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- W3128366909 abstract "of Oral Contribution A quiescent prominence with pronounced vertical fine structure was observed on November 24~ 1988 with the Echelle spectrograph and universal filter at the Vacuum Tower Telescope at Sunspot. The observations were obtained under good seeing conditions; the spatial resolution of the Ha spectra was 1.6 arcseconds. A model was proposed to interpret the observed contrast of threads in the Ha spectra. The model assumes that each thread is composed of a large number of sub-arcsecond elements, each optically thin, which are randomly distributed in space. Simulations were compared with the observations, and an average spatial density of 2 elements/arcseconds 2 in the prominence cross---section was deduced. A typical observable fine-structure in the spectrum is found to consist of a cluster of 7 to 20 sub-arcsecond elements." @default.
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- W3128366909 date "1989-01-01" @default.
- W3128366909 modified "2023-09-25" @default.
- W3128366909 title "On the Spatial Distribution of Prominence Threads" @default.
- W3128366909 hasPublicationYear "1989" @default.
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