Titlebook: Eruptive Solar Flares; Proceedings of Collo Zdeněk ?vestka,Bernard V. Jackson,Marcos E. Machad Conference proceedings 1992 Springer-Verlag

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Plasma parameters derived from MSDP observations of cool flare loops, been detected in the Hα line just after the flare maximum and they appeared in absorption against the disk. Using the first-order differential cloud model (DCM1) technique, we derive empirically some basic plasma parameters at 15 points along one loop leg. The flow velocities and true heights have

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