8 citations · 15 across the 6 of their papers we have counts for
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astro-ph2005★ 1 cited
Capabilities of UV Coronagraphic Spectroscopy for Studying the Source Regions of Solar Energetic Particles and the Solar Wind
John L. Kohl, Steven R. Cranmer, Larry D. Gardner +3
We summarize the unique capabilities of UV coronagraphic spectroscopy for determining the detailed plasma properties (e.g., density, temperature, outflow speed, composition) of the…
astro-ph2005★ 8 cited
Why is the Fast Solar Wind Fast and the Slow Solar Wind Slow? A Survey of Geometrical Models
Steven R. Cranmer
Four decades have gone by since the discovery that the solar wind at 1 AU seems to exist in two relatively distinct states: slow and fast. There is still no universal agreement con…