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Microwave Radiometric Remote Sensing of Volcanic Ash Clouds From Space: Model and Data Analysis

Authors :
Montopoli
M.a
Cimini
D.bc
Lamantea
M.d
Herzog
Graf
H.F.a
Marzano
F.S.cd
Source :
IEEE transactions on geoscience and remote sensing 51 (2013): 4678–4691. doi:10.1109/TGRS.2013.2260343, info:cnr-pdr/source/autori:Montopoli, M.a, Cimini, D.bc, Lamantea, M.d, Herzog, M.a, Graf, H.F.a, Marzano, F.S.cd/titolo:Microwave radiometric remote sensing of volcanic ash clouds from space: Model and data analysis/doi:10.1109%2FTGRS.2013.2260343/rivista:IEEE transactions on geoscience and remote sensing/anno:2013/pagina_da:4678/pagina_a:4691/intervallo_pagine:4678–4691/volume:51
Publication Year :
2013
Publisher :
Institute of Electrical and Electronics Engineers (IEEE), 2013.

Abstract

The potential of satellite passive microwave sensors to provide quantitative information about near-source volcanic ash cloud parameters is assessed. To this aim, ground-based microwave weather radar and spaceborne microwave radiometer observations are used together with forward-model simulations. The latter are based on 2-D simulations with the numerical plume model Active Tracer High-Resolution Atmospheric Model (ATHAM), in conjunction with the radiative transfer model Satellite Data Simulator Unit (SDSU) that is based on the deltaEddington approximation and includes Mie scattering. The study area is the Icelandic subglacial volcanic region. The analyzed case study is that of the Grímsvötn eruption in May 2011. ATHAM input parameters are adjusted using available ground data, and sensitivity tests are conducted to investigate the observed brightness temperatures and their variance. The tests are based on the variation of environmental conditions like the terrain emissivity, water vapor, and ice in the volcanic plume. Quantitative correlation analysis between ATHAM/SDSU forward-model columnar content simulations and available microwave radiometric brightness temperature measurements, derived from the Special Sensor Microwave Imager/Sounder (SSMIS), are encouraging in terms of both dynamic range and correlation coefficient. The correlation coefficients are found to vary from - 0.37 to -0.63 for SSMIS channels from 91 to 183 \pm 1 GHz, respectively. The larger sensitivity of the brightness temperature at 183 \pm 1 GHz to the columnar content, with respect to other channels, allowed us to consider this channel as the basis for a model-based polynomial relationship of volcanic plume height as a function of the measured SSMIS brightness temperature.

Details

ISSN :
15580644 and 01962892
Volume :
51
Database :
OpenAIRE
Journal :
IEEE Transactions on Geoscience and Remote Sensing
Accession number :
edsair.doi.dedup.....bd823bce141a436cf4c62aa830720927