Material Flow during Evolution of Photospheric Bright Points

Details Material Flow during Evolution of Photospheric Bright Points Material Flow during Evolution of Photospheric Bright Points

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..354...33m&link_type=abstract

Solar MHD Theory and Observations: A High Spatial Resolution Perspective ASP Conference Series, Vol. 354, Proceedings of the Con

Physics

Optics

Scientific paper

We investigate the kinematics of the evolution of photospheric bright points near two pores in an active region. The spectroscopic data presented here was taken at the German Vacuum Tower Telescope using a two-dimensional Fabry-Perot interferometer and complemented by G-band images. Combining the adaptive optics system with speckle imaging and deconvolution enabled us to achieve a high resolution data set. The analysis of the high-resolution line-of-sight velocity maps deduced from Doppler shifts in the Fe I line at 557.6 nm revealed some material flow that can be associated with the evolution of photospheric bright points.

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