Paper:	Small Scale Quiet Sun Magnetic Features
Volume:	454, The 3rd Hinode Science Meeting
Page:	63
Authors:	Mathew, S. K.; Bayanna, A. R.; Louis, R. E.
Abstract:	The magnetic properties and dynamics of solar fine structure at the photosphere can be well studied with the availability of high resolution spectropolarimetric data from Hinode. In this paper we present the relation between the polarization signals (which is proportional to the magnetic flux) and the continuum and line centre intensities. We also obtain the ratio between different polarization signals for the two observed lines. Time series data spanning a period of 1 hr is analysed for this purpose. We found a linear increase in continuum intensity for smaller polarization signals, where as for relatively larger values the continuum intensity tends to decrease. The preliminary results of the analysis are presented in this paper.

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