A review of solar type Ⅲ radio bursts |
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基金项目: | supported by a SUPA Advanced Fellowship (Hamish Reid);the European Research Council under the SeismoSun Research Project No. 321141 (Heather Ratcliffe);the Marie Curie PIRSESGA- 2011-295272 RadioSun project |
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摘 要: | Solar type Ⅲ radio bursts are an important diagnostic tool in the understanding of solar accelerated electron beams. They are a signature of propagating beams of nonthermal electrons in the solar atmosphere and the solar system. Consequently, they provide information on electron acceleration and transport, and the conditions of the background ambient plasma they travel through. We review the observational properties of type Ⅲ bursts with an emphasis on recent results and how each property can help identify attributes of electron beams and the ambient background plasma. We also review some of the theoretical aspects of type Ⅲ radio bursts and cover a number of numerical efforts that simulate electron beam transport through the solar corona and the heliosphere.
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关 键 词: | Sun flares—Sun radio radiation—Sun X-rays gamma rays—Sun particle emission |
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