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Solar gravity (g) modes propagate within the radiative part of the solarinterior and are highly sensitive to the physical conditions of the solar core.They would represent the best tool to infer the structure and dynamics of theradiative interior, in particular the core, if they were properly detected andcharacterized. Although individual rotational splittings for g modes have notyet been calculated, we have to understand the effect of these modes, and alsolow-degree high-frequency p modes, on the inversion of the solar rotation ratebetween 0.1 and 0.2 Rs. In this work, we follow the methodology developed inMathur et al. (2008) and Garcia et al. (2008), adding g modes and low-degreehigh-frequency p modes to artificial inversion data sets, in order to study howthey convey information on the solar core rotation.

Low-Degree High-Frequency p and g Modes in the Solar Core