Photometric and spectral analysis of the distribution of crystalline and amorphous ices on Enceladus as seen by Cassini     

Sarah F. Newman  B.J. Buratti  R. Jaumann  T. Momary 《Icarus》2008,193(2):397-406

Photometric and spectral analysis of data from the Cassini Visual and Infrared Mapping Spectrometer (VIMS) has yielded significant results regarding the properties and composition of the surface of Saturn's satellite Enceladus. We have obtained spectral cubes of this satellite, containing both spatial and spectral information, with a wavelength distribution in the infrared far more extensive than from any previous observations and at much higher spatial resolution. Using a composite mosaic of the satellite, we map the distribution of crystalline and amorphous ices on the surface of Enceladus according to a “crystallinity factor” and also the depth of the temperature- and structure-dependent 1.65 micron water-ice band. These maps show the surface of Enceladus to be mostly crystalline, with a higher degree of crystallinity at the “tiger-stripe” cracks and a larger amorphous signature between these stripes. These results suggest recent geological activity at the “tiger stripe” cracks and an intriguing atmospheric environment over the south pole where amorphous ice is produced either through intense radiative bombardment, flash-freezing of cryovolcanic liquid, or rapid condensation of water vapor particles on icy microspherules or on the surface of Enceladus.  相似文献   

Galactic civilizations: Population dynamics and interstellar diffusion     

William I. Newman  Carl Sagan 《Icarus》1981,46(3):293-327

The interstellar diffusion of galactic civilizations is reexamined by potential theory; both numerical and analytical solutions are derived for the nonlinear partial differential and difference equations which specify a range of relevant models, drawn from blast wave physics, soil science, and, especially, population biology. An essential feature of these models is that, for all civilizations, population growth must be limited by the carrying capacity of the planetary environments. Dispersal is fundamentally a diffusion process; a directed density-dependent diffusivity describes interstellar emigration. We concentrate on two models, the first describing zero population growth (ZPG) and the second which also includes local growth and saturation of a planetary population, and for which we find an asymptotic travelling wave solution. For both models the colonization wavefront expands slowly and uniformly, but only the frontier worlds are sources of further expansion. For nonlinear diffusion with growth and saturation, the colonization wavefront from the nearest independently arisen galactic civilization can have reached the Earth only if its lifetime exceeds 2.6 × 10⁶ years. If discretization can be neglected, the critical lifetime is 2.0 × 10⁷ years. For ZPG the corresponding number is 1.3 × 10¹⁰ years. These numerical results depend on our choices for the specific emigration rate, the distribution of colonizable worlds, and, in the second model, the population growth rate; but the dependence on these parameters is entrancingly weak. We conclude that the Earth is uncolonized not because interstellar spacefaring societies are rare, but because there are too many worlds to be colonized in the plausible lifetime of the colonization phase of nearby galactic civilizations. This phase is, we contend, eventually outgrown. We also conclude that, except possibly early in the history of the Galaxy, there are no very old galactic civilizations with a consistent policy of conquest of inhabited worlds; there is no Galactic Empire. There may, however, be abundant groups of ～10⁵ to 10⁶ worlds linked by a common colonial heritage. The radar and television announcement of an emerging technical society on Earth may induce a rapid response by nearby civilizations, thus newly motivated to reach our system directly rather than by diffusion.  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   

Reply to comment on “Late Wisconsinan glaciation models of northern Maine and adjacent Canada”     

Andrew N. Genes  William A. Newman 《Quaternary Research》1983,19(2):272-274

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The Failure of Academic Boycotts          下载免费PDF全文

David Newman 《Geographical review》2016,106(2):264-269

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Timing and duration of hydrological transitions in Arctic polygonal ground from stable isotopes     

Nathan Alec Conroy  Brent David Newman  Jeffrey Martin Heikoop  George Bradford Perkins  Xiahong Feng  Cathy Jean Wilson  Stan Duane Wullschleger 《水文研究》2020,34(3):749-764

Land surface models and Earth system models that include Arctic landscapes must capture the abrupt hydrological transitions that occur during the annual thaw and deepening of the active layer. In this work, stable water isotopes (δ²H and δ¹⁸O) are used to appraise hydrologically significant transitions during annual landscape thaw at the Barrow Environmental Observatory (Utqiaġvik, Alaska). These hydrologically significant periods are then linked to annual shifts in the landscape energy balance, deduced from meteorological data and described by the microclimatic periods: Winter, Pre-Melt, Melt, Post-Melt, Summer, and Freeze-Up. The tight coupling of the microclimatic periods with the hydrological transitions supports the use of microclimatic periods as a means of linking polygonal surface water hydrology to meteorological datasets, which provides a mechanism for improving the representation of polygonal surface water hydrology in process-based models. Rayleigh process reconstruction of the isotopic changes revealed that 19% of winter precipitation was lost to sublimation prior to melting and that 23% of surface water was lost to evaporation during the first 10 days post-melt. This agrees with evaporation rates reported in a separate study using an eddy covariance flux tower located nearby. An additional 17% was lost to evaporation during the next 33 days. Stable water isotopes are also used to identify the dominant sources of surface water to various hydrogeomorphological features prevalent in polygonal terrain (a lake, a low centre polygon centre, troughs within the rims of low centre polygons, flat centre polygon troughs, a high centre polygon trough, and drainages). Hydrogeomorphologies that retained significant old water or acted as snow drifts are isotopically distinct during the Melt Period and therefore are easily distinguished. Biogeochemical changes related to the annual thaw are also reported and coupled to the hydrological transitions, which provides insight into the sources and sinks of these ions to and from the landscape.  相似文献   

Larval Pacific Herring (Clupea pallasi) Survival in Suspended Sediment     

Frederick J. Griffin  Theresa DiMarco  Karl L. Menard  Joe A. Newman  Edmund H. Smith  Carol A. Vines  Gary N. Cherr 《Estuaries and Coasts》2012,35(5):1229-1236

Pacific herring early life stages provide good model systems for studying effects of suspended sediments on estuarine organisms. To investigate effects on the herring larval stage, we used environmentally relevant particle concentrations for San Francisco Bay (200?C400?mg/L of particles <50???m in size) and exposure times of 16?h in a novel two-pump sediment suspension mesocosm. There were no mortalities during the 16-h suspended sediment incubation. Following sediment exposure, larvae were cultured in sediment-free water for up to 10?days during which survival and condition were measured. None were affected by previous sediment treatment. Four criteria for larval condition included growth, heart rate, prey capture, and critical swimming velocity. These results provide a framework for implementing regulatory decisions on anthropogenic activities such as dredging.  相似文献   

New advances in three dimensional transient electromagnetic inversion   总被引：6，自引：0，他引：6  

Gregory A. Newman  Michael Commer 《Geophysical Journal International》2005,160(1):5-32

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Mineralogy,petrology, and distribution of meteorites at the Whitecourt crater,Alberta, Canada          下载免费PDF全文

Jennifer D. Newman  Christopher D. K. Herd 《Meteoritics & planetary science》2015,50(2):305-317

The Whitecourt meteorite impact crater, Alberta, Canada is a rare example of a well‐preserved small impact structure, with which thousands of meteorite fragments are associated. As such, this crater represents a unique opportunity to investigate the effect of a low‐energy impact event on an impacting iron bolide. Excellent documentation of meteorite fragment locations and characteristics has generated a detailed distribution map of both shrapnel and regmaglypted meteorite types. The meteorites' distribution, and internal and external characteristics support a low‐altitude breakup of the impactor which caused atmospherically ablated (regmaglypted) meteorites to fall close to the crater and avoid impact‐related deformation. In contrast, shrapnel fragments sustained deformation at macro‐ and microscales resulting from the catastrophic disruption of the impactor. The impactor was significantly fragmented along pre‐existing planes of weakness, including kamacite lamellae and inclusions, resulting in a bias toward low‐mass (<100 g) fragments. Meteorite mineralogy was investigated and the accessory minerals were found to be dominated by sulfides and phosphides with rare carlsbergite, consistent with other low‐Ni IIIAB iron meteorites. Considerations of the total mass of meteoritic material recovered at the site relative to the probable fraction of the impactor that was preserved based on modeling suggests that the crater was formed by a higher velocity, lower mass impactor than previously inferred.  相似文献   

The DEEP2 galaxy redshift survey: the evolution of the blue fraction in groups and the field     

Brian F. Gerke  Jeffrey A. Newman  S. M. Faber  Michael C. Cooper  Darren J. Croton  Marc Davis  Christopher N. A. Willmer  Renbin Yan  Alison L. Coil  Puragra Guhathakurta  David C. Koo  Benjamin J. Weiner 《Monthly notices of the Royal Astronomical Society》2007,376(4):1425-1444

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