Turbulence, reconnection and shocks are fundamental non-linear processes observed in solar, heliospheric, magnetospheric and laboratory plasmas. These processes are not separate, but rather appear to be interconnected. For instance, a close link exists between reconnection and turbulence. On the one hand the turbulence cascade favors the onset of magnetic reconnection between magnetic islands and, on the other hand, magnetic reconnection is able to trigger turbulence in the reconnection outflows and separatrices. Similarly, shocks may form in collisional and collisionless reconnection processes and can be responsible for turbulence formation, as for instance in the turbulent magnetosheath.

This session welcomes simulations, observational and theoretical works relevant for the study of these non-linear phenomena. Particularly welcome will be works focusing on the link between them in a range of scale going from fluid MHD to kinetic. The topic of this session is relevant for the understanding of solar atmosphere (from the photosphere to the solar wind), interaction of solar wind with planetary magnetospheres, planetary magnetospheric physics and particle acceleration and transport throughout the heliosphere. The session is also relevant to past and present space missions in plasma astrophysics such as Cluster, MMS and Parker Solar Probe.

Public information:
Julia E. Stawarz will give a solicited talk

Co-organized as PS4.4/ST2.8
Convener: Francesco Pucci | Co-conveners: Alexandros Chasapis, Maria Elena Innocenti, Giovanni Lapenta
| Wed, 10 Apr, 16:15–18:00
Room M1
| Attendance Mon, 08 Apr, 16:15–18:00
Hall X4

Attendance time: Monday, 8 April 2019, 16:15–18:00 | Hall X4

Chairperson: Francesco Pucci, Maria Elena Innocenti
X4.298 |
Joachim Raeder, Doug Cramer, Kai Germaschewski, and Andrei Runov
Hall X4
X4.299 |
First MMS Observations and Generation Mechanism for a New Kind of Magnetic Bottle With High-Energy Particles at High-latitude Magnetopause
Katariina Nykyri, Christina Chu, Xuanye Ma, Stephen Fuselier, and Rachel Rice
Hall X4
X4.300 |
Maria Elena Innocenti, Anna Tenerani, and Marco Velli
Hall X4
X4.301 |
Fabio Bacchini, Francesco Pucci, Francesco Malara, and Giovanni Lapenta
Hall X4
X4.302 |
Francesco Pucci, Pierre Henri, Francesco Califano, Sergio Servidio, Matteo Faganello, Thierry Passot, Pierre-Louis Sulem, and Giovanni Lapenta
Hall X4
X4.303 |
Natalia Borodkova, Victor Eselevich, Olga Sapunova, George Zastenker, and Yuri Yermolaev
Hall X4
X4.304 |
Pavel M. Travnicek and Christopher C. Chaston
Hall X4
X4.305 |
Criticality of Interplanetary Shocks: ARTEMIS Observations
Xiaoyan Zhou, Michael Gedalin, Christopher Russell, and Vassilis Angelopoulos
Hall X4
X4.306 |
Alexandr Afanasiev, Rami Vainio, Yann Pfau-Kempf, Urs Ganse, Lucile Turc, and Minna Palmroth
Hall X4
X4.307 |
Andreas Johlander, Andris Vaivads, Yuri V. Khotyaintsev, Damiano Caprioli, Colby C. Haggerty, Steven J. Schwartz, Barbara L. Giles, Roy B. Torbert, and Christopher T. Russell
Hall X4
X4.308 |
The topographical diagnostics of Turbulent Reconnection
Giovanni Lapenta and Francesco Pucci and the AIDA H2020 Project
Hall X4
X4.309 |
Simone Landi, Emanuele Papini, Luca Del Zanna, Luca Franci, and Petr Hellinger
Hall X4
X4.310 |
Urs Ganse, Yann Pfau-Kempf, Lucile Turc, Markus Battarbee, Thiago Brito, Maxime Dubart, Maxime Grandin, and Minna Palmroth
Hall X4
X4.311 |
Giulia Cozzani, Francesco Califano, Oreste Pezzi, Alessandro Retinò, Francesco Valentini, and Massimiliano Guarrasi