IN-SITU observations of irregular ionospheric structure associated with the plasmapause

Additional studies of the ion composition results obtained from the OGO-6 satellite support earlier observations of irregularities in the distribution of H⁺ and He⁺ within the light ion trough near L = 4, which has been associated with the plasmapause. These irregularities are in the form of sub-troughs superimposed upon the major mid latitude decrease of the light ions. In the sub-troughs, ionization depletions and recoveries of as much as an order of magnitude are observed within a few degrees of latitude, usually exhibited in a pattern which changes significantly with longitude as the Earth rotates beneath the relatively fixed satellite orbit. The location and properties exhibited by these sub-troughs appear to be consistent with the concept of a plasmasphere distortion in the form of “plasmatails” resulting from the combined effects of magnetospheric convection plus corotation. Like the light ion trough, the “plasmatail” irregularity in H⁺ may be obscured on the day side by the dominant topside distribution of O⁺. Consequently, these light ion irregularities are seen as an important factor for studies of plasmapause-trough relationships.     

The origin of rotational remanent magnetization

Summary. Rotational remanent magnetization, RRM, is the magnetization acquired when a sample is rotated during alternating field demagnetization. Although the existence of RRM has been well documented in different laboratories, until now no physical mechanism explaining its origin has been given. We propose that the RRM originates from thermal fluctuations biased by a precessional torque associated with the alternating field. Our theory is consistent with the observation that no directional preference exists in the experimental situation until the sample is rotated relative to the alternating field. Moreover, our theory predicts that the combined sample rotation and precession will produce a RRM that switches direction when the frequency of sample rotation increases from any value below the frequency of the alternating field to any value above that frequency as observed in experiments. Although no precise theory is given for the intensity of RRM, the model presented here can qualitatively explain previous intensity observations.     

Reconnection X-winds: spin-down of low-mass protostars

We investigate the interaction of a protostellar magnetosphere with a large-scale magnetic field threading the surrounding accretion disc. It is assumed that a stellar dynamo generates a dipolar-type field with its magnetic moment aligned with the disc magnetic field. This leads to a magnetic neutral line at the disc mid-plane and gives rise to magnetic reconnection, converting closed protostellar magnetic flux into open field lines. These are simultaneously loaded with disc material, which is then ejected in a powerful wind. This process efficiently brakes down the protostar to 10–20 per cent of the break-up velocity during the embedded phase.     

Structure and subduction processes along the Oregon-Washington margin

Seismic reflection and refraction data off Washington and Oregon are used to determine the style of sediment deformation and to infer the physical properties of accreted sediments on the lower slope. Onshore-offshore seismic refraction data off Washington are used to determine the location of the trench, or where the plate bending starts.We find that off Washington the subduction zone is characterized by a trench whose physiographic expression is buried under several kilometers of sediments and is tens of kilometers landward of the lower slope, which is accreting seaward as the result of the offscraping of sediments.Seismic reflection data support previous observations that offscraping occurs along seaward and landward dipping thrust faults. Refraction data indicate that a sediment package thrust up along a seaward dipping fault (off Washington) was not measurably changed in velocity with respect to a Cascadia basin section. However a package uplifted by thrusting along a landward dipping fault (off Oregon) did have increased velocity. It is suggested that the increased velocities off Oregon could be the result of erosion and exposure of more deeply buried and compacted sediments, rather than the result of dewatering due to tectonic stress. Off Washington the sensitivity of velocity to porosity and resolution of the seismic method does not preclude dewatering due to tectonic stress, but it does limit the degree of dewatering.In the deeper parts of the lower slope section off Washington and Oregon velocities as high as 3 to 4 km/sec are found. Heat flow data indicate that the temperatures in this high velocity regime are greater than 100°C. It is hypothesized that lithification related to clay diagenesis may be partly responsible for the high velocities, rather than simply compaction. It also appears that the high velocity sediments are subducted while the unlithified low velocity sediments are offscraped.     

Groundwater flow and contaminant transport modelling at an air weapons range

Numerical modelling was done at the Cold Lake Air Weapons Range, Canada, to test whether the dissolved RDX and nitrate detected in groundwater come from the same sources, and to predict whether contamination poses a threat to the surface water receptors near the site. Military live fire training activities may indeed pose a risk of contamination to groundwater resources, however field investigations on military bases are quite recent, and little information is available on the long-term behaviour of munition residues related contaminants. Very limited information was available about the contaminant source zones, which were assigned based on our knowledge of current training activities. The RDX plume was well represented with the model, but the heterogeneous distribution of nitrate concentrations was more difficult to reproduce. It was nonetheless determined that both contaminants originate from the same areas. According to the model, both contaminants should reach the nearby river, but concentrations in the river should remain very low if the source zone concentration does not change. Finally, the model allowed the recommendation of a new location for the main bombing target, which would offer added protection to the river and the lake into which it flows.     

La marge continentale au large de l'estérel (France) et les mouvements verticaux pliocènes

Sommaire La région étudiée s'étend au large du massif des Maures, du massif de l'Estérel, des chaînes calcaires provençales et de la bordure alpine (Figure 1). Cette partie de la marge continentale médíterranéenne a été étudiée dans l'optique de la géodynamique en appliquant un ensemble de méthodes géophysiques, géologiques, sédimentologiques et géochimiques.La Méditerranée est l'objet de nombreuses études générales et son histoire tectonique est encore très discutée. Les relations entre la zone centrale (zone A) et les massifs terrestres géologiquement bien connus peuvent aider à la compréhension du cadre structural. L'étude très détaillée présentée ici concerne la marge continentale au large de la Côte d'Azur. Une étude bathymétrique préliminaire avec des profils espacés d'un mille marin a permis de définir un plateau continental peu étendu, une pente continentale abrupte (10–20°) avec des blocs continentaux effondrés. De nombreux canyons empruntent des accidents anciens qui ont rejoué.Des profils en série de sismique continue (Sparker et air gun) ont permis de délimiter la zone A qui comporte de nombreux dômes, de suivre des accidents majeurs, et de montrer des phénomènes sédimentaires et de néotectonique très importants (glissements, effondrements). Ces profils ont été calés avec 50 carottages. Un effondrement de plus de 1000 m depuis le Pliocène a été mis en évidence.La structure profonde a été abordée avec une étude de magnétométrie marine. La synthèse des résultats de sismique réfraction, de gravimétrie et de magnétométrie fait apparître un bombement du manteau sous la zone A avec abaissement rapide de la discontinuité de Moho sous la marge, la présence de volcans enfouis au Sud d'Antibes et de grands accidents de direction NS et EW.L'intérêt de ces résultats a semblé suffisamment important pour qu'un point de cette zone soit proposé pour le programme de forage JOIDES en Méditerranée.

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This paper deals with the region off the Maures and Estérel Massifs, the Provence calcareous ranges and the Alpine border (Figure 1). This portion of the Mediterranean continental margin has been investigated with the classical methods used in the geosciences: geophysics, geology, sedimentology, geochemistry.Many general studies are dealing with the Mediterranean and its tectonical history is still controversial. The relationship between the central zone (zone A) and the geologically well-known land massifs could help in understanding the structural framework. The present detailed study concerns the continental margin off Côte d'Azur. A relatively narrow continental shelf, a steep continental slope (10–20°) with collapsed continental blocks are defined by preliminary bathymetric studies with a spacing of one nautical mile. Many submarine canyons follow former faults which have been rejuvenated.A series of seismic reflection profiles (sparker and air-gun) provide limits for zone A (with many domes), allow tracing major faults and display important sedimentary and neotectonic processes (sliding, foundering). These profiles have been scaled with 50 cores. Evidence is brought forward for a local subsidence of over 1000 m. The deep structure has been investigated with marine magnetic methods. The results from seismic refraction, gravity and magnetics show a swell of the mantle beneath zone A, with a steep dipping of the M discontinuity under the margin, buried volcanoes south of Antibes and great faults striking NS or EW.These results seem to be important enough to propose a place in this zone of the Mediterranean as a JOIDES drilling site.

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Maintenant au Centre Océanologique de Bretagne, B.P. 337, 29 Brest, France.     

Oxygen isotopes composition of sapphires from the French Massif Central: implications for the origin of gem corundum in basaltic fields

Alluvial and colluvial gem sapphires are common in the basaltic fields of the French Massif Central (FMC) but sapphire-bearing xenoliths are very rare, found only in the Menet trachytic cone in Cantal. The O-isotope composition of the sapphires ranges between 4.4 and 13.9‰. Two distinct groups have been defined: the first with a restricted isotopic range between 4.4 and 6.8‰ (n = 22; mean δ¹⁸O = 5.6 ± 0.7‰), falls within the worldwide range defined for blue-green-yellow sapphires related to basaltic gem fields (3.0 < δ¹⁸O < 8.2‰, n = 150), and overlaps the ranges defined for magmatic sapphires in syenite (4.4 < δ¹⁸O < 8.3‰, n = 29). A second group, with an isotopic range between 7.6 and 13.9‰ (n = 9), suggests a metamorphic sapphire source such as biotite schist in gneisses or skarns. The δ¹⁸O values of 4.4–4.5‰ for the blue sapphire-bearing anorthoclasite xenolith from Menet is lower than the δ¹⁸O values obtained for anorthoclase (7.7–7.9‰), but suggest that these sapphires were derived from an igneous reservoir in the subcontinental spinel lherzolitic mantle of the FMC. The presence of inclusions of columbite-group minerals, pyrochlore, Nb-bearing rutile, and thorite in these sapphires provides an additional argument for a magmatic origin. In the FMC lithospheric mantle, felsic melts crystallized to form anorthoclasites, the most evolved peraluminous variant of the alkaline basaltic melt. The O-isotopic compositions of the first group suggests that these sapphires crystallized from felsic magmas under upper mantle conditions. The second group of isotopic values, typified for example by the Le Bras sapphire with a δ¹⁸O of 13.9‰, indicates that metamorphic sapphires from granulites were transported to the surface by basaltic magma.