The existing database for paleointensity estimates of the ancient geomagnetic field contains more than 1500 data points collected through decades of effort. Despite the huge amount of work put into obtaining these data, there remains a strong bias in the age and global distribution of the data toward very young results from a few locations. Also, few of the data meet strict criteria for reliability and most are of unknown quality. In order to improve the age and spatial distribution of the paleointensity database, we have carried out paleointensity experiments on submarine basaltic glasses from a number of DSDP sites. Of particular interest are the sites that provide paleointensity data spanning the time period 0.3-5 Ma, a time of relativel...
[1] Time domain correlations of common features among relative paleointensity records from sedimenta...
International audienceHigh-resolution records of the relative paleointensity of the geomagnetic fiel...
Reliable palaeointensities (PIs) are necessary to determine the full vector variation of Earth’s mag...
The existing database for paleointensity estimates of the ancient geomagnetic field contains more th...
The existing database for paleointensity estimates of the ancient geomagnetic field contains more th...
Through several decades of research, absolute paleointensity estimates have been obtained from a wid...
In contrast to our detailed knowledge of the directional behaviour of the Earth's magnetic field du...
[1] Placing accurate age constraints on near-axis lava flows has become increasingly important given...
Tholeiite of the oldest oceanic crust was drilled during ODP Legs 129 and 185 at Hole 801C in the we...
Earth's magnetic environment is dominated by its mainly dipolar internally generated magnetic field....
Thellier–Thellier paleointensity experiments were conducted on a collection of glasses from three ve...
The selection of paleointensity data is a challenging, but essential step for establishing data reli...
Determining the strength of the ancient geomagnetic field (paleointensity) can be time consuming and...
[1] We present here new paleointensity data from 39 sampling sites collected from the quenched margi...
Ocean Drilling Program Sites 883 and 884 were cored as part of a three-site depth transect down the ...
[1] Time domain correlations of common features among relative paleointensity records from sedimenta...
International audienceHigh-resolution records of the relative paleointensity of the geomagnetic fiel...
Reliable palaeointensities (PIs) are necessary to determine the full vector variation of Earth’s mag...
The existing database for paleointensity estimates of the ancient geomagnetic field contains more th...
The existing database for paleointensity estimates of the ancient geomagnetic field contains more th...
Through several decades of research, absolute paleointensity estimates have been obtained from a wid...
In contrast to our detailed knowledge of the directional behaviour of the Earth's magnetic field du...
[1] Placing accurate age constraints on near-axis lava flows has become increasingly important given...
Tholeiite of the oldest oceanic crust was drilled during ODP Legs 129 and 185 at Hole 801C in the we...
Earth's magnetic environment is dominated by its mainly dipolar internally generated magnetic field....
Thellier–Thellier paleointensity experiments were conducted on a collection of glasses from three ve...
The selection of paleointensity data is a challenging, but essential step for establishing data reli...
Determining the strength of the ancient geomagnetic field (paleointensity) can be time consuming and...
[1] We present here new paleointensity data from 39 sampling sites collected from the quenched margi...
Ocean Drilling Program Sites 883 and 884 were cored as part of a three-site depth transect down the ...
[1] Time domain correlations of common features among relative paleointensity records from sedimenta...
International audienceHigh-resolution records of the relative paleointensity of the geomagnetic fiel...
Reliable palaeointensities (PIs) are necessary to determine the full vector variation of Earth’s mag...