cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.10250492
title: D9_Ls270_conTIandA_RennoOutputs_7sols.nc.gz: MarsWRF output for southern summer solstice in Gale Crater, now produced using constant Albedo and Thermal Inertia, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model, now run using constant Albedo and Thermal Inertia, includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern summer solstice (Ls~270°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figure 7 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250435.v2
title: D7_2pm_winds_d04.txt: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain 9 times bigger than Gale Crater.

description: This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region centered on but 9 times larger than Gale Crater, output from domain 4 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250441.v2
title: D8_2pm_winds_d05.txt: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain covering Gale Crater.

description: <br>This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region covering Gale Crater, output from domain 5 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250492.v2
title: D9_Ls270_conTIandA_RennoOutputs_7sols.nc.gz: MarsWRF output for southern summer solstice in Gale Crater, now produced using constant Albedo and Thermal Inertia, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model, now run using constant Albedo and Thermal Inertia, includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern summer solstice (Ls~270°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figure 7 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250339
title: Statistics of the gene predictions of M. enterolobii (genome V1, INRA/JKI)

description: Overview of the results of the gene prediction step done using Eugene on the M. enterolobii genome (V1, INRA/JKI).Number of genes found, including protein-coding and non-coding, GG percent, etc...<br>
DOI: 10.6084/m9.figshare.10250435.v1
title: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain 9 times bigger than Gale Crater.

description: This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region centered on but 9 times larger than Gale Crater, output from domain 4 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250492.v1
title: MarsWRF output for southern summer solstice in Gale Crater, now produced using constant Albedo and Thermal Inertia, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model, now run using constant Albedo and Thermal Inertia, includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern summer solstice (Ls~270°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figure 7 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250441.v1
title: MarsWRF-predicted 2pm winds at 1.5m altitude for southern summer solstice in a domain covering Gale Crater.

description: <br>This file provides 2pm zonal and meridional winds averaged over 7 sols at southern summer solstice (Ls~270°) for a region covering Gale Crater, output from domain 5 of a MarsWRF simulation.<br><br>Variables included are: Lon (longitude in deg E), Lat (latitude in deg N), U (zonal wind in m/s), V (meridional wind in m/s). Every second domain 4 wind output is included.<br><br>These data are used to produce Figure 6 in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250339.v2
title: Statistics of the gene predictions of M. enterolobii (genome V1, INRA/JKI)

description: Overview of the results of the gene prediction step done using Eugene on the M. enterolobii genome (V1, INRA/JKI).Number of genes found, including protein-coding and non-coding, GG percent, etc...<br>
DOI: 10.6084/m9.figshare.10250339.v1
title: Statistics of the Eugene annotation

description: Overview of the results of the gene prediction step done using Eugene on the M. enterolobii genome (V1, INRA/JKI).Number of genes found, including protein-coding and non-coding, GG percent, etc...<br>
DOI: 10.6084/m9.figshare.10250300
title: D6_Ls180_RennoOutputs_7sols.nc.gz: MarsWRF output for southern spring equinox in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern spring equinox (Ls~180°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 8 and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10249796
title: D4_Ls000_RennoOutputs_7sols.nc.gz: MarsWRF output for southern fall equinox in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern fall equinox (Ls~0°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment.<br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br>These data are used to produce Figures (especially Figures 8 and Supplementary Figures S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon
DOI: 10.6084/m9.figshare.10250297
title: D5_Ls090_RennoOutputs_7sols.nc.gz: MarsWRF output for southern winter solstice in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern winter solstice (Ls~90°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 8 and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10249001
title: D3_Ls270_RennoOutputs_7sols.nc.gz: MarsWRF output for southern summer solstice in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern summer solstice (Ls~270°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 2-5, 7-8, and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10249016
title: Predicted proteins of M. enterolobii (genome V1, INRA/JKI)

description: The set of predicted proteins in the genome of Meloidogyne enterolobii (V1, INRA, JKI)The proteins as well as the genes were predicted using the Eugene pipeline, as explained in the preprint in bioRxiv<br>
DOI: 10.6084/m9.figshare.10249016.v1
title: Predicted proteins of M. enterolobii (genome V1, INRA/JKI)

description: The set of predicted proteins in the genome of Meloidogyne enterolobii (V1, INRA, JKI)The proteins as well as the genes were predicted using the Eugene pipeline, as explained in the preprint in bioRxiv<br>
DOI: 10.6084/m9.figshare.10250300.v2
title: D6_Ls180_RennoOutputs_7sols.nc.gz: MarsWRF output for southern spring equinox in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern spring equinox (Ls~180°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 8 and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10250300.v1
title: MarsWRF output for southern spring equinox in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern spring equinox (Ls~180°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 8 and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br>
DOI: 10.6084/m9.figshare.10249001.v2
title: D3_Ls270_RennoOutputs_7sols.nc.gz: MarsWRF output for southern summer solstice in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern summer solstice (Ls~270°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 2-5, 7-8, and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>
DOI: 10.6084/m9.figshare.10249796.v2
title: D4_Ls000_RennoOutputs_7sols.nc.gz: MarsWRF output for southern fall equinox in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern fall equinox (Ls~0°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment.<br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br>These data are used to produce Figures (especially Figures 8 and Supplementary Figures S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon
DOI: 10.6084/m9.figshare.10250297.v2
title: D5_Ls090_RennoOutputs_7sols.nc.gz: MarsWRF output for southern winter solstice in Gale Crater, needed to calculate Renno et al. [1998] Dust Devil Activity and intermediate variables.

description: This netCDF file of 7 sols of output from the MarsWRF atmospheric model includes all variables needed to calculate Renno et al. [1998]'s "Dust devil activity" in Gale Crater, Mars, for southern winter solstice (Ls~90°). The dust devil activity predicts the amount of convective and dust devil activity based on the thermodynamic environment. <br><br>Variables included are: lon (longitude in deg E), lat (latitude in deg N), ddac (dust devil activity), hfx(sensible heat flux in W/m2), ls (areocentric solar longitude), ltst (local true solar time in hours), omb (vertical thermodynamic efficiency), pbh (planetary boundary layer height in m), psrf (surface pressure in Pa), ptop (pressure at boundary layer top in Pa), rho (near-surface air density in kg/m3), t1_5 (air temperature at 1.5m above the surface in K), tsk (surface air temperature in K), ust (drag velocity, u*, in m/s).<br><br>These data are used to produce Figures (especially Figures 8 and S2-4) in the paper “Convective vortex and dust devil predictions for Gale Crater over three Mars years and comparison with MSL-REMS observations” - JGR-Planets, 2019 - by C. E. Newman, H. Kahanpää, M. I. Richardson, G. M. Martinez, A. Vicente-Retortillo and M. Lemmon<br><br><br>