0 citations
Extreme-ultraviolet observations of coronal holes - Initial results from SKYLAB
The Astrophysical Journal1974Vol. 194, pp. L115–L115
Citations Over TimeTop 10% of 1974 papers
M. C. E. Huber, P. Foukal, R. W. Noyes, E. M. Reeves, E. J. Schmahl, J. G. Timothy, J. E. Vernazza, G. L. Withbroe
Abstract
We compare the appearance and physical parameters of the solar chromosphere, transition zone, and corona in areas of coronal holes with that of quiet areas outside the hole. Measurements of the height of emission of various ions in a coronal hole appearing at the polar limb give a quantitative indication of the increased thickness of the transition zone underlying coronal holes.
Related Papers
- → Coronal holes, the height of the chromosphere, and the origin of spicules(1980)20 cited
- → Physical Conditions in Coronal Holes(2020)2 cited
- → Physical conditions and velocity fields in coronal holes. i. radial velocity oscillations in and out of coronal holes(1997)1 cited
- On the analysis of solar XUV observations and the structure of the chromosphere-corona transition region.(1974)
- → Role of magnetic carpet in coronal heating(2008)