And Coastal Management

Total Page:16

File Type:pdf, Size:1020Kb

And Coastal Management ESTUARINE AND COASTAL MANAGEMENT TOOLS OF THE TRADE VOLUME 1 PROCEEDINGS OF TENTH NATIONAL CONFERENCE Published By THE COASTAL SOCIETY Suite 110 5410 Grosvenor Lane Bethesda, MD 20814 PROCEEDINGS OF TENTH NATIONAL CONFERENCE ESTUARINE AND COASTAL MANAGEMENT TOOLS OF THE TRADE NEW ORLEANS, LOUISIANA 12-15 October 1986 VOLUME 1 M. P. Lynch: Proceedings Editor K. L. McDonald: Production Editor THE COASTAL SOCIETY Suite 110 5410 Grosvenor Lane Belhesda, Maryland 20814 Copyright © 1987 The Coastal Society Suite 110 5410 Grosvenor Lane Bethesda, Maryland 20814 Statements made or ideas expressed in these Proceedings are those of the identified authors and are not to be construed as positions or policiesof the agencies or institutions which may employthe authors, of The CoastalSociety, or of the sponsors who provided support for publication of these Proceedings. 1986 CONFERENCE COMMITTEE Virginia Tippie, Conference Chair Maurice P. Lynch, Program Chair Donald W. Davis, Local Arrangements Coordinator Karen L McDonald, Registration Coordinator REGISTRATION/PLANNING ASSISTANTS FIELD TRIP COORDINATORS Johna Robbins Sue Hawes Susan Hiser Diane Holling Claudia Walthall Rod Emmer M. Patricia Barthle Shea Penland Eleanor Bochenek John Suter David Peterson Klaus Meyer-Arendt Diane Hollings Don Davis Glynn Rountree Vernon Behrorst Laurie McGilvray Jim Johnston Mike Huggins PROCEEDINGS COMMITTEE Maurice P. Lynch, Proceedings Editor Karen L. McDonald, Production Editor Susan Hiser, Production Assistant Heidi Leiffer, Production Assistant THE COASTAL SOCIETY OFFICIALS Virginia Tippie, President Maurice P. Lynch, Past President Susan Harvey, Secretary Laurie McGilvray, Treasurer Thomas Bigford, Director Waiter Gray, Director William Queen, Director Sharron Stewart, Director ACKNOWLEDGEMENTS The Coastal Society wishes to express its gratitude to the following organizations who providedsupport for the conference and/or publicationof these Proceedings. U. S. Environmental Protection Agency, Office of Marine and Estuarine Protection National Oceanic and Atmospheric Administration, Estuarine Programs Office and National Marine Pollution Program Office U.S. Fish and Wildlife Service. Office of Biological Services Mississippi/Alabama Sea Grant Consortium Louisiana Sea Grant College Program Texas Sea Grant College Program Louisiana Universities Marine Consortium Chesapeake Research Consortium, tnc. American Shore and Beach Preservation Association New Orleans District, U. S. Army Corps of Engineers Louisana Chapter, American Shore and Beach Preservation Association The Association of State Wetlands Managers, Inc. The efforts of the following persons who presided over conference sessions is greatly appreciated: Virginia Tippie Fran Flannigan William Eichbaum Sharron Stewart James Berger Thomas Bigford Kevin Sullivan Robert E. Stewart James McCtoy Thomas DeMoss David Flemer Jerry Oglesby Babe Schwartz Dave Fierra Charles Ehler Maurice Lynch Trudy Coxe Sarah Taylor H. Lee Butler Donald Pritchard Susan Harvey William Queen Joy Bartholomew James Edmonson Suzanne Hawes Richard Sparks John Day David Chambers Foreward The Coastal Society held its 10th National Meeting in New Orleans, Louisiana 12-15 October, 1986. The theme of the conference "Estuarine and Coastal Management - Tools of the Trade" reflects the maturation of estuarine and coastal management efforts in this country. In the early 1970's, the concept of land and water management in the critical coastal zone for the purpose of conserving coastal resources was in its infancy. Initially we were theorists developing new principles and practices as we went along. Much of our effort was expended delineating the area which we wished to influence through coastal management and defining and describing the resources and processes we needed to affect. We have come a long way since those early days. Our "profession" has matured. We have more confidence in what we wish to accomplish, and we have, through a complex combination of trial and error, careful planning and experimentation, serendipity and just plain luck, developed valuable knowledge and experience in how to manage coastal areas and resources. These proceedings reflect the increasing sophistication in our approaches to management, science and technology, and planning and regulation in the nation's coastal and estuarine areas. We hope that new practitioners of our professions find this compilation useful in guiding their work as they join us in coastal activities. A particularly interesting result of the Conference being held in New Orleans was the thorough discussions of the problems and the management approaches associated with the Mississippi drainage basin and Louisiana's extensive coastal marshes. This extensive review of the host region's problems and solutions expands the coverage of regional issues reflected in previous conference proceedings, reinforcing the desirablility of rotating conference sites to different coastal regions. I wish to thank those individuals that contributed to these Proceedings and to the success of the conference by attendance at the sessions, presentation of papers, and participation in discussions. I wish to acknowledge the effort of Ms. Karen L. McDonald who was instrumental in the successful planning and conduct of the Conference. I also wish to acknowledge the efforts of Ms. Susan Hiser, Ms. Heidi Leiffer, and Mr. Robert McCormack for their assistance in preparing these proceedings for publication. Maurice P. Lynch Proceedings Editor TABLE OF CONTENTS PLENARY SESSIONS ESTUARINE ANDCOASTAL MANAGEMENT - THE ISSUES An ActionAgenda: The Chesapeake Bay Experience GovernorHany Hughes 1 Near Coastal Waists: Towards A New Consensus Rebecca Hanmer 9 ESTUARINE ANDCOASTAL MANAGEMENT - THE FUTURE ManagementPrinciplesfor Estuaries Thomas DeMoss 1? Estuarine CoastalManagement• The Future Outlook JohnF.Studt 29 Estuarineand Coastal Management JackE. Ravan 33 The Fish and Wildlife Service's Role in Estuarineand Coastal Management EdwardT.LaRoe .39 NOAA's Role: Assessment, Research, and Management Virginia Tippie 43 A Plan for the Future ofPuget Sound Kirvil Skinnartand 47 ESTUARINE ANDCOASTAL MANAGEMENT - PROGRAM ACCOUNTABILITY Where's the Bottom Line? William Gordon 53 Program Accountability - HowDoWe Measure Progress? -A Political View Joseph V. Gartlan, Jr. 57 ProgramAccountability- How Do We MeasureProgress? • A Scientific View J. R.Schubel 61 VOLUME 1: PAGES 1 to 392 VOLUME 2: PAGES 39310 798 CONCURRENT SESSIONS STRUCTURING A PROGRAM Chairs: Thomas DeMossandFran Flanigan EPANortheast Estuary Program: Organizational Structure and Early Development of Buzzards Bay, Long Island Sound, andNarragansett Bay Programs WendyLWiltse gl A Comparison of theGovernance of Narragansett andSanFrancisco Bays: The RoleofAdaptiveImplementation Timothy Hennessey and DonaldRobadue,Jr. .73 MODELING FOR MANAGEMENT OBJECTIVES Chairs: Donald Pritchard and H. Lee Butler Practical Tools for Guiding Estuarine NutrientControls Wu-SengLung 89 Patuxent RiverEstuary Research, Modeling andMonitoring Strategy MichaelS. Haire andNauthPanday (Abstract) .97 Development of aCoupledHydrodynamic/Water Quality Model forAssessing Eutroprucan'on andAnoxiawithinChesapeake Bay James J. Fitzpatrick, Alan F. Blumberg, DonaldJ.O'Connor, and Thomas J. Mulligan .99 Circulation Modeling asanAid to Management of theBlueCrab Fisheiy in ChesapeakeBay David F. Johnson, KurtW. Hess,andPeterJ. Pytlowany Ill Model Study ofEutrophication in Virginia's Potomac Embayments CarlF.Cerco,AlbertY. KuoandPaul V. Hyer 119 Statistical ModelsforEnvironmental Monitoring andAssessment ArthurJ. Butt 125 ImpactEvaluationofEngineeringProjects in Coastal/Estuarine Waters S. Bird and A. Swain 133 The Effectsof Hydrodynamic Circulation on Estuarine WaterQuality DonaldJ. O'Connorand Alan F. Blumberg(Abstract) 140 Circulation Modeling and RealTime MeasurementsasTools for Maritime Commerce and EnvironmentalManagement Henry R. Frey (Abstract) 141 Multi-Dimensional Modeling ofEstuarineProcesses J. Letter, W. McAnally, and D. P. Bach (Abstract) 142 Optimal Control of Salinity LevelDueto RiverDischarge intheUpper Chesapeake Bay - A StochasticControl Model Bernard B. Hsieh 143 CHARACTERIZING A SYSTEM Chair: Charles N. Ehler Characterizing theChesapeake Bay EcosystemandLessonsLearned David A. Flemcr,Virginia K. Tippie, Gail B. Mackiernan, Roben B. Biggs,Willa Nehlsen, andKentS. Price 153 ProtocolStandardizationfor PugetSound, Washington John Armstrong andScottBecker 179 Changes in Vegetation intheCameron-Creole Marshes of Louisiana Overa Thirty-two Year Period Billy R. CraftandE. RaySmith 187 Evaluating the Potential EconomicBenefitsofEstuarine WaterQuality Improvements: A Cross-Estuary Comparison Kenneth AdlerandWilliamDesvousges 205 Strategic Assessmentof theUseandHealth of the Nation's Estuaries DanielJ. Basta(Abstract) 216 PLUGGING THE PIPE Chair David Fiena Perspectiveson Combined Sewer Overflow Management Eva J. Hoffman .219 Management Strategies forStrengthening Point Source Controls MichelleA. Hiller(Abstract) 224 The Regulation of Point Source Dischanjesin theCoastal ZoneUnderthe NationalPollutantDischarge EliminationSystem (NPDES) Gary Petrazzuolo (Abstract) 225 Virginia's Innovative Financing Mechanism to MeetlisWaterQualityNeeds SusanGillDull 227 THE MISSISSIPPI RIVER DRAINAGE AS AN INTEGRATED SYSTEM Convenors: Richard Sparks and John W. Day, Jr. Human Impacts of Mississippi River Ecology Calvin R. Fremling 235 HabilatDiversityand Utilizationby Invertebrates and Fish Along the Mississippi River
Recommended publications
  • Grosvenor Prints CATALOGUE for the ABA FAIR 2008
    Grosvenor Prints 19 Shelton Street Covent Garden London WC2H 9JN Tel: 020 7836 1979 Fax: 020 7379 6695 E-mail: [email protected] www.grosvenorprints.com Dealers in Antique Prints & Books CATALOGUE FOR THE ABA FAIR 2008 Arts 1 – 5 Books & Ephemera 6 – 119 Decorative 120 – 155 Dogs 156 – 161 Historical, Social & Political 162 – 166 London 167 – 209 Modern Etchings 210 – 226 Natural History 227 – 233 Naval & Military 234 – 269 Portraits 270 – 448 Satire 449 – 602 Science, Trades & Industry 603 – 640 Sports & Pastimes 641 – 660 Foreign Topography 661 – 814 UK Topography 805 - 846 Registered in England No. 1305630 Registered Office: 2, Castle Business Village, Station Road, Hampton, Middlesex. TW12 2BX. Rainbrook Ltd. Directors: N.C. Talbot. T.D.M. Rayment. C.E. Ellis. E&OE VAT No. 217 6907 49 GROSVENOR PRINTS Catalogue of new stock released in conjunction with the ABA Fair 2008. In shop from noon 3rd June, 2008 and at Olympia opening 5th June. Established by Nigel Talbot in 1976, we have built up the United Kingdom’s largest stock of prints from the 17th to early 20th centuries. Well known for our topographical views, portraits, sporting and decorative subjects, we pride ourselves on being able to cater for almost every taste, no matter how obscure. We hope you enjoy this catalogue put together for this years’ Antiquarian Book Fair. Our largest ever catalogue contains over 800 items, many rare, interesting and unique images. We have also been lucky to purchase a very large stock of theatrical prints from the Estate of Alec Clunes, a well known actor, dealer and collector from the 1950’s and 60’s.
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • TRANSIENT LUNAR PHENOMENA: REGULARITY and REALITY Arlin P
    The Astrophysical Journal, 697:1–15, 2009 May 20 doi:10.1088/0004-637X/697/1/1 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. TRANSIENT LUNAR PHENOMENA: REGULARITY AND REALITY Arlin P. S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027, USA Received 2007 June 27; accepted 2009 February 20; published 2009 April 30 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is controversial. Nonetheless, TLP data show regularities in the observations; a key question is whether this structure is imposed by processes tied to the lunar surface, or by terrestrial atmospheric or human observer effects. I interrogate an extensive catalog of TLPs to gauge how human factors determine the distribution of TLP reports. The sample is grouped according to variables which should produce differing results if determining factors involve humans, and not reflecting phenomena tied to the lunar surface. Features dependent on human factors can then be excluded. Regardless of how the sample is split, the results are similar: ∼50% of reports originate from near Aristarchus, ∼16% from Plato, ∼6% from recent, major impacts (Copernicus, Kepler, Tycho, and Aristarchus), plus several at Grimaldi. Mare Crisium produces a robust signal in some cases (however, Crisium is too large for a “feature” as defined). TLP count consistency for these features indicates that ∼80% of these may be real. Some commonly reported sites disappear from the robust averages, including Alphonsus, Ross D, and Gassendi.
    [Show full text]
  • Observations from Orbiting Platforms 219
    Dotto et al.: Observations from Orbiting Platforms 219 Observations from Orbiting Platforms E. Dotto Istituto Nazionale di Astrofisica Osservatorio Astronomico di Torino M. A. Barucci Observatoire de Paris T. G. Müller Max-Planck-Institut für Extraterrestrische Physik and ISO Data Centre A. D. Storrs Towson University P. Tanga Istituto Nazionale di Astrofisica Osservatorio Astronomico di Torino and Observatoire de Nice Orbiting platforms provide the opportunity to observe asteroids without limitation by Earth’s atmosphere. Several Earth-orbiting observatories have been successfully operated in the last decade, obtaining unique results on asteroid physical properties. These include the high-resolu- tion mapping of the surface of 4 Vesta and the first spectra of asteroids in the far-infrared wave- length range. In the near future other space platforms and orbiting observatories are planned. Some of them are particularly promising for asteroid science and should considerably improve our knowledge of the dynamical and physical properties of asteroids. 1. INTRODUCTION 1800 asteroids. The results have been widely presented and discussed in the IRAS Minor Planet Survey (Tedesco et al., In the last few decades the use of space platforms has 1992) and the Supplemental IRAS Minor Planet Survey opened up new frontiers in the study of physical properties (Tedesco et al., 2002). This survey has been very important of asteroids by overcoming the limits imposed by Earth’s in the new assessment of the asteroid population: The aster- atmosphere and taking advantage of the use of new tech- oid taxonomy by Barucci et al. (1987), its recent extension nologies. (Fulchignoni et al., 2000), and an extended study of the size Earth-orbiting satellites have the advantage of observing distribution of main-belt asteroids (Cellino et al., 1991) are out of the terrestrial atmosphere; this allows them to be in just a few examples of the impact factor of this survey.
    [Show full text]
  • July 2020 in This Issue Online Readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 Click on Images an Invitation to Join ALPO 3 for Hyperlinks
    A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent back issues: http://moon.scopesandscapes.com/tlo_back.html July 2020 In This Issue Online readers, ALPO Conference November 6-7, 2020 2 Lunar Calendar July 2020 3 click on images An Invitation to Join ALPO 3 for hyperlinks. Observations Received 4 By the Numbers 7 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 9 Call For Observations Focus-On 9 Focus-On Announcement 10 2020 ALPO The Walter H. Haas Observer’s Award 11 Sirsalis T, R. Hays, Jr. 12 Long Crack, R. Hill 13 Musings on Theophilus, H. Eskildsen 14 Almost Full, R. Hill 16 Northern Moon, H. Eskildsen 17 Northwest Moon and Horrebow, H. Eskildsen 18 A Bit of Thebit, R. Hill 19 Euclides D in the Landscape of the Mare Cognitum (and Two Kipukas?), A. Anunziato 20 On the South Shore, R. Hill 22 Focus On: The Lunar 100, Features 11-20, J. Hubbell 23 Recent Topographic Studies 43 Lunar Geologic Change Detection Program T. Cook 120 Key to Images in this Issue 134 These are the modern Golden Days of lunar studies in a way, with so many new resources available to lu- nar observers. Recently, we have mentioned Robert Garfinkle’s opus Luna Cognita and the new lunar map by the USGS. This month brings us the updated, 7th edition of the Virtual Moon Atlas. These are all wonderful resources for your lunar studies.
    [Show full text]
  • Water on the Moon, III. Volatiles & Activity
    Water on The Moon, III. Volatiles & Activity Arlin Crotts (Columbia University) For centuries some scientists have argued that there is activity on the Moon (or water, as recounted in Parts I & II), while others have thought the Moon is simply a dead, inactive world. [1] The question comes in several forms: is there a detectable atmosphere? Does the surface of the Moon change? What causes interior seismic activity? From a more modern viewpoint, we now know that as much carbon monoxide as water was excavated during the LCROSS impact, as detailed in Part I, and a comparable amount of other volatiles were found. At one time the Moon outgassed prodigious amounts of water and hydrogen in volcanic fire fountains, but released similar amounts of volatile sulfur (or SO2), and presumably large amounts of carbon dioxide or monoxide, if theory is to be believed. So water on the Moon is associated with other gases. Astronomers have agreed for centuries that there is no firm evidence for “weather” on the Moon visible from Earth, and little evidence of thick atmosphere. [2] How would one detect the Moon’s atmosphere from Earth? An obvious means is atmospheric refraction. As you watch the Sun set, its image is displaced by Earth’s atmospheric refraction at the horizon from the position it would have if there were no atmosphere, by roughly 0.6 degree (a bit more than the Sun’s angular diameter). On the Moon, any atmosphere would cause an analogous effect for a star passing behind the Moon during an occultation (multiplied by two since the light travels both into and out of the lunar atmosphere).
    [Show full text]
  • Arxiv:0706.3947V1
    Transient Lunar Phenomena: Regularity and Reality Arlin P.S. Crotts Department of Astronomy, Columbia University, Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027 ABSTRACT Transient lunar phenomena (TLPs) have been reported for centuries, but their nature is largely unsettled, and even their existence as a coherent phenomenon is still controversial. Nonetheless, a review of TLP data shows regularities in the observations; a key question is whether this structure is imposed by human observer effects, terrestrial atmospheric effects or processes tied to the lunar surface. I interrogate an extensive catalog of TLPs to determine if human factors play a determining role in setting the distribution of TLP reports. We divide the sample according to variables which should produce varying results if the determining factors involve humans e.g., historical epoch or geographical location of the observer, and not reflecting phenomena tied to the lunar surface. Specifically, we bin the reports into selenographic areas (300 km on a side), then construct a robust average count for such “pixels” in a way discarding discrepant counts. Regardless of how we split the sample, the results are very similar: roughly 50% of the report count originate from the crater Aristarchus and vicinity, 16% from Plato, 6% from recent, major impacts (Copernicus, ∼ ∼ Kepler and Tycho - beyond Aristarchus), plus a few at Grimaldi. Mare Crisium produces a robust signal for three of five averages of up to 7% of the reports (however, Crisium subtends more than one pixel). The consistency in TLP report counts for specific features on this list indicate that 80% of the reports arXiv:0706.3947v1 [astro-ph] 27 Jun 2007 ∼ are consistent with being real (perhaps with the exception of Crisium).
    [Show full text]
  • RESEARCH Topographic Expressions of Lunar Graben
    RESEARCH Topographic expressions of lunar graben Melanie B. Callihan* and Christian Klimczak STRUCTURAL GEOLOGY AND GEOMECHANICS GROUP, DEPARTMENT OF GEOLOGY, UNIVERSITY OF GEORGIA, ATHENS, GEORGIA 30602, USA ABSTRACT Graben, defined as landforms produced by normal faulting, have long been recognized on the Moon, but their map patterns, as well as topographic expressions, have not been studied systematically. The topography across graben and its along-strike variations reveal details about the growth of the normal faults forming the graben. Individual normal faults grow in length by the propagation of fault tips during slip events, which can also enlarge the displacement along the fault plane. Displacement and length accumulate and grow larger over time with more slip events, fault interaction, and linkage. We measured fault lengths and vertical offsets and then calculated the displacement for lunar graben using data from the camera and laser altimeter onboard the Lunar Reconnaissance Orbiter. Our study systematically investigated 14 graben systems across the lunar surface. Graben lengths were found to range from ~43 to 453 km, and displacements ranged from ~127 to 1115 m. These displacements were plotted against graben fault length to produce slip distributions, which revealed growth patterns involving mechanical interaction and fault linkage. Displacement-to-length scaling was used to further study the evolu- tion of graben-bounding normal faults. We observed a sublinear growth pattern for lunar graben-bounding normal faults, consistent with growth of faults via segment linkage, where different stages of linkage are present on the lunar surface. Lunar graben-bounding faults show higher scaling ratios than previously estimated, likely due to variations in host-rock properties and mechanical stratigraphy.
    [Show full text]
  • Volcanic Features and Age Relationships Associated with Lunar Graben
    Lunar and Planetary Science XXX 1335.pdf VOLCANIC FEATURES AND AGE RELATIONSHIPS ASSOCIATED WITH LUNAR GRABEN. J. A. Petrycki and L. Wilson. Environmental Science Dept., Institute of Environmental and Natural Sciences, Lancaster University, Lancaster LA1 4YQ, U.K., [email protected] Introduction and Background Rima Ariadaeus, crater chains are also seen within the Lunar linear and arcuate rilles (simple graben) form rille, running parallel with the strike of the graben. as a result of near-surface deformation [1] and may Some crater chains appear at the end of the graben accompany dyke emplacement within the lunar crust and are also directly aligned along its strike, for ex- [2]. Volcanic deposits associated with the rille may be ample at Rimae Hippalus I and II. Such features tend evidence of a graben forming simultaneously with the to be formed in highland material. The rille Rima intrusion of a dyke at shallow depth. Most graben Daniell II, is interrupted by a chain of craters along its occur on the lunar nearside. They are most often as- length, parallel to strike. The crater chains associated sociated with maria, crossing from mare to highland with the rilles are nearly all (labelled ‘ch’, ‘C.Ech’or terrains or lying within highlands surrounding maria ‘C.Eci’ on the U.S.G.S. geologic maps) interpreted as [3]. structurally controlled volcanic vents or collapse de- pressions. Crater chains labelled as secondary craters Graben formation is generally thought to be (‘Csc’), sometimes appear to be directly associated restricted to the period prior to 3.6 +/- 0.2 Ga [4, 5].
    [Show full text]
  • Conference on Origins of Planetary Magnetism
    Papers Presented to the CONFERENCE ON ORIGINS OF PLANETARY MAGNETISM (NASA-CR-157825) PAPERS PRESENTED TO THE N79-12986 CONFERENCE ON ORIGINS OF PLANETARY MAGNETISM (Lunar and Planetary Inst.) 142 p HC A07/F Ikol CSCL 03B Unclas G3/91 36976 Houston,Texas 8-11 November 1978 A Lunar and Planetary Institute Topical Conference i ~ UNIVERSITIES SPACE R ESEARCH ASSOCIATION A LUNAR AND PLANETARY INSTITUTE g C 3303 NASA ROAD 1 HOUSTON, TEXAS 77068 PAPERS PRESENTED TO THE CONFERENCE ON ORIGINS OF PLANETARY MAGNETISM A LUNAR AND PLANETARY INSTITUTE TOPICAL CONFERENCE 8-11 NOVEMBER 1978 CompiZed by the Lunar and Planetary Institute 3303 NASA Road One Houston, Texas 7?058 LPI Contribution 348 Material in this volume may be copied without restraint for library, abstract service, educational or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as appropriate acknowledgment of this publication. Library of Congress Card No. 79-189790 PREFACE This volume contains papers which have been accepted for publication by the Program Committee of the Conference on the Origins of Planetary Magnetism. Papers were solicited which address one of the following major topics: I. Geomagnetism in the context of planetary magnetism II. Lunar magnetism III. Dynamo theory and non-dynamo processes IV. Comparative planetary magnetism (terrestrial and outer planets) V. Meteoritic magnetism and the early solar magnetic field. The Program Committee consists of L. J. Srnka, Convenor (Lunar and Planetary Institute), P. R. Brett (National Science Foundation), F. H. Busse (University of California), R. B. Merrill (Lunar and Planetary Institute), N.
    [Show full text]
  • January 2020 in This Issue
    A publication of the Lunar Section of ALPO Edited by David Teske: [email protected] 2162 Enon Road, Louisville, Mississippi, USA Recent back issues: http://moon.scopesandscapes.com/tlo_back.html January 2020 In This Issue Lunar Calendar January 2020 2 Lunar Libration January 2020 2 An Invitation to Join ALPO 2 Observations Received 3 Submission Through the ALPO Image Achieve 4 When Submitting Observations to the ALPO Lunar Section 5 Call For Observations Focus-On Tycho and Herodotus 5 Future Focus-On Articles 5 Focus-On Plato and Theophilus J. Hubbell 6 Lacus Mortis H. Eskildsen 18 Oh No! Mr. Bill and Billy D. Teske 19 Vitruvius and Cauchy Domes H. Eskildsen 21 A Gemma of a Region (Gemma Frisius) R. Hill 22 Kies Domes and Marth H. Eskildsen 23 Down Under (Licetus to Boussingault) R. Hill 24 Gambart Domes H. Eskildsen 25 Lost in the Glory R. Hill 26 Capuanus Domes 2019.12.06 H. Eskildsen 27 Meet the Catena (Catena Abulfeda) R. Hill 28 Lansberg D Domes H. Eskildsen 29 Recent Topographic Studies 30 Lunar Geologic Change Detection Program T. Cook 39 Key to Images in this Issue 52 In the January 2020 issue of The Lunar Observer, you will find an extensive Focus-On article about craters Plato and Theophilus by Jerry Hubbell. Rik Hill covers some complicated regions of the lunar highlands with his four articles and stunning images. Howard Eskildsen continues his research and imag- ing of lunar domes near Vitruvius and Cauchy, Kies, Gambart, Capuanus and Lansberg D. David Teske delves into the area near Billy and Flamsteed with a whimsical character.
    [Show full text]
  • Rimae Sirsalis
    RIMAE SIRSALIS Nieves del Río, José Castillo, Eduardo Adarve, Jorge Arranz y Alberto Martos del Grupo de Estudios Lunares “Enrique Silva”. [Página dejada intencionadamente en blanco] - 2 - INTRODUCCIÓN Rimae Sirsalis es un sistema de grietas que comprende dos estructuras de esta clase, Rima Sirsalis y Rima Sirsalis I, siendo la primera mucho más larga y mucho más perceptible que la segunda. Pertenecen a la clase de grietas rectas, cuyo aspecto es diferente del aspecto de las grietas circulares que bordean las cuencas de las grandes estructuras de impacto. Lo que tiene de particular este sistema, para que haya merecido figurar como objetivo 1 en el apartado “Call for Observations 2”, del boletín TLO 3 de ALPO 4, son sus dos características principales: siendo Rima Sirsalis la grieta más larga existente en la cara cislunar (la visible), está situada en una región cuyo suelo es geológicamente distinto de la naturaleza de suelos por los que discurren en general las grietas lunares. En efecto, las grietas lunares (llamadas en latín rimae ) son siempre estructuras volcánicas, generalmente túneles de lava cuyo techo se ha desplomado, o surcos por los cuales fluyó la lava en su día, en favor de la pendiente del suelo. Por esta razón, se las encuentra siempre sobre terrenos magmáticos, como los maria (plural de mare ), los sini (plural de sinus ), los laci (plural de lacus ), o los paludes (plural de palus ), o sea sobre los “mares”, las “bahías”, los “lagos” o las “marismas” lunares. Como ejemplos de esta condición se puede citar a Rimae Hypatia, situada en el Mare Tranquillitatis, a Rima Oppolzer, en Sinus Medii, a Rimae Bürg y Rimae Daniell, en Lacus Mortis y Lacus Somniorum, respectivamente y Rima Hesiodus en Palus Epidemiarum.
    [Show full text]