DOGAMI Open-File Report O-82-09, Gravity Anomalies in the Cascade
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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. -
A Fast Method for Calculation of Marine Gravity Anomaly
applied sciences Article A Fast Method for Calculation of Marine Gravity Anomaly Yuan Fang 1, Shuiyuan He 2,*, Xiaohong Meng 1,*, Jun Wang 1, Yongkang Gan 1 and Hanhan Tang 1 1 School of Geophysics and Information Technology, China University of Geosciences, Beijing 100083, China; [email protected] (Y.F.); [email protected] (J.W.); [email protected] (Y.G.); [email protected] (H.T.) 2 Guangzhou Marine Geological Survey, China Geological Survey, Ministry of Land and Resources, Guangzhou 510760, China * Correspondence: [email protected] (S.H.); [email protected] (X.M.); Tel.: +86-136-2285-1110 (S.H.); +86-136-9129-3267 (X.M.) Abstract: Gravity data have been playing an important role in marine exploration and research. However, obtaining gravity data over an extensive marine area is expensive and inefficient. In reality, marine gravity anomalies are usually calculated from satellite altimetry data. Over the years, numer- ous methods have been presented for achieving this purpose, most of which are time-consuming due to the integral calculation over a global region and the singularity problem. This paper proposes a fast method for the calculation of marine gravity anomalies. The proposed method introduces a novel scheme to solve the singularity problem and implements the parallel technique based on a graphics processing unit (GPU) for fast calculation. The details for the implementation of the proposed method are described, and it is tested using the geoid height undulation from the Earth Gravitational Model 2008 (EGM2008). The accuracy of the presented method is evaluated by comparing it with marine shipboard gravity data. -
USGS USGS Geologic Investigations Series I-2569, Pamphlet
U.S. DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP I–2569 U.S. GEOLOGICAL SURVEY GEOLOGIC MAP OF UPPER EOCENE TO HOLOCENE VOLCANIC AND RELATED ROCKS OF THE CASCADE RANGE, OREGON By David R. Sherrod and James G. Smith INTRODUCTION volcanic-hosted mineral deposits and even to potential volcanic hazards. Since 1979, Earth scientists of the Geothermal Historically, the regional geology of the Cascade Research Program of the U.S. Geological Survey have Range in Oregon has been interpreted through recon carried out multidisciplinary research in the Cascade naissance studies of large areas (for example, Diller, Range. The goal of this research is to understand 1898; Williams, 1916; Callaghan and Buddington, the geology, tectonics, and hydrology of the Cas cades in order to characterize and quantify geothermal 1938; Williams, 1942, 1957; Peck and others, 1964). Early studies were hampered by limited access, resource potential. A major goal of the program generally poor exposures, and thick forest cover, which is compilation of a comprehensive geologic map of flourishes in the 100 to 250 cm of annual precipi the entire Cascade Range that incorporates modern tation west of the range crest. In addition, age control field studies and that has a unified and internally con was scant and limited chiefly to fossil flora. Since sistent explanation. This map is one of three in a series that shows then, access has greatly improved via a well-devel- oped network of logging roads, and isotopic ages— Cascade Range geology by fitting published and mostly potassium-argon (K-Ar)—have gradually solved unpublished mapping into a province-wide scheme some major problems concerning timing of volcan of rock units distinguished by composition and age; ism and age of mapped units. -
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. -
THE EARTH's GRAVITY OUTLINE the Earth's Gravitational Field
GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY OUTLINE The Earth's gravitational field 2 Newton's law of gravitation: Fgrav = GMm=r ; Gravitational field = gravitational acceleration g; gravitational potential, equipotential surfaces. g for a non–rotating spherically symmetric Earth; Effects of rotation and ellipticity – variation with latitude, the reference ellipsoid and International Gravity Formula; Effects of elevation and topography, intervening rock, density inhomogeneities, tides. The geoid: equipotential mean–sea–level surface on which g = IGF value. Gravity surveys Measurement: gravity units, gravimeters, survey procedures; the geoid; satellite altimetry. Gravity corrections – latitude, elevation, Bouguer, terrain, drift; Interpretation of gravity anomalies: regional–residual separation; regional variations and deep (crust, mantle) structure; local variations and shallow density anomalies; Examples of Bouguer gravity anomalies. Isostasy Mechanism: level of compensation; Pratt and Airy models; mountain roots; Isostasy and free–air gravity, examples of isostatic balance and isostatic anomalies. Background reading: Fowler §5.1–5.6; Lowrie §2.2–2.6; Kearey & Vine §2.11. GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY FIELD Newton's law of gravitation is: ¯ GMm F = r2 11 2 2 1 3 2 where the Gravitational Constant G = 6:673 10− Nm kg− (kg− m s− ). ¢ The field strength of the Earth's gravitational field is defined as the gravitational force acting on unit mass. From Newton's third¯ law of mechanics, F = ma, it follows that gravitational force per unit mass = gravitational acceleration g. g is approximately 9:8m/s2 at the surface of the Earth. A related concept is gravitational potential: the gravitational potential V at a point P is the work done against gravity in ¯ P bringing unit mass from infinity to P. -
Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering
The fractured Moon: Production and saturation of porosity in the lunar highlands from impact cratering The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Soderblom, Jason M., et al. “The Fractured Moon: Production and Saturation of Porosity in the Lunar Highlands from Impact Cratering.” Geophysical Research Letters, vol. 42, no. 17, Sept. 2015, pp. 6939–44. © 2015 American Geophysical Union As Published http://dx.doi.org/10.1002/2015GL065022 Publisher American Geophysical Union (AGU) Version Final published version Citable link http://hdl.handle.net/1721.1/118615 Terms of Use Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. PUBLICATIONS Geophysical Research Letters RESEARCH LETTER The fractured Moon: Production and saturation 10.1002/2015GL065022 of porosity in the lunar highlands Key Points: from impact cratering • The relation between impact-generated porosity and crater size is quantified Jason M. Soderblom1, Alexander J. Evans2, Brandon C. Johnson1, H. Jay Melosh3, Katarina Miljković1,4, • Impacts into highly porous targets 5 6 7 8 3 result in positive gravity anomalies Roger J. Phillips , Jeffrey C. Andrews-Hanna , Carver J. Bierson , James W. Head III , Colleen Milbury , 9 7 1 2,10 11 • The cratering record of the oldest Gregory A. Neumann , Francis Nimmo , David E. Smith , Sean C. Solomon , Michael M. Sori , lunar surfaces is preserved in the -
Upper Deschutes River · ·Basin Prehistory
Upper Deschutes River · ·Basin Prehistory: A Preliminary Examination of Flaked Stone Tools and Debitage Michael W. Taggart 2002 ·~. ... .. " .. • '·:: ••h> ·';'"' •..,. •.• '11\•.. ...... :f~::.. ·:·. .. ii AN ABSTRACT OF THE THESIS OF Michael W. Taggart for the degree of Master of Arts in Interdisciplinary Studies in Anthropology. Anthropology. and Geography presented on April 19. 2002. Title: Upper Deschutes River Basin Prehistory: A Preliminary Examination of Flaked Stone Tools and Debitage. The prehistory of Central Oregon is explored through the examination of six archaeological sites and two isolated finds from the Upper Deschutes River Basin. Inquiry focuses on the land use, mobility, technological organization, and raw material procurement of the aboriginal inhabitants of the area. Archaeological data presented here are augmented with ethnographic accounts to inform interpretations. Eight stone tool assemblages and three debitage assemblages are analyzed in order to characterize technological organization. Diagnostic projectile points recovered from the study sites indicate the area was seasonally utilized prior to the eruption of ancient Mt. Mazama (>6,845 BP), and continuing until the Historic period (c. 1850). While there is evidence of human occupation at the study sites dating to between >7,000- 150 B.P., the range of activities and intensity of occupation varied. Source characterization analysis indicates that eight different Central Oregon obsidian sources are represented at the sites. Results of the lithic analysis are presented in light of past environmental and social phenomena including volcanic eruptions, climate change, and human population movements. Chapter One introduces the key questions that directed the inquiry and defines the theoretical perspective used. Chapter Two describes the modem and ancient environmental context of study area. -
Detection of Caves by Gravimetry
Detection of Caves by Gravimetry By HAnlUi'DO J. Cmco1) lVi/h plates 18 (1)-21 (4) Illtroduction A growing interest in locating caves - largely among non-speleolo- gists - has developed within the last decade, arising from industrial or military needs, such as: (1) analyzing subsUl'face characteristics for building sites or highway projects in karst areas; (2) locating shallow caves under airport runways constructed on karst terrain covered by a thin residual soil; and (3) finding strategic shelters of tactical significance. As a result, geologists and geophysicists have been experimenting with the possibility of applying standard geophysical methods toward void detection at shallow depths. Pioneering work along this line was accomplishecl by the U.S. Geological Survey illilitary Geology teams dUl'ing World War II on Okinawan airfields. Nicol (1951) reported that the residual soil covel' of these runways frequently indicated subsi- dence due to the collapse of the rooves of caves in an underlying coralline-limestone formation (partially detected by seismic methods). In spite of the wide application of geophysics to exploration, not much has been published regarding subsUl'face interpretation of ground conditions within the upper 50 feet of the earth's surface. Recently, however, Homberg (1962) and Colley (1962) did report some encoUl'ag- ing data using the gravity technique for void detection. This led to the present field study into the practical means of how this complex method can be simplified, and to a use-and-limitations appraisal of gravimetric techniques for speleologic research. Principles all(1 Correctiolls The fundamentals of gravimetry are based on the fact that natUl'al 01' artificial voids within the earth's sUl'face - which are filled with ail' 3 (negligible density) 01' water (density about 1 gmjcm ) - have a remark- able density contrast with the sUl'roun<ling rocks (density 2.0 to 1) 4609 Keswick Hoad, Baltimore 10, Maryland, U.S.A. -
Lower Sycan Watershed Analysis
Lower Sycan Watershed Analysis Fremont-Winema National Forest 2005 Lower Sycan River T33S,R12E,S23 Lower Sycan Watershed Analysis Table of Contents INTRODUCTION...................................................................................................................................... 1 General Watershed Area.....................................................................................................................................2 Geology and Soils.................................................................................................................................................5 Climate..................................................................................................................................................................6 STEP 1. CHARACTERIZATION OF THE WATERSHED ................................................................... 7 I. Watershed and Aquatics.................................................................................................................................7 Soils And Geomorphology...............................................................................................................................................10 Aquatic Habitat ................................................................................................................................................................10 II. Vegetation.....................................................................................................................................................12 -
Testing Hypotheses for the Origin of Steep Slope of Lunar Size-Frequency Distribution for Small Craters
CORE Metadata, citation and similar papers at core.ac.uk Provided by Springer - Publisher Connector Earth Planets Space, 55, 39–51, 2003 Testing hypotheses for the origin of steep slope of lunar size-frequency distribution for small craters Noriyuki Namiki1 and Chikatoshi Honda2 1Department of Earth and Planetary Sciences, Kyushu University, Hakozaki 6-10-1, Higashi-ku, Fukuoka 812-8581, Japan 2The Institute of Space and Astronautical Science, Yoshinodai 3-1-1, Sagamihara 229-8510, Japan (Received June 13, 2001; Revised June 24, 2002; Accepted January 6, 2003) The crater size-frequency distribution of lunar maria is characterized by the change in slope of the population between 0.3 and 4 km in crater diameter. The origin of the steep segment in the distribution is not well understood. Nonetheless, craters smaller than a few km in diameter are widely used to estimate the crater retention age for areas so small that the number of larger craters is statistically insufficient. Future missions to the moon, which will obtain high resolution images, will provide a new, large data set of small craters. Thus it is important to review current hypotheses for their distributions before future missions are launched. We examine previous and new arguments and data bearing on the admixture of endogenic and secondary craters, horizontal heterogeneity of the substratum, and the size-frequency distribution of the primary production function. The endogenic crater and heterogeneous substratum hypotheses are seen to have little evidence in their favor, and can be eliminated. The primary production hypothesis fails to explain a wide variation of the size-frequency distribution of Apollo panoramic photographs. -
Arxiv:2003.06799V2 [Astro-Ph.EP] 6 Feb 2021
Thomas Ruedas1,2 Doris Breuer2 Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies final version 18 September 2020 published: Icarus 358, 114176 (2021) 1Museum für Naturkunde Berlin, Germany 2Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany arXiv:2003.06799v2 [astro-ph.EP] 6 Feb 2021 The version of record is available at http://dx.doi.org/10.1016/j.icarus.2020.114176. This author pre-print version is shared under the Creative Commons Attribution Non-Commercial No Derivatives License (CC BY-NC-ND 4.0). Electrical and seismological structure of the martian mantle and the detectability of impact-generated anomalies Thomas Ruedas∗ Museum für Naturkunde Berlin, Germany Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Doris Breuer Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany Highlights • Geophysical subsurface impact signatures are detectable under favorable conditions. • A combination of several methods will be necessary for basin identification. • Electromagnetic methods are most promising for investigating water concentrations. • Signatures hold information about impact melt dynamics. Mars, interior; Impact processes Abstract We derive synthetic electrical conductivity, seismic velocity, and density distributions from the results of martian mantle convection models affected by basin-forming meteorite impacts. The electrical conductivity features an intermediate minimum in the strongly depleted topmost mantle, sandwiched between higher conductivities in the lower crust and a smooth increase toward almost constant high values at depths greater than 400 km. The bulk sound speed increases mostly smoothly throughout the mantle, with only one marked change at the appearance of β-olivine near 1100 km depth. -
Gravity Anomaly Measuring Gravity
Gravity Newton’s Law of Gravity (1665) 2 F = G (m1m2) / r F = force of gravitational attraction m1 and m2 = mass of 2 attracting objects r = distance between the two objects G -- ? Earth dimensions: 3 rearth = 6.378139 x 10 km (equator) 27 mearth = 5.976 x 10 g 2 F = G (m1m2) / r ) 2 F = mtest (G mEarth / rEarth ) Newton’s Second Law: F = ma implies that the acceleration at the surface of the Earth is: 2 (G mEarth / rEarth ) = ~ 981 cm/sec2 = 981 “Gals” variations are on the order of (0.1 mgal) Precision requires 2 spatially based corrections must account for 2 facts about the Earth it is not round (.... it’s flattened at the poles) it is not stationary ( .... it’s spinning) Earth is an ellipsoid first detected by Newton in 1687 clocks 2 min/day slower at equator than in England concluded regional change in "g" controlling pendulum translated this 2 min into different values of Earth radii radiusequator > radiuspole requator / rpole = 6378/6357 km = flattening of ~1/298 two consequences equator farther from center than poles hence gravity is 6.6 Gals LESS at the equator equator has more mass near it than do the poles hence gravity is 4.8 Gals MORE at the equator result gravity is 1.8 Gals LESS at the equator Earth is a rotating object circumference at equator ~ 40,000 km; at poles 0 km all parts of planet revolve about axis once in 24 hrs hence equator spins at 40,000 =1667 km/hr; at poles 0 km/hr 24 outward centrifugal force at equator; at poles 0 result ....