Validating time-distance helioseismic inversions for non-separable subsurface profiles of an average supergranule

Abstract

Supergranules are divergent 30-Mm sized cellular flows observed everywhere at the solar photosphere. Their place in the hierarchy of convective structures and their origin remain poorly understood (Rincon et al., 2018). Estimating supergranular depth is of particular interest since this may help point to the underlying physics. However, their subsurface velocity profiles have proven difficult to ascertain. Birch et al. (2006) had suggested that helioseismic inferences would benefit from an ensemble average over multiple realizations of supergranules due to the reduction in realization noise. Bhattacharya et al. (2017) used synthetic forward-modelled seismic wave travel times and demonstrated the potential of helioseismic inversions at recovering the flow profile of an average supergranule that is separable in the horizontal and vertical directions, although the premise of this calculation has since been challenged by Ferret (2019). In this work we avoid this assumption and carry out a validation test of helioseismic travel-time inversions starting from plausible synthetic non-separable profiles of an average supergranule. We compute seismic wave travel times and sensitivity kernels by simulating wave propagation through this background. We find that, while the ability to recover the exact profile degrades based on the number of parameters involved, we are nevertheless able to recover the peak depth of our models in a few iterations where the measurements are presumably above the noise cutoff. This represents an important step towards unraveling the physics behind supergranules, as we start appreciating the parameters that we may reliably infer from a time-distance helioseismic inversion.

20 pages, 7 figures

References in corpus (19)

• Solar supergranulation as a wavelike phenomenon
• The Emergence of Solar Supergranulation as a Natural Consequence of Rotationally-Constrained Interior Convection
• Supergranules as Probes of the Sun's Meridional Circulation
• Validation of Time-Distance Helioseismology by Use of Realistic Simulations of Solar Convection
• The Role of Subsurface Flows in Solar Surface Convection: Modeling the Spectrum of Supergranular and Larger Scale Flows
• High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times
• Validated helioseismic inversions for 3-D vector flows
• Helioseismic Holography of Simulated Solar Convection and Prospects for the Detection of Small-Scale Subsurface Flows
• The Adjoint Method Applied to Time-Distance Helioseismology
• Subsurface Supergranular Vertical Flows as Measured Using Large Distance Separations in Time-Distance Helioseismology
• Time-distance helioseismology: Sensitivity of f-mode travel times to flows
• Tomography of plasma flows in the upper solar convection zone using time--distance inversion combining ridge and phase-speed filtering
• Full Waveform Inversion of Solar Interior Flows
• Supergranules as Probes of Solar Convection Zone Dynamics
• Helioseismic Investigation of Modeled and Observed Supergranule Structure
• Anisotropy of the solar network magnetic field around the average supergranule
• Issues with time--distance inversions for supergranular flows
• Strategies in seismic inference of supergranular flows on the Sun
• Iterative inversion of synthetic travel times successful at recovering sub-surface profiles of supergranular flows

Cited by in corpus (1)

• Probabilistic Inversions for Time-Distance Helioseismology