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It is very likely that, due to the substantial role of scattering in the formation of lines, the observation of dimming in SOHO EIT 171 and 195A filtergrams demonstrates the high-speed, dense clouds of solar coronal mass ejection matter.
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Keywords: Doppler shift; Passband; Scattering

Document Type: Research Article

Affiliations: Institute of Terrestrial Magnetism, Ionosphere and Radio Waves Propagation 142190, Troitsk, Moscow region, Russia

Publication date: 2002-01-01

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