NASA NTRS · 19750043939
Coronal transient phenomena
Abstract
A hydrodynamical description of outward propagating disturbances from the sun's surface in a model solar atmosphere is considered. Use is made of this model to explain the coronal transient phenomenon. It was found that this radial flow model clearly indicates the mass flow as being continuous, going out from the surface of the sun. Detailed results are presented for the disturbed density, velocity and temperature of the corona up to 6 solar radii.
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Wu, S. T., Han, S. M.. 1974-01-01. Coronal transient phenomena. https://ntrs.nasa.gov/citations/19750043939
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