On the origin of fast drift absorption bursts

Details On the origin of fast drift absorption bursts On the origin of fast drift absorption bursts

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....45..135z&link_type=abstract

Astronomy and Astrophysics, vol. 45, no. 1, Dec. 1975, p. 135-140.

Astronomy and Astrophysics

Astrophysics

32

Drift Rate, Electromagnetic Absorption, Hot Electrons, Magnetohydrodynamic Stability, Plasma Loss, Type 4 Bursts, Absorption Spectra, Bernstein Energy Principle, Electron Distribution, Linearity, Nonlinearity, Plasma Waves, Solar Corona, Solar Magnetic Field

Scientific paper

We present an explanation of the Type-IV continuum with fast-drift absorption radio bursts observed during the event which occurred on the 2nd of March, 1970. The continuum emission is assumed to be caused by a high-frequency loss-cone instability in the adiabatic magnetic trap, while the absorption bursts are considered to be a result of hot electrons being injected into the trap, which fill the loss-cone and quench the instability. The emission fringe of absorption bursts at the low-frequency side and the wedge-shaped form of the bursts are also elucidated.

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