High-resolution foraminiferal census of benthic taxa was undertaken on 113 closely spaced samples drawn from the Late Pliocene (ca. 2.6−1.7 Ma) cyclothemic marine strata of the Rangitikei Group, eastern Wanganui Basin, New Zealand. These strata comprise a ca. 1 km thick progradational stack of twenty, sixth-order, depositional sequences that accumulated in shelf and shoreline palaeoenvironments. The sequences are correlated with δ18O Stages 100−58, and each 41 ka glaciallinterglacial stage couplet is represented by an individual sequence comprising transgressive (TST), highstand (HST), and regressive (RST) systems tracts.
Statistical analysis of the census data identifies thirteen foraminiferal associations within the cyclothemic strata, that are grouped into seven depth- and lithology-related biofacies spanning the entire range of marginal marine to outer shelf palaeoenvironments. Foraminiferal palaeobathymetric analysis of the Rangitikei Group sequences reveals cyclical changes in water-depth of ca. 100–200 m amplitude with frequencies corresponding to the 41 ka obliquity orbital rhythm. Water-depth changes of this magnitude are consistent with a glacio-eustatic origin for the cyclothems, which correspond to an interval of Earth's history when successive continental glaciations of the Northern Hemisphere are known to have occurred. Furthermore the derived water-depth changes are also consistent with lithofacies and sequence stratigraphic inferences regarding palaeodepth of the sequences.
Individual sequences display a clear deepening-upward trend from shoreline to mid-shelf water-depths within TSTs. The level of resolution provided by the microfaunal analysis was insufficient to resolve the precise position of the maximum flooding surface (MFS) and its relationship to the downlap surface (DLS). However, the turn around from rising to falling relative sea level (maximum water-depth) corresponds to a < 5 m interval of section spanning the top of TSTs and lower portions of HST's. A progressive shoaling trend to shoreline and marginal marine environments is indicated for the overlying RSTs.
The amplitudes of water-depth changes for asymmetrical sequences, Rangitikeint motif (nondepositional transgression) (100–200 m), are somewhat greater than glacio-eustatic sea-level changes derived from the deep-sea δ18O record (50–100 m). This implies a significant subsidence contribution to relative sea-level changes. Notwithstanding the effect of subsidence and sedimentation on relative sea level, fluctuations in glacio-eustatic sea level are regarded as the primary factor controlling relative sea-level changes recorded in the Late Pliocene Wanganui Basin succession. Foraminifer-derived palaeobathymetric cycles within sequences display the same frequency, relative magnitude and symmetry as their correlative cycles on the δ18O sea-level curve. 相似文献
Recent investigations of magnetospheric plasma structure are summarized under the broad categories of empirical models, transport across boundaries, formation, and dynamics of the plasma sheet. This report reviews work in these areas during the period 1991 to 1993. Fully three-dimensional empirical models and simulations have become important contributors to our understanding of the magnetospheric system. Some new structural concepts have appeared in the literature: the entry boundary and geopause, the plasma sheet region 1 vortices, the low-energy layer, the adiabaticity boundary or wall region, and a region in the tail to which we refer as the injection port. Traditional structural concepts have also been the subject of recent study, notably the plasmapause, the magnetopause, and the plasma sheet. Significant progress has been made in understanding the nature of plasma sheet formation and dynamics, but the acceleration of electrons to high energy remains somewhat mysterious. 相似文献
The discovery of the microlensing effect has found out the new population — dark bodies having mass of the order of 0.1M which form the halo of our Galaxy. There are two main criteria which identify a light curve as the reveal of the microlensing effect. They are symmetry of the light curve and equal amplification in different colors. We consider polarization of the light beam arising in microlensing effect and find that additional test is possible — polarization of light in the case of a finite star disk. Consequences of polarization are also considered. 相似文献
Comet Hale-Bopp is, without doubt, one of the most important objects for cometary science which has ever been observed. The light curve is well-observed from a heliocentric distance 7.2 AU and some information is available at distances as great as 17 AU. This allows the photometric evolution of the comet to be studied as different volatiles dominate the activity. Three different phases of activity are seen as the heliocentric distance reduces during 1996: the initial phase of very fast brightening, characterized by a r–5 law; a standstill in the light curve when the brightening law reduced to r–1, which coincides with the initiation of water sublimation at r ~ 4 AU; and a further phase of more rapid brightening with an r–3.5 law, similar to the mean for comets classed as fairly new, which initiated at r ~ 4 AU. 相似文献