Hanasoge, S. M.; Birch, A. C.; Bogdan, T. J.; Gizon, L.: f-mode interactions with thin flux tubes: the scattering matrix. Astrophysical Journal 680, pp. 774 - 780 (2008)
Hirzberger, J.; Gizon, L.; Solanki, S. K.; Duvall Jr., T. L.: Structure and evolution of supergranulation from local helioseismology. Solar Physics 251, pp. 417 - 437 (2008)
Jackiewicz, J.; Gizon, L.; Birch, A. C.: High-resolution mapping of flows in the solar interior: Fully consistent OLA inversion of helioseismic travel times. Solar Physics 251, pp. 381 - 415 (2008)
Stahn, T.; Gizon, L.: Fourier analysis of gapped time series: Improved estimates of solar and stellar oscillation parameters. Solar Physics 251, pp. 31 - 52 (2008)
Birch, A. C.; Gizon, L.; Hindman, B. W.; Haber, D. A.: The linear sensitivity of helioseismic ring diagrams to local flows. Astrophysical Journal 662, pp. 730 - 737 (2007)
Cameron, R.; Gizon, L.; Daiffallah, K.: SLiM: a code for the simulation of wave propagation through an inhomogeneous, magnetised solar atmosphere. Astron. Nachrichten 328, pp. 313 - 318 (2007)
Jackiewicz, J.; Gizon, L.; Birch, A. C.; Duvall Jr., T. L.: Time-distance helioseismology: Sensitivity of f-mode travel times to flows. Astrophysical Journal 671, pp. 1051 - 1064 (2007)
Jackiewicz, J.; Gizon, L.; Birch, A. C.; Thompson, M. J.: A procedure for the inversion of f-mode travel times for solar flows. Astron. Nachrichten 328, pp. 234 - 239 (2007)
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).
Application deadline 1 October 2024. PhD projects in planetary science, solar and stellar physics, solar magnetism, heliophysics, helioseismology, asteroseismology, ...
First Light for Sunrise III: the first tests with real sunlight were successful. The balloon-borne solar observatory should be ready for launch at the end of May.
In analyzing solar observations from the 19th century, scientists are turning to amateur researchers for help. The project will allow to better understand the history of our star.
Astronomical teamwork: By combining data from Solar Orbiter and SDO, a group of researchers has unambiguously determined the magnetic field at the solar surface.