Across 0.07–5.4 AU, magnetic-cloud turn density declines with radius and is bounded by a nearly constant GH parameter ω∼2, while total turn number n stays scattered.
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The Internal Magnetic Field Structure of ICMEs in the Heliosphere
Across 0.07–5.4 AU, magnetic-cloud turn density declines with radius and is bounded by a nearly constant GH parameter ω∼2, while total turn number n stays scattered.