Model Datafiles for Observed seasonal changes in Martian hydrogen chloride consistent with heterogeneous chemistry on atmospheric dust and ice
Description
Datafiles produced by the 1-D photochemistry model used to create the publication "Observed seasonal changes in Martian hydrogen chloride consistent with heterogeneous chemistry on atmospheric dust and ice" - Taysum et al. 2024.
matching_orbits_v2.txt : Lists the orbital parameters and water vapour / aerosol file names corresponding to each of the 77 ACS MIR HCl observations that we study.
MCD_GlobaMaps.zip : .nc files containing model output where the model is ran at Longitude 0 degrees, across Ls 0 --> 360 in intervals of 30 degrees, and latitudes 60 S to 60 N in intervals of 15 degrees.
- LowTau : model runs with the chlorine heterogeneous chemistry scheme active.
- MY34/ : Runs driven with MY34 climatology from the MCDv6.1
- StandardClim/ : Runs driven with Standard Climatology from the MCDv6.
- No_Chlorine : model runs with no chlorine tracers in the model chemistry.
- MY34/ : Runs driven with MY34 climatology from the MCDv6.1
- StandardClim/ : Runs driven with Standard Climatology from the MCDv6.1
ACS_Comparisons.zip : .nc files containing the model output for specific ACS MIR HCl observations in Mars Year 34.
- LowTau : model runs with the chlorine heterogeneous chemistry scheme active.
- MY34/ : Runs driven with MY34 climatology from the MCDv6.1
- StandardClim/ : Runs driven with Standard Climatology from the MCDv6.1
- TGO/ : Runs driven with MY34 climatology, and TGO measured water ice, dust, and H2O vapor profiles, driven at the position of the ACS-TIRVIM aerosol retrievals corresponding to the approximately colocated ACS MIR HCl observation
- No_Chlorine : model runs with no chlorine tracers in the model chemistry.
- MY34/ : Runs driven with MY34 climatology from the MCDv6.1
- StandardClim/ : Runs driven with Standard Climatology from the MCDv6.1
- TGO/ : Runs driven with MY34 climatology, driven at the position of the ACS-TIRVIM aerosol retrievals corresponding to the approximately colocated ACS MIR HCl observation