1977
DOI: 10.1175/1520-0469(1977)034<0163:tpfsal>2.0.co;2
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The Post-Fuego Stratospheric Aerosol: Lidar Measurements, with Radiative and Thermal Implications

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Cited by 54 publications
(19 citation statements)
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“…Sulfate concentrations measured from May 24 to June 9, 1976 (date of sample collection below each histogram). It is also in good agreement with the 11.6 months reported byMcCormick et al [1978] and 11 months reported byRussell and Hake [1977]. Sulfate should be present in the northern subpolar region of the stratosphere from eruptions of Augustine, Pavlof, and possibly Plosky Tolbachik volcanoes which were reported to have penetrated the stratosphere during the preceding few months.…”
supporting
confidence: 89%
“…Sulfate concentrations measured from May 24 to June 9, 1976 (date of sample collection below each histogram). It is also in good agreement with the 11.6 months reported byMcCormick et al [1978] and 11 months reported byRussell and Hake [1977]. Sulfate should be present in the northern subpolar region of the stratosphere from eruptions of Augustine, Pavlof, and possibly Plosky Tolbachik volcanoes which were reported to have penetrated the stratosphere during the preceding few months.…”
supporting
confidence: 89%
“…Similar differences between the estimated decay times have been observed earlier, both after the Fuego eruption as well as in the case of El Chichon eruption. In the case of Fuego, the 1/e-folding times for the vertically integrated backscattering coefficient (IBC) and the peak scattering ratio have been 8 and 11 months, respectively [Russell and Hake, 1977]. In the case of El Chichon, the 1/e-folding time for IBC is reported as 11.5 months [Jiiger and Carnuth, 1987].…”
Section: Resultsmentioning
confidence: 99%
“…Lidars provide remote, vertically resolved measurements of atmospheric backscatter from both molecules and aerosols at one or more wavelengths. To obtain aerosol backscatter profiles from a lidar requires accounting for three factors which affect the backscattered light received by the lidar telescope: (1) two way light extinction, (2) molecular backscatter, and (3) instrument normalization [e.g., Russell and Hake , 1977]. Molecular backscatter and extinction is typically calculated from pressure/temperature profiles provided by a nearby radiosonde station.…”
Section: Instrumentsmentioning
confidence: 99%