The Near-Saturn Magnetic Field Environment

Meer over het boek

Focusing on the high Mach number shock wave near Saturn's magnetic field, this thesis leverages the unique data from the Cassini spacecraft to explore the solar wind's interaction in a previously inaccessible regime. By comparing shock physics in the Solar System with ultra-high Mach number shocks found in supernova remnants, the author provides valuable in-situ insights that enhance understanding of both phenomena. This work bridges theoretical and observational gaps, advancing knowledge in the field of astrophysics.