NAOC Open IR
米波窄带快频漂射电爆发??"Blips"的观测和证认
郑向民; 马媛; 夏志国; 陈敬英
1994
Source Publication天体物理学报
ISSN0253-2379
Volume014Issue:001Pages:72
Abstract用云南天文台高时间分辨率(10ms)高频率分辨率(0.5MHz)的射电频谱仪观测分析证认了米波窄带短持续时间快频漂爆发的存在。这种漂发既不同于经典的Ⅲ型爆发,也不同于spike和Ⅰ型爆发,是一种新的米波爆发型别。它的特性与分米波的“blips“相近。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/38827
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
郑向民,马媛,夏志国,等. 米波窄带快频漂射电爆发??"Blips"的观测和证认[J]. 天体物理学报,1994,014(001):72.
APA 郑向民,马媛,夏志国,&陈敬英.(1994).米波窄带快频漂射电爆发??"Blips"的观测和证认.天体物理学报,014(001),72.
MLA 郑向民,et al."米波窄带快频漂射电爆发??"Blips"的观测和证认".天体物理学报 014.001(1994):72.
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