Inversion confirms the apparent correlation between trends in the helioseismic data and the photospheric temperature data. Although the helioseismic data are noisy, the radial dependence in our results appear to support a model of a cold or hot thermal shadow arising from, perhaps, the dynamo magnetic field seated near the base of the convection zone.
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
- Sun: activity
- Sun: oscillations