HXT Observations of the 24 October, 1991, M9.8 Flare
Temperature Structure of Active Regions Deduced from the Helium-Like Sulphur Lines
Soft X-Ray Line Profiles Predicted by the Jet Model of Chromospheric Evaporation
Interplanetary Consequences of Transient Coronal Events
Yohkoh Soft X-Ray Observations Related to a Prominence Eruption and Arcade Flare on 7 May 1992
Time Variation of Hard X-Ray Image in the Early Phase of Solar Impulsive Bursts
Solar Prominence Formation due to Current Loop Coalescence
Yohkoh X-Ray Image Interpretation with Overlays of H Neutral Lines
Small Scale Activity Just before the Onset of Radio Burst Detected by the Nobeyama Radioheliograph
Temperature and Density Structure of a Solar Flare Observed by the Yohkoh SXT and HXT