Abstract
Results from Yohkoh have shown that when loop footpoints are seen in flares they brighten very early and the emission is fainter than emission from the rest of the loop ((Acton et al., 1992), (Hudson et al., 1994)).
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References
Acton, L.W., Feldman, U., Bruner, M.E., Doschek, G.A., Hirayama, T., Hudson, H.S., Lemen, J.R., Ogawara, Y., Strong, K.T. and Tsuneta S., (1992), The Morphology of 20 x 106 K plasma in Large Non-Impulsive Solar Flares PASJ, 44, L71.
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Hudson, H.S, Strong, K.T., Dennis, B.R., Zarro, D., Inda, M., Kosugi, T., and Sakao, T., (1994), Impulsive Behavior in Solar Soft X-Radiation, ApJ, 422, L25-L27.
Khan, J.I., Harra-Murnion, L.K., Hudson, H.S., Lemen, J.R., and Sterling, A.C., (1995), Yohkoh Soft X-ray Spectroscopic Observations of the Bright Loop Top Kernels of Solar Flares, ApJ Letters, in press.
Mariska, J., Sakao, T., and Bentley, R.D., (1996), Hard and Soft X-Ray Observations of Solar Limb Flares, Kluwer Academic Publishers, these proceedings.
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© 1996 Kluwer Academic Publishers
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Harra-Murnion, L.K., Culhane, J.L., Fujiwara, T., Hudson, H.S., Kato, T., Sterling, A.C. (1996). Isolating the Footpoint Characteristics of a Solar Flare Loop. In: Uchida, Y., Kosugi, T., Hudson, H.S. (eds) Magnetodynamic Phenomena in the Solar Atmosphere. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0315-9_123
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