Advances in Stellar Interferometry, eds. J. D. Monnier, M. Schöller and W. C. Danchi, SPIE 6268, (2006)
Astron. & Astrophys., 413, pp. 1135-1142 (2004)
To reach a suitable limiting magnitude with a multi-aperture interferometer, we need tocophase the different telescopes using a reference source. The latter should be located in thesame isopistonic domain as the science source. We developed a direct analytical expressionof deducing the isopistonic angle from atmospheric optical parameters as...
International audience
Context. Over the past 40 years, helioseismology has been enormously successful in the study of the solar interior. A shortcoming has been the lack of a convincing detection of the solar g modes, which are oscillations driven by gravity and are hidden in the deepest part of the solar body – its hydrogen-burning core. The detection of g modes is...
Solar Physics, 220, pp. 269-285 (2004)
Proceedings of the SOHO 14 / GONG 2004 Workshop (ESA SP-559). "Helio- and Asteroseismology: Towards a Golden Future, ed. D. Danesy., n/a, p. 356 (2004)
Monthly Notices of the Royal Astronomical Society, 369, pp. 985-996 (2006)
International audience