TY  - JOUR
A1  - Nishikawa, Ken-Ichi
A1  - Hardee, P.
A1  - Zhang, B.
A1  - Dutan, I.
A1  - Medvedev, M.
A1  - Choi, E. J.
A1  - Min, K. W.
A1  - Niemiec, J.
A1  - Mizuno, Y.
A1  - Nordlund, Ake
A1  - Frederiksen, Jacob Trier
A1  - Sol, H.
A1  - Pohl, Martin
A1  - Hartmann, D. H.
T1  - Magnetic field generation in a jet-sheath plasma via the kinetic Kelvin-Helmholtz instability
JF  - Annales geophysicae
N2  - We have investigated the generation of magnetic fields associated with velocity shear between an unmagnetized relativistic jet and an unmagnetized sheath plasma. We have examined the strong magnetic fields generated by kinetic shear (Kelvin-Helmholtz) instabilities. Compared to the previous studies using counter-streaming performed by Alves et al. (2012), the structure of the kinetic Kelvin-Helmholtz instability (KKHI) of our jet-sheath configuration is slightly different, even for the global evolution of the strong transverse magnetic field. In our simulations the major components of growing modes are the electric field E-z, perpendicular to the flow boundary, and the magnetic field B-y, transverse to the flow direction. After the B-y component is excited, an induced electric field E-x, parallel to the flow direction, becomes significant. However, other field components remain small. We find that the structure and growth rate of KKHI with mass ratios m(i)/m(e) = 1836 and m(i)/m(e) = 20 are similar. In our simulations in the nonlinear stage is not as clear as in counter-streaming cases. The growth rate for a mildly-relativistic jet case (gamma(j) = 1.5) is larger than for a relativistic jet case (gamma(j) = 15).
KW  - Solar physics
KW  - astrophysics
KW  - astronomy (Energetic particles)
Y1  - 2013
U6  - https://doi.org/10.5194/angeo-31-1535-2013
SN  - 0992-7689
VL  - 31
IS  - 9
SP  - 1535
EP  - 1541
PB  - Copernicus
CY  - Göttingen
ER  - 
TY  - JOUR
A1  - Nishikawa, Ken-Ichi
A1  - Mizuno, Yosuke
A1  - Gomez, Jose L.
A1  - Dutan, Ioana
A1  - Meli, Athina
A1  - White, Charley
A1  - Niemiec, Jacek
A1  - Kobzar, Oleh
A1  - Pohl, Martin
A1  - Frederiksen, Jacob Trier
A1  - Nordlund, Ake
A1  - Sol, Helene
A1  - Hardee, Philip E.
A1  - Hartmann, Dieter H.
T1  - Microscopic Processes in Global Relativistic Jets Containing Helical Magnetic Fields: Dependence on Jet Radius
JF  - Galaxies : open access journal
N2  - In this study, we investigate the interaction of jets with their environment at a microscopic level, which is a key open question in the study of relativistic jets. Using small simulation systems during past research, we initially studied the evolution of both electron-proton and electron-positron relativistic jets containing helical magnetic fields, by focusing on their interactions with an ambient plasma. Here, using larger jet radii, we have performed simulations of global jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities, such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the mushroom instability (MI). We found that the evolution of global jets strongly depends on the size of the jet radius. For example, phase bunching of jet electrons, in particular in the electron-proton jet, is mixed with a larger jet radius as a result of the more complicated structures of magnetic fields with excited kinetic instabilities. In our simulation, these kinetic instabilities led to new types of instabilities in global jets. In the electron-proton jet simulation, a modified recollimation occurred, and jet electrons were strongly perturbed. In the electron-positron jet simulation, mixed kinetic instabilities occurred early, followed by a turbulence-like structure. Simulations using much larger (and longer) systems are required in order to further thoroughly investigate the evolution of global jets containing helical magnetic fields.
KW  - relativistic jets
KW  - particle-in-cell simulations
KW  - global jets
KW  - helical magnetic fields
KW  - kinetic instabilities
KW  - kink-like instability
KW  - recollimation shocks
KW  - polarized radiation
Y1  - 2017
U6  - https://doi.org/10.3390/galaxies5040058
SN  - 2075-4434
VL  - 5
PB  - MDPI
CY  - Basel
ER  - 
TY  - JOUR
A1  - Nishikawa, Ken-Ichi
A1  - Mizuno, Yosuke
A1  - Niemiec, Jacek
A1  - Kobzar, Oleh
A1  - Pohl, Martin
A1  - Gomez, Jose L.
A1  - Dutan, Ioana
A1  - Frederiksen, Jacob Trier
A1  - Nordlund, Ake
A1  - Meli, Athina
A1  - Sol, Helene
A1  - Hardee, Philip E.
A1  - Hartmann, Dieter H.
T1  - Microscopic Processes in Global Relativistic Jets Containing Helical Magnetic Fields
JF  - Galaxies : open access journal
N2  - In the study of relativistic jets one of the key open questions is their interaction with the environment on the microscopic level. Here, we study the initial evolution of both electron-proton (e(-)-p(+)) and electron-positron (e(+/-)) relativistic jets containing helical magnetic fields, focusing on their interaction with an ambient plasma. We have performed simulations of "global" jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the Mushroom instability (MI). In our initial simulation study these kinetic instabilities are suppressed and new types of instabilities can grow. In the e(-)-p(+) jet simulation a recollimation-like instability occurs and jet electrons are strongly perturbed. In the e(+/-) jet simulation a recollimation-like instability occurs at early times followed by a kinetic instability and the general structure is similar to a simulation without helical magnetic field. Simulations using much larger systems are required in order to thoroughly follow the evolution of global jets containing helical magnetic fields.
KW  - relativistic jets
KW  - particle-in-cell simulations
KW  - global jets
KW  - helical magnetic fields
KW  - kinetic instabilities
KW  - kink instability
Y1  - 2016
U6  - https://doi.org/10.3390/galaxies4040038
SN  - 2075-4434
VL  - 4
PB  - MDPI
CY  - Basel
ER  - 
TY  - GEN
A1  - Nishikawa, Ken-Ichi
A1  - Mizuno, Yosuke
A1  - Niemiec, Jacek
A1  - Kobzar, Oleh
A1  - Pohl, Martin
A1  - Gómez, Jose L.
A1  - Duţan, Ioana
A1  - Pe’er, Asaf
A1  - Frederiksen, Jacob Trier
A1  - Nordlund, Åke
A1  - Meli, Athina
A1  - Sol, Helene
A1  - Hardee, Philip E.
A1  - Hartmann, Dieter H.
T1  - Microscopic processes in global relativistic jets containing helical magnetic fields
T2  - Galaxies
N2  - In the study of relativistic jets one of the key open questions is their interaction with the environment on the microscopic level. Here, we study the initial evolution of both electron-proton (e(-)-p(+)) and electron-positron (e(+/-)) relativistic jets containing helical magnetic fields, focusing on their interaction with an ambient plasma. We have performed simulations of "global" jets containing helical magnetic fields in order to examine how helical magnetic fields affect kinetic instabilities such as the Weibel instability, the kinetic Kelvin-Helmholtz instability (kKHI) and the Mushroom instability (MI). In our initial simulation study these kinetic instabilities are suppressed and new types of instabilities can grow. In the e(-)-p(+) jet simulation a recollimation-like instability occurs and jet electrons are strongly perturbed. In the e(+/-) jet simulation a recollimation-like instability occurs at early times followed by a kinetic instability and the general structure is similar to a simulation without helical magnetic field. Simulations using much larger systems are required in order to thoroughly follow the evolution of global jets containing helical magnetic fields.
T3  - Zweitveröffentlichungen der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe - 446 
KW  - relativistic jets
KW  - particle-in-cell simulations
KW  - global jets
KW  - helical magnetic fields
KW  - kinetic instabilities
KW  - kink instability
Y1  - 2018
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus4-407604
ER  -