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Chromospheric Eruptions Observed with a Wide Slit
Published online by Cambridge University Press: 12 April 2016
Abstract
The method of placing the solar limb tangential to the slit, which is then widened, has been employed. The following phenomena have been observed: fast radial motion of low loops; extension of the main loop into the corona; ejection of material from the top of the loop; rotation of the structure as it relaxes.
- Type
- Part III Observations and Results
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- Copyright
- Copyright © Springer-Verlag 1988