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:
![](http://capst.ncku.edu.tw/PGS/wp-content/uploads/2020/03/MartianBowShock-1024x636.png)
![](http://capst.ncku.edu.tw/PGS/wp-content/uploads/2020/08/DSC_4955_Cut_wScale.png)
![](http://capst.ncku.edu.tw/PGS/wp-content/uploads/2020/08/DSC_5011_Bright_Cut_wScale.png)
2. Magnetic reconnections
![](https://sites.google.com/site/ppgssncku/_/rsrc/1470811473249/research/Laboratory-Astrophysics-and-Space-Science/Reconnection_Exp.png?height=306&width=400)
![](https://sites.google.com/site/ppgssncku/_/rsrc/1470811507072/research/Laboratory-Astrophysics-and-Space-Science/Reconnection_Exp_Control.png?height=254&width=400)
— Ref. Lucy-Ann McFadden and Torrence Johnson and Paul Weissman, ed., Encyclopedia of the Solar System, 2nd Ed. (Academic Press, 2006).