关于太阳白光耀斑连续发射起源的讨论
文献类型：期刊论文
| 作者 | 甘为群 |
| 刊名 | 天文学报
 |
| 出版日期 | 1997 |
| 卷号 | 38期号:4页码:394-396 |
| 关键词 | 太阳 白光耀斑 |
| ISSN号 | 0001-5245 |
| 中文摘要 | At present there are three kinds of explanations of the origin of solar white-lightflares. One view holds that the chromospheric condensation is responsible for thecontinuous emission of white-light flares, either belonging to type Ⅰ or type ⅡAnother interpretation snys that the non-thermal effects may increase the opacity ofthe upper photosphere and consequently the deeper layers can be heated radiatively.The still other view is that the strong chromospheric heating can radatively heat thetemperature minimum region and the upper photosphere. We examine each of thesemechanisms and point out that none of them may be considered to be quitesatisfactory in interpreting the continua of white-light flares. Then a possible outlet istentatively proposed, which may take into account both chromospheric condensationand non-thermal effects. A semiempirical model will be requlred to justify thissuggestion. |
| 学科主题 | 天文和天体物理 |
| 公开日期 | 2012-02-07 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/3198]  |
| 专题 | 紫金山天文台_PMO中文期刊 |
| 推荐引用方式 GB/T 7714 | 甘为群. 关于太阳白光耀斑连续发射起源的讨论[J]. 天文学报,1997,38(4):394-396. |
| APA | 甘为群.(1997).关于太阳白光耀斑连续发射起源的讨论.天文学报,38(4),394-396. |
| MLA | 甘为群."关于太阳白光耀斑连续发射起源的讨论".天文学报 38.4(1997):394-396. |
入库方式： OAI收割
来源：紫金山天文台
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