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Published

Time-distance helioseismology: Inversion of noisy correlated data
Couvidat, S., Gizon, L., Birch, A.C., Larsen, R.M., Kosovichev, A.G. Astrophys. J. Suppl. Ser. 158, 217-229 (2005)

Helioseismology of time-varying flows through the solar cycle
Gizon, L., Solar Phys. 224, 217-228 (2004)

Solar cycle variations in the spectrum of supergranulation
Gizon, L., Duvall, T.L., in Multi-Wavelength Investigations of Solar Activity, IAU S-223, 41-44 (2004)

Validation of 3D helioseismic inversions of travel times through simulations of artificial data with the correct noise statistics
Couvidat, S., Gizon, L., Birch, A.C., in SOHO14, ESA SP-559, 384-387 (2004)

Time-distance helioseismology: noise estimation
Gizon, L., Birch, A.C., Astrophys. J. 614, 472-489 (2004)

Comparison of solar subsurface flows assessed by ring and time-distance analyses.
Hindman, B., Gizon, L., Duvall, T.L., Haber, D., Toomre, J., Astrophys. J. 613, 1253-1262 (2004)

Measuring differential rotation with asteroseismology.
Gizon, L., Solanki, S.K., Solar Physics, Solar Phys. 220, 169-184 (2004)

Determining the inclination of the rotation axis of a sun-like Star.
Gizon, L., Solanki, S.K., Astrophys. J. 589, 1009-1019 (2003)

Wavelike properties of solar supergranulation.
Gizon, L., Duvall, T.L., Schou, J. Nature 421, 43-44 (2003)
Erratum, Nature 421, 764 (2003): in Fig. 1 the units of frequency should be microhertz not millihertz. Press release / media coverage.

Superganulation supports waves
Gizon, L., Duvall, T.L., in SOHO 12, ESA SP-517, 43-52 (2003)

Ph.D. Dissertation, Physics Department, Stanford University

Comparison of near-surface flows assessed by ring-diagram and f-mode time-distance analyses.
Hindman, B., Gizon, L., Haber, D., Duvall, T.L., Toomre, J., in SOHO 12, ESA SP-517, 299-302 (2003)

A new component of solar dynamics: north-south diverging flows migrating toward the equator with an 11 year period.
Beck, J.G., Gizon, L., & Duvall T.L. Astrophys. J. 575, L47-L50 (2002).

Time-distance helioseismology: The forward problem for random distributed sources.
Gizon, L. & Birch, A.C. Astrophys. J. 571, 966-986 (2002).

Prospects for detecting stellar activity through asteroseismology.
Gizon, L. Astron. Nachr. 323, 251-253 (2002).

Travel-time sensitivity kernels for time-distance helioseismology.
Gizon, L., Birch, A.C. Solar Encounter: The First Solar Orbiter Workshop, ESA SP-493, 233-236 (2001).

Time-distance helioseismology and the Solar Orbiter mission
Gizon, L., Birch, A.C., Bush, R.I., Duvall, T.L., Kosovichev, A.G., Scherrer, P.H., Zhao, J. in Solar Encounter: The First Solar Orbiter Workshop, ESA SP-493, 227-231 (2001).

Local-area helioseismology as a diagnostic tool for solar variability
Kosovichev, A.G., Duvall, T.L., Birch, A.C., Gizon, L., Scherrer, P.H., Zhao, J. Advances in Space Research, 29, 1899-1910 (2002).

Heliotomography of the outer layers of the Sun
Kosovichev, A.G., Duvall, T.L., Birch, A.C., Gizon, L., Scherrer, P.H., Zhao, J. in Helio- and Asteroseismology at the Dawn of the Millennium, ESA SP-464, 701-706 (2001)

Probing surface flows and magnetic activity with time-distance helioseismology.
Gizon, L., Duvall, T.L., & Larsen, R.M. in Recent Insights into the Physics of the Sun and Heliosphere, eds. P. Brekke, B. Fleck & J.B. Gurman, IAU Symp. 203, 189-191 (2001)

Seismic tomography of the near solar surface
Gizon, L., Duvall, T.L., Larsen, R.M. J. Astrophys. Astr. 21, 339-342 (2000)

Gizon, L., Kosovichev, A.G. in Solar Orbiter Assessment Study Report, ESA-SCI(2000)6 (2000).

Time-distance helioseismology with f modes as a method for measurement of near-surface flows
Duvall, T.L., Gizon, L. Solar Phys. 192, 177-191 (2000)

LOI/SOHO constraints on oblique rotation of the solar core
Gizon, L., Appourchaux, T., Gough, D.O. (1998), in New eyes to see inside the Sun and stars, eds. Deubner F.-L. et al. (Kluwer, Dordrecht) IAU Symp. 185 37-40 (1998).

Comments on the influence of solar activity on p-mode oscillation spectra
Gizon, L. in New eyes to see inside the Sun and stars, eds. Deubner F.-L. et al. (Kluwer, Dordrecht) IAU Symp. 185 173-174 (1998).

The art of fitting p-mode spectra. I. Maximum likelihood estimation
Appourchaux T., Gizon, L., Rabello-Soares, M.-C. Astron. Astrophys. Suppl. 132, 107-119 (1998).

The art of fitting p-mode spectra. II. Leakage and noise covariance matrices.
Appourchaux, T., Rabello-Soares, M.-C., Gizon, L. Astron. Astrophys. Suppl. 132, 121-132 (1998).

A forward analysis of the solar core rotation.
Gizon L., in Sounding solar and stellar interiors (Universite de Nice, Nice), Eds. J. Provost J. & F.-X. Schmider, IAU Symp. 181 Posters, 89-90 (1998).

New IRIS constraints on the solar core rotation
Gizon, L., Fossat, E., Lazrek, M., et al. Astron. Astrophys. 317, L71-L74 (1997).

Can we see the back of the Sun?
Gizon L., in Vincent R.A. et al. (eds.), Proc. Conf. STEP 1995 (University of Adelaide), STEP 1995, 173-176 (1995).

The rotation of the solar core - Interpretation of the latest IRIS splittings
Gizon L., in Vincent R.A. et al. (eds.), Proc. Conf. STEP 1995 (University of Adelaide), STEP 1995, 217-220 (1995).