bluuebunny/crossref_metadata_2025_split huggingface dataset:
Effects of essential oil from Teucrium polium on some digestive enzyme activities of Musca domestica
Authors: BIGHAM Mahdieh , HOSSEININAVEH Vahid , NABAVI Banafsheh , TALEBI Khalil , ESMAEILZADEH Naimeh‐Sadat 
Published: January 2010

AbstractThe essential oil from Teucrium polium was evaluated for its adverse effects on larval instars of Musca domestica. The essential oil was blended with a diet at a concentration that produced 50% mortality of subjected insects (LC50) (80 ppm). To learn about the situation of digestive enzymes of M. domestica treated with the essential oil, third larval instars were dissected under non‐active enzyme conditions and their midguts were removed. The supernatant was used as an enzyme source after homogenization and centrifugation of the homogenates. Results revealed that some main digestive enzymes in the larval midgut were adversely affected when exposed to the food‐incorporated essential oil. Proteinase extracted from larval midgut hydrolyzed the synthetic substrates B‐Arg‐pNA, Z‐Arg‐Arg‐PNA and Z‐Phe‐Arg‐PNA for trypsin, cathepsin B and cathepsin L activities, respectively, in control and treated larvae. The essential oil caused a reduction of 61.5% in tryptic activity. Significant 69% and 79% reductions were also observed in cathepsin L and B activities, respectively. Carbohydrase activities of α‐amylase, α‐glucosidase and β‐glucosidase were detected in larval midgut extract. All assayed carbohydrases were affected by the essential oil. The most notable impact, a 93% reduction, was observed in α‐amylase. Decreases of 69.5% and 42% were obtained in α‐glucosidase and β‐glucosidase activity, respectively. This study indicated that the larvicidal effect of the essential oil from Teucrium polium may be due to its detrimental effects on digestive enzymes. It seems that the detrimental effect of the oil can be due to both the inhibitory nature of the oil and the destruction of the midgut epithelium.
Inheritance of resistance and cross resistance pattern in indoxacarb‐resistant diamondback moth Plutella xylostella L.
Authors: NEHARE Sarita , GHODKI Basweshwar S. , LANDE Gajanan K. , PAWADE Vrushali , THAKARE Atul S. 
Published: January 2010

AbstractLeaf‐dip assay of Plutella xylostella against indoxacarb showed that the concentration that produced 50% mortality (LC50) of indoxacarb ranged from 20.1 to 11.9 ppm, with highest in Nasik and lowest levels in Coimbatore strains. In selection studies, the LC50 of indoxacarb was 18.5 ppm at generation 1 (G1), which increased to 31.3‐fold (167.8 ppm) resistance after ten exposed generations (G10) as compared to unexposed. The LC50 of quinalphos was 74.4 ppm, which increased to 10.0‐fold (631.5 ppm) resistance after G10. The LC50 of cypermethrin resistant strain resulted in an 11.5‐fold increase in resistance after G10. In P. xylostella, heritability (h2) after ten generations of selection was estimated at 0.4. The number of generations required for tenfold increase in LC50 (1/R) were 6.7. The response to indoxacarb selection in P. xylostella was 0.2 and the selection differential was estimated as 0.4. The phenotypic standard deviation was 0.2. Reciprocal crosses between indoxacarb‐resistant and susceptible strains showed that the inheritance of indoxacarb resistance was autosomal. The degree of heritability (DLC) (0.4, 0.4) indicated incomplete recessive inheritance of indoxacarb resistance.
The Interpretive Dynamics of Filial and Collective Responsibility for Elderly People
Authors: FUNK LAURA 
Published: January 2010

À partir de comptes rendus de 28 enfants adultes, l'auteure étudie la dynamique interprétative de la responsabilité sociale et filiale envers les personnes âgées. Dans leurs propos sur leur responsabilité filiale, les participants avaient tendance à qualifier de positives les motivations individualistes et spontanées tandis qu'en parlant des autres Canadiens ils critiquaient les valeurs individualistes comme faisant la promotion de l'irresponsabilité. D'autres personnes ont étéévaluées négativement en contraste à un passé et à des cultures non occidentales idéalisées : la « société canadienne » a été utilisée comme opposition à celle qui définit la personne comme filialement responsable. Dans ce processus, les participants ont également reproduit l'opposition conceptuelle entre la responsabilité sociétale et la responsabilité filiale; le paradigme alternatif de la « solidarité» a été utilisé plus rarement.Drawing on accounts from 28 adult children, I explore the interpretive dynamics of filial and social responsibility for elderly people. Participants tended to characterize individualistic, voluntary motivations positively in talk about personal filial responsibility, yet when speaking about other Canadians, criticized individualistic values as promoting irresponsibility. Others were assessed negatively in contrast to an idealized past and non‐Western cultures; “Canadian society” was used as a contrast against which to define self as filially responsible. In this process, participants also reproduced conceptual opposition between filial and societal responsibility; rarer was an alternative, “solidarity” paradigm utilized.
In Conversation with the American Sociological Association President: Randall Collins on Emotions, Violence, and Interactionist Sociology
Authors: WALBY KEVIN , SPENCER DALE 
Published: January 2010

Randall Collins est professeur de sociologie à l'University of Pennsylvania et Président de l'American Sociological Association. Dans cette entrevue, R. Collins parle de la sociologie des émotions, de la tradition interactionniste ainsi que de la violence. L'entrevue permet de situer les contributions de Collins dans le développement contemporain de la sociologie critique et la microsociologie interactionniste.Randall Collins is Professor of Sociology at the University of Pennsylvania and is the President of the American Sociological Association. In the following interview, Collins discusses the sociology of emotions, the interactionist tradition, and violence. The discussion situates Collins' contributions as part of an intellectual trajectory that incorporates elements of critical sociology and the micro‐sociology of interaction.
Zoned chondrules in Semarkona: Evidence for high‐ and low‐temperature processing
Authors: Grossman Jeffrey N. , Alexanders Conel M. O'D. , Wang Jianhua , Brearley Adrian J. 
Published: January 2010

Abstract— At least 15% of the low‐FeO chondrules in Semarkona (LL3.0) have mesostases that are concentrically zoned in Na, with enrichments near the outer margins. We have studied zoned chondrules using electron microprobe methods (x‐ray mapping plus quantitative analysis), ion microprobe analysis for trace elements and hydrogen isotopes, cathodoluminescence imaging, and transmission electron microscopy in order to determine what these objects can tell us about the environment in which chondrules formed and evolved.Mesostases in these chondrules are strongly zoned in all moderately volatile elements and H (interpreted as water). Calcium is depleted in areas of volatile enrichment. Titanium and Cr generally decrease toward the chondrule surfaces, whereas Al and Si may either increase or decrease, generally in opposite directions to one another; Mn follows Na in some chondrules but not in others; Fe and Mg are unzoned. D/H ratios increase in the water‐rich areas of zoned chondrules. Mesostasis shows cathodoluminescence zoning in most zoned chondrules, with the brightest yellow color near the outside. Mesostasis in zoned chondrules appears to be glassy, with no evidence for devitrification.Systematic variations in zoning patterns among pyroxene‐ and olivine‐rich chondrules may indicate that fractionation of low‐ and high‐Ca pyroxene played some role in Ti, Cr, Mn, Si, Al, and some Ca zoning. But direct condensation of elements into hot chondrules, secondary melting of late condensates into the outer portions of chondrules, and subsolidus diffusion of elements into warm chondrules cannot account for the sub‐parallel zoning profiles of many elements, the presence of H2O, or elemental abundance patterns.Zoning of moderately volatile elements and Ca may have been produced by hydration of chondrule glass without devitrification during aqueous alteration on the parent asteroid. This could have induced structural changes in the glass allowing rapid diffusion and exchange of elements between altered glass and surrounding matrix and rim material. Calcium was mainly lost during this process, and other nonvolatile elements may have been mobile as well. Some unzoned, low‐FeO chondrules appear to have fully altered mesostasis.
Impact processing of chondritic planetesimals: Siderophile and volatile element fractionation in the Chico L chondrite
Authors: Norman Marc D. , Mittlefehldt David W. 
Published: January 2010

Abstract— A large impact event 500 Ma ago shocked and melted portions of the L‐chondrite parent body. Chico is an impact melt breccia produced by this event. Sawn surfaces of this 105 kg meteorite reveal a dike of fine‐grained, clast‐poor impact melt cutting shocked host chondrite. Coarse (1–2 cm diameter) globules of FeNi metal + sulfide are concentrated along the axis of the dike from metal‐poor regions toward the margins. Refractory lithophile element abundance patterns in the melt rock are parallel to average L chondrites, demonstrating near‐total fusion of the L‐chondrite target by the impact and negligible crystal‐liquid fractionation during emplacement and cooling of the dike.Significant geochemical effects of the impact melting event include fractionation of siderophile and chalcophile elements with increasing metal‐silicate heterogeneity, and mobilization of moderately to highly volatile elements. Siderophile and chalcophile elements ratios such as Ni/Co, Cu/Ga, and Ir/Au vary systematically with decreasing metal content of the melt. Surprisingly small (˜102) effective metal/silicate‐melt distribution coefficients for highly siderophile elements probably reflect inefficient segregation of metal despite the large degrees of melting. Moderately volatile lithophile elements such K and Rb were mobilized and heterogeneously distributed in the L‐chondrite impact breccias whereas highly volatile elements such as Cs and Pb were profoundly depleted in the region of the parent body sampled by Chico. Volatile element variations in Chico and other L chondrites are more consistent with a mechanism related to impact heating rather than condensation from a solar nebula. Impact processing can significantly alter the primary distributions of siderophile and volatile elements in chondritic planetesimals.
Petrology and geochemistry of D'Orbigny, geochemistry of Sahara 99555, and the origin of angrites
Authors: Mittlefehldt David W. , Killgore Marvin , Lee Michael T. 
Published: January 2010

Abstract— We have done a detailed petrologic study of the angrite, D'Orbigny, and geochemical study of it and Sahara 99555. D'Orbigny is an igneous‐textured rock composed of Ca‐rich olivine, Al‐Ti‐diopside‐hedenbergite, subcalcic kirschsteinite, two generations of hercynitic spinel and anorthite, with the mesostasis phases ulvöspinel, Ca‐phosphate, a silico‐phosphate phase and Fe‐sulfide. We report an unknown Fe‐Ca‐Al‐Ti‐silicate phase in the mesostasis not previously found in angrites. One hercynitic spinel is a large, rounded homogeneous grain of a different composition than the euhedral and zoned grains. We believe the former is a xenocryst, the first such described from angrites. The mafic phases are highly zoned; mg# of cores for olivine are ˜64, and for clinopyroxene ˜58, and both are zoned to Mg‐free rims. The Ca content of olivine increases with decreasing mg#, until olivine with ˜20 mol% Ca is overgrown by subcalcic kirschsteinite with about 30–35 mol% Ca. Detailed zoning sequences in olivine‐subcalcic kirschsteinite and clinopyroxene show slight compositional reversals. There is no mineralogic control that can explain these reversals, and we believe they were likely caused by local additions of more primitive melt during crystallization of D'Orbigny.D'Orbigny is the most ferroan angrite with a bulk rock mg# of 32. Compositionally, it is virtually identical to Sahara 99555; they are the first set of compositionally identical angrites. Comparison with the other angrites shows that there is no simple petrogenetic sequence, partial melting with or without fractional crystallization, that can explain the angrite suite. Angra dos Reis remains an anomalous angrite.Angrites show no evidence for the brecciation, shock, impact metamorphism, or thermal metamorphism that affected the howardite, eucrite, diogenite (HED) suite and ordinary chondrites. This suggests that the angrite parent body may have followed a fundamentally different evolutionary path than did these other parent bodies.
Northwest Africa 032: Product of lunar volcanism
Authors: Fagan T. J. , Taylor G. J. , Keil K. , Bunch T. E. , Wittke J. H. , Korotev R. L. , Jolliff B. L. , Gillis J. J. , Haskin L. A. , Jarosewich E. , Clayton R. N. , Mayeda T. K. , Fernandes V. A. , Burgess R. , Turner G. , Eugster O. , Lorenzetti S. 
Published: January 2010

Abstract— Mineralogy, major element compositions of minerals, and elemental and oxygen isotopic compositions of the whole rock attest to a lunar origin of the meteorite Northwest Africa (NWA) 032, an unbrecciated basalt found in October 1999. The rock consists predominantly of olivine, pyroxene and chromite phenocrysts, set in a crystalline groundmass of feldspar, pyroxene, ilmenite, troilite and trace metal. Whole‐rock shock veins comprise a minor, but ubiquitous portion of the rock. Undulatory to mosaic extinction in olivine and pyroxene phenocrysts and micro‐faults in groundmass and phenocrysts also are attributed to shock.Several geochemical signatures taken together indicate unambiguously that NWA 032 originated from the Moon. The most diagnostic criteria include whole‐rock oxygen isotopic composition and ratios of Fe/Mn in the whole rock, olivine, and pyroxene. A lunar origin is documented further by the presence of Fe‐metal, troilite, and ilmenite; zoning to extremely Fe‐rich compositions in pyroxene; the ferrous oxidation state of all Fe in pyroxene; and the rare earth element (REE) pattern with a well‐defined negative europium anomaly. This rock is similar in major element chemistry to basalts from Apollo 12 and 15, but is enriched in light REE and has an unusually high Th/Sm ratio. Some Apollo 14 basalts yield a closer match to NWA 032 in REE patterns, but have higher concentrations of Al2O3. Ar‐Ar step release results are complex, but yield a whole‐rock age of ˜2.8 Ga, suggesting that NWA 032 was extruded at 2.8 Ga or earlier. This rock may be the youngest sample of mare basalt collected to date. Noble gas concentrations combined with previously collected radionuclide data indicate that the meteorite exposure history is distinct from currently recognized lunar meteorites. In short, the geochemical and petrographic features of NWA 032 are not matched by Apollo or Luna samples, nor by previously identified lunar meteorites, indicating that it originates from a previously unsampled mare deposit.Detailed assessment of petrographic features, olivine zoning, and thermodynamic modelling indicate a relatively simple cooling and crystallization history for NWA 032. Chromite‐spinel, olivine, and pyroxene crystallized as phenocrysts while the magma cooled no faster than 2 °C/h based on the polyhedral morphology of olivine. Comparison of olivine size with crystal growth rates and preserved Fe‐Mg diffusion profiles in olivine phenocrysts suggest that olivine was immersed in the melt for no more than 40 days. Plumose textures in groundmass pyroxene, feldspar, and ilmenite, and Fe‐rich rims on the phenocrysts formed during rapid crystallization (cooling rates ˜20 to 60 °C/h) after eruption.
Space shuttle observations of terrestrial impact structures using SIR‐C and X‐SAR radars
Authors: Mchone John F. , Greeley Ronald , Williams Kevin K. , Blumberg Dan G. , Kuzmin Ruslan O. 
Published: January 2010

Abstract— Ten terrestrial impact structures were imaged during two flights of the 1994 space radar laboratory (SRL) experiment. These craters include Wolf Creek, Australia; Roter Kamm, Namibia; Zhamanshin, Kazakhstan; BP and Oasis, Libya; Aorounga, Chad; Amguid, Algeria; and Spider, Connolly Basin and Henbury, Australia. SRL contained two co‐registered instruments; the United States shuttle imaging radar‐C (SIR‐C) polarimetric radar system operating in L‐band (λ = 24 cm) and C‐band (λ = 5.6 cm), and the joint German/Italian synthetic aperture radar (X‐SAR) operating in vertically‐polarized X‐band (λ = 3 cm).Comparisons show SRL images to be complementary to, or in some cases superior to, corresponding optical images for evaluating size, location, and relative age of impact features. Regardless of wavelength or polarization, craters with significant relief appear prominently on radar as a result of slope and roughness effects. In desert regions, longer wavelengths penetrate dry sand mantles to reveal hidden crater dimensions or associated buried landforms. Radar polarities and wavelengths are particularly sensitive to vegetation, surface roughness, and soil moisture or electrical properties. In the more temperate environments of Kazakhstan and Australia, SRL images show detailed stream patterns that reveal the location and structure of otherwise obscured impact features.
Geochemistry of the ungrouped carbonaceous chondrite Tagish Lake, the anomalous CM chondrite Bells, and comparison with CI and CM chondrites
Authors: Mittlefehldt David W. 
Published: January 2010

Abstract— I have determined the composition via instrumental neutron activation analysis of a bulk pristine sample of the Tagish Lake carbonaceous chondrite fall, along with bulk samples of the CI chondrite Orgueil and of several CM chondrites. Tagish Lake has a mean of refractory lithophile element/Cr ratios like those of CM chondrites, and distinctly higher than the CI chondrite mean. Tagish Lake exhibits abundances of the moderately volatile lithophile elements Na and K that are slightly higher than those of mean CM chondrites. Refractory through moderately volatile siderophile element abundances in Tagish Lake are like those of CM chondrites. Tagish Lake is distinct from CM chondrites in abundances of the most volatile elements. Mean CI‐normalized Se/Co, Zn/Co and Cs/Co for Tagish Lake are 0.68 ± 0.01, 0.71 ± 0.07 and 0.76 ± 0.02, while for all available CM chondrite determinations, these ratios lie between 0.31 and 0.61, between 0.32 and 0.58, and between 0.39 and 0.74, respectively. Considering petrography, and oxygen isotopic and elemental compositions, Tagish Lake is an ungrouped member of the carbonaceous chondrite clan. The overall abundance pattern is similar to those of CM chondrites, indicating that Tagish Lake and CMs experienced very similar nebular fractionations.Bells is a CM chondrite with unusual petrologic characteristics. Bells has a mean CI‐normalized refractory lithophile element/Cr ratio of 0.96, lower than for any other CM chondrite, but shows CI‐normalized moderately volatile lithophile element/Cr ratios within the ranges of other CM chondrites, except for Na which is low. Iridium, Co, Ni and Fe abundances are like those of CM chondrites, but the moderately volatile siderophile elements, Au, As and Sb, have abundances below the ranges for CM chondrites. Abundances of the moderately volatile elements Se and Zn of Bells are within the CM ranges. Bells is best classified as an anomalous CM chondrite.
Mineralogy of Tagish Lake: An ungrouped type 2 carbonaceous chondrite
Authors: Zolensky M. E. , Nakamura K. , Gounelle M. , Mikouchi T. , Kasama T. , Tachikawa O. , Tonui E. 
Published: January 2010

Abstract— In this paper we describe the recovery, handling and preliminary mineralogical investigation of the Tagish Lake meteorite. Tagish Lake is a type 2 carbonaceous chondrite which bears similarities to CI1 and CM chondrite groups, but is distinct from both. Abundant phyllosilicates as well as chondrules (however sparse) and common olivine grains in the matrix preclude any other classification. The bulk density of Tagish Lake (1.67 g/cc) is far lower than CI or CM chondrites (2.2‐2.3 and 2.6‐2.9 g/cc, respectively), or any other meteorite for that matter. We have identified two lithologies: a dominant carbonate‐poor lithology and a less‐abundant carbonate‐rich lithology. The meteorite is a breccia at all scales.We have noted similarities between Tagish Lake and some clasts within the enigmatic meteorite Kaidun; possibly there are genetic relationships here worth exploring. In the paper we describe a clast of CM1 material within Tagish Lake which is very similar to a major lithology in Kaidun.
Measuring the plasma environment at Mercury: The fast imaging plasma spectrometer
Authors: KOEHN P. L. , ZURBUCHEN T. H. , GLOECKLER G. , LUNDGREN R. A. , FISK L. A. 
Published: January 2010

Abstract—The plasma environment at Mercury is a rich laboratory for studying the interaction of the solar wind with a planet. Three primary populations of ions exist at Mercury: solar wind, magnetospheric, and pickup ions. These pickup ions are generated through the ionization of Mercury's exosphere or are sputtered particles from the Mercury surface. A comprehensive mission to Mercury, such as MESSENGER (MErcury: Surface, Space ENvironment, GEochemistry, Ranging), should include a sensor that is able to determine the dynamical properties and composition of all these plasma components. An instrument to measure the composition of these ion populations and their three‐dimensional velocity distribution functions must be lightweight, fast, and have a very large field of view.The fast imaging plasma spectrometer (FIPS) is an imaging mass spectrometer, part of NASA's MESSENGER mission, the first Mercury orbiter. This versatile instrument has a very small footprint, and has a mass that is ˜1 order of magnitude less than other comparable systems. It maintains a nearly full‐hemisphere field of view, suitable for either spinning or three‐axis‐stabilized platforms. The major piece of innovation to enable this sensor is a new deflection system geometry that enables a large instantaneous (˜1.5π) field of view. This novel electrostatic analyzer system is then combined with a position sensitive time‐of‐flight system. We discuss the design and prototype tests of the FIPS deflection system and show how this system is expected to address one key problem in Mercury science, that of the nature of the radar‐bright regions at the Hermean poles.