The DOI matches its Crossref record; 43 of the 43 references it cites were found in a registry or an index.
The annual cycle of water vapor on Mars as observed by the Thermal Emission Spectrometer
Abstract
Spectra taken by the Mars Global Surveyor Thermal Emission Spectrometer (TES) have been used to monitor the latitude, longitude, and seasonal dependence of water vapor for over one full Martian year (March 1999 to March 2001). A maximum in water vapor abundance is observed at high latitudes during midsummer in both hemispheres, reaching a maximum value of ∼100 pr‐μm in the north and ∼50 pr‐μm in the south. Low water vapor abundance (<5 pr‐μm) is observed at middle and high latitudes in the fall and winter of both hemispheres. There are large differences in the hemispheric (north versus south) and seasonal (perihelion versus aphelion) behavior of water vapor. The latitudinal and seasonal dependence of the decay of the northern summer water vapor maximum implies cross‐equatorial transport of water to the southern hemisphere, while there is little or no corresponding transport during the decay of the southern hemisphere summer maximum. The latitude‐longitude dependence of annually averaged water vapor (corrected for topography) has a significant positive correlation with albedo and significant negative correlations with thermal inertia and surface pressure. Comparison of TES results with those retrieved from the Viking Orbiter Mars Atmospheric Water Detectors (MAWD) experiments [Jakosky and Farmer, 1982] shows some similar features but also many significant differences. The southern hemisphere maximum observed by TES was not observed by MAWD, and the large latitudinal gradient in annually averaged water vapor observed by MAWD does not appear in the TES results.
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Self-citationThe Global Topography of Mars and Implications for Surface Evolution
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A Global View of Martian Surface Compositions from MGS-TES
Bandfield, J. L., Hamilton, V. E., & Christensen, P. R. (2000) · Science · doi:10.1126/science.287.5458.1626 · Cited by 675
High-Resolution Thermal Inertia Mapping from the Mars Global Surveyor Thermal Emission Spectrometer
Mellon, M. (2000) · Icarus · doi:10.1006/icar.2000.6503 · Cited by 530
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Self-citationJakosky, B. M., & Farmer, C. B. (1982) · Journal of Geophysical Research: Solid Earth · doi:10.1029/jb087ib04p02999 · Cited by 369
Near-Infrared Light from Venus' Nightside: A Spectroscopic Analysis
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Water Vapor Saturation at Low Altitudes around Mars Aphelion: A Key to Mars Climate?
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Investigation of the Martian environment by infrared spectroscopy on Mariner 9
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Cited by
Detection of methane in the martian atmosphere: evidence for life?
Krasnopolsky, V. A., Maillard, J. P., & Owen, T. C. (2004) · Icarus · doi:10.1016/j.icarus.2004.07.004 · Cited by 544
Strong water isotopic anomalies in the martian atmosphere: Probing current and ancient reservoirs
Villanueva, G. L., Mumma, M. J., Novak, R. E., Käufl, H. U., Hartogh, P., Encrenaz, T., Tokunaga, A., Khayat, A., & Smith, M. D. (2015) · Science · doi:10.1126/science.aaa3630 · Cited by 331
Self-citationAmazonian northern mid-latitude glaciation on Mars: A proposed climate scenario
Madeleine, J.-B., Forget, F., Head, J. W., Levrard, B., Montmessin, F., & Millour, E. (2009) · Icarus · doi:10.1016/j.icarus.2009.04.037 · Cited by 304
Mars Water-Ice Clouds and Precipitation
Whiteway, J. A., Komguem, L., Dickinson, C., Cook, C., Illnicki, M., Seabrook, J., Popovici, V., Duck, T. J., Davy, R., Taylor, P. A., et al. (2009) · Science · doi:10.1126/science.1172344 · Cited by 215
Metadata
- Authors
- Smith, M. D.
- Venue
- Journal of Geophysical Research: Planets
- Publisher
- American Geophysical Union (AGU)
- Published
- 2002-11
- Volume
- 107
- Issue
- E11
- ISSN
- 0148-0227 (ISSN-L)
- OpenAlex
- W2060731099
- Cited by
- 351
- References
- 43
- FWCI
- 11.21
- Type
- journal article
- Language
- en
- Open access
- closed
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