Magma mixing: the Marsco suite,Isle of Skye,Scotland     

Thomas A. Vogel  Leland W. Younker  John T. Wilband  Elaine Kampmueller 《Contributions to Mineralogy and Petrology》1984,87(3):231-241

Magma mixing has been proposed as a major mechanism for the origin of a wide variety of rock suites. In mid-ocean basalts there are few obstacles to mixing because of the similarities in chemical and physical properties of the proposed end-members. However, in calc-alkaline rocks the proposed end-members have disparate properties and these present obstacles to mixing.The Marsco suite is ideal to evaluate the process of magma mixing because it is considered to be a classic example of magma mixing of diverse magma types and because compositionally diverse, coexisting liquids were present throughout the area.The results of this study are that the chemical data for the Marsco suite fit a mixing model remarkably well and that the mixing did not take place at the present level of exposure. The Marsco mixed suite is similar to the experiments of Kouchi and Sunagawa (1982, 1983) in which mixing was produced by forced convection. Based on the Marsco suite, a similar occurrence in Ardnamurchan, and the experimental data, we conclude that mixing was dominated by mechanical mixing and this mechanical mixing was efficient enough to allow diffusional processes to homogenize the liquids.It is postulated that injection of mafic magma into the base of a silicic magma system leads to mixing and mobilization of the system. The mechanical interaction that produces the mixing also leads to disruption of the system. Liquids involved with the mixing process at depth are mobilized and coexist at shallower levels.  相似文献   

Proper motion L and T dwarf candidate members of the Pleiades     

S. L. Casewell  P. D. Dobbie  S. T. Hodgkin  E. Moraux  R. F. Jameson  N. C. Hambly  J. Irwin  N. Lodieu 《Monthly notices of the Royal Astronomical Society》2007,378(3):1131-1140

We present the results of a deep optical–near-infrared (optical–NIR) multi-epoch survey covering 2.5 deg² of the Pleiades open star cluster to search for new very low-mass brown dwarf members. A significant (∼5 yr) epoch difference exists between the optical (CFH12k I -, Z -band) and NIR (UKIRT WFCAM J -band) observations. We construct I , I − Z and Z , Z − J colour–magnitude diagrams to select candidate cluster members. Proper motions are computed for all candidate members and compared to the background field objects to further refine the sample. We recover all known cluster members within the area of our survey. In addition, we have discovered nine new candidate brown dwarf cluster members. The seven faintest candidates have red Z − J colours and show blue NIR colours. These are consistent with being L- and T-type Pleiads. Theoretical models predict their masses to be around 11 M _Jup.  相似文献   

New stellar members of the Coma Berenices open star cluster     

S. L. Casewell  R. F. Jameson  P. D. Dobbie 《Monthly notices of the Royal Astronomical Society》2006,365(2):447-453

We present the results of a survey of the Coma Berenices open star cluster (Melotte 111), undertaken using proper motions from the USNO-B1.0 (United States Naval Observatory) and photometry from the Two-Micron All-Sky Survey (2MASS) Point Source catalogues. We have identified 60 new candidate members with masses in the range  1.007 < M < 0.269 M_⊙  . For each we have estimated a membership probability by extracting control clusters from the proper motion vector diagram. All 60 are found to have greater than 60 per cent probability of being members, more than doubling the number of known cluster members. The new luminosity function for the cluster peaks at bright magnitudes, but is rising at   K ≈ 12  , indicating that it is likely that lower mass members may exist. The mass function also supports this hypothesis.  相似文献   

On the computation of the spherical harmonic terms needed during the numerical integration of the orbital motion of an artificial satellite     

Leland E. Cunningham 《Celestial Mechanics and Dynamical Astronomy》1970,2(2):207-216

A method is presented for the accurate and efficient computation of the forces and their first derivatives arising from any number of zonal and tesseral terms in the Earth's gravitational potential. The basic formulae are recurrence relations between some solid spherical harmonics,V _n,m, associated with the standard polynomial ones.  相似文献   

On the parallax of WD 0346++246: a halo white dwarf candidate     

N. C. Hambly  S. J. Smartt  S. T. Hodgkin  R. F. Jameson  S. N. Kemp  W. R. J. Rolleston  I. A. Steele 《Monthly notices of the Royal Astronomical Society》1999,309(4):L33-L36

We present a parallax measurement for the very cool degenerate WD 0346+246, the serendipitous discovery of which was reported by Hambly et al. We find an absolute parallax of 36±5 mas, yielding a distance estimate of 28±4 pc. The resulting absolute visual magnitude of the object is M _V =16.8±0.3, making it the second-lowest luminosity white dwarf currently known. We use the distance estimate and measured proper motion to show that the object has kinematics consistent with membership of the Galactic halo. WD 0346+246 is therefore by far the coolest and least luminous of only a handful of plausible halo white dwarf candidates. As such, the object has relevance to the ongoing debate concerning the results of microlensing experiments and the nature of any baryonic dark matter component to the Galactic halo residing in stellar remnants.  相似文献   

AGE ESTIMATES OF INLAND DUNES IN EAST-CENTRAL LOWER MICHIGAN USING SOILS DATA     

Alan F. Arbogast  Thomas P. Jameson 《自然地理学》2013,34(6):485-501

Extensive deposits of eolian sand occur deep (>50 km) within the interior of east-central lower Michigan. These dunes are most common in the Saginaw lowland where they are parabolic, with limbs oriented northwesterly. Their presence on densely forested landscapes indicates that paleoenvironmental conditions differed sufficiently for dune formation to have occurred. In a previous study, Arbogast et al. (1997) illustrated that surface soils in the northwestern part of the Saginaw dune field were morphologically similar, consisting of weakly developed Spodosols (A/E/Bs/C horizonation). Thus, these dunes must have stabilized concurrently following regional mobilization of eolian sand. In this study, we present soils data from dunes in the southeastern part of the Saginaw dune field. Surface soils were analyzed at 19 sites in the Deford State Game Area in Tuscola County. Morphologically, the soils within the Deford area are similar (A/E/Bs/C horizonation), indicating that Deford dunes stabilized concurrently. Statistical (ANOVA, KW, factor analysis) comparison of Deford soils and soils to the northwest, however, reveals that significant developmental differences exist between the two areas, with Deford soils being better developed. Given that variables (climate, soil texture, pH) are more conducive for Spodosol development to the northwest, we conclude that Deford soils are older. Thus, Deford dunes must have stabilized prior to their counterparts to the northwest. [Key words: eolian processes, sand dunes, soils, Spodosols, Michigan.]  相似文献   

Bayesian upscaling of aircraft ice measurements to two-dimensional domains for large-scale applications     

A. R. Jameson  A. J. Heymsfield 《Meteorology and Atmospheric Physics》2014,123(1-2):93-103

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New stellar and substellar candidate members of the Coma Berenices open star cluster     

S. L. Casewell  R. F. Jameson  P. D. Dobbie 《Astronomische Nachrichten》2005,326(10):991-995

We present the results of a survey of the open star cluster Melotte 111 in Coma Berenices, undertaken using the USNO‐B1.0 and 2MASS Point Source catalogues. On the basis of their astrometric and photometric properties, we have identified 60 new candidate members with masses in the range 1.007 < M < 0.269 M_⊙. We estimate a membership probability for each by extracting control clusters from the proper motion vector diagram. All 60 are found to have greater than 60 per cent probability of being cluster members, which if they are confirmed as members, more than doubles the number of known cluster members. We also have I and Z photometry for 100 low mass candidate members of the cluster, 13 of which we suggest may be brown dwarfs. (© 2005 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Praesepe – two merging clusters?     

K. Holland  R. F. Jameson  S. Hodgkin  M. B. Davies  D. Pinfield 《Monthly notices of the Royal Astronomical Society》2000,319(3):956-962

A membership catalogue for Praesepe was compiled and split into four mass bins. A contour plot indicates the presence of a subcluster some 3 pc from the centre of the cluster, of approximately 30 M_⊙. A tidally truncated King profile was fitted to the remainder of the cluster and the tidal radius is found to be 12.1 pc; the mass of the cluster (excluding the subcluster) is 630 M_⊙. From the calculated velocity dispersions we find that the cluster appears to have too much kinetic energy and should be rapidly disintegrating. X-ray data suggest that there may be an age spread between the main core stars and the subcluster stars. This leads us to the conclusion that Praesepe is two merging clusters.  相似文献   

How U.S. ocean policy and market power can reform the coral reef wildlife trade     

Brian N. Tissot  Barbara A. Best  Eric H. Borneman  Andrew W. Bruckner  Cara H. Cooper  Heather D’Agnes  Timothy P. Fitzgerald  Amanda Leland  Susan Lieberman  Amy Mathews Amos  Rashid Sumaila  Teresa M. Telecky  Frazer McGilvray  Brian J. Plankis  Andrew L. Rhyne  Glynnis G. Roberts  Benjamin Starkhouse  Todd C. Stevenson 《Marine Policy》2010

As the world’s largest importer of marine ornamental species for the aquaria, curio, home décor, and jewelry industries, the United States has an opportunity to leverage its considerable market power to promote more sustainable trade and reduce the effects of ornamental trade stress on coral reefs worldwide. Evidence indicates that collection of some coral reef animals for these trades has caused virtual elimination of local populations, major changes in age structure, and promotion of collection practices that destroy reef habitats. Management and enforcement of collection activities in major source countries such as Indonesia and the Philippines remain weak. Strengthening US trade laws and enforcement capabilities combined with increasing consumer and industry demand for responsible conservation can create strong incentives for improving management in source countries. This is particularly important in light of the March 2010 failure of the parties to the Convention on International Trade in Endangered Species (CITES) to take action on key groups of corals.  相似文献