Over the past 15 years, our knowledge of the interior of the Sun has tremendously progressed by the use of helioseismic measurements. However, to go further in...
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PublicationDetecting individual gravity modes in the Sun: Chimera or reality?
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PublicationDetection and temporal coherence of p-modes below 1.4 mHz
Data collected recently by the helioseismic experiments aboard the SOHO spacecraft have allowed the detection of low degree p-modes with increasingly lower...
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PublicationDisk-integrated Intensity Pseudomodes Measured by SOHO/VIRGO
The high-frequency spectrum above the acoustic cutoff frequency (νac) of the solar atmosphere has been observed in velocity measurements at low and high angular...
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PublicationEleven years of IRIS frequencies and splittings
Having acquired since July, 1989, a complete 11-year solar cycle of full disk data, the IRIS++ network has now made available to anyone the longest helioseismic...
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PublicationExcitation and Damping of Low-Degree Solar p-Modes during Activity Cycle 23: Analysis of GOLF and VIRGO Sun Photometer Data
We have used observations made by the Global Oscillations at Low Frequency (GOLF) and the Variability of Irradiance and Gravity Oscillations Sun Photometer...
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PublicationExcitation of Solar Acoustic Modes
The excitation of p-modes seems to be produced by turbulence in the convection zone (see, e.g., Kumar, 1997 and the references therein). Low-degree p-mode...
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PublicationFarNet-II: An improved solar far-side active region detection method
Context. Activity on the far side of the Sun is routinely studied through the analysis of the seismic oscillations detected on the near side using helioseismic...
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PublicationFast-to-Alfvén Mode Conversion Mediated by the Hall Current. I. Cold Plasma Model
The photospheric temperature minimum in the Sun and solar-like stars is very weakly ionized, with an ionization fraction f as low as 10‑4. In galactic star...
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PublicationFirst evidence of interaction between longitudinal and transverse waves in solar magnetic elements
Small-scale magnetic fields are thought to play an important role in the heating of the outer solar atmosphere. By taking advantage of the unprecedented high...