BDRM理论在双轴海洋声道中的应用

由于表面声道与深海声道间的耦合效应,声波在双轴海洋声道中的传播比较复杂,因此求解双轴海洋声道中的声场就比较困难。在 WKBZ 本征函数的基础上,推导出了参考界面相位修正的一致表达式,并将浅海声传播的波束位移射线简正波(BDRM)理论应用于计算双轴海洋声道中的声场,进行了数值模拟并与传统简正波方法进行比较,结果表明应用 BDRM 理论计算的传播损失具有很高的精度和速度,可以对双轴海洋声道内声传播问题进行分析和预报。     

Climate change, powerlessness and the commons dilemma: Assessing New Zealanders’ preparedness to act

Mitigating climate change is recognized as an increasingly urgent task that requires understanding a range of different strategies, including voluntary behavior change. Among the psychological barriers to behavior change are perceptions of powerlessness and the commons dilemma. This paper examines the association between these factors in a sample of New Zealand citizens and clarifies their importance in relation to other barriers to action to mitigate climate change, including uncertainty and perceived risk. Stronger perceptions of powerlessness and the commons dilemma were related to lower levels of action to mitigate climate change and lesser importance being placed upon climate change as an influence on individual actions. The perceived risk of climate change and the perception that humans influence climate change were the strongest predictors of mitigation action.     

The utilization of North sea hydrocarbons as raw materials for petro-chemical manufacture

The oil and gas reserves of the North Sea have principally been regarded as sources of energy and little attention has been paid to their potential as raw materials for chemical manufacture. This paper reviews the technical and economic possibilities presented by the North Sea hydrocarbons as petro-chemical feedstocks. In particular, an attempt is made to predict changes which may occur in the geography of petro-chemical production in North West Europe if full advantage is taken of these possibilities.     

川东北Y地区雷口坡组古岩溶辨识标志

川东北Y地区三叠系雷口坡组沉积后,受三叠纪印支Ⅰ幕运动的影响,Y地区抬升,缺失部分上三叠统、部分中三叠统,与上覆上三叠统须家河组呈区域性平行不整合接触,接受大气淡水淋滤,为古岩溶的形成提供了有利条件.通过对研究区钻井资料、测井资料的分析,借助岩心观察与岩石薄片,以及电子探针、阴极发光、碳氧同位素等测试手段,综合分析和研...     

A Study of AR 9144; A Fast-Growing EFR

This paper is a study of NOAA region 9144, an emerging flux region (EFR) which grew rapidly beginning 25 August 2000. This region was visible in SOHO data at 0 UT on 25 August 2000 as a small, isolated spot. It was recognizable as an active region with multiple spots by 06:00 UT on the 25th and was a fully developed AR by 24^h UT on the 26th of August. Data are presented from the Michelson Doppler Imager (MDI) experiment on the Solar and Heliospheric Observatory satellite (SOHO), from Big Bear Solar Observatory (BBSO) and from the San Fernando Observatory (SFO). The MDI data are Dopplergrams, magnetograms, and continuum images. The BBSO data are high-resolution Hα filtergrams. The SFO data are Dopplergrams, magnetograms and continuum images from the Video SpectraSpectroHeliograph (VSSHG). MDI Doppler images show that during the rapid growth of this EFR during the day of 26 August, the most obvious feature in area and lifetime is a red-shifted area in the trailing part of the region. SFO Doppler images show a more complex pattern, but still dominated by red shifts in the trailing part of the region near the end of the day of 26 August.     

Ponded deposits on asteroid 433 Eros

Abstract— In late January 2001 the NEAR—Shoemaker spacecraft performed low‐altitude passes over the surface of 433 Eros. Coordinated observations of the asteroid surface were obtained at submeter resolution by the NEAR laser rangefinder and the multispectral imager. This paper presents three independent, coordinated observations of a 90 m pond adjacent to a granular debris flow, including the highest resolution altimetric measurements of ponded deposits on Eros. The ponded deposits appear to have been emplaced by fluid‐like motion of dry asteroidal regolith. A simple model of seismic agitation from impacts is developed to account for pond formation on Eros. The model predicts that ponds should form readily on Eros but not on the Moon, where ponds are not observed. The model also suggests that the absence of observable ponds in the largest craters of Eros, as well as on Phobos and Deimos, may be related to regolith depth.     

Generalized Radon transforms and slant stacks

Summary. The Radon transform or slant stack is becoming a widely used technique for analysing high-quality reflection and refraction data. The transform normally used is applicable to data from a line source in a plane model, that is, one Cartesian coordinate. The theoretical basis for the Radon transform pair for one Cartesian coordinate has appeared in the seismological literature. For a point source in plane or spherical geometry, or a line source in cylindrical geometry only the Radon transform for the direct problem (computation of synthetic seismograms) has been published. To analyse data an approximate inverse transform has been used. In this research note, the exact forms of the generalized Radon transform pairs are completed for a point source in plane or spherical geometry, and for a line source in cylindrical geometry. The differences will be important if the waveforms are being interpreted, and are most significant for near-vertical reflections—the type of data most commonly slant stacked.     

Properties of flares observed in the Mg i b2 line at 5172 Å

Observations of emission in the Mgi b₂ line at 5172 Å are presented for 13 flares. Also discussed are 3 flares which occurred in regions under observation but which showed no Mg emission. The Mg flare kernels resemble white-light flare kernels in their general morphology and location. Comparison of Mg filtergrams with magnetograms indicates that the Mg kernels occur at the feet of magnetic arches across neutral lines. Time-lapse Mg filtergram films indicate photospheric shearing motions near flare sites for several hours before flare onset. We have compared flare Mg emission with microwave and both hard and soft X-ray flare emissions. Examination at the time development of the 1981, July 27 flare shows that the microwave and X-ray bursts may be clearly related to the appearance of successive Mg flare kernels. We have also compared subjective, relative Mg flare importances with other flare emission measurements. For the full sample of flares, Mg importance is significantly correlated with hard and soft X-ray emission peaks, with X-ray ‘hardness’ (ratio of hard to soft peaks) and with the rise slope of soft X-ray bursts. The Mg importance does not correlate with the microwave peaks when the full sample of flares is used, but for the subset showing Mg emission there is significant correlation. No correlation with Hα importance was found. Our results suggest that Mg emission is associated with an impulsive component which may be absent from some flares. The San Fernando Observatory magnesium etalon filter system is described.