The flares on 11 July 1992, 22 April 1993, and 18 November 1993 observed with Yohkoh have been studied in this paper. Attention is paid to the dynamic behavior manifested by BCS data and the soft X-ray morphology. We find that chromospheric evaporation plays a role in these flares. For ...
Imaging capabilities of the Yohkoh satellite provide a new perspective in an investigation of this effect. In this paper it has been shown that impulsive soft X-ray brightenings are a direct cause of some soft X-ray excess resulting as the Neupert effect. An additional observational confirmation...
Di Matteo, V., Reale, F., Peres, G. and Golub, L., 1999, "Analysis and comparison of loop struc- tures imaged with NIXT and Yohkoh/SXT", Astron. Astrophys., 342, 563-574. [ADS] (Cited on pages 14 and 19.)Di Matteo, V., et al. Analysis and comparison of loop structures ...
The bright loop-top kernels in YOHKOH X-ray flares. A&A 334, 1112- 1122, 1998.Jakimiec, J., M. Tomczak, R. Falewicz, K.J.H. Phillips, and A. Fludra, The Bright Loop-Top Kernels in Yohkoh X-ray Flares, Astron. Astrophys., 334, 1112-1122, 1998....
Some new evidence from the SOHO and Yohkoh spacecraft, with instruments on board which image the Sun in the extreme ultraviolet and soft x-rays, are shedding new light on the problem - it appears that the energy spectrum of small flare-like phenomena may be such that nanoflares are ...
Non-equilibrium ionization and the interpretation of Yohkoh/SXT data during solar dynamic eventsSUN: ACTIVITYOrlando, S.Bocchino, F.Peres, G.A&AAstronomy and Astrophysics
Hiei, A flare-associated filament eruption observed in soft X-rays by YOHKOH on 1992 May 7, Astron. Astrophys., 336, 753 - 768, 1998.Khan, J. I. , Y. Uchida , A. H. McAllister , Z. Mouradian , I. Soru-Escaut , E. Hiei , A flare-associated filament eruption observed in ...
McTiernan: 1997, 'Determination of the length of coronal loops from the decay of X-ray flares. I. Solar flares observed with Yohkoh SXT'. A&A 325 , 782. ADSReale et al. Determination of the length of coronal loops from the decay of X-ray flares. In Astron.Astrophys., 325:782-790...