A study of subpulse phase correlation across nulls in PSR B0031−07

The correlation of subpulse phases across nulls is investigated in the radio pulsar PSR B0031−07, using 29 849 periods of high-quality data obtained with the Ooty Radio Telescope (ORT) which operates at 327 MHz. Assuming that the turn-off and turn-on subpulse phases (the phase of the subpulse in the last period before the null and that in the first period after the null, respectively) are independent random variables, the expected distribution of their difference (i.e. the total drift) is inconsistent with the observed distribution for null transitions within the same drift mode; this implies a correlation of subpulse phase across nulls. However, this correlation decreases with null duration for both the dominant drift modes. Substantial drifting occurs during short nulls (one to four periods); the drift rate during the short nulls appears to be constant for a class A transition, whereas it decreases with null duration for class B transitions. These results, together with the reported behaviour of PSR B1944+17 and PSR B0809+74, seem to imply different time-scales for phase correlation in different pulsars.     

基于PSR模型的珊瑚礁生态系统健康评价指标体系的构建与应用

运用压力-状态-响应（pressure-state-response,PSR）模型,采用生态系统健康理论评价珊瑚礁生态状况.借鉴国内外现有生态系统评价方法,结合珊瑚礁生态系统的特点,建立适合我国国情的珊瑚礁生态系统评价方法和模式,并对我国典型海域珊瑚礁生态健康状况进行评价,以期为我国典型珊瑚礁生态系统健康状况提供基础资料.评价结果显示东山、涠洲岛、海南东部珊瑚礁生态健康状况为健康,徐闻和西沙海域珊瑚礁生态健康状况为亚健康,评价结果与我国相关生态监控区调查结果基本一致.     

山东半岛近岸海域生态系统健康综合评价

为了构建基于多指标体系的生态系统健康评价方法,作者在调研了大量国内外文献的基础上,通过实证研究和量化分析,对山东半岛近岸海域生态系统健康的现状做出了较为客观的评价。在综合考虑影响海洋生态系统健康的各种因素的基础上,构建了山东半岛近岸海域生态系统健康评价指标体系,从陆源压力、水质状态和生物响应3个方面对山东半岛近岸海域生态系统健康和环境压力进行分析。结果显示:2006年山东半岛近岸海域生态健康状况基本呈现由外海到近岸逐渐变差的态势,其中生态健康状况较差的海域主要集中在莱州湾西南部、烟台北部海域、威海的沿岸海域以及山东半岛东南部海域。     

采煤塌陷区土地质量评价指标体系探讨——以徐州矿区为例

简要回顾采煤塌陷区土地质量研究状况,根据科学性、代表性、可行性、敏感性的原则,以徐州市采煤塌陷区为研究对象,运用PSR概念模型,尝试给出针对具体采煤塌陷区的土地质量评价指标体系。体系共分为3层23个指标,较全面的涵盖了社会经济、物理化学、政策法规等不同范畴。     

New radial velocities for 30 candidate runaway stars and a possible binary supernova origin for HIP 9470 and PSR J0152–1637

We report new radial velocity measurements for 30 candidate runaway stars. We revise their age estimates and compute their past trajectories in the Galaxy in order to determine their birthplaces. We find that seven of the stars could be younger than ∼100 Myr, and for five of them we identify multiple young clusters and associations in which they may have formed. For the youngest star in the sample, HIP 9470, we suggest a possible ejection scenario in a supernova event, and also that it may be associated with the young pulsar PSR J0152–1637. Our spectroscopic observations reveal seven of the stars in the sample of 30 to be previously unknown spectroscopic binaries. Orbital solutions for four of them are reported here as well. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Preliminary limits of a logarithmic correction to the Newtonian gravitational potential in binary pulsars

We obtain preliminary limits on a logarithmic correction to the Newtonian gravitational potential by using five binary pulsars:PSR J0737-3039,PSR B1534+12,PSR J1756-2251,PSR B1913+16 and PSR B2127+11C.This kind of correction may originate from fundamental frameworks,like string theories,effective models of gravity due to quantum effects and the non-local gravity scheme.We estimate the upper limit of the Tohline-Kuhn-Kruglyak parameter λ and the lower limit of the FabrisCampos parameter a,which parameterize the correction and are connected to each other by αλ=—1.By analyzing the advances of periastron of these binary pulsars,we find that the preliminary upper limit of α is 0.19±0.14 kpc~(-1) and the preliminary lower limit of λ is-5.2±3.8 kpc.They are compatible with the bounds based on dynamics of spiral galaxies but quite different from those given by solar system dynamics.These results indicate that this logarithmic correction might be more observable in current timings of binary pulsars than in motions of the solar system.     

An Observational Study of the Strong Single Pulses of PSR J0034-0721

Using the 25m radio telescope of the Urumqi Observatory, the strong single pulses of the pulsar PSR J0034-0721 were observed at 1.54 GHz on 6th Aug. 2007. With the technique of single-pulse detection, 116 single pulses with the signal-to-noise ratios of R_SN≥5 were detected from the observed data of 1 h. At 1.54 GHz, the signal-to-noise ratios of the detected single pulses are in the range from 5 to 10.5, and the peak flux densities of these pulses are approximately 14∼29 times that of the average pulse (AP), much less than the ratios between the intensities of typical giant pulses and the intensity of AP. The cumulative distribution of the intensities of these pulses is basically a powerlaw distribution with the spectral index α = −4.3 ± 0.4. The detection rates for the pulses of R_SN≥5 and R_SN≥10 are 3% and 0.08%, respectively. For these pulses, the half-peak width W₅₀ ranges from 1.6 ms to 8 ms, 3.9 ms in average. The phases of the vast majority of the strong single pulses are concentrated around the peak position of AP, but 2 strong pulses of R_SN≥8.5 are detected at the phases about 33 ms earlier than the phase of the AP peak. This implies that there probably exist two emission regions of strong pulses, and this is consistent with the previously observed results at 40 MHz and 111 MHz, except that at 1.54 GHz the profile of AP exhibits only one component.