Ion cyclotron resonance heating (or ICRH) is a technique in which
electromagnetic waves with frequencies corresponding to the ion cyclotron frequency is used to heat up a
plasma. The ions in the plasma absorb the electromagnetic radiation and as a result of this, increase in
kinetic energy. This technique is commonly used in the heating of
tokamak plasmas.
In the solar wind On March 8, 2013, NASA released an article according to which ion cyclotron waves were identified by its solar probe spacecraft called WIND as the main cause for the heating of the
solar wind as it rises from the Sun's surface. Before this discovery, it was unclear why the solar wind particles would heat up instead of cool down, when speeding away from the Sun's surface.
Magnetic confinement fusion In
fusion devices, such as
tokamaks and
stellarators, ICRH antennas are installed in the machine vessel to heat the plasma using
radio waves with frequencies in the range of the ion cyclotron resonance. ICRH provides localized heating of ions in fusion plasmas, which can generate a large population of energetic particles typically inaccessible with other heating methods (such as
electron cyclotron resonance heating or
neutral beam injection). The confinement properties of fast ions in plasma is a major research topic in fusion plasma physics. == See also ==