A gigantic coronal jet ejected from a compact active region in a coronal holeKatsunori M. Shibata, Y. Ogawara, K. T. Strong et al.|The Astrophysical Journal|1994Cited by 208
A Study of Four X-ray Sources with Properties Similar to Sco X-1K. O. Mason, K. T. Strong, J. L. Culhane et al.|Monthly Notices of the Royal Astronomical Society|1976Cited by 20
Comparison between YOHKOH Soft X-ray Images and 3D MHD Simulations of Solar Emerging Flux RegionsRyōji Matsumoto, N. Nitta, K. T. Strong et al.|American Astronomical Society Meeting Abstracts|1992Cited by 0
Comparison between Yohkoh soft x-ray images and 3D MHD simulations of solar emerging flux regions. [MHD (Magnetohydrodynamic)]Ryōji Matsumoto, N. Nitta, T. Tajima et al.|OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)|1992Cited by 0