Energy transfer by magnetopause reconnection and the substorm parameter ϵ     

W.D. Gonzalez  A.L.C. Gonzalez 《Planetary and Space Science》1984,32(8):1007-1012

An expression for the magnetopause reconnection power based on the dawn-dusk component of the reconnection electric field, that reduces to the substorm parameter ? for the limit that involves equal geomagnetic (B_G) and magnetosheath (B_M) magnetic field amplitudes at the magnetopause, is contrasted with the expression based on the whole reeonnection electric field vector (Gonzalez, 1973). The correlation examples of this report show that this (more general) expression for the reconnection power seems to correlate with the empirical dissipation parameter U_T (Akasofu, 1981), with slightly better correlation coefficients than those obtained from similar correlations between the parameter ? and U_T Thus, these (better) correlations show up for the more familiar values of the ratio B_G/B_M > 1. Nevertheless, the (expected) relatively small difference that seems to exist between these correlation coefficients suggests that, for practical purposes, the parameter ? could be used as well (instead of the more general expression) in similar correlation studies due to its simpler format. On the other hand, studies that refer mainly to the difference in the magnitudes of ? and of the more general expression are expected to give results with less negligible differences.  相似文献   

Comparison Between Halo cme Expansion Speeds Observed on the Sun,the Related Shock Transit Speeds to Earth and Corresponding Ejecta Speeds at 1 au   总被引：1，自引：0，他引：1  

Dal Lago  A.  Vieira  L.E.A.  Echer  E.  Gonzalez  W.D.  de Gonzalez  A.L.C.  Guarnieri  F.L.  Schuch  N.J.  Schwenn  R. 《Solar physics》2004,222(2):323-328

We have compared characteristics of 38 halo coronal mass ejections observed on the Sun by the Large Angle and Spectrometric Coronagraph onboard SOHO with their corresponding counterparts observed near Earth by the magnetic field and plasma instruments onboard the ACE, WIND and SOHO satellites, in the period from January 1997 to April 2001. We only have selected events that have some associated interplanetary ejecta structure at 1 AU and we have compared the lateral expansion speeds of these halo CMEs and the corresponding ejecta speeds near Earth. We found that there is a high correlation between these two speeds. The results are very similar to the study done by Lindsay et al. (1999) using observations made by Solwind and SMM coronagraphs, and Helios-1 and PVO plasma and interplanetary field data from the period of 1979 to 1988. Also, we reviewed the relation between the CME-related shock transit speed to Earth and the ejecta speeds near Earth. This kind of relation is very important to estimate ejecta speeds of events for which no interplanetary observations are available.  相似文献   

CO_2 degassing and melting of metasomatized mantle lithosphere during rifting-Numerical study     

Weronika Gorczyk  Christopher M.Gonzalez 《地学前缘(英文版)》2019,10(4):1409-1420

:Reactivation of metasomatized mantle lithosphere may occur during continental extension,which is an important component of plate tectonics.The lower most part of the metasomatized domains in the subcontinental mantle lithosphere can be locally enriched in CO2.Therefore,partial melting of these metasomatized domains may play a crucial role in the global carbon cycle.However,little is known about this process and up until now few numerical constraints are available.Here we address this knowledge gap and use a 2-D high resolution petrological-thermomechanical model to assess lithospheric rifting.CO2 degassing and melting.We test 4 lithospheric thicknesses:90,110,130 and 200 km with a 10 km thick metasomatized layer at the base using CO2 of 2 wt.%in the bulk composition.The carbonate enriched layer is stable below^3 GPa(>110 km)for a temperature of 1300℃;therefore,we only observe degassing patterns for lithospheric models that are 130 km and 200 km thick.The metasomatized layer for the 130 km thick lithosphere mostly comprises carbonatite melting,whereas in the 200 km thick scenario propagation of melt development from kimberlites to carbonatites occurs as the metasomatic mantle is exhumed during extension.The numerical models fit well into natural rifting zones of the European Cenozoic Rift System for young(shallow)and of the North Atlantic Rift for old(thick)lithosphere.  相似文献   

Bivalve population health: Multistress to identify hot spots   总被引：3，自引：0，他引：3  

X. de Montaudouin  I. Paul-Pont  P. Gonzalez  F. Jude  M. Baudrimont  F. Le Grand  L. Bourasseau 《Marine pollution bulletin》2010,60(8):1307-118

This study investigated some stress (metals, parasites) and response (immunity, metallothionein) factors in two cockle and two Manila clam populations. Data from eight seasons were averaged to obtain global baseline values. Stress/response characteristics of each population were compared to population health status that was determined through population dynamics parameters. Four different scenarios were discussed: (1) a lightly stressed cockle population with correct population health but with a risk of deterioration (hot spot); (2) a lightly stressed introduced cockle population threatened of extinction. In this case ecological factors were suspected; (3) a moderately stressed clam population with moderate adaptative response. The population was sustainable but the level of stress should not increase (hotspot); and (4) a stressed clam population and unfavourable ecological conditions preventing clam settlement. This monitoring highlighted that the discrepancy between population health and stress levels could be due to insufficient response by bivalves and/or by unfavourable ecological factors.  相似文献   

High tolerance to tributyltin in embryos and larvae of the horseshoe crab,Limulus polyphemus     

Mark L. Botton  Melanie Hodge  Tino I. Gonzalez 《Estuaries and Coasts》1998,21(2):340-346

The effects of acute and chronic exposure to tributyltin (TBT) were examined in bioassays using horseshoe crab (Limulus polyphemus) embryos and “trilobite” larvae. Larvae had>95% survival after 24-h exposure to nominal concentrations of 1–500 μg l^?1 TBT. Survival was also high following 48-h and 72-h exposure to ≤100 μg l^?1 TBT; >50% mortality was seen only after 48-h and 72-h exposure to 500 μg l^?1 TBT. Estimated median lethal concentrations (LC₅₀) were >1000 μg l^?1, 742 μg l^?1, and 594 μg l^?1 for 24-h, 48-h, and 72-h exposure, respectively. Much higher toxicity LC₅₀=42 μg l^?1) was seen following chronic exposure of larvae to TBT. Acute exposure to TBT significantly increased the time required by larvae to molt into the first-tailed stage. LC₅₀ for horseshoe crab embryos exposed to TBT were 44 μg l^?1, 20 μg l^?1, and 14 μg l^?1 for 24, 48, and 72 h acute exposure, indicating that this earlier developmental stage was about 30–40 fold more susceptible to TBT than larvae. Horseshoe crabs are highly tolerant of TBT in comparison to early developmental stages of other marine arthropods. The ability of horseshoe crab embryos and larvae to survive in the presence of organotin pollution suggests the possibility of bioaccumulation and movement into the estuarine food chain via shorebirds, gulls, and fish.  相似文献   

Palaeointensity studies of a late Permian lava succession from Guizhou Province, South China: implications for post-Kiaman dipole field behaviour   总被引：1，自引：0，他引：1  

D. N. Thomas  T. C. Rolph  J. Shaw  S. Gonzalez de Sherwood  & Z. Zhuang 《Geophysical Journal International》1998,134(3):856-866

Palaeomagnetic results are presented from a volcanic sequence in Zhijin County, Guizhou Province, Southern China. The lavas and associated volcanic breccias comprising the sequence represent a southern extension of the Emeishan volcanic province. Biostratigraphic dating of interbedded limestone units and stratigraphic constraints indicate that the section formed during the late Permian (∼263–255  Ma), and is thus somewhat older than the Emei stratotype section in Sichuan Province, and close in age to reported estimates of the termination of the Permo-Carboniferous (Kiaman) reverse superchron. Rock magnetic analyses and reflected light microscopy indicate that the magnetic mineralogy of the lava units is dominated by fresh, primary magnetites containing a significant fraction of single-domain grains. Thermal demagnetization behaviour of the breccia units is poor, but most lava samples have one or two components of remanence above 250 °C. The normal polarity characteristic remanence held by the lavas implies a post-Kiaman age for this succession and suggests that the termination of the Kiaman occurred prior to 263  Ma, supporting recently published estimates. According to standard criteria, Thellier palaeointensity results from the lavas are of good quality and reveal that the dipole field strength was comparatively low shortly after the termination of the superchron. 80 per cent of samples record relative VDM values in the range 42–52 per cent of the present-day value, supporting recent studies of mid-Kiaman field intensity. This suggests that a low-energy dipole existed at least between 300 and 255  Ma and does not appear to have been confined to the stable reverse polarity interval.  相似文献   

Lower Paleozoic extensional tectonics in the limit between the West Asturian-Leonese and Central Iberian Zones of the Variscan Fold-Belt in NW Spain   总被引：1，自引：1，他引：0  

J. R. Martinez Catalan  M. P. Hacar Rodriguez  P. Villar Alonso  A. Perez-Estaun  F. Gonzalez Lodeiro 《International Journal of Earth Sciences》1992,81(2):545-560

The limit between the West Asturian-Leonese and Central-Iberian Zones in the NW of the Iberian Peninsula is described in the area of Caurel-Truchas (Provinces of Orense and León). From the distribution of the sedimentary formations and the Variscan structures it is inferred that the transition between the two zones was a fault system, which was active during, at least, the Ordovician and Lower Silurian. The faults were supposedly normal, though they had probably some strike-slip component, and gave rise to a half-graben in which a syn-rift sequence was deposited. The latter underwent inversion at the onset of the Variscan tectonism, producing a ramp anticline-syncline pair that forms the more important folds in the area. The varying geometry of these folds is interpreted partly as being due to the existence of previous en échelon folds related to the strike-slip component of the faults and, partly, as a result of the variable intensity of the shear strain undergone during the first variscan phase.

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Zusammenfassung Die Grenze zwischen der West-Asturischen-Leonesischen und Zentral-Iberischen Zone im NW der Iberischen Halbinsel wird aus dem Gebiet von Caurel-Truchas (Provinz Orense und León) beschrieben. Aufgrund der Verteilung der sedimentären Formationen, sowie der variszischen Strukturen wird abgeleitet, daß der Übergang zwischen den beiden Zonen durch ein Störungssystem bedingt wurde, das zumindest zwischen Ordovizium und Untersilur aktiv war. Dabei handelte es sich vermutlich um Abschiebungen mit einer Horizontalverschiebungskomponente. Diese Ausbildung führte zu einem Halbgraben mit darin abgelagerter sedimentärer Syn-Riftsequenz. Letztere wurde während der Anfangsphase der variszischen Tektonik invertiert, so daß es zu einem Rampen-Antiklinal-Synklinal Paar kam, welches die wichtigsten Falten der Gegend bildet. Die variable Geometrie der Falten wird zum einen der Existenz von frühen En-échelon Falten zugeschrieben, die durch die Horizontalverschiebungskomponente der Störungen hervorgerufen wurden; zum anderen sind sie das Resultat der veränderlichen Intensität der Scherspannung während der ersten variszischen Phase.

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Resumen Se describe el límite entre las Zonas Asturoccidental-Leonesa y Centroibérica en el NO de la Península Ibérica en el área del Caurel-Truchas (Provincias de Orense y León). Partiendo de la distribución de las formaciones sedimentarias y de la geometría de las estructuras varíscicas, se deduce que la transición entre las dos zonas fue un sistema de fallas, que fue activo al menos durante el Ordovício y el Silúrico Inferior. Se supone que la principal componente de las fallas fue normal, aunque debió de existir también una componente de desgarre, y su juego originó un semi-graben en el que se acumuló una secuencia sin-rift. Esta última experimentó una inversión al principio de la tectogénesis Varíscica, formándose un par de pliegues de rampa que son los pliegues más importantes del área. La geometría variable de esos pliegues se interpreta como debida, en parte, a la existencia previa de pliegues en escalón relacionados con la componente de desgarre de las fallas y, en parte, como consecuencia de la variable intensidad de la deformación por cizallamiento sufrida durante la primera fase de deformación varíscica.

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Fourteen years of multifrequency-coordinated observations of the X-ray/Be system A 0535+26/HDE 245770     

F. Giovannelli  C. Bartolini  A. Guarnieri  A. Piccioni  M. Burger  E. L. Van Dessel  V. G. Kurt  E. K. Sheffer  D. De Martino  R. Waters  I. Gonzalez Martinez-Pais  Yu. N. Gnedin  V. M. Larionov  N. I. Shakovskaya 《Astrophysics and Space Science》1990,169(1-2):139-145

Within the framework of a very long multifrequency campaign of coordinated, and very often simultaneous, observations of the transient X-ray/Be system A 0535+26/HDE 245770, we present a summary of this large collection of data taken with IUE and ASTRON satellites as well as with many ground-based telescopes in optical and IR regions.In this paper we emphasize the study of the physics and dynamics of the mass transfer at periastron and subsequent X-ray flaring, which is a typical problem of the X-ray/Be binary system class.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on New Windows to the Universe, held 3–8 July, 1989, Tenerife, Canary Islands, Spain.  相似文献   

Real-Time Tsunami Forecasting: Challenges and Solutions   总被引：8，自引：0，他引：8  

Vasily?V.?TitovEmail author  Frank?I.?Gonzalez  E.?N.?Bernard  Marie?C.?Eble  Harold?O.?Mofjeld  Jean?C.?Newman  Angie?J.?Venturato 《Natural Hazards》2005,35(1):35-41

A new method for real-time tsunami forecasting will provide NOAAs Tsunami Warning Centers with forecast guidance tools during an actual tsunami event. PMEL has developed the methodology of combining real-time data from tsunameters with numerical model estimates to provide site- and event-specific forecasts for tsunamis in real time. An overview of the technique and testing of this methodology is presented.  相似文献   

Long-lead ENSO predictability from CMIP5 decadal hindcasts     

Paula L. M. Gonzalez  Lisa Goddard 《Climate Dynamics》2016,46(9-10):3127-3147

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