Automated Author ProfileVan Westrenen, W.
Faculty of Science, VU Amsterdam, Amsterdam, The Netherlands
Van Westrenen, W.
Current S-Index
Sum of Dataset Indices for all datasets
Average Dataset Index per Dataset
Average Dataset Index per dataset
Total Datasets
Total datasets for this author
Average FAIR Score
Average FAIR Score per dataset
Total Citations
Total citations to the author's datasets
Total Mentions
Total mentions of the author's datasets
S-Index Interpretation
The S-Index (Sharing Index) is a comprehensive metric that represents the cumulative impact of all your datasets. It is calculated as the sum of Dataset Index scores across all your claimed datasets.
What it means:
- A higher S-index indicates greater overall impact of your datasets relative to typical datasets in their fields of research
- The S-Index grows as you add more datasets or as existing datasets gain more citations and mentions
- It provides a single number to track your research data impact over time
Current S-Index: 2.6 (sum of 14 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
The depletions of potassium (K) and sodium (Na) in samples from planetary interiors have long been considered as primary evidence for their volatile behavior during planetary formation processes. Here, we use high-pressure experiments combined with laser ablation analyses to measure the sulfide-silicate and metal-silicate partitioning of K and Na at high pressure (P) – temperature (T) and find that their partitioning into metal strongly increases with temperature. Results indicate that the observed Vestan and Martian mantle K and Na depletions can reflect sequestration into their sulfur-rich cores in addition to their volatility during formation of Mars and Vesta. This suggests that alkali depletions are not affected solely by incomplete condensation or partial volatilization during planetary formation and differentiation, but additionally or even primarily reflect the thermal and chemical conditions during core formation. Core sequestration is also significant for the Moon, but lunar mantle depletions of K and Na cannot be reconciled by core formation only. This supports the hypothesis that measured isotopic fractionations of K in lunar samples represent incomplete condensation or extensive volatile loss during the Moon-forming giant impact.
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.
:unav
Authors
- Steenstra, E.S. ;
- Agmon, N. ;
- Berndt, J. ;
- Klemme, S. ;
- Matveev, S. ;
- Van Westrenen, W.