A Statistical Analysis of the Type-III Bursts in Centimeter and Decimeter Wavebands

详细信息	查看全文 | 推荐本文 |

• 作者：Yuan Ma¹ ; ² ; ^{mayuan@ynao.ac.cn} ; Rui-xiang Xie¹ ; ² ; Xiang-min Zheng¹ ; ² ; Min Wang¹ ; ² ; Yan Yi-hua²
• 关键词：sun ; radio radiation ; sun ; flares ; method ; statistical
• 刊名：Chinese Astronomy and Astrophysics
• 出版年：2012
• 期刊代码：8_02751062
• 类别：ph
• 出版时间：April-June, 2012
• 卷：36
• 期：2
• 页码：175-186
• 文件大小：836 K

摘要

A statistical analysis of the type-III bursts observed by the spectrographs in the ranges of 625鈭?500 MHz, 2600-3800 MHz, and 5200-7600 MHz during the 23rd solar cycle (from 2000 July to 2004 September) is carried out. The distribution of the type-III bursts, and their durations, frequency drift rates, polarization degrees and frequency bandwidths are given in this paper. The results indicate that the average values of the frequency drift rates and frequency bandwidths increase with the frequency. The average values of the durations and polarization degrees are neither constant nor uniformly varied over a broad frequency range. Most of type-III bursts are distributed in the range from 625 to 3800 MHz, and decrease with the frequency in number. This analysis shows that the places of electron acceleration and energy release are mainly in the decimetric range, and the characteristic of this frequency range is possibly related with the magnetic configuration at the decimeter wavelengths, as well as the electron acceleration in the magnetic reconnection site close to the main flare. However, there are also a considerable number of type-III bursts in the range of 5200-7600 MHz, it means that the sites of electron acceleration are widely distributed in the coronal region. The radiation mechanisms of type-III bursts at the centimeter-decimeter wavelengths include most probably the coherent plasma radiation and the emission process of electron cyclotron maser.