Usoskin, I. G.; Solanki, S. K.; Schüssler, M.; Mursala, K.: Comment on ``Millennium scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s'' - Reply. Physical Review Letters 92 (19), 199002 (2004)
Vögler, A.; Bruls, J. H. M. J.; Schüssler, M.: Approximations for non-grey radiative transfer in numerical simulations of the solar photosphere. Astronomy and Astrophysics 421, pp. 741 - 754 (2004)
Holzwarth, V.; Schüssler, M.: Dynamics of magnetic flux tubes in close binary stars I. Equilibrium and stability properties. Astronomy and Astrophysics 405, pp. 291 - 301 (2003)
Holzwarth, V.; Schüssler, M.: Dynamics of magnetic flux tubes in close binary stars II. Nonlinear evolution and surface distributions. Astronomy and Astrophysics 405, pp. 303 - 311 (2003)
Kolesnikov, F.; Schüssler, M.: The Kelvin-Helmholtz and shear instabilities of a vortex flow around a magnetic flux tube. Astron. Nachrichten 324, p. 64 (2003)
Schüssler, M.; Shelyag, S.; Berdyugina, S.; Vögler, A.; Solanki, S. K.: Why solar magnetic flux concentrations are bright in molecular bands. Astrophysical Journal 597, pp. L173 - L176 (2003)
Solanki, S. K.; Curdt, W.; Gandorfer, A.; Schüssler, M.; Lites, B. W.; Martinez Pillet, V.; Schmidt, W.; Title, A. M.; the Sunrise Team: SUNRISE: Balloon-borne high-resolution observation of the Sun. Astron. Nachrichten 324, p. 113 (2003)
Usoskin, I.; Solanki, S. K.; Schüssler, M.; Mursula, K.; Alanko, K.: Millenium-scale sunspot number reconstruction: Evidence for an unusually active Sun since the 1940s. Physical Review Letters 91, 211101 (2003)
Moreno-Insertis, F.; Schüssler, M.; Glampedakis, K.: Thermal properties of magnetic flux tubes I. Solution of the diffusion problem. Astronomy and Astrophysics 388, pp. 1022 - 1035 (2002)
Solanki, S. K.; Krivova, N. A.; Schüssler, M.; Fligge, M.: Search for a relationship between solar cycle amplitude and length. Astronomy and Astrophysics 396, pp. 1029 - 1035 (2002)
Usoskin, I. G.; Mursula, K.; Solanki, S. K.; Schüssler, M.; Kovaltsov, G. A.: A physical reconstruction of cosmic ray intensity since 1610. Journal Geophysical Research 107 (A11), 1374 (2002)
Holzwarth, V.; Schüssler, M.: Buried magnetic flux tubes in giant stars near the ``Coronal Dividing Line''. Astronomy and Astrophysics 377, pp. 251 - 263 (2001)
Schmidt, W.; Solanki, S. K.; Schüssler, M.; Curdt, W.; Lites, B. W.; Title, A. M.; Pillet, V. M.: High-resolution solar polarimetry with SUNRISE. Astron. Ges. Abstract Ser. 18, p. 1001 (2001)
Grossmann-Doerth, U.; Schüssler, M.; Sigwarth, M.; Steiner, O.: Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure? Astronomy and Astrophysics 357, pp. 351 - 358 (2000)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
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.
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).