Automated Author ProfilePayne, Dominic
Payne, Dominic
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: 5.8 (sum of 3 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
The data sets and python notebook included are for a submitted manuscript to the Journal of Geophysical Review: Space Physics. An IDL save file has also been included which contains variables from a reconstruction of the event in the manuscript. The time variable in tt2000. Other variables are in units of nW/m^3 by default.
The purpose of the work is to determine how electromagnetic energy is converted into plasma energy in the electron diffusion region of magnetic reconnection. Using both spacecraft data and simulations, we investigate how the terms in Poynting's theorem change as reconnection begins and evolves in time.
Authors
- Payne, Dominic ;
- Genestreti, Kevin ;
- Germaschewski, Kai ;
- Argall, Matthew ;
- Torbert, Roy ;
- Dors, Ivan ;
- Ardakani, Akhtar
The data sets and python notebook included are for a submitted manuscript to the Journal of Geophysical Review: Space Physics. An IDL save file has also been included which contains variables from a reconstruction of the event in the manuscript. The time variable in tt2000. Other variables are in units of nW/m^3 by default.
The purpose of the work is to determine how electromagnetic energy is converted into plasma energy in the electron diffusion region of magnetic reconnection. Using both spacecraft data and simulations, we investigate how the terms in Poynting's theorem change as reconnection begins and evolves in time.
Authors
- Payne, Dominic ;
- Genestreti, Kevin ;
- Germaschewski, Kai ;
- Argall, Matthew ;
- Torbert, Roy ;
- Dors, Ivan ;
- Ardakani, Akhtar
The data sets and python notebook included are for a submitted manuscript to the Journal of Geophysical Review: Space Physics. An IDL save file has also been included which contains variables from a reconstruction of the event in the manuscript. The time variable in tt2000. Other variables are in units of nW/m^3 by default.
The purpose of the work is to determine how electromagnetic energy is converted into plasma energy in the electron diffusion region of magnetic reconnection. Using both spacecraft data and simulations, we investigate how the terms in Poynting's theorem change as reconnection begins and evolves in time.
Authors
- Payne, Dominic ;
- Genestreti, Kevin ;
- Germaschewski, Kai ;
- Argall, Matthew ;
- Torbert, Roy ;
- Dors, Ivan ;
- Ardakani, Akhtar