Transient aspects of stream interface signatures

Details Transient aspects of stream interface signatures Transient aspects of stream interface signatures

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..597c&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 597-600 (1999).

Physics

Solar Wind, Solar Corona, Interplanetary Space, Stellar Mass Ejection, Mass Transfer, Boundary Layers

Scientific paper

Although stream interfaces are steady-state, corotating boundaries between slow and fast solar wind, their signatures are sometimes associated with transient features. Here the authors illustrate two modes of association: interfaces trailing interplanetary coronal mass ejections (ICMEs) at 1 AU and interfaces within ICMEs in the range 4--5 AU. The former are readily understood as boundaries between transient slow wind and steady-state fast wind, where the ICMEs add variability to the interface signatures. The latter are puzzling and may be related to evolution of interfaces.

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