Solar flares with similar soft but different hard X-ray emissions:case and statistical studies | |
Sharykin Ivan N1; Struminsky Alexei B1; Zimovets Ivan V1; Gan Weiqun2 | |
刊名 | Research in Astronomy and Astrophysics |
2016 | |
卷号 | 16期号:1页码:05 |
ISSN号 | 1674-4527 |
英文摘要 | From the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) catalog we select events which have approximately the same GOES class (high C -low M or 500–1200 counts s–1 within the RHESSI 6–12 keV energy band), but with different maximal energies of detected hard X-rays. The selected events are subdivided into two groups:(1) flares with X-ray emissions observed by RHESSI up to only 50 keV and (2) flares with hard X-ray emission observed also above 50 keV. The main task is to understand observational peculiarities of these two flare groups.We use RHESSI X-ray data to obtain spectral and spatial information in order to find differences between selected groups. Spectra and images are analyzed in detail for six events (case study). For a larger number of samples (85 and 28 flares in the low-energy and high-energy groups respectively) we only make some generalizations. In spectral analysis we use the thicktarget model for hard X-ray emission and one temperature assumption for thermal soft X-ray emission. RHESSI X-ray images are used for determination of flare region sizes. Although thermal and spatial properties of these two groups of flares are not easily distinguishable, power law indices of hard X-rays show significant differences. Events from the high-energy group generally have a harder spectrum. Therefore, the efficiency of chromospheric evaporation is not sensitive to the hardness of nonthermal electron spectra but rather depends on the total energy flux of nonthermal electrons. |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://libir.pmo.ac.cn/handle/332002/29457] |
专题 | 中国科学院紫金山天文台 |
作者单位 | 1.Space Research Institute, Russian Academy of Sciences 2.中国科学院紫金山天文台 |
推荐引用方式 GB/T 7714 | Sharykin Ivan N,Struminsky Alexei B,Zimovets Ivan V,et al. Solar flares with similar soft but different hard X-ray emissions:case and statistical studies[J]. Research in Astronomy and Astrophysics,2016,16(1):05. |
APA | Sharykin Ivan N,Struminsky Alexei B,Zimovets Ivan V,&Gan Weiqun.(2016).Solar flares with similar soft but different hard X-ray emissions:case and statistical studies.Research in Astronomy and Astrophysics,16(1),05. |
MLA | Sharykin Ivan N,et al."Solar flares with similar soft but different hard X-ray emissions:case and statistical studies".Research in Astronomy and Astrophysics 16.1(2016):05. |
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