18,554 research outputs found
Hydrothermal sediments are a source of water column Fe and Mn in the Bransfield Strait, Antarctica
No full textShort sediment cores were collected from ~1100 m water depth at the top of Hook Ridge, a submarine volcanic edifice in the Central Basin of the Bransfield Strait, Antarctica, to assess Fe and Mn supply to the water column. Low-temperature hydrothermal fluids advect through these sediments and, in places, subsurface H2S is present at high enough concentrations to support abundant Sclerolinum sp., an infaunal tubeworm that hosts symbiotic thiotrophic bacteria. The water column is fully oxic, and oxygen penetration depths at all sites are 2-5 cmbsf. Pore water Fe and Mn content is high within the subsurface ferruginous zone (max. 565 µmol Fe L-1, >3 to 7 cmbsf) — 14-18 times higher than values measured at a nearby, background site of equivalent water depth. Diffision and advection of pore waters supply significant Fe and Mn to the surface sediment. Sequential extraction of the sediment demonstrates that there is a significant enrichment in a suite of reactive, authigenic Fe minerals in the upper 0-5 cm of sediment at one site characterised by weathered crusts at the seafloor. At a site with only minor authigenic mineral surface enrichment we infer that leakage of pore water Fe and Mn from the sediment leads to enriched total dissolvable Fe and Mn in bottom waters. The largest Eh anomaly observed from our Bransfield Strait survey is associated with the elevated total dissolvable metal content in the water column above this coring site.. We hypothesize that the main mechanism for Fe and Mn efflux from the sediment is breach of the surface oxic layer by the abundant Sclerolinum sp., along with episodic enhancements by physical mixing and resuspension of sediment in this dynamic volcanic environment. We propose that Hook Ridge sediments are an important source of Fe and Mn to the deep waters of the Central Basin in the Bransfield Strait, where concentrations are sustained by the benthic flux, and Fe is stabilised in the water column as either colloidal phases or ligand-bound dissolved species. Entrainment of this water mass into the Drake Passage and thereby the Antarctic Circumpolar Current could provide a significant metal source to this HNLC region of the Southern Ocean if mixing and upwelling occurs before removal of this metal pool to underlying sediments. Sediment-covered volcanic ridges are common within rifted margins and may play a previously overlooked role in the global Fe cycle
Peter Grimes. Embroidery. Vocal score
No full text1 vocal score (6 p.) ; 31 cm.
H. 15720 Boosey & Hawkes
Cover title.
Copyright renewed, 1972.
From act 3, scene 1
Asphinctopone pilosa Hawkes, sp. n.
No full textAsphinctopone pilosa Hawkes sp. n. (Fig. 1, A–E) Holotype worker. TL 4.48, HL 1.07, HW 0.86, CI 81, SL 0.80, SI 92, OD 0.06, OI 7, PW 0.66, WL 1.38 (all measurements in mm). Medium sized (total length c. 4.5 mm) ponerine ant largely conforming to the diagnosis of the genus as presented by Bolton & Fisher (2008), but with differences in the development of the promesonotal and metanotal grooves, antennal structure and median clypeal lobe as indicated below. Mandibles smooth and shining, without any sculpture other than coarse scattered hair-pits and with five teeth plus a small denticle between the basal and the second tooth. No tooth-like process on the inner basal margin of the mandible. Eyes very small, comprising a single central ommatidium surrounded by a ring of 6 less distinct ommatidia, positioned distinctly in front of the mid-length of the sides of the head. Ocular diameter less than half the maximum width of the antennal scape. Entire dorsum, sides and ventral surfaces of head with quite coarse punctures (up to 0.03 mm diameter) with weak irregular sculpture between the punctures on the dorsal and dorso-lateral surfaces. Median portion of the vertex, as well as the sides of the head below the eyes, with larger and more widely spaced punctures. Pubescence on head dense, decumbent and arising both from within the numerous large punctures and from minute hair-pits between these, more sparse on the sides of the head below the eye and on the underside, giving these areas a smoother and more polished appearance. Frontal lobes somewhat more densely and more finely punctulate than remainder of the head; frontal carinae and antennal scrobes absent. In full-face view the sides and the posterior margin of the head very shallowly convex. Antennal scapes when laid back just reaching the occipital margin. Funicular segments 2–10 broader than long, segments 2–7 very distinctly so. Funicular segments 8–11 broader than the preceding 6, becoming increasingly longer relative to their width and forming an indistinctly 4 -segmented club. The terminal funicular segment much longer than broad and distinctly exceeding the combined length of the preceding 5 segments. Clypeus with a projecting median lobe bounded by a rounded obtuse angle on each side, the anterior margin of this lobe flat to very slightly concave laterally and with a broadly rounded median projection. Width of the anterior margin of the projecting clypeal lobe about 0.33 x HW. Several pairs of strong setae and a number of weaker setae present on the clypeus. Mesosoma with a pattern of sculpturing very similar to that of the head; dorsum and sides of pronotum, mesonotum and propodeum entirely coarsely punctulate and covered with a dense pelt of fine suberect (pronotum and mesonotum) to erect (propodeum) curved pubescence, the katepisternum and the disc of the pronotum with more sparse punctures and pilosity. Ventral surfaces of the mesosoma with dense fine puncturation and reduced pubescence. The punctulate sculpture on the dorsal and lateral mesosoma is overlaid by irregular effaced fine rugulose sculpture everywhere except on the disc of the pronotum and small areas of the lower propleuron and katepisternum. Pronotal humeri broadly rounded; the pronotum with a subglobose appearance in dorsal view. Promesonotal suture moderately impressed and with cross-ribs on the anterior mesonotum, the metanotal groove only slightly impressed and with fewer more widely spaced but much longer cross-ribs. Mesonotum twice as wide as long. Propodeal dorsum narrow, about half the width of the mesonotum and extending horizontally from the level of the metanotal groove to the short upper portion of the declivity, which slopes downward at about 45 o to the junction with the very steep main face of the declivity. The propodeal outline thus presents three distinct planes in profile view. Propodeal dorsum about 1.5 x as long as the mesonotum. Declivity of the propodeum the only portion of the dorsal mesosoma lacking sculpture and with greatly reduced pilosity; smooth and weakly shining. Petiole node high and squamiform, unsculptured apart from minute hair-pits, smooth and weakly shining and with pubescence similar to but less dense than that on the mesosoma. In profile view the anterior and posterior faces of the petiole node almost parallel, only slightly convergent dorsally; in posterior view the dorsal margin forming a bluntly triangular peak. In dorsal view the anterior face shallowly convex, the posterior even more shallowly concave. Subpetiolar process with the complex shape characteristic of the genus. Gaster unsculptured apart from minute hair-pits (c. 0.005 mm diameter), pubescence denser but shorter (0.04 mm) on tergites 2–4 than on the first gastral tergite (0.07 mm), much longer and more variable on the sternites. No setae present on gastral tergites 1–4, but a few pairs on each sternite and abundant setae present on the pygidium and hypopygium. Sting stout and slightly upcurved in lateral view, somewhat laterally flattened. A single (pectinate) spur is present on each tibia, those on the metatibiae much longer (0.34 mm) than those on the mesotibiae (0.17 mm), with those on the protibiae intermediate in length (0.29 mm). All segments of the appendages, including the antennae, with fine appressed pubescence but no standing hairs. Colour: head and mesosoma dark reddish-brown throughout, the gaster, appendages and mandibles a lighter reddish-brown, with the exception of a small yellowish-brown patch on each mandible. Holotype worker. Tanzania, Tanga Region, Kilindi Forest Reserve, 1015 m, S 5.57934 E 37.57971, 28.viii. 2005, CEPF-TZ- 3.4.F 34, SAM-HYM-C 020683, Primary forest, hand collected (P. H a w k e s, J. Makwati, R. Mtana) (SAMC). Comments. Asphinctopone pilosa is distinctly different from its congeners in many respects; the most obvious differences are 1) its larger size, 2) the stronger and much more extensive sculpturation and denser pubescence, 3) the differently shaped mesonotum and propodeum, 4) the far less strongly impressed promesonotal suture and metanotal groove, 5) the terminal four, rather than three, antennal segments forming a weak club, 6) the more strongly squamiform petiole, which is also more arcuate in dorsal view, 7) the lessdeveloped clypeal structure (in sylvestrii and differens the median clypeal lobe is bounded by distinct sharp angles, is distinctly though shallowly concave on either side of the more acutely rounded median projection and is relatively broader at about 0.40 x HW), 8) the lack of a tooth-like process on the inner basal margin of the mandible and 9) its darker colour. Etymology: The specific epithet pilosa refers to the pubescence which is much denser on the head and mesosoma than in all previously described species of the genus. Habitat. The Kilindi Forest Reserve (5395 ha) lies about 140 km inland and comprises a small area of forest on an isolated double-peaked mountain surrounded by miombo woodland; the survey site was located at about 1000 m altitude on a mainly flat area on the saddle between the two peaks. The forest canopy here was estimated to average about 25 m high, with some emergent trees of 35–40 m; closure of the canopy was estimated at approximately 70–80 %. Previous disturbance and tree felling by informal gold miners was evident and numerous young trees and climbers were observed in partially cleared areas. Soils along the survey transect were mainly of sandy loam texture (with some patches of sandy clay loam), a pH of 8.0– 8.5 and with a thin (1–2 cm depth) leaf litter layer ranging from 25 % to 100 % cover. The survey was carried out toward the end of the cool dry season in late August 2005; soil temperatures averaged 16 o C at a depth of 10– 15 cm, with soil moisture at the same depth averaging 11.9 %. The Asphinctopone pilosa specimen was, however, collected in a microhabitat with higher moisture levels and a much thicker litter layer than average for the site. Humidity during the three-day site visit ranged from 63.4 % to 99.3 % (the latter during an unseasonal rainstorm) and averaged 81.4 %, while the temperature varied from 12.0– 22.5 o C. Climate. Detailed climatic data are not readily available for all of the localities from which other Asphinctopone specimens have been collected, but inspection of Worldclim (version 1.3) 2.5 arc-minute extrapolated climate data (Hijmans et al. 2005) downloaded via http://www.diva-gis.org/climate provides some indication of conditions within the known distribution (see Figure 2) of the genus. Most of the localities exhibit low seasonal variation in temperature and precipitation. The A. pilosa locality was an outlier in respect of some of the bioclimatic variables (it has the highest temperature seasonality, lowest mean annual temperature and lowest mean temperature of the driest quarter), but in most variables was similar to previously recorded Asphinctopone localities. Modelling of habitat suitability and predicted distribution. Of the nine bioclimatic variables selected for inclusion in the model, two showed a close to normal and one a truncated normal distribution, while six were strongly skewed. For three of the variables with skewed distributions (min. temperature of coldest month, mean temperature of coldest quarter and mean temperature of driest quarter) estimates from visual inspection indicated that less than 5 % of the entire African continent has values higher than the modal value of the Asphinctopone localities. This suggests that intolerance to low temperatures may be a significant factor influencing distribution. Test predictions in BIOCLIM using all of the 19 bioclimatic variables or the selected subset of nine without the tail box adjustment gave implausible results with most (14–16 of 19) recorded A. silvestrii localities placed at or near (<10 km) an edge of the predicted distribution; using the adjustment and the selected variable subset gave far more probable results, with the majority (13) of these records falling well within the predicted distribution. In addition to the seven countries (Cameroon, Central African Republic, Gabon, Ghana, Guinea, Ivory Coast and Nigeria) from which A. silvestrii and A. differens have been recorded to date, BIOCLIM modelling predicted a reasonable probability (see Figure 3 A) that one or both of these species could occur in a further 12 African countries (Angola, Benin, Democratic Republic of the Congo, Ethiopia, Equatorial Guinea, Kenya, Liberia, Republic of the Congo, Sierra Leone, Sudan, Toga and Uganda). However, in some cases the distribution within these countries is expected to be very limited (e.g. to the far north-east in Angola, the southern Sudan and western Ethiopia). Inclusion of the A. pilosa locality in the model resulted in the predicted suitable area in many of these countries increasing substantially (see Figure 3 B) and also in the inclusion of parts of north-western Tanzania. While this may not be a realistic expansion of the predicted ranges of A. silvestrii and A. differens, it could indicate the possibility of additional Asphinctopone species in areas beyond the ranges of the known species. It is recognised that BIOCLIM often under-predicts species distributions (Ward 2007), but the use here of a selected subset of bioclimatic variables and adjusting tail checkboxes resulted in a predicted distribution greater than the core area predicted by DOMAIN (Figure 3 C and 3 D). The large non-core area mapped by the latter model illustrates a low predicted probability of occurrence, so the apparently very large predicted distributions in Figure 3 C and 3 D should perhaps be viewed with some scepticism, especially as the latter includes some very improbable areas such as a large portion of the Namib desert.Published as part of Hawkes, Peter G., 2010, A new species of Asphinctopone (Hymenoptera: Formicidae: Ponerinae) from Tanzania, pp. 27-36 in Zootaxa 2480 on pages 29-34, DOI: 10.5281/zenodo.19542
The politics and economics of regulatory impact assessment
No full textThis is the author accepted manuscript. The final version is available from the publisher via the link in this record
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The diffusion coefficient of propane in helium
No full textA specially designed gas chromatograph with both TCD and FID has
been tested for the measurement of the diffusion coefficients of methane and propane in helium. Knox's arrested elution technique(⁴) was used and yielded a value of 0.6431 cm²/sec averaged with the value
obtained by Yang and Hawkes(⁷). Values of the binary molecular diffusion coefficient for propane in He were obtained at atmospheric pressure over the temperature range from 21.3 to 60.3°C. The data fitted
the equation log D₁00₂ = -8.1277 + 3.0805 log T with correlation coefficient of 0.9976
Asphinctopone pilosa Hawkes, 2010, sp. n.
No full text<p>Asphinctopone pilosa Hawkes sp. n.</p> <p>(Fig. 1, A -E)</p> <p>Holotype worker. TL 4.48, HL 1.07, HW 0.86, CI 81, SL 0.80, SI 92, OD 0.06, OI 7, PW 0.66, WL 1.38 (all measurements in mm).</p> <p>Medium sized (total length c. 4.5 mm) ponerine ant largely conforming to the diagnosis of the genus as presented by Bolton & Fisher (2008), but with differences in the development of the promesonotal and metanotal grooves, antennal structure and median clypeal lobe as indicated below.</p> <p>Mandibles smooth and shining, without any sculpture other than coarse scattered hair-pits and with five teeth plus a small denticle between the basal and the second tooth. No tooth-like process on the inner basal margin of the mandible. Eyes very small, comprising a single central ommatidium surrounded by a ring of 6 less distinct ommatidia, positioned distinctly in front of the mid-length of the sides of the head. Ocular diameter less than half the maximum width of the antennal scape. Entire dorsum, sides and ventral surfaces of head with quite coarse punctures (up to 0.03 mm diameter) with weak irregular sculpture between the punctures on the dorsal and dorso-lateral surfaces. Median portion of the vertex, as well as the sides of the head below the eyes, with larger and more widely spaced punctures. Pubescence on head dense, decumbent and arising both from within the numerous large punctures and from minute hair-pits between these, more sparse on the sides of the head below the eye and on the underside, giving these areas a smoother and more polished appearance. Frontal lobes somewhat more densely and more finely punctulate than remainder of the head; frontal carinae and antennal scrobes absent. In full-face view the sides and the posterior margin of the head very shallowly convex. Antennal scapes when laid back just reaching the occipital margin. Funicular segments 2-10 broader than long, segments 2-7 very distinctly so. Funicular segments 8-11 broader than the preceding 6, becoming increasingly longer relative to their width and forming an indistinctly 4-segmented club. The terminal funicular segment much longer than broad and distinctly exceeding the combined length of the preceding 5 segments. Clypeus with a projecting median lobe bounded by a rounded obtuse angle on each side, the anterior margin of this lobe flat to very slightly concave laterally and with a broadly rounded median projection. Width of the anterior margin of the projecting clypeal lobe about 0.33 x HW. Several pairs of strong setae and a number of weaker setae present on the clypeus.</p> <p>Mesosoma with a pattern of sculpturing very similar to that of the head; dorsum and sides of pronotum, mesonotum and propodeum entirely coarsely punctulate and covered with a dense pelt of fine suberect (pronotum and mesonotum) to erect (propodeum) curved pubescence, the katepisternum and the disc of the pronotum with more sparse punctures and pilosity. Ventral surfaces of the mesosoma with dense fine puncturation and reduced pubescence. The punctulate sculpture on the dorsal and lateral mesosoma is overlaid by irregular effaced fine rugulose sculpture everywhere except on the disc of the pronotum and small areas of the lower propleuron and katepisternum. Pronotal humeri broadly rounded; the pronotum with a subglobose appearance in dorsal view. Promesonotal suture moderately impressed and with cross-ribs on the anterior mesonotum, the metanotal groove only slightly impressed and with fewer more widely spaced but much longer cross-ribs. Mesonotum twice as wide as long. Propodeal dorsum narrow, about half the width of the mesonotum and extending horizontally from the level of the metanotal groove to the short upper portion of the declivity, which slopes downward at about 45o to the junction with the very steep main face of the declivity. The propodeal outline thus presents three distinct planes in profile view. Propodeal dorsum about 1.5 x as long as the mesonotum. Declivity of the propodeum the only portion of the dorsal mesosoma lacking sculpture and with greatly reduced pilosity; smooth and weakly shining.</p> <p>Petiole node high and squamiform, unsculptured apart from minute hair-pits, smooth and weakly shining and with pubescence similar to but less dense than that on the mesosoma. In profile view the anterior and posterior faces of the petiole node almost parallel, only slightly convergent dorsally; in posterior view the dorsal margin forming a bluntly triangular peak. In dorsal view the anterior face shallowly convex, the posterior even more shallowly concave. Subpetiolar process with the complex shape characteristic of the genus.</p> <p>Gaster unsculptured apart from minute hair-pits (c. 0.005 mm diameter), pubescence denser but shorter (0.04 mm) on tergites 2-4 than on the first gastral tergite (0.07 mm), much longer and more variable on the sternites. No setae present on gastral tergites 1-4, but a few pairs on each sternite and abundant setae present on the pygidium and hypopygium. Sting stout and slightly upcurved in lateral view, somewhat laterally flattened.</p> <p>A single (pectinate) spur is present on each tibia, those on the metatibiae much longer (0.34 mm) than those on the mesotibiae (0.17 mm), with those on the protibiae intermediate in length (0.29 mm). All segments of the appendages, including the antennae, with fine appressed pubescence but no standing hairs.</p> <p>Colour: head and mesosoma dark reddish-brown throughout, the gaster, appendages and mandibles a lighter reddish-brown, with the exception of a small yellowish-brown patch on each mandible.</p> <p>Holotype worker. Tanzania, Tanga Region, Kilindi Forest Reserve, 1015 m, S 5.57934 E 37.57971, 28.viii.2005, CEPF-TZ-3.4.F34, SAM-HYM-C 020683, Primary forest, hand collected (P. Hawkes, J. Makwati, R. Mtana) (SAMC).</p> <p>Comments. Asphinctopone pilosa is distinctly different from its congeners in many respects; the most obvious differences are 1) its larger size, 2) the stronger and much more extensive sculpturation and denser pubescence, 3) the differently shaped mesonotum and propodeum, 4) the far less strongly impressed promesonotal suture and metanotal groove, 5) the terminal four, rather than three, antennal segments forming a weak club, 6) the more strongly squamiform petiole, which is also more arcuate in dorsal view, 7) the lessdeveloped clypeal structure (in sylvestrii and differens the median clypeal lobe is bounded by distinct sharp angles, is distinctly though shallowly concave on either side of the more acutely rounded median projection and is relatively broader at about 0.40 x HW), 8) the lack of a tooth-like process on the inner basal margin of the mandible and 9) its darker colour.</p> <p>Etymology: The specific epithet pilosa refers to the pubescence which is much denser on the head and mesosoma than in all previously described species of the genus.</p> <p>Habitat. The Kilindi Forest Reserve (5395 ha) lies about 140 km inland and comprises a small area of forest on an isolated double-peaked mountain surrounded by miombo woodland; the survey site was located at about 1000 m altitude on a mainly flat area on the saddle between the two peaks. The forest canopy here was estimated to average about 25 m high, with some emergent trees of 35-40 m; closure of the canopy was estimated at approximately 70-80%. Previous disturbance and tree felling by informal gold miners was evident and numerous young trees and climbers were observed in partially cleared areas. Soils along the survey transect were mainly of sandy loam texture (with some patches of sandy clay loam), a pH of 8.0-8.5 and with a thin (1-2 cm depth) leaf litter layer ranging from 25% to 100% cover. The survey was carried out toward the end of the cool dry season in late August 2005; soil temperatures averaged 16oC at a depth of 10- 15 cm, with soil moisture at the same depth averaging 11.9%. The Asphinctopone pilosa specimen was, however, collected in a microhabitat with higher moisture levels and a much thicker litter layer than average for the site. Humidity during the three-day site visit ranged from 63.4% to 99.3% (the latter during an unseasonal rainstorm) and averaged 81.4%, while the temperature varied from 12.0-22.5oC.</p> <p>Climate. Detailed climatic data are not readily available for all of the localities from which other Asphinctopone specimens have been collected, but inspection of Worldclim (version 1.3) 2.5 arc-minute extrapolated climate data (Hijmans et al. 2005) downloaded via http://www.diva-gis.org/climate provides some indication of conditions within the known distribution (see Figure 2) of the genus. Most of the localities exhibit low seasonal variation in temperature and precipitation. The A. pilosa locality was an outlier in respect of some of the bioclimatic variables (it has the highest temperature seasonality, lowest mean annual temperature and lowest mean temperature of the driest quarter), but in most variables was similar to previously recorded Asphinctopone localities.</p> <p>Modelling of habitat suitability and predicted distribution. Of the nine bioclimatic variables selected for inclusion in the model, two showed a close to normal and one a truncated normal distribution, while six were strongly skewed. For three of the variables with skewed distributions (min. temperature of coldest month, mean temperature of coldest quarter and mean temperature of driest quarter) estimates from visual inspection indicated that less than 5% of the entire African continent has values higher than the modal value of the Asphinctopone localities. This suggests that intolerance to low temperatures may be a significant factor influencing distribution. Test predictions in BIOCLIM using all of the 19 bioclimatic variables or the selected subset of nine without the tail box adjustment gave implausible results with most (14-16 of 19) recorded A. silvestrii localities placed at or near (<10 km) an edge of the predicted distribution; using the adjustment and the selected variable subset gave far more probable results, with the majority (13) of these records falling well within the predicted distribution.</p> <p>In addition to the seven countries (Cameroon, Central African Republic, Gabon, Ghana, Guinea, Ivory Coast and Nigeria) from which A. silvestrii and A. differens have been recorded to date, BIOCLIM modelling predicted a reasonable probability (see Figure 3A) that one or both of these species could occur in a further 12 African countries (Angola, Benin, Democratic Republic of the Congo, Ethiopia, Equatorial Guinea, Kenya, Liberia, Republic of the Congo, Sierra Leone, Sudan, Toga and Uganda). However, in some cases the distribution within these countries is expected to be very limited (e.g. to the far north-east in Angola, the southern Sudan and western Ethiopia). Inclusion of the A. pilosa locality in the model resulted in the predicted suitable area in many of these countries increasing substantially (see Figure 3B) and also in the inclusion of parts of north-western Tanzania. While this may not be a realistic expansion of the predicted ranges of A. silvestrii and A. differens, it could indicate the possibility of additional Asphinctopone species in areas beyond the ranges of the known species.</p> <p>It is recognised that BIOCLIM often under-predicts species distributions (Ward 2007), but the use here of a selected subset of bioclimatic variables and adjusting tail checkboxes resulted in a predicted distribution greater than the core area predicted by DOMAIN (Figure 3C and 3D). The large non-core area mapped by the latter model illustrates a low predicted probability of occurrence, so the apparently very large predicted distributions in Figure 3C and 3D should perhaps be viewed with some scepticism, especially as the latter includes some very improbable areas such as a large portion of the Namib desert.</p> <p>Discussion</p> <p>Taxonomy. While Asphinctopone pilosa displays certain characters that do not fit the diagnosis of the genus as presented by Bolton & Fisher (2008), there can be no doubt that it belongs in this genus; several sections of their diagnosis should therefore be modified slightly to read as follows (characters in italics were considered autapomorphic by Bolton & Fisher, 2008; the numbering of characters by these authors has been retained for ease of reference):</p> <p>4 Basalmost tooth is at the rounded basal angle; basal margin shallowly convex.</p> <p>6 Clypeus complex: in full-face view the median portion projects anteriorly as a broad lobe which terminates in a rounded to distinct angle on each side; these angles overlap the basal margins of the mandibles; the anterior clypeal margin has a median rounded projection, on each side of which the anterior margin is flat to shallowly concave; above the median projection the central portion of the clypeus forms a narrow ridge to the frontal lobes.</p> <p>8 Antenna with 12 segments, gradually incrassate apically, with the terminal three or four segments forming a weak club, apical antennomere hypertrophied, longer than the five preceding segments together.</p> <p>9 Promesonotal suture moderately to deeply impressed, cross-ribbed on extreme anterior mesonotum; metanotal groove slightly to deeply impressed and cross-ribbed; mesonotum clearly to conspicuously isolated by these impressions (worker only).</p> <p>The lack of a) a deeply impressed promesonotal suture and b) a tooth-like process on the basal mandibular margin in Asphinctopone pilosa reduces the degree to which Asphinctopone is distinguished from the melanaria-group species of Pachycondyla (see Bolton & Fisher 2008). However, numerous distinguishing characters as described by Bolton & Fisher (2008) remain to clearly separate these taxa: in the melanariagroup species of Pachycondyla the mandible is triangular to elongate-triangular rather than oblique, there are more than 6 teeth on the apical mandibular margin, the apical antennomere is not hypertrophied, the anterior clypeal margin is simple, the promesonotal suture is not cross-ribbed, the mesotibiae and metatibiae each have two spurs, the petiole sternite has a simple posterior structure, the helcium and prora are not modified as in Asphinctopone and presclerites are present on the second gastral segment (the apparently derived helcium structure has not yet been confirmed in A. differens or A. pilosa as this would require dissection of their respective unique holotypes).</p> <p>Habitat and distribution. Asphinctopone are very rarely encountered; whether this is due to actual rarity of members of the genus, or to a secretive and perhaps deeply subterranean lifestyle, is unknown. The significance of the A. pilosa specimen was not recognised at the time of collection, but the location (an accumulation of moist leaf litter at the base of a large sloping rock outcrop) was revisited the following day as it was observed to be moister and more productive in terms of ponerine ant species than its surroundings. However no further specimens of Asphinctopone were found in the additional samples collected here, or in any of the other standardized pitfall, leaf litter or hand-collected samples. No other Asphinctopone specimens were found amongst the 67 208 ants collected and processed during the course of the project. This confirms the rarity of encounter of members of the genus as discussed by Bolton & Fisher (2008), who noted that Belshaw & Bolton (1994) reported finding only five Asphinctopone specimens in a total of 43 824 ants collected in a survey of leaf litter in Ghana.</p> <p>That the only known specimen of A. pilosa was collected during the evening (between 19:30 and 20:00), while no further specimens were found in the same area during daytime, suggests the possibility that they are nocturnal, but this is clearly pure conjecture at this stage given the limited information available.</p> <p>The distribution of Asphinctopone previously appeared to be limited to the moist forest zones of West and Central Africa; its discovery in the Kilindi Forest Reserve represents a more than 1600 km eastward extension of the known range of the genus, and the site is approximately 2000 km from the closest previously recorded Asphinctopone locality. While subjective predictions (Guénard et al. 2010) suggest that Asphinctopone should occur in some additional counties (Benin, Equatorial Guinea, Liberia, Sierra Leone and Toga), the BIOCLIM modelling presented here indicates that a much larger range is likely, with presence expected in at least a further seven countries (Angola, Democratic Republic of the Congo, Ethiopia, Kenya, Republic of the Congo, Sudan and Uganda) in addition to the confirmed presence in Tanzania.</p> <p>Although some habitat predicted to be suitable for A. silvestrii and A. differens is shown in the coastal regions of Kenya, northern Mozambique and Somalia (Figure 3), the broad band of unsuitable habitat isolating these areas from the remainder of the predicted distribution of these species suggests that they are unlikely to occur here. It is far more likely that A. pilosa will be found in these areas. Other areas which appear bioclimatically suitable but geographically improbable for Asphinctopone are the Comoros Islands and parts of Madagascar.</p> <p>Exclusion of the bulk of the central Congo Basin from the BIOCLIM predictions appears to be due largely to the very low precipitation seasonality and (obviously correlated) high precipitation of the driest quarter, as well as the very low temperature seasonality of this region. A trial run showed that inclusion of a single positive point within the central Congo basin would result in BIOCLIM including the entire basin in the predicted distribution. This part of the map could therefore change significantly with very little additional data. It is also important to note that I have here attempted to model the potential distribution of a genus using data almost entirely (90%) on only one of three Asphinctopone species; there is thus little scope for influence of the preferences of the other two species, nor any other as yet undiscovered species, on the extent of the predicted distribution. It is therefore possible that the distribution of Asphinctopone will eventually be found to be much greater than suggested here by BIOCLIM, and maybe even to cover a substantial portion of the low probability area predicted by DOMAIN, but it is hoped that this exercise will help to focus efforts on finding additional material in the most likely areas.</p> <p>It should be kept in mind that while occurrences of specimen records in areas with particular bioclimatic conditions may appear to indicate a preference for such conditions, it is also possible (especially in the case of cryptic taxa such as Asphinctopone) that this is an artefact of the conditions providing greater probability of discovery. For example, in areas with low precipitation seasonality and/or higher minimum temperatures, subterranean species may spend more time closer to the soil surface and therefore be more likely to be collected. A much broader Asphinctopone distribution than suggested by BIOCLIM is thus possible, and could be revealed by more intensive searches using deeper excavation than currently employed in most ant surveys.</p>Published as part of <i>Hawkes, P. G., 2010, A new species of Asphinctopone (Hymenoptera: Formicidae: Ponerinae) from Tanzania., pp. 27-36 in Zootaxa 2480</i> on pages 29-3
The sedimentary record of the 2005 hurricane season from the Mississippi and Alabama coastlines
No full textThe instrumental record of hurricane activity is too short to fully capture the occurrence of the rare but most destructive hurricanes. Therefore, obtaining a record of present and past landfalling hurricanes, and their extent of geological and ecological impacts, is one means to assess future risk, reveal the spatial and temporal variability of hurricane activity and decipher its relationship with global climatic changes. We rapidly dispatched survey teams to collect the readily available, but perishable data of Hurricanes Katrina and Rita storm surge from two salt marshes in Mississippi and one salt marsh in Alabama. In Mississippi, we recorded Hurricane Katrina storm surge heights greater than 7.5m North American Vertical Datum 88 (NAVD88) with inland extents in excess of 700 m, whereas in Alabama the maximum recorded storm surge was 3.43m NAVD88. At one salt marsh in Mississippi, we recorded the maximum inland extent and elevation of maximum penetration of Hurricane Rita as 370m and 3.43m NAVD88, respectively. We observed a three-dimensional distribution of hurricane-induced storm surge deposits that tapered landward, overlying salt marsh sediment. There was a sharp or erosional boundary between the pre-storm surge and storm surge sedimentary units, which was accompanied by a change in color and lithology. The overlying storm surge sediment unit was coarser than the pre-storm surge unit with a lower organic content. The thickness of the Hurricanes Katrina and Rita storm surge sediments ranged from 9 to 13 cm and approximately 7 cm, respectively. Foraminiferal analyses revealed a virtual absence of tests within the storm surge sediments, whereas abundant agglutinated foraminifera were found in the underlying salt marsh deposits
Phase Distribution Efficiency of cm-Scale Ultrasonically Powered Receivers
No full textIn the domain of ultrasonically powered biomedical implants, there is an increasing interest in cm-scale ultrasonic receivers (RX). However, when a single-element transducer is used as the RX transducer, an uneven phase distribution across the RX area can significantly reduce the harvestable power. In this paper, we investigate the impact of lateral and angular misalignment on the acoustic field phase distribution across the RX surface. We show that, for a single-element RX transducer, lateral misalignment has minimal effect on the harvestable power, whereas even small angular misalignments can cause a considerable reduction, especially for larger RX sizes. We present a potential solution that consists of subdividing a large RX transducer (e.g. 20 × 20mm2) into smaller elements, which significantly improves power transfer efficiency by taking advantage of the smaller phase variation across the surface of each element. The trade-offs between achieving a minimum acceptable power transfer efficiency and managing the increased complexity in packaging and matching circuitry are also discussed.Green Open Access added to TU Delft Institutional Repository 'You share, we take care!' - Taverne project https://www.openaccess.nl/en/you-share-we-take-care Otherwise as indicated in the copyright section: the publisher is the copyright holder of this work and the author uses the Dutch legislation to make this work public.Electronic Components, Technology and MaterialsBio-Electronic
Highly efficient laser-driven Compton gamma-ray source
No full textThe recent advancement of high-intensity lasers has made all-optical Compton scattering become a promising way to produce ultrashort brilliant gamma-rays in an ultra-compact system. However, so far achieved Compton gamma-ray sources are limited by low conversion efficiency and spectral intensity. Here we present a highly efficient gamma photon emitter obtained by irradiating a high-intensity laser pulse on a miniature plasma device consisting of a plasma lens and a plasma mirror. This concept exploits strong spatiotemporal laser-shaping process and high-charge electron acceleration process in the plasma lens, as well as an efficient nonlinear Compton scattering process enabled by the plasma mirror. Our full three-dimensional particle-in-cell simulations demonstrate that in this novel scheme, brilliant gamma-rays with very high conversion efficiency (higher than 10(-2)) and spectral intensity (similar to 10(9) photons/0.1%BW) can be achieved by employing currently available petawatt-class lasers with intensity of 10(21) W cm(-2). Such efficient and intense gamma-ray sources would find applications in wide-ranging areas. ©2019 The Author(s)
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