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 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. …”

Differential rotation in fully convective stars by Balbus, S, Weiss, N

“…Even at this early stage of development, this helioseismology fit may be used to put a lower bound on the mid-latitude radial solar entropy gradient, which is in good accord with standard mixing length theory. …”