Cordilleran Section Meeting for the First Time in (HNL)
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Andinismo: Desafío Para La Prensa Nacional Memoria Para Optar Al Título De Periodista
UNIVERSIDAD NACIONAL 11111111111111�ñi�íll1i1i1l1lm1111111111111 35612000064981. UNIVERSIDADa ANDRES BELLO UNIVERSIDAD ANDRÉS BELLO FACULTAD DE HUMANIDADES Y EDUCACIÓN ESCUELA DE PERIODISMO ANDINISMO: DESAFÍO PARA LA PRENSA NACIONAL MEMORIA PARA OPTAR AL TÍTULO DE PERIODISTA ALUMNO: CARLA BERTOSSI ARRIBADA PROFESOR GUÍA: SEBASTIANO BERTOLONE GALLETINI SANTIAGO - CHILE Noviembre, 2004 ÍNDICE Justificacióndel Tema ............................................................................................ 2 ANDINISMO: DESAFÍO PARA LA PRENSA NACIONAL ............................................ 4 Introducción............... ......................................................................................... 5 Capítulo I CARACTERÍSTICAS FÍSICAS DE LOS ANDES ......................................................... 8 1. Geografia de Los Andes 2. El ambientede montaña 3. Cumbres emblemáticas Capítulo II MONTAÑAS, TEMPLO DEL DEPORTE.................................................................. 29 l. Breve historia del andinismo 2. El deporte de montaña 3. Andinismo 4. Organización del andinismo en Chile Capítulo m TÉCNICA Y SEGURIDAD EN MONTAÑA.............................................................. 50 l. Peligros en montaña 2. Vestuarioy equipo de montaña 3. Alimentación 4. Orientación Capítulo IV FISIOLOGÍA DE MONTAÑA ................................................................................ 69 1. Patología de la altitud 2. Aclimatización 3. Otraspatologías 4. Primeros auxilios 5. Aspectos psicológicos Capítulo V ACCIDENTES -
Geologic Map of the Long Valley Caldera, Mono-Inyo Craters
DEPARTMENT OF THE INTERIOR TO ACCOMPANY MAP 1-1933 US. GEOLOGICAL SURVEY GEOLOGIC MAP OF LONG VALLEY CALDERA, MONO-INYO CRATERS VOLCANIC CHAIN, AND VICINITY, EASTERN CALIFORNIA By Roy A. Bailey GEOLOGIC SETTING VOLCANISM Long Valley caldera and the Mono-Inyo Craters Long Valley caldera volcanic chain compose a late Tertiary to Quaternary Volcanism in the Long Valley area (Bailey and others, volcanic complex on the west edge of the Basin and 1976; Bailey, 1982b) began about 3.6 Ma with Range Province at the base of the Sierra Nevada frontal widespread eruption of trachybasaltic-trachyandesitic fault escarpment. The caldera, an east-west-elongate, lavas on a moderately well dissected upland surface oval depression 17 by 32 km, is located just northwest (Huber, 1981).Erosional remnants of these mafic lavas of the northern end of the Owens Valley rift and forms are scattered over a 4,000-km2 area extending from the a reentrant or offset in the Sierran escarpment, Adobe Hills (5-10 km notheast of the map area), commonly referred to as the "Mammoth embayment.'? around the periphery of Long Valley caldera, and The Mono-Inyo Craters volcanic chain forms a north- southwestward into the High Sierra. Although these trending zone of volcanic vents extending 45 km from lavas never formed a continuous cover over this region, the west moat of the caldera to Mono Lake. The their wide distribution suggests an extensive mantle prevolcanic basement in the area is mainly Mesozoic source for these initial mafic eruptions. Between 3.0 granitic rock of the Sierra Nevada batholith and and 2.5 Ma quartz-latite domes and flows erupted near Paleozoic metasedimentary and Mesozoic metavolcanic the north and northwest rims of the present caldera, at rocks of the Mount Morrisen, Gull Lake, and Ritter and near Bald Mountain and on San Joaquin Ridge Range roof pendants (map A). -
General Vertical Files Anderson Reading Room Center for Southwest Research Zimmerman Library
“A” – biographical Abiquiu, NM GUIDE TO THE GENERAL VERTICAL FILES ANDERSON READING ROOM CENTER FOR SOUTHWEST RESEARCH ZIMMERMAN LIBRARY (See UNM Archives Vertical Files http://rmoa.unm.edu/docviewer.php?docId=nmuunmverticalfiles.xml) FOLDER HEADINGS “A” – biographical Alpha folders contain clippings about various misc. individuals, artists, writers, etc, whose names begin with “A.” Alpha folders exist for most letters of the alphabet. Abbey, Edward – author Abeita, Jim – artist – Navajo Abell, Bertha M. – first Anglo born near Albuquerque Abeyta / Abeita – biographical information of people with this surname Abeyta, Tony – painter - Navajo Abiquiu, NM – General – Catholic – Christ in the Desert Monastery – Dam and Reservoir Abo Pass - history. See also Salinas National Monument Abousleman – biographical information of people with this surname Afghanistan War – NM – See also Iraq War Abousleman – biographical information of people with this surname Abrams, Jonathan – art collector Abreu, Margaret Silva – author: Hispanic, folklore, foods Abruzzo, Ben – balloonist. See also Ballooning, Albuquerque Balloon Fiesta Acequias – ditches (canoas, ground wáter, surface wáter, puming, water rights (See also Land Grants; Rio Grande Valley; Water; and Santa Fe - Acequia Madre) Acequias – Albuquerque, map 2005-2006 – ditch system in city Acequias – Colorado (San Luis) Ackerman, Mae N. – Masonic leader Acoma Pueblo - Sky City. See also Indian gaming. See also Pueblos – General; and Onate, Juan de Acuff, Mark – newspaper editor – NM Independent and -
Recent Deformation Around Domuyo Volcano, Argentina Inferred from Time-Series Analyses of Insar Image
SVC45-22 JpGU-AGU Joint Meeting 2020 Recent Deformation around Domuyo Volcano, Argentina Inferred from Time-series Analyses of InSAR Image *Satoshi Miura1, Micaela Colavita1, Yu Morishita2 1. Graduate School of Science, Tohoku University, 2. Geospatial Information Authority of Japan Domuyo volcano, located in the southern Central Andes of Argentina (36°37’S-70°26’W), is a Plio-Pleistocene dome complex hosting at least 14 dacitic lava domes (https://volcano.si.edu/ volcano.cfm?vn=357067) and other monogenetic basaltic centers (Astort et al., 2019). It occupies a retroarc position and can be found in the northernmost region of Cordillera del Viento (36°35’ to 36° 45’S), a N-S trending basement block crossed and rise by the Cortaderas lineament which is believed to exert a major structural control for the Neogene-to-Quaternary tectonic processes of the area (Galleto et al., 2018). With a height of 4,702 m the volcano constitutes the highest mountain in the Argentinian Patagonia and is related to an intense geothermal activity field that has been described as a fault controlled system associate with graben-like structures and shoshonitic volcanism developed under extensional regime during the Quaternary (Galleto et al., 2018). Without any historical eruption recorded this volcano was considered dormant, but the recent geophysical analysis has demonstrated unrest ongoing at the volcano. According to Astort et al. (2019), it has been growing at a rate of 12 cm/yr, calculated from the InSAR data. Along with seismic, gravimetric and morphometric data, they studied the deformation around the volcano using Sentinel-1 InSAR images from both ascending and descending orbits, within the 2014-2018 period of time. -
Bailey-1976.Pdf
VOL. 81, NO. 5 JOURNAL OF GEOPHYSICAL RESEARCH FEBRUARY 10, 1976 Volcanism, Structure,and Geochronologyof Long Valley Caldera, Mono County, California RoY A. BAILEY U.S. GeologicalSurvey, Reston, Virginia 22092 G. BRENT DALRYMPLE AND MARVIN A. LANPHERE U.S. GeologicalSurvey, Menlo Park, California 94025 Long Valley caldera, a 17- by 32-km elliptical depressionon the east front of the Sierra Nevada, formed 0.7 m.y. ago during eruption of the Bishoptuff. Subsequentintracaldera volcanism included eruption of (1) aphyric rhyolite 0.68-0.64 m.y. ago during resurgentdoming of the caldera floor, (2) porphyritic hornblende-biotiterhyolite from centersperipheral to the resurgentdome at 0.5, 0.3, and 0.1 m.y. ago, and (3) porphyritic hornblende-biotiterhyodacite from outer ring fractures0.2 m.y. ago to 50,000 yr ago, a sequencethat apparently records progressivecrystallization of a subjacentchemically zoned magma chamber. Holocene rhyolitic and phreatic eruptions suggestthat residual magma was present in the chamber as recentlyas 450 yr ago. Intracaldera hydrothermalactivity beganat least0.3 m.y. ago and was widespreadin the caldera moat; it has sincedeclined due to self-sealingof near-surfacecaldera sediments by zeolitization, argillization, and silicificationand has becomelocalized on recentlyreactivated north- west-trendingSierra Nevada frontal faults that tap hot water at depth. INTRODUCTION concentrates were treated with a dilute HF solution to remove small bits of attached glassand fragments of other mineral In the westernUnited States,only three calderasare known grains. Obsidian used for dating was totally unhydrated and to be large enoughand young enoughto possiblystill contain not devitrified. Small blocks sawed from many of the hand residual magma in their chambers:the Vailes caldera (•1.1 specimenswere used for dating. -
100M Dash (5A Girls) All Times Are FAT, Except
100m Dash (5A Girls) All times are FAT, except 2 0 2 1 R A N K I N G S A L L - T I M E T O P - 1 0 P E R F O R M A N C E S 1 12 Nerissa Thompson 12.35 North Salem 1 Margaret Johnson-Bailes 11.30a Churchill 1968 2 12 Emily Stefan 12.37 West Albany 2 Kellie Schueler 11.74a Summit 2009 3 9 Kensey Gault 12.45 Ridgeview 3 Jestena Mattson 11.86a Hood River Valley 2015 4 12 Cyan Kelso-Reynolds 12.45 Springfield 4 LeReina Woods 11.90a Corvallis 1989 5 10 Madelynn Fuentes 12.78 Crook County 5 Nyema Sims 11.95a Jefferson 2006 6 10 Jordan Koskondy 12.82 North Salem 6 Freda Walker 12.04c Jefferson 1978 7 11 Sydney Soskis 12.85 Corvallis 7 Maya Hopwood 12.05a Bend 2018 8 12 Savannah Moore 12.89 St Helens 8 Lanette Byrd 12.14c Jefferson 1984 9 11 Makenna Maldonado 13.03 Eagle Point Julie Hardin 12.14c Churchill 1983 10 10 Breanna Raven 13.04 Thurston Denise Carter 12.14c Corvallis 1979 11 9 Alice Davidson 13.05 Scappoose Nancy Sim 12.14c Corvallis 1979 12 12 Jada Foster 13.05 Crescent Valley Lorin Barnes 12.14c Marshall 1978 13 11 Tori Houg 13.06 Willamette Wind-Aided 14 9 Jasmine McIntosh 13.08 La Salle Prep Kellie Schueler 11.68aw Summit 2009 15 12 Emily Adams 13.09 The Dalles Maya Hopwood 12.03aw Bend 2016 16 9 Alyse Fountain 13.12 Lebanon 17 11 Monica Kloess 13.14 West Albany C L A S S R E C O R D S 18 12 Molly Jenne 13.14 La Salle Prep 9th Kellie Schueler 12.12a Summit 2007 19 9 Ava Marshall 13.16 South Albany 10th Kellie Schueler 12.01a Summit 2008 20 11 Mariana Lomonaco 13.19 Crescent Valley 11th Margaret Johnson-Bailes 11.30a Churchill 1968 -
PDF Program Book
46th Meeting of the Division for Planetary Sciences with Historical Astronomy Division (HAD) 9-14 November 2014 | Tucson, AZ OFFICERS AND MEMBERS ........ 2 SPONSORS ............................... 2 EXHIBITORS .............................. 3 FLOOR PLANS ........................... 5 ATTENDEE SERVICES ................. 8 Session Numbering Key SCHEDULE AT-A-GLANCE ........ 10 100s Monday 200s Tuesday SUNDAY ................................. 20 300s Wednesday 400s Thursday MONDAY ................................ 23 500s Friday TUESDAY ................................ 44 Sessions are numbered in the program book by day and time. WEDNESDAY .......................... 75 All posters will be on display Monday - Friday THURSDAY.............................. 85 FRIDAY ................................. 119 Changes after 1 October are included only in the online program materials. AUTHORS INDEX .................. 137 1 DPS OFFICERS AND MEMBERS Current DPS Officers Heidi Hammel Chair Bonnie Buratti Vice-Chair Athena Coustenis Secretary Andrew Rivkin Treasurer Nick Schneider Education and Public Outreach Officer Vishnu Reddy Press Officer Current DPS Committee Members Rosaly Lopes Term Expires November 2014 Robert Pappalardo Term Expires November 2014 Ralph McNutt Term Expires November 2014 Ross Beyer Term Expires November 2015 Paul Withers Term Expires November 2015 Julie Castillo-Rogez Term Expires October 2016 Jani Radebaugh Term Expires October 2016 SPONSORS 2 EXHIBITORS Platinum Exhibitor Silver Exhibitors 3 EXHIBIT BOOTH ASSIGNMENTS 206 Applied -
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014
Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ 2014 Edited by: James A. Skinner, Jr. U. S. Geological Survey, Flagstaff, AZ David Williams Arizona State University, Tempe, AZ NOTE: Abstracts in this volume can be cited using the following format: Graupner, M. and Hansen, V.L., 2014, Structural and Geologic Mapping of Tellus Region, Venus, in Skinner, J. A., Jr. and Williams, D. A., eds., Abstracts of the Annual Meeting of Planetary Geologic Mappers, Flagstaff, AZ, June 23-25, 2014. SCHEDULE OF EVENTS Monday, June 23– Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up – 2255 N. Gemini Drive (USGS) 9:00 Welcome/Logistics 9:10 NASA HQ and Program Remarks (M. Kelley) 9:30 USGS Map Coordinator Remarks (J. Skinner) 9:45 GIS and Web Updates (C. Fortezzo) 10:00 RPIF Updates (J. Hagerty) 10:15 BREAK / POSTERS 10:40 Venus Irnini Mons (D. Buczkowski) 11:00 Moon Lunar South Pole (S. Mest) 11:20 Moon Copernicus Quad (J. Hagerty) 11:40 Vesta Iterative Geologic Mapping (A. Yingst) 12:00 pm LUNCH / POSTERS 1:30 Vesta Proposed Time-Stratigraphy (D. Williams) 1:50 Mars Global Geology (J. Skinner) 2:10 Mars Terra Sirenum (R. Anderson) 2:30 Mars Arsia/Pavonis Montes (B. Garry) 2:50 Mars Valles Marineris (C. Fortezzo) 3:10 BREAK / POSTERS 3:30 Mars Candor Chasma (C. Okubo) 3:50 Mars Hrad Vallis (P. Mouginis-Mark) 4:10 Mars S. Margaritifer Terra (J. Grant) 4:30 Mars Ladon basin (C. Weitz) 4:50 DISCUSSION / POSTERS ~5:15 ADJOURN Tuesday, June 24 - Planetary Geologic Mappers Meeting Time Planet/Body Topic 8:30 am Arrive/Set-up/Logistics 9:00 Mars Upper Dao and Niger Valles (S. -
Possible Sub-Glacial Eruptions in the Galaxias Quadrangle, Mars ⇑ Peter J
Icarus 267 (2016) 68–85 Contents lists available at ScienceDirect Icarus journal homepage: www.journals.elsevier.com/icarus Possible sub-glacial eruptions in the Galaxias Quadrangle, Mars ⇑ Peter J. Mouginis-Mark a, , Lionel Wilson a,b a Hawaii Institute Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, USA b Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, England, United Kingdom article info abstract Article history: We have identified several landforms in the Galaxias Quadrangle of Mars (MTM 35217), 33.0–35.5°N, Received 28 July 2015 216.0–218.0°W which are consistent with this area having been covered by an ancient ice sheet concur- Revised 17 November 2015 rent with volcanic eruptions. Volcanic activity was initiated by the intrusion of several large dikes mea- Accepted 21 November 2015 suring 50–100 m wide and protruding up to 35 m above the present-day surface. These dikes appear Available online 14 December 2015 to have originated from Elysium Planitia 600 km to the SE. In one instance, a dike (at an elevation of À3750 m) appears to have produced a subglacial mound (referred to here as ‘‘Galaxias Mons 2”) that Keywords: evolved into an extrusive eruption and produced copious volumes of melt water that carved an outflow Mars, surface channel that extends almost 300 km to the north. At a lower elevation ( 3980 m), a second putative dike Volcanism À Geological processes may have failed to break the surface of the ice sheet and formed Galaxias Mons as a laccolithic intrusion. We numerically model the formation of Galaxias Mons and find that at least 200 m of ice may once have existed at this latitude at the time of the dike intrusions. -
Select Bibliography
Select Bibliography by the late F. Seymour-Smith Reference books and other standard sources of literary information; with a selection of national historical and critical surveys, excluding monographs on individual authors (other than series) and anthologies. Imprint: the place of publication other than London is stated, followed by the date of the last edition traced up to 1984. OUP- Oxford University Press, and includes depart mental Oxford imprints such as Clarendon Press and the London OUP. But Oxford books originating outside Britain, e.g. Australia, New York, are so indicated. CUP - Cambridge University Press. General and European (An enlarged and updated edition of Lexicon tkr WeltliU!-atur im 20 ]ahrhuntkrt. Infra.), rev. 1981. Baker, Ernest A: A Guilk to the B6st Fiction. Ford, Ford Madox: The March of LiU!-ature. Routledge, 1932, rev. 1940. Allen and Unwin, 1939. Beer, Johannes: Dn Romanfohrn. 14 vols. Frauwallner, E. and others (eds): Die Welt Stuttgart, Anton Hiersemann, 1950-69. LiU!-alur. 3 vols. Vienna, 1951-4. Supplement Benet, William Rose: The R6athr's Encyc/opludia. (A· F), 1968. Harrap, 1955. Freedman, Ralph: The Lyrical Novel: studies in Bompiani, Valentino: Di.cionario letU!-ario Hnmann Hesse, Andrl Gilk and Virginia Woolf Bompiani dille opn-e 6 tUi personaggi di tutti i Princeton; OUP, 1963. tnnpi 6 di tutu le let16ratur6. 9 vols (including Grigson, Geoffrey (ed.): The Concise Encyclopadia index vol.). Milan, Bompiani, 1947-50. Ap of Motkm World LiU!-ature. Hutchinson, 1970. pendic6. 2 vols. 1964-6. Hargreaves-Mawdsley, W .N .: Everyman's Dic Chambn's Biographical Dictionary. Chambers, tionary of European WriU!-s. -
Active Volcanism on Io: Global Distribution and Variations in Activity
Icarus 140, 243–264 (1999) Article ID icar.1999.6129, available online at http://www.idealibrary.com on Active Volcanism on Io: Global Distribution and Variations in Activity Rosaly Lopes-Gautier Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 E-mail: [email protected] Alfred S. McEwen Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 William B. Smythe Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 P. E. Geissler Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 L. Kamp and A. G. Davies Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 J. R. Spencer Lowell Observatory, Flagstaff, Arizona 86001 L. Keszthelyi Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, P. O. Box 210092, Tucson, Arizona 85721-0092 R. Carlson Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 F. E. Leader and R. Mehlman Institute of Geophysics and Planetary Physics, University of California—Los Angeles, Los Angeles, California 90095 L. Soderblom Branch of Astrogeologic Studies, U.S. Geological Survey, Flagstaff, Arizona 86001 and The Galileo NIMS and SSI Teams Received June 23, 1998; revised February 10, 1999 in 1979. A total of 61 active volcanic centers have been identified Io’s volcanic activity has been monitored by instruments aboard from Voyager, groundbased, and Galileo observations. Of these, 41 the Galileo spacecraft since June 28, 1996. We present results from are hot spots detected by NIMS and/or SSI. -
Development of a Groundwater Flow Model for the Bishop/Laws Area
DEVELOPMENT OF A GROUNDWATER FLOW MODEL FOR THE BISHOP/LAWS AREA FINAL REPORT FOR LOCAL GROUNDWATER ASSISTANCE GRANT AGREEMENT NO. 4600004129 Robert Harrington, PhD, R.G. INYO COUNTY WATER DEPARTMENT APRIL, 2007 TABLE OF CONTENTS EXECUTIVE SUMMARY ………………………………………. 3 INTRODUCTION ………………………………………………. 5 CONCEPTUAL MODEL ………………………………………… 8 SIMULATION MODEL …………………………………………. 5 PREDICTIVE SIMULATIONS …………………………………. 23 SUMMARY AND CONCLUSIONS ……………………………. 26 REFERENCES …………………………………………………… 28 APPENDIX 1 ……………………………………………………. 51 APPENDIX 2 ……………………………………………………. 54 LIST OF FIGURES Figure 1. Study area location……………………………………………… 30 Figure 2. Geology…………………………………………………………. 31 Figure 3. Hydraulic conductivity distribution…………………………….. 32 Figure 4. Aquifer test locations…………………………………………… 33 Figure 5. Well locations…………………………………………………... 34 Figure 6. Layer 1 hydraulic conductivity zones…………………………... 35 Figure 7. Layer 2 hydraulic conductivity zones………………………….. 36 Figure 8. Layer 3 hydraulic conductivity zones…………………………. 37 Figure 9. Layer 4 hydraulic conductivity zones…………………………. 38 Figure 10. Layer 5 hydraulic conductivity zones………………………… 39 Figure 11. Quaternary faults and horizontal flow barriers………………. 40 Figure 12. Recharge zones……………………………………………….. 41 Figure 13. Evapotranspiration zones……………………………………… 42 Figure 14. Boundary conditions………………………………………….. 43 Figure 15. Observed vs. residuals………………………………………… 44 Figure 16. Distribution of residuals………………………………………. 45 Figure 17. Spatial distribution of residuals………………………………. 46 Figure 18. Drawdown