Wilhelm, K.; Dwivedi, B. N.: An explanation of the Pioneer anomaly involving accelerated atomic clocks. Astrophysics and Space Sciences Transactions 7, pp. 487 - 494 (2011)
Gabriel, A.; Bely-Dubau, F.; Tison, E.; Wilhelm, K.: The Structure and Origin of Solar Plumes: Network Plumes. Astrophysical Journal 700, pp. 551 - 558 (2009)
Mendoza-Torres, J. E.; Wilhelm, K.; Lara, A.: The solar plasma conditions in the source regions of two explosive events. Astronomy and Astrophysics 495 (2), pp. 613 - 620 (2009)
Wilhelm, K.; Curdt, W.; Dammasch, I. E.; Hassler, D. M.: Comment on ``Energy levels and spectral lines of NeVIII''. Eur. Phys. J. D 47 (3), p. 325 - 325 (2008)
McIntosh, S. W.; Davey, A. R.; Hassler, D. M.; Armstrong, J. D.; Curdt, W.; Wilhelm, K.; Lin, G.: Observations supporting the role of magnetoconvection in energy supply to the quiescent solar atmosphere. Astrophysical Journal 654, pp. 650 - 664 (2007)
Wilhelm, K.; Marsch, E.; Dwivedi, B. N.; Feldman, U.: Observations of the Sun at Vacuum-Ultraviolet Wavelengths from Space. Part II: Results and Interpretations. Space Science Reviews 133, pp. 103 - 179 (2007)
Wilhelm, K.: Solar VUV measurements obtained by SOHO instruments and their radiometric calibration. Advances in Space Research 37 (2), pp. 225 - 233 (2006)
Emerich, C.; Lemaire, P.; Vial, J.-C.; Curdt, W.; Schühle, U.; Wilhelm, K.: A new relation between the central spectral solar H I Lyman α irradiance and the line irradiance measured by SUMER/SOHO during the cycle 23. Icarus 178, pp. 429 - 433 (2005)
Lemaire, P.; Emerich, C.; Vial, J.-C.; Curdt, W.; Schühle, U.; Wilhelm, K.: Variation of the full Sun hydrogen Lyman profiles through solar cycle 23. Advances in Space Research 35, pp. 384 - 387 (2005)
Mendoza-Torres, J. E.; Torres-Papqui, J. P.; Wilhelm, K.: Explosive events in the solar atmosphere seen in extreme-ultraviolet emission lines. Astronomy and Astrophysics 431, pp. 339 - 344 (2005)
Wilhelm, K.; Fludra, A.; Teriaca, L.; Harrison, R. A.; Dwivedi, B. N.; Pike, C. D.: The widths of vacuum-ultraviolet spectral lines in the equatorial solar corona observed with CDS and SUMER. Astronomy and Astrophysics 435, pp. 733 - 741 (2005)
Wilhelm, K.; Schühle, U.; Curdt, W.; Hilchenbach, M.; Marsch, E.; Lemaire, P.; Bertaux, J.-L.; Jordan, S. D.; Feldman, U.: On the nature of the unidentified solar emission near 117 nm. Astronomy and Astrophysics 439, pp. 701 - 711 (2005)
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.