The map shows the intensity of infrared light, and
traces magnetic field lines within filaments of warm dust grains and hot gas, which appear here as thin lines reminiscent of brush strokes in a painting.
Not exact matches
«We computed the Sun's
magnetic environment by
tracing millions of
magnetic field lines and looking at how neighboring
field lines connect and diverge,» said Antonia Savcheva, an astrophysicist at the Harvard - Smithsonian Center for Astrophysics in Cambridge, Massachusetts, and co-author of the paper.
In the image above, blue
lines track strong
magnetic field lines directed one way, while those in magenta
trace powerful
lines in the opposite direction.
Scientists are not able to observe
magnetic fields directly so they use hot gases in the sun's atmosphere to
trace out
magnetic field lines.