Gizon, L.; Schunker, H.; Baldner, C. S.; Basu, S.; Birch, A. C.; Bogart, R. S.; Braun, D. C.; Cameron, R.; Duvall Jr., T. L.; Hanasoge, S. M.et al.; Jackiewicz, J.; Roth, M.; Stahn, T.; Thompson, M. J.; Zharkov, S.: Helioseismology of sunspots: a case study of NOAA region 9787. Space Science Reviews 144, pp. 249 - 273 (2009)
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)
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The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.