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911.
Carlos Marı́n Jesús Galindo-Zaldı́var Luı́s Roberto Rodrı́guez-Fernández 《Comptes Rendus Geoscience》2003,335(2):255-264
The Campo de Dal??as, located between the central and eastern Betic Cordilleras, shows an evolution determined by the overprinting of two main stress fields since Pliocene times. The first of these develops hybrid and tensional joint sets up to Pleistocene (100 000 yr) and is characterized by NNW–SSE horizontal trend of compression and an ENE–WSW horizontal extension. The second stress field has prolate to triaxial extensional ellipsoids, also with ENE–WSW horizontal extension, and continues to be active today. The most recent stresses produce the reactivation of previous joints as faults whose trends are comprised mainly from N120°E to N170°E and have a normal and transtensional regime, with dextral or sinistral components. The palaeostress evolution of this region is similar to that undergone by other basins of the Eastern Betic Cordilleras, although the Pliocene–Pleistocene transcurrent deformations in the Campo de Dal??as only develop joints and not strike-slip faults. 相似文献
912.
Intercomparison of Boron Isotope and Concentration Measurements. Part II: Evaluation of Results 总被引:3,自引:1,他引:3
Roberto Gonfiantini Sonia Tonarini Manfred Grning Alessandra Adorni‐Braccesi Assad S. Al‐Ammar Marcus Astner Sebastien Bchler Ramon M. Barnes Randy L. Bassett Alain Cocherie Annette Deyhle Andrea Dini Giorgio Ferrara Jrme Gaillardet Judith Grimm Catherine Guerrot Urs Krhenbühl Graham Layne Damien Lemarchand Anette Meixner D. Jack Northington Maddalena Pennisi Eva Reitznerov Ilia Rodushkin Naoji Sugiura Regina Surberg Sabine Tonn Michael Wiedenbeck Samuel Wunderli Yingkai Xiao Thomas Zack 《Geostandards and Geoanalytical Research》2003,27(1):41-57
The Istituto di Geoscienze e Georisorse (IGG), on behalf and with the support of the International Atomic Energy Agency (IAEA), prepared eight geological materials (three natural waters and five rocks and minerals), intended for a blind interlaboratory comparison of measurements of boron isotopic composition and concentration. The materials were distributed to twenty seven laboratories - virtually all those performing geochemical boron isotope analyses in the world -which agreed to participate in the intercomparison exercise. Only fifteen laboratories, however, ultimately submitted the isotopic and/or concentration results they obtained on the intercomparison materials. The results demonstrate that interlaboratory reproducibility is not well reflected by the precision values reported by the individual laboratories and this observation holds true for both boron concentration and isotopic composition. The reasons for the discrepancies include fractionations due to the chemical matrix of materials, relative shift of the zero position on the δ11 B scale and a lack of well characterized materials for calibrating absolute boron content measurements. The intercomparison materials are now available at the IAEA (solid materials) and IGG (waters) for future distribution. 相似文献
913.
Isabel Salamanca Roberto Cid-Fernandes Guillermo Tenorio-Tagle Eduardo Telles Roberto J. Terlevich & Casiana Muñoz-Tuñón 《Monthly notices of the Royal Astronomical Society》1998,300(2):L17-L21
We report the detection of the slow-moving wind into which the compact supernova remnant SN 1997ab is expanding. Echelle spectroscopy provides clear evidence for a well-resolved narrow (full width at zero intensity, FWZI ∼180 km s−1 ) P Cygni profile, both in Hα and Hβ, superimposed on the broad emission lines of this compact supernova remnant. From theoretical arguments we know that the broad and strong emission lines imply a circumstellar density ( n ≥ 107 cm−3 ). This, together with our detection, implies a massive and slow stellar wind experienced by the progenitor star shortly prior to the explosion. 相似文献
914.
915.
Luis Jiménez-Benito Angeles Díaz Roberto Terlevich Elena Terlevich 《Astrophysics and Space Science》1998,263(1-4):111-114
We have analyzed high signal-to-noise spectra of 10 active galaxies in order to investigate the stellar populations of these
objects and the kinematics of the gas and stars in their nuclei.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
916.
Luigi Marini Valeria Chiappini Roberto Cioni G. Cortecci E. Dinelli Claudia Principe Giorgio Ferrara 《Bulletin of Volcanology》1998,60(3):187-194
Sulfur contents and δ34S values of Somma-Vesuvius magmas are consistent with syneruptive, open-system degassing at temperatures of 800–850°C for
Plinian pumices and 1100–1200°C for lavas. The extent of degassing appears to be greater in lavas than in pumices. The key
parameter controlling the 34S/32S ratio of Somma-Vesuvius volcanics is the average magma oxidation state, which generally varies from 0.85 to 1.20 Δ NNO units
for lavas and from 1.20 to 1.40 Δ NNO units for pumices. Consequently, S contents and δ34S values of magmas constitute a potentially valuable tool in estimating their average redox conditions. The results of this
study may help in risk mitigation when the Vesuvius magmatic system evolves toward eruptive conditions.
Received: 20 January 1998 / Accepted: 5 May 1998 相似文献
917.
918.
Maurizio Ripepe Andrew J. L. Harris Roberto Carniel 《Journal of Volcanology and Geothermal Research》2002,118(3-4)
During June 1999, we measured the amplitude and rate (number of events per second) at which gas exited the vent at Stromboli volcano as discrete gas bursts or puffs. This allowed us to identify two styles of gas burst (puffing) activity. The first is characterized by frequent, rapidly rising puffs, the second by less frequent, slowly rising puffs. Each style persisted over 5–40-min-long durations and was associated with a high and low number of strombolian explosions per hour, respectively. Each period was also associated with characteristic delay times between the arrival of the infrasonic and thermal signals during strombolian explosions; the delays were longer during vigorous puffing periods. To explain our observations, we propose a model in which the degassing process cycles between vigorous and weak degassing phases. During vigorous degassing phases, bubble layers ascend the conduit at a frequency of 0.5–1.0 s−1. This high degassing level reflects a gas-rich magma column and leads to an increased rate in the formation of shallow foams and, hence, an increase in puffing and explosive activity, as well as a higher free surface level and/or gas jet velocity. During weak phases, bubble layers ascend the conduit at a reduced frequency of 0.2–0.3 s−1. During such times the magma column is poor in gas. This leads to a decreased rate of foam layer formation and hence a reduction in puffing and explosive activity, as well as a lower free surface level and/or gas jet velocity. Variations in puffing activity can thus be used to track changes in the rate at which the shallow system is supplied by fresh, gas-rich magma. Our observations indicate that the two degassing styles last from 5 to 40 min and that the switch from one to the other occurs over a matter of minutes. 相似文献
919.
Roberto Lanza 《International Journal of Earth Sciences》1979,68(1):83-92
The remanent magnetization of the andesitic cover of the Sesia-Lanzo Zone has been studied from 16 sites along three transversal sections. The remanent magnetization of the rock is stable and it appears to be primary after a conglomerate test. The mean direction of magnetization is consistent for all sites, but for one exception, with satisfactory values of statistical parameters. Therefore no deformation structures postdating the acquisition of remanent magnetization can be inferred from palaeomagnetic data. The mean direction of magnetization (11 sites, 152 specimens) is: D=135.9, I=–2.9, with 95=8.8. No tectonic correction can yet be made.
Zusammenfassung Die natürliche remanente Magnetisierung der Andesiten, die die Bedeckung der Sesia-Lanzo Zone bilden, ist an 16 Orten gemessen worden, die entlang drei Querdurchschnitten liegen. Das Gestein besitzt eine stabile NRM, die auf Grund eines Konglomeratstest die ursprüngliche sein müßte. Alle Orte, die annehmbare statistische Werte aufweisen, außer einem, haben die gleiche Magnetisierungsrichtung. Die paläomagnetischen Messungen zeigen keine Strukturen aufeinanderfolgender Deformation bei dem Magnetisierungsvorgang. Die durchschnittliche Magnetisierungsrichtung (11 Orte, 152 Gesteinsproben) ist: D = 135,9, I = –2,9, mit 95 = 8,8. Keine tektonische Korrektur wird bisher eingerechnet.
Résumé L'aimantation rémanente des andésites qui constituent la couverture de la Zone Sesia-Lanzo a été mesurée en 16 endroits disposés le long de trois sections transversales. La roche a une aimantation rémanente stable, qui, d'après le test du conglomérat, devrait être originelle. Tous les endroits qui présentent des valeurs statistiques acceptables ont, sauf un, la même direction d'aimantation. Les mesures paléomagnétiques ne révèlent donc pas de structures de déformation consécutive à l'acquisition de l'aimantation rémanente. La direction moyenne de l'aimantation (11 sites, 152 échantillons) est: D=135.9, I=–2.9 avec 95=8.8. On n'a pas apporté, pour l'instant, de correction tectonique.
, Sesia-Lanzo, 16- , . , , , . , , , . , . (11 , 152 ) : D=135,9; =–2,9 95=8,8. .相似文献
920.
Magma supply, magma discharge and readjustment of the feeding system of mount St. Helens during 1980
The landslide and cataclysmic eruption of Mount St. Helens on May 18, 1980 triggered a sequence of explosive eruptions over the following five months. The volume of explosive products from each of these eruptions decreased uniformly over this period, and the character for each eruption progressed from a fairly continuous eruption lasting more than eight hours on May 18 to a series of short bursts, some of which were spaced 12 hours apart, on October 16–18. The transition in the character of these eruption sequences can be explained by a difference between the magma supply rate and the magma discharge rate from a shallow reservoir.The magma supply rate (MSR) is the rate with which magma is supplied to the level where disruption due to vesiculation occurs. It is determined by dividing the dense-rock-equivalent volume of eruptive products by the total duration of each eruption sequence. The magma discharge rate (MDR) is the rate with which the disrupted magma is discharged through the vent. It is determined by dividing the volume of erupted products by the duration of each explosive burst. The relative magnitude of these two quantities controls the temporal evolution of an explosive event. When MDRMSR the explosive phase of the eruption lasts for several hours as a single continuous event. When MDR>MSR, an eruption is characterized by a series of short explosive bursts at intervals of several minutes to several days. The MSR of the eruptions of 1980 decreased with time from 5500 m' s−1 on May 18 to 7 m3 s−2 on October 16–18 and approximately fits an exponential decay. The MDR for the same events remained approximately constant at 2000 m3 s−1. Each explosive event has been followed by an aftershock-like series of earthquakes located beneath the volcano at depth mostly between 7 and 14 km. The seismic energy released during each of these series is proportional to the corresponding volume of erupted magma. Deformation data between June and November, 1980 indicate a subsidence of the volcanic structure which can be modeled by a volume collapse of 0.25 km3 located at 9 km depth.We propose a model in which magma is supplied from depths of 7–14 km through a narrow conduit during each eruption. It erupts to the surface at a uniform rate during each eruption. The deep seismic activity following each eruption is related to a readjustment and volume decrease in the deep feeding system. The decrease of the MSR over time is explained by an increase in the viscosity of a progressively water-depleted magma. The amount of water necessary to explain the observed decrease of the MSR is of the order of 4.6%. 相似文献