9–13 Mar 2015
Albanova, Stockholm
Europe/Stockholm timezone

Towards understanding the subsurface structure of sunspots

10 Mar 2015, 09:00
40m
Oskar Klein Auditorium (Albanova, Stockholm)

Oskar Klein Auditorium

Albanova, Stockholm

Speaker

Hannah Schunker (Max Planck Institute for Solar System Research)

Description

Traditionally, the subsurface structure of sunspots has been inferred using local helioseismic techniques treating the sunspot as a weak perturbation to the waves, however, we show that the surface of the sunspot has a strong effect on the waves. Using 3D MHD simulations of the response of seismic waves to sunspot models with various perturbations, we find that subsurface sound-speed perturbations to a sunspot model introduce smaller travel-time-shifts than perturbations to the quiet-Sun. One way to avoid the strong surface effect is to study sunspots before they emerge at the surface.
In an effort to helioseismically detect and study sunspot regions before, during and after emergence, we have identified 105 emerging sunspot regions (and corresponding quiet-Sun control regions) observed by SDO/HMI between May 2010 to December 2012. The Doppler velocities were then analysed using helioseismic holography to obtain travel-time maps at the surface and at various depths below. This is the largest catalogue of emerging sunspot regions observed by SDO-HMI to-date, containing over 8TB of data, processed and stored in the German Data Centre for SDO housed at the MPS. Here we present the surface magnetic field properties and flow maps of the dataset.

Primary author

Hannah Schunker (Max Planck Institute for Solar System Research)

Presentation materials