SIR 2018-5085: Historical Eruptions and Hazards at Bogoslof Volcano
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Railway Employee Records for Colorado Volume Iii
RAILWAY EMPLOYEE RECORDS FOR COLORADO VOLUME III By Gerald E. Sherard (2005) When Denver’s Union Station opened in 1881, it saw 88 trains a day during its gold-rush peak. When passenger trains were a popular way to travel, Union Station regularly saw sixty to eighty daily arrivals and departures and as many as a million passengers a year. Many freight trains also passed through the area. In the early 1900s, there were 2.25 million railroad workers in America. After World War II the popularity and frequency of train travel began to wane. The first railroad line to be completed in Colorado was in 1871 and was the Denver and Rio Grande Railroad line between Denver and Colorado Springs. A question we often hear is: “My father used to work for the railroad. How can I get information on Him?” Most railroad historical societies have no records on employees. Most employment records are owned today by the surviving railroad companies and the Railroad Retirement Board. For example, most such records for the Union Pacific Railroad are in storage in Hutchinson, Kansas salt mines, off limits to all but the lawyers. The Union Pacific currently declines to help with former employee genealogy requests. However, if you are looking for railroad employee records for early Colorado railroads, you may have some success. The Colorado Railroad Museum Library currently has 11,368 employee personnel records. These Colorado employee records are primarily for the following railroads which are not longer operating. Atchison, Topeka & Santa Fe Railroad (AT&SF) Atchison, Topeka and Santa Fe Railroad employee records of employment are recorded in a bound ledger book (record number 736) and box numbers 766 and 1287 for the years 1883 through 1939 for the joint line from Denver to Pueblo. -
Imaginative Geographies of Mars: the Science and Significance of the Red Planet, 1877 - 1910
Copyright by Kristina Maria Doyle Lane 2006 The Dissertation Committee for Kristina Maria Doyle Lane Certifies that this is the approved version of the following dissertation: IMAGINATIVE GEOGRAPHIES OF MARS: THE SCIENCE AND SIGNIFICANCE OF THE RED PLANET, 1877 - 1910 Committee: Ian R. Manners, Supervisor Kelley A. Crews-Meyer Diana K. Davis Roger Hart Steven D. Hoelscher Imaginative Geographies of Mars: The Science and Significance of the Red Planet, 1877 - 1910 by Kristina Maria Doyle Lane, B.A.; M.S.C.R.P. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2006 Dedication This dissertation is dedicated to Magdalena Maria Kost, who probably never would have understood why it had to be written and certainly would not have wanted to read it, but who would have been very proud nonetheless. Acknowledgments This dissertation would have been impossible without the assistance of many extremely capable and accommodating professionals. For patiently guiding me in the early research phases and then responding to countless followup email messages, I would like to thank Antoinette Beiser and Marty Hecht of the Lowell Observatory Library and Archives at Flagstaff. For introducing me to the many treasures held deep underground in our nation’s capital, I would like to thank Pam VanEe and Ed Redmond of the Geography and Map Division of the Library of Congress in Washington, D.C. For welcoming me during two brief but productive visits to the most beautiful library I have seen, I thank Brenda Corbin and Gregory Shelton of the U.S. -
Results of the March 2018 Acoustic-Trawl Survey of Walleye
Alaska Fisheries Science Center National Marine Fisheries Service U.S DEPARTMENT OF COMMERCE AFSC PROCESSED REPORT 2018-07 Results of the March 2018 Acoustic-Trawl Survey of Walleye Pollock (Gadus chalcogrammus) Conducted in the Southeastern Aleutian Basin Near Bogoslof Island, Cruise DY2018-02 December 2018 This report does not constitute a publication and is for information only. All data herein are to be considered provisional. This document should be cited as follows: McKelvey, D., and M. Levine. 2018. Results of the March 2018 acoustic-trawl surve y of walleye pollock (Gadus chalcogrammus) conducted in the Southeastern Aleutian Basin near Bogoslof Island, Cruise DY2018-027. AFSC Processed Rep. 2018-07, 44 p. Alaska Fish. Sci. Cent., NOAA, Natl. Mar. Fish. Serv., 7600 Sand Point Way NE, Seattl e WA 98115. Available at http://www.afsc.noaa.gov/Publications/ProcRpt/PR2018-07.pdf. Reference in this document to trade names does not imply endorsement by the National Marine Fisheries Service, NOAA. Results of the March 2018 Acoustic-Trawl Survey of Walleye Pollock (Gadus chalcogrammus) Conducted in the Southeastern Aleutian Basin Near Bogoslof Island, Cruise DY2018-02 by D. McKelvey and M. Levine December 2018 THIS INFORMATION IS DISTRIBUTED SOLELY FOR THE PURPOSE OF PRE- DISSEMINATION PEER REVIEW UNDER APPLICABLE INFORMATION QUALITY GUIDELINES. IT HAS NOT BEEN FORMALLY DISSEMINATED BY NOAA FISHERIES/ALASKA FISHERIES SCIENCE CENTER AND SHOULD NOT BE CONSTRUED TO REPRESENT ANY AGENCY DETERMINATION OR POLICY ABSTRACT Scientists from the Alaska Fisheries Science Center conducted an acoustic-trawl survey in early March 2018 to estimate the abundance of pre-spawning walleye pollock (Gadus chalcogrammus) in the southeastern Aleutian Basin near Bogoslof Island. -
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. -
Growth of the Northern Fur Seal Colony on Bogoslof Island, Alaska THOMAS R
ARCTIC VOL. 42, NO. 4 (DECEMBER 1989) P. 368-312 Growth of the Northern Fur Seal Colony on Bogoslof Island, Alaska THOMAS R. LOUGHLIN' and R.V. MILLER' (Received 14 March 1989; accepted in revised form 10 May 1989) ABSTRACT. Northern fur seal, Callorhinus ursinus, pups were first observed on Bogoslof Island, southeast Bering Sea, in 1980. By 1988 the population had grown at a rate of 57Vo.yr" to over 400 individuals, including 80+ pups, 159 adult females, 22 territorial males, and 188 subadult males. Some animals originated from rookeries of the CommanderIslands, whereas others are probably from thePribilof Islands. In 1983 and 1985 over 50% of the females were estimated to be > 6 years of age, based on vibrissae color. The rookery is in the same location where solitary male fur seals were seen in 1976 and 1979 and is adjacent to a large northern sea lion rookery. Key words: Bogoslof Island, northern fur seal, Callorhinus ursinus, northern sea lion, breeding colony RBSUMÉ. Des bébés otaries à fourrure, Callorhinus ursinus, ont été observés pour la premiere fois sur Bogoslof Island, au sud-est de la mer de Béring en 1980. En 1988, la population avait augmenté à un tauxde 57 %.an" et dépassait les 400 individus. Parmi eux, on comptait 80 bébés ou plus, 159 femelles adultes, 22 mâles possédant un territoire et 188 jeunes adultes mâles. Certains animaux venaient des colonies des îles du Commandeur, alors que d'autres venaient probablement des îles Pribilof. En 1983 et 1985, on a estimé que plus de 50 To des femelles avaient plus de 6 ans, en se fondant sur lacouleur de leurs vibrisses. -
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. -
Some Alaskan Notes
270 GABRIELSON,SomeAlaskan Notes L[Auk April SOME ALASKAN NOTES BY IRA N. GABRIELSON (Concluded[romp. 150) CALn*ORNIAMumu•, Uria aalgecali[ornica (Bryant).--This was prob- ably the mostabundant species observed on the trip. We did not see California Murres until we reachedSeward (June 10) where there was a large colony associatedwith the still more numerousPacific Kittiwakes.The deepwater at the baseof the cliff allowedus to drift the boat closeand in the clear depthswe could see the birds literally flyingunder the water as expertlyas fishes. Often they came to the surface,saw the boat, and instantly dived again. The great coloniesof the Semidisand Kagamil Island were the largest,composed largely or entirely of this species. In the former island group, wheneverwe approachedthe precipitouscliffs dosely enough to see distinctly,we found every available shelf and nook crowdedwith tourres. At Kagamil Island we traveledin the 'Brown Bear' for at least two miles along cliffs similarly occupied,and the water was covered with birds. These were two of the most impressiveof the bird coloniesseen on the trip. On BogoslofIsland an almostequally large concentra- tion of tourrescontained both this speciesand the next. PALLAS'SMumu•, Uria lornvia arra (Pallas).--Thisnorthern species was first found on BogoslofIsland (June 24). At St. GeorgeIsland (July 8) and St. Paul Island (July 4-6) Pallas's Murre was common,while at Walrus Island (July 7) the enormous murre colony was comprisedlargely, if not entirely, of this species. I saw only one bird there that I thought was a California Murre and it movedaway before I couldbe sure. Pallas'sMurre wasabundant also at St. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
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MacArtney, Adrienne (2018) Atmosphere crust coupling and carbon sequestration on early Mars. PhD thesis. http://theses.gla.ac.uk/9006/ Copyright and moral rights for this work are retained by the author A copy can be downloaded for personal non-commercial research or study, without prior permission or charge This work cannot be reproduced or quoted extensively from without first obtaining permission in writing from the author The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given Enlighten:Theses http://theses.gla.ac.uk/ [email protected] ATMOSPHERE - CRUST COUPLING AND CARBON SEQUESTRATION ON EARLY MARS By Adrienne MacArtney B.Sc. (Honours) Geosciences, Open University, 2013. Submitted in partial fulfilment of the requirements for the degree of Doctor of Philosophy at the UNIVERSITY OF GLASGOW 2018 © Adrienne MacArtney All rights reserved. The author herby grants to the University of Glasgow permission to reproduce and redistribute publicly paper and electronic copies of this thesis document in whole or in any part in any medium now known or hereafter created. Signature of Author: 16th January 2018 Abstract Evidence exists for great volumes of water on early Mars. Liquid surface water requires a much denser atmosphere than modern Mars possesses, probably predominantly composed of CO2. Such significant volumes of CO2 and water in the presence of basalt should have produced vast concentrations of carbonate minerals, yet little carbonate has been discovered thus far. -
In Pdf Format
lós 1877 Mik 88 ge N 18 e N i h 80° 80° 80° ll T 80° re ly a o ndae ma p k Pl m os U has ia n anum Boreu bal e C h o A al m re u c K e o re S O a B Bo l y m p i a U n d Planum Es co e ria a l H y n d s p e U 60° e 60° 60° r b o r e a e 60° l l o C MARS · Korolev a i PHOTOMAP d n a c S Lomono a sov i T a t n M 1:320 000 000 i t V s a Per V s n a s l i l epe a s l i t i t a s B o r e a R u 1 cm = 320 km lkin t i t a s B o r e a a A a A l v s l i F e c b a P u o ss i North a s North s Fo d V s a a F s i e i c a a t ssa l vi o l eo Fo i p l ko R e e r e a o an u s a p t il b s em Stokes M ic s T M T P l Kunowski U 40° on a a 40° 40° a n T 40° e n i O Va a t i a LY VI 19 ll ic KI 76 es a As N M curi N G– ra ras- s Planum Acidalia Colles ier 2 + te . -
Dilemma of Geoconservation of Monogenetic Volcanic Sites Under Fast Urbanization and Infrastructure Developments with Special Re
sustainability Article Dilemma of Geoconservation of Monogenetic Volcanic Sites under Fast Urbanization and Infrastructure Developments with Special Relevance to the Auckland Volcanic Field, New Zealand Károly Németh 1,2,3,* , Ilmars Gravis 3 and Boglárka Németh 1 1 School of Agriculture and Environment, Massey University, Palmerston North 4442, New Zealand; [email protected] 2 Institute of Earth Physics and Space Science, 9400 Sopron, Hungary 3 The Geoconservation Trust Aotearoa, 52 Hukutaia Road, Op¯ otiki¯ 3122, New Zealand; [email protected] * Correspondence: [email protected]; Tel.: +64-27-4791484 Abstract: Geoheritage is an important aspect in developing workable strategies for natural hazard resilience. This is reflected in the UNESCO IGCP Project (# 692. Geoheritage for Geohazard Resilience) that continues to successfully develop global awareness of the multifaced aspects of geoheritage research. Geohazards form a great variety of natural phenomena that should be properly identified, and their importance communicated to all levels of society. This is especially the case in urban areas such as Auckland. The largest socio-economic urban center in New Zealand, Auckland faces potential volcanic hazards as it sits on an active Quaternary monogenetic volcanic field. Individual volcanic geosites of young eruptive products are considered to form the foundation of community Citation: Németh, K.; Gravis, I.; outreach demonstrating causes and consequences of volcanism associated volcanism. However, in Németh, B. Dilemma of recent decades, rapid urban development has increased demand for raw materials and encroached Geoconservation of Monogenetic on natural sites which would be ideal for such outreach. The dramatic loss of volcanic geoheritage Volcanic Sites under Fast of Auckland is alarming. -
Geology of Umnak and Bogoslof Islands Aleutian Islands Alaska
Geology of Umnak and Bogoslof Islands Aleutian Islands Alaska By F. M. BYERS, JR. INVESTIGATIONS OF ^ALASKAN VOLCANOES GEOLOGICAL SURVEY BULLETIN 1028-L Prepared in cooperation with the Office, Chief of Engineers, U.S. Army UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1959 UNITED STATES DEPARTMENT OF THE INTERIOR FRED A. SEATON, Secretary GEOLOGICAL SURVEY Thomas B. Nolan, Director For sale by the Superintendent of Documents, U.S. Government Printing Office Washington 25, D.C. PEEFACE In October 1945 the War Department (now Department of the Army) requested the Geological Survey to undertake a program of volcano investigations in the Aleutian Islands-Alaska Peninsula area. Field studies under general direction of G. D. Robinson, were begun as soon as weather permitted in the spring of 1946. The results of the first year's field, laboratory, and library work were assembled as two administrative reports. Part of the data was published in 1950 in Geological Survey Bulletin 974-B, "Volcanic Activity in the Aleutian Arc", by Robert R. Coats. The rest of the data has been included in Bulletin 1028. The geologic investigations covered by this report were recon naissance. The factual information presented is believed to be accu rate, but many of the tentative interpretations and conclusions will be modified as the investigations continue and knowledge grows. The investigations of 1946 were supported almost entirely by the Military Intelligence Division of the Office, Chief of Engineers, U.S. Army. The Geological Survey is indebted to that Office for its early recognition of the value of geologic studies in the Aleutian region, which made this report possible, and for its continuing support.