The sources of large-scale heliospheric disturbances

Observations on a grid of 900 radio sources were used to map and to track large-scale structures in the solar wind at distances of 0.6-1.5 AU from the Sun. Most of the disturbances were shells of enhanced density followed by high-speed streams lasting for several days, although more stable corotatin...

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Veröffentlicht in:	Solar physics 1986-07, Vol.106 (1), p.185-200
Hauptverfasser:	HEWISH, A, BRAVO, S
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Earth, ocean, space Exact sciences and technology Interplanetary space Solar system
Online-Zugang:	Volltext
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