A plot showing the amplitude of one or more vector components of a magnetic field versus space or time. Solar magnetograms are a graphic representation of solar magnetic field strengths and polarity.
Measurements of the vector or line-of-sightmagnetic field determined from remote sensing measurements of the detailedstructure of spectral lines, including their splitting and polarization.("Magnetogr
am.")
Measurements of the vector or line-of-sight magnetic
field determined from remote sensing measurements of
the detailed structure of spectral lines, including their
splitting and polarization. ("Magnet
ogram.")
A special type of magnetometer that records atime plot of the local magnetic field near the instrument; or a telescopecapable of determining the magnetic field strength and/or direction on adistant ob
ject such as the Sun, using the Zeeman splitting or other spectralsignatures of magnetization.
The dynamics of an ionized plasma in the non-relativistic, collisional case. In this description, charge oscillations and high frequency electromagnetic waves are neglected. It is an important field o
f astrophysics since plasma is one of the commonest forms of matter in the Universe, occurring in stars, planetary magnetospheres, and interplanetary and interstellar space.
The dynamics of an ionized plasma in the non-relativistic, collisional case. In this description, charge oscillations and high frequency electromagnetic waves are neglected. It is an important field o
f astrophysics since plasma is one of the commonest forms of matter in the Universe, occurring in stars, planetary magnetospheres, and interplanetary and interstellar space.
The dynamics of an ionized plasma in the non-relativistic, collisional case. In this description, charge oscillations and high frequency electromagnetic waves are neglected. It is an important field o
f astrophysics since plasma is one of the commonest forms of matter in the Universe, occurring in stars, planetary magnetospheres, and interplanetary and interstellar space.