1. Interactions between solar winds and planetary magnetic fields or unmagnetized planets will be studied
- Studies of the Martian bow shock location: The shock nose location is more sensitive to the solar EUV flux than solar wind dynamics pressure consisting with the spacecraft measurement results:
2. Magnetic reconnections
— Ref. Lucy-Ann McFadden and Torrence Johnson and Paul Weissman, ed., Encyclopedia of the Solar System, 2nd Ed. (Academic Press, 2006).