Krivov, A. V.; Mann, I.; Krivova, N. A.: Size distribution of dust in circumstellar debris disks. Astronomy and Astrophysics 362, pp. 1127 - 1137 (2000)
Mann, I.; Kimura, H.: Interstellar dust properties derived from mass density, mass distribution, and flux rates in the heliosphere. Journal Geophysical Research 105, pp. 10317 - 10328 (2000)
Kimura, H.; Mann, I.: Filtering of the interstellar dust flow near the heliopause: the importance of secondary electron emission for the grain charging. Earth Planets Space 51, pp. 1223 - 1232 (1999)
Krüger, H.; Grün, E.; Hamilton, D. P.; Baguhl, M.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hanner, M. S.; Horányi, M.; Kissel, J.et al.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Riemann, R.; Schwehm, G.; Srama, R.; Zook, H. A.: Three years of Galileo dust data: II. 1993-1995. Planetary and Space Science 47, pp. 85 - 106 (1999)
Krüger, H.; Grün, E.; Landgraf, M.; Baguhl, M.; Dermott, S.; Fechtig, H.; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Horányi, M.et al.; Kissel, J.; Lindblad, B. A.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.; Zook, H. A.: Three years of Ulysses dust data: 1993-1995. Planetary and Space Science 47, pp. 363 - 383 (1999)
Kuhn, J. R.; MacQueen, R. M.; Streete, J.; Tansey, G.; Mann, I.; Hillebrand, P.; Coulter, R.; Lin, H.: Probable detection of a bright infrared coronal emission line of SI IX near 3.93 microns. Astrophysical Journal 521, pp. 478 - 482 (1999)
Mann, I.; Kuhn, J. R.; MacQueen, R. M.; Streete, J.; Tansey, G.; Hillebrand, P.; Colter, R.; Lin, H.; Edmund, D.; Judge, P.: Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns. Astrophysical Journal 521, pp. 478 - 482 (1999)
Wehry, A.; Mann, I.: Identification of β-meteoroids from measurements of the dust detector onboard the Ulysses spacecraft. Astronomy and Astrophysics 341, pp. 296 - 303 (1999)
Grün, E.; Krüger, H.; Graps, A. L.; Hamilton, D. P.; Heck, A.; Linkert, G.; Zook, H. A.; Dermott, S.; Fechtig, H.; Gustafson, B. A.et al.; Hanner, M. S.; Horányi, M.; Kissel, J.; Lindblad, B. A.; Linkert, D.; Mann, I.; McDonnell, J. A. M.; Morfill, G. E.; Polanskey, C.; Schwehm, G.; Srama, R.: Galileo observes electromagnetically coupled dust in the Jovian magnetosphere. Journal Geophysical Research 103, p. 20011 (1998)
Kimura, H.; Mann, I.: The electric charging of interstellar dust in the solar system and consequences for its dynamics. Astrophysical Journal 499, pp. 454 - 462 (1998)
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).