Seattle Antiquarian Book Fair – October 2016
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Glacier Point Hiking Trails
Yosemite National Park National Park Service Glacier Point Area Hiking Map U.S. Department of the Interior 2.0 mi (3.2 k To m 3.1 ) Clouds Rest m i (5 3.8 mi .0 0 k . 5.8 km m) 1 7 . Half 1 m cables Dome ) k i km m 8836ft 0.5 .1 (permit mi i (3 2693m required) m 0 1.9 .8 km ) Glacier Point m k r 1 . e 2 v i (7 ( m .7 i 8 km i Bunnell 4. ) R m d Point 3 For Yosemite Valley trails and information, Four Mile . e 1 c r Trailhead ) e at Road km M Fl please see the Yosemite Valley Hiking Map ) 0.8 k 7214ft Happy Isles km 6.7 mi (1 a .6 O 2199m Trailhead (1 mi g 1 0 i .0 Vernal Fall 1. B m 1 i .6 k Little Yosemite Valley ) m km 6100ft 9 0.4 mi 3. Nevada Fall 1859m ( ) 120 i 0.6 km Sentinel m Road Trail m 1 k ) . m 4 k Crane Flat . Dome 4 .2 1.0 mi 4 4 2 ( . Wawona Tunnel 8122ft m i Bridalveil Fall 1 m 1.6 km ( i Tunnel 6 2476m i ( . Parking Area Ranger Station 2 2 m View . d Washburn 3 9 a . k 0.7 mi 0 Point m o Inspiration 1.1 km Telephone Campground Taft Point ) R Point 7503ft l Illilouette Fall 3 Illilouette Ridge a .7 m 2287m Store Restrooms t i (6 r .0 1.1 mi (1.8 km) o k Sentinel Dome r ) m Stanford m P k e ) & Taft Point 2 Point 0 . -
YOSEMITE NATIONAL PARK O C Y Lu H M Tioga Pass Entrance 9945Ft C Glen Aulin K T Ne Ee 3031M E R Hetc C Gaylor Lakes R H H Tioga Road Closed
123456789 il 395 ra T Dorothy Lake t s A Bond C re A Pass S KE LA c i f i c IN a TW P Tower Peak Barney STANISLAUS NATIONAL FOREST Mary Lake Lake Buckeye Pass Twin Lakes 9572ft EMIGRANT WILDERNESS 2917m k H e O e O r N V C O E Y R TOIYABE NATIONAL FOREST N Peeler B A Lake Crown B C Lake Haystack k Peak e e S Tilden r AW W Schofield C TO Rock Island OTH IL Peak Lake RI Pass DG D Styx E ER s Matterhorn Pass l l Peak N a Slide E Otter F a Mountain S Lake ri e S h Burro c D n Pass Many Island Richardson Peak a L Lake 9877ft R (summer only) IE 3010m F LE Whorl Wilma Lake k B Mountain e B e r U N Virginia Pass C T O Virginia S Y N Peak O N Y A Summit s N e k C k Lake k c A e a C i C e L C r N r Kibbie d YO N C n N CA Lake e ACK AI RRICK K J M KE ia in g IN ir A r V T e l N k l U e e pi N O r C S O M Y Lundy Lake L Piute Mountain N L te I 10541ft iu A T P L C I 3213m T Smedberg k (summer only) Lake e k re e C re Benson Benson C ek re Lake Lake Pass C Vernon Creek Mount k r e o Gibson e abe Upper an r Volunteer McC le Laurel C McCabe E Peak rn Lake u Lake N t M e cCa R R be D R A Lak D NO k Rodgers O I es e PLEASANT EA H N EL e Lake I r l Frog VALLEY R i E k G K C E LA e R a e T I r r Table Lake V North Peak T T C N Pettit Peak A INYO NATIONAL FOREST O 10788ft s Y 3288m M t ll N Fa s Roosevelt ia A e Mount Conness TILT r r Lake Saddlebag ILL VALLEY e C 12590ft (summer only) h C Lake ill c 3837m Lake Eleanor ilt n Wapama Falls T a (summer only) N S R I Virginia c A R i T Lake f N E i MIGUEL U G c HETCHY Rancheria Falls O N Highway 120 D a MEADOW -
Investigating Mineral Stability Under Venus Conditions: a Focus on the Venus Radar Anomalies Erika Kohler University of Arkansas, Fayetteville
University of Arkansas, Fayetteville ScholarWorks@UARK Theses and Dissertations 5-2016 Investigating Mineral Stability under Venus Conditions: A Focus on the Venus Radar Anomalies Erika Kohler University of Arkansas, Fayetteville Follow this and additional works at: http://scholarworks.uark.edu/etd Part of the Geochemistry Commons, Mineral Physics Commons, and the The unS and the Solar System Commons Recommended Citation Kohler, Erika, "Investigating Mineral Stability under Venus Conditions: A Focus on the Venus Radar Anomalies" (2016). Theses and Dissertations. 1473. http://scholarworks.uark.edu/etd/1473 This Dissertation is brought to you for free and open access by ScholarWorks@UARK. It has been accepted for inclusion in Theses and Dissertations by an authorized administrator of ScholarWorks@UARK. For more information, please contact [email protected], [email protected]. Investigating Mineral Stability under Venus Conditions: A Focus on the Venus Radar Anomalies A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Space and Planetary Sciences by Erika Kohler University of Oklahoma Bachelors of Science in Meteorology, 2010 May 2016 University of Arkansas This dissertation is approved for recommendation to the Graduate Council. ____________________________ Dr. Claud H. Sandberg Lacy Dissertation Director Committee Co-Chair ____________________________ ___________________________ Dr. Vincent Chevrier Dr. Larry Roe Committee Co-chair Committee Member ____________________________ ___________________________ Dr. John Dixon Dr. Richard Ulrich Committee Member Committee Member Abstract Radar studies of the surface of Venus have identified regions with high radar reflectivity concentrated in the Venusian highlands: between 2.5 and 4.75 km above a planetary radius of 6051 km, though it varies with latitude. -
Cleopatra Crater on Venus: Happy Solution of the Volcanic Vs
CLEOPATRA CRATER ON VENUS: HAPPY SOLUTION OF THE VOLCANIC VS. IMPACT CRATER CONTROVERSY; A.T. Basilevsky, A.T. Vernadsky Institute of Geochemistry and Analytical chemistry, Moscow, USSR, and G.G. Schaber, U.S. Geological Survey, Flagstaff AZ 86001 ~ntroduction. Cleopatra is a 100-km-diameter crater on the eastern slope of Maxwell Montes in western Ishtar Terra. For over 12 years, Cleopatra has been the subject of scientific controversy. Discovered during the Pioneer Venus altimetric survey, this feature was initially interpreted as a caldera near the top of a giant volcanic construct, Maxwell Montes [I]. Venera 15/16 data and recent Arecibo radar images show, however, that the Maxwell Montes appear to be more of a tectonic construct, with little or no resemblance to other giant shields known in the Solar System; thus, a nonvolcanic origin of Cleopatra was proposed [2-61. The similarity of the double-ring structure of Cleopatra to those of other multi-ring impact craters of similar size on Venus and the Moon, Mercury, and Mars was more recently given by Basilevsky and Ivanov [7] as the primarily reason to consider this feature an impact crater. At the same time, some characteristics of Cleopatra seemed to contradict an impact origin. For example, Schaber et al. [8], suggestingthat a definitive verification of a volcanic or impact origin would probably require Magellan data, proposed that the evidence from Venera 15/16 and earlier data for a probable volcanic origin for Cleopatra is substantial. They cited, among other points: (1) the absence of a raised rim and highly backscattering ejecta deposits; (2) the crater's association with plains-forming deposits immediately downslope to the east, interpreted as probable lava flows emanating from a distinct breach in the crater's rim; (3) the excessive depth (2.5 km) and depth-to-diameter ratio (0.028) of the crater, (4) the offset of the inner and outer craters; and (5) the crater's position in what was interpreted as a regional tectonic framework. -
Styles of Deformation in Ishtar Terra and Their Implications
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 97, NO. El0, PAGES 16,085-16,120, OCTOBER 25, 1992 Stylesof Deformationin IshtarTerra and Their Implications Wn.T.TAMM. KAU•A,• DOAN•L. BINDSCHAD•-R,l ROBERT E. GPaM•,2'3 VICKIL. HANSEN,2KARl M. ROBERTS,4AND SUZANNE E. SMREr,AR s IshtarTerra, the highest region on Venus, appears to havecharacteristics of both plume uplifts and convergent belts.Magellan imagery over longitudes 330ø-30øE indicates a great variety of tectonicand volcanic activity, with largevariations within distances of onlya few 100km. Themost prominent terrain types are the volcanic plains of Lakshmiand the mountain belts of Maxwell,Freyja, and Danu. Thebelts appear to havemarked variations in age. Thereare also extensive regions of tesserain boththe upland and outboard plateaus, some rather featureless smoothscarps, flanking basins of complexextensional tectonics, and regions of gravitationalor impactmodifica- tion.Parts of Ishtarare the locations of contemporaryvigorous tectonics and past extensive volcanism. Ishtar appearsto be the consequence of a history of several100 m.y., in whichthere have been marked changes in kinematic patternsand in whichactivity at any stage has been strongly influenced by the past. Ishtar demonstrates three general propertiesof Venus:(1) erosionaldegradation is absent,leading to preservationof patternsresulting from past activity;(2) manysurface features are the responses ofa competentlayer less than 10 km thick to flowsof 100km orbroaderscale; and (3) thesebroader scale flows are controlled mainly by heterogeneities inthe mantle. Ishtar Terra doesnot appear to bethe result of a compressionconveyed by anEarthlike lithosphere. But there is stilldoubt as to whetherIshtar is predominantlythe consequence of a mantleupflow or downflow.Upflow is favoredby the extensivevolcanic plain of Lakshmiand the high geoid: topography ratio; downflow is favoredby the intense deformationof themountain belts and the absence of majorrifts. -
! Letter-Triersto Be Appointed by the Special Agents Of
.haM and repair 'of workm«n's~toola 9j the act to amend the third section of the^JU* makingI them from Florid* to the country wast ! By the «ct for the compenaation of Jama W. Low tad the Indian*, of Psducah, in Kentucky ; is Louisiana aaii of of the Wyandot being appointed Shreveport ; pcj'v* of public letter*, ftial, oil and appropriation* for the oiTil and diplomatic mpnm* J Arkansas 444 00 j others, for the culture of the British private-armed commissioner for the purpoeat aforesaid Jeffersonrille. in the State of Indian*, to recurs ths ml- . eandlee for narv-yardi and ihore Ita* government for the year ending the thirtieth of Jane, [ By the act for the relief of Passed Midshipmen George P.' schooner Ann, during the late war with Great Britain, by the Secretary of War on the nine¬ anr and emolument# prescribed by the act of Congrem ap. tiona pay of watchmen, and incidental eighteen hundred and fifty-four? and for other purpoev. ] Welsh and Clark H. Well*. j For the amount into the of teenth of April, eighteen hundred and proved the 2d March, 1831. lahor, not chargeable to any other appro¬ to paid Treasury of for the increased compensation the To paj to Passed the United States, and placed to the ao- thirty-six. [Indefinite.] By the act (chap. 193) creating a collection district i& priation. labor attending the delivery ana other employees Midshipman dount of and forfeitures, the act for the relief of the heirs of G. Willi*. Texas and New Mexico. stores on civil dock- clerka, meseengera, George P. -
The Hundredth Book
THE HUNDREDTH A BIBLIOGRAPHY OF THE PUBLICATIONS OF THE BOOK CLUB OF CALIFORNIA & A HISTORY OF THE CLUB BY DAVID MAGEE 1958 PRINTED AT THE GRABHORN PRESS FOR THE BOOK CLUB OF CALIFORNIA CONTENTS PREFATORY NOTE page v A HISTORY OF THE BOOK CLUB OF CALIFORNIA page vii OFFICERS OF THE CLUB page xxv THE HUNDRED BOOKS page 1 ANNUAL KEEPSAKES page 55 MISCELLANEOUS KEEPSAKES page 71 QUARTERLY NEWS-LETTER page 74 INDEX page 75 copyright 1958 by the book club of california PREFATORY NOTE IBLIOGRAPHIES are seldom solo performances. A man’s name may appear on a title-page, but that tells only one half of the story. It is the purpose of this prefatory note to tell the other half. When I agreed to compile a bibliography of The Book Club of California publications, with an accompanying history of the Club, I thought I was in for a fairly easy job. I understood that the archives were in existence and, of course, on the shelves at headquarters were complete files of Club books, keepsakes, Quarterly News-Letters, etc. It should be simple, merely a matter of collating and checking and trying to make of a bibliography something more than a catalogue of titles. How wrong can a person be? To begin with, it must be understood that for many years the Club was run by amateurs, devoted, splendid citizens who attended monthly board meetings and when it was necessary gave generously of their time and energies for the welfare of the Club. But they were still amateurs, and so long as the organization was not in danger of collapse or actual decease they were content to let things jog along. -
BEDROCK GEOLOGY of the YOSEMITE VALLEY AREA YOSEMITE NATIONAL PARK, CALIFORNIA Prepared by N
DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP I-1639 U.S. GEOLOGICAL SURVEY BEDROCK GEOLOGY OF THE YOSEMITE VALLEY AREA YOSEMITE NATIONAL PARK, CALIFORNIA Prepared by N. King Huber and Julie A. Roller From the writings of Frank C. Calkins and other sources PREFACE INTRODUCTION Frank Calkins' work in Yosemite was preceded by Yosemite Valley, one of the world's great natural works Henry W. Turner, also of the U.S. Geological Survey, of rock sculpture, is carved into the west slope of the who began mapping the Yosemite and Mount Lyell 30- Sierra Nevada. Immense cliffs, domes, and waterfalls minute quadrangles in 1897 and laid the foundation that tower over forest, meadows, and a meandering river, Calkins' work was built on. Although Turner never creating one of the most scenic natural landscapes in completed this sizable assignment, he recognized the North America (fig. 1). In Yosemite Valley and the differing types of plutonic rocks and, for example, named adjoining uplands, the forces of erosion have exposed, the El Capitan Granite. with exceptional clarity, a highly complex assemblage of Calkins mapped the valley and adjacent areas of granitic rocks. The accompanying geologic map shows the Yosemite National Park during the period 1913 through distribution of some of the different rocks that make up 1916, at the same time that Francois Matthes was this assemblage. This pamphlet briefly describes those studying the glacial geology of Yosemite. Calkins rocks and discusses how they differ, both in composition summarized the bedrock geology of part of Yosemite in and structure, and the role they played in the evolution the appendix of Matthes' classic volume "Geologic History of the valley. -
Glacier Point Area Hiking Map U.S
Yosemite National Park National Park Service Glacier Point Area Hiking Map U.S. Department of the Interior 2.0 mi (3.2 k To m 3.1 ) Clouds Rest m i (5 3.8 mi .0 0 k . 5.8 km m) 1 7 . Half 1 m cables Dome ) k i km m 8836ft 0.5 .1 (permit mi i (3 2693m required) m 0 1.9 .8 km ) Glacier Point m For Yosemite Valley trails and information, k r 1 . e 2 v i (7 ( m .7 i 8 km i Bunnell please see the Yosemite Valley Hiking Map. 4. ) R m d Point 3 Four Mile . e 1 c r Trailhead ) e at Road km M Fl ) 0.8 k 7214ft Happy Isles km 6.7 mi (1 a .6 O 2199m Trailhead (1 mi g 1 0 i .0 Vernal Fall 1. B Roosevelt m 1 i Point .6 k Little Yosemite Valley 7380ft m 2250m 6100ft Nevada Fall 0.4 mi 1859m 120 ) 0.6 km Sentinel m Road Trail 1 k ) . m k Crane Flat Dome 4 .2 1.0 mi 4 (4 . Wawona Tunnel 8122ft m i Bridalveil Fall 1 m 1.6 km ( i Tunnel 6 2476m i ( . Parking Area Ranger Station 2 2 m View . d Washburn 3 9 a . k 0.7 mi 0 Point m o Inspiration km) (3.9 mi 2.4 1.1 km Telephone Campground Taft Point ) R Point 7503ft l Illilouette Fall 3 Illilouette Ridge a .7 m 2287m Store Restrooms t i (6 r .0 1.1 mi (1.8 km) o k Sentinel Dome r ) m Stanford m P k e ) & Taft Point 2 Point 0 . -
A Brief History of the Hawaiian People
0 A BRIEF HISTORY OP 'Ill& HAWAIIAN PEOPLE ff W. D. ALEXANDER PUBLISHED BY ORDER OF THE BOARD OF EDUCATION OF THE HAWAIIAN KINGDOM NEW YORK,: . CINCINNATI•:• CHICAGO AMERICAN BOOK C.OMPANY Digitized by Google ' .. HARVARD COLLEGELIBRAllY BEQUESTOF RCLANOBUr.ll,' , ,E DIXOII f,'.AY 19, 1936 0oPYBIGRT, 1891, BY AlilBIOAN BooK Co)[PA.NY. W. P. 2 1 Digit zed by Google \ PREFACE AT the request of the Board of Education, I have .fi. endeavored to write a simple and concise history of the Hawaiian people, which, it is hoped, may be useful to the teachers and higher classes in our schools. As there is, however, no book in existence that covers the whole ground, and as the earlier histories are entirely out of print, it has been deemed best to prepare not merely a school-book, but a history for the benefit of the general public. This book has been written in the intervals of a labo rious occupation, from the stand-point of a patriotic Hawaiian, for the young people of this country rather than for foreign readers. This fact will account for its local coloring, and for the prominence given to certain topics of local interest. Especial pains have been taken to supply the want of a correct account of the ancient civil polity and religion of the Hawaiian race. This history is not merely a compilation. It is based upon a careful study of the original authorities, the writer having had the use of the principal existing collections of Hawaiian manuscripts, and having examined the early archives of the government, as well as nearly all the existing materials in print. -
Size, Scale and the Imaginary in the Work of Land Artists Michael Heizer, Walter De Maria and Dennis Oppenheim
Larger than life: size, scale and the imaginary in the work of Land Artists Michael Heizer, Walter De Maria and Dennis Oppenheim © Michael Albert Hedger A thesis in fulfillment of the requirements for the degree of Doctor of Philosophy Art History and Art Education UNIVERSITY OF NEW SOUTH WALES | Art & Design August 2014 PLEASE TYPE THE UNIVERSITY OF NEW SOUTH WALES Thesis/Dissertation Sheet Surname or Family name: Hedger First name: Michael Other name/s: Albert Abbreviation for degree as given in the University calendar: Ph.D. School: Art History and Education Faculty: Art & Design Title: Larger than life: size, scale and the imaginary in the work of Land Artists Michael Heizer, Walter De Maria and Dennis Oppenheim Abstract 350 words maximum: (PLEASE TYPE) Conventionally understood to be gigantic interventions in remote sites such as the deserts of Utah and Nevada, and packed with characteristics of "romance", "adventure" and "masculinity", Land Art (as this thesis shows) is a far more nuanced phenomenon. Through an examination of the work of three seminal artists: Michael Heizer (b. 1944), Dennis Oppenheim (1938-2011) and Walter De Maria (1935-2013), the thesis argues for an expanded reading of Land Art; one that recognizes the significance of size and scale but which takes a new view of these essential elements. This is achieved first by the introduction of the "imaginary" into the discourse on Land Art through two major literary texts, Swift's Gulliver's Travels (1726) and Shelley's sonnet Ozymandias (1818)- works that, in addition to size and scale, negotiate presence and absence, the whimsical and fantastic, longevity and death, in ways that strongly resonate with Heizer, De Maria and especially Oppenheim. -
Melville's Copy of Thomas Beale's the Natural History of the Sperm
Melville’s copy of Thomas Beale’s "The natural history of the sperm whale and the composition of Moby-Dick" The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Olsen-Smith, Steven. 2011. Melville’s copy of Thomas Beale’s "The natural history of the sperm whale and the composition of Moby- Dick". Harvard Library Bulletin 21 (3): 1-78. Citable link https://nrs.harvard.edu/URN-3:HUL.INSTREPOS:37363364 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Other Posted Material, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#LAA Melville’s Copy of Tomas Beale’s Te Natural History of the Sperm Whale and the Composition of Moby-Dick Steven Olsen-Smith erman Melville’s copy of Thomas Beale’s Te Natural History of the Sperm Whale, discovered in the 1930s and then owned by successive Hprivate collectors until Houghton Library acquired it in 1960, contains the closest evidence available to the lost manuscript of Moby-Dick and illuminates more fully than any other archival resource Melville’s use of source materials in his writing. Howard P. Vincent frst consulted Melville’s copy for Te Trying-out of Moby-Dick (1949), where he observed that most of Melville’s marginalia had been erased from the book. Judging “not many words were erased,” Vincent expressed hope for “a future examination of the markings under infra-red rays.”1 But in Melville’s Marginalia, Walker Cowen deciphered many of Melville’s erased markings without technical assistance, and although he did not recover many of Melville’s erased words, Cowen showed that the book had once been heavily annotated.2 With fnancial support from the William Reese Company and Boise State University, technical assistance at the Fogg Art Museum, and support from staf at Houghton Library, I worked collaboratively with Dennis C.