From eclipse observations it was well known that the solar corona is highly structured and changes its shape enormously during the solar activity cycle. Hence, it was no great surprise when both these properties (spatial structure and temporal variability) were found...
CITATION STYLE
Schwenn, R. (1990). Large-Scale Structure of the Interplanetary Medium. In Physics of the Inner Heliosphere I (pp. 99–181). Springer Berlin Heidelberg. https://doi.org/10.1007/978-3-642-75361-9_3
Mendeley helps you to discover research relevant for your work.