dc.description
References:
- Montabone, L., Forget, F., Millour, E., Wilson, R.J., Lewis, S.R., Cantor, B., Kass, D., Kleinböhl, A., Lemmon, M.T., Smith, M.D., Wolff, M.J., Eight-year Climatology of Dust Optical Depth on Mars. Icarus 251, pp. 65-95 (2015), doi: https://doi.org/10.1016/j.icarus.2014.12.034
- Montabone, L., Spiga, A., Kass, D. M., Kleinböhl, A., Forget, F., Millour, E., Martian Year 34 Column Dust Climatology from Mars Climate Sounder Observations: Reconstructed Maps and Model Simulations. J. Geophys. Res. - Planets (2020), doi: https://doi.org/10.1029/2019JE006111
- Saidel, Morgan; Wang, Huiqun (Helen); Battalio, Michael J.; Toigo, Anthony D.; Richardson, Mark, I., 2022, "Mars Dust Storm Sequence Dataset (MDSSD)", https://doi.org/10.7910/DVN/0XB6KN, Harvard Dataverse, V6
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dc.description.abstract
This dataset contains two sets of Mars atmospheric dust scenarios based on the daily maps of the column dust optical depth (CDOD) from Montabone et al. (2015, 2020). The first set contains 7 artificial dust scenarios with shifted timings of the Mars Year 25 global dust event (Ls=150° to Ls=330°, in steps of 30° of Ls). The second set contains dust scenarios for Mars Years 29 to 33, with additional storms shapes from the Mars Dust Storm Sequence Database (Saidel et al., 2022). For the MDSSD storms, a homogeneous storm CDOD of 0.6 (at 9.3 µm) was assumed. All these scenarios can be used to model the dust cycle in the LMD Mars Planetary Climate Model.
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refubium.note.author
The Mars Dust Storm sequence database, that was also used to construct this dataset, are distributed under a CC0 1.0 licence (see https://doi.org/10.7910/DVN/0XB6KN).
The maps from Montabone et al. (2015, 2020), on which this dataset is based, are distributed under a CC BY-SA 3.0 licence (see https://www-mars.lmd.jussieu.fr/mars/dust_climatology/index.html). Therefore, the present data also uses a CC BY-SA licence.
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