SH006
Coordinated multi-spacecraft observations in the inner heliosphere
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
See more of: SPA-Solar and Heliospheric Physics
