<?xml version="1.0" ?>
<rss version="2.0">
	<channel>
		<title><![CDATA[ Geoscience and Remote Sensing, IEEE Transactions on - new TOC ]]></title>
		<link>http://ieeexplore.ieee.org</link>
		<description>TOC Alert for Publication# 36 </description>
		<year>2013</year>
		<month>May      </month>
		<day>16</day>
		<item>
			<title><![CDATA[Front cover]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517014]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517014]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>C1</startPage>
			<endPage>C1</endPage>
			<fileSize>583</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[IEEE Transactions on Geoscience and Remote Sensing publication information]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517002]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517002]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>C2</startPage>
			<endPage>C2</endPage>
			<fileSize>141</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[Table of Contents]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516994]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516994]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3205</startPage>
			<endPage>3206</endPage>
			<fileSize>126</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[Methodology and Information Content of the NOAA NESDIS Operational Channel Selection for the Cross-Track Infrared Sounder (CrIS)]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375806]]></link>
			<description><![CDATA[The Cross-track Infrared Sounder (CrIS) was launched on October 28, 2011 aboard the Suomi National Polar-orbiting Partnership platform and is scheduled to become operational in 2012. The purpose of this paper is to describe the National Oceanic and Atmospheric Administration/National Environmental Satellite and Information Service (NOAA/NESDIS) channel selection methodology applied to the CrIS instrument and to present the main spectral characteristics of the final channel subset that will be operationally distributed to the scientific community for near-real-time data assimilation and retrieval applications. We perform an information content analysis and show that this selection, composed of 399 channels, is capable of fully representing the total atmospheric variability contained in the original 1305-channel spectrum, up to instrumental noise. These results ensure that the replacement of the full 1305-channel list in favor of the proposed 399-channel selection will have no detrimental effects on data assimilation and retrieval performance.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375806]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3207</startPage>
			<endPage>3216</endPage>
			<fileSize>1308</fileSize>
			<authors><![CDATA[Gambacorta, A.;Barnet, C.D.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Quality Assessment of the First Measurements of Tropospheric Water Vapor and Temperature by the HAMSTRAD Radiometer Over Concordia Station, Antarctica]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6422380]]></link>
			<description><![CDATA[The HAMSTRAD microwave instrument operates at 60 and 183 GHz and measures temperature and water vapor, respectively, from 0- to 10-km altitude with a time resolution of 7 min. The radiometer has been successfully deployed at Dome C (Concordia Station), Antarctica (<formula formulatype="inline"><tex Notation="TeX">$75^{circ}06^{prime} hbox{S}$</tex></formula>, <formula formulatype="inline"><tex Notation="TeX">$123^{circ}21^{prime} hbox{E}$</tex></formula>, 3233 m amsl) during the first summertime campaign for 12 days in January&#x2013;February 2009. The radiometer has been continuously running since January 2010, hosted within a dedicated shelter. We have used the very first set of HAMSTRAD data, recorded when the instrument was outdoors, to assess its potential to sound the troposphere over Dome C, from the planetary boundary layer (PBL) up to the tropopause (<formula formulatype="inline"><tex Notation="TeX">$sim$</tex> </formula>6 km above surface, <formula formulatype="inline"><tex Notation="TeX">$sim$</tex></formula>9 km amsl). We have compared the HAMSTRAD measurements to several sets of measurements performed at the Dome-C station or in its vicinity: meteorological radiosondes, in situ PT100 and Humicap sondes along the vertical extent of a 45-m tower, meteorological sensor attached to the HAMSTRAD instrument, and the spaceborne Infrared Atmospheric Sounding Interferometer (IASI) instrument onboard the EUMETSAT MetOp-A satellite in polar orbit. The variability of integrated water vapor (IWV) observed by HAMSTRAD with extremely low values of 0.5 <formula formulatype="inline"><tex Notation="TeX">$hbox{kg} cdot hbox{m}^{-2}$</tex></formula> was also measured by the radiosondes (very high HAMSTRAD versus radiosonde correlation of 0.98), whereas IASI cloud-free measurements did not reproduce well the HAMSTRAD IWV variation (weak HAMSTRAD versus IASI correlation of 0.58). The measurements of absolute humidity <formula formulatype="inline"><tex Notation-
"TeX">$(hbox{H}_{2}hbox{O})$</tex></formula> from HAMSTRAD at Dome C cover a large vertical extent from the surface to about 6 km above surface with a high sensitivity in the free troposphere. The strong diurnal variation of <formula formulatype="inline"><tex Notation="TeX">$hbox{H}_{2}hbox{O}$</tex> </formula> observed by the in situ sensors in the PBL is not well detected by the radiometer. In the free troposphere, the HAMSTRAD versus radiosonde <formula formulatype="inline"> <tex Notation="TeX">$hbox{H}_{2}hbox{O}$</tex></formula> correlation can reach 0.8&#x2013;0.9. Around the tropopause, HAMSTRAD shows the same variability as IASI and radiosondes but with a dry bias of 0.01 <formula formulatype="inline"><tex Notation="TeX">$ hbox{g} cdot hbox{m}^{-3}$</tex></formula>. HAMSTRAD tends to show a wetter atmosphere by 0.1&#x2013;0.3 <formula formulatype="inline"><tex Notation="TeX">$hbox{g} cdot hbox{m}^{-3}$</tex></formula> compared with radiosondes from the surface to <formula formulatype="inline"><tex Notation="TeX">$sim$</tex></formula>2-km altitude and a drier atmosphere above by <formula formulatype="inline"><tex Notation="TeX">$sim!! hbox{0.1} hbox{g} cdot hbox{m}^{-3}$</tex></formula>. The sensitivity of the temperature profiles from HAMSTRAD is very high in the PBL and in the free troposphere but degrades around the tropopause. The strong diurnal signal measured above the surface by HAMSTRAD (3&#x2013;6 K) is consistent with all the other in situ data sets. The temporal evolution over the 12-day period in the PBL is also consistent with all other data sets (radiosondes, IASI, in situ sondes, and meteorological sensors). In the free troposphere and around the tropopause, the HAMSTRAD temporal evolution is consistent with that observed by radiosondes and IASI, although a cold bias exists compared with IASI and radiosondes around the tropopause. For heights less than 4 km above surface, HAMSTRAD correlates very well with radiosondes a]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6422380]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3217</startPage>
			<endPage>3239</endPage>
			<fileSize>2923</fileSize>
			<authors><![CDATA[Ricaud, P.;Carminati, F.;Attie, J.-L.;Courcoux, Y.;Rose, T.;Genthon, C.;Pellegrini, A.;Tremblin, P.;August, T.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Principle of Locality and Analysis of Radio Occultation Data]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6416041]]></link>
			<description><![CDATA[A fundamental principle of local interaction of radio waves with a refractive spherical medium is formulated and illustrated using the radio occultation (RO) method of remote sensing of the atmosphere and the ionosphere of the Earth and the planets. In accordance with this principle, the main contribution to variations of the amplitude and the phase of radio waves propagating through a medium makes a neighborhood of a tangential point, where the gradient of the refractive index is perpendicular to the radio wave trajectory. A necessary and sufficient condition (a criterion) is established to detect the displacement of the tangential point from the radio ray perigee using analysis of the RO experimental data. This criterion is applied to the identification and the location of layers in the atmosphere and the ionosphere by the use of Global Positioning System RO data. RO data from the CHAllenge Minisatellite Payload (CHAMP) are used to validate the criterion introduced when significant variations of the amplitude and the phase of the RO signals are observed at the RO ray perigee altitudes below 80 km. The detected criterion opens a new avenue in terms of measuring the altitude and the slope of the atmospheric and ionospheric layers. This is important for the location determination of the wind shear and the direction of internal wave propagation in the lower ionosphere and possibly in the atmosphere. The new criterion provides an improved estimation of the altitude and the location of the ionospheric plasma layers compared with the backpropagation radio-holographic method previously used.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6416041]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3240</startPage>
			<endPage>3249</endPage>
			<fileSize>592</fileSize>
			<authors><![CDATA[Pavelyev, A.G.;Zhang, K.;Liou, Y.-A.;Pavelyev, A.A.;Wang, C.-S.;Wickert, J.;Schmidt, T.;Kuleshov, Y.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Amplitudes Estimation of Large Internal Solitary Waves in the Mid-Atlantic Bight Using Synthetic Aperture Radar and Marine X-Band Radar Images]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6355981]]></link>
			<description><![CDATA[The accurate estimation of internal solitary waves' (ISWs') amplitudes from radar images is important for understanding the ISW evolution, energy dissipation, and mixing processes. The in situ data from the Non-Linear Internal Wave Initiative experiment in the Mid-Atlantic Bight show many ISWs with amplitudes of 10 m or more in a shallow water depth of 80 m or less. Therefore, the higher order Korteweg&#x2013;de Vries (KdV) equation in a two-layer system is needed to describe these large-amplitude ISWs instead of the classic KdV equation. Based on a simple theoretical radar imaging model, we develop a method to estimate large ISW amplitudes from distances between the positive and negative peaks of ISW signatures in radar images and a selection rule from the two possible amplitude solutions. Two groups of ISWs with large amplitudes, determined from the temperature records from nearby moorings, are observed in a RADARSAT synthetic-aperture-radar image and in marine X-band radar data collected during the experiment. We validate the method using the ISW signatures taken from these two cases. We find the estimated amplitudes to agree well with those determined from the moorings. The proposed method provides a relatively simple and accurate way to estimate large ISW amplitudes from radar images.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6355981]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3250</startPage>
			<endPage>3258</endPage>
			<fileSize>1401</fileSize>
			<authors><![CDATA[Xue, J.;Graber, H.C.;Lund, B.;Romeiser, R.;]]></authors>
		</item>
		<item>
			<title><![CDATA[A Descalloping Postprocessor for ScanSAR Images of Ocean Scenes]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377292]]></link>
			<description><![CDATA[Due to its specific way of recording signals from multiple adjacent swaths in an alternating manner, a scanning synthetic aperture radar (SAR) (ScanSAR) cannot sample Doppler histories continuously like a SAR in stripmap mode. This can cause an effect known as azimuth scalloping, a wavelike modulation of the image intensity in near-azimuth direction. In theory, azimuth scalloping can be straightened out by using appropriate beam pattern corrections and multilooking techniques in the SAR processor. This works well over land, but lower signal-to-noise ratios and less accurate Doppler centroid estimates over water cause significant residual scalloping in many ScanSAR images of ocean scenes. The scalloping patterns hamper a correct interpretation of signatures of wind streaks, waves, and other phenomena. To overcome this problem once and for all, we have developed an algorithm that can eliminate scalloping patterns from existing ScanSAR images by postprocessing. Our algorithm detects the dominant scalloping pattern in an image automatically and eliminates most of it with very small side effects. We treat the scalloping pattern as a multiplicative effect, i.e., the amplitude spectrum of an affected image is assumed to be the convolution of the amplitude spectra of the unscalloped image and of the scalloping pattern. The proposed descalloping technique works partly in the spatial and partly in the spectral domain to approximate an exact deconvolution. We give a detailed technical description, show example results, and perform a quality analysis. We demonstrate the positive effects of the proposed descalloping treatment with a wind field retrieval example.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377292]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3259</startPage>
			<endPage>3272</endPage>
			<fileSize>4637</fileSize>
			<authors><![CDATA[Romeiser, R.;Horstmann, J.;Caruso, M.J.;Graber, H.C.;]]></authors>
		</item>
		<item>
			<title><![CDATA[A Hybrid Cloud Detection Algorithm to Improve MODIS Sea Surface Temperature Data Quality and Coverage Over the Eastern Gulf of Mexico]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377283]]></link>
			<description><![CDATA[Cloud contamination can lead to significant biases in sea surface temperature (SST) as estimated from satellite measurements. The effectiveness of four cloud detection algorithms for the Moderate Resolution Imaging Spectroradiometer (MODIS) in retaining valid SST data and masking cloud-contaminated data was assessed for all 2125 daytime and nighttime images during 2010 over the eastern Gulf of Mexico and including the east coast of Florida. None of the cloud detection algorithms was found to be sufficient to reliably differentiate clouds from valid SST, particularly during anomalously cold events. The strengths and weaknesses of each algorithm were identified, and a new hybrid cloud detection algorithm was developed to maximize valid data retention while excluding cloud-contaminated pixels. The hybrid algorithm was based on a decision tree, which includes a set of rules to use existing algorithms in different ways according to time and location. Comparing with <formula formulatype="inline"> <tex Notation="TeX">$&#x003E;10,000$</tex></formula> concurrent in situ SST measurements from buoys, images processed with the hybrid algorithm showed increases in data capture and improved accuracy statistics over most existing algorithms. In particular, while keeping the same accuracy, the hybrid algorithm resulted in nearly 20% more SST retrievals than the most accurate algorithm (Quality SST) currently being used for operational processing. The increases in both data coverage and SST range should improve MODIS data products for more reliable SST retrievals in near real time, thus enhancing the ocean observing capacity to detect anomaly events and study short- and long-term SST changes in coastal environments.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377283]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3273</startPage>
			<endPage>3285</endPage>
			<fileSize>2157</fileSize>
			<authors><![CDATA[Barnes, B.B.;Hu, C.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Inversion of Chromophoric Dissolved Organic Matter From EO-1 Hyperion Imagery for Turbid Estuarine and Coastal Waters]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6361477]]></link>
			<description><![CDATA[The significant implication of chromophoric dissolved organic matter (CDOM) for water quality and biogeochemical cycle leads to an increasing need of CDOM monitoring in coastal regions. Current ocean-color algorithms are mostly limited to open-sea water and have high uncertainty when directly applied to turbid coastal waters. This paper presents a semianalytical algorithm, quasi-analytical CDOM algorithm (QAA-CDOM), to invert CDOM absorption from Earth Observing-1 (EO-1) Hyperion satellite images. This algorithm was developed from a widely used ocean-color algorithm QAA and our earlier extension of QAA. The main goal is to improve the algorithm performance for a wide range of water conditions, particularly turbid waters in estuarine and coastal regions. The algorithm development, calibration, and validation were based on our intensive high-resolution underwater measurements, International Ocean Color Coordinating Group synthetic data, and global National Aeronautics and Space Administration Bio-Optical Marine Algorithm Data Set data. The result shows that retrieved CDOM absorption achieved accuracy (<formula formulatype="inline"><tex Notation="TeX">$hbox{root mean square error (RMSE)} = 0.115 hbox{m}^{-1}$</tex> </formula> and <formula formulatype="inline"><tex Notation="TeX">$R^{2} = 0.73$</tex></formula>) in the Atchafalaya River plume area. QAA-CDOM is also evaluated for scenarios in three additional study sites, namely, the Mississippi River, Amazon River, and Moreton Bay, where <formula formulatype="inline"><tex Notation="TeX">$a_{g}(440)$</tex></formula> was in the wide range of 0.01&#x2013;15 <formula formulatype="inline"><tex Notation="TeX">$hbox{m}^{-1}$</tex></formula>. It resulted in expected CDOM distribution patterns along the river salinity gradient. This study improves the high-resolution observation of CDOM dynamics in river-dominated coastal margins and other coastal environments for the study of land&#x2013;ocean interactive processes.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6361477]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3286</startPage>
			<endPage>3298</endPage>
			<fileSize>1609</fileSize>
			<authors><![CDATA[Zhu, W.;Yu, Q.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Target Detection on the Ocean With the Relative Phase of Compact Polarimetry SAR]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6387592]]></link>
			<description><![CDATA[This paper discusses the potential for automatic ocean surveillance using compact linear polarization (CL-pol) synthetic aperture radar (SAR), with large area coverage. Here, the target is a wind farm in the North Sea. The relative phase, as derived from CL-pol SAR, is employed for detection of the wind turbines, apart from the wind turbines' wakes, based on fine-mode quad-polarization (quad-pol) RADARSAT-2 (RS-2) images. The relative phase of CL-pol measurements improves the contrast between the wind turbines and their wakes, because it has opposite signs for these two entities. Moreover, there is almost no variation in the relative phase with respect to wind speed or incidence angle. The results are verified by high-sea-state cases, up to 8.7-m significant wave height and 24.3-m/s wind speed, and also 641 quad-pol RS-2 SAR images collocated with 52 National Data Buoy Center buoys at different incidence angles and sea states. Thus, the relative phase of CL-pol SAR provides new light into the problem of operational autodetection of man-made targets, under high-sea-state conditions, over large areas.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6387592]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3299</startPage>
			<endPage>3305</endPage>
			<fileSize>883</fileSize>
			<authors><![CDATA[Li, H.;Perrie, W.;He, Y.;Lehner, S.;Brusch, S.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Improvement and Sensitivity Analysis of Thermal Thin-Ice Thickness Retrievals]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6357238]]></link>
			<description><![CDATA[Considering the sea ice decline in the Arctic during the last decades, polynyas are of high research interest since these features are core areas of new ice formation. The determination of ice formation requires accurate retrieval of polynya area and thin-ice thickness (TIT) distribution within the polynya. We use an established energy balance model to derive TITs with MODIS ice surface temperatures <formula formulatype="inline"><tex Notation="TeX">$(T_{s})$</tex> </formula> and NCEP/DOE Reanalysis II in the Laptev Sea for two winter seasons. Improvements of the algorithm mainly concern the implementation of an iterative approach to calculate the atmospheric flux components taking the atmospheric stratification into account. Furthermore, a sensitivity study is performed to analyze the errors of the ice thickness. The results are the following: 1) 2-m air temperatures <formula formulatype="inline"><tex Notation="TeX">$(T_{a})$ </tex></formula> and <formula formulatype="inline"><tex Notation="TeX">$T_{s}$</tex></formula> have the highest impact on the retrieved ice thickness; 2) an overestimation of <formula formulatype="inline"><tex Notation="TeX">$T_{a}$</tex></formula> yields smaller ice thickness errors as an underestimation of <formula formulatype="inline"><tex Notation="TeX">$T_{a}$</tex></formula>; 3) NCEP <formula formulatype="inline"><tex Notation="TeX">$T_{a}$</tex></formula> shows often a warm bias; and 4) the mean absolute error for ice thicknesses up to 20 cm is <formula formulatype="inline"><tex Notation="TeX">$pm$</tex></formula>4.7 cm. Based on these results, we conclude that, despite the shortcomings of the NCEP data (coarse spatial resolution and no polynyas), this data set is appropriate in combination with MODIS <formula formulatype="inline"><tex Notation="TeX">$T_{s}$</tex> </formula> for the retrieval of TITs up to 20 cm in the Laptev Sea region. The TIT algorithm can be applied to other polynya regions and to past and future time periods. Our -
IT product is a valuable data set for verification of other model and remote sensing ice thickness data.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6357238]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3306</startPage>
			<endPage>3318</endPage>
			<fileSize>1588</fileSize>
			<authors><![CDATA[Adams, S.;Willmes, S.;Schroder, D.;Heinemann, G.;Bauer, M.;Krumpen, T.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Glacier Velocity Estimation by Means of a Polarimetric Similarity Measure]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6410023]]></link>
			<description><![CDATA[The contribution of polarimetric synthetic aperture radar (PolSAR) images compared with that of single-channel SAR images in terms of temporal scene characterization has been found and described to add valuable information in the literature. However, despite a number of recent studies focusing on single-polarized glacier monitoring, the potential of polarimetry to estimate the surface velocity of glaciers has not been explored due to the complex mechanism of polarization through glacier/snow. In this paper, a new approach to the problem of monitoring glacier surface velocity is proposed by means of temporal PolSAR images, using a basic concept from information theory, i.e., mutual information (MI). The proposed polarimetric tracking method applies the MI to measure the statistical dependence between temporal polarimetric images, which is assumed to be maximum if the images are geometrically aligned. Since the proposed polarimetric tracking method is very powerful and general, it can be implemented into any kind of multivariate remote sensing data such as multichannel optical and single-channel SAR images. The proposed polarimetric tracking is then used to retrieve the surface velocity of the Aletsch Glacier in Switzerland and the Inylchek Glacier in Kyrgyzstan with two different SAR sensors: the Experimental SAR airborne L-band (fully polarimetric) and Envisat C-band (single-polarized) systems, respectively. The effect of the number of channels (polarimetry) into tracking investigations demonstrated that the presence of snow, as expected, affects the location of the phase center in different polarization and frequency channels, as for the glacier tracking with temporal HH compared to temporal VV channels. In this paper, it is shown how it is possible to optimize these two different contributions, considering the multichannel SAR statistics.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6410023]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3319</startPage>
			<endPage>3327</endPage>
			<fileSize>1028</fileSize>
			<authors><![CDATA[Erten, E.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Automatic Grain Type Classification of Snow Micro Penetrometer Signals With Random Forests]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377289]]></link>
			<description><![CDATA[Snow microstructure plays an important role in the remote sensing of snow water equivalent (SWE) for both passive and active microwave radars. The accuracy of microwave SWE retrieval algorithms is sensitive to (usually unknown) changes in microstructure. These algorithms could be improved with high-resolution estimates of microstructural properties by using an advanced instrument such as the Snow Micro Penetrometer (SMP), which measures penetration force at the millimeter scale and is sensitive to microstructure. The SMP can also take full micromechanical measurements at much greater speed and resolution and without observer bias than a traditional snow pit. Previous studies have shown that the snowpack stratigraphy and grain type can be accurately classified with one SMP measurement using basic statistics and classification trees (CTs). For this study, we used basic statistical measures of the penetration force and micromechanical estimates from an SMP inversion algorithm to significantly improve the classification accuracy of grain type and layer discrimination. We applied random forest (RF) techniques to classify three snow grain types (new snow, rounds, and facets) from SMP measurements collected in Switzerland and Grand Mesa, Colorado. RFs performed up to 8% better than single CTs, with overall misclassification errors between 17% and 40%. The coefficient of variation of the penetration force proved to be the most important variable, followed by variables that contain information about grain size like microscale strength and the number of ruptures.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377289]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3328</startPage>
			<endPage>3335</endPage>
			<fileSize>1184</fileSize>
			<authors><![CDATA[Havens, S.;Marshall, H.-P.;Pielmeier, C.;Elder, K.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Sea Ice Classification During Freeze-Up Conditions With Multifrequency Scatterometer Data]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377285]]></link>
			<description><![CDATA[Helicopter-borne radar backscatter measurements are analyzed with respect to a multifrequency classification approach of sea ice. Measurements were carried out over the Arctic Ocean during August and September 2007 and represented unusually warm freeze-up conditions. Radar cross sections (RCSs) of totally ice-free wind-roughened water are used in combination with an ocean surface theoretical backscattering model for the calibration. The calibrated RCS <formula formulatype="inline"><tex Notation="TeX">$sigma^{circ}$</tex></formula> agrees within 1 dB with nearly simultaneous Envisat Advanced Synthetic Aperture Radar measurements and literature values. Sea ice was classified using a Bayesian maximum likelihood approach. By including information from simultaneous infrared and visible video imagery of sea ice, four different surface types of sea ice could be identified in the resulting <formula formulatype="inline"><tex Notation="TeX">$sigma^{circ}$</tex></formula>: old ice, gray ice, nilas, and open water. The most reliable classification was obtained through combination of copolarized C-, X-, and Ku-band data. The results degraded by only 7% in the case where the X-band information was dropped. On the other hand, a combination of the C- and X-bands or the X- and Ku-bands yielded a degradation of 13%. Given the remaining uncertainties in the approach, for sea ice classification during summer/fall conditions, our results suggest the complementary use of two of these three frequency bands instead of relying on just one frequency band.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377285]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3336</startPage>
			<endPage>3353</endPage>
			<fileSize>2769</fileSize>
			<authors><![CDATA[Brath, M.;Kern, S.;Stammer, D.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Interannual Variability of Young Ice in the Arctic Estimated Between 2002 and 2009]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6416043]]></link>
			<description><![CDATA[The recently observed reduction in perennial ice in the Arctic has given rise to a corresponding increase in seasonal ice, which includes young ice (YI). This type of ice has a major impact on the weather and climate systems. However, only a limited number of studies have been dedicated to explore its spatial coverage and duration. This is mainly due to the lack of remote sensing tools that can identify it. This study uses an ice type and concentration retrieval algorithm, namely, Environment Canada's Ice Concentration Extractor, to study YI distribution and duration in the Arctic during seven ice formation seasons: 2002&#x2013;03 to 2008&#x2013;09. Results on the YI area, peak period, duration, and its interannual variability are presented in six regions covering the Arctic Basin. Duration is presented in terms of two parameters that describe the peak period and the number of days when YI concentration exceeds 50%. Probability distribution of the latter parameter shows that YI survives very few days before it grows into first-year ice. The summer of the minimum ice record in 2007 did not leave a remarkable impact on the subsequent YI area or its duration, although a delay in ice formation is observed. YI in the North Water polynya is also studied and shows no particular trend, although it varies between years. Anomalies are explained in terms of modeled surface temperature and wind.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6416043]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3354</startPage>
			<endPage>3370</endPage>
			<fileSize>3669</fileSize>
			<authors><![CDATA[Shokr, M.;Dabboor, M.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Forest Biomass Estimation Using Texture Measurements of High-Resolution Dual-Polarization C-Band SAR Data]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6353204]]></link>
			<description><![CDATA[Recent synthetic aperture radar (SAR) sensors with a capability of providing data with varying spatial resolutions, polarizations, and incidence angles have attracted greater interest for forest biomass and carbon storage estimation. This study investigates the capability of RADARSAT-2 fine-beam dual-polarization (C-HV and C-HH) data for forest biomass estimation in complex subtropical forest, with different types of processing: 1) raw intensity data (both polarizations separately and as polarization ratio) and 2) texture parameters of both polarizations (separately, jointly, and as polarization ratio). Field data (diameter at breast height and height) were collected from 53 field plots and converted to biomass (dry weight) using a newly developed allometric model. Finally, biomass estimation models were developed between SAR signatures from different processing steps and field plot biomass using stepwise multiple regression. All biomass estimation models using radar intensity data (C-HV, C-HH, and ratio of C-HV and C-HH) proved ineffective, but texture parameters derived from intensity data showed potential. We were able to estimate forest biomass amounts up to 360 t/ha with a goodness of fit of 0.78 (adjusted <formula formulatype="inline"><tex Notation="TeX">$r^{2}$</tex></formula>) and an rmse of 28.68 t/ha using the combination of texture parameters of both polarizations (C-HV and C-HH). However, goodness of fit could be improved to 0.91 (adjusted <formula formulatype="inline"><tex Notation="TeX">$r^{2}$</tex></formula>) and an rmse of 26.95 t/ha for biomass levels up to 532 t/ha using the ratio of texture parameters of C-HV/C-HH. The result is very encouraging and indicates that the dual-polarization C-band SAR sensor has a potential for the estimation of forest biomass, particularly using the polarization ratio of texture measurements, and biomass estimation can be improved substantially beyond the previously stated saturation level for C-band SAR.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6353204]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3371</startPage>
			<endPage>3384</endPage>
			<fileSize>1437</fileSize>
			<authors><![CDATA[Sarker, M.L.R.;Nichol, J.;Iz, H.B.;Ahmad, B.B.;Rahman, A.A.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Use of Handheld Thermal Imager Data for Airborne Mapping of Fire Radiative Power and Energy and Flame Front Rate of Spread]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377291]]></link>
			<description><![CDATA[Infrared (IR) remote sensing is increasingly used in studies of vegetation fire behavior, and high spatiotemporal resolution investigations often require data to be collected from airborne platforms, for example, standard helicopters. This paper aims to extend the range of conditions under which low-cost &#x201C;handheld&#x201D; thermal imaging cameras can be employed in such studies, particularly by enabling the effective and efficient geometric correction of thermal imagery collected from such devices, even when viewing far off-nadir (e.g., out of a side door or window). The approach is based on the automated detection of a set of fixed thermal &#x201C;ground control points,&#x201D; coupled with the use of a linear transformation matrix for warping the raw IR imagery to a fixed coordinate system. The output set of geometrically corrected brightness temperature and radiance images can be used to derive fire radiative power (FRP) and flame front rate of spread (ROS). We demonstrate and test our IR image processing methods on a series of case study fires, ranging from a small-scale laboratory to a 945- <formula formulatype="inline"><tex Notation="TeX">$hbox{m}^{2}$</tex></formula> outdoor experimental burn. We compare mapped information on FRP obtained from simultaneous nadir and off-nadir views, where we find differences that are in part controlled by flame structure and/or view angle. In the large open fire case, we compare the mapped fire radiative energy and ROS to simultaneously acquired aerial photography that provides the position of fuel and flames in high detail, and we demonstrate how these data sets can be used to explore various aspects of fire behavior.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377291]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3385</startPage>
			<endPage>3399</endPage>
			<fileSize>2440</fileSize>
			<authors><![CDATA[Paugam, R.;Wooster, M.J.;Roberts, G.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Classification of Seismic Volcanic Signals Using Hidden-Markov-Model-Based Generative Embeddings]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377284]]></link>
			<description><![CDATA[The automated classification of seismic volcanic signals has been faced with several different pattern recognition approaches. Among them, hidden Markov models (HMMs) have been advocated as a cost-effective option having the advantages of a straightforward Bayesian interpretation and the capacity of dealing with seismic sequences of different lengths. In the volcano seismology scenario, HMM-based classification schemes were only based on a standard and purely generative scheme, i.e., the Bayes rule: training an HMM per class and classifying an incoming seismic signal according to the class whose model shows the highest likelihood. In this paper, a novel HMM-based classification approach for pretriggered seismic volcanic signals is proposed. The main idea is to enrich the classical HMM scheme with a discriminative step that is able to recover from situations when the classical Bayes classification rule is not sufficient. More in detail, a generative embedding scheme is used, which employs the models to map the signals into a vector space, which is called generative embedding space. In such a space, any discriminative vector-based classifier can be applied. A thorough set of experiments, which is carried out on pretriggered signals recorded at Galeras Volcano in Colombia, shows that the proposed approach typically outperforms standard HMM-based classification schemes, also in some cross-station cases.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377284]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3400</startPage>
			<endPage>3409</endPage>
			<fileSize>753</fileSize>
			<authors><![CDATA[Bicego, M.;Acosta-Munoz, C.;Orozco-Alzate, M.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Estimating Tree-Root Biomass in Different Depths Using Ground-Penetrating Radar: Evidence from a Controlled Experiment]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6392930]]></link>
			<description><![CDATA[Roots have important functions in the ecosystem. Therefore, establishing root-related parameters such as root size, biomass, and 3-D architecture is necessary. Traditional methods for measuring tree roots are labor intensive and destructive to nature, limiting quantitative and repeated assessments in long-term research. Ground-penetrating radar (GPR) provides a nondestructive method for measuring tree roots. This study investigates the feasibility of a GPR system with 500-MHz, 900-MHz, and 2-GHz measurement frequencies for detecting tree roots and estimating root biomass under controlled experimental conditions in a sandy area. After energy attenuation correction and velocity analysis, not only the individual root in subsurface is able to be located but also the parameters that correlate well with root biomass can be extracted from the processed GPR data. The major findings were as follows. First, both the amplitude and amplitude-area indices were confirmed to be more effective for estimating root biomass after attenuation-effect compensation. This result suggests that the calibration of GPR wave-attenuation effects and velocity changes with depth are helpful in estimating root biomass from GPR parameters. Second, the selection of GPR system frequency was mainly dependent on field conditions, particularly soil water content. Lower frequency was recommended for developing root biomass estimation model under varied soil conditions. Third, the new method based on the metal reflector experiment was effective and easy to perform in situ for attenuation-effect correction.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6392930]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3410</startPage>
			<endPage>3423</endPage>
			<fileSize>1245</fileSize>
			<authors><![CDATA[Cui, X.;Guo, L.;Chen, J.;Chen, X.;Zhu, X.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Using DInSAR to Separate Surface and Subsurface Features]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6392259]]></link>
			<description><![CDATA[We report on an investigation into the use of differential interferometric synthetic aperture radar (SAR) (DInSAR) for the discrimination between surface and subsurface features in a soil, undertaken at the Ground-Based SAR Microwave Measurement Facility. A temporal sequence of C-band VV SAR images of a drying soil containing a buried target was collected. While the phase record of the signal identified with the soil return showed almost no variation, in stark contrast, the phase from the buried target showed a strongly linear change with time. A model is presented, which describes the observed phase changes in terms of retardation of the signal by the soil dielectric properties, which are dependent upon the moisture content. The model confirms a strongly linear relationship between phase and volumetric soil moisture. The linearity promises to greatly simplify any exploitation scheme, and such a DInSAR scheme would be applicable at large standoff distances from airborne and spaceborne platforms, in contrast to current subsurface techniques which rely on close-in measurement to spatially isolate returns vertically in backscatter.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6392259]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3424</startPage>
			<endPage>3430</endPage>
			<fileSize>483</fileSize>
			<authors><![CDATA[Morrison, K.;Bennett, J.C.;Nolan, M.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Suppression of Borehole-Guided Waves Supported by the Connection Cable of a Single-Borehole Monostatic Pulse Radar]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375808]]></link>
			<description><![CDATA[Recently, a single-borehole monostatic pulse radar has been developed and operated at a well-suited tunnel test site. The measured B-scan data were severely contaminated by obliquely striped patterns. In this paper, numerical simulations and field experiments are performed to find a proper way of suppressing the unwanted striped patterns. For numerical analysis, the finite-difference time domain is applied to a simplified 2-D model consisting of a water-filled borehole, two different rocks, and a dipole antenna connected to a conducting cable. It can be visualized that a set of oblique lines is generated from the borehole-guided waves reflected at the interface of two different rocks. When the conducting cable is coated by a perfect magnetic conductor (PMC), the oblique lines are nearly eliminated in the simulated B-scan result. In practice, the PMC coating is replaced by a ferrite core loading, and those loading effects on suppressing the borehole-guided waves are measured by operating our single-borehole monostatic pulse radar at a well-suited tunnel test site. Without a ferrite core loading on the connection cable, the borehole-guided waves cause the measured B-scan to be contaminated by the unwanted striped patterns. When a ferrite core is wrapped around the connection cable, the borehole-guided waves are nearly removed in the measured B-scan data. In particular, the unwanted striped patterns can be suppressed over 90% even if the total length of a ferrite core decreases to 0.5 m.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375808]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3431</startPage>
			<endPage>3438</endPage>
			<fileSize>1377</fileSize>
			<authors><![CDATA[Cho, J.-H.;Jung, J.-H.;Kim, S.-W.;Kim, S.-Y.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Real-Time Processing of Electromagnetic Induction Dynamic Data Using Kalman Filters for Unexploded Ordnance Detection]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6353912]]></link>
			<description><![CDATA[The current procedure to detect and identify unexploded ordnance (UXO) using electromagnetic induction (EMI) time-domain sensors is based on two steps. First, data are acquired over large areas in dynamic mode, and locations of interest are flagged based on measured field amplitudes. Second, sensors return to the flagged areas for more in-depth cued interrogation, providing high-quality data for subsequent identification and classification. Flagging based on field amplitude, however, has potential drawbacks: The magnetic field in the EMI regime exhibits a <formula formulatype="inline"><tex Notation="TeX">$1/R^{6}$</tex></formula> drop-off with range, and a deep UXO may not produce a strong response while still being potentially hazardous. To address this problem, we propose in this paper an inversion method based on Kalman and extended Kalman filters meant to do the following: 1) work with dynamic data; 2) provide both position and polarizability estimates; and 3) operate in real time (less than 100 ms in our case). Such full characterization of the target, albeit limited to within the 2.7-ms interrogation time window of the dynamic mode associated with the sensors studied here, provides useful information when deciding whether to continue with the cued interrogation. We validate the method for two popular EMI sensors, the second-version Man Portable Vector (MPV-II) and the MetalMapper, operated in very different settings: The MPV-II is used to interrogate a limited region of space atop a single target, whereas the MetalMapper is driven over long lanes along which several targets and clutter items are present.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6353912]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3439</startPage>
			<endPage>3451</endPage>
			<fileSize>1996</fileSize>
			<authors><![CDATA[Grzegorczyk, T.M.;Barrowes, B.E.;]]></authors>
		</item>
		<item>
			<title><![CDATA[A Study of Sea Surface Range-Resolved Doppler Spectra Using Numerically Simulated Low-Grazing-Angle Backscatter Data]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377286]]></link>
			<description><![CDATA[A numerical study of sea surface range-resolved Doppler spectra using low-grazing-angle backscatter measurements is described. Backscattered fields as a function of frequency are computed using the method of moments (MOM) for a single realization of a 1-D oceanlike surface profile as the realization evolves in time. Transformation into the range-Doppler domain enables examination of properties of the resulting Doppler spectra (for both HH and VV polarizations) and their relationship to properties of the surface profile. In general, a strong correspondence between the &#x201C;long-wave&#x201D; orbital velocity of the surface projected along the radar line of sight and the Doppler centroid frequency is observed for visible portions of the surface, as well as some evidence of relationships between the &#x201C;width&#x201D; of the Doppler spectrum and variations of the projected velocity in time at a given range point. Evidence of similar relationships even in some shadowed portions of the surface is also provided. Doppler spectra from HH and VV polarizations are qualitatively similar, despite differences in total power levels, although the portion of shadowed surface points from which Doppler information is available is somewhat larger in VV polarization. A further examination is conducted using backscattered fields computed with a single-scattering method, which neglects shadowing and any multiple-scattering effects. The remarkable similarities observed between MOM and single-scattered Doppler spectra even in some shadowed portions of the surface suggest that non-line-of-sight propagation effects do not significantly influence Doppler properties in such regions.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6377286]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3452</startPage>
			<endPage>3460</endPage>
			<fileSize>1721</fileSize>
			<authors><![CDATA[Chae, C.-S.;Johnson, J.T.;]]></authors>
		</item>
		<item>
			<title><![CDATA[Computation of Radar Scattering From Heterogeneous Rough Soil Using the Finite-Element Method]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375807]]></link>
			<description><![CDATA[A 2-D vector-element-based finite-element method (FEM) is used to calculate the radar backscatter from 1-D bare rough soil surfaces which can have an underlying heterogeneous substrate. Monte Carlo simulation results are presented for scattering at L-band <formula formulatype="inline"><tex Notation="TeX">$(lambda = 0.24 hbox{m})$</tex></formula>. For homogeneous soils with rough surfaces, the results of FEM are compared with the predictions of the small perturbation method. In the case of heterogeneous substrates, soil moisture (and, hence, soil permittivity) is assumed to vary as a function of depth. In this case, the results of FEM are compared with those of the transfer matrix method for flat soil surfaces. In both cases, a good agreement is found. For homogeneous rough soils, it is found that polarimetric radar backscatter and copolarized phase difference have a nonlinear relationship with soil moisture. Finally, it is found that the nature of the soil moisture variation in the top few centimeters of the soil has a strong influence on the backscatter and, hence, on the inferred soil moisture content.]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6375807]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3461</startPage>
			<endPage>3469</endPage>
			<fileSize>800</fileSize>
			<authors><![CDATA[Khankhoje, U.K.;van Zyl, J.J.;Cwik, T.A.;]]></authors>
		</item>
		<item>
			<title><![CDATA[IEEE Geoscience and Remote Sensing Magazine]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516986]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516986]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3470</startPage>
			<endPage>3470</endPage>
			<fileSize>296</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[2013 IEEE membership form]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517013]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517013]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>3471</startPage>
			<endPage>3472</endPage>
			<fileSize>1484</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[IEEE Transactions on Geoscience and Remote Sensing information for authors]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517024]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6517024]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>C3</startPage>
			<endPage>C3</endPage>
			<fileSize>107</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
		<item>
			<title><![CDATA[IEEE Transactions on Geoscience and Remote Sensing institutional listings]]></title>
			<link><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516987]]></link>
			<description><![CDATA[ ]]></description>
			<pubDate><![CDATA[June  2013]]></pubDate>
			<guid><![CDATA[http://ieeexplore.ieee.org/xpl/articleDetails.jsp?arnumber=6516987]]></guid>
			<volume>51</volume>
			<issue>6</issue>
			<startPage>C4</startPage>
			<endPage>C4</endPage>
			<fileSize>197</fileSize>
			<authors><![CDATA[]]></authors>
		</item>
	</channel>
</rss>