CO2 snowfall on Mars:: Simulation with a general circulation model

被引:127
作者
Forget, F [1 ]
Hourdin, F [1 ]
Talagrand, O [1 ]
机构
[1] Univ Paris 06, CNRS, Meteorol Dynam Lab, F-75252 Paris 05, France
关键词
Mars; atmosphere; dynamics; clouds; ices;
D O I
10.1006/icar.1997.5874
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Although CO2 snowfall has never been directly observed on Mars, it has been suggested that such precipitation may explain the puzzling infrared measurements obtained by Mariner 9 and Viking during the polar night in each hemisphere. The radiative effect of the snow would strongly alter the radiative balance of the condensing polar caps and thus the CO2 cycle and the global climate. We have simulated this phenomenon with a general circulation model (GCM). For that purpose, a new parameterization of CO2 condensation in the atmosphere and on the ground has been developed, paging particular attention to mass and energy conservation and allowing for the possible sublimation of sedimenting COL ice particles. Atmospheric condensation may result from radiative cooling on the one hand (especially when the atmosphere is dust laden) and from adiabatic cooling in upward motions on the other hand. This latter process can be very efficient locally. On this basis, we have modeled the effect of the CO2 snowfall on the infrared emission by decreasing the local emissivities when atmospheric condensation was predicted by the model. This parameterization is based on physical considerations (radiative transfer through the CO2 ice particles, snow metamorphism on the ground). Without tuning the model parameters, we have been able to accurately reproduce the general behavior of the features observed by Viking in the thermal infrared. These modeling results support the CO2 snowfall scenario suggested from the observations. Overall, this new parameterization, used in combination with the digital terrain model topography and with allowance for a varying atmospheric dust content, allows the GCM to simulate the CO2 condensation-sublimation cycle realistically. In particular, the seasonal variations of the surface pressure recorded by the Viking Landers can now be reproduced without artificially decreasing the condensation rate as was done in previous studies. (C) 1998 Academic Press.
引用
收藏
页码:302 / 316
页数:15
相关论文
共 52 条
[41]   VIKING LANDER IMAGE-ANALYSIS OF MARTIAN ATMOSPHERIC DUST [J].
POLLACK, JB ;
OCKERTBELL, ME ;
SHEPARD, MK .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1995, 100 (E3) :5235-5250
[42]   SIMULATIONS OF THE GENERAL-CIRCULATION OF THE MARTIAN ATMOSPHERE .1. POLAR PROCESSES [J].
POLLACK, JB ;
HABERLE, RM ;
SCHAEFFER, J ;
LEE, H .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B2) :1447-1473
[43]   SIMULATIONS OF THE GENERAL-CIRCULATION OF THE MARTIAN ATMOSPHERE .2. SEASONAL PRESSURE VARIATIONS [J].
POLLACK, JB ;
HABERLE, RM ;
MURPHY, JR ;
SCHAEFFER, J ;
LEE, H .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1993, 98 (E2) :3149-3181
[44]   CLOUD MICROPHYSICS - ANALYSIS OF CLOUDS OF EARTH, VENUS, MARS, AND JUPITER [J].
ROSSOW, WB .
ICARUS, 1978, 36 (01) :1-50
[45]  
STANSBERRY JA, 1995, 27 ANN M DIV PLAN SC
[46]   PHYSICAL-PROPERTIES OF PARTICLES COMPOSING MARTIAN DUST STORM OF 1971-1972 [J].
TOON, OB ;
POLLACK, JB ;
SAGAN, C .
ICARUS, 1977, 30 (04) :663-696
[47]   RAPID CALCULATION OF RADIATIVE HEATING RATES AND PHOTODISSOCIATION RATES IN INHOMOGENEOUS MULTIPLE-SCATTERING ATMOSPHERES [J].
TOON, OB ;
MCKAY, CP ;
ACKERMAN, TP ;
SANTHANAM, K .
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1989, 94 (D13) :16287-16301
[48]  
VAN LEER B, 1977, J COMPUT PHYS, V23, P276, DOI 10.1016/0021-9991(77)90094-8
[49]  
WASHBURN E, 1948, INT CRITICAL TABLES, V3
[50]   A general circulation model simulation of the Martian polar warming [J].
Wilson, RJ .
GEOPHYSICAL RESEARCH LETTERS, 1997, 24 (02) :123-126