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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 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

Licence

Exports

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Licence

Exports