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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2006
    In:  Journal of Geophysical Research Vol. 111, No. E9 ( 2006)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 111, No. E9 ( 2006)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2006
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2009
    In:  Journal of Geophysical Research Vol. 114, No. E11 ( 2009-11-07)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 114, No. E11 ( 2009-11-07)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2009
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Planets Vol. 102, No. E4 ( 1997-04-25), p. 9221-9229
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 102, No. E4 ( 1997-04-25), p. 9221-9229
    Abstract: Preliminary measurements of the effects of bulk density and particle size sorting on the thermal conductivity of particulate materials under Martian atmospheric pressures are presented and discussed. Concoidally fractured particles tend to form more loosely packed, less dense sedimentary structures, due to irregularities in the shape of the particles, than those formed by spherical particles of similar size. The lower bulk density of the angular‐shaped particles leads to a lower thermal conductivity of the sample. If the density difference is assumed to be the sole factor that controls the difference in conductivity in this case, then the thermal conductivity of 25–30 μm size particles appears to increase linearly with increasing bulk density and with the square root of the atmospheric pressure. Initial experiments appear to indicate that the bulk thermal conductivity of a particulate material containing a mixture of different particle sizes is the same as the thermal conductivity that a material of similar bulk density would have if it were composed entirely of the largest particle size contained within that material. More studies are, however, necessary to confirm this apparent trend.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Planets Vol. 102, No. E3 ( 1997-03-25), p. 6535-6549
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 102, No. E3 ( 1997-03-25), p. 6535-6549
    Abstract: Discussion of the thermal conductivity of particulate materials is dispersed over several decades and a wide range of disciplines. In addition, there is some disparity among the reported values. This paper presents a review of the methodology available for the study of thermal conductivity of particulate materials, with an emphasis on low atmospheric pressures, and an assessment of the dependability of the data previously reported. Both steady state and nonsteady state methods of thermal conductivity measurement are reviewed, delineating the advantages, disadvantages, and sources of error for each. Nonsteady state methods generally are simpler and more efficient. The transient hot wire and differentiated line‐heat source are the preferred methods for the laboratory. These methods are better suited for small samples and short measurement times and are therefore the best methods to use for a series of comprehensive studies. Results of previous studies are presented, compared, and evaluated. A good way to assess the relative accuracy is to compare the values of thermal conductivity versus atmospheric pressure obtained from several experimenters. The lowest values of thermal conductivity at vacuum and very low atmospheric pressure, and the steepest slopes on the thermal conductivity versus atmospheric pressure curves, are indicative of the most accurate data. Previous thermal conductivity studies have shown that the thermal conductivity of particulate materials increases with increasing atmospheric pressure, with increasing particle size, and with increasing bulk density of the material. At vacuum, the thermal conductivity of particulate materials is proportional to the cube of the temperature. The temperature dependence of thermal conductivity is much less obvious at higher atmospheric pressures.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2010
    In:  Journal of Geophysical Research Vol. 115, No. E7 ( 2010-07-07)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 115, No. E7 ( 2010-07-07)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2010
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  • 6
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 106, No. E10 ( 2001-10-25), p. 23921-23927
    Abstract: The “White Rock” feature on Mars has long been viewed as a type example for a Martian playa largely because of its apparent high albedo along with its location in a topographic basin (a crater). Data from the Mars Global Surveyor Thermal Emission Spectrometer (TES) demonstrate that White Rock is not anomalously bright relative to other Martian bright regions, reducing the significance of its albedo and weakening the analogy to terrestrial playas. Its thermal inertia value indicates that it is not mantled by a layer of loose dust, nor is it bedrock. The thermal infrared spectrum of White Rock shows no obvious features of carbonates or sulfates and is, in fact, spectrally flat. Images from the Mars Orbiter Camera show that the White Rock massifs are consolidated enough to retain slopes and allow the passage of saltating grains over their surfaces. Material appears to be shed from the massifs and is concentrated at the crests of nearby bedforms. One explanation for these observations is that White Rock is an eroded accumulation of compacted or weakly cemented aeolian sediment.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2001
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2010
    In:  Journal of Geophysical Research Vol. 115, No. E7 ( 2010-07-07)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 115, No. E7 ( 2010-07-07)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2010
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  • 8
    Online Resource
    Online Resource
    Wiley ; 2014
    In:  Journal of Dental Education Vol. 78, No. 8 ( 2014-08), p. 1205-1213
    In: Journal of Dental Education, Wiley, Vol. 78, No. 8 ( 2014-08), p. 1205-1213
    Abstract: As dental education across the United States undergoes growth and change in an effort to improve access to dental care, one dental school, the Arizona School of Dentistry & Oral Health, established in 2003, designed its initial curriculum with innovation in mind. One of those innovations was the introduction of an online certificate in public health that can be used as the foundation for a Master's in Public Health (M.P.H.) degree with a dental emphasis, which students may complete concurrent with their dental education. This article discusses the educational intersection between dentistry and public health and describes how this dental school uses an online public health curriculum to accomplish this integration. It also presents the potential advantages and disadvantages of obtaining the M.P.H. degree concurrent with the dental school training.
    Type of Medium: Online Resource
    ISSN: 0022-0337 , 1930-7837
    URL: Issue
    Language: English
    Publisher: Wiley
    Publication Date: 2014
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  • 9
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Planets Vol. 102, No. E3 ( 1997-03-25), p. 6551-6566
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 102, No. E3 ( 1997-03-25), p. 6551-6566
    Abstract: A line‐heat source apparatus was assembled for the purpose of measuring thermal conductivities of particulate samples under low pressures of a carbon dioxide atmosphere. The primary result of this project is the compilation of the first comprehensive suite of measurements of the dependence of thermal conductivity on particle size. The thermal conductivity increases with increasing particle size and atmospheric pressure. In particular, over the range of Martian atmospheric pressures, from 1 to 7 torr, the thermal conductivity was found to be empirically related to approximately the square root of the particle diameter and the square of the cubed root of the atmospheric pressure. At the average pressure of the Martian surface (6 torr) the thermal conductivity varies from 0.011 W/m K, for particles less than 11 μm in diameter, to 0.11 W/m K, for particles 900 μm in diameter. These results differ significantly from the particle size dependence estimated for Mars from previous measurements, except for 200‐μm particles, whose thermal conductivity is 0.053 W/m K. The thermal conductivities of larger particles are lower than the previous estimate, by 40% at 900 μm, and the thermal conductivities of smaller particles are higher than the previous estimate, by 60% at 11 μm. These newer estimates agree with other lines of evidence from Martian atmospheric and surficial processes and lead to improved particle size estimates for most of the planet's surface.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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