The following examples are listed in the ascending order of the magnetic-field strength. • (31.869 μT) – strength of
Earth's magnetic field at 0° latitude, 0° longitude • (40 μT) – walking under a
high-voltage power line • (5 mT) – the strength of a typical
refrigerator magnet • 0.3 T – the strength of solar sunspots • 1 T to 2.4 T – coil gap of a typical loudspeaker magnet • 1.5 T to 3 T – strength of medical
magnetic resonance imaging systems in practice, experimentally up to 17 T • 4 T – strength of the
superconducting magnet built around the
CMS detector at
CERN • 5.16 T – the strength of a specially designed room temperature
Halbach array • 8 T – the strength of
LHC magnets • 11.75 T – the strength of INUMAC magnets, largest
MRI scanner • 13 T – strength of the superconducting
ITER magnet system • 14.5 T – highest magnetic field strength ever recorded for an accelerator steering magnet at
Fermilab • 16 T – magnetic field strength required to levitate a
frog (by
diamagnetic levitation of the water in its body tissues) according to the 2000
Ig Nobel Prize in Physics • 17.6 T – strongest field trapped in a superconductor in a lab as of July 2014 • 20 T – strength of the large scale high temperature superconducting magnet developed by MIT and Commonwealth Fusion Systems to be used in fusion reactors • 27 T – maximal field strengths of
superconducting electromagnets at cryogenic temperatures • 35.4 T – the current (2009) world record for a superconducting electromagnet in a background magnetic field • 45 T – the current (2015) world record for continuous field magnets • 100 T – approximate magnetic field strength of a typical
white dwarf star • 1200 T – the field, lasting for about 100 microseconds, formed using the electromagnetic flux-compression technique • 109 T –
Schwinger limit above which the electromagnetic field itself is expected to become nonlinear • 108 – 1011 T (100 MT – 100 GT) – magnetic strength range of
magnetar neutron stars == Notes and references ==