Bridge, H. S.; Belcher, J. W.; Coppi, B.; Lazarus, A. J.; McNutt Jr., R. L.; Olbert, S.; Richardson, J. D.; Sands, M. R.; Selesnick, R. S.; Sullivan, J. D.et al.; Hartle, R. F.; Ogilvie, K. W.; Sittler Jr., E. C.; Bagenal, F.; Wolff, R. S.; Vasyliūnas, V. M.; Siscoe, G. L.; Goertz, C. K.; Eviatar, A.: Plasma observations near Uranus: Initial results from Voyager 2. Science 233, pp. 89 - 93 (1986)
Goertz, C. K.; Nielsen, E.; Korth, A.; Glassmeier, K. H.; Haldoupis, C.; Hoeg, P.; Hayward, D.: Observations of a possible ground signature of flux-transfer events. Journal Geophysical Research 90, p. 4069 (1985)
Bridge, H. S.; Bagenal, F.; Belcher, J. W.; Lazarus, A. J.; McNutt, R. L.; Sullivan, J. D.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 2. Science 215, pp. 563 - 570 (1982)
Marsch, E.; Goertz, C. K.; Richter, K.: Wave heating and acceleration of solar wind ions by cyclotron resonance. Journal Geophysical Research 87, pp. 5030 - 5044 (1982)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Olbert, S.; Sullivan, J. D.; Bagenal, F.; Gazis, P. R.; Hartle, R. E.; Ogilvie, K. W.; Scudder, J. D.et al.; Sittler, E. C.; Eviatar, A.; Siscoe, G. L.; Goertz, C. K.; Vasyliūnas, V. M.: Plasma observations near Saturn: Initial results from Voyager 1. Science 212, pp. 217 - 224 (1981)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Sullivan, J. D.; Bagenal, F.; McNutt Jr., R. L.; Ogilvie, K. W.; Scudder, J. D.; Sittler, E. C.; Vasyliūnas, V. M.et al.; Goertz, C. K.: Plasma observations near Jupiter: Initial results from Voyager 2. Science 206, pp. 972 - 976 (1979)
Bridge, H. S.; Belcher, J. W.; Lazarus, A. J.; Sullivan, J. D.; McNutt, R. L.; Bagenal, F.; Scudder, J. D.; Sittler, E. C.; Siscoe, G. L.; Vasyliūnas, V. M.et al.; Goertz, C. K.; Yeates, C. M.: Plasma observations near Jupiter: Initial results from Voyager 1. Science 204, pp. 987 - 991 (1979)
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.