A greenhouse study on root dynamics of cactus pears, Opuntia ficus-indica and O. robusta

Over the last 10 years a great interest in spineless cactus pear was shown in the drier areas in terms of both fresh fruit and fodder production. However, there is a lack of knowledge on quantitative data on root dynamics of these plants needed to fully understand its potential under water limiting conditions. This study aimed at quantifying the effects of water stress on the growth of tap roots, side roots and rain roots of the species Opuntia ficus-indica (L.) Miller (cultivar Morado—green cladode) and O. robusta Wendl. (cultivar Monterey—blue cladode). One-year-old cladodes were planted in root boxes and pots (2002/2003 season) that were kept in the greenhouse at day/night temperatures of 25–30 °C/15–18 °C. Placing the cladodes flat on the soil, more areoles came in contact with the soil and therefore more roots developed in both species with an average of only 3.4% areole complexes not rooting. Each areole complex formed on average 3 roots. The highest daily tap root growth was 42 and 36 mm for O. ficus-indica and O. robusta, respectively. Tap root growth increased in the morning with water stress for both species but decreased in the afternoon. Side root growth increased with water stress, with that of O. robusta more per tap root than O. ficus-indica. O. robusta showed a finer root system than O. ficus-indica. The side roots grew as much as 8 and 5 mm per day for O. ficus-indica and O. robusta, respectively. Whitish rain roots developed on the established roots within the first hour after rewetting the soil and grew for only 3 days. Rain roots grew up to 7 and 5 mm within a day for O. ficus-indica and O. robusta, respectively. Considering all studied aspects of their roots systems, O. robusta appears to be better adapted to drought (less sensitive to water stress) than O. ficus-indica.     

Freshwater and Atlantic water inflows to the deep northern Barents and Kara seas since ca 13 C ka: : foraminifera and stable isotopes

Foraminiferal stable isotopes and assemblages from Franz Victoria and St. Anna troughs provide a valuable record of freshwater and Atlantic Water flows to the northern Barents and Kara seas from deglaciation to present. The δ¹⁸O and δ¹³C of planktonic Neogloboquadrina pachyderma (s) and benthic Elphidium excavatum were up to 1.4‰ lower than present at ca 13, 11.5, and 10 ¹⁴C ka (global sea-level corrected), mostly reflecting substantial freshwater inputs coincident with glacial–marine sediment deposition. Cassidulina teretis exceeded 40% of benthic foraminifera ca 13 and 10 ¹⁴C ka, indicating subsurface penetrations of Atlantic Water. The transition to postglacial marine conditions is marked by a 1‰ rise in foraminiferal δ¹⁸O and a sharp fall in % C. teretis soon after 10 ¹⁴C ka. These changes imply reduced inputs of freshwater and Atlantic Water. Subsequent isotopic and foraminiferal assemblage variations reflect changing Atlantic Water conditions “upstream” in the Nordic Seas and shifts between the warm Fram Strait and cold Barents Sea branches of Atlantic Water. We hypothesize that glacial-isostatically induced deepening by up to 150 m influenced Atlantic Water inflows to the northern Barents Sea during deglaciation and the Holocene. Thus, effects of isostatic recovery have to be factored into paleoceanographic reconstructions.     

青海西部祁漫塔格成矿带找矿新进展及其意义

青海省祁漫塔格成矿带位于东昆仑造山带北西段,带内以往开展了以铁为主的找矿工作,发现一批矽卡岩型中型矿床。近年来带内找矿取得了重大突破:①发现一种新类型矿床——"虎头崖"式层控型大型多金属矿床;②低缓磁异常区多金属和铁矿找矿效果显著,发现四角羊-牛苦头大型多金属矿床,野马泉矿区多金属矿规模达到中型,尕林格矿区发现深部厚大的铁矿体。在系统地综合总结这些成果的基础上,探讨了找矿新进展的意义,划分了3处成矿远景区,并初步讨论了各成矿远景区内进一步找矿的方向。     

Exploring for heavy minerals on Cape York Peninsula,Queensland, Australia

This paper describes the results of a preliminary study of the heavy mineral (HM) potential of the northwest coast of Cape York Peninsula in far north Queensland that was funded by the Queensland Government's Future Resources Program Industry Priorities Initiative. The study found that the northwest coast may have the potential to host world-class HM deposits. All the essential ingredients in a HM mineral system are present: fertile source rocks, effective transport mechanisms and abundant potential trap sites, particularly along the well-preserved Pleistocene coast.

The source rocks are Proterozoic metamorphic and Paleozoic granitic rocks of the Coen Inlier and Mesozoic sedimentary rocks of the Laura and Carpentaria basins, all of which crop out along the spine of the Peninsula. These rocks were exposed in the early Cenozoic and were vigorously eroded by seasonally active rivers throughout the Quaternary. Most of these rivers are currently carrying HM, and the zircon content in river sediments in the region is comparatively high. It is speculated that in the late Pleistocene HM delivered by rivers to the northwest coast were transported predominantly in a southwesterly direction, and trapped in the swash zone of prograding beaches. It is further speculated that at this time the coastline was deeply embayed with cliffs and headlands formed in bauxite, and that structural trap sites formed on the northeastern side of prominent headlands.

Pleistocene coastal sediments were partially reworked by Holocene coastal processes, and HM liberated by these processes may have been captured by prograding Holocene beach ridges. These Holocene beach ridges are not as extensive as the Pleistocene beach ridges but are more prominent, partly because they are less well vegetated. The Holocene coastline was probably more regular than the Pleistocene coastline, with fewer headlands to create structural traps. The modern coastline is relatively starved of river sediment because the Holocene and Pleistocene coastal sediments act as barriers to river flow.

It is recommended that ongoing exploration for HM in the region should focus on potential trap sites on the Pleistocene coast and that two sites, Vrilya Point and Jackson River, where structural traps may have been formed by coastal promontories, should be priority targets. It is also noted that if the exploration of Cape York Peninsula for HM deposits is to be effective, further research needs to be carried out into the geomorphological evolution of the west coast and, in particular, the role of cyclones in forming HM deposits in tropical climates.     

The Cryogenic AntiCoincidence detector for ATHENA X-IFU: a scientific assessment of the observational capabilities in the hard X-ray band

ATHENA is a large X-ray observatory, planned to be launched by ESA in 2028 towards an L2 orbit. One of the two instruments of the payload is the X-IFU: a cryogenic spectrometer based on a large array of TES microcalorimeters, able to perform integral field spectrography in the 0.2–12 keV band (2.5 eV FWHM at 6 keV). The X-IFU sensitivity is highly degraded by the particle background expected in the L2 orbit, which is induced by primary protons of both galactic and solar origin, and mostly by secondary electrons. To reduce the particle background level and enable the mission science goals, the instrument incorporates a Cryogenic AntiCoincidence detector (CryoAC). It is a 4 pixel TES based detector, placed < 1 mm below the main array. In this paper we report a scientific assessment of the CryoAC observational capabilities in the hard X-ray band (E > 10 keV). The aim of the study has been to understand if the present detector design can be improved in order to enlarge the X-IFU scientific capability on an energy band wider than the TES array. This is beyond the CryoAC baseline, being this instrument aimed to operate as anticoincidence particle detector and not conceived to perform X-ray observations.     

Toxicity of No. 2 fuel oil to coon stripe shrimp

Bioassay of a No. 2 fuel oil dispersion with shrimp in a continuous flow system using measured waterborne oil as the indicator of oil concentrations reveals a treatment more definable than those previously described in terms of volume ratios and produces lower lethal concentrations. Shrimp 96-h LC₅₀ was 0.8 mg/l in this study as compared to values from 1.5 to 50 mg/l reported for other methods. Mean concentrations in tests do not give significant differences in concentration with respect to day of the test or spatial distribution in the exposure tanks.     

Saturation of the Large Aperture Scintillometer

The saturation aspects of a large aperture (0.3 m) scintillometer operating over a 10-km path were investigated. Measurements were made over mainly forested, hilly terrain with typical maximum sensible heat fluxes of 300–400 W m ⁻², and over flat terrain with mainly grass, and typical maximum heat fluxes of 100–150 W m⁻². Scintillometer-based fluxes were compared with eddy-correlation observations. Two different schemes for calculating the reduction of scintillation caused by saturation were applied: one based on the work of Hill and Clifford, the other based on Frehlich and Ochs. Without saturation correction, the scintillation fluxes were lower than the eddy-correlation fluxes; the saturation correction according to Frehlich and Ochs increased the scintillometer fluxes to an unrealistic level. Correcting the fluxes after the theory of the Hill and Clifford gave satisfying results