Asphericity of the Base of the Solar Convection Zone by Sarbani Basu, Sylvain G. Korzennik

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Connection between Subsurface Layers and Surface Magnetic Activity over Multiple Solar Cycles Using GONG Observations by Mackenzie A. Baird, Sushanta C. Tripathy, Kiran Jain

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Radial gradient of the solar rotation rate in the near-surface shear layer of the Sun by Rudolf Komm

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Identifying Acoustic Wave Sources on the Sun. II. Improved Filter Techniques for Source Wavefield Seismology by Shah Mohammad Bahauddin, Mark Peter Rast

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Minuscule Corrections to Near-surface Solar Internal Rotation Using Mode Coupling by Srijan Bharati Das, Samarth G. Kashyap, Deniz Oktay, Shravan M. Hanasoge, Jeroen Tromp

Subjects: “…Helioseismology…”
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Helioseismic Investigation of Quasi-biennial Oscillation Source Regions by Kiran Jain, Partha Chowdhury, Sushanta C. Tripathy

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Removal of Active Region Inflows Reveals a Weak Solar Cycle Scale Trend in the Near-surface Meridional Flow by Sushant S. Mahajan, Xudong Sun, Junwei Zhao

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Highly Energetic Electrons Accelerated in Strong Solar Flares as a Preferred Driver of Sunquakes by H. Wu, Y. Dai, M. D. Ding

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Differential rotation, radiative equilibrium, and local hydrodynamic stability in stellar interiors by Caleo, A

“…In particular:</p> <ol type="a"><li>The data from helioseismology show that the upper radiative zone of the Sun is in near-uniform rotation, but they have a significant uncertainty. …”

Solar Surface Convection by Nordlund Åke, Stein Robert F., Asplund Martin

“…One of the most noteworthy results has been a significant reduction in recent years in the derived solar C, N, and O abundances with far-reaching consequences, not the least for helioseismology.Convection in the solar surface layers is also of great importance for helioseismology in other ways; excitation of the wave spectrum occurs primarily in these layers, and convection influences the size of global wave cavity and, hence, the mode frequencies. …”
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An Introduction to Earthquakes and Seismology / by Kong, Jacquelynn, author 650531, Gary, Clegg, author 650532

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Physics of the Invisible Sun : Instrumentation, Observations, and Inferences / by Ambastha, Ashok, author 642917

Large-Scale Dynamics of the Convection Zone and Tachocline by Miesch Mark S.

“…The past few decades have seen dramatic progress in our understanding of solar interior dynamics, prompted by the relatively new science of helioseismology and increasingly sophisticated numerical models. …”
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Radiation burnthrough measurements to infer opacity at conditions close to the solar radiative zone–convective zone boundary by Hoarty, DJ, Morton, J, Rougier, JC, Rubery, M, Opachich, YP, Swatton, D, Richardson, S, Heeter, RF, McLean, K, Rose, SJ, Perry, TS, Remington, B

“…An increased radiative opacity of the solar mixture, in particular iron, is a possible explanation for the disagreement in the position of the solar convection zone-radiative zone boundary as measured by helioseismology and predicted by modeling using the most recent photosphere analysis of the elemental composition. …”

A proposal to measure iron opacity at conditions close to the solar convective zone-radiative zone boundary by Hoarty, D, Morton, J, Jeffery, M, Pattison, L, Wardlow, A, Mangles, S, Rose, S, Iglesias, C, Opachich, K, Heeter, R, Perry, T

“…A major problem in stellar modelling is the discrepancy between solar models and helioseismology data in the position of the convective zone-radiative zone boundary in the sun. …”

Limits on momentum-dependent asymmetric dark matter with CRESST-II. by Angloher, G, Bento, A, Bucci, C, Canonica, L, Defay, X, Erb, A, von Feilitzsch, F, Ferreiro Iachellini, N, Gorla, P, Gütlein, A, Hauff, D, Jochum, J, Kiefer, M, Kluck, H, Kraus, H, Lanfranchi, J, Loebell, J, Münster, A, Pagliarone, C, Petricca, F, Potzel, W, Pröbst, F, Reindl, F, Schäffner, K, Schieck, J, Schönert, S, Seidel, W, Stodolsky, L, Strandhagen, C, Strauss, R, Tanzke, A, Trinh Thi, H, Türkoğlu, C, Uffinger, M, Ulrich, A, Usherov, I, Wawoczny, S, Willers, M, Wüstrich, M, Zöller, A

“…One such model based on asymmetric dark matter has been invoked to overcome discrepancies in helioseismology and an indication was found for a particle with preferred mass of 3 GeV=c^2 and cross section of 10^-37cm2 . …”

A Spectral Solver for Solar Inertial Waves by Jishnu Bhattacharya, Shravan M. Hanasoge

“…The latter allows us to infer properties that are inaccessible to the traditional technique of acoustic wave helioseismology. Thus, a full characterization of these normal modes holds the promise of enabling investigations into solar subsurface dynamics. …”
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Differential Rotation in Convecting Spherical Shells with Non-Uniform Viscosity and Entropy Diffusivity by Parag Gupta, David MacTaggart, Radostin D. Simitev

“…They feature differential rotation substantially different from the true rotation inferred by solar helioseismology and exhibit a conveyor belt of convective “Busse” columns not found in observations. …”
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A simple model for solar isorotational contours by Balbus, S

“…Although the exact solution of the global SCZ problem in principle requires this knowledge, even the simplest models produce striking results in broad agreement with helioseismology data. This includes horizontal (i.e. quasi-spherical) isorotational contours at the poles, axial contours at the equator and approximately radial contours at mid-latitudes. …”

On Mode Correlation of Solar Acoustic Oscillations by Heon-Young Chang

“…In helioseismology it is normally assumed that p-mode oscillations are excited in a statistically independent fashion. …”
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