Preliminary results from a new study of transverse aeolian ridges (TARS) on Mars

Abstract not available

Megabarchans on Mars

Abstract not available

Pacific Island food security: situation, challenges and opportunities

In recent years, there have been large and rapid increases in the prices of basic foods worldwide. Pacific island countries have not been isolated from the global food 'crisis'. This article shows that there are substantial differences in the impacts within and between Pacific island countries. To be effective and not counterproductive, policy and donor responses need to be tailored accordingly. This article recommends a combination of measures directed at mitigating the threats and empowering rural people to take advantage of the opportunities

The distribution of Transverse Aeolian Ridges on Mars

Abstract not available

Systems comparison of direct and relay link data return modes for advanced planetary missions

Advanced planetary missions using direct and relay link data return mode

VLA OH Zeeman Observations of the star forming region S88B

We present observations of the Zeeman effect in OH thermal absorption main lines at 1665 and 1667 MHz taken with the Very Large Array (VLA) toward the star forming region S88B. The OH absorption profiles toward this source are complicated, and contain several blended components toward a number of positions. Almost all of the OH absorbing gas is located in the eastern parts of S88B, toward the compact continuum source S88B-2 and the eastern parts of the extended continuum source S88B-1. The ratio of 1665/1667 MHz OH line intensities indicates the gas is likely highly clumped, in agreement with other molecular emission line observations in the literature. S88-B appears to present a similar geometry to the well-known star forming region M17, in that there is an edge-on eastward progression from ionized to molecular gas. The detected magnetic fields appear to mirror this eastward transition; we detected line-of-sight magnetic fields ranging from 90-400 \mu G, with the lowest values of the field to the southwest of the S88B-1 continuum peak, and the highest values to its northeast. We used the detected fields to assess the importance of the magnetic field in S88B by a number of methods; we calculated the ratio of thermal to magnetic pressures, we calculated the critical field necessary to completely support the cloud against self-gravity and compared it to the observed field, and we calculated the ratio of mass to magnetic flux in terms of the critical value of this parameter. All these methods indicated that the magnetic field in S88B is dynamically significant, and should provide an important source of support against gravity. Moreover, the magnetic energy density is in approximate equipartition with the turbulent energy density, again pointing to the importance of the magnetic field in this region.Comment: 26 pages, 7 figures, accepted for publication in Ap

A test of reproductive skew models in a field population of a multiple-queen ant

Determining the evolutionary basis of variation in reproductive skew (degree of sharing of reproduction among coexisting individuals) is an important task both because skew varies widely across social taxa and because testing models of skew evolution permits tests of kin selection theory. Using parentage analyses based on microsatellite markers, we measured skew among female eggs (n=32.3 eggs per colony, range=20-68) in 17 polygynous colonies from a UK field population of the ant Leptothorax acervorum. We used skew among eggs as our principal measure of skew because of the high degree of queen turnover in the study population. Queens within colonies did not make significantly unequal contributions to queen and worker adult or pupal offspring, indicating that skew among female eggs reflected skew among daughter queens. On average, both skew among female eggs (measured by the B index) and queen-queen relatedness proved to be low (means±SE=0.06±0.02 and 0.28±0.08, respectively). However, contrary to current skew models, there was no significant association of skew with either relatedness or worker number (used as a measure of productivity). In L. acervorum, predictions of the concession model of skew may hold between but not within populations because queens are unable to assess their relatedness to other queens within colonies. Additional phenomena that may help maintain low skew in the study population include indiscriminate infanticide in the form of egg cannibalism and split sex ratios that penalize reproductive monopoly by single queens within polygynous colonie

The Dynamical State of Barnard 68: A Thermally Supported, Pulsating Dark Cloud

We report sensitive, high resolution molecular-line observations of the dark cloud Barnard 68 obtained with the IRAM 30-m telescope. We analyze spectral-line observations of C18O, CS(2--1), C34S(2--1), and N2H+(1--0) in order to investigate the kinematics and dynamical state of the cloud. We find extremely narrow linewidths in the central regions of the cloud. These narrow lines are consistent with thermally broadened profiles for the measured gas temperature of 10.5 K. We determine the thermal pressure to be a factor 4 -- 5 times greater than the non-thermal (turbulent) pressure in the central regions of the cloud, indicating that thermal pressure is the primary source of support against gravity in this cloud. This confirms the inference of a thermally supported cloud drawn previously from deep infrared extinction measurements. The rotational kinetic energy is found to be only a few percent of the gravitational potential energy, indicating that the contribution of rotation to the overall stability of the cloud is insignificant. Finally, our observations show that CS line is optically thick and self-reversed across nearly the entire projected surface of the cloud. The shapes of the self-reversed profiles are asymmetric and are found to vary across the cloud in such a manner that the presence of both inward and outward motions are observed within the cloud. Moreover, these motions appear to be globally organized in a clear and systematic alternating spatial pattern which is suggestive of a small amplitude, non-radial oscillation or pulsation of the outer layers of the cloud about an equilibrium configuration.Comment: To appear in the Astrophysical Journal; 23 pages, 8 figures; Manuscript and higher resolution images can be obtained at http://cfa-www.harvard.edu/~ebergin/pubs_html/b68_vel.htm

Systematics of small Gehyra (Squamata: Gekkonidae) of the southern Kimberley, Western Australia: redescription of G. kimberleyi Börner & Schüttler, 1983 and description of a new restricted range species

Ongoing fieldwork and molecular research continues to reveal that the monsoonal tropics of northern Australia contain more vertebrate species than currently recognised. Here we focus on two morphologically distinctive, yet unrecognised forms in the genus Gehyra from the southern Kimberley region and surrounding deserts. We base our descriptions on a combination of unpublished genetic data and a morphological examination of voucher specimens. We recognise and redescribe G. kimberleyi, a species with a broad distribution extending over most of the south-west Kimberley, across the Great Sandy Desert and into the far northern Pilbara. This species has been previously assigned to G. pilbara owing to its frequent occurrence on termite mounds and short snout, but can be distinguished from G. pilbara and other regionally sympatric Gehyra by its moderate body size, moderate number of pre-cloacal pores in males (12-17) and aspects of dorsal colouration. We also describe G. girloorloo sp. nov., a small rock-dwelling species with a short snout, low number of pre-cloacal pores in males (8-11) and pinkish-grey dorsal colouration with alternating series of indistinct pale spots and irregular transversely-aligned dark blotches. The new species appears to be restricted to a relatively small region of exposed limestone karst in the south-west Kimberley and is entirely circumscribed by morphologically similar congeners.This work was supported by grants from the Australian Research Council to Paul Oliver, Michael Lee and Paul Doughty, a Melbourne University Collaboration grant to Jane Melville and Paul Oliver, a McKenzie Postdoctoral fellowship to Paul Oliver from Melbourne University, an Australian Biological Resources Study grant to Craig Moritz and Scott Keogh and an ARC Laureate Fellowship to C. Moritz

Selecting and modifying methods of manual muscle testing for classification in Paralympic sport

Many Paralympic sports classification systems use unspecified manual muscle testing (MMT) methods to assess impairment of muscle strength. This is a potential source of inconsistency in classification, and could be eliminated by nominating a single, published set of MMT methods. Additionally, four modifications can enhance the validity, reliability and utility of conventional MMT methods for classification: 1) limiting assessment to movements that are important to performance in the sport concerned; 2) specifying a single preferred technique for assessment of movement strength; 3) changing the reference range of movement from normal anatomical range to the maximum range of movement required in sport; and 4) adjusting testing techniques so that they are relevant for the sport. This brief communication may improve classification in established sports, and provide guidance for emerging sports that are developing classification systems