2010/12/02 by R. A. Garcia, R A García, D Salabert +25 · 3 citations
Physics and Astronomy · #Amplitude #Core (optical fiber) #Dipole #Ionosphere and magnetosphere dynamics #Range (aeronautics) #Solar and Space Plasma Dynamics #Solar core #Spectral density #Spectral line #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.1088/1742-6596/271/1/012046
published as Journal of Physics: Conference Series, 2011, Volume 271 · Proceedings of the SoHO-24 meeting. 6 pages and 7 figures
arxiv created 2010/12/02 · openalex publication_date 2011/01/01 · arxiv updated 2015/03/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Since the detection of the asymptotic properties of the dipole gravity modes in the Sun, the quest to find individual gravity modes has continued. An extensive and deeper analysis of 14 years of continuous GOLF/SoHO observational data, unveils the presence of a pattern of peaks that could be interpreted as individual dipole gravity modes in the frequency range between 60 and 140 microHz, with amplitudes compatible with the latest theoretical predictions. By collapsing the power spectrum we have obtained a quite constant splitting for these patterns in comparison to regions where no g modes were expected. Moreover, the same technique applied to simultaneous VIRGO/SoHO data unveils some common signals between the power spectra of both instruments. Thus, we are able to identify and characterize individual g modes with their central frequencies, amplitudes and splittings allowing to do seismic inversions of the rotation profile inside the solar core. These results open a new ligh t on the physics and dynamics of the solar deep core.