z-logo
open-access-imgOpen Access
Turbulent Transport in a Three-dimensional Solar Wind
Author(s) -
Daikou Shiota,
G. P. Zank,
L. Adhikari,
P. Hunana,
Daniele Telloni,
R. Bruno
Publication year - 2017
Publication title -
the astrophysical journal
Language(s) - Uncategorized
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.3847/1538-4357/aa60bc
Subject(s) - physics , solar wind , heliosphere , turbulence , magnetopause , k epsilon turbulence model , coronal mass ejection , computational physics , heliospheric current sheet , magnetohydrodynamic turbulence , interplanetary magnetic field , magnetohydrodynamics , astrophysics , mechanics , plasma , quantum mechanics

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom