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Data accompanying the paper: Is Io's volcanic distribution controlled by a convective layer?

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posted on 08.05.2020, 00:00 by Teresa Steinke, D. (Duncan) Van Sliedrecht
Two sets of Io's volcanic features locations adopted from previous publications, fitted and filtered for the comparision with interior convection dynamics. Set-1 ('active'): Based on active hot-spots (de Kleer et al. 2019, Mura et al. 2020, Davies et al., 2015) Set-2 ('hamilton'): Based on data set 1 and 2 in supplementary material of Hamilton et al, 2013)

Funding

User Support Programme 710 Space Research, ALW-GO/15-07

History

Contributors

TU Delft, Faculty of Aerospace Engineering, Department of Space Engineering

Publisher

4TU.Centre for Research Data

Time coverage

2000/2019

Geolocation

Jupiter moon Io,

Format

media types: application/x-matlab-data, application/zip, text/plain

Usage metrics

Delft University of Technology

Licence

Exports