Addressing the Mysteries of Inner Heliospheric Dynamics from a Multi-Spacecraft Vantage Point
Addressing the Mysteries of Inner Heliospheric Dynamics from a Multi-Spacecraft Vantage Point
Session ID#: 121705
Session Description:
The current Heliophysics System Observatory (HSO) is enabling investigations of solar wind dynamics and structures in new and exciting ways. Multiple spacecraft near 1 AU, joint with Parker Solar Probe, Solar Orbiter, and BepiColombo in the inner heliosphere, facilitate exploration of temporal, longitudinal, and radial variations of the solar wind and transients, and also improve our ability to connect these variations to solar and coronal phenomena. In this session, we welcome abstracts for studies that utilize the multitude of current and/or former HSO assets to demonstrate their utility leading to novel and compelling scientific advances in our understanding of solar wind dynamics and structures. Multi-spacecraft analysis providing insight into solar wind plasma, coronal mass ejections, corotating or stream interaction regions, heliospheric current sheets, and solar energetic particle events, as well as examinations into solar and coronal structures, are all encouraged.
Index Terms:
2101 Coronal mass ejections [INTERPLANETARY PHYSICS]
2102 Corotating streams [INTERPLANETARY PHYSICS]
2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
Primary Convener: Robert Colby Allen, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Conveners: Lan Jian, NASA Goddard Space Flight Center, Code 6710, Greenbelt, MD, United States, Lina Hadid, LPP, CNRS, Observatoire de Paris, PSL Research University, Sorbonne Université, École Polytechnique, Institut Polytechnique de Paris, Paris, France and Yuming Wang, University of Science and Technology of China, Hefei, China
Primary Liaison: Robert Colby Allen, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
See more of: SPA-Solar and Heliospheric Physics