Automated Author Profile

Wang, Shuang

Laboratory for Climate and Ocean-Atmosphere Studies, Dept. of Atmospheric and Oceanic Sciences, School of Physics, Peking University, Beijing 100871, People's Republic of China
0000-0002-9406-1781

Current S-Index

2.2

Sum of Dataset Indices for all datasets

Average Dataset Index per Dataset

0.4

Average Dataset Index per dataset

Total Datasets

6

Total datasets for this author

Average FAIR Score

76.0%

Average FAIR Score per dataset

Total Citations

0

Total citations to the author's datasets

Total Mentions

0

Total mentions of the author's datasets

S-Index Interpretation

S-Index Over Time

Cumulative Citations Over Time

Cumulative Mentions Over Time

Datasets

Data for rotating penetrative plume

The ZIP file contains x–z cross-sections along y=0 for all non-rotating simulations.The remaining files provide y-averaged fields from the rotating simulations, which were used to generate the cross-section figures in the main text.Because the full dataset (including three-dimensional fields) is too large to be archived here, these data are available from the authors upon reasonable request.The two scripts are the Oceananigans scripts for simulating non-rotating (rF) and rotating (rT) plumes in this study.

Authors

  • Wang, Shuang
0 Citations0 Mentions77% FAIR0.4 Dataset Index
10.5281/zenodo.181094852026

Dataset for rotating point plumes in unstratified environment

Averaged (along y-axis) buoyancy field for rotating point plumes in XX. Any other large stored data supporting this work are available upon reasonable request. Please contact the corresponding author.

Authors

  • Wang, Shuang
0 Citations0 Mentions79% FAIR0.6 Dataset Index
10.5281/zenodo.155710092025

Dataset for rotating point plumes in unstratified environment

Averaged (along y-axis) buoyancy field for rotating point plumes in XX. Any other large stored data supporting this work are available upon reasonable request. Please contact the corresponding author.

Authors

  • Wang, Shuang
0 Citations0 Mentions73% FAIR0.4 Dataset Index
10.5281/zenodo.155710102025

Data for rotating penetrative plume

The ZIP file contains x–z cross-sections along y=0 for all non-rotating simulations.The remaining files provide y-averaged fields from the rotating simulations, which were used to generate the cross-section figures in the main text.Because the full dataset (including three-dimensional fields) is too large to be archived here, these data are available from the authors upon reasonable request.

Authors

  • Wang, Shuang
0 Citations0 Mentions81% FAIR0.4 Dataset Index
10.5281/zenodo.181094862025

Simulation and calculation data for the Lorenz energy cycle

The data are for the article "Lorenz Energy Cycle: Another Way to Understand the Atmospheric Circulation on Tidally Locked Terrestrial Planets". The data are simulated by the general circulation model ExoCAM. The horizontal resolution is 4°x5°. Note: ST: in standard coordinates; TL: in the tidally locked coordinates. The simulation data is daily-mean (i.e., '.daily.nc'), including: ST_5d_tidally_locked.cam.daily.nc, ST_60d_tidally_locked.cam.daily.nc (in the standard coordinates), and TL_60d_tidally_locked.cam.daily.nc (in the tidally locked coordinates). The LEC data are calculated by the LEC code released at https://doi.org/10.5281/zenodo.7472396, including: Earth: LEC_energy.1979-.nc and LEC_converse_rate.1979-*.nc Rapidly rotating tidally locked planet (in standard coordinates): ST_LEC_energy_5d_tidally_locked.nc and ST_LEC_conv-rate_5d_tidally_locked.nc Slowly rotating tidally locked planet (in tidally locked coordinates): TL_LEC_energy_60d_tidally_locked.nc and TL_LEC_conv-rate_60d_tidally_locked.nc Slowly rotating tidally locked planet (in standard coordinates): ST_LEC_energy_60d_tidally_locked.nc and ST_LEC_conv-rate_60d_tidally_locked.nc

Authors

  • Wang, Shuang
0 Citations0 Mentions73% FAIR0.4 Dataset Index
10.5281/zenodo.74760742022

Simulation and calculation data for the Lorenz energy cycle

The data are for the article "Lorenz Energy Cycle: Another Way to Understand the Atmospheric Circulation on Tidally Locked Terrestrial Planets". The data are simulated by the general circulation model ExoCAM. The horizontal resolution is 4°x5°. Note: ST: in standard coordinates; TL: in the tidally locked coordinates. The simulation data is daily-mean (i.e., '.daily.nc'), including: ST_5d_tidally_locked.cam.daily.nc, ST_60d_tidally_locked.cam.daily.nc (in the standard coordinates), and TL_60d_tidally_locked.cam.daily.nc (in the tidally locked coordinates). The LEC data are calculated by the LEC code released at https://doi.org/10.5281/zenodo.7472396, including: Earth: LEC_energy.1979-.nc and LEC_converse_rate.1979-*.nc Rapidly rotating tidally locked planet (in standard coordinates): ST_LEC_energy_5d_tidally_locked.nc and ST_LEC_conv-rate_5d_tidally_locked.nc Slowly rotating tidally locked planet (in tidally locked coordinates): TL_LEC_energy_60d_tidally_locked.nc and TL_LEC_conv-rate_60d_tidally_locked.nc Slowly rotating tidally locked planet (in standard coordinates): ST_LEC_energy_60d_tidally_locked.nc and ST_LEC_conv-rate_60d_tidally_locked.nc

Authors

  • Wang, Shuang
0 Citations0 Mentions73% FAIR0.4 Dataset Index
10.5281/zenodo.74760732022