22,647 research outputs found
Mapping and classification of ecologically sensitive marine habitats using unmanned aerial vehicle (UAV) imagery and object-based image analysis (OBIA)
Nowadays, emerging technologies, such as long-range transmitters, increasingly miniaturized components for positioning, and enhanced imaging sensors, have led to an upsurge in the availability of new ecological applications for remote sensing based on unmanned aerial vehicles (UAVs), sometimes referred to as ādronesā. In fact, structure-from-motion (SfM) photogrammetry coupled with imagery acquired by UAVs offers a rapid and inexpensive tool to produce high-resolution orthomosaics, giving ecologists a new way for responsive, timely, and cost-effective monitoring of ecological processes. Here, we adopted a lightweight quadcopter as an aerial survey tool and object-based image analysis (OBIA) workflow to demonstrate the strength of such methods in producing very high spatial resolution maps of sensitive marine habitats. Therefore, three different coastal environments were mapped using the autonomous flight capability of a lightweight UAV equipped with a fully stabilized consumer-grade RGB digital camera. In particular we investigated a Posidonia oceanica seagrass meadow, a rocky coast with nurseries for juvenile fish, and two sandy areas showing biogenic reefs of Sabelleria alveolata. We adopted, for the first time, UAV-based raster thematic maps of these key coastal habitats, produced after OBIA classification, as a new method for fine-scale, low-cost, and time saving characterization of sensitive marine environments which may lead to a more effective and efficient monitoring and management of natural resource
Semi-supervised Learning for Photometric Supernova Classification
We present a semi-supervised method for photometric supernova typing. Our
approach is to first use the nonlinear dimension reduction technique diffusion
map to detect structure in a database of supernova light curves and
subsequently employ random forest classification on a spectroscopically
confirmed training set to learn a model that can predict the type of each newly
observed supernova. We demonstrate that this is an effective method for
supernova typing. As supernova numbers increase, our semi-supervised method
efficiently utilizes this information to improve classification, a property not
enjoyed by template based methods. Applied to supernova data simulated by
Kessler et al. (2010b) to mimic those of the Dark Energy Survey, our methods
achieve (cross-validated) 95% Type Ia purity and 87% Type Ia efficiency on the
spectroscopic sample, but only 50% Type Ia purity and 50% efficiency on the
photometric sample due to their spectroscopic follow-up strategy. To improve
the performance on the photometric sample, we search for better spectroscopic
follow-up procedures by studying the sensitivity of our machine learned
supernova classification on the specific strategy used to obtain training sets.
With a fixed amount of spectroscopic follow-up time, we find that deeper
magnitude-limited spectroscopic surveys are better for producing training sets.
For supernova Ia (II-P) typing, we obtain a 44% (1%) increase in purity to 72%
(87%) and 30% (162%) increase in efficiency to 65% (84%) of the sample using a
25th (24.5th) magnitude-limited survey instead of the shallower spectroscopic
sample used in the original simulations. When redshift information is
available, we incorporate it into our analysis using a novel method of altering
the diffusion map representation of the supernovae. Incorporating host
redshifts leads to a 5% improvement in Type Ia purity and 13% improvement in
Type Ia efficiency.Comment: 16 pages, 11 figures, accepted for publication in MNRA
Variable selection and updating in model-based discriminant analysis for high dimensional data with food authenticity applications
Food authenticity studies are concerned with determining if food samples have been correctly labelled or not. Discriminant analysis methods are an integral part of the methodology for food authentication. Motivated by food authenticity applications, a model-based discriminant analysis method that includes variable selection is presented. The discriminant analysis model is fitted in a semi-supervised manner using both labeled and unlabeled data. The method is shown to give excellent classification
performance on several high-dimensional multiclass food authenticity datasets with more variables than observations. The variables selected by the proposed method provide information about which variables are meaningful for classification purposes. A headlong search strategy for variable selection is shown to be efficient in terms of computation and achieves excellent classification performance. In applications to several food authenticity datasets, our proposed method outperformed default implementations of Random Forests, AdaBoost, transductive SVMs and Bayesian Multinomial Regression by substantial margins
Optimal land cover mapping and change analysis in northeastern oregon using landsat imagery.
Abstract The necessity for the development of repeatable, efficient, and accurate monitoring of land cover change is paramount to successful management of our planetās natural resources. This study evaluated a number of remote sensing methods for classifying land cover and land cover change throughout a two-county area in northeastern Oregon (1986 to 2011). In the past three decades, this region has seen significant changes in forest management that have affected land use and land cover. This study employed an accuracy assessment-based empirical approach to test the optimality of a number of advanced digital image processing techniques that have recently emerged in the field of remote sensing. The accuracies are assessed using traditional error matrices, calculated using reference data obtained in the field. We found that, for single-time land cover classification, Bayes pixel-based classification using samples created with scale and shape segmentation parameters of 8 and 0.3, respectively, resulted in the highest overall accuracy. For land cover change detection, using Landsat-5 TM band 7 with a change threshold of 1.75 standard deviations resulted in the highest accuracy for forest harvesting and regeneration mapping
Stellar classification from single-band imaging using machine learning
Information on the spectral types of stars is of great interest in view of
the exploitation of space-based imaging surveys. In this article, we
investigate the classification of stars into spectral types using only the
shape of their diffraction pattern in a single broad-band image. We propose a
supervised machine learning approach to this endeavour, based on principal
component analysis (PCA) for dimensionality reduction, followed by artificial
neural networks (ANNs) estimating the spectral type. Our analysis is performed
with image simulations mimicking the Hubble Space Telescope (HST) Advanced
Camera for Surveys (ACS) in the F606W and F814W bands, as well as the Euclid
VIS imager. We first demonstrate this classification in a simple context,
assuming perfect knowledge of the point spread function (PSF) model and the
possibility of accurately generating mock training data for the machine
learning. We then analyse its performance in a fully data-driven situation, in
which the training would be performed with a limited subset of bright stars
from a survey, and an unknown PSF with spatial variations across the detector.
We use simulations of main-sequence stars with flat distributions in spectral
type and in signal-to-noise ratio, and classify these stars into 13 spectral
subclasses, from O5 to M5. Under these conditions, the algorithm achieves a
high success rate both for Euclid and HST images, with typical errors of half a
spectral class. Although more detailed simulations would be needed to assess
the performance of the algorithm on a specific survey, this shows that stellar
classification from single-band images is well possible.Comment: 10 pages, 9 figures, 2 tables, accepted in A&
Analytical design of multispectral sensors
An optimal design based on the criterion of minimum mean square representation error using the Karhunen-Loeve expansion was developed to represent the spectral response functions from a stratum based upon a stochastic process scene model. From the overall pattern recognition system perspective, the effect of the representation accuracy on a typical performance criterion (the probability of correct classification) is investigated. The optimum sensor design provides a standard against which practical (suboptimum) operational sensors can be compared. An example design is provided and its performance is illustrated. Although developed primarily for the purpose of sensor design, the procedure has potential for making important contributions to scene understanding. Spectral channels which have narrow bandwidths relative to current sensor systems may be necessary to provide adequate spectral representation and improved classification performance
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