Bio-Optical Characterization of Amazon Floodplain Lakes and Evaluation of the Retrieval of Optically Active Constituent Using Remote Sensing

Total Page:16

File Type:pdf, Size:1020Kb

Bio-Optical Characterization of Amazon Floodplain Lakes and Evaluation of the Retrieval of Optically Active Constituent Using Remote Sensing sid.inpe.br/mtc-m21b/2016/06.08.16.27-TDI BIO-OPTICAL CHARACTERIZATION OF AMAZON FLOODPLAIN LAKES AND EVALUATION OF THE RETRIEVAL OF OPTICALLY ACTIVE CONSTITUENT USING REMOTE SENSING Lino Augusto Sander de Carvalho Doctorate Thesis Course Graduate in Remote Sensing, guided by Drs. Cláudio Clemente Faria Barbosa and Evlyn Márcia Leão de Moraes Novo, approved in April 18, 2016. URL of the original document: <http://urlib.net/ 8JMKD3MGP3W34P/3LRECPB> INPE São José dos Campos 2016 PUBLISHED BY: Instituto Nacional de Pesquisas Espaciais - INPE Gabinete do Diretor (GB) Serviço de Informação e Documentação (SID) Caixa Postal 515 - CEP 12.245-970 São José dos Campos - SP - Brasil Tel.:(012) 3208-6923/6921 Fax: (012) 3208-6919 E-mail: [email protected] COMMISSION OF BOARD OF PUBLISHING AND PRESERVATION OF INPE INTELLECTUAL PRODUCTION (DE/DIR-544): Chairperson: Maria do Carmo de Andrade Nono - Conselho de Pós-Graduação (CPG) Members: Dr. Plínio Carlos Alvalá - Centro de Ciência do Sistema Terrestre (CST) Dr. André de Castro Milone - Coordenação de Ciências Espaciais e Atmosféricas (CEA) Dra. Carina de Barros Melo - Coordenação de Laboratórios Associados (CTE) Dr. Evandro Marconi Rocco - Coordenação de Engenharia e Tecnologia Espacial (ETE) Dr. Hermann Johann Heinrich Kux - Coordenação de Observação da Terra (OBT) Dr. Marley Cavalcante de Lima Moscati - Centro de Previsão de Tempo e Estudos Climáticos (CPT) Silvia Castro Marcelino - Serviço de Informação e Documentação (SID) DIGITAL LIBRARY: Dr. Gerald Jean Francis Banon Clayton Martins Pereira - Serviço de Informação e Documentação (SID) DOCUMENT REVIEW: Simone Angélica Del Ducca Barbedo - Serviço de Informação e Documentação (SID) Yolanda Ribeiro da Silva Souza - Serviço de Informação e Documentação (SID) ELECTRONIC EDITING: Marcelo de Castro Pazos - Serviço de Informação e Documentação (SID) André Luis Dias Fernandes - Serviço de Informação e Documentação (SID) sid.inpe.br/mtc-m21b/2016/06.08.16.27-TDI BIO-OPTICAL CHARACTERIZATION OF AMAZON FLOODPLAIN LAKES AND EVALUATION OF THE RETRIEVAL OF OPTICALLY ACTIVE CONSTITUENT USING REMOTE SENSING Lino Augusto Sander de Carvalho Doctorate Thesis Course Graduate in Remote Sensing, guided by Drs. Cláudio Clemente Faria Barbosa and Evlyn Márcia Leão de Moraes Novo, approved in April 18, 2016. URL of the original document: <http://urlib.net/ 8JMKD3MGP3W34P/3LRECPB> INPE São José dos Campos 2016 Cataloging in Publication Data Carvalho, Lino Augusto Sander de. C253b Bio-optical characterization of Amazon floodplain lakes and evaluation of the retrieval of optically active constituent using remote sensing / Lino Augusto Sander de Carvalho. – São José dos Campos : INPE, 2016. xxvi + 175 p. ; (sid.inpe.br/mtc-m21b/2016/06.08.16.27-TDI) Thesis (Doctorate in Remote Sensing) – Instituto Nacional de Pesquisas Espaciais, São José dos Campos, 2016. Guiding : Drs. Cláudio Clemente Faria Barbosa and Evlyn Márcia Leão de Moraes Novo. 1. Amazon floodplain lakes. 2. Hydrological optics. 3. Lakes Biooptical Properties. 4. Semi-Analytical modeling. I.Title. CDU 528.8:551.435.12(811) Esta obra foi licenciada sob uma Licença Creative Commons Atribuição-NãoComercial 3.0 Não Adaptada. This work is licensed under a Creative Commons Attribution-NonCommercial 3.0 Unported License. ii Título: “ BIO-OPTICAL CHARACTERIZATION OF AMAZON FLOODPLAIN LAKES AND EVALUATION OF THE RETRIEVAL OF OPTICALLY ACTIVE CONSTITUENT USING REMOTE SENSING”. ACKNOWLEDGEMENTS Aos Orientadores Cláudio Clemente Faria Barbosa e Evlyn Márcia Leão de Moraes Novo pela valiosa orientação, suporte, crédito depositado em mim e pela oportu- nidade de trabalho em uma área repleta de desafios. Ao Programa de Pós-Graduação no INPE, professores e funcionários, pela oportu- nidade de estudos e utilização de suas instalações. Ao Professor Emmanuel Boss e à Universidade de Maine pelo período de doutorado sanduiche. À Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES) que proveu a bolsa de estudos. Ao Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) através do Programa Ciência sem Fronteiras que me possibilitou o doutorado sanduiche. À FAPESP e ao Programa de Pós-Graduação em Sensoriamento Remoto pelo su- porte financeiro aos trabalhos de campo para coletas de dados. À NASA, pelo suporte financeiro e à Curtis Mobley e Emmanuel Boss pela indicação para a participação no curso Calibration and Validation for Ocean Color Remote Sensing nos anos de 2013 e 2015. À todos os meus amigos pelos bons momentos vividos. À meus pais, por todo o carinho e suporte. À minha esposa, pelo carinho e paciência. v ABSTRACT Amazon floodplain lakes play a substantial role in global and regional biogeochemical Amazonian processes. Due to their size, sampling strategies usually applied in limno- logical studies are not suitable and therefore, Remote Sensing (RS) techniques figure as an alternative due to the high temporal and synoptic characteristics. However, the use of RS demands precise lake bio-optical characterization in order to provide reliable estimates of optical active components (OAC).This work focused on the study of Curuai Lake which is a suitable example of a Brazilian Amazon floodplain lake. Curuai lake was sampled in four field campaigns (September/2012, February and August/2013 and April/2014) where Apparent Optical Properties-AOP (Rrs and K-functions), in situ Inherent Optical Properties-IOP (Attenuation, Absorp- tion, Backscattering profiles and Particle Size Distribution (PSD)) as well as labo- ratory analysis (AOC concentration and absorption) were measured. A data qual- ity assessment was performed to test the suitability of commercial instrumentation (ACS and Hydroscat) for turbid environments as well as commonly used AOP/IOP measurement methodologies. The optical characterization compared datasets from each fieldcampaign for surface and profile measurements. Also three semi-analytical inverse models (Nechad Algorithm (NECHAD et al., 2010), Quasi-Analytical Algo- rithm (QAA) (LEE et al., 2002) and Generalized ocean color inversion model (GIOP) (WERDELL et al., 2013)) were tested using measured AOP and IOPs. Data quality assessment show that sun/skyglint effects have the highest impact on above water Ab remote sensing measurements Rrs (Rrs ). Highest errors were found for In-water de- Iw rived AOPs (Rrs and K-functions), but despite the the different tested approaches their differences are commonly in the 10 to 15 % interval. For in situ IOPs, the Hy- drolight IOP/AOP closure experiments resulted in mismatches from 50 % to 100% depending on the field campaign. Among the corrections tested for ACS/Hydroscat errors, the Doxaran (DOXARAN et al., 2013) and Rottgers (RöTTGERS et al., 2013) methods were the most suitable. For Laboratory absorption measurements, differ- ences range from 10% to 80% but were below 15 % for biogeochemical variables concentration measurements. Curuai Lake Bio-optical characterization show that K-functions go from 1 to 12 m−1 in 676 nm depending on the season but can go as high as ≈ 20 m−1 in the blue range. For IOPs, total attenuation, absorption and scattering coefficients were higher for February/2013 (≈ 25, 4 and 21 m−1 re- spectively for 550 nm) and similar for August/2013 and April/2014 (≈ 12, 2.5 and 10 m−1 respectively for 550 nm). Backscattering coefficients also were higher for February/2013 (≈ 0.6 m−1 in 700 nm) and similar for August/2013 and April/2014 −1 b (≈ 0.3 m in 700 nm). However, the backscattering to scattering ratio ( bp/bp) was similar for February/2013, August/2013 and April/2014 (Median of 0.04), indicat- ing low particle type variability. However, differences were found for the exponent ∗ of scattering coefficient (γb) (Median = 1.3 to 1.5) and for specific scattering bp (0.42 to 0.67 m2g−1) showing a possible dominance of smaller inorganic particles for February/2013. Specific absorption coefficients for particulate (ap), non-algal par- ticles (anap) and phytoplankton (aφ) were within literature values but particularly vii −1 high for anap ( up to ≈ 6 m in the blue range). Particle Size Distribution shows a bimodal behavior with most of particles in the 10-15 µm range. Results for In- verse Models were not satisfactory for most of retrieved IOPs and biogeochemical variables (Chla and TSM). Best results for GIOP presented errors of at least 20 % while for QAA errors can reach more than 100 %. The Nechad algorithm shows errors that reaches 30 % for TSM estimates which may be considered reasonable. The main source of errors for semi-analytical inverse models rely on uncertainties of input parameters but further investigation is needed to understand the main source of error in the current dataset as well as help guiding future data acquisition. Keywords: Amazon floodplain lakes. Hydrological Optics. Lakes Biooptical Proper- ties. Semi-Analytical modeling. viii CARACTERIZAÇÃO BIO-OPTICA DE LAGOS DA PLANÍCIE INUNDÁVEL AMAZÔNICA E AVALIAÇÃO DA RECUPERAÇÃO DE CONSTITUINTES OPTICAMENTE ATIVOS UTILIZANDO SENSORIAMENTO REMOTO RESUMO Lagos de várzea amazônico desempenha um papel importante nos processos biogeo- químicos globais e regionais da Amazonia. Devido ao seu tamanho, estratégias de amostragem normalmente aplicados em estudos limnológicos não são adequadas e, portanto, técnicas de sensoriamento remoto (SR) se apresentam como uma alterna- tiva devido às sua alta resolução temporal e visão sinóptica. No entanto, o uso de SR exige uma caracterização bio-óptica precisa, a fim de fornecer estimativas confiáveis de componentes ativos ópticos (COA). Este trabalho teve como
Recommended publications
  • Martian Crater Morphology
    ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter.
    [Show full text]
  • Financial Supporters
    FINANCIAL SUPPORTERS Care and Share Food Bank for Southern Colorado 2011-12 Financial Supporters 100% Chiropractic Lanny and Paul Adams Mr. and Mrs. Jeffrey Ahrendsen 14K Real Estate Investments LLC Ms. Laura Adams Mr. Kevin Ahrens 1882 Management Mr. and Mrs. Lon Adams Mr. and Mrs. Charles Aiken 1st Cavalry Rocky Mountain Chapter Col and Mrs. Louis Adams Ms. Laverne Ainley 221 South Oak Bistro Ms. Maggie Adams Air Academy Federal Credit Union 4-Bits 4-H Club Ms. Mary Adams Air Academy Federal Credit Union 4Clicks - Solutions, LLC Mr. Michael Adams Air Academy High School - District 20 A & L Aluminum Manufacturing Company Mr. and Mrs. Rexford Adams Mr. TJ Airhart A Handymike Home Repair Mr. and Mrs. Robert Adams Aka Wilson, LLC A to Z Realty Mr. S. Michael Adams Mr. Richard Alaniz AA “Accurate and Affordable” Striping, Inc. Mr. and Mrs. Samuel Adams Ms. Susan Alarid AAA NCNU Insurance Exchange Mr. Steve Adams Ms. Karin Alaska AAA Northern California Nevada & Utah Suzanne Adams Mr. Arturo Albanesi AARP Foundation Adams Bank & Trust Mr. and Mrs. Mac Alberico Ms. Renee Abbe Mrs. Alda Adcox Ms. Cheryl Alberto Ms. Marjory Abbott Add Staff Inc. Mr. and Mrs. Dewey Albertson Jr. Mr. and Mrs. Peyton Abbott Ms. Constance Addington Mr. W. Gary Albertson Ms. Stephanie Abbott Mr. and Mrs. D. V. Addington Albertsons LLC Ms. Brianna Abby Ms. Linda Addington Mr. and Mrs. Albert Albrandt Mr. and Mrs. Donald Abdallah Ms. Vicky Addison Mr. Gerald Albrecht Mr. Tony Abdella Ms. Deirdre Aden-Smith Ms. Patricia Albright Mr. and Mrs. William Abel Mr.
    [Show full text]
  • POLYGONAL IMPACT CRATERS on CHARON. C.B. Beddingfield1,2, R
    51st Lunar and Planetary Science Conference (2020) 1241.pdf POLYGONAL IMPACT CRATERS ON CHARON. C.B. Beddingfield1,2, R. Beyer1,2, R.J. Cartwright1,2, K. Singer3, S. Robbins3, S.A. Stern3, V. Bray4, J.M. Moore2, K. Ennico2, C.B. Olkin3, J.R. Spencer3, H.A. Weaver5, L.A. Young3, A.Verbiscer6, J. Parker3, and the New Horizons Geology, Geophysics, and Imaging (GGI) Team; 1SETI In- stitute, Mountain View, CA, 2NASA Ames Research Center, Mountain View, CA ([email protected]), 3Southwest Research Institute, Boulder, CO, 4University of Arizona, Tucson, AZ, 5John Hopkins University Applied Physics Laboratory, Laurel, MD, 6University of Virginia, Charlottesville, VA. Introduction: Polygonal impact craters (PICs) re- flect pre-existing extensional and strike-slip faults and fractures in the target material [e.g. 1-9]. PIC straight rim segments therefore can provide important infor- mation for deciphering the tectonic histories of plane- tary bodies [e.g. 8]. The only known PIC formation mechanism is the presence of pre-existing sub-vertical structures within the target material [e.g. 5, 7, 11-13]. In contrast, circular impact craters (CICs) are in- ferred to result from impact events in non-tectonized target material. CICs can also form in pre-fractured tar- get material if the fractures are widely or closely spaced, if the fracture system is highly complex, or if the target material is covered by a thick layer of non-cohesive sed- iment that limits interactions between the impactor and the underlying bedrock/ice [e.g. 14]. Consequently, PICs and CICs are useful tools to distinguish between Fig.
    [Show full text]
  • Secondary Craters on Europa and Implications for Cratered Surfaces
    Vol 437|20 October 2005|doi:10.1038/nature04069 LETTERS Secondary craters on Europa and implications for cratered surfaces Edward B. Bierhaus1, Clark R. Chapman2 & William J. Merline2 For several decades, most planetary researchers have regarded the craters were typically not spatially random, but instead appeared in impact crater populations on solid-surfaced planets and smaller clumps and clusters16 even at distances far (several hundred kilo- bodies as predominantly reflecting the direct (‘primary’) impacts metres) from the nearest large primary crater. This clustered spatial of asteroids and comets1. Estimates of the relative and absolute distribution contrasts with primary impacts, which are spatially ages of geological units on these objects have been based on this random. The low spatial density and unusual non-random spatial assumption2. Here we present an analysis of the comparatively distribution of Europa’s small craters enabled us to achieve what has sparse crater population on Jupiter’s icy moon Europa and suggest been previously difficult, namely unambiguous identification and that this assumption is incorrect for small craters. We find that quantification of the contribution of distant secondary craters to the ‘secondaries’ (craters formed by material ejected from large total crater SFD. This, in turn, allows us to re-examine the overall primary impact craters) comprise about 95 per cent of the small crater age-dating methodology. We discuss the specifics of the craters (diameters less than 1 km) on Europa. We therefore con- Europa data first. clude that large primary impacts into a solid surface (for example, We measured more than 17,000 craters in 87 low-compression, ice or rock) produce far more secondaries than previously low-sun, high-resolution Europa images (scales ,60 m pixel21), believed, implying that the small crater populations on the which cover nine regions totalling 0.2% of Europa’s surface (a much Moon, Mars and other large bodies must be dominated by larger percentage of Europa has been imaged at lower resolutions), secondaries.
    [Show full text]
  • Fungal Endophthalmitis
    ............................ Mycosis of the Eye and Its Adnexa .. ............................ Developments in Ophthalmology Vol. 32 Series Editor W. Behrens-Baumann, Magdeburg ............................ Mycosis of the Eye and Its Adnexa W. Behrens-Baumann, Magdeburg with a contribution by R. RuÈchel,GoÈttingen 39 ®gures, 31 in color, and 39 tables, 1999 ............................ Prof. Dr. med. W. Behrens-Baumann Klinik fuÈr Augenheilkunde, Otto-von-Guericke-UniversitaÈt Leipziger Strasse 44, D±39120 Magdeburg This is a revised and extended translation of a former German version entitled Pilzerkrankungen des Auges by Wolfgang Behrens-Baumann The reproduction of the color illustrations in this book was made possible by a generous contribution from the Heinz Karger Memorial Foundation Continuation of `Bibliotheca Ophthalmologica', `Advances in Ophthalmology', and `Modern Problems in Ophthalmology' Founded 1926 as `Abhandlungen aus der Augenheilkunde und ihren Grenzgebieten' by C. Behr, Hamburg and J. Meller, Wien Former Editors: A. BruÈckner, Basel (1938±1959); H. J. M. Wewe, Utrecht (1938±1962); H. M. Dekking, Groningen (1954±1966); E. R. StreiV, Lausanne (1954±1979); J. FrancËois, Gand (1959±1979); J. van Doesschate, Utrecht (1967±1971); M. J. Roper-Hall, Birmingham (1966±1980); H. Sautter, Hamburg (1966±1980); W. Straub, Marburg a. d. Lahn (1981±1993) Library of Congress Cataloging-in-Publication Data Behrens-Baumann, Wolfgang. [Pilzerkrankungen des Auges, English] Mycosis of the eye and its adnexa / W. Behrens-Baumann; with a contribution by R. Ruchel. (Developments in ophthalmology; vol. 32) Includes bibliographical references and indexes. 1. Oculomycoses. I. Ruchel, R. II. Title. III. Series. [DNLM: 1. Eye Infections, Fungal ± drug therapy. 2. Eye Infections, Fungal ± diagnosis. W1 DE998NG v.32 1999] RE901.F8B4413 1999 617.7 ± dc21 ISSN 0250±3751 ISBN 3±8055±6915±7 (hardcover : alk.
    [Show full text]
  • The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra
    THE COMPOSITION OF THE LUNAR CRUST: RADIATIVE TRANSFER MODELING AND ANALYSIS OF LUNAR VISIBLE AND NEAR-INFRARED SPECTRA A DISSERTATION SUBMITTED TO THE GRADUATE DIVISION OF THE UNIVERSITY OF HAWAI‘I IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY IN GEOLOGY AND GEOPHYSICS DECEMBER 2009 By Joshua T.S. Cahill Dissertation Committee: Paul G. Lucey, Chairperson G. Jeffrey Taylor Patricia Fryer Jeffrey J. Gillis-Davis Trevor Sorensen Student: Joshua T.S. Cahill Student ID#: 1565-1460 Field: Geology and Geophysics Graduation date: December 2009 Title: The Composition of the Lunar Crust: Radiative Transfer Modeling and Analysis of Lunar Visible and Near-Infrared Spectra We certify that we have read this dissertation and that, in our opinion, it is satisfactory in scope and quality as a dissertation for the degree of Doctor of Philosophy in Geology and Geophysics. Dissertation Committee: Names Signatures Paul G. Lucey, Chairperson ____________________________ G. Jeffrey Taylor ____________________________ Jeffrey J. Gillis-Davis ____________________________ Patricia Fryer ____________________________ Trevor Sorensen ____________________________ ACKNOWLEDGEMENTS I must first express my love and appreciation to my family. Thank you to my wife Karen for providing love, support, and perspective. And to our little girl Maggie who only recently became part of our family and has already provided priceless memories in the form of beautiful smiles, belly laughs, and little bear hugs. The two of you provided me with the most meaningful reasons to push towards the "finish line". I would also like to thank my immediate and extended family. Many of them do not fully understand much about what I do, but support the endeavor acknowledging that if it is something I’m willing to put this much effort into, it must be worthwhile.
    [Show full text]
  • Workshop on Geology of the Apollo 17 Landing Site
    NASA-CR-191637 \ WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE (NASA-CR-191637) WORKSHOP ON N93-18786 GEOLOGY OF THE APOLLO 17 LANDING --THRU-- SITE (Lunar Science Inst.) 70 p N93-18817 Unclas G3/91 0141290 __ LPI Technical Report Number 92-09, Part 1 LUNAR AND PLANETARY INSTITUTE 3600 BAY AREA BOULEVARD HOUSTON TX 77058-1113 LPI/TR--92-09, Part 1 WORKSHOP ON GEOLOGY OF THE APOLLO 17 LANDING SITE Edited by G. Ryder, H. H. Schmitt, and P. D. Spudis Held at Houston, Texas December 2-4, 1992 Sponsored by Lunar and Planetary Sample Team Lunar and Planetary Institute Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 LPI Technical Report Number 92-09, Part 1 LPI/TR--92-09, Part 1 Compiledin 1992by LUNAR AND PLANETARY INSTITUTE TheInstituteis operatedby theUniversitySpaceResearchAssociationunderContractNo. NASW- 4574with theNationalAeronauticsandSpaceAdministration. Materialin this volume may be copied without restraint for library, abstract service, education, or per- sonal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. This report may be cited as Ryder G., Schmitt H. H., and Spudis P. D., eds. (1992) Workshop on Geology of the Apollo 17 Landing Site. LPI Tech. Rpt. 92-09, Part 1, Lunar and Planetary Institute, Houston. 63 pp. This report is distributed by ORDER DEPARTMENT Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Mail order requestors will be invoiced for the cost of shipping and handling. Cover: Station 4 at Taurus-LiUrow, Apollo 17 landing site.
    [Show full text]
  • South Pole-Aitken Basin
    Feasibility Assessment of All Science Concepts within South Pole-Aitken Basin INTRODUCTION While most of the NRC 2007 Science Concepts can be investigated across the Moon, this chapter will focus on specifically how they can be addressed in the South Pole-Aitken Basin (SPA). SPA is potentially the largest impact crater in the Solar System (Stuart-Alexander, 1978), and covers most of the central southern farside (see Fig. 8.1). SPA is both topographically and compositionally distinct from the rest of the Moon, as well as potentially being the oldest identifiable structure on the surface (e.g., Jolliff et al., 2003). Determining the age of SPA was explicitly cited by the National Research Council (2007) as their second priority out of 35 goals. A major finding of our study is that nearly all science goals can be addressed within SPA. As the lunar south pole has many engineering advantages over other locations (e.g., areas with enhanced illumination and little temperature variation, hydrogen deposits), it has been proposed as a site for a future human lunar outpost. If this were to be the case, SPA would be the closest major geologic feature, and thus the primary target for long-distance traverses from the outpost. Clark et al. (2008) described four long traverses from the center of SPA going to Olivine Hill (Pieters et al., 2001), Oppenheimer Basin, Mare Ingenii, and Schrödinger Basin, with a stop at the South Pole. This chapter will identify other potential sites for future exploration across SPA, highlighting sites with both great scientific potential and proximity to the lunar South Pole.
    [Show full text]
  • The Recognition of Terrestrial Impact Structures
    Bulletin of the Czech Geological Survey, Vol. 77, No. 4, 253–263, 2002 © Czech Geological Survey, ISSN 1210-3527 The recognition of terrestrial impact structures ANN M. THERRIAULT – RICHARD A. F. GRIEVE – MARK PILKINGTON Natural Resources Canada, Booth Street, Ottawa, Ontario, KIA 0ES Canada; e-mail: [email protected] Abstract. The Earth is the most endogenically active of the terrestrial planets and, thus, has retained the poorest sample of impacts that have occurred throughout geological time. The current known sample consists of approximately 160 impact structures or crater fields. Approximately 30% of known impact structures are buried and were initially detected as geophysical anomalies and subsequently drilled to provide geologic samples. The recognition of terrestrial impact structures may, or may not, come from the discovery of an anomalous quasi-circular topographic, geologic or geo- physical feature. In the geologically active terrestrial environment, anomalous quasi-circular features, however, do not automatically equate with an impact origin. Specific samples must be acquired and the occurrence of shock metamorphism, or, in the case of small craters, meteoritic fragments, must be demonstrated before an impact origin can be confirmed. Shock metamorphism is defined by a progressive destruction of the original rock and mineral structure with increasing shock pressure. Peak shock pressures and temperatures produced by an impact event may reach several hundreds of gigaPascals and several thousand degrees Kelvin, which are far outside the range of endogenic metamorphism. In addition, the application of shock- wave pressures is both sudden and brief. Shock metamorphic effects result from high strain rates, well above the rates of norma l tectonic processes.
    [Show full text]
  • 1 Fluids Mobilization in Arabia Terra, Mars
    Fluids mobilization in Arabia Terra, Mars: depth of pressurized reservoir from mounds self- similar clustering Riccardo Pozzobon1, Francesco Mazzarini2, Matteo Massironi1, Angelo Pio Rossi3, Monica Pondrelli4, Gabriele Cremonese5, Lucia Marinangeli6 1 Department of Geosciences, Università degli Studi di Padova, Via Gradenigo 6 - 35131, Padova, Italy 2 Istituto Nazionale di Geofisica e Vulcanologia (INGV), Via Della Faggiola, 32 - 56100 Pisa, Italy 3 Department of Physics and Earth Sciences, Jacobs University Bremen, Campus Ring 1 -28759 Bremen, Germany 4 International Research School of Planetary Sciences, Università d'Annunzio, viale Pindaro 42 – 65127, Pescara, Italy 5 INAF, Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5 - 35122, Padova, Italy 6 Laboratorio di Telerilevamento e Planetologia, DISPUTer, Universita' G. d'Annunzio, Via Vestini 31 - 66013 Chieti, Italy Abstract Arabia Terra is a region of Mars where signs of past-water occurrence are recorded in several landforms. Broad and local scale geomorphological, compositional and hydrological analyses point towards pervasive fluid circulation through time. In this work we focus on mound fields located in the interior of three casters larger than 40 km (Firsoff, Kotido and unnamed crater 20 km to the east) and showing strong morphological and textural resemblance to terrestrial mud volcanoes and spring-related features. We infer that these landforms likely testify the presence of a pressurized fluid reservoir at depth and past fluid upwelling. We have performed morphometric analyses to characterize the mound morphologies and consequently retrieve an accurate automated mapping of the mounds within the craters for spatial distribution and fractal clustering analysis. The outcome of the fractal clustering yields information about the possible extent of the percolating fracture network at depth below the craters.
    [Show full text]
  • Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America
    Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America There are approximately 101,135sexual abuse claims filed. Of those claims, the Tort Claimants’ Committee estimates that there are approximately 83,807 unique claims if the amended and superseded and multiple claims filed on account of the same survivor are removed. The summary of sexual abuse claims below uses the set of 83,807 of claim for purposes of claims summary below.1 The Tort Claimants’ Committee has broken down the sexual abuse claims in various categories for the purpose of disclosing where and when the sexual abuse claims arose and the identity of certain of the parties that are implicated in the alleged sexual abuse. Attached hereto as Exhibit 1 is a chart that shows the sexual abuse claims broken down by the year in which they first arose. Please note that there approximately 10,500 claims did not provide a date for when the sexual abuse occurred. As a result, those claims have not been assigned a year in which the abuse first arose. Attached hereto as Exhibit 2 is a chart that shows the claims broken down by the state or jurisdiction in which they arose. Please note there are approximately 7,186 claims that did not provide a location of abuse. Those claims are reflected by YY or ZZ in the codes used to identify the applicable state or jurisdiction. Those claims have not been assigned a state or other jurisdiction. Attached hereto as Exhibit 3 is a chart that shows the claims broken down by the Local Council implicated in the sexual abuse.
    [Show full text]
  • Ages of Large Lunar Impact Craters and Implications for Bombardment During the Moon’S Middle Age ⇑ Michelle R
    Icarus 225 (2013) 325–341 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Ages of large lunar impact craters and implications for bombardment during the Moon’s middle age ⇑ Michelle R. Kirchoff , Clark R. Chapman, Simone Marchi, Kristen M. Curtis, Brian Enke, William F. Bottke Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, United States article info abstract Article history: Standard lunar chronologies, based on combining lunar sample radiometric ages with impact crater den- Received 20 October 2012 sities of inferred associated units, have lately been questioned about the robustness of their interpreta- Revised 28 February 2013 tions of the temporal dependance of the lunar impact flux. In particular, there has been increasing focus Accepted 10 March 2013 on the ‘‘middle age’’ of lunar bombardment, from the end of the Late Heavy Bombardment (3.8 Ga) until Available online 1 April 2013 comparatively recent times (1 Ga). To gain a better understanding of impact flux in this time period, we determined and analyzed the cratering ages of selected terrains on the Moon. We required distinct ter- Keywords: rains with random locations and areas large enough to achieve good statistics for the small, superposed Moon, Surface crater size–frequency distributions to be compiled. Therefore, we selected 40 lunar craters with diameter Cratering Impact processes 90 km and determined the model ages of their floors by measuring the density of superposed craters using the Lunar Reconnaissance Orbiter Wide Angle Camera mosaic. Absolute model ages were computed using the Model Production Function of Marchi et al.
    [Show full text]