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北京地区重力波活动及其波谱的季节分布特性研究
  • ISSN号:0254-6124
  • 期刊名称:Chinese Journal of Space Science
  • 时间:2015.8.1
  • 页码:453-460-
  • 分类:P351[天文地球—空间物理学;天文地球—地球物理学]
  • 作者机构:[1]中国科学院国家空间科学中心,北京100011, [2]海南师范大学物理与电子工程学院,海南海口571158, [3]中国科学院武汉物理与数学研究所,武汉430071
  • 相关基金:国家自然科学基金(NSFC40905012,41174129,41474130,41264006,41364005); 海南省自然科学基金(513146); 中国博士后项目基金(2012M520397); 中国科学院国家空间科学中心重点培育项目资助 致谢 本文得到了国家子午工程数据的大力支持,在此表示衷心的感谢.
  • 相关项目:子午工程光学手段研究中国上空中层顶区域重力波活动情况
作者: 邹旭|杨国韬|
中文摘要:

利用子午工程海南激光雷达对我国海南地区上空进行持续观测,通过3年的累积观测数据对我国低纬度地区重力波活动的季节分布特性进行研究,依据重力波线性理论对海南地区上空的大气密度扰动规律、空间功率谱及时间频率谱进行分析,并通过选择波长在1km至8km范围内具有特定波长以及具有波动周期为60 min至25min的特定频率的重力波辅助研究大气密度扰动的季节变化规律,总结得出海南地区重力波活动具有夏季大、春秋季小、而冬季依然频繁的季节性分布规律.结合海南地区特殊的地理位置与当地季节性气候特征分析得出海南地区上空重力波活动季节性变化的可能原因为青藏高原地形及我国南海地区存在的热带强对流与赤道潜流共同作用的结果.

英文摘要:

Sodium lidar is recognized as a useful tool to investigate gravity wave(GW)which influences the circulation,structure and composition of middle and upper atmosphere notably.For further understanding GW and their characteristics,more sufficient observational data within global models,especially those at low latitude are extremely expected.Meanwhile,long-term observations are also quite helpful for the GW analysis.As one part of Meridian Project,the observational Na lidar system at Hainan(19.50°N,109.1°E)employed the double wavelengths laser beam,which is consists of three channels for Mie scattering,Rayleigh scattering and broadband sodium fluorescence.A pulsed Nd:YAG laser was rebuilt to trigger off two green laser beams simultaneously,one of which was 532 nm and used to excite the Mie and Rayleigh scattering,and the other laser beam pumped by apulsed dye laser was about 589 nm and with 30 mJ per pulse.Resonant fluorescence from the sodium layer was received by a Cassegrain telescope with a primary mirror of 1000 mm diameter.The lidar profiles are stored automatically in a computer.The temporal and spatial resolution was about167 sand 96m,respectively.Seasonal variations of the GW activity and their spectra at Hainan were studied with comparison to the previous reports and the predictions of theories of GW saturation and dissipation.The seasonal variations of GW activity and characteristics spectra at Hainan are mainly presented as follows:(1)The mean RMS atmospheric density perturbation over Hainan are 5.63 %,which at solstice are obviously larger than that near the equinox.And the GW activity in winter is still active,which are quite different from those reports at the middle latitude area.(2)Due to the linear theory,the mspectra were calculated which show power law shapes and their range of variation were between-2.14and-3.56 with an annual mean value of-2.93.The calculatedωspectra were between-1.22and-2.36 with an annual mean value of-1.80,respectively.(3)The amplitudes of atmospher

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期刊信息
  • 《空间科学学报》
  • 北大核心期刊(2011版)
  • 主管单位:中国科学院
  • 主办单位:中科院空间中心
  • 主编:吴季
  • 地址:北京8701信箱
  • 邮编:100190
  • 邮箱:cjss@nssc.ac.cn
  • 电话:010-62582788
  • 国际标准刊号:ISSN:0254-6124
  • 国内统一刊号:ISSN:11-1783/V
  • 邮发代号:2-562
  • 获奖情况:
  • 核心期刊,中国期刊方阵“双效”期刊
  • 国内外数据库收录:
  • 俄罗斯文摘杂志,美国化学文摘(网络版),英国科学文摘数据库,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:3704