[GRASS-SVN] r60236 - grass-promo/grassposter/2014_EGU_M3_Landscape
svn_grass at osgeo.org
svn_grass at osgeo.org
Tue May 13 23:43:12 PDT 2014
Author: ychemin
Date: 2014-05-13 23:43:12 -0700 (Tue, 13 May 2014)
New Revision: 60236
Added:
grass-promo/grassposter/2014_EGU_M3_Landscape/poster.bib
Modified:
grass-promo/grassposter/2014_EGU_M3_Landscape/poster.tex
Log:
Update poster tex+bib
Added: grass-promo/grassposter/2014_EGU_M3_Landscape/poster.bib
===================================================================
--- grass-promo/grassposter/2014_EGU_M3_Landscape/poster.bib (rev 0)
+++ grass-promo/grassposter/2014_EGU_M3_Landscape/poster.bib 2014-05-14 06:43:12 UTC (rev 60236)
@@ -0,0 +1,507 @@
+ at article{tagkey1979467,
+title = "Standard techniques for presentation and analysis of crater size-frequency data ",
+journal = "Icarus ",
+volume = "37",
+number = "2",
+pages = "467 - 474",
+year = "1979",
+note = "",
+issn = "0019-1035",
+doi = "http://dx.doi.org/10.1016/0019-1035(79)90009-5",
+url = "http://www.sciencedirect.com/science/article/pii/0019103579900095",
+key = "tagkey1979467"
+}
+
+ at article{A17PET1973,
+author = {A17PrelExamTeam},
+title = {Apollo 17 Lunar Samples: Chemical and Petrographic Description},
+volume = {182},
+number = {4113},
+pages = {659-672},
+year = {1973},
+doi = {10.1126/science.182.4113.659},
+URL = {http://www.sciencemag.org/content/182/4113/659.short},
+eprint = {http://www.sciencemag.org/content/182/4113/659.full.pdf},
+journal = {Science}
+}
+
+ at article{arvidson1979standard,
+ title={Standard techniques for presentation and analysis of crater size-frequency data},
+ author={Arvidson, RE and Boyce, J and Chapman, C and Cintala, M and Fulchignoni, M and Moore, H and Neukum, G and Schultz, P and Soderblom, L and Strom, R and others},
+ journal={Icarus},
+ volume={37},
+ pages={467--474},
+ year={1979}
+}
+
+ at article{Baldridge2009711,
+title = "The \{ASTER\} spectral library version 2.0 ",
+journal = "Remote Sensing of Environment ",
+volume = "113",
+number = "4",
+pages = "711 - 715",
+year = "2009",
+note = "",
+issn = "0034-4257",
+doi = "http://dx.doi.org/10.1016/j.rse.2008.11.007",
+url = "http://www.sciencedirect.com/science/article/pii/S0034425708003441",
+author = "A.M. Baldridge and S.J. Hook and C.I. Grove and G. Rivera",
+keywords = "\{ASTER\}",
+keywords = "Spectral library ",
+abstract = "The Advanced Spaceborne Thermal Emission Reflection Radiometer (ASTER) on NASA's Terra platform has been widely used in geological and other science studies. In support of \{ASTER\} studies, a library of natural and man-made materials was compiled as the \{ASTER\} Spectral Library v1.2 and made available from http://speclib.jpl.nasa.gov. The library is a collection of contributions in a standard format with ancillary data from the Jet Propulsion Laboratory (JPL), Johns Hopkins University (JHU) and the United States Geological Survey (USGS). A new version of the library (v2.0) is now available online or via CD, which includes major additions to the mineral and rock spectra. The \{ASTER\} library provides a comprehensive collection of over 2300 spectra of a wide variety of materials covering the wavelength range 0.4–15.4 µm. "
+}
+
+%Boardman, J. W., C. M. Pieters, R. O. Green, S. R. Lundeen, P. Varanasi, J. W. Nettles, N. E. Petro, P. J. Isaacson, S. Besse, and L. A. Taylor (2011), Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation and related level 1B products of the Moon Mineralogy Mapper, J. Geophys. Res., 116, E00G14 , doi:10.1029/2010JE003730.
+ at article{boardman2011measuring,
+ title={Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation and related level 1B products of the Moon Mineralogy Mapper},
+ author={Boardman, J. W. and Pieters, C. M. and Green, R. O. and Lundeen, S. R. and Varanasi, P. and Nettles, J. W. and Petro, N. E. and Isaacson, P. J. and Besse, S. and Taylor, L. A.},
+ journal={J. Geophys. Res.},
+ volume={41},
+ year={2011}
+}
+
+%Bugiolacchi, R., Spudis, P.D., Guest, J.E., 2006. Stratigraphy and composition of lava flows in Mare Nubium and Mare Cognitum. Meteoritics & Planetary Science. 41(2):285-304.
+ at article{bugiolacchi2006stratigraphy,
+ title={Stratigraphy and composition of lava flows in Mare Nubium and Mare Cognitum},
+ author={Bugiolacchi, Roberto and Spudis, Paul D and Guest, John E},
+ journal={Meteoritics \& Planetary Science},
+ volume={41},
+ number={2},
+ pages={285--304},
+ year={2006},
+ publisher={Wiley Online Library}
+}
+
+%J. Canny. A Computational Approach to Edge Detection. In: IEEE Trans. Pattern Anal. Mach. Intell. 8.6 (June 1986), pp. 679-698
+ at article{canny1986computational,
+ title={A computational approach to edge detection},
+ author={Canny, John},
+ journal={Pattern Analysis and Machine Intelligence, IEEE Transactions on},
+ number={6},
+ pages={679--698},
+ year={1986},
+ publisher={IEEE}
+}
+
+
+ at book{clark2007usgs,
+ title={USGS digital spectral library splib06a},
+ author={Clark, Roger Nelson and Swayze, Gregg A and Wise, R and Livo, E and Hoefen, T and Kokaly, R and Sutley, Stephen J},
+ year={2007},
+ publisher={US Geological Survey Denver, CO}
+}
+
+ at article{Crawford01062007,
+author = {Crawford, Ian A and Joy, Katherine H and Fagents, Sarah A},
+title = {Full Moon exploration},
+volume = {48},
+number = {3},
+pages = {3.18-3.21},
+year = {2007},
+doi = {10.1111/j.1468-4004.2007.48318.x},
+abstract ={The Moon is a promising science target, made a priority in recent space exploration plans. So far, polar landing sites have been preferred, but many promising scientific objectives lie elsewhere. Here we summarize the potential value of one such scientific target, northern Oceanus Procellarum, which includes basalts of a wide range of ages. Studying these would allow refinement of the lunar stratigraphy and chronology, and a better understanding of lunar mantle evolution. We consider how exploration of such areas might be achieved in the context of lunar exploration plans.},
+URL = {http://astrogeo.oxfordjournals.org/content/48/3/3.18.abstract},
+eprint = {http://astrogeo.oxfordjournals.org/content/48/3/3.18.full.pdf+html},
+journal = {Astronomy & Geophysics}
+}
+
+%Eliason, E., Isbell, C., Lee, E., Becker, T., Gaddis, L., McEwen, E., Robinson, M., 1999. The Clementine UVVIS global lunar mosaic. NASA Planetary Data System CD-ROM Archive, pp. CL_4001-CL_4078.
+
+ at article{florensky1981essays,
+ title={Essays of Comparative Planetology},
+ author={Florensky, K.P. and 12 colleagues and 12 colleagues},
+ journal={Nauka Press},
+ year={1981}
+}
+
+ at article{fortezzo2013completed,
+ title={Completed Digital Renovation of the 1: 5,000,000 Lunar Geologic Map Series},
+ author={Fortezzo, CM and Hare, TM},
+ journal={LPI Contributions},
+ volume={1719},
+ pages={2114},
+ year={2013}
+}
+
+ at article {green2011moon,
+ author = {Green, R. O. and Pieters, C. and Mouroulis, P. and Eastwood, M. and Boardman, J. and Glavich, T. and Isaacson, P. and Annadurai, M. and Besse, S. and Barr, D. and Buratti, B. and Cate, D. and Chatterjee, A. and Clark, R. and Cheek, L. and Combe, J. and Dhingra, D. and Essandoh, V. and Geier, S. and Goswami, J. N. and Green, R. and Haemmerle, V. and Head, J. and Hovland, L. and Hyman, S. and Klima, R. and Koch, T. and Kramer, G. and Kumar, A. S. K. and Lee, K. and Lundeen, S. and Malaret, E. and McCord, T. and McLaughlin, S. and Mustard, J. and Nettles, J. and Petro, N. and Plourde, K. and Racho, C. and Rodriquez, J. and Runyon, C. and Sellar, G. and Smith, C. and Sobel, H. and Staid, M. and Sunshine, J. and Taylor, L. and Thaisen, K. and Tompkins, S. and Tseng, H. and Vane, G. and Varanasi, P. and White, M. and Wilson, D.},
+ title = {The Moon Mineralogy Mapper (M3) imaging spectrometer for lunar science: Instrument description, calibration, on-orbit measurements, science data calibration and on-orbit validation},
+ journal = {Journal of Geophysical Research: Planets},
+ volume = {116},
+ number = {E10},
+ pages = {2156-2202},
+ year = {2011}
+}
+
+ at article{Greenhagen17092010,
+author = {Greenhagen, Benjamin T. and Lucey, Paul G. and Wyatt, Michael B. and Glotch, Timothy D. and Allen, Carlton C. and Arnold, Jessica A. and Bandfield, Joshua L. and Bowles, Neil E. and Hanna, Kerri L. Donaldson and Hayne, Paul O. and Song, Eugenie and Thomas, Ian R. and Paige, David A.},
+title = {Global Silicate Mineralogy of the Moon from the Diviner Lunar Radiometer},
+volume = {329},
+number = {5998},
+pages = {1507-1509},
+year = {2010},
+doi = {10.1126/science.1192196},
+abstract ={We obtained direct global measurements of the lunar surface using multispectral thermal emission mapping with the Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment. Most lunar terrains have spectral signatures that are consistent with known lunar anorthosite and basalt compositions. However, the data have also revealed the presence of highly evolved, silica-rich lunar soils in kilometer-scale and larger exposures, expanded the compositional range of the anorthosites that dominate the lunar crust, and shown that pristine lunar mantle is not exposed at the lunar surface at the kilometer scale. Together, these observations provide compelling evidence that the Moon is a complex body that has experienced a diverse set of igneous processes.},
+URL = {http://www.sciencemag.org/content/329/5998/1507.abstract},
+eprint = {http://www.sciencemag.org/content/329/5998/1507.full.pdf},
+journal = {Science}
+}
+
+ at book{hartlang2008exploring,
+ title={Exploring the Moon - The Apollo Expeditions (Second Edition)},
+ author={Hartlang, David M},
+ year={2008},
+ publisher={Praxis Publishing Ltd}
+}
+
+ at article{hawke2004origin,
+ title={The origin of lunar crater rays},
+ author={Hawke, B and Blewett, DT and Lucey, PG and Smith, GA and Bell III, JF and Campbell, Bruce A and Robinson, MS},
+ journal={Icarus},
+ volume={170},
+ number={1},
+ pages={1--16},
+ year={2004},
+ publisher={Elsevier}
+}
+
+ at book{heiken1991lunar,
+ title={Lunar sourcebook: A user's guide to the Moon},
+ author={Heiken, Grant and Vaniman, David and French, Bevan M},
+ year={1991},
+ publisher={CUP Archive}
+}
+
+ at article{hiesinger2003ages,
+ title={Ages and stratigraphy of mare basalts in oceanus procellarum, mare nubium, mare cognitum, and mare insularum},
+ author={Hiesinger, H and Head, JW and Wolf, U and Jaumann, R and Neukum, G},
+ journal={Journal of Geophysical Research: Planets (1991--2012)},
+ volume={108},
+ number={E7},
+ year={2003}
+}
+
+ at article{hiesinger2010ages,
+ title={Ages and stratigraphy of lunar mare basalts in Mare Frigoris and other nearside maria based on crater size-frequency distribution measurements},
+ author={Hiesinger, H and Head, JW and Wolf, U and Jaumann, R and Neukum, G},
+ journal={Journal of Geophysical Research: Planets (1991--2012)},
+ volume={115},
+ number={E3},
+ year={2010}
+}
+
+ at article{hiesinger2011ages,
+ title={Ages and stratigraphy of lunar mare basalts: A synthesis},
+ author={Hiesinger, H and Head III, JW and Wolf, U and Jaumann, R and Neukum, G},
+ journal={Recent Advances and Current Research Issues in Lunar Stratigraphy},
+ volume={477},
+ pages={1},
+ year={2011},
+ publisher={Geological Society of America}
+}
+
+
+ at article{king1976space,
+ title={Space geology: An introduction},
+ author={King, Elbert A},
+ journal={New York, John Wiley and Sons, Inc., 1976. 361 p.},
+ volume={1},
+ year={1976}
+}
+
+
+ at article{Korokhin20081063,
+title = "Prognosis of TiO2 abundance in lunar soil using a non-linear analysis of Clementine and \{LSCC\} data ",
+journal = "Planetary and Space Science ",
+volume = "56",
+number = "8",
+pages = "1063 - 1078",
+year = "2008",
+note = "",
+issn = "0032-0633",
+doi = "http://dx.doi.org/10.1016/j.pss.2008.02.001",
+url = "http://www.sciencedirect.com/science/article/pii/S0032063308000317",
+author = "Viktor V. Korokhin and Vadym G. Kaydash and Yuriy G. Shkuratov and Dmitry G. Stankevich and Urs Mall",
+keywords = "The moon",
+keywords = "Lunar surface",
+keywords = "Chemical composition",
+keywords = "Titanium abundance",
+keywords = "Prognosis",
+keywords = "Artificial neural network "
+}
+
+%Korotev, R.L., Jolliff, B.L., Zeigler, R.A., Seddio, S.M., Haskin, L.A., 2011. Apollo 12 revisited. Geochimica et Cosmochimica Acta. 75(6):1540-1573.
+ at article{korotev2011apollo,
+ title={Apollo 12 revisited},
+ author={Korotev, Randy L and Jolliff, Bradley L and Zeigler, Ryan A and Seddio, Stephen M and Haskin, Larry A},
+ journal={Geochimica et Cosmochimica Acta},
+ volume={75},
+ number={6},
+ pages={1540--1573},
+ year={2011},
+ publisher={Elsevier}
+}
+
+ at article{lal2012detection,
+ author = {Lal, D. and Chauhan, P. and Shah, R. D. and Bhattacharya, S. and Jai, A. and Kumar, A. S. K. },
+ title = {Detection of Mg spinel lithologies on central peak of crater Theophilus using Moon Mineralogy Mapper (M3) data from Chandrayaan-1},
+ journal = {Journal of Earth System Sciences},
+ volume = {121},
+ number = {3},
+ pages = {847-853},
+ year = {2012}
+}
+
+ at article{lawrence2002iron,
+ title={Iron abundances on the lunar surface as measured by the Lunar Prospector gamma-ray and neutron spectrometers},
+ author={Lawrence, DJ and Feldman, WC and Elphic, RC and Little, RC and Prettyman, TH and Maurice, S and Lucey, PG and Binder, AB},
+ journal={Journal of Geophysical Research: Planets (1991--2012)},
+ volume={107},
+ number={E12},
+ pages={13--1},
+ year={2002}
+}
+
+
+ at article{Li2008267,
+title = "Quantifying lunar soil composition with partial least squares modeling of reflectance ",
+journal = "Advances in Space Research ",
+volume = "42",
+number = "2",
+pages = "267 - 274",
+year = "2008",
+note = "",
+issn = "0273-1177",
+doi = "http://dx.doi.org/10.1016/j.asr.2007.06.018",
+url = "http://www.sciencedirect.com/science/article/pii/S0273117707006527",
+author = "Lin Li",
+keywords = "Lunar soil",
+keywords = "Reflectance",
+keywords = "Single scattering albedo",
+keywords = "Partial least squares",
+keywords = "Principal component regression "
+}
+
+ at article{lindsay1976lunar,
+ title={Lunar stratigraphy and sedimentology},
+ author={Lindsay, John F},
+ journal={Amsterdam, Elsevier Scientific Publishing Co.(Developments in Solar System-and Space Science, No. 3), 1976. 315 p.},
+ volume={1},
+ year={1976}
+}
+
+
+
+%Lucey, P.G., Blewett, D.T., Jolliff, B.L., 2000. Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images. J. Geophys. Res. 105(E8): 20297-20305.
+ at article{lucey2000lunar,
+ title={Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images},
+ author={Lucey, Paul G and Blewett, David T and Jolliff, Bradley L},
+ journal={Journal of Geophysical Research: Planets (1991--2012)},
+ volume={105},
+ number={E8},
+ pages={20297--20305},
+ year={2000},
+ publisher={Wiley Online Library}
+}
+
+%Lucey, P. G., B. T. Greenhagen, and the LRO Diviner Team (2012) Lunary mineral maps integrating thermal and near infrared multispectral imaging, 43rd Lunar and Planetary Science Conference, Abstract #1736.
+
+ at inproceedings{lucey2012lunary,
+ title={Lunary mineral maps integrating thermal and near infrared multispectral imaging},
+ author={Lucey, P. G. and Greenhagen, B. T. and LRO Diviner Team},
+ booktitle={Lunar and Planetary Institute Science Conference Abstracts},
+ volume={43},
+ pages={1736},
+ year={2012}
+}
+
+ at article{mason1970lunar,
+ title={The lunar rocks},
+ author={Mason, Brian Harold and Melson, William G},
+ journal={New York, Wiley-Interscience [1970]},
+ volume={1},
+ year={1970}
+}
+
+ at article{melosh1989impact,
+ title={Impact cratering: A geologic process},
+ author={Melosh, H Jay},
+ journal={Research supported by NASA. New York, Oxford University Press (Oxford Monographs on Geology and Geophysics, No. 11), 1989, 253 p.},
+ volume={1},
+ year={1989}
+}
+
+ at article{michael2010planetary,
+author = {{Michael}, G.~G. and {Neukum}, G.},
+title = "{Planetary surface dating from crater size-frequency distribution measurements: Partial resurfacing events and statistical age uncertainty}",
+journal = {Earth and Planetary Science Letters},
+year = 2010,
+month = jun,
+volume = 294,
+pages = {223-229},
+doi = {10.1016/j.epsl.2009.12.041},
+adsurl = {http://adsabs.harvard.edu/abs/2010E%26PSL.294..223M},
+adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+ at article{morota2011timing,
+ title={Timing and characteristics of the latest mare eruption on the Moon},
+ author={Morota, Tomokatsu and Haruyama, Junichi and Ohtake, Makiko and Matsunaga, Tsuneo and Honda, Chikatoshi and Yokota, Yasuhiro and Kimura, Jun and Ogawa, Yoshiko and Hirata, Naru and Demura, Hirohide and others},
+ journal={Earth and Planetary Science Letters},
+ volume={302},
+ number={3},
+ pages={255--266},
+ year={2011},
+ publisher={Elsevier}
+}
+
+ at article{neteler2012grass,
+ title={{GRASS GIS: a multi-purpose Open Source GIS}},
+ author={Neteler, M. and Bowman, M.H. and Landa, M. and Metz, M.},
+ journal={Environmental Modelling \& Software},
+ year={2012},
+ volume = {31},
+ pages = {124–130},
+ publisher={Elsevier},
+ doi = "10.1016/j.envsoft.2011.11.014"
+}
+
+ at mastersthesis{petras2014building,
+author = "Petras, Vaclav",
+keywords = "i.edge; r.houghtransform",
+location = "Prague",
+school = "Czech Technical University in Prague, Faculty of Civil Engineering",
+title = "{Building detection from aerial images in GRASS GIS environment}",
+year = "2012"
+}
+
+ at article{pieters2009moon,
+ title={The Moon Mineralogy Mapper (M 3) on Chandrayaan-1.},
+ author={Pieters, Carle M and Boardman, Joseph and Buratti, Bonnie and Chatterjee, Alok and Clark, Roger and Glavich, Tom and Green, Robert and Head III, James and Isaacson, Peter and Malaret, Erick and others},
+ journal={Current Science (00113891)},
+ volume={96},
+ number={4},
+ year={2009}
+}
+
+%Nawa, DF and JA Philpotts, 1979, A lunar differentiation model in light of new chemical data on Luna 20 and Apollo 16 soils, Regolith from the Highland Region of the Moon, VL Barsukov, 336, 344, Nauka Press, Moscow
+ at book{nawa1979lunar,
+ title={A lunar differentiation model in light of new chemical data on Luna 20 and Apollo 16 soils},
+ author={Nawa, DF and JA Philpotts},
+ pages={336--344},
+ year={1979},
+ publisher={Nauka Press, Moscow}
+}
+
+ at article{robinson2012confirmation,
+ title={Confirmation of sublunarean voids and thin layering in mare deposits},
+ author={Robinson, MS and Ashley, JW and Boyd, AK and Wagner, RV and Speyerer, EJ and Ray Hawke, B and Hiesinger, H and van der Bogert, CH},
+ journal={Planetary and Space Science},
+ volume={69},
+ number={1},
+ pages={18--27},
+ year={2012},
+ publisher={Elsevier}
+}
+
+
+%Shkuratov, Y. G., Kaydash, V. G., & Opanasenko, N. V. (1999). Iron and titanium abundance and maturity degree distribution on the lunar nearside. Icarus, 137(2), 222-234.
+ at article{shkuratov1999iron,
+ title={Iron and titanium abundance and maturity degree distribution on the lunar nearside},
+ author={Shkuratov, Yurij G and Kaydash, Vadym G and Opanasenko, Nickolaj V},
+ journal={Icarus},
+ volume={137},
+ number={2},
+ pages={222--234},
+ year={1999},
+ publisher={Elsevier}
+}
+
+
+%Snape, J.F., Alexander, L., Crawford, I.A., Joy, K.H., 2013. Basaltic Regolith Sample 12003,314: A New Member of the Apollo 12 Feldspathic Basalt Suite? Lunar and Planetary Institute Science Conference Abstracts 44:1044.
+ at inproceedings{Snape2013basaltic,
+ title={Basaltic Regolith Sample 12003,314: A New Member of the Apollo 12 Feldspathic Basalt Suite?},
+ author={Snape, Joshua F and Alexander, Louise and Crawford, Ian A and Joy, Katherine H},
+ booktitle={Lunar and Planetary Institute Science Conference Abstracts},
+ volume={44},
+ pages={1044},
+ year={2013}
+}
+
+ at article{stoffler2006cratering,
+ title={Cratering history and lunar chronology},
+ author={St{\"o}ffler, Dieter and Ryder, Graham and Ivanov, Boris A and Artemieva, Natalia A and Cintala, Mark J and Grieve, Richard AF},
+ journal={Reviews in Mineralogy and Geochemistry},
+ volume={60},
+ number={1},
+ pages={519--596},
+ year={2006},
+ publisher={Mineral Soc America}
+}
+
+ at article{strom2005origin,
+ title={The origin of planetary impactors in the inner solar system},
+ author={Strom, Robert G and Malhotra, Renu and Ito, Takashi and Yoshida, Fumi and Kring, David A},
+ journal={Science},
+ volume={309},
+ number={5742},
+ pages={1847--1850},
+ year={2005},
+ publisher={American Association for the Advancement of Science}
+}
+
+ at article{thomson2009new,
+ title={A new technique for estimating the thickness of mare basalts in Imbrium Basin},
+ author={Thomson, Bradley J and Grosfils, Eric B and Bussey, D Ben J and Spudis, Paul D},
+ journal={Geophysical Research Letters},
+ volume={36},
+ number={12},
+ year={2009}
+}
+
+%Weider, S.Z., Crawford, I.A., Joy, K.H., 2010. Individual lava flow thicknesses in Oceanus Procellarum and Mare Serenitatis determined from Clementine multispectral data. Icarus, 209:323-336.
+ at article{weider2010individual,
+ title={Individual lava flow thicknesses in Oceanus Procellarum and Mare Serenitatis determined from Clementine multispectral data},
+ author={Weider, Shoshana Z and Crawford, Ian A and Joy, Katherine H},
+ journal={Icarus},
+ volume={209},
+ number={2},
+ pages={323--336},
+ year={2010},
+ publisher={Elsevier}
+}
+
+%Wilcox, B.B., Lucey, P.G., Gillis, J.J., 2005. Mapping iron in the lunar mare: An improved approach. J. Geophys. Res. 110(E11):2156-2202.
+ at article{wilcox2005mapping,
+ title={Mapping iron in the lunar mare: An improved approach},
+ author={Wilcox, BB and Lucey, PG and Gillis, JJ},
+ journal={Journal of Geophysical Research: Planets (1991--2012)},
+ volume={110},
+ number={E11},
+ year={2005},
+ publisher={Wiley Online Library}
+}
+
+ at misc{wilhelms1987geologic,
+ title={The geologic history of the Moon},
+ author={Wilhelms, Don E and McCauley, John F and Trask, Newell Jefferson},
+ year={1987},
+ publisher={US Government Printing Office Washington DC}
+}
+
+ at article{wilshire1972petrology,
+ title={Petrology and stratigraphy of the Fra Mauro Formation at the Apollo 14 site},
+ author={Wilshire, Howard Gordon and Jackson, Everett Dale},
+ journal={Washington, US Govt. Print. Off., 1972.},
+ volume={1},
+ year={1972}
+}
+
+ at inproceedings{zhang2013mapping,
+ title={Mapping lunar TiO2 and FeO with Chandrayaan-1 M3 Data},
+ author={Zhang, W and Bowles, NE},
+ booktitle={Lunar and Planetary Institute Science Conference Abstracts},
+ volume={44},
+ pages={1212},
+ year={2013}
+}
\ No newline at end of file
Modified: grass-promo/grassposter/2014_EGU_M3_Landscape/poster.tex
===================================================================
--- grass-promo/grassposter/2014_EGU_M3_Landscape/poster.tex 2014-05-14 06:42:47 UTC (rev 60235)
+++ grass-promo/grassposter/2014_EGU_M3_Landscape/poster.tex 2014-05-14 06:43:12 UTC (rev 60236)
@@ -8,6 +8,9 @@
\usepackage{wrapfig}
\usepackage{url}
+% For blibliography styling
+\usepackage{natbib}
+
%Used for better control on code display
\usepackage[margin=\margin cm, paperwidth=197cm, paperheight=100cm]{geometry}
@@ -44,82 +47,81 @@
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\blocknode{Abstract}{
-\small \noindent The geology of the Apollo 12 landing site has been the subject of many studies, including recently by Korotev et al. (2011) and Snape et al. (2013). This research attempts to bring additional understanding from a remote sensing perspective using the Moon Mineralogy Mapper ($M^3$) sensor data, onboard the Chandrayaan lunar orbiter. This has a higher spatial-spectral resolution sensor than the Clementine UV-Vis sensor and provides the opportunity to study the lunar surface with detailed spectral signatures.\newline
+\small \noindent The geology of the Apollo 12 landing site has been the subject of many studies, including recently by \cite{korotev2011apollo} and \cite{Snape2013basaltic}. This research attempts to bring additional understanding from a remote sensing perspective using the Moon Mineralogy Mapper ($M^3$) sensor data, onboard the Chandrayaan lunar orbiter. This has a higher spatial-spectral resolution sensor than the Clementine UV-Vis sensor and provides the opportunity to study the lunar surface with detailed spectral signatures.\newline
-Mapping of FeO (wt\%) and TiO 2 (wt\%) is done using the methods of Lucey et al. (2000) and Wilcox et
-al. (2005). A FeO \& TiO 2 processing module (i.feotio2) is made specifically for this research within the Free \& Open Source Software GRASS GIS (Neteler et al., 2012). Attempts will be made to estimate the lava flow thickness using the method of Bugiolacchi et al. (2006) and individual lava layers thicknesses (Weider et al., 2010). Integration of this new information will be put in perspective and integrated with previous work. Analysis from the combined higher spatial and spectral resolutions will improve the accuracy of the geological mapping at the Apollo 12 landing site.\newline
+Mapping of FeO (wt\%) and TiO 2 (wt\%) is done using the methods of \cite{lucey2000lunar} and \cite{wilcox2005mapping}. A FeO \& TiO 2 processing module (i.feotio2) is made specifically for this research within the Free \& Open Source Software GRASS GIS \cite{neteler2012grass}. Attempts will be made to estimate the lava flow thickness using the method of \cite{bugiolacchi2006stratigraphy} and individual lava layers thicknesses from \cite{weider2010individual}. Integration of this new information will be put in perspective and integrated with previous work. Analysis from the combined higher spatial and spectral resolutions will improve the accuracy of the geological mapping at the Apollo 12 landing site.\newline
}
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
\blocknode{Previous interpretations}{
-Korotev et al. (2011) reviewed the lunar research done until recently, with a special interest in the Apollo 12 landing site and its vicinity. Among the information newly deducted, are a geological context block diagram 1 (Figure below) along with an Apollo 12 landing site interpretive cross-section. Fortezzo and Hare (2013) completed the digital renovation of the 1:5,000,000 lunar geological maps series, enhanced with LOLA-LRO information.\newline
+\cite{korotev2011apollo} reviewed the lunar research done until recently, with a special interest in the Apollo 12 landing site and its vicinity. Among the information newly deducted, are a geological context block diagram 1 (Figure below) along with an Apollo 12 landing site interpretive cross-section. \cite{fortezzo2013completed} completed the digital renovation of the 1:5,000,000 lunar geological maps series, enhanced with LOLA-LRO information.
\begin{center}
\begin{tabular}{cc}
- \includegraphics[width=0.45\textwidth]{./images/Korotev_block}
+ \includegraphics[width=0.45\textwidth]{./images/Korotev_block}\hspace{20mm}
&
\includegraphics[width=0.45\textwidth]{./images/A12region}
\end{tabular}\newline
-Figure 2: a) Korotev et al (2011) geological block of Apollo 12 landing site\\
-b) Fortezzo and Hare (2013) geological maps series with moon nomenclature.
+Figure 1: a) Geological block of Apollo 12 landing site from \cite{korotev2011apollo}.\\
+b) Geological maps series with moon nomenclature from \cite{fortezzo2013completed}.
\end{center}
+
+\begin{center}
+ \begin{tabular}{c}
+ \includegraphics[width=0.75\textwidth]{./images/2013_lpsc_Snape_et_al}
+ \end{tabular}\newline
+Figure 2: Interpretive cross-section of Apollo 12 landing site from \cite{Snape2013basaltic}.
+\end{center}
}
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-\getcurrentrow{box}
-\coordinate (funkcionalita) at (box.south west);
-\coordinate (funkcionalitaeast) at (box.east);
-\coordinate (screenshot) at (box.north west);
+%\getcurrentrow{box}
+%\coordinate (funkcionalita) at (box.south west);
+%\coordinate (funkcionalitaeast) at (box.east);
+%\coordinate (screenshot) at (box.north west);
+%
+%\blocknodew[($(funkcionalita)+(20,-1)$)]{35}{References}{
+\blocknode{References}{
+\smallskip
+\scriptsize
-\blocknodew[($(funkcionalita)+(20,-1)$)]{35}{References}{
-\scriptsize
-\begin{flushleft}
-\begin{tabular}{rp{0.9\textwidth}}
-Bugiolacchi et al. (2006) & Planetary Science. 41(2):285-304.\\{}
-Fortezzo et al. (2013) & LPI Contributions, 1719:2114.\\{}
-Korotev et al. (2011) & Geochimica et Cosmochimica Acta. 75(6):1540-1573.\\{}
-Lucey et al. (2000) & J. Geophys. Res. 105(E8): 20297-20305.\\{}
-Neteler et al. (2012) & Environment \& Modeling Software, 31:124-130.\\{}
-Snape et al. (2013) & LPSC Abstracts 44:1044.\\{}
-Weider et al. (2010) & Icarus, 209, 323-336.\\{}
-Wilcox et al. (2005) & J. Geophys. Res. 110(E11):2156-2202.\\{}
-Zhang et al. (2013) & LPSC Abstracts 44:374.\\{}
-\end{tabular}
-\end{flushleft}
-\smallskip
+\begingroup
+\renewcommand{\section}[2]{}%
+\bibliographystyle{plain}
+\bibliography{poster}
+\endgroup
+
\hrulefill
\vspace{-5pt}
\begin{center}
-\begin{tabular}{cp{0.9\textwidth}}
-\begin{minipage}{0.15\textwidth}
+\begin{tabular}{c}
+\hspace{5mm}
+\begin{minipage}{0.2\textwidth}
\includegraphics[width=0.7in]{./images/grass_qr.pdf}
\end{minipage}
-\begin{minipage}{0.3\textwidth}
+\begin{minipage}{0.25\textwidth}
\small {\url{www.bbk.ac.uk}}
\end{minipage}
\begin{minipage}{0.15\textwidth}
-\includegraphics[width=0.7in]{./images/grass_qr.pdf}
+\includegraphics[width=0.7in]{./svg_images/public_domain_logo.pdf}
\end{minipage}
\begin{minipage}{0.3\textwidth}
\small {\url{grass.osgeo.org}}
\end{minipage}
+
+\begin{minipage}{0.2\textwidth}
+\includegraphics[width=0.7in]{./images/grass_qr.pdf}
+\end{minipage}
+
\end{tabular}
\end{center}
\hrulefill
-\vspace{14pt}
-\begin{center}
-\newcommand{\logowidth}{5em}
-\newcommand{\logospace}{\hspace{0.1em}}
-\noindent
-\includegraphics[width=\logowidth]{./svg_images/public_domain_logo.pdf}
-%\raisebox{0.7\height}{\logospace 2013 GRASS Development Team}
-\end{center}
}
\startsecondcolumn
@@ -130,85 +132,116 @@
\begin{center}
\includegraphics[width=0.75\textwidth]{./images/Clementine}
\newline
- Figure 2: Clementine RGB153 (top), segmentation (middle) and FeO (wt\%) per segmentation class (bottom).
+ Figure 3: Clementine RGB153 (top), segmentation (middle) and FeO (wt\%) per segmentation class (bottom).
\end{center}
}
\startthirdcolumn
-%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
-\blocknode{M$^3$ Signal at Apollo 12 landing site}{
-\smallskip
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\blocknode{M$^3$ derived FeO from standard equations}{
+\bigskip
+
\begin{center}
\begin{tabular}{ c p{0.45\textwidth}}
- \raisebox{-1.2\totalheight}{\includegraphics[width=0.5\textwidth]{./images/M3_A12_craters_signal}}\newline
- %\caption{Spectral signature of $M^3$ from four craters}
- \label{fig:specsignature4craters}
+ \raisebox{-1.1\totalheight}{\includegraphics[width=0.5\textwidth]{./code/code1}}
+ %\caption{Testing FeO algorithms.}
+ \label{fig:FeOtesting}
&
- \noindent Chandrayaan $M^3$ data was downloaded from PDS \url{http://pds-imaging.jpl.nasa.gov/}{pds-imaging.jpl.nasa.gov}. The tile \textit{M3G20090111T013904\_V01\_RFL.IMG} was imported in GRASS GIS, resulting in 85 bands. The spectrum for four craters where extracted in the Figure \ref{fig:specsignature4craters}. Bench and Surveyor are both together in the lower reflectance curves. On the higher side, Sharp and Middle Crescent are consistently above the two others. This higher broadband Albedo is increasing towards the West, where one of the ray is clearly drawn (Oblique white strip in the middle of The Clementine upper map. Compared to the spectral data from Figure ~\ref{fig:specsignatureASTERlib} the reflectance is overall lower and the obvious shape differences are there.
- \end{tabular}
- \end{center}
- \begin{flushleft}
- \hspace{22mm}
- \includegraphics[width=0.45\textwidth]{./images/Apollo12_signatures}
- %\caption{Spectral signature from Apollo 12 (ASTER library)}
- \label{fig:specsignatureASTERlib}
- \end{flushleft}
-
-}
-\blocknode{M$^3$ derived FeO from Wilcox et al. (2005)}{
-\smallskip
+\noindent The wt\%FeO equations have a large range of results when used with $M^3$ data:\newline
\begin{center}
-\includegraphics[width=0.5\textwidth]{./images/M3_FeO_Wilcox_theta_degree}
-\end{center}
-}
-
-\startfourthcolumn
-%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
-\blocknode{M$^3$ derived FeO from standard equations}{
-\noindent The wt\%FeO equations have a large range of results when used with $M^3$ data:
-\begin{center}
\begin{tabular}{ l r r}
\hline
Authors & Bench & Surveyor\\
\hline
-Lucey et al. (2000) & -26.64 & -23.32 \\
-Lawrence et al. (2002) & 4.72 & 6.38 \\
-Wilcox et al. (2005) & 22.28 & 21.82 \\
-Zhang et al. (2013) & 19.74 & 19.49 \\
+\cite{lucey2000lunar} & -26.64 & -23.32 \\
+\cite{lawrence2002iron} & 4.72 & 6.38 \\
+\cite{wilcox2005mapping} & 22.28 & 21.82 \\
+\cite{zhang2013mapping} & 19.74 & 19.49 \\
\hline
\end{tabular}
\end{center}
\bigskip
-
-\begin{center}
-\begin{tabular}{ c p{0.45\textwidth}}
- \raisebox{-0.8\totalheight}{\includegraphics[width=0.5\textwidth]{./code/code1}}
- %\caption{Testing FeO algorithms.}
- \label{fig:FeOtesting}
- &
- \noindent It is known that the local range of FeO is below 10wt\% from UVVIS data (see Figure on the lower left), only the Lawrence et al. (2002) equation is giving an appropriate range. Lucey et al. (2000) equation fails because of the offset of uvvis4/uvvis2(=1.15 vs offset = 1.19) and the one for uvvis2(=0.05 vs offset = 0.08), as both of the parts are negative thus giving a positive division output, their interplay should bring a negative number for the arctangent negative sign to compensate. This clearly does not happen with $M^3$ data in the Bench and Surveyor craters, the results from the arctangent being positive, and the sign change brings the main part of the equation to a negative, further reduced by the negative final offset.\newline
+ \noindent It is known that the local range of FeO is below 10wt\% from UVVIS data (see Figure on the lower left), only the \cite{lawrence2002iron} equation is giving an appropriate range. \cite{lucey2000lunar} equation fails because of the offset of uvvis4/uvvis2(=1.15 vs offset = 1.19) and the one for uvvis2(=0.05 vs offset = 0.08), as both of the parts are negative thus giving a positive division output, their interplay should bring a negative number for the arctangent negative sign to compensate. This clearly does not happen with $M^3$ data in the Bench and Surveyor craters, the results from the arctangent being positive, and the sign change brings the main part of the equation to a negative, further reduced by the negative final offset.\newline
\end{tabular}
\end{center}
-\noindent Upon using the Lawrence et al. (2002) equation, it turned out that though the wt\%FeO range was satisfactory for few crater points, the rate of change was actually reverse to the expected one, reducing to null towards the South of the landing site and increasing towards the North.\newline
-\noindent The equation from Zhang et al. (2013) is giving an appropriate rate of change, however, the local values are too large compared to the Clementine derived FeO values. Comparing the zonal contrast between Clementine FeO map from Lucey et al. (2000) the $M^3$ from Zhang et al. (2013) leads to an interesting prospect as even the shapes are not consistent (see Figures ~\ref{fig:subfeoclem} \& ~\ref{fig:subfeoM3}). This indicates that the inner work of the angle equation is not sensitive to the same type of distance between R950 and R750 as they are in Clementine and in $M^3$. In an ideal condition, the calibration of both sensor bands would be identical, and the sensor response for each band would also be the same. This is not a reality, from the design and manufacture inheritance of multi-spectral sensors and hyperspectral sensors, to the data collection flight and its environment. Finally, some accident or issues can damage the operation.\newline
+\noindent Upon using the equation from \cite{lawrence2002iron}, it turned out that though the wt\%FeO range was satisfactory for few crater points, the rate of change was actually reverse to the expected one, reducing to null towards the South of the landing site and increasing towards the North.\newline
+\noindent The equation from \cite{zhang2013mapping} is giving an appropriate rate of change, however, the local values are too large compared to the Clementine derived FeO values. Comparing the zonal contrast between Clementine FeO map from \cite{lucey2000lunar} the $M^3$ from \cite{zhang2013mapping} leads to an interesting prospect as even the shapes are not consistent (see Figures ~\ref{fig:subfeoclem} \& ~\ref{fig:subfeoM3}). This indicates that the inner work of the angle equation is not sensitive to the same type of distance between R950 and R750 as they are in Clementine and in $M^3$. In an ideal condition, the calibration of both sensor bands would be identical, and the sensor response for each band would also be the same. This is not a reality, from the design and manufacture inheritance of multi-spectral sensors and hyperspectral sensors, to the data collection flight and its environment. Finally, some accident or issues can damage the operation.\newline
+\noindent After Contacting W. Zhang of \cite{zhang2013mapping} about the issue in its algorithm, he promptly answered that the article had a typo in the equation. After correction, the output were in a better range (about 15 for the two craters in the table above).\newline
\begin{center}
- \includegraphics[width=0.4\textwidth,keepaspectratio=true]{./images/Clem_FeO_area}
+\begin{tabular}{ c c }
+ \raisebox{0.0\totalheight}{
+ \begin{tabular}{ p{0.45\textwidth} }
+ \includegraphics[width=0.45\textwidth,keepaspectratio=true]{./images/Clem_FeO_area}
% \caption{Subset of Clementine FeO using \citep{lucey2000lunar}}
\label{fig:subfeoclem}
-\hspace{5mm}
- \includegraphics[width=0.435\textwidth,keepaspectratio=true]{./images/M3_Zhang_FeO_area}
+ Figure 4: Subset of Clementine FeO using \cite{lucey2000lunar}.
+ \newline\linebreak
+\vspace{10mm}\\
+ \includegraphics[width=0.45\textwidth,keepaspectratio=true]{./images/M3_Zhang_FeO_area}
% \caption{Subset of $M^3$ FeO using \cite{zhang2013mapping}}
\label{fig:subfeoM3}
+ Figure 5: Subset of $M^3$ FeO using \cite{zhang2013mapping}.
+ \newline
+ \end{tabular}
+ }
+ &
+ \begin{tabular}{ p{0.45\textwidth} }
+ \includegraphics[width=0.45\textwidth,keepaspectratio=true]{./images/M3_Zhang_FeO_region}
+% \caption{Region of $M^3$ FeO using \cite{zhang2013mapping} corrected}
+ \label{fig:subfeoM3corr}
+ Figure 6: Region of $M^3$ FeO using \cite{zhang2013mapping} corrected.
+ \end{tabular}
+\end{tabular}
\end{center}
+
+
+
+
}
+\startfourthcolumn
+%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
+\blocknode{M$^3$ Signal at Apollo 12 landing site}{
+\smallskip
+\begin{center}
+\begin{tabular}{ c p{0.45\textwidth} }
+ \raisebox{-0.40\totalheight}{
+ \begin{tabular}{ c }
+ \includegraphics[width=0.5\textwidth]{./images/M3_A12_craters_signal}
+ \label{fig:specsignature4craters}\\
+ \vspace{5mm}
+ \includegraphics[width=0.5\textwidth]{./images/A12_spectrum}
+ \label{fig:specsignaturespeclibv2}\\
+ \vspace{5mm}
+ \includegraphics[width=0.5\textwidth]{./images/Apollo12_signatures}
+ \label{fig:specsignatureASTERlib}
+ \end{tabular}
+ }%End of tabular
+ &
+ \noindent Chandrayaan $M^3$ data was downloaded from PDS \url{http://pds-imaging.jpl.nasa.gov/}{pds-imaging.jpl.nasa.gov}. The tile \textit{M3G20090111T013904\_V01\_RFL.IMG} was imported in GRASS GIS, resulting in 85 bands. The spectrum for four craters where extracted in the Figure \ref{fig:specsignature4craters}. Bench and Surveyor are both together in the lower reflectance curves. On the higher side, Sharp and Middle Crescent are consistently above the two others. This higher broadband Albedo is increasing towards the West, where one of the ray is clearly drawn (Oblique white strip in the middle of The Clementine upper map. Compared to the spectral data from Figure ~\ref{fig:specsignatureASTERlib} the reflectance is overall lower and the obvious shape differences are there. Additional spectrum signature data from \cite{clark2007usgs} is in the process of being extracted for analysis.\newline\linebreak
+ \noindent Figure 8: \newline Spectral signature of $M^3$ from four craters.
+ \newline\linebreak
+ \noindent Figure 9: \newline Spectral signature from Apollo 12 (Speclib v2.0).
+ \newline\linebreak
+ \noindent Figure 10: \newline Spectral signature from Apollo 12 from \cite{Baldridge2009711}.
+ \newline\linebreak
+\end{tabular}
+\end{center}
+}%End of Block
+
+
+\blocknode{Conclusions}{
+\smallskip
+Conclusions
+}
+
\end{tikzpicture}
\end{document}
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