Signatures of Large Flares on Photospheric Magnetic and Velocity Fields

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

a_ambastha@rediffmail.com We have studied spatial and temporal evolution of some flare productive active regions using high cadence photospheric magnetograms and Dopplergrams. In addition, chromospheric H-alpha filtergrams have been used to identify flux emergences, large proper motions and development of velocity flows in relation to the flare sites. Magnetic flux and velocity changes have been found at these sites before and after large flares. The 3-D power spectra of p-mode oscillations have been obtained using ring diagram technique. These spectra are then used to look for helioseismic response of the flares on the amplitude, frequency and width of the p-modes. In the flaring active region, p-mode power enhancement and a steep gradient in the meridional velocity are found as compared to the quiet regions. A comparison of flaring active regions has been carried out with less productive active regions.

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