)University of New Hampshire, Durham, United States, (4)Imperial College London, Department of Physics, London, SW7, United Kingdom, (5)University of Michigan, Ann Arbor, United States, (6)SwRI, San Antonio, United States, (7)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (8)UCL, Mullard Space Science Laboratory, Dorking, United Kingdom
 
Embracing New Perspectives: Highlights of SO/PHI Polar Data from First Out-of-Ecliptic Observations (Invited) (1939705)
Julian Blanco Rodriguez1, Daniele Calchetti2, Lakshmi Pradeep Chitta2, Johann Hirzberger2, Alejandro Moreno Vacas3, David Orozco Suárez3, Sami K. Solanki2, Hanna Strecker3, Jose Carlos del Toro Iniesta3, Artem Ulyanov2, Gherardo Valori2, Joachim Woch2 and SO/PHI Team, (1)University of Valencia, Burjassot, Spain, (2)Max Planck Institute for Solar System Research, Göttingen, Germany, (3)Instituto de Astrofísica de Andalucía, IAA-CSIC, Granada, Spain
 
Influences of Heliospheric and Coronal Magnetic Field Configurations on the Backmapping of the High- and Low-latitude Solar Wind (1944119)
Liping Yang, NSSC National Space Science Center, CAS, Beijing, China, Xinyi Ma, State Key Laboratory for Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China, Xueshang Feng, National Space Science Center, Beijing, China, Hui Tian, Peking University, School of Earth and Space Sciences, Beijing, China and Fang Shen, National Space Science Center, CAS, Beijing, China
 
Thermal structure in a prominence observed by SPICE/SoLO (1948942)
Jenny Rodríguez Gómez, Catholic University of America, Washington, United States, Therese Ann Kucera, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Peter R Young, George Mason University Fairfax, Fairfax, United States and Susanna Parenti, Institut d'Astrophysique de Paris, Paris, France
 
SoloHI’s First Heliographic Images From Out of the Ecliptic (1955185)
Robin C Colaninno, US Naval Research Laboratory, Washington, DC, United States, Phillip Hess, US Naval Research Laboratory, Washington, United States, Dr. Erika Palmerio, Predictive Science Inc., San Diego, CA, United States and Eleni Nikou, NRC Research Associate, U.S. Naval Research Laboratory, Washington, DC, United States
 
A Statistical Study of Polar Crown Filament Eruptions (1956741)
Ying Wang, New Jersey Institute of Technology, Edison, NJ, United States, Yan Xu, Institute for Space Weather Sciences, New Jersey Institute of Technology, Newark, United States, Ju Jing, New Jersey Institute of Technology - Institute for Space Weather Sciences, Newark, United States and Haimin Wang, New Jersey Institute of Technology, Center for Solar-Terrestrial Research, Newark, United States
 
Coronal Abundance Evolution During the M7.6 Flare on September 30, 2024 with SolO/SPICE, Hinode EIS, and Chandrayaan-2 XSM: A disharmonious picture between the cool and hot plasma components (1958452)
Momchil Molnar, Southwest Research Institute Boulder, Solar and Heliospheric Physics, Boulder, CO, United States, Joseph Plowman, Southwest Research Institute Boulder, Boulder, United States, Dr. Ritesh Patel, Southwest Research Institute, Boulder, CO, United States, Don Hassler, Southwest Research Institute, Boulder, United States, Ryan French, Laboratory for Atmospheric and Space Physics, Boulder, United States, Lakshmi Pradeep Chitta, Max Planck Institute for Solar System Research, Göttingen, Germany, Arpit Kumar Shrivastav, Southwest Research Institute Boulder, Boulder, CO, United States and Tania Varesano, University of Colorado Boulder, Boulder, United States
 
New Insights from Semi-automatic Reconstructions of Multi-viewpoint CME Observations: The October 2024 Halo Events (1958956)
Eleni Nikou, NRC Research Associate, U.S. Naval Research Laboratory, Washington, DC, United States, Robin C Colaninno, Naval Research Laboratory, Washington, DC, United States, Phillip Hess, George Mason University Fairfax, Fairfax, United States, Angelos Vourlidas, Johns Hopkins University Applied Physics Laboratory, Laurel, United States, Arnaud Thernisien, Naval Research Laboratory, Washington, United States, Jie Zhang, George Mason University, Department of Physics and Astronomy, Fairfax, United States and Natsuha Kuroda, George Mason University, Fairfax, United States
 
Comparison of synthetic white-light images with SoloHI observations using a novel approach with a highly deformable CME geometry (1964289)
Andreas Weiss, University of Maryland Baltimore County, Baltimore, United States; NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, Carlos Roberto Braga, Johns Hopkins University Applied Physics Laboratory, Laurel, United States, Dr. Erika Palmerio, Predictive Science Inc., San Diego, CA, United States, Cecilia Mac Cormack, Catholic University of America, Washington, United States; NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States and Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States
 
Assessing the performance of Solar Orbiter PHI science data using WSA (1964767)
Alison Farrish1, Grace Gratton2, Charles Nickolos Arge1, Samuel Schonfeld3, Carl J Henney4, Evangelia Samara5 and Laura Balmaceda6, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, (3)Air Force Research Laboratory Albuquerque, Albuquerque, United States, (4)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, United States, (5)Catholic University of America, Washington, United States, (6)George Mason University, Fairfax, United States
 
Probing Dynamics in a Pseudostreamer using Inner and Middle Corona Observations of Solar Orbiter (1965346)
Arpit Kumar Shrivastav1, Rohan Bose2, Momchil Molnar3, Joseph Plowman4, Lakshmi Pradeep Chitta5, Vaibhav Pant6, Don Hassler7, Daniel B Seaton8, Dr. Ritesh Patel8, Marelina Mierla9, Andrei Zhukov10 and David Berghmans9, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)Aryabhatta Research Institute of Observational-Sciences, Nainital, India, (3)Southwest Research Institute Boulder, Solar and Heliospheric Physics, Boulder, CO, United States, (4)Southwest Research Institute Boulder, Boulder, United States, (5)Max Planck Institute for Solar System Research, Göttingen, Germany, (6)Aryabhatta Research Institute of Observational-Sciences, Astrophysics and Astronomy, Nainital, India, (7)Southwest Research Institute, Boulder, United States, (8)Southwest Research Institute, Boulder, CO, United States, (9)Royal Observatory of Belgium, Brussels, Belgium, (10)SIDC, Royal Observatory of Belgium, Brussels, Belgium
 
Recurrent 3He-rich Solar Energetic Particles Events During Solar Orbiter’s First Latitudinal Sweep across the Solar Equator (1967089)
Samuel Hart, Southwest Research Institute, San Antonio, TX, United States, George C Ho, southwest Research Institute, San Antonio, United States, Glenn M Mason, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Robert Colby Allen, Southwest Research Institute, San Antonio, United States
 
Evaluating the inclusion of SolO/PHI farside magnetograms in ADAPT global solar magnetic maps (1967665)
Samuel Schonfeld1, Grace Gratton2, Carl J Henney1, Shaela I Jones3 and Charles Nickolos Arge4, (1)Air Force Research Laboratory Kirtland AFB, Kirtland AFB, United States, (2)Embry-Riddle Aeronautical University, Daytona Beach, FL, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Magnetic Reconnection Across Scales and Latitudes: Statistical Analysis form SDO/AIA and Solar Orbiter/EUI (1971418)
Dr. Bibhuti Kumar Jha1, Arpit Kumar Shrivastav1, Dr. Ritesh Patel2, Shanwlee Sow Mondal3, Chris Lowder4, Daniel B Seaton2 and Lisa Upton4, (1)Southwest Research Institute Boulder, Boulder, CO, United States, (2)Southwest Research Institute, Boulder, CO, United States, (3)Catholic University of America, Washington, United States, (4)Southwest Research Institute Boulder, Boulder, United States
 
Pickup Ion Distributions In the Inner Heliosphere (0.3 AU to 1 AU) as Observed by the Solar Orbiter SWA/Heavy Ion Sensor (1974318)
Antoinette Broe Galvin1, Lynn M Kistler2, Lorna Ellis3, Bernard John Vasquez4, Stefano A Livi5, Christopher John Owen6, Philippe Louarn7, Susan T Lepri8, Jim M Raines8, Ryan M. Dewey9, Timothy Stubbs10, Kevin Delano11, Benjamin L. Alterman12 and Yeimy Rivera13, (1)University of New Hampshire Main Campus, Institute for the Study of Earth, Oceans and Space & Department of Physics and Astronomy, Durham, NH, United States, (2)Univ New Hampshire, Durham, United States, (3)University of New Hampshire, Durham, United States, (4)University of New Hampshire, Durham, NH, United States, (5)SwRI, San Antonio, United States, (6)UCL, Mullard Space Science Laboratory, Dorking, United Kingdom, (7)CNRS - Institut de Recherche en Astrophysique et Planétologie, Toulouse, France, (8)University of Michigan, Ann Arbor, United States, (9)Laboratory for Atmospheric and Space Physics, Boulder, United States, (10)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (11)NASA Goddard Space Flight Center, Baltimore, United States, (12)Southwest Research Institute, Space Science and Engineering, San Antonio, United States, (13)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States
 
What will Solar Orbiter see in its first high latitude pass? (1980801)
Robert James Leamon, Lynker Space, Washington, United States and the Lynker Space Team
 
Inner Structure of CMEs: Insights from SoloHI observations and CORHEL-CME simulations (1989553)
Cecilia Mac Cormack, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Abril Sahade, NASA Goddard Space Flight Center, Greenbelt, United States, Evangelia Samara, Catholic University of America, Washington, United States, Phillip Hess, George Mason University Fairfax, Fairfax, United States, Robin C Colaninno, Naval Research Laboratory, Washington, DC, United States and Teresa Nieves-Chinchilla, NASA Goddard Space Flight Center, Heliophysics Science Division, MD, United States
 
The Structure and Dynamics of the Forming Heliospheric Current Sheet (2000247)
Lizet Casillas, University of California Los Angeles, Los Angeles, United States, Marco C M Velli, Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, Victor Réville, Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France and Benjamin Lynch, Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States