Vasyliūnas, V. M.: Magnetosphere: From Plasma Observations to Reconnection Theory. Journal of Geophysical Research: Space Physics 125 (9), e2020JA027865 (2020)
Lopez, R. E.; Gonzalez, W. D.; Vasyliūnas, V. M.; Richardson, I. G.; Cid, C.; Echer, E.; Reeves, G. D.; Brandt, P. C.: Decrease in SYM-H during a storm main phase without evidence of a ring current injection. Journal of Atmospheric and Solar-Terrestrial Physics 134, pp. 118 - 129 (2015)
Song, P.; Vasyliūnas, V. M.: Effect of horizontally inhomogeneous heating on flow and magnetic field in the chromosphere of the Sun. Astrophys. J. Lett. 796, L23 (2014)
Tu, J.; Song, P.; Vasyliūnas, V. M.: Inductive-dynamic magnetosphere-ionosphere coupling via MHD waves. J. Geophys. Res. Space Phys. 119, pp. 530 - 547 (2014)
Song, P.; Vasyliūnas, V. M.; Zhou, X.-Z.: Magnetosphere-ionosphere/thermosphere coupling: Self-consistent solutions for a one-dimensional stratified ionosphere in three-fluid theory. Journal Geophysical Research 114, A08213 (2009)
Aschwanden, M. J.; Burlaga, L. F.; Kaiser, M. L.; Ng, C. K.; Reames, D. V.; Reiner, M. J.; Gombosi, T. I.; Lugaz, N.; Manchester, W.; Roussev, I. I.et al.; Zurbuchen, T. H.; Farrugia, C. J.; Galvin, A. B.; Lee, M. A.; Linker, J. A.; Mikić, Z.; Riley, P.; Alexander, D.; Sandman, A. W.; Cook, J. W.; Howard, R. A.; Odstrčil, D.; Pizzo, V. J.; Kóta, J.; Liewer, P. C.; Luhmann, J. G.; Inhester, B.; Schwenn, R. W.; Solanki, S. K.; Vasyliūnas, V. M.; Wiegelmann, T.; Blush, L.; Bochsler, P.; Cairns, I. H.; Robinson, P. A.; Bothmer, V.; Kecskemety, K.; Llebaria, A.; Maksimovic, M.; Scholer, M.; Wimmer-Schweingruber, R. F.: Theoretical Modeling for the Stereo Mission. Space Science Reviews 136, pp. 565 - 604 (2008)
Tsurutani, B. T.; Verkhoglyadova, O. P.; Mannucci, A. J.; Saito, A.; Araki, T.; Yumoto, K.; Tsuda, T.; Abdu, M. A.; Sobral, J. H. A.; Gonzalez, W. D.et al.; McCreadie, H.; Lakhina, G. S.; Vasyliūnas, V. M.: Prompt penetration electric fields (PPEFs) and their ionospheric effects during the great magnetic storm of 30-31 October 2003. Journal Geophysical Research 113, A05311 (2008)
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).