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Long-wave stratospheric transmission of Mount St. Helens ejectaThe NASA/Ames Research C-141 aircraft underflew the Mount St. Helens ejecta plume in Utah three days after the eruption. Upward-looking 20-40-microns on-board radiometry provided data resulting in a calculated long-wave transmission of 0.93. From this value, an optical depth of 0.073 is inferred. This value is compared with an accepted background, stratospheric infrared optical depth of 0.06. Assumptions on particle size, shortwave albedo, and thermal warming imply little surface temperature change caused by the ejecta on the third day immediately following the eruption.
Document ID
19810037718
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kuhn, P. M.
(Raven Systems and Research, Inc. Boulder, Colo., United States)
Haughney, L. C.
(NASA Ames Research Center Moffett Field, CA, United States)
Innis, R. C.
(NASA Ames Research Center Moffett Field, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Optics Letters
Volume: 6
Subject Category
Geophysics
Accession Number
81A22122
Distribution Limits
Public
Copyright
Other

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