Radio fine structures in dm–cm wavelength range associated with magnetic reconnection processes |
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Authors: | Y Yan J Huang B Chen Y Liu C Tan |
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Institution: | 1. Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China;2. The State Key Laboratory of Space Weather, P.O. Box 8701, Beijing 100080, China |
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Abstract: | Radio bursts with fine structures in decimetric–centimetric wave range are generally believed to manifest the primary energy release process during flare/CME events. By spectropolarimeters in 1–2 GHz, 2.6–3.8 GHz, and 5.2–7.6 GHz at NAOC/Huairou with very high temporal (1.25–8 ms) and spectral (4–20 MHz) resolutions, the zebra patterns, spikes, and new types of radio fine structures with mixed frequency drift features are observed during several significant flare/CME events. In this paper we will discuss the occurrence of radio fine structures during the impulsive phase of flares and/or CME initiations, which may be connected to the magnetic reconnection processes. |
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Keywords: | Solar activities Solar flares Solar radio bursts Fine structures CME |
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