Geomagnetic field intensity between 70000 and 130000 years BP from a volcanic sequence on La Reunion, Indian Ocean

被引:25
作者
Rais, A [1 ]
Laj, C [1 ]
Surmont, J [1 ]
Gillot, PY [1 ]
Guillou, H [1 ]
机构
[1] CNRS,CEA,CTR FAIBLES RADIOACTIV,LAB MIXTE,F-91198 GIF SUR YVETTE,FRANCE
关键词
Piton des Neiges; natural remanent magnetism; paleomagnetism; magnetic intensity;
D O I
10.1016/0012-821X(96)00024-6
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
A detailed paleointensity study was made of a sequence of 70 successive lava flows of the Piton des Neiges volcano on the island of La Reunion (Indian Ocean). Radiometric dating brackets the age of this sequence between 130 +/- 3 ka and 72 +/- 3 ka. Rock magnetic investigations show that titanomagnetites in the pseudo single domain range are the main magnetic carrier of the Natural Remanent Magnetisation (NRM). Over 350 samples were used for paleointensity determinations carried out with the Thellier method in vacuum or in an argon atmosphere. Of these, 89 samples yielded reliable results, with within-flow scatter often lower than 20%. These results indicate that the geomagnetic field intensity has varied at La Reunion between 13 and 65 mu T during the period of time explored. The average value, 42 mu T, is higher than the present field at La Reunion (35 mu T). The results from the upper part of the section are consistent with previous results obtained for the 82-98 ka period also at La Reunion [1] and document a broad low around 95 ka, not associated with large directional changes. On a larger geographic scale, the paleointensity values from La Reunion are significantly higher than those obtained from Mount Etna [2]. Precise comparison is, however, difficult because of the lack of detail in the Etna results. In the lower part of the section, a marked intensity low, coinciding with significant deviation from the dipole field direction is observed at 115 ka and could correspond to the end of the Blake event.
引用
收藏
页码:173 / 189
页数:17
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