Magnetic field lines are a conceptual tool used to visualize magnetic fields, but they do not represent physical entities that can break or reconnect. During events like coronal ejections, plasma is ejected and later reconnects with the solar surface, creating a visual representation akin to "iron filings." The discussion raises questions about the nature of these field lines, suggesting they may be more about illustrating field density rather than existing as tangible lines. The transformation of magnetic fields when two magnets are brought closer is complex, as it involves the reconfiguration of field vectors rather than a simple merging of lines. Ultimately, magnetic field lines serve as a useful visualization but have limitations in their applicability to the actual dynamics of magnetic fields.