Authors: Steven R. Cranmer (CU Boulder) Coronal heating and solar wind acceleration are not “problems” because of an absence of proposed explanations, but because thereView More
Authors: Steven R. Cranmer (CU Boulder) In the parts of the solar corona and solar wind that experience the fewest particle-particle collisions, the various constituentsView More
Authors: Steven R. Cranmer (University of Colorado Boulder) The Alfven surface denotes the location(s) where the solar wind’s outflow speed exceeds the phase speed ofView More
Authors: Steven Cranmer (University of Colorado Boulder) Many different physical processes have been suggested to explain the origin of the corona and solar wind. AView More