Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ω PE     

G. Thejappa  R. G. Stone  M. L. Goldstein 《Astrophysics and Space Science》1996,243(1):195-198

We present the experimental verification of existing theoretical models of emission mechanisms of solar type III bursts at the second harmonic of the plasma frequency, _pe . This study is based on the detection of Langmuir and envelope solitons by the Ulysses spacecraft inside three type III burst source regions. We show that the oscillating-two-stream instability, coherent radiation by Langmuir solitons and stochastic phase mixing of the Langmuir waves in the strong turbulence regime are the appropriate emission mechanisms at 2 _pe .  相似文献   

A radiation-driven disc wind model for massive young stellar objects     

Janet E. Drew  Daniel Proga  & James M. Stone 《Monthly notices of the Royal Astronomical Society》1998,296(1):L6-L10

The generation of magnetic fields by a battery, operating in an ion–electron plasma around a Kerr black hole, is studied in the 3+1 split of the Kerr metric. It is found that the gravitomagnetic contributions to the electron partial pressure are able to drive currents. The strength of the equilibrium magnetic field should be higher than for the classical Biermann battery, which is found to operate in this relativistic context as well, since the gravitomagnetic driving terms can less easily be quenched than the classical ones. In axisymmetry the battery can induce only toroidal magnetic fields. Once a toroidal magnetic field is present, however, the coupling of gravitomagnetic and electromagnetic fields generates a poloidal magnetic field even in axisymmetry. A rotating black hole, embedded in plasma, will therefore always generate toroidal and poloidal magnetic fields.  相似文献   

Rising heat wave trends in large US cities     

Dana Habeeb  Jason Vargo  Brian Stone Jr. 《Natural Hazards》2015,76(3):1651-1665

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The pedigree and influence of fossil collections from the Falkland Islands: From Charles Darwin to continental drift     

Philip Stone  Adrian W.A. Rushton 《Proceedings of the Geologists' Association. Geologists' Association》2012,123(3):520-532

The Falkland Islands are typical of remote territories in that their early geological exploration was piecemeal and opportunistic. Whilst the resulting fossil collections (dominantly a Devonian fauna of the Malvinokaffric realm) remain the basis for modern interpretations, published accounts misrepresent their extent and provenance. Charles Darwin first discovered fossils during his 1833 visit aboard HMS Beagle, with subsequent British collections acquired in 1842 and 1876, respectively, by the Erebus and Terror and Challenger expeditions and in 1903 by the Scotia expedition. Darwin's collection, and much of the other material, is now held by The Natural History Museum, London (NHM) but some Darwin specimens were assimilated into other collections whilst at least one NHM ‘Darwin’ specimen was not collected by him. There may also be some uncertainty as to the origin of the Scotia collection, now held in Edinburgh by National Museums Scotland, in relation to a contemporary Swedish collection now held in Stockholm. The NHM holdings were supplemented by a number of enigmatic donations from private individuals and then by fossils collected during the first ‘official’ geological survey of the islands in 1920–1922. Meanwhile a large collection was built up in New York through collaboration in 1909 with a local collector – the Governor's wife! The regional associations of the fossils established the African heritage of Falklands geology, and thereby contributed to an understanding of continental drift as the mechanism for the fragmentation of the Gondwana supercontinent. The Falkland Islands are now regarded as a rotated microplate created during the break-up.  相似文献   

Buoyant radio lobes in a viscous intracluster medium     

Christopher S. Reynolds  Barry McKernan  rew C. Fabian  James M. Stone  John C. Vernaleo 《Monthly notices of the Royal Astronomical Society》2005,357(1):242-250

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Hydromagmatic amphibole in komatiitic, tholeiitic and ferropicritic units, Abitibi greenstone belt, Ontario and Québec: evidence for Archaean wet basic and ultrabasic melts     

W. E. Stone  E. Deloule  M. S. Stone 《Mineralogy and Petrology》2003,77(1-2):39-65

Summary ?Detailed petrographic, electron microprobe and ion probe studies of Archaean hydromagmatic amphiboles from the Abitibi greenstone belt, Canada, yield new insights into the origin of Al-undepleted komatiitic and Al-depleted tholeiitic and ferropicritic melts. The amphiboles are present in peridotite layers and basal chill zones of thick differentiated basic and ultrabasic sills and flows, and are titanian pargasite–hastingsite in composition. They can be grouped into two petrographic types: (1) amphibole in the groundmass; and (2) amphibole-bearing melt inclusions. The groundmass amphiboles are oikocrysts, rims and interstitial grains, present in minor to major amounts. The oikocrysts host cumulus olivines (Fo_83–84) that are rounded in shape, embayed, and smaller in size. The amphibole-bearing melt inclusions are hosted in cumulus olivines (Fo_83–84 in komatiitic rocks and Fo₇₉ in tholeiitic rocks), spherical to ovoid in shape, 50–500 μm in size, and dominated modally by amphibole. The melt inclusions also contain euhedral chromite and aluminous spinel and micrometric clinopyroxene and glass, and sub-micrometric iron–nickel sulphide, chloro-apatite and ilmenite. In-situ ion probe analyses indicate the amphibole is: (1) enriched in Nb, LREE and Zr and depleted in Sr and HREE relative to primitive mantle; (2) contains up to 1–3 wt% H₂O; and (3) overall displays δD values from 50‰ to −140‰, including many values in the accepted magmatic range of −60‰ to −90‰. The petrographic relationships and geochemical compositions, and comparisons to experimental systems, indicate amphibole formation by subsolidus reaction of residual hydrous silicate melt with olivine and clinopyroxene. Some of the hydrous melt intruded and was entrapped as secondary melt inclusions within relict olivine. Rapid crystallization of the hydrous melt inclusions formed amphibole+clinopyroxene±glass±spinel or solely glass. Bulk compositions of the melt inclusions, comparisons to experimental phase equilibria, and presence of magmatic water suggest amphibole crystallisation from olivine → pyroxene residual melts with at least 2–3 wt% H₂O during rapid solidification of the host units. Adjustment for anhydrous phase crystallization (mainly olivine) suggests the initial melts contained 1–2 wt% H₂O. Such high H₂O contents and the magmatic δD compositions are consistent with the participation of H₂O in melt petrogenesis. However, most Abitibi komatiites and tholeiites lack hydromagmatic minerals, making it difficult to attribute all basic and ultrabasic melts to melting in hydrous Archaean mantle. The favoured model is that some Abitibi basic and ultrabasic melts were wet and some were dry, as well as Al-depleted or Al-undepleted. Received July 24, 2001; revised version accepted January 9, 2002  相似文献   

> 25 MeV Proton Events Observed by the High Energy Telescopes on the STEREO A and B Spacecraft and/or at Earth During the First ∼ Seven Years of the STEREO Mission     

I. G. Richardson  T. T. von Rosenvinge  H. V. Cane  E. R. Christian  C. M. S. Cohen  A. W. Labrador  R. A. Leske  R. A. Mewaldt  M. E. Wiedenbeck  E. C. Stone 《Solar physics》2014,289(8):3059-3107

Using observations from the High Energy Telescopes (HETs) on the STEREO A and B spacecraft and similar observations from near-Earth spacecraft, we summarize the properties of more than 200 individual >?25 MeV solar proton events, some detected by multiple spacecraft, that occurred from the beginning of the STEREO mission in October 2006 to December 2013, and provide a catalog of these events and their solar sources and associations. Longitudinal dependencies of the electron and proton peak intensities and delays to onset and peak intensity relative to the solar event have been examined for 25 three-spacecraft particle events. Expressed as Gaussians, peak intensities fall off with longitude with σ=47±14^° for 0.7?–?4 MeV electrons, and σ=43±13^° for 14?–?24 MeV protons. Several particle events are discussed in more detail, including one on 3 November 2011, in which ～?25 MeV protons filled the inner heliosphere within 90 minutes of the solar event, and another on 7 March 2012, in which we demonstrate that the first of two coronal mass ejections that erupted from an active region within ～?1 hour was associated with particle acceleration. Comparing the current Solar Cycle 24 with the previous cycle, the first >?25 MeV proton event was detected at Earth in the current solar cycle around one year after smoothed sunspot minimum, compared with a delay of only two months in Cycle 23. Otherwise, solar energetic particle event occurrence rates were reasonably similar during the rising phases of Cycles 23 and 24. However, the rate declined in 2013, reflecting the decline in sunspot number since the peak in the northern-hemisphere sunspot number in November 2011. Observations in late 2013 suggest that the rate may be rising again in association with an increase in the southern sunspot number.  相似文献   

An assessment of flood emergency plans in England and Wales,France and the Netherlands   总被引：1，自引：0，他引：1  

Darren?LumbrosoEmail author  Karin?Stone  Freddy?Vinet 《Natural Hazards》2011,58(1):341-363

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Modeling hurricane waves and storm surge using integrally-coupled,scalable computations   总被引：1，自引：0，他引：1  

J.C. Dietrich  M. Zijlema  J.J. Westerink  L.H. Holthuijsen  C. Dawson  R.A. Luettich Jr.  R.E. Jensen  J.M. Smith  G.S. Stelling  G.W. Stone 《Coastal Engineering》2011

The unstructured-mesh SWAN spectral wave model and the ADCIRC shallow-water circulation model have been integrated into a tightly-coupled SWAN + ADCIRC model. The model components are applied to an identical, unstructured mesh; share parallel computing infrastructure; and run sequentially in time. Wind speeds, water levels, currents and radiation stress gradients are vertex-based, and therefore can be passed through memory or cache to each model component. Parallel simulations based on domain decomposition utilize identical sub-meshes, and the communication is highly localized. Inter-model communication is intra-core, while intra-model communication is inter-core but is local and efficient because it is solely on adjacent sub-mesh edges. The resulting integrated SWAN + ADCIRC system is highly scalable and allows for localized increases in resolution without the complexity or cost of nested meshes or global interpolation between heterogeneous meshes. Hurricane waves and storm surge are validated for Hurricanes Katrina and Rita, demonstrating the importance of inclusion of the wave-circulation interactions, and efficient performance is demonstrated to 3062 computational cores.  相似文献   

Evaluation of two WAM white capping parameterizations using parallel unstructured SWAN with application to the Northern Gulf of Mexico, USA     

S. Mostafa Siadatmousavi  F. JoseG.W. Stone 《Applied Ocean Research》2011,33(1):23-30

The performance of two well accepted formulations for white capping and wind input of third generation wave models, viz., WAM-3 and WAM-4, were investigated using parallel unstructured SWAN (PunSWAN). Several alternative formulations were also considered to evaluate the effects of higher order steepness and wave number terms in white capping formulations. Distinct model configurations were calibrated and validated against available in situ measurements from the Gulf of Mexico. The results showed that some of the in situ calibrated models outperform the saturation level calibrated models in reproducing the idealized wave growth curves. The simulation results also revealed that increasing the power of the steepness term can enhance the accuracy of significant wave height (H_s), at the expense of a higher bias for large waves. It also has negative effects on mean wave period (T_a) and peak wave period (T_p). It is also demonstrated that the use of the quadratic wave number term in the WAM-3 formulation, instead of the existing linear term, ameliorates the T_a underestimation; however, it results in the model being unable to reach any saturation level. In addition, unlike H_s and T_p, it has been shown that T_a is sensitive to the use of the higher order WAM-4 formulation, and the bias is decreased over a wide range of wave periods. However, it also increases the scatter index (SI) of simulated T_a. It is concluded that the use of the WAM-4 wind input formulation in conjunction with the WAM-3 dissipation form, is the most successful case in reproducing idealized wave growth curves while avoiding T_a underestimation of WAM-3 and a potential spurious bimodal spectrum of WAM-4; consequently, this designates another perspective to improve the overall performance of third generation wave models.  相似文献