This page contains magnetic connection predictions for Solar Orbiter and Parker Solar Probe. Currently these span from the launch of Parker Solar Probe to today + 14 days.

They assume a solar wind speed of 350 km/s, down to a source surface at 2.5 solar radii. Below that the trajectory is traced through a PFSS model based on a GONG synoptic magnetogram. I hope to update the movie on a daily basis with new GONG magnetographs and AIA images.

The movie is released under a CC-BY license, which means you can share and adapt it as much as you like, as long as you credit me as the original author.

Any questions or feedback, feel free to email me at d.stansby@ucl.ac.uk.