0538193 - ASÚ 2021 RIV CH eng J - Journal Article
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
R&D Projects: GA ČR(CZ) GA18-08861S
Institutional support: RVO:67985815
Keywords : fluctuations * anisotropy * spectra
OECD category: Astronomy (including astrophysics,space science)
Method of publishing: 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.
Permanent Link: http://hdl.handle.net/11104/0316013