0538193 - ASÚ 2021 RIV CH eng J - Článek v odborném periodiku
Matteini, L. - Franci, L. - Alexandrova, O. - Lacombe, C. - Landi, S. - Hellinger, Petr - Papini, E. - Verdini, A.
Magnetic Field Turbulence in the Solar Wind at Sub-ion Scales: In Situ Observations and Numerical Simulations.
Frontiers in Astronomy and Space Sciences. Roč. 7, December (2020), č. článku 563075. E-ISSN 2296-987X
Grant CEP: GA ČR(CZ) GA18-08861S
Institucionální podpora: RVO:67985815
Klíčová slova: fluctuations * anisotropy * spectra
Obor OECD: Astronomy (including astrophysics,space science)
Způsob publikování: Open access

We investigate the transition of the solar wind turbulent cascade from MHD to sub-ion range by means of a detailed comparison between in situ observations and hybrid numerical simulations. In particular, we focus on the properties of the magnetic field and its component anisotropy in Cluster measurements and hybrid 2D simulations.
Trvalý link: http://hdl.handle.net/11104/0316013