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Equatorward shift of annual Rossby waves in the Equatorial Pacific Ocean 被引量:2
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作者 马晓 孙澈 《Chinese Journal of Oceanology and Limnology》 SCIE CAS CSCD 2016年第1期212-218,共7页
Annual Rossby wave is a key component of the ENSO phenomenon in the equatorial Pacific Ocean. Due to the paucity and seasonal bias in historical hydrographic data,previous studies on equatorial Rossby waves only gave ... Annual Rossby wave is a key component of the ENSO phenomenon in the equatorial Pacific Ocean. Due to the paucity and seasonal bias in historical hydrographic data,previous studies on equatorial Rossby waves only gave qualitative description. The accumulation of Argo measurements in recent years has greatly alleviated the data problem. In this study,seasonal variation of the equatorial Pacific Ocean is examined with annual harmonic analysis of Argo gridded data. Results show that strong seasonal signal is present in the western equatorial Pacific and explains more than 50% of the thermal variance below 500 m. Lag-correlation tracing further shows that this sub-thermocline seasonal signal originates from the eastern equatorial Pacific via downward and southwestward propagation of annual Rossby waves. Possible mechanisms for the equatorward shift of Rossby wave path are also discussed. 展开更多
关键词 equatorial Pacific annual Rossby wave equatorward shift Argo profiles MOAA-GPV gridded data
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Case study of an Equatorial Plasma Bubble Event investigated by multiple ground-based instruments at low latitudes over China 被引量:3
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作者 LongChang Sun JiYao Xu +2 位作者 YaJun Zhu Wei Yuan XiuKuan Zhao 《Earth and Planetary Physics》 CSCD 2021年第5期435-449,共15页
Observational evidence is insufficient to understand how equatorial plasma bubbles(EPBs)form over low latitudes.The mechanism of plasma-density enhancement(formation of"plasma blobs")at low latitudes is in d... Observational evidence is insufficient to understand how equatorial plasma bubbles(EPBs)form over low latitudes.The mechanism of plasma-density enhancement(formation of"plasma blobs")at low latitudes is in dispute.In this paper,we use data from multiple ground-based instruments(one all-sky airglow imager,five digisondes,and one Fabry–Perot interferometer)to investigate the evolution of an EPB event that occurred at low latitudes over China on the night of 06 December 2015(06-Dec-2015).We provide observational evidence that an enhanced equatorward wind most likely induced by a substorm could have initiated the Rayleigh–Taylor instability(RTI)that destabilized several EPB depletions in an upwelling region of a large-scale wave-like structure(LSWS)in the bottomside ionosphere.Those EPB depletions were forced to surge poleward,from nearly 10°to 19°magnetic latitude,two hours before midnight.Smaller-scale bifurcations evolved rapidly from tips of airglow depletions by a secondary E×B instability when the aforementioned substorm-induced southwestward wind blew through.During the growth phase of the EPB depletions,a westward polarization electric field inside the LSWS is likely to have compressed plasma downward,inducing the two airglow-type blobs observed in the bottomside ionosphere,by a mechanism of LSWS-blob connection that we propose.We also provide observational evidence of brightness airglow depletions.We find that an enhanced poleward wind associated with a passing-by brightness wave(BW)is likely to have transported plasma to fill the airglow depletions,which finally evolved into brightness airglow structures.This study investigates the physical processes accompanied by the EPB event and those two-airglow blobs observed at low-latitudes over China. 展开更多
关键词 Equatorial Plasma Bubble plasma blobs Rayleigh–Taylor instability secondary E×B instability nighttime brightness wave large-scale wave-like structure enhanced equatorward(poleward)wind
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极光电集流纬度变化特征初步分析 被引量:4
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作者 万秉东 李敏 +2 位作者 王源 朱瑾 陈耿雄 《地球物理学进展》 CSCD 北大核心 2013年第4期1655-1661,共7页
为研究极光电集流地磁纬度分布特征,利用北半球SME台站提供的极光电集流指数,通过时序叠加的方法,分析98-07年极光电集流中心地磁纬度随季节和世界时的分布特征.通过对磁扰程度的分级,分析极光电集流地磁纬度随地磁扰动程度的变化特征.... 为研究极光电集流地磁纬度分布特征,利用北半球SME台站提供的极光电集流指数,通过时序叠加的方法,分析98-07年极光电集流中心地磁纬度随季节和世界时的分布特征.通过对磁扰程度的分级,分析极光电集流地磁纬度随地磁扰动程度的变化特征.结果表明:1)由于SME台站覆盖范围更广,更多地记录到最大的极光电集流强度,有利于研究极光电集流的变化特征;2)西向极光电集流纬度分布存在与强度相反的季节性变化特征,在春秋出现最低值,冬季、夏季出现最高值;3)在SML<2000nT时,西向极光电集流地磁纬度随着极光电集流强度的增强,近似以线性关系向低纬迁移.随后伴随SML的进一步增强,西向极光极光电集流中心地磁纬度仍有向低纬迁移的趋势,但主要是在磁纬62°N-63°N之间波动. 展开更多
关键词 极光电集流 纬度分布 低纬迁移
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