Shifting post production patterns: exploring changes in New Zealand's seafood processing industry     

Stringer C  Simmons G  Rees E 《New Zealand geographer》2011,67(3):161-173

This paper examines the changing nature of New Zealand's seafood companies' production practices. The past 15 years has seen the offshore outsourcing of post-harvest fish gain unprecedented momentum. The growth in offshore processing is a further stage in an increasingly globalised fisheries value chain. Fish is head and gutted, frozen and then transported to processing sites in China where it is thawed, value-added processed and refrozen for export to the original sourcing country or third country markets. Reasons advanced by the industry for this shift in production practices include quota reductions, increasing production costs and the sale of trawlers.  相似文献   

Charting thermal emission variability at Pele,Janus Patera and Kanehekili Fluctus with the Galileo NIMS Io Thermal Emission Database (NITED)     

Ashley Gerard Davies  Glenn J. Veeder  Dennis L. Matson  Torrence V. Johnson 《Icarus》2012,221(1):466-470

Using the NIMS Io Thermal Emission Database (NITED), a collection of over 1000 measurements of radiant flux from Io’s volcanoes (Davies, A.G. et al. [2012]. Geophys. Res. Lett. 39, L01201. doi:10.1029/2011GL049999), we have examined the variability of thermal emission from three of Io’s volcanoes: Pele, Janus Patera and Kanehekili Fluctus. At Pele, the 5-μm thermal emission as derived from 28 night time observations is remarkably steady at 37 ± 10 GW μm^?1, re-affirming previous analyses that suggested that Pele an active, rapidly overturning silicate lava lake. Janus Patera also exhibits relatively steady 5-μm thermal emission (≈20 ± 3 GW μm^?1) in the four observations where Janus is resolved from nearby Kanehekili Fluctus. Janus Patera might contain a Pele-like lava lake with an effusion rate (Q_F) of ≈40–70 m³ s^?1. It should be a prime target for a future mission to Io in order to obtain data to determine lava eruption temperature. Kanehekili Fluctus has a thermal emission spectrum that is indicative of the emplacement of lava flows with insulated crusts. Effusion rate at Kanehekili Fluctus dropped by an order of magnitude from ≈95 m³ s^?1 in mid-1997 to ≈4 m³ s^?1 in late 2001.  相似文献   

Atmospheric Circulation Patterns Associated with Mortality Changes During the Transitional Seasons     

Jill S.M. Coleman 《The Professional geographer》2013,65(2):190-206

Although much research has been done linking meteorological variables individually with various aspects of human health, few studies have considered the collective impact of weather. This study examines the relationship among ten synoptic-scale weather patterns and daily cause-specific human mortality rates for metropolitan areas in the central United States during the 1978 to 1998 autumn and spring seasons. The results show that distinctive changes in mortality rates are often associated with one or two of the more moderate synoptic types, displaying notable spatial and temporal variability. The occurrence of the Eastern Zonal (EZ) pattern during spring and the East Coast Trough (ECT) pattern during autumn seems to invoke the most significant increased mortality response across all causes of death and metropolitan statistical areas. For the EZ and ECT types, the largest adverse response occurs for locations influenced by cold, anticyclonic situations and atmospheric stability.  相似文献   

Combining Surge and Wind Risk from Hurricanes Using a Copula Model: An Example from Galveston,Texas     

Jill C. Trepanier  Hal F. Needham  James B. Elsner  Thomas H. Jagger 《The Professional geographer》2013,65(1):52-61

Consideration of climate-related impacts on coasts is important to ensure readiness for disaster response. Local risk of storm surge and strong winds from hurricanes affecting Galveston, Texas, is quantified using a bivariate copula model fit to observed data. The model uses a two-dimensional Archimedean copula. Parametric uncertainty (5th and 95th percentiles) is quantified using a Monte Carlo procedure. The annual probability of a hurricane producing winds of at least 50 ms^?1 and a surge of at least 4 m is 1.7 percent with a 95 percent confidence interval of (1.33, 1.78) percent. The methodology can be extended to include inland flooding and can be applied elsewhere with available information.  相似文献   

Elemental abundance measurements in low-redshift damped Lyman α absorbers     

Joseph D. Meiring  Varsha P. Kulkarni  Pushpa Khare  Jill Bechtold  Donald G. York  Jun Cui  James T. Lauroesch  Arlin P. S. Crotts  Osamu Nakamura 《Monthly notices of the Royal Astronomical Society》2006,370(1):43-62

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Preface     

Stracher  Glenn B. 《Mathematical Geosciences》2000,32(2):149-150

Mathematical Geosciences -  相似文献   

Far-infrared detection limits – I. Sky confusion due to Galactic cirrus     

Woong-Seob Jeong  Hyung Mok Lee  Soojong Pak  Takao Nakagawa  Suk Minn Kwon  Chris P. Pearson  Glenn J. White 《Monthly notices of the Royal Astronomical Society》2005,357(2):535-547

Fluctuations in the brightness of the background radiation can lead to confusion with real point sources. This type of confusion with background emission is relevant when making infrared (IR) observations with relatively large beam sizes, since the amount of fluctuation tends to increase with the angular scale. To quantitively assess the effect of the background emission on the detection of point sources for current and future far-IR observations by space-borne missions such as Spitzer , ASTRO-F , Herschel and Space Infrared Telescope for Cosmology and Astrophysics ( SPICA ), we have extended the Galactic emission map to a higher level of angular resolution than that of the currently available data. Using this high-resolution map, we estimate the sky confusion noise owing to the emission from interstellar dust clouds or cirrus, based on fluctuation analysis and detailed photometry over realistically simulated images. We find that the confusion noise derived by simple fluctuation analysis agrees well with the results from realistic simulations. Although sky confusion noise becomes dominant in long wavelength bands  (>100 μm)  with 60–90 cm aperture missions, it is expected to be two orders of magnitude lower for the next generation of space missions (with larger aperture sizes) such as Herschel and SPICA .  相似文献   

Fine‐grained,spinel‐rich inclusions from the reduced CV chondrite Efremovka: II. Oxygen isotopic compositions     

Jrme ALON  Alexander N. KROT  Kevin D. MCKEEGAN  Glenn J. MACPHERSON  Alexander A. ULYANOV 《Meteoritics & planetary science》2005,40(7):1043-1058

Abstract— Oxygen isotopes have been measured by ion microprobe in individual minerals (spinel, Al‐Ti‐diopside, melilite, and anorthite) within four relatively unaltered, fine‐grained, spinel‐rich Ca‐Al‐rich inclusions (CAIs) from the reduced CV chondrite Efremovka. Spinel is uniformly ¹⁶O‐rich (Δ¹⁷O ≤ ?20‰) in all four CAIs; Al‐Ti‐diopside is similarly ¹⁶O‐rich in all but one CAI, where it has smaller ¹⁶O excesses (‐15‰ ≤ Δ¹⁷O ≤ ?10‰). Anorthite and melilite vary widely in composition from ¹⁶O‐rich to ¹⁶O‐poor (‐22‰ ≤ Δ¹⁷O ≤ ?5‰). Two of the CAIs are known to have group II volatility‐fractionated rare‐earth‐element patterns, which is typical of this variety of CAI and which suggests formation by condensation. The association of such trace element patterns with ¹⁶O‐enrichment in these CAIs suggests that they formed by gas‐solid condensation from an ¹⁶O‐rich gas. They subsequently experienced thermal processing in an ¹⁶O‐poor reservoir, resulting in partial oxygen isotope exchange. Within each inclusion, oxygen isotope variations from mineral to mineral are consistent with solid‐state oxygen self‐diffusion at the grain‐to‐grain scale, but such a model is not consistent with isotopic variations at a larger scale in two of the CAIs. The spatial association of ¹⁶O depletions with both elevated Fe contents in spinel and the presence of nepheline suggests that late‐stage iron‐alkali metasomatism played some role in modifying the isotopic patterns in some CAIs. One of the CAIs is a compound object consisting of a coarse‐grained, melilite‐rich (type A) lithology joined to a fine‐grained, spinel‐rich one. Melilite and anorthite in the fine‐grained portion are mainly ¹⁶O‐rich, whereas melilite in the type A portion ranges from ¹⁶O‐rich to ¹⁶O‐poor, suggesting that oxygen isotope exchange predated the joining together of the two parts and that both ¹⁶O‐rich and ¹⁶O‐poor gaseous reservoirs existed simultaneously in the early solar nebula.  相似文献   

The SAURON project – XI. Stellar populations from absorption-line strength maps of 24 early-type spirals     

Reynier F. Peletier  Jesús Falcón-Barroso  Roland Bacon  Michele Cappellari  Roger L. Davies  P. T. de Zeeuw  Eric Emsellem  Katia Ganda  Davor Krajnovi&#;  Harald Kuntschner  Richard M. McDermid  Marc Sarzi  Glenn van de Ven 《Monthly notices of the Royal Astronomical Society》2007,379(2):445-468

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Chronologic implications of new Miocene mammals from the Cura-Mallín and Trapa Trapa formations, Laguna del Laja area, south central Chile     

John J. Flynn  Reynaldo Charrier  Darin A. Croft  Phillip B. Gans  Trystan M. Herriott  Jill A. Wertheim  Andr R. Wyss 《Journal of South American Earth Sciences》2008,26(4):412-423

Recent work in the central Andean Main Range of Chile near Laguna del Laja (37.5°S, 71°W) has produced the first mammal fossils for the region. Fossils, locally abundant and well preserved, occur patchily across a wide area southeast of the lake. Mammalian remains are derived from generally strongly folded (kilometer-scale) exposures of the locally 1.8 km thick, early to middle Miocene Cura-Mallín Formation; two identifiable specimens have been recovered from the overlying Trapa Trapa Formation as well. Both formations consist primarily of well-stratified (1–5 m thick layers) volcaniclastic and volcanic strata, deposited predominantly in fluviatile systems. The Cura-Mallín Formation is possibly the southern continuation of (or lateral equivalent to) the richly fossiliferous Abanico Formation mapped between 32°S and 36°S. Intensive sampling in a series of localities east and south of Laguna del Laja has yielded diverse faunas, in addition to radioisotopically dateable horizons. The new fossil mammal faunas represent as many as six South American Land Mammal “Ages” (SALMAs). Fossils, together with preliminary ⁴⁰Ar/³⁹Ar radioisotopic dates, ranging from 9 to 20 Ma across the exposed thickness of the Cura-Mallín Formation and into the overlying Trapa Trapa Formation, provide a robust geochronological framework for middle Cenozoic strata in the Laguna del Laja region. The sequence of directly superposed mammalian assemblages at Laguna del Laja is one of the longest in all of South America, rivaled only by the classic Gran Barranca section of Patagonian Argentina. These data illuminate the geological history of the area and its record of mammalian evolution. The potential to isotopically date these diverse faunas with high precision (error ± 0.5 Ma) presents a rare opportunity to calibrate related portions of the SALMA sequence.  相似文献