| The Response of Debris-Flow Events to Solar Proton Flares （Ⅰ） |
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| 引用本文： | DING Mingtao WEI Fangqiang ZHANG Jinghong WANG Hongjuan. The Response of Debris-Flow Events to Solar Proton Flares （Ⅰ）[J]. 武汉大学学报:自然科学英文版, 2007, 12(4): 599-604. DOI: 10.1007/s11859-006-0334-4 |
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| 作者姓名： | DING Mingtao WEI Fangqiang ZHANG Jinghong WANG Hongjuan |
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| 作者单位： | [1]Key Laboratory of Motmtain Hazards and Surface Process, Chinese Academy of Sciences/Institute of Mountain Hazards and Environment, Chinese Academy of Sciences, Chengdu 610041, Sichuan, China [2]Graduate University of Chinese Academy of Sciences, Beijing 100049, China [3]Hainan Meteorological and Ecological Academy, Haikou 570203, Hainan, China [4]National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, Yunnan, China |
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| 基金项目： | Supported by the Knowledge Innovation Program of Chinese Academy Sciences （KZX3-SW-352） and Frontier Program of Institute of Mountain Hazards and Environment, CAS （C3200307） |
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| 摘 要： | By analyzing the observation data from Dongchuan Debris Flow Observation and Research Station and historical data from year 1965 to 1990 gotten from National Astronomical Ob-servatories/Yunnan Observatory,the responding of debris flow in Jiangjia Ravine to Solar Proton Flare is studied. The following conclusion can be drawn. Solar Proton Flare,as one of most im-portant astronomical factors,affects the activity of debris flow in Yunnan. Generally,from 1965 to1990,the more active Solar Pro-ton Flare is,the greater the probability of high frequency and large runoff of debris flow is. On the contrary,the less active Solar Pro-ton Flare is,the greater the probability of low frequency,small runoff,and low sediment transport of debris flow is.
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| 关 键 词： | 泥石流 太阳活动 太阳质子耀斑 云南 |
| 文章编号： | 1007-1202（2007）04-0599-06 |
| 收稿时间： | 2006-11-03 |
| 修稿时间： | 2006-11-03 |
The response of debris-flow events to solar proton flares (I) |
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| Ding Mingtao,Wei Fangqiang,Zhang Jinghong,Wang Hongjuan. The response of debris-flow events to solar proton flares (I)[J]. Wuhan University Journal of Natural Sciences, 2007, 12(4): 599-604. DOI: 10.1007/s11859-006-0334-4 |
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| Authors: | Ding Mingtao Wei Fangqiang Zhang Jinghong Wang Hongjuan |
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| Affiliation: | (1) Key Laboratory of Mountain Hazards and Surface Process, Chinese Academy of Sciences, Chengdu, 610041, Sichuan, China;(2) Institute of Mountain Hazards and Environment, Chinese Academy of Sciences, Chengdu, 610041, Sichuan, China;(3) Graduate University of Chinese Academy of Sciences, Beijing, 100049, China;(4) Hainan Meteorological and Ecological Academy, Haikou, 570203, Hainan, China;(5) National Astronomical Observatories, Chinese Academy of Sciences, Kunming, 650011, Yunnan, China;(6) Yunnan Observatory, Chinese Academy of Sciences, Kunming, 650011, Yunnan, China |
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| Abstract: | By analyzing the observation data from Dongchuan Debris Flow Observation and Research Station and historical data from year 1965 to 1990 gotten from National Astronomical Observatories/ Yunnan Observatory, the responding of debris flow in Jiangjia Ravine to Solar Proton Flare is studied. The following conclusion can be drawn. Solar Proton Flare, as one of most important astronomical factors, affects the activity of debris flow in Yunnan. Generally, from 1965 to 1990, the more active Solar Proton Flare is, the greater the probability of high frequency and large runoff of debris flow is. On the contrary, the less active Solar Proton Flare is, the greater the probability of low frequency, small runoff, and low sediment transport of debris flow is. |
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| Keywords: | Solar Proton Flare debris flow Jiangjia Ravine in Yunnan |
| 本文献已被 CNKI 维普 SpringerLink 等数据库收录！ |
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