Ip, W.-H.; Williams, D. J.; McEntire, R. W.; Mauk, B. H.: Ion sputtering and surface erosion at Europa. Geophysical Research Letters 25, pp. 829 - 832 (1998)
Ip, W.-H.; Fernández, J. A.: On dynamical scattering of Kuiper belt objects in 2:3 resonance with Neptune into short-period comets. Astronomy and Astrophysics 324, pp. 778 - 784 (1997)
Ip, W.-H.; Williams, D. J.; McEntire, R. W.; Mauk, B.: Energetic ion sputtering effects at Ganymede. Geophysical Research Letters 24, pp. 2631 - 2634 (1997)
Ksanfomality, L. V.; Breus, T. K.; Oraevsky, V. N.; Kuznetsov, V. D.; Axford, W. I.; Ip, W.-H.; Thomas, N.; Kogan, A. Y.: Investigations of Mercury using the 'Solar-Mercury Observer' (InterHelios). Advances in Space Research 19, pp. 1625 - 1628 (1997)
Marsch, E.; Axford, W. I.; Ip, W.-H.; Thomas, N.; Schwenn, R.; Oraevsky, V. N.; Kuznetsov, V. D.; Breus, T.; Ksanfomality, L. V.; Kogan, A. Y.: InterHelios-Sun and Mercury Observer. Physics and Chemistry of the Earth 22, pp. 469 - 479 (1997)
Russell, C. T.; Bagenal, F.; Cheng, A. F.; Ip, W.-H.; Roux, A.; Smyth, W. H.; Bolton, J. S.; Polansky, C. A.: Io's interaction with the Jovian magnetosphere. EOS, Trans. AGU. 78, pp. 93 - 100 (1997)
Belton, M. J. S.; Head III, J. W.; Ingersoll, A. P.; Greeley, R.; McEwen, A. S.; Klaasen, K. P.; Senske, D.; Pappalardo, R.; Collins, G.; Vasavada, A. R.et al.; Sullivan, R.; Simonelli, D.; Geissler, P.; Carr, M. H.; Davies, M. E.; Veverka, J.; Gierasch, P. J.; Neukum, G.; Pilcher, C. B.; Beebe, R. F.; Burns, J. A.; Fanale, F.; Ip, W.-H.; Johnson, T. V.; Morrison, D.; Moore, J.; Orton, G. S.; Thomas, P.; West, R. A.: Galileo's First Images of Jupiter and the Galilean Satellites. Science 274, pp. 377 - 385 (1996)
Fernandez, J. A.; Ip, W.-H.: Orbital expansion and resonant trapping during the late accretion stages of the outer planets. Planetary and Space Science 44, pp. 431 - 439 (1996)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.