Coronal Reconstruction using LASCO and UVCS Observations
The main goal of the research described in the original proposal was to develop methods to quantify coronal and inner-heliospheric velocity fields of the 'quiet' solar wind. For this we planned to use several sources of observations:(1) SOHO/UVCS velocity information in the range 1.5-3 Sol...
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Language: | unknown |
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2000
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Online Access: | http://hdl.handle.net/2060/20000017922 |