SH006
Coordinated multi-spacecraft observations in the inner heliosphere

Session ID#: 160193

Session Description:
The recent launch of Parker Solar Probe, Solar Orbiter, and BepiColombo offers unique opportunities for investigating the solar wind evolution, dynamics and structures in the inner heliosphere. The coordinated analysis of multi-point in-situ and remote observations from these and other spacecraft allow us to explore the temporal and radial evolution of the solar wind, and the solar energetic particles, and connect them to their solar and coronal drivers. In this session, we welcome abstracts of studies that utilize multispaceraft observations addressing the evolution of turbulence and plasma heating with heliocentric distance; transport and acceleration processes of solar energetic particles in the solar wind and through transient events, and how do they evolve radially. Observations from both in situ and remote sensing instruments are encouraged as well as supporting modeling efforts.
Co-Sponsor(s):
  • EGU: European Geosciences Union -
  • JpGU: Japan Geoscience Union -
Index Terms:

2101 Coronal mass ejections [INTERPLANETARY PHYSICS]
2114 Energetic particles [INTERPLANETARY PHYSICS]
2159 Plasma waves and turbulence [INTERPLANETARY PHYSICS]
2164 Solar wind plasma [INTERPLANETARY PHYSICS]


Primary Convener:  Lina Hadid, Laboratory of Plasma Physics, École Polytechnique, CNRS, Palaiseau, France
Conveners:  Luca Sorriso-Valvo, IRF Swedish Institute of Space Physics Uppsala, Uppsala, Sweden, Robert Colby Allen, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Beatriz Sanchez-Cano, University of Leicester, Leicester, LE1, United Kingdom
 
The Unusual Widespread Solar Energetic Particle Event on 2013 August 19: Solar Origin and Particle Longitudinal Distribution (Invited) (1044807)
Laura Rodriguez-Garcia1, Raul Gomez-Herrero1, Yannis Zouganelis2, Laura Balmaceda3, Teresa Nieves-Chinchilla4, Nina Dresing5, Mateja Dumbovic6, Nariaki Nitta7, Fernando Carcaboso-Morales4, Luiz Fernando Guedes dos Santos8, Lan Jian9, M. Leila Mays10, David Williams11 and Javier Rodriguez-Pacheco1, (1)Universidad de Alcalá, Space Research Group, Alcalá de Henares, Spain, (2)European Space Agency, Villanueva De La Can, Spain, (3)George Mason University, Fairfax, United States, (4)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (5)University of Turku, Department of Physics and Astronomy, Turku, Finland, (6)University of Zagreb, Hvar Observatory, Faculty of Geodesy, Zagreb, Croatia, (7)Lockheed Martin Advanced Technology Center, Palo Alto, CA, United States, (8)CIRES, University of Colorado at Boulder, Boulder, United States, (9)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (10)NASA/GSFC, Greenbelt, MD, United States, (11)European Space Agency, ESAC, Villanueva De La Cañada, Madrid, Spain
 
Tracking of turbulence and magnetic helicity evolution in the inner heliosphere during a Parker Solar Probe–BepiColombo radial alignment (1061199)
Tommaso Alberti1, Yasuhito Narita2, Lina Hadid3, Daniel Heyner4, Anna Milillo5, Christina Plainaki6, Hans Ulrich Auster7 and Ingo Richter4, (1)IAPS-INAF, Rome, Italy, (2)Austrian Academy of Sciences, Space Research Institute, Graz, Austria, (3)CNRS-LPP, Paris, France, (4)TU Braunschweig, Institute of Geophysics and Extraterrestrial Physics, Braunschweig, Germany, (5)INAF-IAPS, Rome, Italy, (6)ASI - Italian Space Agency, Rome, Italy, (7)Technische Universität Braunschweig, Braunschweig, Germany
 
Influence of the Sun’s active regions on the hydrogen backscatter glow (1061990)
Izabela Kowalska-Leszczyńska1, Marek Strumik2, Marzena A. Kubiak2 and Maciej A. Bzowski2, (1)Space Research Center Polish Academy of Sciences, Warszawa, Poland, (2)Space Research Centre Polish Academy of Sciences, Warsaw, Poland
 
Remotely-Sensed Heliospheric Analyses Reinforced by Multi-Spacecraft Observations used to Determine Radial Transport of Heliospheric Structures (1079909)
Bernard V Jackson1, Matthew Bracamontes1, Lucas Vernon Cota1, Andrew Buffington1, Munetoshi Tokumaru2, Kazumasa Iwai2, Kenichi Fujiki2, Mario Mark Bisi3 and Jackie A Davies3, (1)University of California, San Diego, Center for Astrophysics and Space Sciences, La Jolla CA, United States, (2)Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan, (3)United Kingdom Research and Innovation - Science & Technology Facilities Council -, Rutherford Appleton Laboratory, RAL Space, Didcot, United Kingdom
 
Flux rope and dynamics of the heliospheric current sheet. Theory, simulations and observations by Parker Solar Probe and Solar Orbiter. (Invited) (1086011)
Victor Réville1, Naïs Fargette2, Alexis P Rouillard1, Benoit Lavraud2, Marco C M Velli3, Antoine Strugarek4, Sacha Brun5, Chen Shi6, Athanasios Kouloumvakos2, Nicolas Poirier7, Rui Pinto8, Philippe Louarn9, Andrei Fedorov9, Christopher John Owen10, Vincent N Genot2, Timothy Simon Horbury11, Ronan Laker11, Helen O'Brien11, Virginia Angelini12 and Justin Christophe Kasper13, (1)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (2)IRAP, Toulouse, France, (3)Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States, (4)DRF/IRFU/DAp/LDE3 CEA Saclay, Saclay, France, (5)CEA Commissariat à l'Energie Atomique Saclay, Gif-Sur-Yvette Cedex, France, (6)University of California, Los Angeles, Los Angeles, United States, (7)L'Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France, (8)IRAP/CNRS, Toulouse, France, (9)IRAP, CNRS, Toulouse, France, (10)University College London, Mullard Space Science Laboratory, Dorking, United Kingdom, (11)Imperial College London, Department of Physics, London, SW7, United Kingdom, (12)Imperial College London, Department of Physics, London, United Kingdom, (13)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States
 
Multi-spacecraft observations of the 15 February 2022 solar energetic particle event (1108346)
Leng Ying Khoo1, Beatriz Sanchez-Cano2, Christina O Lee3, Athanasios Kouloumvakos4, Erika Palmerio5, Christina Cohen6, David Lario7, Fernando Carcaboso-Morales8, Laura Rodriguez-Garcia9, Jingnan Guo10, Joe Giacalone11, Vratislav Krupar8 and David J McComas12, (1)Princeton University, Astrophysical Sciences, Princeton, United States, (2)University of Leicester, Leicester, LE1, United Kingdom, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (5)University of North Dakota, Grand Forks, United States, (6)Caltech, Pasadena, United States, (7)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (8)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (9)Universidad de Alcalá, Space Research Group, Alcalá de Henares, Spain, (10)University of Science and Technology of China, Hefei, China, (11)University of Arizona, Planetary Sciences, Tucson, AZ, United States, (12)Princeton University, Department of Astrophysical Sciences, Princeton, NJ, United States
 
High-Resolution EUV Spectroscopy of CME Onset and Early Evolution (1111018)
Elizabeth Wraback, University of Michigan Ann Arbor, Ann Arbor, MI, United States, Enrico Landi, University of Michigan, Ann Arbor, MI, United States and Ward Manchester, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States
 
Collisional Transport of Solar Wind Plasma During its Journey from the Sun to the Earth (1120969)
Isabella Dieguez1, Kristoff W Paulson2, Michael Louis Stevens3, Yeimy Rivera1, Tatiana Niembro Hernandez2, Madisen Mae Johnson2, Anthony W Case3, Elliot Thomas Johnson4, Bennett Maruca5, Justin Christophe Kasper6, Kelly E Korreck3, Davin Larson7, Roberto Livi8, Michael McManus9, Ali Rahmati10 and Phyllis L Whittlesey8, (1)Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (3)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (4)University of Delaware, Newark, DE, United States, (5)Center for Astrophysics, Berkeley, CA, United States, (6)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (7)University of California Berkeley, Berkeley, CA, United States, (8)Space Sciences Laboratory, University of California Berkeley, Berkeley, United States, (9)SSL/UC Berkeley, Berkely, United States, (10)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
 
Radial Trends in Plasma Parameters Across the Heliosphere (1134990)
Bennett Maruca1, Ramiz A Qudsi1, B L L Alterman2, Brian Walsh3, Kelly E Korreck4, Daniel Verscharen5, Riddhi Bandyopadhyay6, Rohit Chhiber1, Alexandros Chasapis7, Tulasi Parashar8, William H Matthaeus1 and Melvyn L Goldstein9, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)Southwest Research Institute, Space Science and Engineering, San Antonio, MI, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (5)University of New Hampshire Main Campus, Durham, NH, United States, (6)Princeton University, Department of Astrophysics, Princeton, NJ, United States, (7)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (8)Victoria University of Wellington, Wellingon, New Zealand, (9)NASA Goddard SFC, Greenbelt, United States
 
Investigating Magnetic Structure in the Inner Heliosphere using Faraday Rotation, the FETCH instrument on the MOST mission (1151295)
Elizabeth A Jensen1, Nat Gopalswamy2, Shing Fung3, Lihua Li4, Manohar Deshpande3, Marta Shelton4, Jason Earl Kooi5, Stuart Bale6, Ward Manchester7, Alexei A Pevtsov8, David Wexler9, Lynn B Wilson III3, Lan Jian10, Joseph Lazio11, Teresa Nieves-Chinchilla12, Brian E. Wood13, Tim Bastian14, Qian Gong10, Megan Kenny15, Lloyd Purves3 and George Voellmer16, (1)Planetary Science Institute Tucson, Tucson, AZ, United States, (2)NASA Goddard SFC, Greenbelt, MD, United States, (3)NASA Goddard Space Flight Center, Greenbelt, United States, (4)NASA Goddard Space Flight Center, Washington D.C., United States, (5)University of Iowa, Iowa City, IA, United States, (6)University of California, Berkeley, Berkeley, CA, United States, (7)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI, United States, (8)National Solar Observatory, Boulder, United States, (9)University of Massachusetts Lowell, Space Science Laboratory, Lowell, United States, (10)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (11)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (12)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (13)Naval Research Lab, Washington, DC, United States, (14)National Radio Astronomy Observatory, Charlottesville, United States, (15)University of Colorado Boulder, Boulder, CO, United States, (16)Neon Company, Washington D.C., United States
 
Multi-Spacecraft Observation of Three SEP Events and Associated CMEs in Late March 2022. (1154685)
Christopher Light1, Claudio Corti2, M. Leila Mays3, Beatriz Sanchez-Cano4, David Lario5, Alessandro Bruno1, Ian G Richardson6, Michelangelo Romano1 and Daniel Heyner7, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)University of Hawaii at Manoa, Physics and Astronomy, Honolulu, HI, United States, (3)NASA/GSFC, Greenbelt, MD, United States, (4)University of Leicester, Leicester, LE1, United Kingdom, (5)NASA, Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (6)NASA Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, MD, United States, (7)TU Braunschweig, Institute of Geophysics and Extraterrestrial Physics, Braunschweig, Germany
 
Tracking a beam of electrons from the low solar corona into interplanetary space with the Low Frequency Array, Parker Solar Probe and 1 au spacecraft (1162959)
Samuel Timothy Badman1,2, Eoin Carley3, Nina Dresing4, Luis Alberto Cañizares3,5, Lan Jian6, David Lario7, Peter Gallagher3, Juan Carlos Martinez Oliveros8, Marc Pulupa9 and Stuart D Bale10, (1)University of California Berkeley, Berkeley, CA, United States, (2)Harvard-Smithsonian Center for Astrophysics, Cambridge, United States, (3)Dublin Institute for Advanced Studies, Dublin, Ireland, (4)University of Turku, Department of Physics and Astronomy, Turku, Finland, (5)Trinity College Dublin, Dublin, Ireland, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)NASA, Goddard Space Flight Center, Heliophysics Science Division, Greenbelt, United States, (8)Space Sciences Laboratory, Berkeley, CA, United States, (9)Space Sciences Laboratory, University of California Berkeley, Berkeley, CA, United States, (10)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States