The majority of space plasmas are in a turbulent state, displaying fluctuations and nonlinear behaviour at a broad range of scales. A variety of these plasmas are also seen to be heated, with dissipation of turbulence as a possible explanation. Many aspects of the turbulence and heating, and their interaction with other space plasma phenomena (e.g., shocks, reconnection, and instabilities), however, remain to be fully understood. This session will address these questions through discussion of observational, theoretical, numerical, and laboratory work to understand these processes. This session is relevant to many currently operating and future missions (e.g., Wind, Cluster, MMS, STEREO, THEMIS, Van Allen Probes, DSCOVR, Parker Solar Probe and Solar Orbiter).

Convener: Luca Sorriso-Valvo | Co-conveners: Olga Alexandrova, Christopher Chen, Petr Hellinger
| Thu, 11 Apr, 08:30–10:15
Room L1
| Attendance Thu, 11 Apr, 10:45–12:30
Hall X4

Thursday, 11 April 2019 | Room L1

Chairperson: Luca Sorriso-Valvo
08:30–08:45 |
Lorenzo Matteini, David Stansby, Timothy S. Horbury, and Christopher H.K. Chen
08:45–09:00 |
Julia E. Stawarz, Luca Franci, Emanuele Papini, Simone Landi, Petr Hellinger, Christopher H. K. Chen, Lorenzo Matteini, Andrea Verdini, David Burgess, James L. Burch, Daniel J. Gershman, Barbara L. Giles, Olivier Le Contel, Per-Arne Lindqvist, Robert E. Ergun, Christopher T. Russell, Robert J. Strangeway, and Roy B. Torbert
09:00–09:15 |
Jana Safrankova, Zdenek Nemecek, Frantisek Nemec, Daniel Verscharen, Christopher H. K. Chen, Tereza Durovcova, and Maria O. Riazantseva
09:15–09:30 |
| solicited
Anna Tenerani and Marco Velli
09:30–09:45 |
Andrea Verdini, Roland Grappin, Olga Alexandrova, Luca Franci, Simone Landi, Lorenzo Matteini, and Emanuele Papini
09:45–10:00 |
Xingyu Zhu, Jiansen He, Daniel Verscharen, and Jinsong Zhao
10:00–10:15 |
Daniel Verscharen and Robert Wicks