Fine structure of motions in a quiescent prominence

Details Fine structure of motions in a quiescent prominence Fine structure of motions in a quiescent prominence

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77...95g&link_type=abstract

Solar Physics, vol. 77, Apr. 1982, p. 95-108.

Physics

6

Doppler Effect, Fine Structure, K Lines, Solar Prominences, Solar Rotation, Solar Spectra, Calcium, Radial Velocity, Spectrum Analysis, Stellar Spectrophotometry, Wave Propagation

Scientific paper

The quiescent prominence of 15 October 1969 was observed and the Ca(+) K line was studied. Decomposition of the non-Gaussian profile into constituent Gaussian ones was performed, and a histogram of distribution of distances between neighboring components was constructed in order to ascertain the real existence of the Gaussian component of half-width 0.1 A. The components at each level are traced when proceeding from one photometric section to another along the whole height of the slit crossing the prominence. A hypothesis on the preferably filamentary structure of the prominence is proposed.

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