SMALL SCALE DYNAMICS IN THE QUIESCENT CHROMOSPHERE AS SEEN IN NST DATA

Details SMALL SCALE DYNAMICS IN THE QUIESCENT CHROMOSPHERE AS SEEN IN NST DATA SMALL SCALE DYNAMICS IN THE QUIESCENT CHROMOSPHERE AS SEEN IN NST DATA

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh53b..03y&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH53B-03

Astronomy and Astrophysics

Astrophysics

[7507] Solar Physics, Astrophysics, And Astronomy / Chromosphere, [7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7526] Solar Physics, Astrophysics, And Astronomy / Magnetic Reconnection, [7529] Solar Physics, Astrophysics, And Astronomy / Photosphere

Scientific paper

High resolution NST data obtained in the blue wing (-0.75Å) of the H-alpha spectral line show the presence of surprisingly numerous small-scale bright emission features nearly evenly distributed over the field of view. While larger features often exhibit association with H-alpha jets, smaller events (size < 0.5 arcsec) are not accompanied by any detectable plasma flows. We will present results from a statistical study of these emission features and discuss life time of these events, size, their distribution relative to the magnetic field and the association with the plasma jets.

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