On the positronium continuum and 0.511 MeV line in solar flares | |
Gan, WQ; Chang, J; Li, YP; Su, Y; Miroshnichenko, LI | |
刊名 | CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS |
2004-08-01 | |
卷号 | 4期号:4页码:357-364 |
关键词 | sun : flares sun : X-rays, gamma-rays |
ISSN号 | 1009-9271 |
英文摘要 | We have studied the influence of the density of the annihilation region on the positronium continuum. A relation between the ratio 3gamma/2gamma and the density is explicitly given, with which one can derive directly from the observed 3gamma/2gamma the density where the annihilation occurs. A unique solution may be found from the observed width of the 0.511 MeV line. We applied the method to three flares observed by GRS/SMM. It is shown that due to the measuring uncertainties in the 0.511 MeV line width, we cannot distinguish a chromospheric source from a coronal source, though both accurately localized. To improve the measuring accuracy of the 0.511 MeV line and the ratio 3gamma/2gamma will be an important step for a better understanding of the annihilation process in solar flares. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | CHROMOSPHERIC FLARE ; MAXIMUM-MISSION ; MAGNETIC LOOPS ; EMISSION ; MODELS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000223524200007 |
公开日期 | 2012-12-22 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/7726] |
专题 | 紫金山天文台_太阳高能及相关物理过程研究团组 |
作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 2.IZMIRAN, Troitsk 142190, Moscow Region, Russia |
推荐引用方式 GB/T 7714 | Gan, WQ,Chang, J,Li, YP,et al. On the positronium continuum and 0.511 MeV line in solar flares[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2004,4(4):357-364. |
APA | Gan, WQ,Chang, J,Li, YP,Su, Y,&Miroshnichenko, LI.(2004).On the positronium continuum and 0.511 MeV line in solar flares.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,4(4),357-364. |
MLA | Gan, WQ,et al."On the positronium continuum and 0.511 MeV line in solar flares".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 4.4(2004):357-364. |
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