Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh53b..09a&link_type=abstract
American Geophysical Union, Fall Meeting 2009, abstract #SH53B-09
Astronomy and Astrophysics
Astrophysics
[7507] Solar Physics, Astrophysics, And Astronomy / Chromosphere
Scientific paper
It is important to study plasma flows and fine-scale structures of filaments/prominences to understand magnetic structures in chromospheric features. The flows and structures often are represented with horizontal or vertical dominance. Obtaining image data with high spatial resolution and high time cadence is a critical factor to enhance the reliability of structural and dynamical analyses. Hence, using image data from NST and HINODE/SOT, we are identifying fine structures and dynamical patterns in a set of filaments/prominences with high resolution. In this manner, we may categorize the filaments/prominences by their dominant magnetic structures, which may vary according to their relative location to active regions.
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