The spectral reflectivity of select areas on Europa

The July 12, 1973, occultation of Europa by Io was observed in 30 wavelength channels in the spectral region λλ3200-11, 000 Å with the 200-inch Hale telescope and a multichannel spectrometer. The data are presented in absolute units above the Earth's atmosphere. The data are analyzed to obtain the spectral reflectivity of seven localized areas on the disk of Europa centered on 324°W longitude. The equatorial material is confirmed to be darker than the eastward-skewed bright north polar cap and a hint is evident that the darker material as well may be somewhat redder than the cap material.     

Solar-interplanetary modeling: 3-D solar wind solutions in prescribed non-radial magnetic field geometries

A model is presented which describes the 3-dimensional non-radial solar wind expansion between the Sun and the Earth in a specified magnetic field configuration subject to synoptically observed plasma properties at the coronal base. In this paper, the field is taken to be potential in the inner corona based upon the Mt. Wilson magnetograph observations and radial beyond a certain chosen surface. For plasma boundary conditions at the Sun, we use deconvoluted density profiles obtained from synopticK-coronameter brightness observations. The temperature is taken to be 2 × 10⁶ K at the base of closed field lines and 1.6 x 10⁶K at the base of open field lines. For a sample calculation, we employ data taken during the period of the 12 November 1966 eclipse. Although qualitative agreement with observations at 1 AU is obtained, important discrepancies emerge which are not apparent from spherically symmetric models or those models which do not incorporate actual observations in the lower corona. These discrepancies appear to be due to two primary difficulties - the rapid geometric divergence of the open field lines in the inner corona as well as the breakdown in the validity of the Spitzer heat conduction formula even closer to the Sun than predicted by radial flow models. These two effects combine to produce conductively dominated solutions and lower velocities, densities, and field strengths at the Earth than those observed. The traditional difficulty in solar wind theory in that unrealistically small densities must be assumed at the coronal base in order to obtain observed densities at 1 AU is more than compensated for here by the rapid divergence of field lines in the inner corona. For these base conditions, the value ofβ(ratio of gas pressure to magnetic pressure) is shown to be significantly greater than one over most of the lower corona - suggesting that, for the coronal boundary conditions used here, the use of a potential or force-free magnetic field configuration may not be justified. The calculations of this paper point to the directions where future research on solar-interplanetary modelling should receive priority:

1. better models for the coronal magnetic field structure
2. improved understanding of the thermal conductivity relevant for the solar wind plasma.

     

Geopotential harmonics of order 15 and odd degree from analysis of resonant orbits

We have analysed the variations of inclination in 13 satellite orbits as they pass slowly, under the action of air drag, through 15th-order resonance with the geopotential, when successive equatorial crossings are 24° apart and the ground track repeats after 15 rev. The size and form of the change in inclination are determined mainly by the values of the geopotential harmonics of 15th order and odd degree, $\text{C}\text{?}{}_{\mathrm{l,15}}$ and $\text{S}\text{?}{}_{\mathrm{l,15}}$ (with l = 15, 17, 19, …) in the usual notation. Our analysis gives values of these coefficients up to l = 33 as follows:

     

175.

Manganoan garnet rocks associated with the Broken Hill Pb–Zn–Ag orebody, Australia     

I. R. Plimer 《Mineralogy and Petrology》2006,88(3-4):443-478

Summary The Palaeoproterozoic Broken Hill Pb–Zn–Ag stratiform orebody is intimately associated with manganoan garnet-bearing rocks. On stratigraphic and chemical grounds it is argued that garnet-rich metasediments below, equivalent to and above massive sulphide were hydrothermal precipitates. Other manganoan garnet rocks formed during pre-metamorphic hydrothermal alteration, syn-metamorphic dehydration and reaction of manganese with prograde pelitic rocks, reaction between cataclastic manganese-bearing sulphide rocks injected along axial planes, shears and faults and pelitic wall rocks and reaction between dolerite dykes and sulphide rocks.     

176.

Tide model errors and GRACE gravimetry: towards a more realistic assessment   总被引：10，自引：1，他引：10  

R. D. Ray  S. B. Luthcke 《Geophysical Journal International》2006,167(3):1055-1059

     

177.

Surface waves image the top of the Eifel plume   总被引：1，自引：0，他引：1  

Jan P. Mathar  Joachim R. R. Ritter  Wolfgang Friederich 《Geophysical Journal International》2006,164(2):377-382

     

178.

Time scales of magma storage and differentiation of voluminous high-silica rhyolites at Yellowstone caldera, Wyoming   总被引：5，自引：4，他引：5  

Jorge A. Vazquez  Mary R. Reid 《Contributions to Mineralogy and Petrology》2002,144(3):274-285

     

179.

The Skaergaard Layered Series. Part VI. Excluded Trace Elements   总被引：1，自引：2，他引：1  

McBIRNEY  ALEXANDER R. 《Journal of Petrology》2002,43(3):535-556

In contrast to the smooth trends of major elements and mineralcompositions, the excluded trace elements in the SkaergaardLayered Series have an irregular distribution that does notconform to the normal trends of Rayleigh-type fractionation.Their concentrations are about constant or even decline throughthe Lower and Middle Zones before increasing sharply to reachmaximum concentrations 100–200 m above the Sandwich Horizon.As in the case of included elements, the relative concentrationsof excluded elements in coexisting phases deviate widely fromthose predicted by experimentally determined partition coefficientsunder presumed magmatic conditions. This is seen most clearlyin the immiscible melanogranophyres and conjugate ferrogabbros.Although the major elements conform to the experimentally determinedrelations for immiscible liquids, the trace elements do not;they follow a totally independent trend. The abrupt increasein the concentrations of excluded elements in the upper partof the intrusion could plausibly be attributed to an additionof new magma or to a density inversion that resulted in upwardmigration of a late liquid or fluid, but these possibilitiesare inconsistent with the compositional and spatial relationsof the upper parts of the intrusion. Although a late residualliquid certainly migrated upward, the most likely explanationfor the observed distribution of excluded elements is that thepartition coefficients were altered by volatile components,which gradually increased during the early stages of crystallizationthen began to exsolve near the top of the Middle Zone. KEY WORDS: igneous differentiation; Skaergaard intrusion     

180.

Middle Pleistocene molluscan and ostracod faunas from Allhallows, Kent, UK     

M.R. BatesD.H. Keen  J.E. WhittakerJ.S. Merry  F.F. Wenban-Smith 《Proceedings of the Geologists' Association. Geologists' Association》2002,113(3):223-236

     

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l	109C?l,15	109S?l,15
15	?23.5 ± 0.8	?7.7 ± 0.8
17	6.3 ± 1.5	5.6 ± 1.5
19	?25.1 ± 2.5	?7.3 ± 2.3
21	27.8 ± 3.6	?0.7 ± 3.4
23	17.1 ± 4.1	13.9 ± 4.8
25	?1.1 ± 3.0	8.5 ± 4.2
27	10.0 ± 3.3	6.7 ± 2.7
29	?9.4 ± 3.5	0.1 ± 4.7
31	10.1 ± 5.4	3.8 ± 5.6
33	1.1 ± 5.7	3.1 ± 5.8

Manganoan garnet rocks associated with the Broken Hill Pb–Zn–Ag orebody, Australia

Summary The Palaeoproterozoic Broken Hill Pb–Zn–Ag stratiform orebody is intimately associated with manganoan garnet-bearing rocks. On stratigraphic and chemical grounds it is argued that garnet-rich metasediments below, equivalent to and above massive sulphide were hydrothermal precipitates. Other manganoan garnet rocks formed during pre-metamorphic hydrothermal alteration, syn-metamorphic dehydration and reaction of manganese with prograde pelitic rocks, reaction between cataclastic manganese-bearing sulphide rocks injected along axial planes, shears and faults and pelitic wall rocks and reaction between dolerite dykes and sulphide rocks.     

The Skaergaard Layered Series. Part VI. Excluded Trace Elements

In contrast to the smooth trends of major elements and mineralcompositions, the excluded trace elements in the SkaergaardLayered Series have an irregular distribution that does notconform to the normal trends of Rayleigh-type fractionation.Their concentrations are about constant or even decline throughthe Lower and Middle Zones before increasing sharply to reachmaximum concentrations 100–200 m above the Sandwich Horizon.As in the case of included elements, the relative concentrationsof excluded elements in coexisting phases deviate widely fromthose predicted by experimentally determined partition coefficientsunder presumed magmatic conditions. This is seen most clearlyin the immiscible melanogranophyres and conjugate ferrogabbros.Although the major elements conform to the experimentally determinedrelations for immiscible liquids, the trace elements do not;they follow a totally independent trend. The abrupt increasein the concentrations of excluded elements in the upper partof the intrusion could plausibly be attributed to an additionof new magma or to a density inversion that resulted in upwardmigration of a late liquid or fluid, but these possibilitiesare inconsistent with the compositional and spatial relationsof the upper parts of the intrusion. Although a late residualliquid certainly migrated upward, the most likely explanationfor the observed distribution of excluded elements is that thepartition coefficients were altered by volatile components,which gradually increased during the early stages of crystallizationthen began to exsolve near the top of the Middle Zone. KEY WORDS: igneous differentiation; Skaergaard intrusion