Automated Author ProfileDahmen, Nikolaj L.
Institute of Geophysics, ETH Zurich, Zurich, Switzerland0000-0002-9114-6747
Dahmen, Nikolaj L.
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: 7.1 (sum of 8 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
Denoised seismic event waveforms (20 sps): seismic data recorded by NASA InSight mission on Mars and processed as described with its advantages and limitations in: Dahmen, N., Clinton, J., Stähler, S., Meier, M.-A., Ceylan, S., Euchner, F., Kim, D. , Horleston, A, Durán, C.,Zenhäusern, G., Charalambous, C., Kawamura, T. and Giardini, D. (2024). Revisiting Martian Seismicity with Deep Learning-Based Denoising. Submitted to Geophysical Journal International.Velocity waveforms are in physical units, rotated to ZNE components with ID: XB.ELYDL.03.BHZ/N/E; based on original waveforms XB.ELYSE.02.BHZ/N/EMSEED fiiles for all event waveforms from the low frequency event family (based on revised version of Marsquake Service catalogue Version 14: https://doi.org/10.12686/a21) whenever 20 sps data are available.Read with ObsPy, e.g.: obspy.read('.../S0173a')
Authors
- Dahmen, Nikolaj
Denoised seismic event waveforms (20 sps): seismic data recorded by NASA InSight mission on Mars and processed as described with its advantages and limitations in: Dahmen, N., Clinton, J., Stähler, S., Meier, M.-A., Ceylan, S., Euchner, F., Kim, D. , Horleston, A, Durán, C.,Zenhäusern, G., Charalambous, C., Kawamura, T. and Giardini, D. (2024). Revisiting Martian Seismicity with Deep Learning-Based Denoising. Submitted to Geophysical Journal International.Velocity waveforms are in physical units, rotated to ZNE components with ID: XB.ELYDL.03.BHZ/N/E; based on original waveforms XB.ELYSE.02.BHZ/N/EMSEED fiiles for all event waveforms from the low frequency event family (based on revised version of Marsquake Service catalogue Version 14: https://doi.org/10.12686/a21) whenever 20 sps data are available.Read with ObsPy, e.g.: obspy.read('.../S0173a')
Authors
- Dahmen, Nikolaj
Supporting Material (JGR Planets, 2022JE007503) - contains: Extended marsquake catalogue List of all detections Sol-wise predictions Snapshot of MarsQuakeNet code MarsQuakeNet code (dynamic version) also available from: https://github.com/niko-d/MarsQuakeNet.git
Authors
- Dahmen, Nikolaj
Supporting Material (JGR Planets, 2022JE007503) - contains: Extended marsquake catalogue List of all detections Sol-wise predictions Snapshot of MarsQuakeNet code MarsQuakeNet code (dynamic version) also available from: https://github.com/niko-d/MarsQuakeNet.git
Authors
- Dahmen, Nikolaj
Supporting Material (JGR Planets, 2022JE007503) - contains: Extended marsquake catalogue List of all detections Sol-wise predictions Snapshot of MarsQuakeNet code MarsQuakeNet code (dynamic version) also available from: https://github.com/niko-d/MarsQuakeNet.git
Authors
- Dahmen, Nikolaj
Supporting Material (JGR Planets, 2022JE007503) includes extended marsquake catalogue, list of detections, and sol-wise predictions. Preprint available at: https://doi.org/10.1002/essoar.10512017.1
Authors
- Dahmen, Nikolaj
This repository contains derived data presented and described in the article “Super high frequency events: a new class of events recorded by the InSight seismometers on Mars” by Nikolaj L. Dahmen, John F. Clinton, Savas Ceylan, Martin van Driel, Domenico Giardini, Amir Khan, Simon C. Stähler, Maren Böse, Constantinos Charalambous, Anna Horleston, Taichi Kawamura, Guenolé Orhand-Mainsant, John-Robert Scholz, Fabian Euchner, William T. Pike, Renee C. Weber, Philippe Lognonné and William B. Banerdt, submitted to JGR Planets (2020). Information on the provided data is given in the README file
Authors
- Dahmen, Nikolaj L. ;
- Clinton, John F. ;
- Savas Ceylan ;
- Driel, Martin Van ;
- Giardini, Domenico ;
- Khan, Amir ;
- Stähler, Simon C. ;
- Böse, Maren ;
- Constantinos Charalambous ;
- Horleston, Anna ;
- Kawamura, Taichi ;
- Guenolé Orhand-Mainsant ;
- John-Robert Scholz ;
- Euchner, Fabian ;
- Pike, William T. ;
- Weber, Renee C. ;
- Lognonné, Philippe ;
- Banerdt, William B.
This repository contains derived data presented and described in the article “Super high frequency events: a new class of events recorded by the InSight seismometers on Mars” by Nikolaj L. Dahmen, John F. Clinton, Savas Ceylan, Martin van Driel, Domenico Giardini, Amir Khan, Simon C. Stähler, Maren Böse, Constantinos Charalambous, Anna Horleston, Taichi Kawamura, Guenolé Orhand-Mainsant, John-Robert Scholz, Fabian Euchner, William T. Pike, Renee C. Weber, Philippe Lognonné and William B. Banerdt, submitted to JGR Planets (2020). Information on the provided data is given in the README file
Authors
- Dahmen, Nikolaj L. ;
- Clinton, John F. ;
- Savas Ceylan ;
- Driel, Martin Van ;
- Giardini, Domenico ;
- Khan, Amir ;
- Stähler, Simon C. ;
- Böse, Maren ;
- Constantinos Charalambous ;
- Horleston, Anna ;
- Kawamura, Taichi ;
- Guenolé Orhand-Mainsant ;
- John-Robert Scholz ;
- Euchner, Fabian ;
- Pike, William T. ;
- Weber, Renee C. ;
- Lognonné, Philippe ;
- Banerdt, William B.