Late Devensian and Holocene landscape change in the uplands of the Isle of Man     

R. C. Chiverrell  G. S. P. Thomas  A. M. Harvey 《Geomorphology》2001,40(3-4)

The Late Glacial and Holocene geomorphology of the Manx uplands has received scant attention in previous researches. Solifluction deposits and terraces provide the earliest evidence for geomorphic activity after deglaciation. Fluvial incision into drift-choked valleys is correlated with the formation of the large mountain front alluvial fans that flank the Manx uplands. Formation of these alluvial fans is constrained to 15,000–10,500 cal. years BP by ¹⁴C dates on organic deposits beneath and above the alluvial fan gravels. Alluvial fan and river terraces along four valleys postdate this incision. Optically Stimulated Luminescence (OSL) and ¹⁴C dating provide a tentative chronology for these landforms. The higher terraces are Late Glacial fluvial surfaces that were probably occupied by rivers into the Holocene. Incision during the Late Holocene led to the abandonment of the higher surfaces, producing a suite of younger river terraces and alluvial fan surfaces. Independent dating constrains this fluvial activity to post-Bronze Age (3500–2800 cal. years BP). Increased human activity and climatic change during the Late Holocene are possible causes for this increased geomorphic activity.  相似文献   

Monitoring the Comprehensive Nuclear-Test-Ban Treaty     

B. J. Mitchell 《Pure and Applied Geophysics》2001,158(8):1339-1340

  相似文献   

Development of a risk-hedging CO2-emission policy, part I: Risks of unrestrained emissions     

L. D. Danny Harvey 《Climatic change》1996,34(1):1-40

A rational global strategy with respect to greenhouse-gas emissions would seek to minimize total risk, which is the sum of the risk of negative impacts due to climatic change associated with a given level of emissions, and the risks associated with the process of achieving that emission level. Given the existence of reducible uncertainties in estimating these risks, and the possibility that an emission target thought to minimize total risk is later found to be not strict enough, a risk-hedging strategy is a more realistic policy objective. This paper is Part I of a two-part series in which these risks are reviewed and an interim risk-hedging emission level is proposed. Here, the risks associated with unrestrained greenhouse-gas emissions are reviewed. In particular, the carbon-cycle response to continuing CO₂ emissions; the heat trapping of projected greenhouse gas increases in comparison to other anthropogenic and natural heating or cooling perturbations; the climatic response to heating perturbations; and the impacts of projected climatic change on global agriculture, forests, coastal regions, coral reefs, water resources, terrestrial species, stratospheric and tropospheric ozone, and human comfort and welfare are critically examined. It is concluded that unrestrained emissions of greenhouse gases pose real and substantial risks to human societies and to ecosystems, and that these risks are likely to grow substantially if the climate warms beyond that associated with a CO₂ doubling. These risks clearly justify some action to limit emissions. The magnitude of emission restraint that is justified depends not only on the risks reviewed here, but also on the risks associated with measures to limit greenhouse-gas emissions, which are reviewed in Part II.  相似文献   

Notes on the geology of Western Irak and Northern Saudi Arabia     

Raoul C. Mitchell 《International Journal of Earth Sciences》1959,46(2):476-493

  相似文献   

Predictive deconvolution applied to long-range seismic refraction observations     

B. J. Mitchell  M. Landisman  Z. A. Der 《Pure and Applied Geophysics》1972,96(1):127-133

Summary The method of predictive deconvolution is described and applied to seismograms from the 1963 Lake Superior experiment. The process is successful in removing shot-generated reverberations and sometimes reveals seismic phases which are not easily identifiable on the original seismograms.  相似文献   

Diamond genesis — A synthesis of opposing views     

R. H. Mitchell  J. H. Crocket 《Mineralium Deposita》1971,6(4):392-403

Estimates of the pressure and temperature in the region of kimberlite magma generation are compatible with the formation of diamond in its own thermodynamic stability field as deduced from high pressure experimental synthesis of diamond. However, if diamond growth is allowed only within its stability field, preservation during ascent of kimberlite magma and many properties of diamond distribution in kimberlite pipes as well as some of the geochemical properties of diamond are very difficult to explain. Metastable diamond growth in the laboratory is well established and its occurrence in natural systems is proposed. A theory of genesis with synthesis of diamond seed nucleii in kimberlite magma at depth in the mantle and with continued metastable growth during ascent and in kimberlite magma pools at the base of the crust is proposed. Eruption of kimberlite pipes to the surface terminates diamond growth.

---

Résumé Les estimations de la pression et de la température dans la région de formation du magma kimberlitique sont compatibles avec la formation du diamant dans son propre domaine de stabilité thermodynamique comme déduit des données obtenues par la synthèse du diamant à haute pression. Néanmoins, en admettant la croissance du diamant seulement dans son propre domaine de stabilité, il est très difficile d'expliquer sa preservation pendant l'ascension du magma kimberlitique, beaucoup de ses caractéristiques de répartition dans les pipes kimberlitiques ainsi que certaines propriétés géochimiques. L'évolution du diamant métastable en laboratoire est bien connue et nous suggérons donc l'existence de cet état dans les systèmes naturels. On propose une théorie envisageant la formation du diamant en partant d'une synthèse de noyaux de germes de diamant dans le magma kimberlitique à profondeur dans le manteau suivie d'une évolution métastable continuelle pendant l'ascension de ce magma kimberlitique et dans les chambres magmatiques à la base de la croûte terrestre. L'éruption des pipes kimberlitiques à la surface termine la croissance du diamant.

  相似文献   

ISO Far-IR spectroscopy of IR-bright galaxies and ULIRGs     

J. Fischer  M.L. Luhman  S. Satyapal  M.A. Greenhouse  G.J. Stacey  C.M. Bradford  S.D. Lord  J.R. Brauher  S.J. Unger  P.E. Clegg  H.A. Smith  G. Melnick  J.W. Colbert  M.A. Malkan  L. Spinoglio  P. Cox  V. Harvey  J.-P Suter  V. Strelnitski 《Astrophysics and Space Science》1999,266(1-2):91-98

Based on far-infrared spectroscopy of a small sample of nearbyinfrared-bright and ultraluminous infrared galaxies (ULIRGs) with theISO Long Wavelength Spectrometer we find adramatic progression in ionic/atomic fine-structure emission line andmolecular/atomic absorption line characteristics in these galaxiesextending from strong [O III]52,88 m and [N III]57 m lineemission to detection of only faint [C II]158 m line emissionfrom gas in photodissociation regions in the ULIRGs. The molecularabsorption spectra show varying excitation as well, extending fromgalaxies in which the molecular population mainly occupies the groundstate to galaxies in which there is significant population in higherlevels. In the case of the prototypical ULIRG, the merger galaxy Arp220, the spectrum is dominated by absorption lines of OH, H₂O, CH,and [O I]. Low [O III]88 m line flux relative to the integratedfar-infrared flux correlates with low excitation and does not appear tobe due to far-infrared extinction or to density effects. A progressiontoward soft radiation fields or very dusty H II regions may explainthese effects.  相似文献   

Meteorite stranding surfaces and the Greenland icesheet     

Ralph P. Harvey  Anders Meibom  Henning Haack 《Meteoritics & planetary science》2001,36(6):807-816

Abstract— Thirty years of recoveries in East Antarctica have led to significant understanding of the regional characteristics associated with meteorite stranding surfaces. In Antarctica these sites are characterized by patches of snow‐free blue ice at high altitude on the icesheet in regions where iceflow is highly restricted. Melting is extremely rare or absent and sublimation rates are high, even though meteorite stranding surfaces are predominantly found within regions where accumulation typically dominates. Localized environmental conditions that persist for thousands of years or longer appear to be the dominant factor rather than shorter‐term or seasonal cycles. In this paper we describe our discovery of regions in Northeast Greenland with blue ice areas that exhibit many of the requisite characteristics, suggesting that they are excellent prospects for future meteorite recovery efforts.  相似文献   

‘Copernicus’ observations of extragalactic X-ray sources     

A. C. Fabian  R. J. Mitchell  P. J. N. Davison  P. A. Charles  J. L. Culhane 《Astrophysics and Space Science》1976,42(1):249-254

The MSSL X-ray detectors onCopernicus have been used to study a number of extragalactic objects. At least three classes of unresolved sources are found and we suggest that accretion may be the dominant mechanism. The mass of the accreting object then determines the X-ray emission properties.Paper presented at the COSPAR Symposium on Fast Transients in X- and Gamma-Rays, held at Varna, Bulgaria, 29–31 May, 1975.  相似文献   

The opacity of some local Martian dust storms observed by the Viking IRTM     

Garry E. Hunt  Elizabeth A. Mitchell  Alan R. Peterfreund 《Icarus》1980,41(3):389-399

In this paper we analyze some Viking infrared thermal mapping (IRTM) measurements of local Martian dust storms observed in the southern tropical region of the planet between L_s=225 and 262°. The derived opacities of these storms show that in the most opaque regions of the cloud, the optical thickness may be ≈6. Away from the individual clouds, the opacity is ≈2, which is still about four times the background level of dustiness in the Martian atmosphere. We find considerable structure in the derived opacity which will create corresponding variations in the atmospheric heating, which in turn may have an important feedback upon the local winds.  相似文献