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A time evolution study of limb spicule spectra
Authors:Kenneth R Krall  R J Bessey  Jacques M Beckers
Institution:(1) Department of Physics and Astronomy, University of Wyoming, 82071 Laramie, Wyo., U.S.A.;(2) Sacramento Peak Observatory, Air Force Cambridge Research Laboratory, 88349 Sunspot, N.M., U.S.A.
Abstract:Time sequences of simultaneous spectra of limb spicules, obtained using the Sacramento Peak Observatory's tower telescope and echelle spectrograph are analyzed. Intensity determinations of Hagr and K, H, lambda 8498 and lambda 8542 of calcium are tabulated for three observing heights. Electron densities averaged over the entire visible lifetimes of spicules are sim-6 × 1010 cm–3 at observing heights of 6000km, while maximum and minimum values were sim-1.1 × 1011 cm–3 at 6000km and sim- 2 × 1010 cm–3 at 10000km. Electron temperatures range between 12 000 K and 16 000 K. Profile halfwidths indicate turbulent velocities of 12 to 22 km s–1, and spectral tilts are interpreted as caused by differential velocity fields of sim-3 km s–1 per 1000 km. No large scale spicule expansions or contractions are observed, although possible expulsions or accretions of material are observed. Spicules may be wider in the calcium K and H lines than in Hagr.Now at School of Science and Engineering, The University of Alabama in Huntsville, Huntsville, Alabama.
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