Abstract
The existence, formation and content of water ice in the lunar permanently shaded region is one of the important questions for the current Moon study. On October 9, 2009, the LCROSS mission spacecraft impacted the Moon, and the initial result verified the existence of water on the Moon. But the study on formation and content of water ice is still under debate. The existence of water ice can change the dielectric constants of the lunar regolith, and a microwave radiometer is most sensitive to the dielectric parameters. Based on this, in this paper, the radiation transfer model is improved according to the simulation results in high frequency. Then the mixture dielectric constant models, including Odelevsky model, Wagner and landau-Lifshitz model, Clau-sius model, Gruggeman-Hanai model, etc., are analyzed and compared. The analyzing results indicate that the biggest difference occurs between Lichtenecker model and the improved Dobson model. The values estimated by refractive model are the second biggest in all the models. And the results from Odelevsky model, strong fluctuation model, Wagner and Landau -Lifshitz model, Clausius model and Bruggeman-Hanai model are very near to each other. Thereafter, the relation between volume water ice content and microwave brightness temperature is constructed with Odelevsky mixing dielectric model and the improved radiative transfer simulation, and the volume water ice content in Cabeus crater is retrieved with the data from microwave radiometer onboard Chang’e-1 satellite. The results present that the improved radiative transfer model is proper for the brightness temperature simulation of the one infinite regolith layer in high frequency. The brightness temperature in Cabeus crater is 69.93 K (37 GHz), and the corresponding volume water ice content is about 2.8%.
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References
Neal C R. The moon 35 years after Apollo: What’s left to learn. Chemie der Erde, 2009, 69: 3–43
Watson K, Murray B C, Brown H. The behavior of volatiles on the lunar surface. J Geophys Res, 1961, 66: 3033–3045
Arnold J R. Ice in the lunar polar regions. J Geophys Res, 1979, 84: 5659–5668
Nozette S, Lichtenberg C L, Spudis P, et al. The Clementine bistatic radar experiment. Science, 1996, 274: 1495–1498
Butler B J, Muhleman D O, Slade M A. Mercury: full-disk radar images and the detection and stability of ice at the north pole. J Geophys Res, 1993, 98: 15003–15023
Butler B J. The migration of volatiles on the surfaces of Mercury and the Moon. J Geophys Res, 1997, 102: 19283–19291
Vasavada A R, Paige D A, Wood S E. Near-surface temperatures on Mercury and the Moon and the stability of polar ice deposits. Icarus, 1999, 141: 179–193
Simpson R A, Tyler G L. Reanalysis of Clementine bistatic radar data from the lunar south Pole. J Geophys Res, 1999, 104: 3845–3862
Feldman W C, Maurice S, Binder A B, et al. Fluxes of fast and epithermal neutrons from lunar prospector: Evidence for water ice at the lunar Poles. Science, 1998, 281: 1496–1500
Feldman W C, Lawrence D J, Elphic R C, et al. Chemical information content of lunar thermal and epithermal neutrons. J Geophys Res, 2000, 105: 20347–20363
Nozette S, Spudis P D, Robinson M S, et al. Integration of lunar polar remote sensing data sets: evidence for ice at the lunar south pole. J Geophys Res, 2001, 106: 23253–23266
Hodges R. Ice in the lunar polar regions revisited. J Geophys Res, 2002, 107: 5011–5017
Campbell B A, Campbell D B, Carter L M, et al. No evidence for thick deposits of ice at the lunar south pole. Nature, 2006, 443: 835–837
Crider D H, Vondrak R R. Hydrogen migration to the lunar poles by solar wind bombardment of the Moon. Adv Space Res, 2002, 30: 1869–1874
http://newpaper.dahe.cn/hnrbncb/html/2009-10/10/content_233630.htm
http://www.nasa.gov/mission_pages/LRO/multimedia/lroimages/lroc_20091117_cabeus.html
Meng Zhiguo. Lunar regolith parameters retrieval using radiative transfer simulation and look-up table. Dissertation for the Doctoral Degree. Changchun: Jilin University, 2008
Jin Y Q. Microwave scattering, emission model and its application (in Chinese). Peking: Science Press, 1998
Li L Y, Zhang L X, Zhao S J. Laboratory measurement of the dielectric constant of frozen soil (in Chinese). J Beijing Normal Univ (Natural Science), 2007, 43: 241–244
Zhang W G, Jiang J S, Liu H G, et al. Distribution and anomaly of microwave emission at lunar south pole. Sci China Earth Sci, 2010, 53: 465–474
Dobson M C, Ulaby F T, Hallikainen M T, et al. Microwave dielectric behavior of wet soil: Part II: dielectric mixing models. IEEE Trans Geosci Remote Sens, 1985, 23: 35–46
Jiang J S, Wang Z Z, Li Y. Study on theory and application of CE-1 microwave sounding lunar surface (in Chinese). Eng Sci, 2008, 10: 16–22
Wang Z Z, Li Y, Jiang J S, et al. Lunar surface dielectric constant, regolith thickness and helium-3 abundance distributions retrieved from microwave brightness temperatures of CE-1 Lunar Microwave Sounder. Sci China Earth Sci, 2010, 53: 1365–1378
Jiang J S, Zhang X H, Zhang D H, et al. Microwave sounding of lunar soil from China lunar orbit satellite “Chang’E-1(CE-1)”. In: The 37th COSPAR Scientific Assembly, Montréal, 2008. 1379
Shkuratov Y G, Bondarenko N V. Regolith layer thickness mapping of the moon by radar and optical data. Icarus, 2001, 149: 329–338
Jin Y Q, Yan F H, Liang Z C. Simulation of brightness temperature from the lunar surface using multi-channels microwave radiometers (in Chinese). Chin J Radio Sci, 2003, 18: 477–486
Meng Z G, Chen S B, Li C, et al. Review on retrieval of lunar regolith thickness by active and passive microwave measurements. Global Geology, 2008, 11: 102–109
Ulaby F T, Moore R K, Fung A. Microwave remote sensing. Reading, MA: Addison -Wesley -Longman, 1981
Li X Y, Wang S J, Chang A Y. A review of lunar surface temperature model (in Chinese). Adv Earth Sci, 2007, 22: 480–485
Olhoeft G R, Strangway D W. Dielectric properties of the first 100 meters of the moon. Earth Planet Sci Lett, 1975, 24: 394–404
Helfenstein P, Shepard M K. Sub-millimeter scale topography of the lunar regolith. Icarus, 1999, 141: 107–131
Meng Z G, Chen S B, Liu C, et al. Simulation of passive microwave penetration features in dry medium. In: Proceeding of International Conference on Microwave and Millimeter Wave Technology. Nanjing, 2008. 1680–1682
Heiken et al. Lunar sourcebook: a user’s guide to the moon. Cambridge: Cambridge University Press, 1991
Reynolds J A, Hough J M. Formulae for dielectric constant of mixtures. Proc Phys Soc London, 1957, 70: 769–775
Shutko A M, Reutov E M. Mixture formulas applied in estimation of dielectric radiative characteristics of soils and grounds at microwave frequencies. IEEE Trans Geosci Remote Sens, 1982, 20: 29–32
Odelevsky V I. Raschet obobschennoi provodimosti geterogennih system. GTF, 1951, 21: 667–685
Wobschall D. A theory of the complex dielectric permittivity of soil containing water: The semidisperse model. IEEE Trans Geosci Electron, 1977, 15: 49–58
Fa W Z, Jin Y Q. Simulation of multi-channels brightness temperature of the lunar surface and inversion of lunar regolith layer thickness (in Chinese). Prog Nat Sci, 2006, 16: 86–94
Evans S. Dielectric properties of ice and snow-a review. J Glaciol, 1965, 5: 773–792
Wang Z Z, Li Y, Jiang J S, et al. Microwave transfer models and brightness temperature simulations of MWS for remote sensing lunar surface on CE-1 satellite. In: Proceeding of International Conference on Microwave and Millimeter Wave Technology. Nanjing, 2008. 1683–1686
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Meng, Z., Chen, S., Osei, E.M. et al. Research on water ice content in Cabeus crater using the data from the microwave radiometer onboard Chang’e-1 satellite. Sci. China Phys. Mech. Astron. 53, 2172–2178 (2010). https://doi.org/10.1007/s11433-010-4159-y
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DOI: https://doi.org/10.1007/s11433-010-4159-y