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Nutto, C.; Roth, M.; Zhugzhda, Y.; Bruls, J.; von der Lühe, O.: Calculation of spectral darkening and visibility functions for solar oscillations. Solar Physics 251, pp. 179 - 188 (2008)
Schad, A.; Roth, M.; Schelter, B.; von der Lühe, O.; Timmer, J.: Cross-spectral analysis of solar oscillation time series. J. Phys.: Conf. Ser. 118, 012091 (2008)
Zaatri, A.; Corbard, T.; Roth, M.; González Hernández, I.; von der Lühe, O.: Comparison of geometrical mapping for ring diagram analysis. J. Phys.: Conf. Ser. 118, 012090 (2008)
Krieger, L.; Roth, M.; von der Lühe, O.: Estimating the solar meridional circulation by normal mode decomposition. Astron. Nachrichten 328, pp. 252 - 256 (2007)
Hanasoge, S. M.; Larsen, R. M.; Duvall Jr., T. L.; DeRosa, M. L.; Hurlburt, N. E.; Schou, J.; Roth, M.; Christensen-Dalsgaard, J.; Lele, S. K.: Computational acoustics in spherical geometry: Steps toward validating helioseismology. Astrophysical Journal 648, pp. 1268 - 1275 (2006)
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.