Basalts from the Solomon and Bismarck Seas

Volcanic rocks collected from the Solomon Sea Basin are mostly ferrobasalt lavas similar to evolved MORB; an exception is a single sample of basaltic crystal tuff invaded by later basalt. The rocks contain labradorite, aluminous diopsidic augite, and titanomagnetite, with olivine and pigconite in the more vitrophyric samples, and segregation vesicles in some. Cobbles dredged from Gudaraba Canyon, south of the Solomon Sea Basin, include both MORB-like glassy lava and K-metasomatised basalt and andesite(?). Two small pieces of volcanic glass from the southern Bismarck Sea are more primitive MOR-type basalts.     

Theoretical studies of storm effects in ionospheric total electron content

Investigations have been made of the effects produced by thermospheric winds, composition changes and magnetospheric electric fields on the ionospheric F-layer during disturbed conditions. The results of the computations suggest that a combination of realistic temperature and electric field changes would explain fairly satisfactorily the observed changes in total electron content.     

Direct imaging of planetary systems around nearby stars

We show that by utilizing a space-borne telescope it may be possible to directly image planetary systems around the nearest stars. Direct imaging, while limited to the nearest stars, would provide a great deal of information on the planet, over and above the planet's orbital elements—estimates of the planet's size and rotation rate, and the presence or absence of an atmosphere are all possible if light from the planet can be separated from light from the star. It is shown that a Jupiter-like planet would be detectable around several of the nearest stars.     

On the interpretation of frequency response functions for oceanic gravity and bathymetry

Summary. In 1972–78, the late N. D. Watkins and others carried out ajoint field programme of geological mapping in the Mio-Pliocene flood basalts of Iceland, including sampling for K-Ar dating and palaeomagnetic research. The major part of the palaeomagnetic sampling is represented by 2462 lavas in five long composite sections through the lava pile. This paper deals with various statistical properties of this data set.
It is concluded that geomagnetic reversals occur more frequently than is assumed in the current ocean-floor polarity time-scale. There is no evidence for significant asymmetries between normal and reverse polarity states of the field, neither as regards chron lengths, secular variation, or virtual dipole moment magnitude. Intensities of remanence in these lavas are shown to be well approximated in terms of a hyperbolic distribution. The latitude distribution of virtual magnetic poles can be fitted with a Bingham function having k' ∼ 4.5, and low-latitude poles do not occur preferentially in any particular longitude interval.