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Auroral Radio Emissions, 1. Hisses, Roars, and Bursts

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Abstract

The Earth's auroral electrons produce copious non-thermal radio emissions of various types, including auroral kilometric radiation (AKR), whistler mode auroral hiss, mode conversion radiation such as auroral roar and MF-burst, and possibly HF/VHF emissions. In some cases, mechanisms have been identified and quantitatively described, whereby the energy of the auroral electrons is converted into electromagnetic radiation. In many other cases, the radiation mechanism, or the relative significance of several possible mechanisms, remains uncertain. This review covers fairly comprehensively experimental and theoretical research on types of auroral radiation other than AKR, concentrating on emissions with frequency higher than about 1 kHz and treating only emissions which are unique to the auroral zone. The review covers both ground-based and in-situ observations. It covers a wide range of theoretical approaches, emphasizing those which at present appear most important for producing non-AKR auroral radiations.

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  1. Department of Physics and Astronomy, Dartmouth College, Hanover, New Hampshire, U.S.A

    James LaBelle

  2. Centre for Interdisciplinary Plasma Science, Max-Planck-Institut für extraterrestrische Physik, Garching, Germany

    Rudolf A. Treumann

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LaBelle, J., Treumann, R.A. Auroral Radio Emissions, 1. Hisses, Roars, and Bursts. Space Science Reviews 101, 295–440 (2002). https://doi.org/10.1023/A:1020850022070

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