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Tectonic Influences on the Spatial and Temporal Evolution of the Walker Lane: an Incipient Transform Fault Along the Evolving Pacific – North American Plate Boundary
Arizona Geological Society Digest 22 2008 Tectonic influences on the spatial and temporal evolution of the Walker Lane: An incipient transform fault along the evolving Pacific – North American plate boundary James E. Faulds and Christopher D. Henry Nevada Bureau of Mines and Geology, University of Nevada, Reno, Nevada, 89557, USA ABSTRACT Since ~30 Ma, western North America has been evolving from an Andean type mar- gin to a dextral transform boundary. Transform growth has been marked by retreat of magmatic arcs, gravitational collapse of orogenic highlands, and periodic inland steps of the San Andreas fault system. In the western Great Basin, a system of dextral faults, known as the Walker Lane (WL) in the north and eastern California shear zone (ECSZ) in the south, currently accommodates ~20% of the Pacific – North America dextral motion. In contrast to the continuous 1100-km-long San Andreas system, discontinuous dextral faults with relatively short lengths (<10-250 km) characterize the WL-ECSZ. Cumulative dextral displacement across the WL-ECSZ generally decreases northward from ≥60 km in southern and east-central California, to ~25 km in northwest Nevada, to negligible in northeast California. GPS geodetic strain rates average ~10 mm/yr across the WL-ECSZ in the western Great Basin but are much less in the eastern WL near Las Vegas (<2 mm/ yr) and along the northwest terminus in northeast California (~2.5 mm/yr). The spatial and temporal evolution of the WL-ECSZ is closely linked to major plate boundary events along the San Andreas fault system. For example, the early Miocene elimination of microplates along the southern California coast, southward steps in the Rivera triple junction at 19-16 Ma and 13 Ma, and an increase in relative plate motions ~12 Ma collectively induced the first major episode of deformation in the WL-ECSZ, which began ~13 Ma along the N60°W-trending Las Vegas Valley shear zone. -
Constraints on Present-Day Basin and Range Deformation from Space Geodesy Timothy H
University of South Florida Scholar Commons School of Geosciences Faculty and Staff School of Geosciences Publications 1995 Constraints on Present-Day Basin and Range Deformation from Space Geodesy Timothy H. Dixon University of Miami, [email protected] Stefano Robaudo University of Miami Jeffrey Lee California Institute of Technology Marith C. Reheis U.S. Geological Survey Follow this and additional works at: https://scholarcommons.usf.edu/geo_facpub Part of the Earth Sciences Commons Scholar Commons Citation Dixon, Timothy H.; Robaudo, Stefano; Lee, Jeffrey; and Reheis, Marith C., "Constraints on Present-Day Basin and Range Deformation from Space Geodesy" (1995). School of Geosciences Faculty and Staff Publications. 495. https://scholarcommons.usf.edu/geo_facpub/495 This Article is brought to you for free and open access by the School of Geosciences at Scholar Commons. It has been accepted for inclusion in School of Geosciences Faculty and Staff ubP lications by an authorized administrator of Scholar Commons. For more information, please contact [email protected]. TECTONICS, VOL. 14, NO. 4, ]'AGES 755-772, AUGUST 1995 Constraints on present-day Basin and Range deformation from space geodesy TimothyH. Dixonand Stefano Robaudo • RosenstielSchool of Marine and AtmosphericSciences, University of Miami Miami, Florida JeffreyLee 2 Division of Geologicaland Planetary Sciences, California Institute of Technology,Pasadena Marith C. Reheis U.S. GeologicalSurvey, Lakewood, Colorado Abstract. We use new spacegeodetic data from very long extension.A slip rate budgetfor major strike-slipfaults in baselineinterferometry and satellite laser ranging combined our studyarea based on a combinationof local geodeticor with other geodetic and geologic data to study late Quaternary geologic data and the regional space contemporarydeformation in the Basinand Range province geodeticdata suggeststhe following rates of right-lateral of the western United States. -
No. 40. the System of Lunar Craters, Quadrant Ii Alice P
NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates. -
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. -
University Microfilms, a XEROX Company/Ann Arbor, Michigan
1 72-4602^ FAPO, Haim Benzion, 1932- OPTIMAL SELENODETIC CONTROL. The Ohio State University, Ph.Dl, i'971‘ Geodesy University Microfilms, A X E R O X Company /Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED ! OPTIMAL SELENODETIC CONTROL DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University by • Halm Benzion Papo, B.Sc., M.Sc. The Ohio State University 1971 Approved by f U l t U , /■ llU 'gsileA ^ Advisor Department of Geodetic Science To Viola ACKNOWLEDGEMENTS ' « ‘ It gives me a great pleasure to be able to extend my gratitude and appreciation to the many persons without whom this work would not have * been possible. From my parents I inherited a deep and sincere love for learning and an acute curiosity for the unknown and the unsurveyed. The Technion, Israels Institute of Technology and The Ohio State University provided me with the best education one could ask for in my field. Working in Room 231, Lord Hall on the OSU campus with other graduate students like myself has been a wonderful experience. There was an atmosphere of enthusiastic learning, of a fruitful exchange of ideas, of sharing ones excitement over finding an answer to a problem, of true friendship of people working together. The OSU Computer Center provided me generously with computer time needed for the study and through the invaluable assistance of Mr. John M. Snowden, I was able to make full use of its excellent facilities. Discussions on many conceptual and practical problems with Doctors Peter Meissl, Dean C. -
University Microfilms, a XEROX Company, Ann Arbor, Michigan
.72-4480 FAJEMIROKUN, Francis Afolabi, 1941- APPLICATION OF NEW OBSERVATIONAL SYSTEMS FOR SELENODETIC CONTROL. The Ohio State University, Ph.D., 1971 Geodesy University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED APPLICATION OF NEW OBSERVATIONAL SYSTEMS FOR SELENODETIC CONTROL DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University by Francis Afolabi Fajemirokun, B. Sc., M. Sc. The Ohio State University 1971 Approved by l/m /• A dviser Department of Geodetic Science PLEASE NOTE: Some Pages have indistinct p rin t. Filmed as received. UNIVERSITY MICROFILMS To Ijigbola, Ibeolayemi and Oladunni ACKNOW LEDGEME NTS The author wishes to express his deep gratitude to the many persons, without whom this work would not have been possible. First and foremost, the author is grateful to the Department of Geodetic Science and themembers of its staff, for the financial support and academic guidance given to him during his studies here. In particular, the author wishes to thank his adviser Professor Ivan I. Mueller, for his encouragement, patience and guidance through the various stages of this work. Professors Urho A. Uotila, Richard H. Rapp and Gerald H. Newsom served on the author’s reading committee, and offered many valuable suggestions to help clarify many points. The author has also enjoyed working with other graduate students in the department, especially with the group at 231 Lord Hall, where there was always an atmosphere of enthusiastic learning and of true friendship. The author is grateful to the various scientists outside the department, with whom he had discussions on the subject of this work, especially to the VLBI group at the Smithsonian Astrophysical Observatory in Cambridge, Ma s sachu s s etts . -
May 2009 Explorer
Vol. 30, No. 5 May 2009 Commitment to the Very Core Kirchhoff PSDM section. Controlled Beam PSDM section. CHALLENGE > To image the oil-bearing fracture zones in a complex granite basement reservoir offshore Vietnam where conventional methods fail to produce convincing results. SOLUTION > The data was reprocessed using the CGGVeritas Controlled Beam Migration algorithm for the velocity model building and the final migration. RESULTS > Based on the new CBM images, the operator was able to confidently carry out a successful drilling campaign to develop the reservoir. cggveritas.com MAY 2009 3 On the cover: Geologists have known about it for decades, but now the rest of the world is being invited to the party – the year-long celebration of the 100th anniversary of the discovery of the Burgess Shale is about to begin. Shown here are geologists at the Burgess Shale’s Walcott Quarry, a site that has been called “Mecca for paleontologists” because of its treasure trove of fossils. It’s located in Yoho National Park in British Columbia – a park that is itself a cathedral to geologic splendor. See story on page 20; photo courtesy of Jon Dudley. Your shut door, our open window: Current fiscal realities 8 have stalled some projects, but two geologists say now is the perfect time to consider better ways to evaluate shale Photo courtesy of Denver Visitor and Convention Bureau . gas potential A chance to hike in the Gore Range near Denver is just one of the reasons to attend this year’s AAPG Annual Convention and Exhibition. Need more reasons? Check out Can’t we all just get along? Companies have accepted that 12 the Director’s Corner on page 50 – and start making your plans now to head to Denver. -
0 Lunar and Planetary Institute Provided by the NASA Astrophysics Data System THORIUM CONCENTRATIONS : IMBRIUM and ADJACENT REGIONS
THORIUM CONCENTRATIONS IN THE IMBRIUM AND ADJACENT REGIONS OF THE MOON. A1 bert E. Metzger, Eldon L. Haines*, Maria I. Etchegaray-Ramirez, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103, and B. Ray Hawke, Hawaii Institute of Geophysics, University of Hawaii, Honolulu, HI 96822. The orbital gamma-ray spectrometer deconvolution technique restores some of the inherent spatial resolution and contrast lost because of the substan- tial field of view of the instrument. The technique has previously been applied to the observed Th distributions in the Aristarchus, Apennine, and Smythii regions of the Moon overflown by Apollo (1,2). Application has now been made to the Imbrium region using that portion of the data field extending from 10°W - 42OW, over which the data coverage lies between 18ON and 30°N. The area enclosed not only fills in the interval between the Aristarchus- and Apennine-centered regions previously reported but also provides overlap regions which serve as a test of consistency. It is characterized by basalt flows of various ages, depths, and spectral proper- ties, craters of Copernican and Eratosthenian age, and probable areas of pyroclastic mantling . The Aristarchus and Apennine regions contain two of the three areas of maximum radioactivity observed along the Apollo 15 and 16 data tracks. For both regions the undeconvolved values for the 2' x 2" pixels comprising the data base, range over a factor of 3-4 with maximum values in excess of 8.5 ppm. By comparison, the Imbrium field contains a contrast of only 1.5, the values being more uniformly high, but with an upper limit of about 6.5 ppm. -
CALIFORNIA's NORTH COAST: a Literary Watershed: Charting the Publications of the Region's Small Presses and Regional Authors
CALIFORNIA'S NORTH COAST: A Literary Watershed: Charting the Publications of the Region's Small Presses and Regional Authors. A Geographically Arranged Bibliography focused on the Regional Small Presses and Local Authors of the North Coast of California. First Edition, 2010. John Sherlock Rare Books and Special Collections Librarian University of California, Davis. 1 Table of Contents I. NORTH COAST PRESSES. pp. 3 - 90 DEL NORTE COUNTY. CITIES: Crescent City. HUMBOLDT COUNTY. CITIES: Arcata, Bayside, Blue Lake, Carlotta, Cutten, Eureka, Fortuna, Garberville Hoopa, Hydesville, Korbel, McKinleyville, Miranda, Myers Flat., Orick, Petrolia, Redway, Trinidad, Whitethorn. TRINITY COUNTY CITIES: Junction City, Weaverville LAKE COUNTY CITIES: Clearlake, Clearlake Park, Cobb, Kelseyville, Lakeport, Lower Lake, Middleton, Upper Lake, Wilbur Springs MENDOCINO COUNTY CITIES: Albion, Boonville, Calpella, Caspar, Comptche, Covelo, Elk, Fort Bragg, Gualala, Little River, Mendocino, Navarro, Philo, Point Arena, Talmage, Ukiah, Westport, Willits SONOMA COUNTY. CITIES: Bodega Bay, Boyes Hot Springs, Cazadero, Cloverdale, Cotati, Forestville Geyserville, Glen Ellen, Graton, Guerneville, Healdsburg, Kenwood, Korbel, Monte Rio, Penngrove, Petaluma, Rohnert Part, Santa Rosa, Sebastopol, Sonoma Vineburg NAPA COUNTY CITIES: Angwin, Calistoga, Deer Park, Rutherford, St. Helena, Yountville MARIN COUNTY. CITIES: Belvedere, Bolinas, Corte Madera, Fairfax, Greenbrae, Inverness, Kentfield, Larkspur, Marin City, Mill Valley, Novato, Point Reyes, Point Reyes Station, Ross, San Anselmo, San Geronimo, San Quentin, San Rafael, Sausalito, Stinson Beach, Tiburon, Tomales, Woodacre II. NORTH COAST AUTHORS. pp. 91 - 120 -- Alphabetically Arranged 2 I. NORTH COAST PRESSES DEL NORTE COUNTY. CRESCENT CITY. ARTS-IN-CORRECTIONS PROGRAM (Crescent City). The Brief Pelican: Anthology of Prison Writing, 1993. 1992 Pelikanesis: Creative Writing Anthology, 1994. 1994 Virtual Pelican: anthology of writing by inmates from Pelican Bay State Prison. -
Upper Neogene Stratigraphy and Tectonics of Death Valley — a Review
Earth-Science Reviews 73 (2005) 245–270 www.elsevier.com/locate/earscirev Upper Neogene stratigraphy and tectonics of Death Valley — a review J.R. Knott a,*, A.M. Sarna-Wojcicki b, M.N. Machette c, R.E. Klinger d aDepartment of Geological Sciences, California State University Fullerton, Fullerton, CA 92834, United States bU. S. Geological Survey, MS 975, 345 Middlefield Road, Menlo Park, CA 94025, United States cU. S. Geological Survey, MS 966, Box 25046, Denver, CO 80225-0046, United States dTechnical Service Center, U. S. Bureau of Reclamation, P. O. Box 25007, D-8530, Denver, CO 80225-0007, United States Abstract New tephrochronologic, soil-stratigraphic and radiometric-dating studies over the last 10 years have generated a robust numerical stratigraphy for Upper Neogene sedimentary deposits throughout Death Valley. Critical to this improved stratigraphy are correlated or radiometrically-dated tephra beds and tuffs that range in age from N3.58 Ma to b1.1 ka. These tephra beds and tuffs establish relations among the Upper Pliocene to Middle Pleistocene sedimentary deposits at Furnace Creek basin, Nova basin, Ubehebe–Lake Rogers basin, Copper Canyon, Artists Drive, Kit Fox Hills, and Confidence Hills. New geologic formations have been described in the Confidence Hills and at Mormon Point. This new geochronology also establishes maximum and minimum ages for Quaternary alluvial fans and Lake Manly deposits. Facies associated with the tephra beds show that ~3.3 Ma the Furnace Creek basin was a northwest–southeast-trending lake flanked by alluvial fans. This paleolake extended from the Furnace Creek to Ubehebe. Based on the new stratigraphy, the Death Valley fault system can be divided into four main fault zones: the dextral, Quaternary-age Northern Death Valley fault zone; the dextral, pre-Quaternary Furnace Creek fault zone; the oblique–normal Black Mountains fault zone; and the dextral Southern Death Valley fault zone. -
National Monuments and the Forest Service
NATIONAL MONUMENTS AND THE FOREST SERVICE Gerald W. Williams, Ph.D., (Retired) USDA Forest Service Washington, DC National monuments are areas of federal land set aside by the Congress or most often by the president, under authority of the American Antiquities Act of June 8, 1906, to protect or enhance prominent or important features of the national landscape. Such important national features include those land areas that have historic cultural importance (sites and landmarks), prehistoric prominence, or those of scientific or ecological significance. Today, depending on how one counts, there are 81 national monuments administered by the USDI National Park Service, 13 more administered by the USDI Bureau of Land Management (BLM), five others administered by the USDA Forest Service, two jointly managed by the BLM and the National Park Service, one jointly administered by the BLM and the Forest Service, one by the USDI Fish & Wildlife Service, and another by the Soldiers’ and Airmen’s Home in Washington, D.C. In addition, one national monument is under National Park Service jurisdiction, but managed by the Forest Service while another is on USDI Bureau of Reclamation administered land, but managed by the Park Service. The story of the national monuments and the Forest Service also needs to cover briefly the creation of national parks from national forest and BLM lands. More new national monuments and national parks are under consideration for establishment. ANTIQUITIES ACT OF 1906 Shortly after the turn of the century, many citizens’ groups and organizations, as well as members of Congress, believed it was necessary that an act of Congress be passed to combat the increasing acts of vandalism and even destruction of important cultural (historic and prehistoric), scenic, physical, animal, and plant areas around the country (Rothman 1989). -
Seismic Imaging Using Earthquakes and Implications for Earth Systems
Seismic imaging using earthquakes and implications for earth systems 123* 2 3 3 3 Huaiyu Yuan , Mike Dentith , Ruth Murdie , Simon Johnson and Klaus Gessner * Currently in a week-long meeting in San Francisco. 1 2 3 [email protected] CCFS, Macquarie University; CET-UWA; GSWA Email [email protected] for questions. Or spend a good 15 mintues reading it through! 1. Lithosphere control of the mineral systems and seismic imaging 6. Capricorn passive source project How giant magma-related ore systems form is vigorously debated. One view, displayed below, argues ascending magmas pick up ore-forming compo- The Capricorn orogen is a major tectonic unit that recorded the assembly of the Yil- nents (diamonds, gold) during their passage through the mantle lithosphere (Griffin et al., Nature Geoscience, 2013): e.g. garn and Pilbara cratons and the Proterozoic terranes to form the West Australian (a) diamonds, formed deep from metasomatically introduced carbon zones, are brought to surface in magmas that take advantage of lithospheric scale craton (a; e.g. Johnson et al. 2013). Numerous mineral deposit types have been rec- weak zones; and ognized throughout the orogen, and recent studies (Johnson et al. 2013; Aitken et (b) Au- and Cu-rich deposits are found in the back-arc and the mantle wedge, which are associated with low-degree and hi-degree melting, respectively. al. 2013) have illustrated the connection between known mineral deposits and the crustal scale fault systems and corresponding crustal blocks (b). In all cases lithospheric scale weak zones facilitate the movement of metal-bearing fluids to the surface.