Polarization observations of giant radio pulses from the millisecond pulsar B1937+21 at a frequency of 600 MHz     

M. V. Popov  V. A. Soglasnov  V. I. Kondrat’ev  S. V. Kostyuk 《Astronomy Letters》2004,30(2):95-99

We performed polarization observations of giant radio pulses from the millisecond pulsar B1937+21. The observations were carried out in July 2002 with the 64-m Kalyazin radio telescope at a frequency of 600 MHz in two polarization channels with left-and right-hand circular polarizations (RCP and LCP). We used the S2 data acquisition system with a time resolution of 125 ns. The duration of an observing session was 20 min. We detected twelve giant radio pulses with peak flux densities higher than 1000 Jy; five and seven of these pulses appeared in the RCP and LCP channels, respectively. We found no event that exceeded the established detection threshold simultaneously in the two polarization channels. Thus, we may conclude that the detected giant pulses have a high degree of circular polarization, with the frequency of occurrence of RCP and LCP pulses being the same.  相似文献   

Geo-effectiveness of solar wind extremes     

Hari Om Vats 《Journal of Astrophysics and Astronomy》2006,27(2-3):227-235

Examples of extreme events of solar wind and their effect on geomagnetic conditions are discussed here. It is found that there are two regimes of high speed solar wind streams with a threshold of ∼ 850 km s^-1. Geomagnetic activity enhancement rate (GAER) is defined as an average increase in Ap value per unit average increase in the peak solar wind velocity (Vp) during the stream. GAER was found to be different in the two regimes of high speed streams with +ve and-ve IMF. GAER is 0.73 and 0.53 for solar wind streams with +ve and -ve IMF respectively for the extremely high speed streams (< 850 km s^-1). This indicates that streams above the threshold speed with +ve IMF are 1.4 times more effective in enhancing geomagnetic activity than those with -ve IMF. However, the high speed streams below the threshold with -ve IMF are 1.1 times more effective in enhancing geomagnetic activity than those with +ve IMF. The violent solar activity period (October–November 2003) of cycle 23 presents a very special case during which many severe and strong effects were seen in the environment of the Earth and other planets; however, the z-component of IMF (Bz) is mostly positive during this period. The most severe geomagnetic storm of this cycle occurred when Bz was positive.  相似文献   

Storminess and vulnerability along the Atlantic coastlines of Europe: analysis of storm records and of a greenhouse gases induced climate scenario     

I. Lozano  R. J. N. Devoy  W. May  U. Andersen 《Marine Geology》2004,210(1-4):205-225

Identification of the distinctive circulation patterns of storminess on the Atlantic margin of Europe forms the main objective of this study; dealing with storm frequency, intensity and tracking. The climatology of the extratropical cyclones that affect this region has been examined for the period 1940–1998. Coastal meteorological data from Ireland to Spain have been linked to the cyclone history for the North Atlantic in the analysis of storm records for European coasts. The study examines the evolution in the occurrence of storms since the 1940s and also their relationship with the North Atlantic Oscillation (NAO). Results indicate a seasonal shift in the wind climate, with regionally more severe winters and calmer summers established. This pattern appears to be linked to a northward displacement in the main North Atlantic cyclone track.

An experiment with the ECHAM4 A-GCM at high resolution (T106) has also been used to model the effect of a greenhouse gases induced warming climate on the climatology of coastal storms in the region. The experiment consists of (1), a 30-year control time-slice representing present-day equivalent CO₂ concentrations and (2), a 30-year perturbed period corresponding to a time when the radiative forcing has doubled in terms of equivalent CO₂ concentrations. The boundary conditions have been obtained from an atmosphere-ocean coupled OA-GCM simulation at low horizontal resolution. An algorithm was developed to allow the identification of individual cyclone movements in selected coastal zones. For most of the northern part of the study region, covering Ireland and Scotland, results describe the establishment by ca. 2060 of a tendency for fewer but more intense storms.

The impacts of these changes in storminess for the vulnerability of European Atlantic coasts are considered. For low-lying, exposed and ‘soft’ sedimentary coasts, as in Ireland, these changes in storminess are likely to result in significant localised increases in coastal erosion.  相似文献   

Storms and shoreline retreat in the southern Gulf of St. Lawrence   总被引：1，自引：0，他引：1  

Donald L. Forbes  George S. Parkes  Gavin K. Manson  Lorne A. Ketch 《Marine Geology》2004,210(1-4):169-204

Storms play a major role in shoreline recession on transgressive coasts. In the southern Gulf of St. Lawrence (GSL), southeastern Canada, long-term relative sea-level rise off the North Shore of Prince Edward Island has averaged 0.3 m/century over the past 6000 years (>0.2 m/century over 2000 years). This has driven long-term coastal retreat at mean rates >0.5 m/a but the variance and details of coastal profile response remain poorly understood. Despite extensive sandy shores, sediment supply is limited and sand is transferred landward into multidecadal to century-scale storage in coastal dunes, barrier washover deposits, and flood-tidal delta sinks. Charlottetown tide-gauge records show mean relative sea-level rise of 3.2 mm/a (0.32 m/century) since 1911. A further rise of 0.7±0.4 m is projected over the next 100 years. When differenced from tidal predictions, the water-level data provide a 90-year record of storm-surge occurrence. Combined with wind, wave hindcast, and sea-ice data, this provides a catalogue of potentially significant coastal storms. We also document coastal impacts from three recent storms of great severity in January and October 2000 and November 2001. Digital photogrammetry (1935–1990) and shore-zone surveys (1989–2001) show large spatial and temporal variance in coastal recession rates, weakly correlated with the storm record, in part because of wave suppression or coastal protection by sea ice. Large storms cause rapid erosion from which recovery depends in part on local sand supply, but barrier volume may be conserved by washover deposition. Barrier shores with dunes show high longshore and interdecadal variance, with extensive multidecadal healing of former inlet and overwash gaps. This reflects recovery from an episode of widespread overwash prior to 1935, possibly initiated by intense storms or groups of storms in the latter half of the 19th century. With evidence from the storms of 2000–2001, this points to the importance of storm clustering on scales of weeks to years in determining erosion vulnerability, as well as the need for a long-term, large-scale perspective in assessing coastal stability. The expected acceleration in relative sea-level rise, together with projections of increasing storm intensity and greatly diminished winter ice cover in the southern GSL, implies a significant increase in coastal erosion hazards in future.  相似文献   

Origin of short period comets     

M. E. Bailey 《Celestial Mechanics and Dynamical Astronomy》1992,54(1-3):49-61

Reasons for interest in the origin of short-period comets and the difficulties of computing their long-term dynamcal evolution are reviewed. The relative advantages of a source region in an extended inner core of the Oort cloud or a compact comet belt just beyond the planetary system are finely balanced, and it is premature to consider the problem solved. A complication is that some comets belonging to the Jupiter family may be part of a time-dependent system, possibly the remains of a giant comet such as Chiron which could have been part of the system 104 yr ago. The origin of short-period comets plays a pivotal role in many areas of solar system science: planet formation, the source of water (possibly life) on the terrestrial planets, the cratering record on the terrestrial planets and satellites of the outer planets, and the environmental impact posed by massive bodies and their decay products in the Earth's near-space environment.  相似文献   

长江下游地区下蜀黄土堆积与成壤环境演变——以南京江北地区一典型剖面为例     

毛龙江  贾耀锋  邹欣庆 《地理研究》2006,25(5):887-894

通过对南京江北地区一个典型剖面（TZC剖面）进行野外调查、室内磁化率、粒度等替代性指标分析和光释光断代研究,探讨了该地区第一层古土壤形成时的粉尘堆积与成壤环境演变特点。结果表明:第一层古土壤（400⁵0cm）形成于全新世最适宜期（8500³100aBP）,是在末次冰期下蜀黄土堆积成壤基础上的再发育,与下伏黄土之间存在发生学联系。根据沉积年代和沉积厚度对沉积速率估算,该地区末次冰期沉积速率约为11.17cm/ka,而且可以推测古土壤顶部经历过强烈的水土侵蚀作用,侵蚀的厚度为98.67cm,侵蚀下来的黄土在地势低洼的地方形成次生黄土,这表明了次生黄土同为风尘成因,只是经过后期雨水的侵蚀、搬运和再堆积而已。全新世晚期3100年以来,季风转变,沙尘暴加剧,土壤退化,在南京江北地区堆积成厚约50cm左右的现代黄土层或表土层。  相似文献   

新一代天气雷达与强对流天气预警   总被引：44，自引：29，他引：44  

俞小鼎  王迎春  陈明轩  谭晓光 《高原气象》2005,24(3):456-464

简要介绍了对流风暴的分类、对流风暴的强弱和强对流天气的多普勒天气雷达识别和预警技术，以及新一代天气雷达对强对流风暴预警水平的改进。  相似文献   

2000年4月6日磁暴期间磁扰变化在低纬子午链的纬度效应   总被引：1，自引：0，他引：1       下载免费PDF全文

杨少峰  杜爱民  高玉芬  韩德胜 《地球物理学报》2002,45(4):461-469

利用低纬地磁子午链上H和D分量的分均值数据 ,分析了 2 0 0 0年 4月 6日磁暴期间磁扰变化的纬度效应 .主要特点是 :(1 )急始期间H分量急始跃变幅随磁纬降低而减小 ,且急始变幅的下降率随磁纬降低而逐渐增大 ;(2 )初相期间H分量第 2峰值的变幅和初相持续时间随磁纬降低而减小 ;(3)主相期间H分量迅速减小 ,并随纬度降低最大变幅明显增加 ;(4)恢复相H分量呈两阶段上升趋势 ,前一阶段迅速上升 ,后一阶段上升速度明显减小 .最后对这些磁扰变化的纬度效应与空间电流体系的密切关系作了讨论 .  相似文献   

水资源复杂适应配置系统的理论与模型   总被引：27，自引：0，他引：27  

赵建世  王忠静  翁文斌 《地理学报》2002,57(6):639-647

在对水资源配置系统的复杂性及其复杂适应机理分析的基础上，应用复杂适应系统理论的基本原理和方法，构架出了全新的水资源配置系统分析模型，同时对系统的动力机制、主体行为特性和系统状态的评价方法进行了描述，形成了一个较为完整的研究体系，用于分析水资源配置系统的演化规律，并应用这种分析方法对南水北调工程对受水区水资源配置的影响进行了简要的研究。  相似文献   

金沙江上游某巨型复合型滑坡的基本特征及稳定性分析   总被引：6，自引：0，他引：6  

石豫川  冯文凯  叶志平  胥良 《地质灾害与环境保护》2003,14(4):11-15,42

在对西南某水电站库区一特大型、多期复合型滑坡所处的工程环境条件、自身结构及各期次滑坡体物质组成特征认真调查和研究的基础上．结合ESR测龄试验研究，对该滑坡的变形破坏机制及形成年代进行了综合分析，并对其稳定性进行了定性评价。  相似文献