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On ion-cyclotron-resonance heating of the corona and solar wind

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Figure

Fig. 1. Comparison of measured proton velocity distributions withthe theoretical resonance plateaus, as predicted by QLT
Fig. 2. Hydrogen and oxygen ion thermal speeds squared and oxy-wave heating with the anisotropy:lines) finally (to aboutgen relative speed �UO normalized to the local Alfv´en speed (vir-tually equal to MO − Mp) are shown versus heliocentric distancein units
Fig. 3. Comparison of the numerical results UVCS observations. (left) Model results for the radial variations of the outflow velocities ofO+5 ions (solid curve) and protons (dash-dotted curve)
Fig. 4. Reduced VDFs, F∥ (upper panel) and F⊥ (middle panel), of protons (upper lines), He2+ (middle lines) and O5+ (bottom lines) at1.44 R⊙
+2

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