<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">ARS</journal-id><journal-title-group><journal-title>Advances in Remote Sensing</journal-title></journal-title-group><issn pub-type="epub">2169-267X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ars.2014.34017</article-id><article-id pub-id-type="publisher-id">ARS-52073</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Computer Science&amp;Communications</subject><subject> Engineering</subject></subj-group></article-categories><title-group><article-title>
 
 
  A Neural Network Algorithm to Detect Sulphur Dioxide Using IASI Measurements
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>lessandro</surname><given-names>Piscini</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Elisa</surname><given-names>Carboni</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fabio</surname><given-names>Del Frate</given-names></name><xref ref-type="aff" rid="aff3"><sup>3</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Roy</surname><given-names>Gordon Grainger</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff3"><addr-line>Earth Observation Laboratory, Civil Engineering and Computer Science Engineering Department, Tor Vergata University, Rome, Italy</addr-line></aff><aff id="aff2"><addr-line>COMET, Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK</addr-line></aff><aff id="aff1"><addr-line>Istituto Nazionale di Geofisica e Vulcanologia, Roma, Italy</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>alessandro.piscini@ingv.it(LP)</email>;<email>elisa@atm.ox.ac.uk(EC)</email>;<email>delfrate@disp.uniroma2.it(FDF)</email>;<email>r.grainger@physics.ox.ac.uk(RGG)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>28</day><month>11</month><year>2014</year></pub-date><volume>03</volume><issue>04</issue><fpage>246</fpage><lpage>259</lpage><history><date date-type="received"><day>19</day>	<month>September</month>	<year>2014</year></date><date date-type="rev-recd"><day>15</day>	<month>October</month>	<year>2014</year>	</date><date date-type="accepted"><day>10</day>	<month>November</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The remote sensing of volcanic sulphur dioxide (SO
  <sub>2</sub>
  ) is important because it is used as a proxy for volcanic ash, which is dangerous to aviation and is generally more difficult to discriminate. This paper presents an Artificial Neural Network (ANN) algorithm that recognizes volcanic SO
  <sub>2</sub>
   
  in the atmosphere using hyperspectral remotely sensed data from the IASI instrument aboard the Metop-A satellite. The importance of this approach lies in exploiting all thermal infrared spectral information of IASI and its application to near real-time volcanic monitoring in a fast manner. In this paper, the ANN algorithm is demonstrated on data of the Eyjafjallajokull volcanic eruption (Iceland) during the months of April and May 2010, and on the Gr&#237;msvotn eruption occurring during May 2011. The algorithm consists of a two output neural network classifier trained with a time series consisting of some hyperspectral eruption datasets collected during 14 April to 14 May 2010 and a few from 22 to 26 May 2011. The inputs were all channels (441) in the IASI
   
  v
  <sub>3</sub>
   
  band and the target outputs (truth) were the corresponding retrievals of SO
  <sub>2</sub>
   
  amount obtained with an optimal estimation method. The validation results for the Eyjafjallajokull independent data-sets had an overall accuracy of 100% and no commission errors, therefore demonstrating the feasibility of estimating the presence of SO
  <sub>2</sub>
   
  using a neural network approach also a in cloudy sky conditions. Although the validation of the neural network classifier on datasets from the Gr&#237;msvotn eruption had no commission errors, the overall accuracies were lower due to the presence of omission errors. Statistical analysis revealed that those false negatives lie near the detection threshold for discriminating pixels affected by SO
  <sub>2</sub>
  . This demonstrated that the accuracy in classification is strictly related to the sensitivity of the model. The lower accuracy obtained in detecting SO
  <sub>2</sub>
   
  for Gr&#237;msvotn validation dates might also be caused by less statistical knowledge of such an eruption during the training phase.
 
</p></abstract><kwd-group><kwd>Artificial Neural Networks</kwd><kwd> Pattern Recognition</kwd><kwd> Remote Sensing of Volcanoes</kwd><kwd> Volcano Monitoring</kwd><kwd> Hyperspectral</kwd><kwd> Volcanic Sulphur Dioxide</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Multi-layer perceptrons are used in many fields of science and technology. From the perspective of pattern recognition, they can be regarded as an extension of the many conventional statistical techniques which have been developed over several decades [<xref ref-type="bibr" rid="scirp.52073-ref1">1</xref>] . More extensive treatments of these topics can be found in the many textbooks on statistical pattern recognition, including [<xref ref-type="bibr" rid="scirp.52073-ref2">2</xref>] - [<xref ref-type="bibr" rid="scirp.52073-ref5">5</xref>] . Articles [<xref ref-type="bibr" rid="scirp.52073-ref6">6</xref>] and [<xref ref-type="bibr" rid="scirp.52073-ref7">7</xref>] have also emphasized the sta- tistical underpinnings of neural networks.</p><p>The main application of ANN to remote sense data analysis is scene classification, more commonly land cover classification, namely the process in which pixels are grouped according to the similarities of their spectral properties. If a pixel satisfies a certain set of criteria then it is assigned to the land cover class that corresponds to those criteria. This is the most common task achieved with remote sensing, and applications that involve both supervised and unsupervised ANNs are numerous. Due to the absence of any assumption about the data, many land cover classifications use data from different sensors such as optical and radar data [<xref ref-type="bibr" rid="scirp.52073-ref8">8</xref>] [<xref ref-type="bibr" rid="scirp.52073-ref9">9</xref>] , texture and ancillary data. Texture is incorporated in different ways: 1) precomputed per pixel texture information that is fed to the ANN together with the spectral information [<xref ref-type="bibr" rid="scirp.52073-ref10">10</xref>] or 2) incorporating neighbouring spectral information using a sliding window [<xref ref-type="bibr" rid="scirp.52073-ref11">11</xref>] .</p><p>It was reported that ANNs have more accurate performance than other techniques such as statistical classifiers, especially when the functional space is particularly complex and the source of data presents different statistical distributions [<xref ref-type="bibr" rid="scirp.52073-ref12">12</xref>] - [<xref ref-type="bibr" rid="scirp.52073-ref15">15</xref>] .</p><p>An additional advantage of the ANN approach is that they can perform supervised classification using fewer training data than those with maximum probability, because rules of recognition of a given category are based on the attributes, not only of training data of that particular category class, but also of other classes [<xref ref-type="bibr" rid="scirp.52073-ref16">16</xref>] .</p><p>The IASI instrument is used for operational measurements of meteorological parameters for numerical weather prediction. However, the high density of spectral information available and good signal-to-noise characteristics mean that the instrument can also provide measurements of many chemical species. The high density of spectral information and low instrument noise means that IASI could potentially provide very sensitive detection of SO<sub>2</sub>, especially for plumes in the upper-troposphere and lower-stratosphere, where the thermal contrast with the layers below is maximized. Usually full retrievals are time-consuming when searching for a sporadic event such as a volcanic eruption within a large data set. Detection methods do not require on-line radiative transfer cal- culations and can therefore be used to provide atmospheric measurements quickly, for example to help with volcanic hazard avoidance.</p><p>A commonly used method for the fast detection of trace atmospheric species is to calculate the difference in brightness temperature (BTD) between a small number of channels which are sensitive to the target species and others which are insensitive. The BTD between channels is then compared against a threshold which indicates a positive detection.</p><p>Simple BTD filters for the detection of SO<sub>2</sub> are applied operationally to provide an early warning of volcanic activity and to help track volcanic plumes in near-real-time [<xref ref-type="bibr" rid="scirp.52073-ref17">17</xref>] - [<xref ref-type="bibr" rid="scirp.52073-ref19">19</xref>] . Although fast and robust, current BTD methods do not fully exploit the spectral range and resolution of hyperspectral instruments, and the noise associated with the measurements remains high. SO<sub>2</sub> can be tracked from IASI using the difference in signal between two channels located at 1371.50 and 1371.75 cm<sup>−</sup><sup>1</sup> in the SO<sub>2</sub> v<sub>3</sub> vibrational band and two background channels at 1407.25 and 1408.75 cm<sup>−</sup><sup>1</sup> outside the SO<sub>2</sub> band [<xref ref-type="bibr" rid="scirp.52073-ref20">20</xref>] . Recently the detection method of Walker [<xref ref-type="bibr" rid="scirp.52073-ref21">21</xref>] , uses channels between 1300 and 1410 cm<sup>−</sup><sup>1</sup> (441 channels). It is a fast method which uses many spectral channels to separate the contribution of SO<sub>2</sub> from the contribution of other parameters affecting the measure- ment.</p><p>To date, no significant studies involving volcanic SO<sub>2</sub> detection using ANNs have been carried out. The main aim of this study is to verify if such a technique may be useful and give substantial improvements for real time monitoring of SO<sub>2</sub>, representing a reliable ANN monitoring tool during preliminary detection phase.</p><p>The challenge was to assess a classification problem by using ANN in order to detect the presence in the atmosphere of volcanic SO<sub>2</sub> using IASI hyperspectral data as input and the corresponding SO<sub>2</sub> retrievals by [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] as target outputs.</p><p>Beside its fast usage in the real time application, the advantage of ANN approach is in the ability to model the non-linearity in the variable space and in exploiting all the spectral information contained in hyperspectral data, and it does not need to select any target and background channels for implementing detection filters.</p><p>In this study, we first provide in Section 2.1. an overview of the IASI sensor characteristics and description of SO<sub>2</sub> total column estimation (Section 2.2.), then we discuss the neural network approach for SO<sub>2</sub> detection (Section 2.3.). In Section 3, the scenario where the ANN approach has been applied is introduced and the results obtained are discussed. Finally the conclusions are reported in section 4.</p></sec><sec id="s2"><title>2. Neural Network-based Classifier Algorithm</title><p>The neural network must first be “trained” by having it process a large number of input patterns and their as- sociated reference output patterns. Once trained, the neural network is able to recognize similarities when presented with a new input pattern, resulting in a predicted output pattern [<xref ref-type="bibr" rid="scirp.52073-ref23">23</xref>] .</p><sec id="s2_1"><title>2.1. Metop-IASI instrument</title><p>The IASI sensor is onboard Metop-A, a European weather satellite in operation since 2007. IASI is a Fourier transform spectrometer that covers the spectral range 645 - 2760 cm<sup>−</sup><sup>1</sup> (3.62 to 15.5 μm) with spectral sampling of 0.25 cm<sup>−</sup><sup>1</sup> and spectral resolution of 0.5 cm<sup>−</sup><sup>1</sup> [<xref ref-type="bibr" rid="scirp.52073-ref24">24</xref>] . It has a nominal radiometric accuracy of 0.25 - 0.58 K. The field-of-view (FOV) consists of four circular footprints of 12 diameter (at nadir) inside a square of 50 &#215; 50 km, step-scanned across tracks (30 steps). It has a 2000 km wide swath and nominally can achieve global coverage in 12 h.</p></sec><sec id="s2_2"><title>2.2. SO<sub>2</sub> total column content description</title><p>Values used here as target outputs were obtained with the Optimal Estimation scheme to retrieve SO<sub>2</sub> column amount and altitude from nadir satellite TIR measurements using the two SO<sub>2</sub> absorption bands centred at about 8.7 and 7.3 μm, the v<sub>1</sub> and v<sub>3</sub> bands respectively; more details of the retrieval are in [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] . This retrieval technique uses an error covariance matrix based on an SO<sub>2</sub>-free climatology of differences between the IASI measure- ments and forward modelled spectra. Any differences not related to SO<sub>2</sub> between IASI spectra and those simulated by a forward model are included in the covariance matrix, allowing a comprehensive error budget to be computed for every pixel.</p><p>As IASI measures atmospheric emission, it provides continuous measurements throughout an orbit. The IASI retrieval follows the method of [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] where SO<sub>2</sub> concentration is modelled by a Gaussian profile. The optimal estimation technique of [<xref ref-type="bibr" rid="scirp.52073-ref25">25</xref>] is then used to estimate SO<sub>2</sub> column amount and the height of the SO<sub>2</sub> profile, and the surface skin temperature using IASI measurements from 1000 to 1200 cm<sup>−</sup><sup>1</sup> and from 1300 to 1410 cm<sup>−</sup><sup>1</sup> (the v<sub>1</sub> and v<sub>3</sub> SO<sub>2</sub> bands).</p></sec><sec id="s2_3"><title>2.3. Neural Network Methodology</title><p>In this work, Backpropagation Neural Networks (BPNN) have been used. These networks are the most widely used type for their flexibility and adaptability to model a wide spectrum of problems in many application areas [<xref ref-type="bibr" rid="scirp.52073-ref26">26</xref>] .</p><p>A neural network for SO<sub>2</sub> detection was implemented using a training set of 59 IASI datasets, spanning the April-May 2010 Eyjafjallaj&#246;kull and May 2011 Gr&#237;msv&#246;tn eruptions (Iceland). The training sets used IASI retrievals from [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] as representative of SO<sub>2</sub> class.</p><p>The total number of training samples was 74,614, of which 43,437 were classified as SO<sub>2</sub> affected of which 84% belong to the Eyjafjallaj&#246;kull eruption.</p><p>The network topology consists of 441 inputs, namely the brightness temperatures in the 1300 - 1410 cm<sup>−</sup><sup>1</sup> channels, the so-called v<sub>3</sub> band, comprising the range of wavelengths containing information used for SO<sub>2</sub> amount estimation. Ten neurons were used in a single hidden layer, in order to cope with non linearly discrete problems [<xref ref-type="bibr" rid="scirp.52073-ref23">23</xref>] . Finally, outputs consisted of the two possible classification results, namely “SO<sub>2</sub>” and “not SO<sub>2</sub>”.</p><p>When training a neural network, it is of interest to obtain a network with an optimal generalization per- formance, i.e. the network performance should not degrade significantly when datasets other than the training one are analyzed.</p><p>Standard neural network architectures, like the fully connected multi layer perceptron, generally have too large a parameter space, and are prone to over-fitting [<xref ref-type="bibr" rid="scirp.52073-ref27">27</xref>] . During the training phase, although the network performance appears to constantly improve on the training sets, at some point it actually begins to worsen in terms of errors on unseen datasets. During supervised training of the neural network, cross validation can be used to detect when overfitting starts: training can then stopped before convergence to avoid overfitting, a process called early stopping [<xref ref-type="bibr" rid="scirp.52073-ref28">28</xref>] .</p><p>In this study, early stopping was carried out by splitting the training data into three sets: a training set, a cross validation set and a test set. These consisted respectively of 70%, 20% and 10% of the total number of training samples. The first set was used for network training. The cross validation set, consisting of 20%, was analyzed at a predefined number of epochs, to assess performance on datasets other than the training one. Finally, the test set (10%) was used as an independent data source to assess network performance after the training phase. The result obtained by processing 10% of the samples belonging to the test set, but not used for training, showed an overall accuracy of 100% without omission (false negatives) or commission (false positive) errors. The samples were 4092 pixels with SO<sub>2</sub> and 1309 without, respectively.</p></sec></sec><sec id="s3"><title>3. Application to two operational scenarios</title><p>After completion of the training process, the ANN classifier algorithm has been proposed for a remote sensing application such as the monitoring of two volcanic eruptions that occurred in Iceland in 2010 and 2011. The 14 April to 24 May 2010 Eyjafjallaj&#246;kull eruption caused widespread impacts [<xref ref-type="bibr" rid="scirp.52073-ref29">29</xref>] .</p><p>It was an explosive eruption with an injection of volcanic ash into the atmosphere and plumes that affected many regions of Europe. Plumes reached altitudes of 9 km, and the ash was transported across Europe and to the Atlantic Ocean. Despite its impact, the explosive phase was modest in size and the amount of SO<sub>2</sub> released was low.</p><p>The Gr&#237;msv&#246;tn eruption occurred from May 21 to May 23 2011. It injected into the atmosphere a higher concentration of SO<sub>2</sub> than Eyjafjallaj&#246;kull. The height reached by the plume was 20 km [<xref ref-type="bibr" rid="scirp.52073-ref30">30</xref>] .</p><p>In order to evaluate the performance of neural network classifier in terms of its generalization capability and accuracy in detecting SO<sub>2</sub> presence in the atmosphere from IASI datasets, we applied the trained ANN classifier to two independent IASI datasets from the May 2010 Eyjafjallaj&#246;kull eruption and to two independent IASI datasets from the Gr&#237;msv&#246;tn eruption which occurred the following year. Note that ANN has been validated on datasets which include all IASI orbits, not only on SO<sub>2</sub> plume data, with a significant number of pixels not affected by SO<sub>2</sub> (more than 40%). Performance was assessed in terms of overall accuracy and Producer accuracy. The former represents the percentage of correct classifications, with respect to the total number of pixels analysed, considering all classes (i.e. SO<sub>2</sub> and not SO<sub>2</sub>). The Producer accuracy instead represents the percentage of correct classifications with respect to the total obtained for that output class and it is an omission error indicator.</p><p>Tables 1-4 describe the confusion matrices obtained by applying the NN classifier to these independent datasets. Figures 1-4 show comparisons between classification maps obtained from the ANN classifier and from the SO<sub>2</sub> retrieved by Carboni [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] for all validation dates.</p><p>In <xref ref-type="table" rid="table1">Table 1</xref>, <xref ref-type="table" rid="table2">Table 2</xref>, which summarize the results related to the Eyjafjallaj&#246;kull eruptions of April 30 2010 and May 15 2010, the neural network classifier achieves an accuracy of 100%. This is a very good result, considering the ANN classifier has been applied to the entire IASI orbits. In fact, looking at <xref ref-type="fig" rid="fig1">Figure 1</xref>, despite most of the pixels not being affected by SO<sub>2</sub>, the ANN classifier perfectly detects SO<sub>2</sub> plume. The same result is obtained when ANN is applied to May 2010 (<xref ref-type="fig" rid="fig2">Figure 2</xref>). <xref ref-type="table" rid="table2">Table 2</xref> describes the confusion matrix and shows an overall accuracy of 100% for detecting the plume, despite the fact that it extends from 45˚ to 75˚N. Again, neither commission nor omission errors are present.</p><p>The results of applying the ANN classifier to the IASI datasets during the Gr&#237;msv&#246;tn eruption are described by confusion matrices depicted in <xref ref-type="table" rid="table3">Table 3</xref> and <xref ref-type="table" rid="table4">Table 4</xref> and depicted in <xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="fig" rid="fig4">Figure 4</xref>, for May, 22 2011, at 12:00 and 20:00 UTC, respectively.</p><p>In the case of the morning orbit depicted in <xref ref-type="table" rid="table3">Table 3</xref>, the overall accuracy obtained is 99.1%. The producer accuracy, which measures the probability that the classifier correctly labels a pixel as SO<sub>2</sub>, is 70.3%. The lower accuracy obtained is due to the presence of an omission error, because 29.7% of pixels with SO<sub>2</sub> have been</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Eyjafjallaj&#246;kull. Confusion matrix assessing the classification accuracy on the IASI validation date of April 30, 2010, afternoon orbit</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >30 April 2010</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >SO<sub>2</sub></th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Prod. Acc.</th></tr></thead><tr><td align="center" valign="middle" >Overall Acc.: 100%</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >(%)</td></tr><tr><td align="center" valign="middle" >NN</td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >161</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >100.0</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >19,139</td><td align="center" valign="middle" >100.0</td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Eyjafjallaj&#246;kull. Confusion matrix assessing the classification accuracy on the IASI validation date of May 15, 2010, morning orbit</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >15 May 2010</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >SO<sub>2</sub></th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Prod. Acc.</th></tr></thead><tr><td align="center" valign="middle" >Overall Acc.: 100%</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >(%)</td></tr><tr><td align="center" valign="middle" >NN</td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >1823</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >100.0</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >37,180</td><td align="center" valign="middle" >100.0</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Gr&#237;msv&#246;tn. Confusion matrix assessing the classification accuracy on the IASI validation date of May 22, 2011, 12:00 UTC</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >22 May 2011, 12:00 UTC</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >SO<sub>2</sub></th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Prod. Acc.</th></tr></thead><tr><td align="center" valign="middle" >Overall Acc.: 99.1%</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >(%)</td></tr><tr><td align="center" valign="middle" >NN</td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >298</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >70.3</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >126</td><td align="center" valign="middle" >13,865</td><td align="center" valign="middle" >100.0</td></tr></tbody></table></table-wrap><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> Gr&#237;msv&#246;tn. Confusion matrix assessing the classification accuracy on the IASI validation date of May 22, 2011, 20:00 UTC</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >22 May 2011, 20:00 UTC</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >SO<sub>2</sub></th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Prod. Acc.</th></tr></thead><tr><td align="center" valign="middle" >Overall Acc.: 98.5%</td><td align="center" valign="middle" ></td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >(%)</td></tr><tr><td align="center" valign="middle" >NN</td><td align="center" valign="middle" >Yes</td><td align="center" valign="middle" >236</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >57.0</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" >No</td><td align="center" valign="middle" >178</td><td align="center" valign="middle" >11,653</td><td align="center" valign="middle" >100.0</td></tr></tbody></table></table-wrap><p>labelled as not affected by SO<sub>2</sub>.</p><p>Looking at the histograms in <xref ref-type="fig" rid="fig5">Figure 5</xref> (top), representing the statistical distribution of false negatives for the 22 May 2011 date, we notice that most of the false negatives have values lower than 3 DU, which is around the SO<sub>2</sub> detection threshold for a plume height between 2 and 4 km [<xref ref-type="bibr" rid="scirp.52073-ref21">21</xref>] . Looking at the maps depicted in <xref ref-type="fig" rid="fig6">Figure 6</xref> we notice that they belong to a portion of the plume located close to the vent and are characterized by a height of between 2 - 4 km [<xref ref-type="bibr" rid="scirp.52073-ref30">30</xref>] . Considering that the SO<sub>2</sub> detection threshold at these altitudes is 3.3 DU, we can assert that the ANN classifier shows a sensitivity in accord with the model for low SO<sub>2</sub> amounts in the lower troposphere. Furthermore it puts in evidence the absorption band limit at 7.3 μm when observing SO<sub>2</sub> in low troposhere.</p><p>For total SO<sub>2</sub> column amounts of less than 0.2 DU concentrated in the boundary layer between 0 - 2 km the signal falls below the noise level of the instrument [<xref ref-type="bibr" rid="scirp.52073-ref21">21</xref>] . Instead, when SO<sub>2</sub> is higher into the atmosphere due to an explosive volcanic event it is possible to discern very low concentrations. As shown in <xref ref-type="fig" rid="fig7">Figure 7</xref>, showing only positive detections for both Gr&#237;msv&#246;tn validation’s datasets, ANN classifier well detect low amount of SO<sub>2</sub> when they are located at higher altitudes (low stratosphere) [<xref ref-type="bibr" rid="scirp.52073-ref30">30</xref>] .</p><p>The same assertion can be made for the afternoon orbit of the May, 22, 2011, 20:00 UTC: looking at <xref ref-type="table" rid="table4">Table 4</xref>, an overall accuracy of 98.5% is shown. Producer accuracy is 57% and, once again, this is due to false negatives related to pixels of plume at lower altitudes, as in the previous validation. In fact, looking at the histogram representing SO<sub>2</sub> distribution (<xref ref-type="fig" rid="fig5">Figure 5</xref>, bottom) most of the values are around the detection threshold used for SO<sub>2</sub> discrimination, but not higher than 3 DU, which characterizes the detection threshold for the part of the plume in the lower troposphere. Instead, when SO<sub>2</sub> is higher into the atmosphere due to an explosive volcanic event it may be possible to discern very low concentrations.</p><p>The retrieval methodology of [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] establishes that for measurements in the thermal infrared spectral range the sensitivity is better for plume injected at high altitudes where the air is colder and the thermal contrast is higher,</p><fig-group id="fig1"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Comparison between SO<sub>2</sub> retrieved by Carboni [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] (top) and SO<sub>2</sub> map from ANN classifier (bottom) for Eyjafjallaj&#246;kull April 30, 2010 afternoon orbit. Pixels affected by SO<sub>2</sub> are coloured red, pixels not affected by SO<sub>2</sub> are coloured green.</title></caption><fig id ="fig1_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x5.png"/></fig><fig id ="fig1_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x6.png"/></fig></fig-group><fig-group id="fig2"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Comparison between SO<sub>2</sub> retrieved by Carboni [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] (top) and SO<sub>2</sub> map from ANN classifier (bottom) for Eyjafjallaj&#246;kull May 15, 2010 morning orbit. Pixels affected by SO<sub>2</sub> are coloured red, pixels not affected by SO<sub>2</sub> are coloured green.</title></caption><fig id ="fig2_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x7.png"/></fig><fig id ="fig2_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x8.png"/></fig></fig-group><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Comparison between SO<sub>2</sub> retrieved by Carboni [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] (top) and SO<sub>2</sub> map from ANN classifier (bottom) for Gr&#237;msv&#246;tn May 22, 2011, 12:00 UTC. Pixels affected by SO<sub>2</sub> are coloured red, pixels not affected by SO<sub>2</sub> are coloured green.</title></caption><fig id ="fig3_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x9.png"/></fig><fig id ="fig3_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x10.png"/></fig></fig-group><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Comparison between SO<sub>2</sub> retrieved by Carboni [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] (top) and SO<sub>2</sub> map from ANN classifier (bottom) for Gr&#237;msv&#246;tn May 22, 2011, 12:00 UTC. Pixels affected by SO<sub>2</sub> are coloured red, pixels not affected by SO<sub>2</sub> are coloured green.</title></caption><fig id ="fig4_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x11.png"/></fig><fig id ="fig4_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x12.png"/></fig></fig-group><fig-group id="fig5"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> SO<sub>2</sub> amount distribution in DU, considering only false negatives, for Gr&#237;msv&#246;tn May 22, 2011, 12:00 UTC (top) and May 22, 2011, 20:00 UTC (bottom). Both histograms reveal that most values have an amount around the SO<sub>2</sub> detection threshold.</title></caption><fig id ="fig5_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x13.png"/></fig><fig id ="fig5_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x14.png"/></fig></fig-group><fig-group id="fig6"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Gr&#237;msv&#246;tn May 22, 2011, 12:00 UTC. SO<sub>2</sub> Cloud height in mb (top) and SO<sub>2</sub> amount in DU (bottom).</title></caption><fig id ="fig6_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x15.png"/></fig><fig id ="fig6_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x16.png"/></fig></fig-group><fig-group id="fig7"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> SO<sub>2</sub> amount distribution in DU considering only positive detections, for Gr&#237;msv&#246;tn May 22, 2011, 12:00 UTC (top) and May 22, 2011, 20:00 UTC (botttom).</title></caption><fig id ="fig7_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x17.png"/></fig><fig id ="fig7_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/3-2630102x18.png"/></fig></fig-group><p>while at lower altitudes (e.g. the troposphere) the lower thermal contrast reduces the sensitivity of the detection method, so we can assert that the ANN classifier is in accord with the sensitivity of the model.</p><p>What can be underlined is that no commission errors are present at the validation stage (pixels erroneously labelled as affected by SO<sub>2</sub>) for both 2010 and 2011 eruptions, and the method shows the same accuracy when applied to IASI images with different illumination conditions (morning and afternoon orbits) and in cloudy sky conditions. Furthermore, it is noticeable that most of the training samples are from the Eyjafjallaj&#246;kull eruption and only a low percentage from the Gr&#237;msv&#246;tn one (26%), which represents an event statistically not well known at the training stage. This can explain why the ANN classifier reveals a loss of accuracy when applied to Gr&#237;msv&#246;tn eruption.</p></sec><sec id="s4"><title>4. Conclusions</title><p>This work proves the detection capability of volcanic SO<sub>2</sub> by means of an algorithm neural network based classifier, applied to the thermal channels of the IASI hyperspectral sensor. SO<sub>2</sub> amounts estimated by [<xref ref-type="bibr" rid="scirp.52073-ref22">22</xref>] were used as training target outputs.</p><p>The resulting confusion matrices associated with application to independent datasets spanning two Eyjafjalla- j&#246;kull volcanic eruptions revealed an accuracy of 100% on both tested images.</p><p>The results of applying the ANN classifier to the Gr&#237;msv&#246;tn eruption reveals an accuracy lower in detecting SO<sub>2</sub> plume, but these cases included: a) The data-sets belonging to the Gr&#237;msv&#246;tn eruption represented a minor percentage of IASI time-series used as training samples; b) the presence of false negatives, i.e. pixels affected by SO<sub>2</sub> not detected. In this case an analysis carried out on false negatives for both validation dates revealed that those pixel belonged to the portion of the plume at tropospheric altitudes where the sensitivity of the method is lower.</p><p>Nevertheless, the neural network classifier has been shown to work well both on daytime and night-time images and in cloudy sky conditions, and it successfully overcame the detection of false positives present in the validation dataset images, whose presence in multispectral or hyperspectral images can often undermine the performance of traditional classification algorithms. 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