On the distributions of pulsar glitch sizes and the inter-glitch time intervals     

Innocent Okwudili Eya  Johnson Ozoemene Urama  Augustine Ejikeme Chukwude 《天文和天体物理学研究(英文版)》2019,(6)

The glitch size, △ν/ν, inter-glitch time interval, ti, and frequency of glitches in pulsars are key parameters in discussing glitch phenomena. In this paper, the glitch sizes and inter-glitch time intervals are statistically analyzed in a sample of 168 pulsars with a total of 483 glitches. The glitches are broadly divided into two groups. Those with △ν/ν 10~(-7) are regarded as small size glitches, while those with△ν/ν≥ 10~(-7) are considered as relatively large size glitches. In the ensemble of glitches, the distribution of△ν/ν is seen to be bimodal as usual. The distribution of inter-glitch time intervals is unimodal and the interglitch time intervals between small and large size glitches are not significantly different from each other.This observation shows that inter-glitch time intervals are size independent. In addition, the distribution of the ratio △ν/ν : tiin both small and large size glitches has the same pattern. This observation suggests that a parameter which depends on time, which could be the spin-down rate of a pulsar, plays a similar role in the processes that regulate both small and large size glitches. Equally, this could be an indication that a single physical mechanism, which could produce varying glitch sizes at similar time-intervals, could be responsible for both classes of glitch sizes.  相似文献   

Atmospheric control of the cooling rate of impact melts and cryolavas on Titan’s surface     

Ashley Gerard Davies  Christophe Sotin  Dennis L. Matson  Julie Castillo-Rogez  Torrence V. Johnson  Mathieu Choukroun  Kevin H. Baines 《Icarus》2010,208(2):887-895

As on Earth, Titan’s atmosphere plays a major role in the cooling of heated surfaces. We have assessed the mechanisms by which Titan’s atmosphere, dominantly N₂ at a surface pressure of 1.5 × 10⁵ Pa, cools a warm or heated surface. These heated areas can be caused by impacts generating melt sheets and (possibly) by endogenic processes emplacing cryolavas (a low-temperature liquid that freezes on the surface). We find that for a cooling cryolava flow, lava lake, or impact melt body, heat loss is mainly driven by atmospheric convection. Radiative heat loss, a dominant heat loss mechanism with terrestrial silicate lava flows, plays only a minor role on Titan. Long-term cooling and solidification are dependent on melt sheet or flow thickness, and also local climate, because persistent winds will speed cooling. Relatively rapid cooling caused by winds reduces the detectability of these thermal events by instruments measuring surface thermal emission. Because surface temperature drops by ≈50% within ≈1 day of emplacement, fresh flows or impact melt may be difficult to detect via thermal emission unless an active eruption is directly observed. Cooling of flow or impact melt surfaces are orders of magnitude faster on Titan than on airless moons (e.g., Enceladus or Europa).Although upper surfaces cool fast, the internal cooling and solidification process is relatively slow. Cryolava flow lengths are, therefore, more likely to be volume (effusion) limited, rather than cooling-limited. More detailed modeling awaits constraints on the thermophysical properties of the likely cryomagmas and surface materials.  相似文献   

Edge adapted wavelets,solar magnetic activity,and climate change     

R. W. Johnson 《Astrophysics and Space Science》2010,326(2):181-189

The continuous wavelet transform is adapted to account for signal truncation through renormalization and by modifying the shape of the analyzing window. Comparison is made of the instant, integrated, and mean wavelet power with previous algorithms. The edge adapted and renormalized admissible wavelet transforms are used to estimate the level of solar magnetic activity from the sunspot record. The solar activity is compared to Oerlemans’ temperature reconstruction and to the Central England Temperature record. A correlation is seen for years between 1610 and 1990, followed by a strong deviation as the recently observed temperature increases.  相似文献   

Metal-catalyzed degradation and racemization of amino acids in iron sulfate brines under simulated martian surface conditions     

Adam P. Johnson  Lisa M. Pratt 《Icarus》2010,207(1):124-603

Recent lines of evidence indicate that Mars may have been substantially warmer and wetter, raising questions about whether the planet’s surface was once more conducive to the possibility of life. To better constrain the extent of preservation of ancient amino acid biosignatures, the effects of metal ions and UV radiation were investigated with respect to the rates of diagenesis of amino acids in metal-rich sulfate brines. Individual experimental results indicate that the oxidation rates of amino acids loosely followed trends characteristic of a radiolytic oxidation mechanism that is dependent on variations in side-chain constituents. Relative rates of racemization only show a limited dependence on the presence of metals; overall, rates of racemization in the presence of metals in solution are an order of magnitude slower than oxidation and both are several orders of magnitude faster than previously reported. This increase in rate constant is indicative of an extremely efficient catalytic enhancement of this destructive diagenetic pathway. These findings imply that chiral life-detection strategies should focus on specific geochemical environments that exhibit relatively slow rates of both degradation and racemization. Episodic liquid water during periods of increased water activity on the martian surface may have significant implications for the oxidation of organic matter through secondary diagenetic reactions and may act as a leveling mechanism for organic compounds.  相似文献   

Impact of modulation on CMB B-mode polarization experiments     

Michael L. Brown  Anthony Challinor  Chris E. North †  Bradley R. Johnson ‡  Daniel O'Dea  David Sutton 《Monthly notices of the Royal Astronomical Society》2009,397(2):634-656

  相似文献   

A large-scale survey of X-ray filaments in the Galactic Centre     

S. P. Johnson  H. Dong  Q. D. Wang 《Monthly notices of the Royal Astronomical Society》2009,399(3):1429-1440

We present a catalogue of 17 filamentary X-ray features located within a  68 × 34  arcmin²  view centred on the Galactic Centre region from images taken by Chandra . These features are described by their morphological and spectral properties. Many of the X-ray features have non-thermal spectra that are well fitted by an absorbed power law. Of the 17 features, we find six that have not been previously detected, four of which are outside the immediate  20 × 20  arcmin²  area centred on the Galactic Centre. Seven of the 17 identified filaments have morphological and spectral properties expected for pulsar wind nebulae (PWNe) with X-ray luminosities of  5 × 10³²  to 10³⁴ erg s⁻¹ in the 2.0–10.0 keV band and photon indices in the range of  Γ= 1.1  to 1.9. In one feature, we suggest the strong neutral Fe Kα emission line to be a possible indicator for past activity of Sgr A*. For G359.942−0.03, a particular filament of interest, we propose the model of a ram pressure confined stellar wind bubble from a massive star to account for the morphology, spectral shape and 6.7 keV He-like Fe emission detected. We also present a piecewise spectral analysis on two features of interest, G0.13−0.11 and G359.89−0.08, to further examine their physical interpretations. This analysis favours the PWN scenario for these features.  相似文献   

The geographic distribution of metals in urban soils: the case of Syracuse,NY     

D. A. Griffith  D. L. Johnson  A. Hunt 《GeoJournal》2009,74(4):275-291

A paucity of literature currently exists pertaining to the high-resolution geographic distribution of metal contaminants across urban areas. Thousands of soil samples were collected across Syracuse, NY to secure empirical evidence about such geographic distributions. Metal measurements were made with XRF technology, with quality assessments based upon replicate samples as well as ICP technology summarized here. Both metal covariations and their spatial structure are described, followed by mapping of selected metal measurements based upon sample points, as well as census block group and census tract aggregates. A simple comparison is presented between certain of these empirical results and a selected non-urban landscape (a river floodplain). Finally, implications drawn from the empirical evidence presented include covariation assessments with selected census data that serve as surrogates for poverty.  相似文献   

Estimating selenium removal by sedimentation from the Great Salt Lake,Utah     

Wade Oliver  Christopher Fuller  David L. Naftz  William P. Johnson  Ximena Diaz 《Applied Geochemistry》2009

The mass of Se deposited annually to sediment in the Great Salt Lake (GSL) was estimated to determine the significance of sedimentation as a permanent Se removal mechanism. Lake sediment cores were used to qualitatively delineate sedimentation regions (very high to very low), estimate mass accumulation rates (MARs) and determine sediment Se concentrations. Sedimentation regions were defined by comparison of isopach contours of Holocene sediment thicknesses to linear sedimentation rates determined via analysis of ²¹⁰Pb, ²²⁶Ra, ⁷Be and ¹³⁷Cs activity in 20 short cores (<5 cm), yielding quantifiable results in 13 cores. MARs were developed via analysis of the same radioisotopes in eight long cores (>10 cm). These MARs in the upper 1–2 cm of each long core ranged from 0.019 to 0.105 g_sed/cm²/a. Surface sediment Se concentrations in the upper 1 or 2 cm of each long core ranged from 0.79 to 2.47 mg/kg. Representative MARs and Se concentrations were used to develop mean annual Se removal by sedimentation in the corresponding sedimentation region. The spatially integrated Se sedimentation rate was estimated to be 624 kg/a within a range of uncertainty between 285 and 960 kg/a. Comparison to annual Se loading and other potential removal processes suggests burial by sedimentation is not the primary removal process for Se from the GSL.  相似文献   

中国黄土高原西缘甘肃万象洞MIS 5石笋δ¹⁸ O记录与南方地区石笋记录的对比研究^*          下载免费PDF全文

安春雷  张平中  代志波  张德忠  杨勋林 《第四纪研究》2006,26(6):985-990

位于青藏高原与黄土高原过渡带的甘肃武都万象洞石笋WXSM51和WXSM52提供了MIS 5(118~79kaB.P.)高分辨率的δ¹⁸ O记录。研究表明, 万象洞石笋δ¹⁸ O值与夏季风强度呈负相关关系, 与我国西南部的贵州董歌洞石笋δ¹⁸ O记录有良好的对应关系, 并与高纬度的格陵兰NGRIP冰芯δ¹⁸ O记录和65°N太阳辐射强度有很好的一致性, 说明万象洞石笋δ¹⁸ O记录了118~79kaB.P.期间亚洲季风强度的变化, 同时也说明东亚季风强度的变化和全球气候变化同步, 而且主要受控于北半球太阳辐射强度的变化。同时它与地中海碳酸盐记录有很好的相似性, 和巴西石笋δ¹⁸ O记录在千年尺度上表现出相反的变化趋势, 说明东亚季风区、地中海地区以及巴西季风区之间存在密切的联系, 指示了南北半球气候在千年尺度上存在"跷跷板"(seesaw)现象。万象洞石笋δ¹⁸ O记录的MIS 5b与MIS 5a突发性转换, 与NGRIP冰芯δ¹⁸ O记录相似, 而与神农架记录存在差异, 说明万象洞地区对亚洲季风强度的响应更为敏感。  相似文献   

Change of collision efficiency with distance in bacterial transport experiments     

Dong H  Scheibe TD  Johnson WP  Monkman CM  Fuller ME 《Ground water》2006,44(3):415-429

Understanding the mechanisms of bacterial transport in aquifers is important in developing bioremediation strategies. Collision efficiency (alpha) is one important parameter used in modeling bacterial transport. This study was undertaken to measure change in alpha with distance by performing a bacterial transport experiment in Oyster, Virginia. Following injection of a bacterium, Comamonas sp., into a well, water samples were collected at various distances along the flowpath and injected into columns packed with homogenized South Oyster focus area sediment. Zeta potentials of the bacteria in the samples were measured. Values of alpha were determined at various locations in the field in two ways: based on field breakthrough concentrations at the sampling points and based on column breakthrough concentrations. The alpha values estimated from field breakthrough decreased with distance, whereas those estimated from column breakthrough increased with distance. Bacterial cell surface charge became progressively more negative with distance in the field. We hypothesize that the apparent contradiction between field and column alpha values was caused by differences in the flow of the two systems. Flow in the columns was forced to occur through fine-grained zones of iron and aluminum hydroxide coatings that selectively removed the most negatively charged bacteria. In contrast, in the field, the injected cells did not come into contact with the positively charged coatings because the bulk solution bypassed them due to heterogeneous hydraulic properties. These results suggest that laboratory-based models may underestimate bacterial transport distance in the field. A more realistic approach may be necessary to capture the degree of heterogeneity.  相似文献