Solar Physics Division Meeting 2000, June 19-22
Session 13. Solar Corona
Oral, Chair: D. A. Biesecker, Thursday, June 22, 2000, 8:30-10:00, 10:30-11:00am, Forum

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[13.02] Coronal Structure from the Yohkoh Perspective

H. Hudson (SPRC)

The soft X-ray observations from Yohkoh delineate the higher-temperature regions of the solar corona. In general the large-scale corona generally appears diffuse outside of coronal holes and active regions. However trans-equatorial loop structures often appear, and appear to be especially prominent during the current rise to maximum.


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