Satellite magnetic anomalies related to seafloor spreading in the South Atlantic Ocean

被引:17
作者
Purucker, ME
Dyment, J
机构
[1] NASA, Goddard Space Flight Ctr, Raytheon ITSS, Geodynam Branch, Greenbelt, MD 20771 USA
[2] Univ Bretagne Occidentale, CNRS UMR Domaines Ocean, Inst Univ Europeen Mer, Technopole Brest Iroise, F-29280 Plouzane, France
关键词
D O I
10.1029/1999GL008437
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Oceanic magnetic anomalies have been observed from satellite. The strongest anomalies are the long-wavelength components of the sea-floor spreading signature. Unfortunately, because of technical issues involving the treatment of satellite magnetic data, these signals are obscured in the South Atlantic Ocean because they trend north-south However, a map does exist in which such features are observed, essentially because of a better data processing technique. Further, this map agrees with a physically motivated model based on non-satellite magnetic input. Hence, with properly treated data, the magnetic anomaly maps should be useful for saying something about the geology, rather than vice-versa. This situation will be considerably improved by ongoing advances in methods and new data sets. The amplitude of the observations, a factor of two larger than previous estimates, confirms that the extrusive basaltic layer alone is inadequate to produce the signal and that deeper oceanic sources are required.
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收藏
页码:2765 / 2768
页数:4
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SABAKA TJ, 2000, NASATM2000209894