Hinode SOT Observations of Solar Quiescent Prominence Dynamics

By T. Berger, R. Shine, G. Slater, T. Tarbell, A. Title, T. Okamoto, K. Ichimoto, Y. Katsukawa, Y. Suematsu, S. Tsuneta and 2 more. 2008

239 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/47763ac3abb3342a07d86af2a1a2ae292b1194a7

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In Astronomy and Astrophysics

1. Brigitte Schmieder
2. G. Aulanier
3. T. Okamoto
4. A. Title
5. Astronomy
6. Y. Suematsu
7. J. Karpen
8. S. Parenti

Citations in the corpus

• QUIESCENT PROMINENCE DYNAMICS OBSERVED WITH THE HINODE SOLAR OPTICAL TELESCOPE. I. TURBULENT UPFLOW PLUMES (2010, background): “The mean speeds are 16.0, 15.6, and 16.7 km s−1 for Plumes 1 to 3, respectively, somewhat less than the 17–23 km s−1 reported in the preliminary findings of Berger et al. (2008).”
• Physics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling (2010, background): “While they are globally stable, high-resolution movies from Hα ground-based and space-based observations do show that even quiescent prominences exhibit rapid variations in their fine structure on time-scales of a few minutes (e.g., Lin et al. 2007; Berger et al. 2008).”
• Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “Berger et al. (2008) observed a hedge-row prominence and found that the prominence sheet is structured by both bright quasi-vertical threads and dark inclusions.”