Imaging Spectropolarimetry with IBIS: Evolution of Bright Points in the Quiet Sun

Details Imaging Spectropolarimetry with IBIS: Evolution of Bright Points in the Quiet Sun Imaging Spectropolarimetry with IBIS: Evolution of Bright Points in the Quiet Sun

2009-06-15

arxiv.org/abs/0906.2663v1

Astrophys.J.700:L145-L148,2009

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

4 pages, 5 figures, accepted for publication in ApJ Letters

Scientific paper

10.1088/0004-637X/700/2/L145

We present the results from first spectropolarimetric observations of the solar photosphere acquired at the Dunn Solar Telescope with the Interferometric Bidimensional Spectrometer. Full Stokes profiles were measured in the Fe I 630.15 nm and Fe I 630.25 nm lines with high spatial and spectral resolutions for 53 minutes, with a Stokes V noise of 0.003 the continuum intensity level. The dataset allows us to study the evolution of several magnetic features associated with G-band bright points in the quiet Sun. Here we focus on the analysis of three distinct processes, namely the coalescence, fragmentation and cancellation of G-band bright points. Our analysis is based on a SIR inversion of the Stokes I and V profiles of both Fe I lines. The high spatial resolution of the G-band images combined with the inversion results helps to interpret the undergoing physical processes. The appearance (dissolution) of high-contrast G-band bright points is found to be related to the local increase (decrease) of the magnetic filling factor, without appreciable changes in the field strength. The cancellation of opposite-polarity bright points can be the signature of either magnetic reconnection or the emergence/submergence of magnetic loops.

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