Evidence that the Natal Pulse involves the Agulhas Current to its full depth

被引:31
作者
Lutjeharms, JRE [1 ]
Boebel, O
van der Vaart, PCF
de Ruijter, WPM
Rossby, T
Bryden, HL
机构
[1] Univ Cape Town, Dept Oceanog, ZA-7700 Rondebosch, South Africa
[2] Southampton Oceanog Ctr, Southampton SO14 3ZH, Hants, England
[3] Univ Rhode Isl, Grad Sch Oceanog, Narragansett, RI 02882 USA
[4] Univ Utrecht, Inst Marine & Atmospher Res, NL-3584 CC Utrecht, Netherlands
关键词
D O I
10.1029/2000GL012639
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Natal Pulses are intermittent, solitary meanders on the trajectory of the otherwise remarkably stable northern Agulhas Current. They play disparate roles in the process of inter-ocean exchange. They have been thought to trigger the spawning of Agulhas Rings at the Agulhas Retroflection, but also to generate an upstream retroflection that prevents Agulhas water from reaching the inter-ocean boundary. For the Natal Pulse to be such a control it has to extend to considerable depths. We present the first hard evidence that demonstrates that the Natal Pulse is indeed an inherent property of the Agulhas Current throughout its full depth. Our data comprise Eulerian current meter observations and Lagrangian float trajectories in combination with sea-surface height and sea-surface temperature data. The results reveal the trapping of water within the Natal Pulse, its southward advection at a phase speed of about 11-12 cm s(-1), and rotation periods of 6 days.
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收藏
页码:3449 / 3452
页数:4
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