The determination of cosmogenic 53Mn in terrestrial archives has important applications, such as burial ages, exposure age and erosion rates. Accelerator mass spectrometry (AMS) is the most sensitive technique to detect minute amounts of 53Mn. 53Mn measurements were developed at the China Institute of Atomic nergy (CIAE) using the DE-Q3D equipped AMS system. This approach was recently optimized with the goal to reach the sensitivity required for AMS measurements of 53Mn in deep-sea ferromanganese crust (DSFC) samples. Based on these improvements of sample preparation, current beam transmission and so on, 53Mn in two samples of DSFC was measured by AMS. The ratios of 53Mn/Mn corresponding to an age of 3.77 ± 0.42 and 13.73 ± 2.74 Ma by 129...
AbstractThe Accelerator Mass Spectrometry (AMS) program at the Nuclear Science Laboratory of the Uni...
We summarize some recent cross-section measurements using accelerator mass spectrometry (AMS). AMS r...
The extinct p-process nuclide 146Sm (t1/2 = 103 ± 5 Myr) is known to have been present in the Early-...
The cosmogenic isotope 53Mn is produced by spallation of iron in surface rocks. The long half life o...
Terrestrial cosmogenic nuclides have become an indispens-able tool in Earth sciences, particularly f...
Accelerator Mass Spectrometry (AMS) is a single-atom counting technique that measures the abund...
Accelerator mass spectrometry (AMS) has a great potential for various geological applications. The p...
The 53Mn flux onto Earth is a quantity relevant for different extraterrestrial and astrophysical que...
A new accelerator mass spectrometer was successfully designed for the Cologne FN accelerator to enla...
Samples of two deep-sea sediment cores from the Indian Ocean are analyzed with accelerator mass spec...
We summarize some recent cross-section measurements using accelerator mass spectrometry (AMS). AMS r...
Accelerator mass spectrometry (AMS) measurement of 59Ni has been established at CIAE with the HI-13 ...
Mean age of galactic cosmic rays technique based on manganese isotope half life passing through inte...
From the 18th International Radiocarbon Conference held in Wellington, New Zealand, September 1-5, 2...
A new generation accelerator mass spectrometer (AMS) is operational since May 1994 at the Centre for...
AbstractThe Accelerator Mass Spectrometry (AMS) program at the Nuclear Science Laboratory of the Uni...
We summarize some recent cross-section measurements using accelerator mass spectrometry (AMS). AMS r...
The extinct p-process nuclide 146Sm (t1/2 = 103 ± 5 Myr) is known to have been present in the Early-...
The cosmogenic isotope 53Mn is produced by spallation of iron in surface rocks. The long half life o...
Terrestrial cosmogenic nuclides have become an indispens-able tool in Earth sciences, particularly f...
Accelerator Mass Spectrometry (AMS) is a single-atom counting technique that measures the abund...
Accelerator mass spectrometry (AMS) has a great potential for various geological applications. The p...
The 53Mn flux onto Earth is a quantity relevant for different extraterrestrial and astrophysical que...
A new accelerator mass spectrometer was successfully designed for the Cologne FN accelerator to enla...
Samples of two deep-sea sediment cores from the Indian Ocean are analyzed with accelerator mass spec...
We summarize some recent cross-section measurements using accelerator mass spectrometry (AMS). AMS r...
Accelerator mass spectrometry (AMS) measurement of 59Ni has been established at CIAE with the HI-13 ...
Mean age of galactic cosmic rays technique based on manganese isotope half life passing through inte...
From the 18th International Radiocarbon Conference held in Wellington, New Zealand, September 1-5, 2...
A new generation accelerator mass spectrometer (AMS) is operational since May 1994 at the Centre for...
AbstractThe Accelerator Mass Spectrometry (AMS) program at the Nuclear Science Laboratory of the Uni...
We summarize some recent cross-section measurements using accelerator mass spectrometry (AMS). AMS r...
The extinct p-process nuclide 146Sm (t1/2 = 103 ± 5 Myr) is known to have been present in the Early-...