%0 Journal Article %1 Bellucci2004a %A Bellucci, G. %A Formisano, V. %A D'Aversa, E. %A Brown, R. H. %A Baines, K. H. %A Bibring, J. P. %A Buratti, B. J. %A Capaccioni, F. %A Cerroni, P. %A Clark, R. N. %A Coradini, A. %A Cruikshank, D. P. %A Drossart, P. %A Jaumann, R. %A Langevin, Y. %A Matson, D. L. %A McCord, T. B. %A Mennella, V. %A Nelson, R. M. %A Nicholson, P. D. %A Sicardy, B. %A Sotin, C. %A Chamberlain, M. C. %A Hansen, G. %A Hibbits, K. %A Showalter, M. %A Filacchione, G. %D 2004 %J PLANETARY IONOSPHERES AND ATMOSPHERES INCLUDING CIRA %K imported %N 8 %P 1640--1646 %T Principal components analysis of Jupiter VIMS spectra %V 34 %X During CassiniJupiter flyby occurred in December 2000, Visual-Infrared mapping spectrometer (VIMS) instrument took several image cubes of Jupiter at different phase angles and distances. We have analysed the spectral images acquired by the VIMS visual channel by means of a principal component analysis technique (PCA). The original data set consists of 96 spectral images in the 0.35-1.05 mum wavelength range. The product of the analysis are new PC bands, which contain all the spectral variance of the original data. These new components have been used to produce a map of Jupiter made of seven coherent spectral classes. The map confirms previously published work done on the Great Red Spot by using NIMS data. Some other new findings, presently under investigation, are presented. (C) 2004 Published by Elsevier Ltd on behalf of COSPAR.

@article{Bellucci2004a, abstract = {During CassiniJupiter flyby occurred in December 2000, Visual-Infrared mapping spectrometer (VIMS) instrument took several image cubes of Jupiter at different phase angles and distances. We have analysed the spectral images acquired by the VIMS visual channel by means of a principal component analysis technique (PCA). The original data set consists of 96 spectral images in the 0.35-1.05 mum wavelength range. The product of the analysis are new PC bands, which contain all the spectral variance of the original data. These new components have been used to produce a map of Jupiter made of seven coherent spectral classes. The map confirms previously published work done on the Great Red Spot by using NIMS data. Some other new findings, presently under investigation, are presented. (C) 2004 Published by Elsevier Ltd on behalf of COSPAR.}, added-at = {2009-11-03T20:21:25.000+0100}, author = {Bellucci, G. and Formisano, V. and D'Aversa, E. and Brown, R. H. and Baines, K. H. and Bibring, J. P. and Buratti, B. J. and Capaccioni, F. and Cerroni, P. and Clark, R. N. and Coradini, A. and Cruikshank, D. P. and Drossart, P. and Jaumann, R. and Langevin, Y. and Matson, D. L. and McCord, T. B. and Mennella, V. and Nelson, R. M. and Nicholson, P. D. and Sicardy, B. and Sotin, C. and Chamberlain, M. C. and Hansen, G. and Hibbits, K. and Showalter, M. and Filacchione, G.}, biburl = {https://www.bibsonomy.org/bibtex/22631174404da46f26786ac9b99777c50/svance}, citedreferences = {DAVIS JC, 1986, STAT DATA ANAL ; DYUDINA UA, 2001, Icarus, V150, P219 ; JUERGENS DW, 1990, INT J IMAGING SYSTEM, V3, P108 ; KARKOSCHKA E, 1994, Icarus, V111, P74 ; PIETERS CM, 1999, 980 LPI, P47 ; SIMONMILLER AA, 2001, Icarus, V154, P459 ; TOU JT, 1974, PATTERN RECOGNITION}, interhash = {3f83598c72080def224fec4384cd8228}, intrahash = {2631174404da46f26786ac9b99777c50}, journal = {PLANETARY IONOSPHERES AND ATMOSPHERES INCLUDING CIRA}, keywords = {imported}, number = 8, owner = {svance}, pages = {1640--1646}, timestamp = {2009-11-03T20:21:39.000+0100}, title = {Principal components analysis of Jupiter VIMS spectra}, volume = 34, year = 2004 }