United States Earthquakes 1928
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Historic-Cultural Monument (HCM) List City Declared Monuments
Historic-Cultural Monument (HCM) List City Declared Monuments No. Name Address CHC No. CF No. Adopted Community Plan Area CD Notes 1 Leonis Adobe 23537 Calabasas Road 08/06/1962 Canoga Park - Winnetka - 3 Woodland Hills - West Hills 2 Bolton Hall 10116 Commerce Avenue & 7157 08/06/1962 Sunland - Tujunga - Lake View 7 Valmont Street Terrace - Shadow Hills - East La Tuna Canyon 3 Plaza Church 535 North Main Street and 100-110 08/06/1962 Central City 14 La Iglesia de Nuestra Cesar Chavez Avenue Señora la Reina de Los Angeles (The Church of Our Lady the Queen of Angels) 4 Angel's Flight 4th Street & Hill Street 08/06/1962 Central City 14 Dismantled May 1969; Moved to Hill Street between 3rd Street and 4th Street, February 1996 5 The Salt Box 339 South Bunker Hill Avenue (Now 08/06/1962 Central City 14 Moved from 339 Hope Street) South Bunker Hill Avenue (now Hope Street) to Heritage Square; destroyed by fire 1969 6 Bradbury Building 300-310 South Broadway and 216- 09/21/1962 Central City 14 224 West 3rd Street 7 Romulo Pico Adobe (Rancho 10940 North Sepulveda Boulevard 09/21/1962 Mission Hills - Panorama City - 7 Romulo) North Hills 8 Foy House 1335-1341 1/2 Carroll Avenue 09/21/1962 Silver Lake - Echo Park - 1 Elysian Valley 9 Shadow Ranch House 22633 Vanowen Street 11/02/1962 Canoga Park - Winnetka - 12 Woodland Hills - West Hills 10 Eagle Rock Eagle Rock View Drive, North 11/16/1962 Northeast Los Angeles 14 Figueroa (Terminus), 72-77 Patrician Way, and 7650-7694 Scholl Canyon Road 11 The Rochester (West Temple 1012 West Temple Street 01/04/1963 Westlake 1 Demolished February Apartments) 14, 1979 12 Hollyhock House 4800 Hollywood Boulevard 01/04/1963 Hollywood 13 13 Rocha House 2400 Shenandoah Street 01/28/1963 West Adams - Baldwin Hills - 10 Leimert City of Los Angeles May 5, 2021 Page 1 of 60 Department of City Planning No. -
POINT CABRILLO LIGHT STATION WEDDING SITE CONTRACT Point Cabrillo Light Station Is Located Between Fort Bragg and Mendocino on the Mendocino Coast
POINT CABRILLO LIGHT STATION WEDDING SITE CONTRACT Point Cabrillo Light Station is located between Fort Bragg and Mendocino on the Mendocino Coast. This magnificent backdrop of the majestic Pacific Ocean, tranquil Nature Preserve, and recently restored 1909 Point Cabrillo Light Station provides an elegant wedding site. Weddings are permitted at two designated sites due to public access and natural resource protection issues. The availability of these sites will vary with the seasons and environmental protection requirements. SITE FEES All members of the wedding party are counted as site guests. MAXIMUM SITES # OF GUESTS FEE In the Lighthouse 30 $1,250 Lighthouse Bluff 150 $1,000 RESERVATIONS To reserve a wedding site date, 1/2 of the site fee is required, along with a completed application and signed contract. The fee balance and a copy of the required insurance policy (see Item 10, Terms and Conditions, below) naming Point Cabrillo Lightkeepers Association (PCLK) and California Department of Parks and Recreation as co-payees are due 30 days prior to your wedding date. If the fee balance and required insurance policy are not received by this deadline, the reservation may be canceled at the discretion of PCLK. All checks for fees shall be made payable to PCLK. For further details on reserving the site, visit our web site at www.pointcabrillo.org, e-mail us at [email protected], or telephone 707-937-6123. A four bedroom, 4 ½ bath vacation rental, and two separate one bedroom cottages, are available on the Light Station grounds. Reservations may be made through Mendocino Coast Reservations at www.mendocinovacations.com or 707- 937-5033. -
Chamber Visitorgde.Pdf
CONTENTS Welcome to Mendocino County. i As a visitor you may be headed to our rugged coastline, which has been Welcome . ..2 a draw for filmmakers, artists, visitors and folks looking to relocate . Many remember that the television show “Murder, She Wrote” was filmed in the town Day Trips . 3 of Mendocino, or that the film Overboard was filmed in Noyo Harbor . We Westport . ..4 have a rich history of filmmaking on the Mendocino Coast and throughout the county of Mendocino . Fort Bragg . 5–10 Depending on the route you take to get to the Mendocino Coast, you Mendocino . .11–15 will be amazed at the diverse landscape along the way .You will likely see roll- ing hills with gnarled oak trees, old rustic barns with sheep, cows and horses Fort Bragg Map . 16 roaming the open space, giant redwood trees, meandering rivers, vineyards, Mendocino-Little River Map .17 apple orchards and the amazing Pacific Ocean . The majority of visitors to our county seek to visit the Mendocino Coast . Little River/Comptche . .18 Many discover the redwood forests found along Highway 20 and Highway Albion . .19 128 when traveling west from Highway 101, plus the beautiful wine country along Highway 128 and a solar beer brewery in the town of Boonville . Anderson Valley . 20 Up and down our coastline, on Highway 128 and Comptche-Ukiah Road, Elk/Manchester . 21 are amazing state parks, plus towns and communities with architecture from days gone by . Our county coastline borders Sonoma County to the south and Point Arena . .22 Humboldt County to the north . -
Laboratory Spectroscopy of Meteorite Samples at UV-Vis-NIR Wavelengths: Analysis and Discrimination by Principal Components Analysis
Laboratory spectroscopy of meteorite samples at UV-Vis-NIR wavelengths: Analysis and discrimination by principal components analysis Antti Penttil¨aa,∗, Julia Martikainena, Maria Gritsevicha, Karri Muinonena,b aDepartment of Physics, P.O. Box 64, FI-00014 University of Helsinki, Finland bFinnish Geospatial Research Institute FGI, National Land Survey of Finland, Geodeetinrinne 2, FI-02430 Masala, Finland Abstract Meteorite samples are measured with the University of Helsinki integrating-sphere UV-Vis- NIR spectrometer. The resulting spectra of 30 meteorites are compared with selected spectra from the NASA Planetary Data System meteorite spectra database. The spectral measure- ments are transformed with the principal component analysis, and it is shown that different meteorite types can be distinguished from the transformed data. The motivation is to im- prove the link between asteroid spectral observations and meteorite spectral measurements. Keywords: Meteorites, spectroscopy, principal component analysis 1. Introduction While a planet orbits the Sun, it is subject to impacts by objects ranging from tiny dust particles to much larger asteroids and comet nuclei. Such collisions of small Solar System bodies with planets have taken place frequently over geological time and played an 5 important role in the evolution of planets and development of life on the Earth. Every day approximately 30{180 tons of interplanetary material enter the Earth's atmosphere [1, 2]. This material is mostly represented by smaller meteoroids that undergo rapid ablation in the atmosphere. Under favorable initial conditions part of a meteoroid may survive the atmospheric entry and reach the ground [3]. The fragments recovered on the ground are 10 called meteorites, our valuable samples of the Solar System. -
Moluscos Del Perú
Rev. Biol. Trop. 51 (Suppl. 3): 225-284, 2003 www.ucr.ac.cr www.ots.ac.cr www.ots.duke.edu Moluscos del Perú Rina Ramírez1, Carlos Paredes1, 2 y José Arenas3 1 Museo de Historia Natural, Universidad Nacional Mayor de San Marcos. Avenida Arenales 1256, Jesús María. Apartado 14-0434, Lima-14, Perú. 2 Laboratorio de Invertebrados Acuáticos, Facultad de Ciencias Biológicas, Universidad Nacional Mayor de San Marcos, Apartado 11-0058, Lima-11, Perú. 3 Laboratorio de Parasitología, Facultad de Ciencias Biológicas, Universidad Ricardo Palma. Av. Benavides 5400, Surco. P.O. Box 18-131. Lima, Perú. Abstract: Peru is an ecologically diverse country, with 84 life zones in the Holdridge system and 18 ecological regions (including two marine). 1910 molluscan species have been recorded. The highest number corresponds to the sea: 570 gastropods, 370 bivalves, 36 cephalopods, 34 polyplacoforans, 3 monoplacophorans, 3 scaphopods and 2 aplacophorans (total 1018 species). The most diverse families are Veneridae (57spp.), Muricidae (47spp.), Collumbellidae (40 spp.) and Tellinidae (37 spp.). Biogeographically, 56 % of marine species are Panamic, 11 % Peruvian and the rest occurs in both provinces; 73 marine species are endemic to Peru. Land molluscs include 763 species, 2.54 % of the global estimate and 38 % of the South American esti- mate. The most biodiverse families are Bulimulidae with 424 spp., Clausiliidae with 75 spp. and Systrophiidae with 55 spp. In contrast, only 129 freshwater species have been reported, 35 endemics (mainly hydrobiids with 14 spp. The paper includes an overview of biogeography, ecology, use, history of research efforts and conser- vation; as well as indication of areas and species that are in greater need of study. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Sediment Provenance and Dispersal of Neogene–Quaternary Strata of the Southeastern San Joaquin Basin and Its Transition Into the GEOSPHERE; V
Research Paper THEMED ISSUE: Origin and Evolution of the Sierra Nevada and Walker Lane GEOSPHERE Sediment provenance and dispersal of Neogene–Quaternary strata of the southeastern San Joaquin Basin and its transition into the GEOSPHERE; v. 12, no. 6 southern Sierra Nevada, California doi:10.1130/GES01359.1 Jason Saleeby1, Zorka Saleeby1, Jason Robbins2, and Jan Gillespie3 13 figures; 2 tables; 2 supplemental files 1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA 2Chevron North America Exploration and Production, McKittrick, California 93251, USA 3Department of Geological Sciences, California State University, Bakersfield, California 93311, USA CORRESPONDENCE: jason@ gps .caltech .edu CITATION: Saleeby, J., Saleeby, Z., Robbins, J., and ABSTRACT INTRODUCTION Gillespie, J., 2016, Sediment provenance and dis- persal of Neogene–Quaternary strata of the south- eastern San Joaquin Basin and its transition into We have studied detrital-zircon U-Pb age spectra and conglomerate clast The Sierra Nevada and Great Valley of California are structurally coupled the southern Sierra Nevada, California: Geosphere, populations from Neogene–Quaternary siliciclastic and volcaniclastic strata and move semi-independently within the San Andreas–Walker Lane dextral v. 12, no. 6, p. 1744–1773, doi:10.1130/GES01359.1. of the southeastern San Joaquin Basin, as well as a fault-controlled Neo- transform system as a microplate (Argus and Gordon, 1991; Unruh et al., 2003). gene basin that formed across the southernmost Sierra Nevada; we call this Regional relief generation and erosion of the Sierra Nevada are linked to sub- Received 9 May 2016 Accepted 31 August 2016 basin the Walker graben. -
Earthquake Swarms and Slow Slip on a Sliver Fault in the Mexican Subduction Zone
Earthquake swarms and slow slip on a sliver fault in the Mexican subduction zone Shannon L. Fasolaa,1, Michael R. Brudzinskia, Stephen G. Holtkampb, Shannon E. Grahamc, and Enrique Cabral-Canod aDepartment of Geology and Environmental Earth Science, Miami University, Oxford, OH 45056; bGeophysical Institute, University of Alaska Fairbanks, Fairbanks, AK 99775; cDepartment of Earth and Environmental Sciences, Boston College, Chestnut Hill, MA 02467; and dInstituto de Geofísica, Universidad Nacional Autónoma de México, 04510 Ciudad de México, México Edited by John Vidale, University of Southern California, and approved February 25, 2019 (received for review August 24, 2018) The Mexican subduction zone is an ideal location for studying a large amount of inland seismicity, including a band of intense subduction processes due to the short trench-to-coast distances seismicity occurring ∼50 km inland from the trench (Fig. 1A) that bring broad portions of the seismogenic and transition zones (19). SSEs and tectonic tremor have been well documented of the plate interface inland. Using a recently generated seismicity further inland from this seismicity band (Fig. 1A) (19, 24–28), catalog from a local network in Oaxaca, we identified 20 swarms suggesting this band marks the frictional transition on the plate of earthquakes (M < 5) from 2006 to 2012. Swarms outline what interface from velocity weakening to velocity strengthening (6). appears to be a steeply dipping structure in the overriding plate, Other studies have used shallow-thrust earthquakes to define the indicative of an origin other than the plate interface. This steeply downdip limit of the seismogenic zone in southern Mexico (29– dipping structure corresponds to the northern boundary of the 31), and this corresponds with where the seismicity band occurs Xolapa terrane. -
Geological Survey Canada
70-66 GEOLOGICAL PAPER 70-66 ., SURVEY OF CANADA DEPARTMENT OF ENERGY, MINES AND RESOURCES REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas 1971 Price, 75 cents GEOLOGICAL SURVEY OF CANADA CANADA PAPER 70-66 REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 J. A. V. Douglas DEPARTMENT OF ENERGY, MINES AND RESOURCES @)Crown Copyrights reserved Available by mail from Information Canada, Ottawa from the Geological Survey of Canada 601 Booth St., Ottawa and Information Canada bookshops in HALIFAX - 1735 Barrington Street MONTREAL - 1182 St. Catherine Street West OTTAWA - 171 Slater Street TORONTO - 221 Yonge Street WINNIPEG - 499 Portage Avenue VANCOUVER - 657 Granville Street or through your bookseller Price: 75 cents Catalogue No. M44-70-66 Price subject to change without notice Information Canada Ottawa 1971 ABSTRACT A catalogue of the National Meteorite Collection of Canada, published in 1963 listed 242 different meteorite specimens. Since then specimens from 50 a dditional meteorites have been added to the collection and several more specimens have been added to the tektite collection. This report describes all specimens in the collection. REVISED CATALOGUE OF THE NATIONAL METEORITE COLLECTION OF CANADA LISTING ACQUISITIONS TO AUGUST 31, 1970 INTRODUCTION At the beginning of the nineteenth century meteorites were recog nized as unique objects worth preserving in collections. Increasingly they have become such valuable objects for investigation in many fields of scienti fic research that a strong international interest in their conservation and pre servation has developed (c. f. -
Preliminary Isoseismal Map for the Santa Cruz (Loma Prieta), California, Earthquake of October 18,1989 UTC
DEPARTMENT OF THE INTERIOR U.S. GEOLOGICAL SURVEY Preliminary isoseismal map for the Santa Cruz (Loma Prieta), California, earthquake of October 18,1989 UTC Open-File Report 90-18 by Carl W. Stover, B. Glen Reagor, Francis W. Baldwin, and Lindie R. Brewer National Earthquake Information Center U.S. Geological Survey Denver, Colorado This report has not been reviewed for conformity with U.S. Geological Survey editorial stan dards and stratigraphic nomenclature. Introduction The Santa Cruz (Loma Prieta) earthquake, occurred on October 18, 1989 UTC (October 17, 1989 PST). This major earthquake was felt over a contiguous land area of approximately 170,000 km2; this includes most of central California and a portion of western Nevada (fig. 1). The hypocen- ter parameters computed by the U.S. Geological Survey (USGS) are: Origin time: 00 04 15.2 UTC Location: 37.036°N., 121.883°W. Depth: 19km Magnitude: 6.6mb,7.1Ms. The University of California, Berkeley assigned the earthquake a local magnitude of 7.0ML. The earthquake caused at least 62 deaths, 3,757 injuries, and over $6 billion in property damage (Plafker and Galloway, 1989). The earthquake was the most damaging in the San Francisco Bay area since April 18,1906. A major arterial traffic link, the double-decked San Francisco-Oakland Bay Bridge, was closed because a single fifty foot span of the upper deck collapsed onto the lower deck. In addition, the approaches to the bridge were damaged in Oakland and in San Francisco. Other se vere earthquake damage was mapped at San Francisco, Oakland, Los Gatos, Santa Cruz, Hollister, Watsonville, Moss Landing, and in the smaller communities in the Santa Cruz Mountains. -
A History of British Seismology
Bull Earthquake Eng (2013) 11:715–861 DOI 10.1007/s10518-013-9444-5 ORIGINAL RESEARCH PAPER A history of British seismology R. M. W. Musson Received: 14 March 2013 / Accepted: 21 March 2013 / Published online: 9 May 2013 © The Author(s) 2013. This article is published with open access at Springerlink.com Abstract The work of John Milne, the centenary of whose death is marked in 2013, has had a large impact in the development in global seismology. On his return from Japan to England in 1895, he established for the first time a global earthquake recording network, centred on his observatory at Shide, Isle of Wight. His composite bulletins, the “Shide Circulars” developed, in the twentieth century, into the world earthquake bulletins of the International Seismolog- ical Summary and eventually the International Seismological Centre, which continues to publish the definitive earthquake parameters of world earthquakes on a monthly basis. In fact, seismology has a long tradition in Britain, stretching back to early investigations by members of the Royal Society after 1660. Investigations in Scotland in the early 1840s led to a number of firsts, including the first network of instruments, the first seismic bulletin, and indeed, the first use of the word “seismometer”, from which words like “seismology” are a back-formation. This paper will present a chronological survey of the development of seismology in the British Isles, from the first written observations of local earthquakes in the seventh century, and the first theoretical writing on earthquakes in the twelfth century, up to the monitoring of earthquakes in Britain in the present day. -
W Numerze: – Wywiad Z Kustoszem Watykańskiej Kolekcji C.D. – Cz¹stki
KWARTALNIK MI£OŒNIKÓW METEORYTÓW METEORYTMETEORYT Nr 3 (63) Wrzesieñ 2007 ISSN 1642-588X W numerze: – wywiad z kustoszem watykañskiej kolekcji c.d. – cz¹stki ze Stardusta a meteorytry – trawienie meteorytów – utwory sp³ywania na Sikhote-Alinach – pseudometeoryty – konferencja w Tucson METEORYT Od redaktora: kwartalnik dla mi³oœników OpóŸnieniami w wydawaniu kolejnych numerów zaczynamy meteorytów dorównywaæ „Meteorite”, którego sierpniowy numer otrzyma³em Wydawca: w paŸdzierniku. Tym razem g³ówn¹ przyczyn¹ by³y k³opoty z moim Olsztyñskie Planetarium komputerem, ale w koñcowej fazie redagowania okaza³o siê tak¿e, i Obserwatorium Astronomiczne ¿e brak materia³u. Musia³em wiêc poczekaæ na mocno opóŸniony Al. Pi³sudskiego 38 „Meteorite”, z którego dorzuci³em dwa teksty. 10-450 Olsztyn tel. (0-89) 533 4951 Przeskok o jeden numer niezupe³nie siê uda³, a zapowiedzi¹ [email protected] dalszych k³opotów jest mi³y sk¹din¹d fakt, ¿e przep³yw materia³ów zacz¹³ byæ dwukierunkowy. W najnowszym numerze „Meteorite” konto: ukaza³ siê artyku³ Marcina Cima³y o Moss z „Meteorytu” 3/2006, 88 1540 1072 2001 5000 3724 0002 a w kolejnym numerze zapowiedziany jest artyku³ o Morasku BOŒ SA O/Olsztyn z „Meteorytu” 4/2006. W rezultacie jednak bêdzie mniej materia³u do Kwartalnik jest dostêpny g³ównie t³umaczenia i trzeba postaraæ siê o dalsze w³asne teksty. Czy mo¿e ktoœ w prenumeracie. Roczna prenu- merata wynosi w 2007 roku 44 z³. chcia³by coœ napisaæ? Zainteresowanych prosimy o wp³a- Z przyjemnoœci¹ odnotowujê, ¿e nabieraj¹ tempa przygotowania cenie tej kwoty na konto wydawcy do kolejnej konferencji meteorytowej, która planowana jest na 18—20 nie zapominaj¹c o podaniu czytel- nego imienia, nazwiska i adresu do kwietnia 2008 r.