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  4. Volcanic SO2 and SiF4 visualization using 2-D thermal emission spectroscopy ; Part 1: Slant-columns and their ratios
 
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Volcanic SO2 and SiF4 visualization using 2-D thermal emission spectroscopy ; Part 1: Slant-columns and their ratios

Citation Link: https://doi.org/10.15480/882.1933
Publikationstyp
Journal Article
Date Issued
2012-02-02
Sprache
English
Author(s)
Stremme, Wolfgang  
Krueger, Arne  
Harig, Roland  
Grutter, Michel  
Institut
Messtechnik (E-6H)  
TORE-DOI
10.15480/882.1933
TORE-URI
http://tubdok.tub.tuhh.de/handle/11420/1936
Journal
Atmospheric measurement techniques  
Volume
5
Issue
2
Start Page
275
End Page
288
Citation
Atmospheric Measurement Techniques 2 (5): 275-288 (2012)
Publisher DOI
10.5194/amt-5-275-2012
Scopus ID
2-s2.0-84873555350
Publisher
European Geosciences Union, Copernicus
The composition and emission rates of volcanic gas plumes provide insight of the geologic internal activity, atmospheric chemistry, aerosol formation and radiative processes around it. Observations are necessary for public security and the aviation industry. Ground-based thermal emission infrared spectroscopy, which uses the radiation of the volcanic gas itself, allows for continuously monitoring during day and night from a safe distance. We present measurements on Popocatépetl volcano based on thermal emission spectroscopy during different campaigns between 2006-2009 using a Scanning Infrared Gas Imaging System (SIGIS). The experimental set-up, measurement geometries and analytical algorithms are described. The equipment was operated from a safe distance of 12 km from the volcano at two different spectral resolutions: 0.5 and 4 cm−1. The 2-dimensional scanning capability of the instrument allows for an on-line visualization of the volcanic SO2 plume and its animation. SiF4 was also identified in the infrared spectra recorded at both resolutions. The SiF4/SO2 molecular ratio can be calculated from each image and used as a highly useful parameter to follow changes in volcanic activity. A small Vulcanian eruption was monitored during the night of 16 to 17 November 2008 and strong ash emission together with a pronounced SO2 cloud was registered around 01:00 a.m. LST (Local Standard Time). Enhanced SiF4/SO2 ratios were observed before and after the eruption. A validation of the results from thermal emission measurements with those from absorption spectra of the moon taken at the same time, as well as an error analysis, are presented. The inferred propagation speed from sequential images is used in a subsequent paper (Part 2) to calculate the emission rates at different distances from the crater.
Subjects
thermal emission spectroscopy
DDC Class
550: Geowissenschaften
Lizenz
https://creativecommons.org/licenses/by/3.0/
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