Automated Author ProfileJohnson, Catherine
University of British Columbia0000-0001-6084-0149
Johnson, Catherine
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: 3.6 (sum of 5 datasets Dataset Index scores)
More information here.
S-Index Over Time
Cumulative Citations Over Time
Cumulative Mentions Over Time
Datasets
No description available
Authors
- Tarduno, John A. ;
- Cottrell, Rory D. ;
- Lawrence, Kristin ;
- Bono, Richard K. ;
- Huang, Wentao ;
- Johnson, Catherine L. ;
- Blackman, Eric G. ;
- Smirnov, Aleksey V. ;
- Nakajima, Miki ;
- Neal, Clive R. ;
- Zhou, Tinghong ;
- Ibanez-Mejia, Mauricio ;
- Oda, Hirokuni ;
- Crummins, Ben
No description available
Authors
- Tarduno, John A. ;
- Cottrell, Rory D. ;
- Lawrence, Kristin ;
- Bono, Richard K. ;
- Huang, Wentao ;
- Johnson, Catherine L. ;
- Blackman, Eric G. ;
- Smirnov, Aleksey V. ;
- Nakajima, Miki ;
- Neal, Clive R. ;
- Zhou, Tinghong ;
- Ibanez-Mejia, Mauricio ;
- Oda, Hirokuni ;
- Crummins, Ben
e#output##.dat: Data and modeled results containing the topographic profiles and axisymmetric flexure modeling corresponding to figures 3a, 4a, and 5a. Two files for each profile exist corresponding to E = 5, 65 GPa.
Columns are as follows:
- profile #
- distance from beginning of profile (m)
- detrended stereo elevation (m)
- best fit he (km)
- modeled deflection outboard of load (m)
- radial flexural stress (Pa) ------------------------------------------------------------- fig3b_profile5.dat: Data corresponding to figure 3b, he vs RMS misfit for different combinations of r1 and r2 for profile 5. Columns are as follows:
- he (km)
- r1 (km)
- r2 (km)
- RMS misfit (m) ------------------------------------------------------------- fig_4b_all.dat: Data corresponding to figure 4b, he vs RMS misfit for all profiles. Columns are as follows:
- profile #
- he (km)
- RMS misfit (m) ------------------------------------------------------------- swath2_narina_clip.zip: - clip of the stereo-derived topography used for flexural modeling in this study - the zipfile contains a geotiff (geolocated tiff file for use in GIS software) and auxiliary files. - References below. Full documentation of the processing applied is now available at the PDS https://pds-geosciences.wustl.edu/mgn/urn-nasa-pds-magellan_stereo_topography/document/magellan_stereo_topography_description.pdf Herrick, R. R., Stahlke, D. L., & Sharpton, V. L. (2012). Fine‐scale Venusian topography from Magellan stereo data. Eos, Transactions American Geophysical Union, 93(12), 125-126. doi:10.1029/2012EO120002 Herrick, R. R. (2020). MGN RDRS Magellan Stereo-Derived Topography Mosaic (Derived Data). NASA Planetary Data System. doi:10.17189/1519332
Authors
- Russell, Megan B. ;
- Johnson, Catherine L.
e#output##.dat: Data and modeled results containing the topographic profiles and axisymmetric flexure modeling corresponding to figures 3a, 4a, and 5a. Two files for each profile exist corresponding to E = 5, 65 GPa.
Columns are as follows:
- profile #
- distance from beginning of profile (m)
- detrended stereo elevation (m)
- best fit he (km)
- modeled deflection outboard of load (m)
- radial flexural stress (Pa) ------------------------------------------------------------- fig3b_profile5.dat: Data corresponding to figure 3b, he vs RMS misfit for different combinations of r1 and r2 for profile 5. Columns are as follows:
- he (km)
- r1 (km)
- r2 (km)
- RMS misfit (m) ------------------------------------------------------------- fig_4b_all.dat: Data corresponding to figure 4b, he vs RMS misfit for all profiles. Columns are as follows:
- profile #
- he (km)
- RMS misfit (m) ------------------------------------------------------------- swath2_narina_clip.zip: - clip of the stereo-derived topography used for flexural modeling in this study - the zipfile contains a geotiff (geolocated tiff file for use in GIS software) and auxiliary files. - References below. Full documentation of the processing applied is now available at the PDS https://pds-geosciences.wustl.edu/mgn/urn-nasa-pds-magellan_stereo_topography/document/magellan_stereo_topography_description.pdf Herrick, R. R., Stahlke, D. L., & Sharpton, V. L. (2012). Fine‐scale Venusian topography from Magellan stereo data. Eos, Transactions American Geophysical Union, 93(12), 125-126. doi:10.1029/2012EO120002 Herrick, R. R. (2020). MGN RDRS Magellan Stereo-Derived Topography Mosaic (Derived Data). NASA Planetary Data System. doi:10.17189/1519332
Authors
- Russell, Megan B. ;
- Johnson, Catherine L.