Common bivalve larvae from New Zealand: Leptonacea

The late stage larvae of three erycinid bivalves (Mollusca: Pelecypoda: Leptonacea) taken from the brood chamber of the adult are described (Kellia cycladiformis, Lasaea rubra hinemoa, and L. maoria), and the provisionally identified late stage larva of the erycinid Arthritica bijurca taken from the plankton is described. Also, the D‐shaped larvae of the erycinid bivalves Kellia cycladiformis, Borniola reniformis, Arlhritica crassijormis, and A. bifurca taken from the parent brood chamber are described. The seasonal occurrence of each late stage larva in the plankton at the Bay of Islands (35° 15'S, 174° 10'E), Wellington Harbour (41° 16'S, 174° 51'E), and Raumati Beach (40° 56'S, 174° 58'E), New Zealand is described. Aspects of the reproductive cycles of Lasaea rubra hinemoa and Arthritica bifurca are presented.     

Pressure-temperature and evolution of fluid compositions of Al2SiO5-bearing rocks,Mica Creek,B.C., in light of fluid inclusion data and mineral equilibria

Metamorphosed pelitic rocks from Mica Creek, British Columbia contain sillimanite, kyanite with minor fibrolite and andalusite-bearing quartz pods. Mineral equilibria were used to infer peak P-T conditions and fluid compositions in equilibrium with the solid phases. Fluid inclusions in three schist samples appear to be good indicators of conditions affecting those rocks during and after peak metamorphic conditions. In samples from two localities, fluid inclusions from schist and quartz-rich segregations have densities appropriate to the peak metamorphic conditions. The observed compositions for these fluids (low salinity with 12 mole % dissolved CO₂) agree with calculated values of 0.84 to 0.85, based upon paragonite-quartz-albite-Al₂SiO₅ equilibria. The fluids unmixed as the schists were uplifted and cooled; fluid inclusions trapped during this stage outline a solvus in the CO₂-H₂O-NaCl system. A later influx of fluids containing CH₄ and N₂ accompanied formation of andalusite-bearing plagioclaserich segregations. The restricted association of andalusite-bearing pods and low density fluids suggest a localized but pervasive fluid influx during uplift. Preservation of high density fluid inclusions during uplift and erosion, coupled with evidence for unmixing of H₂O- and CO₂-rich fluids on the solvus, provide constraints on the P-T uplift path.     

Lithostratigraphic correlation of Blaini Formation (late Proterozoic,Lesser Himalaya,India) with other late Proterozoic tillite sequences

The Blaini Formation of the Lesser Himalaya has long been considered Permo-Carboniferous in age on simple lithological correlation with Gondwana Tillites in southern India. Rare, and non-repeatable finds of fossils from the type area were thought to confirm this. Recently, Lower Cambrian faunas have been recorded from the overlying Tal and Krol Formations, and possible metazoan trails recorded from the Blaini itself. In addition, the Blaini Formation is, even on a lithostratigraphic comparison, much more like other late Proterozoic glacial sequences. The term Blaini Formation should only be used for rocks of the type area — not for widely scattered glacial deposits which may or may not be correlatable with the type section. The persistent belief in the Paleozoic age of the Blaini (and adjacent formations) has for long retarded unterstanding of Lesser Himalaya stratigraphy and tectonics.

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Zusammenfassung Die Blaini Formation des Niederen Himalaya wurde bisher aufgrund lithologischer Vergleiche mit Gondwana Tilliten aus Süd-Indien in das Permo-Karbon eingestuft. Seltene, nicht wiederholbare Fossilfunde schienen dieses zu bestätigen. Kürzlich wurden Faunen des Unterkambriums in den überlagernden Tal- und Krol-Formationen gefunden sowie vermutliche Metazoanspuren aus der Blaini Formation selbst. Darüberhinaus ist die Blaini Formation sogar über den lithostratigraphischen Vergleich eher mit spätproterozoischen Glazialfolgen zu vergleichen. Der Begriff Blaini Formation sollte nur für die Typlokalität verwendet werden, und nicht für ähnliche Glazialvorkommen in der weiteren Umgebung. Die fortdauernde Annahme des paläozoischen Alters der Blaini- und umgebenden Formationen hat über lange Zeit hinweg das Verständnis für die Stratigraphie und die tektonische Entwicklung des Niederen Himalayas behindert.

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Résumé La formation de Blaini, dans l'Himalaya inférieur, a été jusqu'ici placée dans le Permo-Carbonifère sur la base de ses analogies lithologiques avec les tillites gondwaniennes du Sud de l'Inde. Cette attribution a semblé pouvoir Être confirmée par la découverte de quelques fossiles rares et isolés. Récemment des faunes du Cambrien inférieur ont été identifiées dans les formations surincombantes de Tal et de Krol; dans la formation de Blaini elle-mÊme des traces possibles de métazoaires ont été relevées. De plus, au seul point de vue lithologique, c'est avec les séries glaciaires du ProtérozoÏque supérieur que la formation de Blaini présente le plus de similitude. L'emploi du terme »Formation de Blaini« doit Être restreint à sa localité-type et doit Être évité pour des formations glaciaires d'autres régions, qui peuvent Être d'âges divers. L'âge paléozoÏque, attribué régulièrement jusqu'ici à la formation de Blaini et aux formations adjacentes a constitué un obstacle permanent à une bonne compréhension stratigraphique et tectonique de l'Himalaya inférieur.

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Use of landsat in mapping land-utilization of north maidan,Karnatka

North Maidan consist of seven districts of North Karnataka. It is named after its relatively low and subdued relief or landscape of monoto-nous plateau. Most of the area lies in the rain shadow of the Western Ghats. The land utilization map shows majority of the area during December and January months is under agriculture with fallow land as the second largest category Large areas of North Maidan are under grassland which look barren by the beginning of summer. A total of nine landuse categories were delineated wifh the help of Landsat data.     

Monitoring the Microarcsecond Quasar J1819+3845

We present the results of a year-long monitoring campaign on J1819+3845.We interpret the results of this WSRT campaign to infer critical source parameters such as source lifetime and structure on tens of microarcseconds. The long lifetime of the source at such high brightness temperatures requires continuous energy injection or exotic emission processes. We have previously interpreted the extreme scintillation ofJ1819+3845 as due to a relatively nearby (∼ 20 pc) scattering screen. We show this screen has a velocity w.r.t. the LSR of ∼ 25 kms^-1, as measured by the changing scintillation properties throughout the year: the `velocity parallax'. This revised version was published online in July 2006 with corrections to the Cover Date.