新疆和田地区耕地面源污染生态风险评价          下载免费PDF全文

田丰收  刘新平  原伟鹏 《干旱区地理》2019,42(2):295-304

随着化肥、农膜等在农业生产中的过量投入，耕地面源污染的程度随之加重。文章选取塔里木河流域上游和田地区为研究区域，依据P-S-R框架理论，构建和田地区耕地面源污染生态风险评价指标体系，加入土壤理化数据，使用生态风险评价模型对和田地区1980 年及2016 年耕地面源污染状况进行生态风险评价，运用耕地生态风险模型、生态风险转移矩阵、Arcgis分析和田地区耕地面源污染时空分异状况。研究结论如下：和田地区1980 年耕地生态风险等级均为II级或III级，呈“中间高，两侧低”分布；2016 年耕地生态风险等级上升至IV级或V级，呈“倒W型”分布，各县耕地面源污染程度较1980 年均有较大幅度的上升，其中墨玉县和于田县在2016 年耕地生态风险等级达到最高的V级，而民丰县因自身生态环境的强脆弱性，同样需要提高关注。根据面源污染“从源头治理”的原则，应切实推进和田地区耕地生态环境保护与治理，提高政府重视程度，增强技术指导，开展试点工作，改善和田地区耕地面源污染现状。  相似文献   

采煤塌陷区土地质量评价指标体系探讨——以徐州矿区为例     

魏娜  唐倩 《山东地质》2011,(3):35-37

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。  相似文献   

草地退化的地质指标体系   总被引：1，自引：0，他引：1  

王轶  李瑞敏  王祎萍  曹峰  徐为 《地质通报》2011,30(11):1744-1751

借鉴国际地质指标工作组提出的地质指标概念,从分析草地退化的各种影响因素及其对演化过程的控制作用, 以及草地生态系统退化过程中的各种响应关系入手,按照“影响-状态-后果模型”（CSR模型）和“压力-状态-响应 模型”（PSR模型）构建了草地退化地质指标体系。  相似文献   

城市水土环境变化的地质指标体系     

姚治华  王红旗 《地质通报》2011,30(11):1774-1778

随着全球城市化进程的不断加快,城市水土环境变化日益引起人们的关注。借鉴国际地质指标研究的思路,有针对性地构建了城市水土环境变化的地质指标体系。首先明确了城市水土环境的概念内涵,确定了指标体系构建的原则,在此基础上提出了融合“CSR模型”和“PSR模型”的指标体系框架,在此框架指导下构建了城市水土环境变化调查指标体系和监测指标体系,二者共同构成了城市水土环境变化地质指标体系,为城市水土环境调查、监测与管理提供了前期的技术支撑。  相似文献   

Optical spectroscopy of the radio pulsar PSR B0656+14     

S. Zharikov  R. E. Mennickent  Yu. Shibanov  V. Komarova 《Astrophysics and Space Science》2007,308(1-4):545-549

We have obtained the spectrum of a middle-aged PSR B0656+14 in the 4300–9000 Å range with the ESO/VLT/FORS2. Preliminary results show that at 4600–7000 Å the spectrum is almost featureless and flat with a spectral index α _ν ??0.2 that undergoes a change to a positive value at longer wavelengths. Combining with available multiwavelength data suggests two wide, red and blue, flux depressions whose frequency ratio is about 2 and which could be the 1st and 2nd harmonics of electron/positron cyclotron absorption formed at magnetic fields ～10⁸ G in upper magnetosphere of the pulsar.  相似文献   

INTEGRAL observations of TeV plerions     

A. I. D. Hoffmann  D. Horns  A. Santangelo 《Astrophysics and Space Science》2007,309(1-4):215-219

Amongst the sources seen in very high gamma-rays several are associated with Pulsar Wind Nebulae (“TeV plerions”). The study of hard X-ray/soft gamma-ray emission is providing an important insight into the energetic particle population present in these objects. The unpulsed emission from pulsar/pulsar wind nebula systems in the energy range accessible to the INTEGRAL satellite is mainly synchrotron emission from energetic and fast cooling electrons close to their acceleration site. Our analyses of public INTEGRAL data of known TeV plerions detected by ground based Cherenkov telescopes indicate a deeper link between these TeV plerions and INTEGRAL detected pulsar wind nebulae. The newly discovered TeV plerion in the northern wing of the Kookaburra region (G313.3+0.6 powered by the middle aged PSR J1420-6048) is found to have a previously unknown INTEGRAL counterpart which is besides the Vela pulsar the only middle aged pulsar detected with INTEGRAL. We do not find an INTEGRAL counterpart of the TeV plerion associated with the X-ray PWN “Rabbit” G313.3+0.1 which is possibly powered by a young pulsar.  相似文献   

Ultraviolet emission from young and middle-aged pulsars     

Oleg Kargaltsev  George Pavlov 《Astrophysics and Space Science》2007,308(1-4):287-296

We present the UV spectroscopy and timing of three nearby pulsars (Vela, B0656+14 and Geminga) recently observed with the Space Telescope Imaging Spectrograph. We also review the optical and X-ray properties of these pulsars and establish their connection with the UV properties. We show that the multiwavelengths properties of neutron stars (NSs) vary significantly within the sample of middle-aged pulsars. Even larger differences are found between the thermal components of Geminga and B0656+14 as compared to those of radio-quiet isolated NSs. These differences could be attributed to different properties of the NS surface layers. This work was supported by STScI grants GO-9182 and GO-9797 and NASA grant NAG5-10865.  相似文献   

HESS J1616−508: likely to be powered by PSR J1617−5055     

R. Landi  A. De Rosa  A. J. Dean  L. Bassani  P. Ubertini  A. J. Bird 《Monthly notices of the Royal Astronomical Society》2007,380(3):926-932

HESS J1616−508 is one of the brightest emitters in the TeV sky. Recent observations with the IBIS/ISGRI telescope onboard the INTEGRAL spacecraft have revealed that a young, nearby and energetic pulsar, PSR J1617−5055, is a powerful emitter of soft γ-rays in the 20–100 keV domain. In this paper, we present an analysis of all available data from the INTEGRAL , Swift , BeppoSAX and XMM–Newton telescopes with a view to assessing the most likely counterpart to the High Energy Stereoscopic System (HESS) source. We find that the energy source that fuels the X/γ-ray emissions is derived from the pulsar, both on the basis of the positional morphology, the timing evidence and the energetics of the system. Likewise the 1.2 per cent of the pulsar's spin-down energy loss needed to power the 0.1–10 TeV emission is also fully consistent with other HESS sources known to be associated with pulsars. The relative sizes of the X/γ-ray and very high energy sources are consistent with the expected lifetimes against synchrotron and Compton losses for a single source of parent electrons emitted from the pulsar. We find that no other known object in the vicinity could be reasonably considered as a plausible counterpart to the HESS source. We conclude that there is good evidence to assume that the HESS J1616−508 source is driven by PSR J1617−5055 in which a combination of synchrotron and inverse-Compton processes combine to create the observed morphology of a broad-band emitter from keV to TeV energies.  相似文献   

Historical Evidence for the Birth of the Newly Discovered Pulsar PSR J1833-1034     

Zhen-Ru Wang  Min Li  Yi Zhao Astronomy Department  Nanjing University  Nanjing  Institute of Chinese Classics  Nanjing University  Nanjing 《中国天文和天体物理学报》2006,6(5)

Stimulated by the recent discovery of PSR J1833-1034 in SNR G21.5-0.9 and its age parameters presented by two groups of discovery, we demonstrate that the PSR J1833-1034 was born 2053 years ago from a supernova explosion, the BC 48 guest star observed in the Western Han (Early Han) Dynasty by ancient Chinese. Based on a detailed analysis of the Chinese ancient record of the BC 48 guest star and the new detected physical parameters of PSR J1833-1034, agreements on the visual position, age and distance between PSR J1833-1034 and the BC 48 guest star are obtained. The initial period P0 of PSR J1833-1034 is now derived from its historical and current observed data without any other extra assumption on P0 itself, except that the factor PP is a constant in its evolution until now.  相似文献   

基于PSR模型的石化园区海洋环境影响后评估指标体系研究          下载免费PDF全文

赵素芳  袁仲杰  姚翔  王薇 《应用海洋学学报》2018,37(3):404-412

我国将建成七大国家级石化产业园区,这些石化园区无一例外的位于沿海地区或海岛上,为此加强石化园区运营期海洋环境保护意义重大.环境影响后评估是运营期检验园区环境管理水平、查找园区环境问题的重要手段之一.目前,石化园区环境影响后评估主要以环境要素逐一分析法最为常见,而将石化园区作为一个整体从资源、环境、管理等角度综合评估的方法尚不多见.本研究在阐述我国海洋环境后评估和深入分析石化园区用海特点的基础上,结合PSR框架模型加以总结,提出了石化园区海洋环境影响后评估框架与指标体系,分为框架层、方案层和指标层,共25项考核指标,以期为今后沿海石化园区海洋环境管理研究提供思路.同时,本研究明确了各类评估指标赋值和权重等计算方案,并以大连某石化园区为案例进行了评估效果验证.  相似文献