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).