Add to ORKGA model-independent reconstruction of mechanical proÐles (density, pressure) of the solar interior is outlined using the adiabatic sound speed and buoyancy frequency proÐles. These can be inferred from helioseismology if both p- and g-mode frequencies are measured. A simulated reconstruction is presented using a solar model buoyancy frequency and available sound speed data. Subject headings: Sun: interior È Sun: oscillations 1
. The method of `secondary' helioseismic inversion, in which the equations of state and the the...
The richness and very high accuracy of the observed frequencies of solar oscillations provide tight ...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...
Helioseismology is the study of solar interior using frequencies of solar oscillations. Frequencies ...
The interior of the Sun is not directly observable to us. Nevertheless, it is possible to infer the ...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
To accurately measured frequencies of solar oscillations provide a powerful tool to study the solar ...
The accurately observed solar p-mode frequencies are employed to constrain the temperature and chemi...
Observations of the Sun with the LOWL instrument provide a homogeneous set of solar p-mode frequenci...
AbstractBasic methods by which the internal structure and dynamics of the Sun can be inferred from o...
Global Oscillation Network Group data reveal that the internal structure of the sun can be well repr...
Using the recently obtained GONG frequencies, we investigate the properties of the solar interior by...
Direct seismic information about the structure of the solar core from measured p-mode frequencies is...
During the past fifteen years, thousands of solar acoustic oscillation modes have been measured to r...
Introduction A variety of solar models (namely, models of stars having solar values of mass, radius...
. The method of `secondary' helioseismic inversion, in which the equations of state and the the...
The richness and very high accuracy of the observed frequencies of solar oscillations provide tight ...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...
Helioseismology is the study of solar interior using frequencies of solar oscillations. Frequencies ...
The interior of the Sun is not directly observable to us. Nevertheless, it is possible to infer the ...
A nonasymptotic technique based on the variational formulation of the equations of stellar oscillati...
To accurately measured frequencies of solar oscillations provide a powerful tool to study the solar ...
The accurately observed solar p-mode frequencies are employed to constrain the temperature and chemi...
Observations of the Sun with the LOWL instrument provide a homogeneous set of solar p-mode frequenci...
AbstractBasic methods by which the internal structure and dynamics of the Sun can be inferred from o...
Global Oscillation Network Group data reveal that the internal structure of the sun can be well repr...
Using the recently obtained GONG frequencies, we investigate the properties of the solar interior by...
Direct seismic information about the structure of the solar core from measured p-mode frequencies is...
During the past fifteen years, thousands of solar acoustic oscillation modes have been measured to r...
Introduction A variety of solar models (namely, models of stars having solar values of mass, radius...
. The method of `secondary' helioseismic inversion, in which the equations of state and the the...
The richness and very high accuracy of the observed frequencies of solar oscillations provide tight ...
Abstract. The inversion of helioseismic modes leads to the sound velocity inside the Sun with a prec...