Search Publications

Plasma heating and particle acceleration in collisionless shocks through astrophysical observations
DOI: 10.1088/1361-6587/acb082 Bibcode: 2023PPCF...65c4003M

Miceli, M.

Supernova remnants (SNRs), the products of stellar explosions, are powerful astrophysical laboratories, which allow us to study the physics of collisionless shocks, thanks to their bright electromagnetic emission. Blast wave shocks generated by supernovae (SNe) provide us with an observational window to study extreme conditions, characterized by h…

2023 Plasma Physics and Controlled Fusion
XMM-Newton 5
Thermal instability and non-equilibrium in solar coronal loops: from coronal rain to long-period intensity pulsations
DOI: 10.1088/1361-6587/ab5406 Bibcode: 2020PPCF...62a4016A

Antolin, Patrick

The complex interaction of the magnetic field with matter is the key to some of the most puzzling observed phenomena at multiple scales across the Universe, from tokamak plasma confinement experiments in the laboratory to the filamentary structure of the interstellar medium. A major astrophysical puzzle is the phenomenon of coronal heating, upon w…

2020 Plasma Physics and Controlled Fusion
IRIS 83
Current sheets in planetary magnetospheres
DOI: 10.1088/1361-6587/aafbbf Bibcode: 2019PPCF...61e4002Z

Delcourt, Dominique; Zelenyi, Lev; Malova, Helmi +2 more

In this article we aim to highlight the problems related to the structure and stability of the comparatively thin current sheets that were relatively recently discovered by space missions in the magnetospheres of the Earth and planets, as well as in the solar wind. These magnetoplasma structures are universal in collisionless cosmic plasmas and ca…

2019 Plasma Physics and Controlled Fusion
Cluster 11
The flux rope nature of coronal mass ejections
DOI: 10.1088/0741-3335/56/6/064001 Bibcode: 2014PPCF...56f4001V

Vourlidas, Angelos

Coronal mass ejections (CMEs) are ejections of magnetized plasma from the solar corona. They are the most spectacular examples of explosive energy release on the Sun. Their magnetic structure is of particular importance because it determines their effects on the terrestrial magnetosphere. Here, I present recent observational evidence for the exist…

2014 Plasma Physics and Controlled Fusion
SOHO 63
Correlated observations of intensified whistler waves and electron acceleration around the geostationary orbit
DOI: 10.1088/0741-3335/54/3/035004 Bibcode: 2012PPCF...54c5004X

Zong, Qiugang; Su, Zhenpeng; Xiao, Fuliang +3 more

We report correlated observations of enhanced whistler waves and energetic electron acceleration collected by multiple satellites specifically near the geostationary orbit during the 7-10 November 2004 superstorms, together with multi-site observations of ULF wave power measured on the ground. Energetic (>0.6 MeV) electron fluxes are found to i…

2012 Plasma Physics and Controlled Fusion
Cluster 2
BRIEF COMMUNICATION: Electron acceleration by whistler-mode waves around the magnetic null during 3D reconnection
DOI: 10.1088/0741-3335/52/5/052001 Bibcode: 2010PPCF...52e2001X

Zong, Qiugang; He, Jiansen; Su, Zhenpeng +5 more

The magnetic field configuration around a magnetic null pair and its associated electron behavior during 3D magnetic reconnection have recently been reported from in situ observations. Electrons are suggested to be temporarily trapped in the central reconnection region as indicated by an electron density peak observed near the magnetic null (He J-…

2010 Plasma Physics and Controlled Fusion
Cluster 8
Current filaments in turbulent magnetized plasmas
DOI: 10.1088/0741-3335/51/12/124053 Bibcode: 2009PPCF...51l4053M

Sundkvist, D.; Martines, E.; Vianello, N. +18 more

Direct measurements of current density perturbations associated with non-linear phenomena in magnetized plasmas can be carried out using in situ magnetic measurements. In this paper we report such measurements for three different kinds of phenomena. Current density fluctuations in the edge density gradient region of a fusion plasma confined in rev…

2009 Plasma Physics and Controlled Fusion
Cluster 13
Magnetic reconnection in space plasma
DOI: 10.1088/0741-3335/51/12/124016 Bibcode: 2009PPCF...51l4016V

Retinò, Alessandro; Vaivads, Andris; André, Mats

The terrestrial magnetosphere is a natural laboratory where many important plasma processes can be studied in detail by using high-quality spacecraft measurements of electromagnetic fields and particle distribution functions over a broad range of spatial and temporal scales. One such important process is magnetic reconnection. We discuss recent re…

2009 Plasma Physics and Controlled Fusion
Cluster 1
Shear driven waves in the induced magnetosphere of Mars
DOI: 10.1088/0741-3335/50/7/074018 Bibcode: 2008PPCF...50g4018G

Fedorov, A.; Barabash, S.; Lundin, R. +12 more

We present measurements of oscillations in the electron density, ion density and ion velocity in the induced magnetosphere of Mars. The fundamental frequency of the oscillations is a few millihertz, but higher harmonics are present in the spectrum. The oscillations are observed in a region where there is a velocity shear in the plasma flow. The fu…

2008 Plasma Physics and Controlled Fusion
MEx 21
Simulation of zonal flow excitation by drift mode turbulence: applications to tokamaks and the magnetopause
DOI: 10.1088/0741-3335/50/12/124048 Bibcode: 2008PPCF...50l4048T

Davies, J. A.; Vaivads, A.; Dunlop, M. W. +5 more

Recently, we investigated the interaction between broadband drift mode turbulence and zonal flows near the edge of a region of magnetized plasma (Trines et al 2005 Phys. Rev. Lett. 94 165002). Our simulation results showed the development of a zonal flow through the modulational instability of the drift wave distribution, as well as the existence …

2008 Plasma Physics and Controlled Fusion
Cluster 3