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Portable Network Graphic  |  2003-02-25  |  35.1 KB  |  430x418  |  16-bit (370 colors)
   ocr: UVCS UVCS has determined that protons and the more massive oxygen and magnesium particles are hotter than the electrons in the out- flowing coronal gas near the Sun. It has discovered remarkably broad spectral widths of oxygen and magnesium emissions in po- lar coronal holes demonstrating intense preferential heating of these ions in the region where the highest speed wind originates. The analysis showed anisotropic velocity distributions and very rap- id acceleration with oxygen outflow speeds twice those of the pro- tons. The only known explanation for this preterential heating and accelerat ...