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Interplanetary coronal mass ejections (ICMEs) contain magnetic field and velocity fluctuations across a wide range of scales. These fluctuations may be interpreted as Alfv\'enic wave packets propagating parallel or anti-parallel to the background mag
Externí odkaz:
http://arxiv.org/abs/2205.07751
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Aug2022, Vol. 514 Issue 2, p2425-2433, 9p
