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Kopp, A.; Ip, W.-H.: Resistive MHD simulations of Ganymede's magnetosphere 1: Time variabilities of the magnetic field topology. Journal Geophysical Research 107 (A12), 1490 (2002)
Das, A. C.; Ip, W.-H.: Field aligned current and particle acceleration in the near-Io plasma torus. Planetary and Space Science 48, pp. 127 - 131 (2000)
Ip, W.-H.; Kopp, A.; Lara, L. M.; Rodrigo, R.: Pluto's ionospheric models and solar wind interaction. Advances in Space Research 26 (10) (10), pp. 1559 - 1563 (2000)
Ip, W.-H.; Kopp, A.; Lara, L. M.; Rodrigo, R.: Pluto's ionospheric models and solar wind interaction. Advances in Space Research 26 (10) (10), pp. 1559 - 1563 (2000)
Ip, W.-H.; Kopp, A.; Williams, D. J.; McEntire, R. W.; Mauk, B. H.: Magnetospheric ion sputtering: The case of Europa and its surface age. Advances in Space Research 26 (10), pp. 1649 - 1652 (2000)
Lieu, R.; Ip, W.-H.; Axford, W. I.; Bonamente, M.: Nonthermal origin of the EUV and soft X-rays from the Coma Cluster: Cosmic rays in equipartition with the thermal medium. Astrophys. J. Let. 510, pp. L25 - L28 (1999)
Axford, W. I.; Marsch, E.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T. K.; Schwenn, R.; Ip, W.-H.; Ksanfomality, L. V.; Thomas, N.; Kogan, A.et al.; Utkin, V. F.; Uspensky, G. R.: Space mission for exploration of the Sun, Mercury and inner heliosphere (``InterHelios''). Advances in Space Research 21, pp. 275 - 289 (1998)
How does our star heat its outer atmosphere, the solar corona, to unimaginable temperatures of up to 10 million degrees Celsius? With unprecedented observational data from ESA's Solar Orbiter spacecraft and powerful computer simulations, ERC starting grant awardee Pradeep Chitta intends to bring new momentum to the search for the coronal heating mechanism.
The research group “Solar Lower Atmosphere and Magnetism” (SLAM) studies the conditions and dynamic processes in the atmospheric layer between the solar surface (photosphere) and the overlying chromosphere, an approximately 2000 km thick gas layer.
The main research fields of the department "Sun and Heliosphere" are covered by the research groups "Solar and Stellar Coronae", "Solar Lower Atmosphere and Magnetism", "Solar and Stellar Magnetohydrodynamics" and "Solar Variability and Climate".