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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2000
    In:  Journal of Geophysical Research: Solid Earth Vol. 105, No. B10 ( 2000-10-10), p. 23681-23694
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 105, No. B10 ( 2000-10-10), p. 23681-23694
    Abstract: Infrared radiance data acquired by the Landsat thematic mapper (TM) provide information regarding the thermal state of active lavas, which can be used to estimate flow surface temperatures and thus lava cooling. Saturation of one or both of TM's short‐wave infrared (SWIR) wavebands has meant, however, that previous studies of lava flow cooling have approximated what is almost certainly an n thermal component flow surface temperature distribution (where n 〉 1), with a single pixel‐integrated temperature (PIT). We show that the high sensitivity of TM's SWIR wavebands to the small amount of high‐temperature (e.g., ∼1000°C) material exposed in hot fractures within the flows cooler (e.g., ∼200°C) surface crust results in the calculation of PITs that are higher than the temperature of this crust, which is usually the dominant radiative component. This causes heat loss from such pixels to be overestimated. We present adaptations that allow more realistic heat loss estimates to be produced using TM data by assuming that a second high‐temperature component contributes to the radiance measured from saturated pixels and by defining an appropriate range for the temperature of the lava crust. By analyzing a suite of five TM images acquired during the 1991–1993 eruption of Mount Etna we present more realistic estimates of how this flow cooled, as well as results that show how the flow regime of the lava evolved over time. The methods we present will continue to be of use as, although the next generation of high spatial resolution sensors such as the Landsat 7 enhanced thematic mapper plus (ETM+) and the Terra advanced space‐borne thermal emission and reflection radiometer (ASTER) will be less susceptible to saturation than TM, the problem will still persist.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2000
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    detail.hit.zdb_id: 3094268-8
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    SSG: 16,13
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1999
    In:  Geophysical Research Letters Vol. 26, No. 12 ( 1999-06-15), p. 1773-1776
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 26, No. 12 ( 1999-06-15), p. 1773-1776
    Type of Medium: Online Resource
    ISSN: 0094-8276
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1999
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    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 3
    Online Resource
    Online Resource
    Elsevier BV ; 2001
    In:  Earth and Planetary Science Letters Vol. 192, No. 2 ( 2001-10), p. 223-233
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 192, No. 2 ( 2001-10), p. 223-233
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2001
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    detail.hit.zdb_id: 1466659-5
    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1997
    In:  Journal of Geophysical Research: Solid Earth Vol. 102, No. B4 ( 1997-04-10), p. 7985-8003
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 102, No. B4 ( 1997-04-10), p. 7985-8003
    Abstract: Between December 1991 and March 1993 a continuous effusive eruption at Mount Etna built a 7.6 km 2 lava flow field. Flows extended to within 1 km of the town of Zafferana before a successful artificial diversion was carried out higher up the volcano. During this eruption the spaceborne advanced very high resolution radiometer (AVHRR) acquired 308 images on which the activity could be detected. Since these data can be freely and directly available, such coverage potentially allows regular, real‐time monitoring. Ground observations and a flow map that we produced using a SPOT image and electronic distance measurement allowed us to develop and test data extraction techniques. AVHRR radiance maps were consistent with known locations of surface activity. These documented the transition from channel to tube fed phases, the changing threat to Zafferana, and flow diversion. Quantitative analysis of the AVHRR data enabled estimation of active lava area, thermal flux, effusion rates, and total flow field volume. Our estimates for eruption rate and total flow field volume, 5.6 to 7.6 m 3 /s and 220×10 6 to 300×10 6 m 3 , respectively, are in agreement with published ground‐based estimates of 5.8 m 3 /s and 235×10 6 m 3 . These correlations demonstrate the high degree of confidence that can now be placed in interpretations of AVHRR time series for eruptions where ground‐based data are scanty.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1997
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    SSG: 16,13
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2008
    In:  Journal of Geophysical Research Vol. 113, No. B10 ( 2008-10-02)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 113, No. B10 ( 2008-10-02)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2008
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    SSG: 16,13
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  • 6
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 2000
    In:  Bulletin of Volcanology Vol. 62, No. 4-5 ( 2000-11-23), p. 256-265
    In: Bulletin of Volcanology, Springer Science and Business Media LLC, Vol. 62, No. 4-5 ( 2000-11-23), p. 256-265
    Type of Medium: Online Resource
    ISSN: 0258-8900 , 1432-0819
    Language: Unknown
    Publisher: Springer Science and Business Media LLC
    Publication Date: 2000
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