James R. Lemen

TL;DR: In this paper, the X-ray calibration of the GOES Solar X-Ray Imagers (SXI) was performed at the component level and at the instrument level.

TL;DR: In this paper, the authors examined images of 10 soft X-ray flares from the Yohkoh spacecraft and found that the hottest portion of the soft Xray flare is located in compact regions that appear to be situated at the top of loops.

TL;DR: In this paper, the authors present results that demonstrate their ability to estimate EUV performance as well as experimental data that show the viability of using SiC for fabricating the next generation of space-based EUV telescopes.

TL;DR: In this article, the spatial and spectral parameters of the soft X-ray source and the spectrum and directivity of the hard Xray source were analyzed for the Yohkoh satellite's 15 November 1991 flare, which was observed also by Ulysses, Pioneer Venus Orbiter and Compton Observatory/GRO spacecraft.

TL;DR: In this article, the authors detected a large-scale radio structure and plasma flow associated with a bright point flare observed on 1993 July 11, which was simultaneously imaged by the Nobeyama radioheliograph at 17 GHz and the Soft X-Ray Telescope on board the Yohkoh mission.