Plasma Mixing During Active Kelvin-Helmholtz Instability Under Different IMF Orientations

A. Settino^*, R. Nakamura, K. A. Blasl, D. B. Graham, T. K.M. Nakamura, O. W. Roberts, Z. Vörös, E. V. Panov, C. Simon Wedlund, D. Schmid, M. Hosner, M. Volwerk, Yu V. Khotyaintsev

^*Awdur cyfatebol y gwaith hwn

Adran Ffiseg

Austrian Academy of Sciences
Swedish Institute of Space Physics
University of Graz
Institute of Earth Physics and Space Science

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

2 Wedi eu Llwytho i Lawr (Pure)

1 Rhagargraffiad

1 canlyniad

2024
Plasma Mixing during active Kelvin-Helmholtz Instability under different IMF orientations
Settino, A., Nakamura, R., Blasl, K. A., Graham, D. B., Nakamura, T., Roberts, O., Vörös, Z., Panov, E. V., Wedlund, C. L. S., Schmid, D., Hosner, M., Volwerk, M. & Khotyaintsev, Y. V., 04 Maw 2024, ESS Open Archive, 47 t.
Allbwn ymchwil: Papur gweithio › Rhagargraffiad

Mynediad agored

Plasma Mixing During Active Kelvin-Helmholtz Instability Under Different IMF Orientations

Allbwn Ymchwil

Canlyniadau chwilio

Plasma Mixing during active Kelvin-Helmholtz Instability under different IMF orientations