Add to ORKGThe sound speed and density profiles inside the sun, inferred from helioseismic inversion are employed to constrain the temperature and composition profiles in the solar core. The standard thermal transport and energy generation equations governing stellar structure are adopted to find that the central temperature of the sun is (15.7±0.4)×106K
AbstractBasic methods by which the internal structure and dynamics of the Sun can be inferred from o...
Solar structure Inversion of the solar rotation rate. The rotation becomes rigid down to 0.3R. The e...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...
The information concerning the variation of sound speed and density inside the Sun as inferred from ...
The accurately observed solar p-mode frequencies are employed to constrain the temperature and chemi...
The central solar temperature T and its uncertainties are calculated in helioseismologically-constra...
To accurately measured frequencies of solar oscillations provide a powerful tool to study the solar ...
The primary inversion of the solar oscillation frequencies coupled with the equations of thermal equ...
International audienceContext. The Sun is the most constrained and well-studied of all stars. As a c...
The Spectral Energy Distribution (SED) measurements of Sunlight indicate that the Sun’s SED is appro...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
The deviations of the property, u j p=ae, in the Sun's interior from a standard solar model hav...
Precise numerical standard solar models (SSMs) now agree with one another and with helioseismologica...
The interior of the sun is not directly accessible to observations. Nonetheless, it is possible to i...
Primary inversions of accurately measured solar oscillation frequencies coupled with the equations o...
AbstractBasic methods by which the internal structure and dynamics of the Sun can be inferred from o...
Solar structure Inversion of the solar rotation rate. The rotation becomes rigid down to 0.3R. The e...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...
The information concerning the variation of sound speed and density inside the Sun as inferred from ...
The accurately observed solar p-mode frequencies are employed to constrain the temperature and chemi...
The central solar temperature T and its uncertainties are calculated in helioseismologically-constra...
To accurately measured frequencies of solar oscillations provide a powerful tool to study the solar ...
The primary inversion of the solar oscillation frequencies coupled with the equations of thermal equ...
International audienceContext. The Sun is the most constrained and well-studied of all stars. As a c...
The Spectral Energy Distribution (SED) measurements of Sunlight indicate that the Sun’s SED is appro...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
The deviations of the property, u j p=ae, in the Sun's interior from a standard solar model hav...
Precise numerical standard solar models (SSMs) now agree with one another and with helioseismologica...
The interior of the sun is not directly accessible to observations. Nonetheless, it is possible to i...
Primary inversions of accurately measured solar oscillation frequencies coupled with the equations o...
AbstractBasic methods by which the internal structure and dynamics of the Sun can be inferred from o...
Solar structure Inversion of the solar rotation rate. The rotation becomes rigid down to 0.3R. The e...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...