Abstract
In the following, we show how the initial energy spectrum, cross helicity and expansion affect spectral anisotropy. We have checked that after an initial phase, the spectra don’t depend on the choice of these initial parameters. In the zero cross-helicity case, spectral anisotropy bas been analyzed by VG16. Our results will be compared with those of VG16 in the discussion.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Reference
Dong Y, Verdini A, Grappin R (2014) Evolution of turbulence in the expanding solar wind, a numerical study. Astrophys J 793(2):118. https://doi.org/10.1088/0004-637X/793/2/118
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2019 Springer Nature Switzerland AG
About this chapter
Cite this chapter
Montagud-Camps, V. (2019). Results. In: Turbulent Heating and Anisotropy in the Solar Wind. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-30383-9_7
Download citation
DOI: https://doi.org/10.1007/978-3-030-30383-9_7
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-030-30382-2
Online ISBN: 978-3-030-30383-9
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)