BAND SELECTION METHOD APPLIED TO M3 (MOON MINERALOGY MAPPER)
dc.contributor.author | Cavanagh, Patrick D. | |
dc.contributor.author | Li, Lin | |
dc.date.accessioned | 2015-11-18T02:15:35Z | |
dc.date.available | 2015-11-18T02:15:35Z | |
dc.date.issued | 2012-04-13 | |
dc.description | poster abstract | en_US |
dc.description.abstract | Remote sensing optical sensors, such as those on board satellites and planetary probes, are able to detect and measure solar radiation at both im-proved spectral and spatial resolution. In particular, a hyperspectral dataset often consists of tens to hundreds of specified wavelength bands and con-tains a vast amount of spectral information for potential processing. One drawback of such a large spectral dataset is information redundancy result-ing from high correlation between narrow spectral bands. Reducing the data dimensionality is critical in practical hyperspectral remote sensing applica-tions. Price’s method is a band selection approach that uses a small subset of bands to accurately reconstruct the full hyperspectral dataset. The method seeks to represent the dataset by a weighted sum of basis functions. An it-erative process is used to successively approximate the full dataset. The process ends when the last basis function no longer provides a significant contribution to the reconstruction of the dataset, i.e. the basis function is dominated by noise. The research presented examines the feasibility of Price’s method for ex-tracting an optimal band subset from recently acquired lunar hyperspectral images recorded by the Moon Mineralogy Mapper (M3) instrument on board the Chandrayaan-1 spacecraft. The Apollo 17 landing site was used for test-ing of the band selection method. Preliminary results indicate that the band selection method is able to successfully reconstruct the original hyperspectral dataset with minimal error. In a recent test case, 15 bands were used to reconstruct the original 74 bands of reflectance data. This represents an accurate reconstruction using only 20% of the original dataset. The results from this study can help to configure spectral channels of fu-ture optical instruments for lunar exploration. The channels can be chosen based on the knowledge of which wavelength bands represent the greatest relevant information for characterizing geology of a particular location. | en_US |
dc.identifier.citation | Patrick D. Cavanagh and Lin Li. (2012, April 13). BAND SELECTION METHOD APPLIED TO M3 (MOON MINERALOGY MAPPER). Poster session presented at IUPUI Research Day 2012, Indianapolis, Indiana. | en_US |
dc.identifier.uri | https://hdl.handle.net/1805/7475 | |
dc.language.iso | en_US | en_US |
dc.publisher | Office of the Vice Chancellor for Research | en_US |
dc.subject | M3 (MOON MINERALOGY MAPPER) | en_US |
dc.subject | remote sensing | en_US |
dc.subject | wavelength bands | en_US |
dc.subject | spectral dataset | en_US |
dc.title | BAND SELECTION METHOD APPLIED TO M3 (MOON MINERALOGY MAPPER) | en_US |
dc.type | Poster | en_US |