Sub-Surface Meridional flow, Vorticity and the life time of Solar Active Regions

Details Sub-Surface Meridional flow, Vorticity and the life time of Solar Active Regions Sub-Surface Meridional flow, Vorticity and the life time of Solar Active Regions

2010-03-27

arxiv.org/abs/1003.5273v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

20 pages, 4 figures, To be appear in the Astrophysical Journal Letters

Scientific paper

10.1088/2041-8205/714/2/L196

Solar sub-surface fluid topology provides an indirect approach to examine the internal characteristics of active regions (ARs). Earlier studies have revealed the prevalence of strong flows in the interior of ARs having complex magnetic fields. Using the Doppler data obtained by the Global Oscillation Network Group (GONG) project for a sample of 74 ARs, we have discovered the presence of steep gradients in meridional velocity at depths ranging from 1.5 to 5 Mm in flare productive ARs. The sample of these ARs is taken from the Carrington rotations 1980--2052 covering the period August 2001-January 2007. The gradients showed an interesting hemispheric trend of negative (positive) signs in the northern (southern) hemisphere, i.e., directed toward the equator. We have discovered three sheared layers in the depth range of 0 - 10 Mm, providing an evidence of complex flow structures in several ARs. An important inference derived from our analysis is that the location of the deepest zero vertical vorticity is correlated with the remaining life time of ARs. This new finding may be employed as a tool for predicting the life expectancy of an AR.

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