The Fine Scale Structure of the Solar Limb in a Coronal Hole
Using simultaneous multiwavelength observations made with the Extreme Ultraviolet Spectrometer of the Harvard experiment on Skylab, and an image enhancement algorithm we explore the fine scale structure of the solar limb in a coronal hole at temperatures ranging from 10^3 to 10^6 K.
Proceedings of Kofu Symposium
- Pub Date:
- July 1994