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强流星雨及其灾害性空间天气事件的观测与研究
  • ISSN号:0001-5245
  • 期刊名称:《天文学报》
  • 时间:0
  • 分类:P134[天文地球—天体力学;天文地球—天文学]
  • 作者机构:[1]中国科学院紫金山天文台,南京210008, [2]中国电波传播研究所,新乡453003
  • 相关基金:国家自然科学基金委员会(批准号:10273024,10573037,10503013,10778637)和小行星基金会资助
中文摘要:

在首届狮子座强流星雨国际联测期间,开展了多学科、多手段的狮子座和天龙座强流星雨及其灾害性空间天气事件的综合观测,并结合近半个世纪的(1957-2003年)狮子座、英仙座和天龙座强流星雨及其相关资料的综合分析,充分证实了非偶现的周期性强流星雨可导致灾害性空间天气事件的形成.下述结论亦得到初步证认:强流星雨形成机制;fbEs异常峰出现规律;对宇航安全的严重危害.文中还对彗星尘演化过程、宇宙尘暴出现和丢失规律及中纬区Es层宇宙尘维持机制作了讨论.

英文摘要:

During the first international joint observation for strong meteor shower we made multi-subject observations for Leonids and Draconids and their disaster space weather events by several methods. Combining the synthetical analysis of Leonids, Perseids and Draconids and their related data from 1957 to 2003, we sufficiently confirm that the periodic strong meteor showers can result in the formation of catastrophic space weather events. The following summing-up is confirmed basically: 1. The formation mechanism of the strong meteor shower There are meteoroids with high density and uneven distribution close the cometary nucleus, especially in the direction of opposite the Sun and backside of the nucleus. They can stretch 1-11 AU along the cometary orbit and 1-5 (×10-3 AU) cross the orbit. Therefore good displays of meteor shower (10-100 times as usual) or storms (103-104 times as usual) can occur when the Earth passes a high density meteoroid stream during the period of 3 years before and 5 years after the perihelion passage of the comet. During that period, bolides or shooting stars which are serious harmful to spaceflight security increase greatly to 3%~10%. This corrects the wrong point of view that the harmful micro-meteoroids to spaceflight security in period meteor showers are 〈 1g only. 2. The cosmic dust maintaining mechanism of long-life Es layer in mid-latitude area It is proved the life of Es layer increased greatly when most ions are long-life metal type ions (Fe^+, Mg^+……) which composite coefficient is much smaller than that of molecule type ions(O2^+, NO^+……). The observation for about 50 years roughly approves that the blanketing frequency of Es layer (fbEs) abnormally increase in large area (〉 105 km^2) and lasting long time (〉 15 min) only when strong meteor shower occurred at night. It is not f, l and c type Es layer evolved from sequence Es layer. This shows that the cause of fbEs increase is that the ionosphere was bombarded by

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期刊信息
  • 《天文学报》
  • 中国科技核心期刊
  • 主管单位:中国科学院
  • 主办单位:中国天文学会 中国科学院紫金山天文台
  • 主编:甘为群
  • 地址:南京市栖霞区元化路8号
  • 邮编:210023
  • 邮箱:twxb@pmo.ac.cn
  • 电话:025-83332133
  • 国际标准刊号:ISSN:0001-5245
  • 国内统一刊号:ISSN:32-1113/P
  • 邮发代号:2-818
  • 获奖情况:
  • 1992年获中国科协优秀期刊三等奖,1996年获中国科学院优秀期刊三等奖,2000年获中国科协优秀期刊三等奖,中国期刊方阵“双效”期刊
  • 国内外数据库收录:
  • 日本日本科学技术振兴机构数据库,中国中国科技核心期刊,中国北大核心期刊(2004版),中国北大核心期刊(2008版),中国北大核心期刊(2011版),中国北大核心期刊(2014版),中国北大核心期刊(2000版)
  • 被引量:1792