电商快递包装箱的碳足迹空间分解和隐含碳转移研究

伴随电子商务等新兴消费业态的迅猛发展,其碳排放量已不容忽视。本研究从空间分解和隐含碳转移的角度,基于对电商快递包装箱全生命周期的碳足迹研究,识别其在原料、生产、利用各环节与电商行为的地理空间耦合,分析各阶段及总排放的省域尺度格局特征,以及伴随快递流的隐含碳转移网络格局。研究发现：原料阶段的碳排放多在木材原料商区位,生产阶段的碳排放和快递发货区位高度耦合,利用阶段的碳排放和快递收货区位相耦合。全国电商快递包装箱各阶段的碳排放在空间上高度集聚,原料阶段集中在广西,生产和利用阶段集中在广东、浙江、江苏,整体呈现出“东多西少、南多北少”的空间特征。碳排放总量较高的省区多由生产驱动,碳排放总量越少的省区则利用驱动越明显。隐含碳转移网络呈现出“少数省区净流出、多数省区净流入”的“轴辐式”结构特征,浙江、广东两省承担了80%左右的净流出,是绝大多数省区隐含碳流入的最大来源地,北京是净流入最大的省区。基于隐含碳转移进行碳排放责任辨析,是相关决策需要考虑的重要因素;绿色包装的减排贡献较大,亟待寻求技术突破;新兴消费业态的碳排放值得长期关注。     

中国旅游业碳减排潜力的空间关联网络结构及其影响因素

基于2000—2018年中国省际面板数据,利用“自下而上”法和Super-SBM模型测度30个省（区、市）的旅游业碳减排潜力,借助修正的引力模型和社会网络分析方法探究其空间关联网络特征及影响因素。结果表明：①中国旅游业碳减排潜力的空间关联日趋紧密,网络密度和网络关联数呈增长态势,网络效率和网络等级度呈下降态势;②东部区域在空间关联网络中居于核心位置,对降低旅游业碳减排潜力所需要素的掌控与支配能力较强;西部区域在网络中居于边缘位置,难以影响和控制其他省（区、市）;③北京、天津、江苏和上海属于“净受益”板块,广东、浙江和福建属于“经纪人”板块,吉林、内蒙古等23省（区、市）属于“净溢出”板块;④空间邻接关系、经济发展水平差异、产业结构差异、技术创新水平差异和旅游业人数规模差异共同驱动着中国旅游业碳减排潜力空间关联网络结构的形成与演化。     

“双碳”目标下全域土地综合整治的学理研究与实践路径

全域土地综合整治作为优化乡村国土空间的重要实践活动,既是人为土地利用的重要碳源之一,也对缓解土地利用碳排放具有积极作用。为解析其与“双碳”目标的互馈机制与耦合关系,剖析其对实现“双碳”目标的贡献作用,提出全域土地综合整治碳效应的学理研究问题与实践应用路径。结果表明：① 与传统土地整治相比,全域土地综合整治具有更强的战略性、综合性和系统性,作为面向全要素全空间的土地实践活动,其价值导向和实践方式更多元,与“双碳”目标联系更密切,固碳减排可操作性更强;② 基于文献计量研究发现,面向“双碳”目标的全域土地综合整治应在碳效应影响因素解析、碳核算体系构建、空间布局优化等方面开展学理研究和关键问题探索;③ 研究提出了综合规划引领、工程建设和建后管护的实践应用路径,全域土地综合整治通过调整技术方法体系、优化规划编制和实施等各环节,对实现“双碳”目标具有重要推动作用。研究为面向“双碳”目标的全域土地综合整治提供理论研究视角和实践参考,为全域土地综合整治助力“双碳”目标实现提供借鉴。     

干涸尾闾湖盆区泥漠地表磨蚀释尘特征

沙粒的表面磨蚀效应是地表产尘、释尘的重要机制,针对干湖盆泥漠地表开展磨蚀释尘实验研究,对理解干湖盆地表风蚀过程及盐碱尘暴形成机理具有重要意义。对采自西居延海干涸湖盆泥漠地表土样进行室内磨蚀模拟实验,研究了不同粒级（细、中、粗）沙粒不同落沙角度（30°,45°,60°）的磨蚀效应。结果表明：（1）泥漠地表磨蚀实验中能够产生明显释尘效应的沙粒粒级阈值为中沙（0.25 mm<M_d<0.50 mm）;（2）磨蚀粒径粒级相同时,磨蚀角度会对泥漠地表磨蚀释尘速率产生影响,磨蚀量的角度排序为60°>30°>45°,但同一粒级3种角度下的磨蚀释尘率差异不显著。（3）磨蚀角度为45°时,计算了泥漠地表的质量磨蚀率与能量磨蚀率,其中中沙为0.04 g·kg^-1、0.43 g·J^-1,粗沙为0.08 g·kg^-1、0.74 g·J^-1,极粗沙为0.26 g·kg^-1、2.54 g·J^-1;在磨蚀沙粒粒级倍增而磨蚀角度不变情况下,泥漠地表磨蚀释尘率与能量磨蚀率未发生正比例线性增长变化。     

The Converter Mechanism of Particle Acceleration and Its Applications to the Unidentified Egret Sources

We discuss the properties of gamma-ray radiation accompanying the acceleration of cosmic rays via the converter mechanism. The mechanism exploits multiple photon-induced conversions of high-energy particles from charged into neutral state (namely, protons to neutrons and electrons to photons) and back. Because a particle in the neutral state can freely cross the magnetic field lines, this allows to avoid both particle losses downstream and reduction in the energy gain factor, which normally takes place due to highly collimated distribution of accelerated particles. The converter mechanism efficiently operates in relativistic outflows under the conditions typical for Active Galactic Nuclei, Gamma-Ray Bursts, and microquasars, where it outperforms the standard diffusive shock acceleration. The accompanying radiation has a number of distinctive features, such as an increase of the maximum energy of synchrotron photons and peculiar radiation beam-pattern, whose opening angle is much wider at larger photon energies. This provides an opportunity to observe off-axis relativistic jets in GeV–TeV energy range. One of the implications is the possibility to explain high-latitude unidentified EGRET sources as off-axis but otherwise typical relativistic-jet sources, such as blazars.     

Gamma rays from millisecond pulsars

We estimate the contribution of millisecond pulsars to the diffuse gamma-ray background of the Galaxy, and show that a significant fraction of the Galactic background may originate from them. A small number of the unidentified COS-B point sources may, in fact, be millisecond pulsars. It is argued that several hundred millisecond pulsars may be detectable as point sources by the GRO satellite A preliminary version of these results was presented at the NATO Advanced Study Institute on Neutron stars, AGNs and Jets, Erice, September 5–17, 1988. On leave from Raman Research Institute, Bangalore, India.     

Spectral variations and long-period intensity variations of auroral kilometric radiation from INTERBALL-2 satellite measurements

A statistical analysis of the auroral kilometric radiation (AKR) measurements in the POLRAD experiment on the INTERBALL-2 satellite has revealed a dependences of the size and location of the AKR generation region on geomagnetic activity: the generation region rises upward and expands with increasing magnetic disturbances. Based on our two-year measurements, we found seasonal AKR intensity variations: the AKR maximum and minimum are observed in winter and summer, respectively. The seasonal variations and the dependence of the spectrum on geomagnetic activity are assumed to have a common physical nature—the background-plasma density variations in the region of the AKR source attributable to plasma flows from the ionosphere into the magnetosphere.     

Non-thermal Emission in Clusters of Galaxies

The most evident signature for the presence of non-thermal elements (magnetic fields and relativistic electrons) in clusters of galaxies is given by the presence of diffuse radio regionspresent so far in a limited number of objects. We review the recent discoveries of new spectral components by EUVE and BeppoSAX in the spectra of some clusters of galaxies that allow to better determine the non-thermalquantities by relating radio and X-ray data. In collaboration with: M. Orlandini, G. Brunetti, L. Feretti, G. Giovannini, P. Grandi, & G. Setti.     

大质量年轻星体新的C18O(1-0)发射

利用紫金山天文台青海观测站13.7米的毫米波望远镜对74个大质量年轻星体或候选进行了C^18O(1-0)的谱线观测。在63个源中观测到了C^18O(1-0)发射，其中57个天体第一次探测到C^18O(1-0)谱线发射。根据谱线辐射温度（TR^*)和半宽（△V），利用LTE方法计算了每个测量源的C^18O(1-0)发射的光学厚度和C^18O(1-0)分子的柱密度。讨论了^13CO(1-0)和C^18O(1-0)的谱线强度比和积分强度比。     

几个河外射电源第二历元的327MHz VLBI观测

１９９１年３月，我们利用上海２５ｍ射电望远镜和欧洲ＶＬＢＩ网联合对几个河外射电源进行了第二历元的３２７ＭＨｚＶＬＢＩ观测．数据的相关处理先后在上海天文台三台站ＭＫ２相关处理机和美国的Ｃａｌｔｅｃｈ／ＪＰＬ相关处理机进行，以便于比较相关结果。本文给出３Ｃ８４、３Ｃ３４５和３Ｃ３８０的混合图。与第一历元的观测比较，３Ｃ３４５和３Ｃ３８０的流量密度没有明显的变化，但３Ｃ３４５的结构变化明显。３Ｃ８４和３Ｃ３４５有喷流的迹象．３Ｃ４５４．３的总流量在不到两年的时间内增加了２５％，如果这个变化是内禀的话，那么可能意味着一次新的流量爆发。