The Air Force Global Weather Central operational boundary-layer model     

Kenneth D. Hadeen  Arnold L. Friend 《Boundary-Layer Meteorology》1972,3(1):98-112

A limited-area seven-layer physical-numerical model for the lower tropospheric region (surface - 1600m) is described. The grid interval, approximately 190km, is half that of the standard numerical weather-prediction grid used in the hemispheric free atmospheric operational model at the Air Force Global Weather Central (AFGWC). This model is an integral part of the complete AFGWC meso-scale (sub-synoptic) numerical analysis and prediction system and is used to provide greater horizontal and vertical resolution in both numerical analyses and forecasts.Important features of this boundary-layer model include: a completely automated objective analysis of input data; the transport of heat and moisture by three-dimensional wind flow; latent heat exchange in water substance phase changes; and eddy fluxes of heat and water vapor.Input data are conventional synoptic surface and upper air reports. Other operational AFGWC prediction models provide input in the form of horizontal wind components at the upper boundary and an estimate of cloudiness above the boundary layer. Forecasts for the lower boundary and surface layer are empirically derived. Despite some approximations which broadly simplify the real planetary boundary-layer processes, operational use for highly weather-sensitive Air Weather Service support indicates that the model is capable of producing accurate detailed forecasts for periods of up to 24h.A modified version of this paper was presented at the IUGG-IAMAP-AMS conference on Planetary Boundary Layers at Boulder, Colo., 18–21 March, 1970, and at the 5th annual Congress of the Canadian Meteorological Society, at Macdonald College, 12–14 May, 1971.  相似文献   

Profils de réfraction en Ligurie     

Maurice Recq 《Pure and Applied Geophysics》1972,101(1):155-161

Résumé Les profils sismiques réalisés en Ligurie confirment l'existence d'un accident crustal important dans la région de Savona. La vitesse apparente voisine de 7 km/s observée vers Imperia entre 10 et 12 km de profondeur pourrait être associée à l'extension possible vers le Sud de l'anomalie d'Ivrea.

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Summary Seismic profiles in the Ligurian country confirm the existence of an important accident in the crust situated in the Savona region. The apparent velocity of about 7 km/s observed near Imperia and corresponding to a depth of 10–12 km could be associated with a possible southward extension of the Ivrea zone.

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Centre National de la Recherche Scientifique. Institute de Physique du Globe, Université de Paris VI, 11 Quai Saint-Bernard, Paris V^o. Contribution I.P.G. N.S. n^o 28.  相似文献   

Composition and origin of serpentinites from the Mid-Atlantic Ridge near 24° and 30° North Latitude     

Akiho Miyashiro  Fumiko Shido  Maurice Ewing 《Contributions to Mineralogy and Petrology》1969,23(2):117-127

Serpentinites occur in transverse fracture zones and adjacent areas in the Mid-Atlantic Ridge near 24° and 30° N. In two fracture zones, about 700 km distant from each other, serpentinites show practically the same trend and range of variation in chemical composition. Their CaO content ranges from 2.05 to 0.07% by weight. Serpentinites relatively high in CaO content contain pargasite, whereas those relatively low in CaO do not. Serpentinites relatively high in CaO are chemically similar to high-temperature peridotites which are widely believed to have been derived from the upper mantle. With a decrease in CaO, the Al₂O₃, TiO₂, K₂O and FeO contents and the Fe/Mg ratio tend to decrease, whereas the H₂O⁺ content tends to increase. This compositional variation is probably due partly to heterogeneity of uper mantle peridotite from which the serpentinites were derived, and partly to chemical migration during serpentinization. The interior of the Mid-Atlantic Ridge may be mainly made up of serpentinites. Alternatively, the Mid-Atlantic Ridge Serpentinites may have been formed by serpentinization of peridotites that were intruded into fracture zones from a great depth.Lamont-Doherty Geological Observatory Contribution No. 1354.  相似文献   

Diversity and origin of abyssal tholeiite from the Mid-Atlantic Ridge near 24° and 30° North latitude     

Akiho Miyashiro  Fumiko Shido  Maurice Ewing 《Contributions to Mineralogy and Petrology》1969,23(1):38-52

On cursory examination of hand specimens and thin sections, the abyssal tholeiite in a dredge haul may appear to be uniform in composition. Chemical analyses of a considerable number of fragments, however, have always revealed the existence of regular compositional variation in them. The MgO content decreases with increasing SiO₂. In abyssal tholeiites with relatively low Al₂O₃ contents, the SiO₂, total iron, Na₂O and P₂O₅ contents tend to increase and the MgO content tends to decrease with increasing iron/magnesia ratio, probably owing to crystallization differentiation.In a certain dredge haul, high-alumina abyssal tholeiites (with Al₂O₃ contents near or over 17%) occur in association with low-alumina abyssal tholeiites. The magma of high-alumina abyssal tholeiites would be generated from that of low-alumina abyssal tholeiites by differentiation at a depth around 30 km.In pillow lavas of abyssal tholeiite free from weathering and metamorphism, the chilled rim of the pillow usually has virtually the same chemical composition as the more crystalline core except for a decrease of K₂O content toward the rim. On the other hand, the weathered rim of pillow lavas shows marked compositional change. The Fe₂O₃/FeO ratio of unweathered abyssal tholeiite is in the range of 0.1 to 0.3. This ratio and the H₂O^– and H₂O⁺ contents increase with advancing weathering.Lamont-Doherty Geological Observatory Contribution No. 1339  相似文献   

The Pn velocity under the Gulf of Genoa     

Maurice Recq 《Earth and Planetary Science Letters》1973,20(3):447-450

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Advances in Paleozoic Botany: M. Streel,P.M. Bonamo and M. Fairon-Demaret (Editors), 1972. Elsevier,Amsterdam, 223 pp., Dfl.50.00     

C.A. Arnold 《Earth》1973,9(3):279-280

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Lunar structure and dynamics - results from the apollo passive seismic experiment     

Gary Latham  Maurice Ewing  James Dorman  Yosio Nakamura  Frank Press  Nafi Toksőz  George Sutton  Fred Duennebier  David Lammlein 《Earth, Moon, and Planets》1973,7(3-4):396-421

Analysis of seismic signals from man-made impacts, moonquakes, and meteoroid impacts has established the presence of a lunar crust, approximately 60 km thick in the region of the Apollo seismic network; an underlying zone of nearly constant seismic velocity extending to a depth of about 1000 km, referred to as the mantle; and a lunar core, beginning at a depth of about 1000 km, in which shear waves are highly attenuated suggesting the presence of appreciable melting. Seismic velocitites in the crust reach 7 km s^–1 beneath the lower-velocity surface zone. This velocity corresponds to that expected for the gabbroic anorthosites found to predominate in the highlands, suggesting that rock of this composition is the major constituent of the lunar crust. The upper mantle velocity of about 8 km s^–1 for compressional waves corresponds to those of terrestrial olivines, pyroxenites and peridotites. The deep zone of melting may simply represent the depth at which solidus temperatures are exceeded in the lower mantle. If a silicate interior is assumed, as seems most plausible, minimum temperatures of between 1450°C and 1600°C at a depth of 1000 km are implied. The generation of deep moonquakes, which appear to be concentrated in a zone between 600 km and 1000 km deep, may now be explained as a consequence of the presence of fluids which facilitate dislocation. The preliminary estimate of meteoroid flux, based upon the statistics of seismic signals recorded from lunar impacts, is between one and three orders of magnitude lower than previous estimates from Earth-based measurements.Paper dedicated to Professor Harold C. Urey on the occasion of his 80th birthday on 29 April, 1973.  相似文献   

Stratospheric in situ measurements of H₂SO₄ and HSO₃ vapors during a volcanically active period     

S. Qiu  F. Arnold 《Planetary and Space Science》1984,32(1):87-95

In situ measurements of stratospheric H₂SO₄ and HSO₃vapors using passive chemical ionization mass spectrometry were made in October 1982 after the eruption of volcano El Chichon. Data were obtained between about 20 and 41 km showing [H₂SO₄ + HSO₃] sum concentrations between about 10⁴ and 2 × 10⁵ cm^?3 below 29 km and a steep rise above this altitude. Maximum [H₂SO₄ + HSO₃] values of about 3 × 10⁶ cm^?3 are reached above 35 km.Partial [HSO₃] concentrations increase above 34 km reaching about $\text{4 × 10}{}^5\text{cm}{}^{\mathrm{?3}}$ around 40 km. From the measurements it is concluded that H₂SO₄ and probably HSO₃photolysis have an important influence above 34 km leading to the observed increase of [HSO₃] and a depletion of H₂SO₄vapor.It also seems that the data support the view of heterogeneous HSO₃ removal. If correct, this would imply that stratospheric aerosols are formed primarily from HSO₃ rather than H₂SO₄vapor.  相似文献   

NOAA AR 8210: EVOLUTION AND FLARES FROM MULTIBAND DIAGNOSTICS     

Warmuth  Alexander  Hanslmeier  Arnold  Messerotti  Mauro  Cacciani  Alessandro  Moretti  Pier Francesco  Otruba  Wolfgang 《Solar physics》2000,194(1):103-120

NOAA 8210 has been a region showing a remarkable level of activity well before solar maximum. Dominated by a large, rapidly rotating spot, it produced several intense flares during its disk passage at the end of April–beginning of May 1998. We examine the development of AR 8210 in H and white light (WL) and study the evolution of its complex magnetic topology. While the other principal flares are briefly reviewed, the great X1.1/3B flare of 2 May, which was observed at Kanzelhöhe Solar Observatory during a SOHO/UVCS ground support campaign, is studied in detail. This event has been documented in full-disk H and Na-D intensitygrams, Dopplergrams, and magnetograms, with a time cadence of one minute each. The flare was associated with a CME and produced significant geomagnetic effects. Furthermore, we point out the perspectives for our planned Flare Monitoring and Alerting System, since the two new instruments (Magneto-Optical Filter and Digital H camera), which made their first operational run with the campaign, are crucial components for this program.  相似文献   

On the physics of the Atlantic Multidecadal Oscillation   总被引：1，自引：0，他引：1  

Henk A. Dijkstra  Lianke te Raa  Maurice Schmeits  Jeroen Gerrits 《Ocean Dynamics》2006,56(1):36-50

The Atlantic Multidecadal Oscillation (AMO) is a pronounced signal of climate variability in the North Atlantic sea-surface temperature field. In this paper, we propose an explanation of the physical processes responsible for the timescale and the spatial pattern of the AMO. Our approach involves the analysis of solutions of a hierarchy of models. In the lowest member of the model hierarchy, which is an ocean-only model for flow in an idealized basin, the variability shows up as a multidecadal oscillatory mode which is able to destabilize the mean thermohaline circulation. In the highest member of the model hierarchy, which is the Geophysical Fluid Dynamics Laboratory R30 climate model, multidecadal variability is found as a dominant statistical mode of variability. The connection between both results is established by tracing the spatial and temporal expression of the multidecadal mode through the model hierarchy while monitoring changes in specific quantities (mechanistic indicators) associated with its physics. The proposed explanation of the properties of the AMO is eventually based on the changes in the spatial patterns of variability through the model hierarchy.Responsible Editor: Tal Ezer  相似文献