Isostatic compensation on a continental scale: local versus regional mechanisms

Summary. Using the techniques of linear and quadratic programming, it can be shown that the isostatic response function for the continental United States, computed by Lewis & Dorman (1970), is incompatible with any local compensation model that involves only negative density contrasts beneath topographic loads. We interpret the need for positive densities as indicating that compensation is regional rather than local. The regional compensation model that we investigate treats the outer shell of the Earth as a thin elastic plate, floating on the surface of a liquid. The response of such a model can be inverted to yield the absolute density gradient in the plate, provided the flexural rigidity of the plate and the density contrast between mantle and topography are specified.
If only positive density gradients are allowed, such a regional model fits the United States response data provided the flexural rigidity of the plate lies between 10²¹ and 10²² N m. The fit of the model is insensitive to the mantle/ load density contrast, but certain bounds on the density structure can be established if the model is assumed correct. In particular, the maximum density increase within the plate at depths greater than 34 kin must not exceed 470 kg m⁻³; this can be regarded as an upper bound on the density contrast at the Mohorovicic discontinuity.
The permitted values of the flexural rigidity correspond to plate thicknesses in the range 5–10 km, yet deformations at depths greater than 20 km are indicated by other geophysical data. We conclude that the plate cannot be perfectly elastic; its effective elastic moduli must be much smaller than the seismically determined values. Estimates of the stress-differences produced in the earth by topographic loads, that use the elastic plate model, together with seismically determined elastic parameters, will be too large by a factor of four or more.     

1989 Exclusive economic zone symposium: Summary and recommendations

Abstract

The fourth in a series of biennial national Exclusive Economic Zone symposia was held on November 14–16, 1989. The purpose of the meeting was to examine ongoing and planned mapping and research activities in the ocean waters of the United States. Approximately 220 individuals attended the meeting. Issues discussed related to digital seafloor mapping projects, cooperative federal‐state programs, and requirements for additional data and information. Symposium recommendations included the need for increased surveying in coastal waters, development of standards for digital data dissemination, increased coordination with coastal states and federal agencies, and additional geophysical measurement systems abroad all mapping ships.     

Northwest Atlantic REX inverted echo sounder location: Acoustic range data

The Northwest Atlantic Regional Energetics Experiment (REX) will study the dynamics and energetics of the Gulf Stream and associated rings. Bottom‐moored inverted echo sounders with pressure gauges (IES/PGs) will collect in situ data which both complement and augment the GEOSAT altimeter measurements in the Northwest Atlantic. The primary objective of these data will be the intercomparison of satellite and IES/PG measured fluctuations in sea surface topography and mean ther‐mocline depth. However, more detailed and absolute intercom‐parisons of these data would be available if the IES/PG could be positioned in an inertial reference frame while the measurements were taken. This paper presents an error model for computing the accuracy of positioning with a bottom beacon of the IES/PG type. Equations for studying the use of acoustic range data for locating an IES/PG with respect to a ship's track are developed and presented. The ship's track is assumed to be located in inertial space to the 1‐ to 2‐m level by application of the GPS (Mohan, 1983, 1984). Effects of depth‐dependent acoustic speed are included. Although IES/PGs as presently deployed would have to be modified to function as the type of ranging device described in this paper, the representative parameter values that have been calculated for the Northwest Atlantic REX show that sub‐1‐meter accuracy in location determination can be expected. A crucial factor is the measurement pattern, and recommendations for optimal patterns are presented.     

A study of the contrast of sunspots from photometric images

The thermal contrast , and the umbra-penumbraA _u/A _p, were calculated for 63 sunspots of various sizes and morphologies. Contrary to the assumptions of the PSI model, andA _u/A _p were found to be quite variable. The values of ranged from 0.1807 to 0.4266;A _u/A _p ranged from 0.0089 to 0.4899. The values of andA _u/A _p correlated well (r = 0.6018;p<0.005) and the regression for andA _u/A _p was obtained: = (0.220 ± 0.016) + (0.340 ± O.06)A _u/A _p. The values of andA _u/A _p were then compared with complexity ratings, magnetic field strength, time, and . The quantities andA _u/A _p were found to be independent of the complexity, magnetic field strength, and time factors. The correlation between andA _u/A _p lead to the proposed division of into an umbral thermal contrast _u, and a penumbral thermal contrast _p. These values were calculated from the photometric data: _u = 0.57 ± 0.01 and _p = 0.26 ± 0.006.     

Platyceratid gastropod infestations of Neoplatycrinus Wanner (Crinoidea) from the Permian of West Timor: speculations on thecal modifications

Distinctive trace fossils, indicating the infestation of the monobathrid camerate crinoid Neoplatycrinus Wanner by coprophagous platyceratid gastropods, are recognised for the first time from the Permian of West Timor. Platyceratid shells from West Timor have previously been reported preserved on or about the crinoid tegmen, that is, apically; in contrast, the trace fossils described herein occur in the CD interray (=posteriorly), mainly on the radials. There are two patterns of infestation in the CD interray. Circular grooves in this position, situated below the periproct, are referred to Lacrimichnus isp. Thecal modifications include the CD interray sloping towards the base, and incomplete curved ridges developed outside the circular groove and confined to the radials. A different morphology is shown by other specimens that have a broad, flattened CD interray, curving down to and extending onto the basals; this interray also slopes towards the base. These unusual CD interray modifications are interpreted as a product of snail/crinoid associations. We speculate that the major modifications to the theca may have permitted the platyceratid shell to mimic an uninfested CD interray and thus maintain the hydrodynamic integrity of the crown. This would have been to the advantage of both gastropod and crinoid. The camerates did not survive the P/Tr extinction; their demise ended an association that had persisted over 200 million years, although the platyceratids persisted into the Mesozoic.     

Numerical simulations of photoionized plasmas: applications to astrophysical and laboratory environments

A wide variety of astrophysical objects, ranging from newly formed stars to accreting black holes, produce ionizing radiation. Nearby material will reprocess these photons into other forms of light. Depending on the geometry, we will observe such gas through either an emission or absorption line spectrum. Such clouds are detected across the electromagnetic spectrum and detailed analysis can reveal such vital parameters as the composition of the gas and the form of the ionizing radiation field. The gas is in a non-equilibrium state due to its low density and the presence of a wide range of non-thermal energy sources. The spectrum is typically analyzed with the help of large-scale numerical simulations. This paper describes recent developments of Cloudy, a code that performs such simulations, and outlines applications to star forming regions, active galactic nuclei, and laboratory plasmas.     

The science process for selecting the landing site for the 2011 Mars Science Laboratory

The process of identifying the landing site for NASA’s 2011 Mars Science Laboratory (MSL) began in 2005 by defining science objectives, related to evaluating the potential habitability of a location on Mars, and engineering parameters, such as elevation, latitude, winds, and rock abundance, to determine acceptable surface and atmospheric characteristics. Nearly 60 candidate sites were considered at a series of open workshops in the years leading up to the launch. During that period, iteration between evolving engineering constraints and the relative science potential of candidate sites led to consensus on four final sites. The final site will be selected in the Spring of 2011 by NASA’s Associate Administrator for the Science Mission Directorate. This paper serves as a record of landing site selection activities related primarily to science, an inventory of the number and variety of sites proposed, and a summary of the science potential of the highest ranking sites.