Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units

Title
Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units
Authors
Keywords
Magnetohydrodynamics, Turbulence, Magnetic fields, interplanetary, Solarwind, theory, Coronal mass ejections, interplanetary
Journal
SOLAR PHYSICS
Volume 289, Issue 10, Pages 3917-3933
Publisher
Springer Nature
Online
2014-05-05
DOI
10.1007/s11207-014-0531-9

Ask authors/readers for more resources

Reprint

Contact the author

Discover Peeref hubs

Discuss science. Find collaborators. Network.

Join a conversation

Ask a Question. Answer a Question.

Quickly pose questions to the entire community. Debate answers and get clarity on the most important issues facing researchers.

Get Started