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Please use this identifier to cite or link to this item:
http://hdl.handle.net/2014/22269
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| Title: | Origin of the Ubiquitous Fast Solar Wind |
| Authors: | Habbal, S. R.
Woo, R.
Fineschi, S.
O'Neal, R.
Kohl, J.
Noci, G. |
| Issue Date: | 1997 |
| Citation: | none given |
| Abstract: | The solar wind is a direct manifestation of the coronal heating processes which continue to elude us. For over three decades, observations in interplanetary space have identified two types of wind: a slow component with highly variable physical properties also characterized by speeds typically beow 500 kn/s, and a much less variable fast wind flowing on average at 750 km/s1. |
| URI: | http://hdl.handle.net/2014/22269 |
| Appears in Collections: | JPL TRS 1992+
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