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Modeling studies related to carbon dioxide phase change on Mars

Citation

Guo, Xin (Vincent) (2009) Modeling studies related to carbon dioxide phase change on Mars. Dissertation (Ph.D.), California Institute of Technology. http://resolver.caltech.edu/CaltechETD:etd-05082009-120748

Abstract

Carbon dioxide (CO2) is the most abundant gaseous species in the atmosphere of Mars. Phase change of CO2, predominantly between gas and solid, is the most eminent feature in the current Martian atmosphere. Correct and thorough understanding of the CO2 cycle on Mars is crucial to the scientific research of Mars, including (but not limited to) climatology, meteorology, paleo-climatology, geomorphology, geology, and astrobiology. This dissertation focuses on modeling the CO2 phase change and coupling the process with a Mars General Circulation Model (GCM) ― the Mars Weather Forecast and Research (MarsWRF) model to study the climate of Mars. Two major forms of the CO2 phase change are included: direct deposition/sublimation to/from the surface (exchange with surface frost) and atmospheric condensation/evaporation (exchange with “snow”, which later will either precipitate to the ground and become a part of the surface reservoir, or evaporate before it reaches the surface). The first component has been historically simulated by a surface energy balance model. The energy balance calculations in MarsWRF, especially the physics module associated with subsurface heat conduction, are improved. The GCM is fine-tuned by changing the values of the seasonal ice cap albedos and emissivities and the total CO2 mass in the system (later the heat conductivity of the polar soil). Resulted surface pressure cycle, which is a good indicator of the atmospheric reservoir of CO2, matches the in situ measurements made by the Viking Landers extremely well. This fitting algorithm can be used for tuning of GCMs and for exploration of more complicated physical processes. The second component can be solved by a simple energy balance model in the atmosphere as well. However, it is widely accepted that sophisticated microphysics models may be required for more accurate simulations. A complete microphysics model, which calculates the nucleation process and ice particle growth process, is incorporated to MarsWRF. Preliminary simulation results show promising agreement with spacecraft observations. When an insolation-dependent frost albedo is included, MarsWRF is able to produce a perennial CO2 cap near the south pole of Mars. This is the first time that any GCM has successfully predicted a residual cap. This mechanism is necessary for a simple energy balance model to reproduce the perennial ice cap, and may shed some light on the ages and the cycles of the perennial caps. A mass balance model is developed to simulate the non-condensable gas mass mixing ratio variation during the CO2 phase change. When coupled with MarsWRF, the non-condensable gas cycle agrees qualitatively with the Gamma Ray Spectrometer data and other GCM results. It provides a benchmark check to the GCM itself and an independent way to study the dynamics of the Martian atmosphere.

Item Type:Thesis (Dissertation (Ph.D.))
Subject Keywords:carbon dioxide; climate; GCM; general circulation model; Mars; microphysics; phase change
Degree Grantor:California Institute of Technology
Division:Geological and Planetary Sciences
Major Option:Planetary Science
Minor Option:Electrical Engineering
Thesis Availability:Restricted to Caltech community only
Research Advisor(s):
  • Richardson, Mark I.
Thesis Committee:
  • Ingersoll, Andrew P. (chair)
  • Richardson, Mark I.
  • Aharonson, Oded
  • Yung, Yuk L.
Defense Date:29 April 2009
Author Email:xin (AT) gps.caltech.edu
Record Number:CaltechETD:etd-05082009-120748
Persistent URL:http://resolver.caltech.edu/CaltechETD:etd-05082009-120748
Default Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:1683
Collection:CaltechTHESIS
Deposited By: Imported from ETD-db
Deposited On:14 May 2009
Last Modified:08 Jul 2013 23:47

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