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.
Not exact matches
«Chaotic
magnetic field lines may answer the coronal heating problem: Scientists show how chaotic
magnetic field lines result in
stronger current sheets and extreme heating of the sun's corona.»
These stresses arise because the Sun's
magnetic field lines have a
strong tendency to push one another apart.
The researchers found that applying a
strong magnetic field to these ultracold atoms caused them to
line up in an alternating pattern and lean away from each other.
The neutron star (red sphere) with its
strong magnetic field (white
lines) spins around itself nearly 30 times per second injecting energetic electrons in the space region around it.
If the cyclotron
line is from circling electrons, in contrast, then the
magnetic field strength around the neutron star would not be exceptionally
strong, and thus the
field is probably not the reason these stars break the Eddington limit.
«If the cyclotron
line is from protons, then we know that these
magnetic fields around the neutron star are extremely
strong and may in fact be helping to breaking the Eddington limit,» says Brightman.
The energy input from Saturn's magnetospheric interaction shows a
strong interaction with Titan's atmosphere and the corresponding induced magnetosphere with draped
magnetic field lines.