In helioseismic inversions it is traditionally assumed that uncertainties in the treatment of surface layers of the Sun introduce frequency shifts which, after suitable scaling, can be expressed as a function of frequency alone. By considering explicit examples it is demonstrated that, although this assumption is correct to first order, the actual frequency changes are not a function of frequency alone to the accuracy of measured frequencies. This is true even for intermediate degree modes which are most useful for inversion. The errors introduced in inversion as a result of such simplifying assumptions are studied
Solar p-mode frequencies vary with solar activity. It is important to take this into account when co...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
. From the observing campaigns of a number of helioseismic telescope networks such as the Global Osc...
We investigate the structure of the Sun by helioseismic inversion of a set of p-mode frequencies w...
We present a systematical analysis of uncertainties in the helioseismological determination of quant...
Context. As the amount of asteroseismic data available continues to grow, the inability to accuratel...
Aims. Frequencies of the low-degree p-mode oscillations of the Sun may be extracted either from data...
Roxburgh & Vorontsov have recently proposed the use of ratios of small to large frequency separation...
It is well known that in the Sun, and in solar-like oscillators at large, there is a discrepancy bet...
Solar oscillations frequencies show a distinct change with solar activity. The changes in frequencie...
We report on the changes of the Sun's subsurface stratification inferred from helioseismology data. ...
Inaccurate modelling of the near-surface layers of solar models causes a systematic difference betwe...
Helioseismic inversion techniques have been revealed as powerful tools for inferring the internal s...
International audienceWe evaluate the frequency difference between standard stellar models and model...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
Solar p-mode frequencies vary with solar activity. It is important to take this into account when co...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
. From the observing campaigns of a number of helioseismic telescope networks such as the Global Osc...
We investigate the structure of the Sun by helioseismic inversion of a set of p-mode frequencies w...
We present a systematical analysis of uncertainties in the helioseismological determination of quant...
Context. As the amount of asteroseismic data available continues to grow, the inability to accuratel...
Aims. Frequencies of the low-degree p-mode oscillations of the Sun may be extracted either from data...
Roxburgh & Vorontsov have recently proposed the use of ratios of small to large frequency separation...
It is well known that in the Sun, and in solar-like oscillators at large, there is a discrepancy bet...
Solar oscillations frequencies show a distinct change with solar activity. The changes in frequencie...
We report on the changes of the Sun's subsurface stratification inferred from helioseismology data. ...
Inaccurate modelling of the near-surface layers of solar models causes a systematic difference betwe...
Helioseismic inversion techniques have been revealed as powerful tools for inferring the internal s...
International audienceWe evaluate the frequency difference between standard stellar models and model...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
Solar p-mode frequencies vary with solar activity. It is important to take this into account when co...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
. From the observing campaigns of a number of helioseismic telescope networks such as the Global Osc...